Sample records for zone sediment recovered

  1. Microbial diversity in Cenozoic sediments recovered from the Lomonosov Ridge in the Central Arctic basin.

    PubMed

    Forschner, Stephanie R; Sheffer, Roberta; Rowley, David C; Smith, David C

    2009-03-01

    The current understanding of microbes inhabiting deeply buried marine sediments is based largely on samples collected from continental shelves in tropical and temperate latitudes. The geographical range of marine subsurface coring was expanded during the Integrated Ocean Drilling Program Arctic Coring Expedition (IODP ACEX). This expedition to the ice-covered central Arctic Ocean successfully cored the entire 428 m sediment stack on the Lomonosov Ridge during August and September 2004. The recovered cores vary from siliciclastic sediment low in organic carbon (< 0.2%) to organic rich ( approximately 3%) black sediments that rapidly accumulated in the early middle Eocene. Three geochemical environments were characterized based on chemical analyses of porewater: an upper ammonium oxidation zone, a carbonate dissolution zone and a deep (> 200 m below sea floor) sulfate reduction zone. The diversity of microbes within each zone was assessed using 16S rRNA phylogenetic markers. Bacterial 16S rRNA genes were successfully amplified from each of the biogeochemical zones, while archaea was only amplified from the deep sulfate reduction zone. The microbial communities at each zone are phylogenetically different and are most closely related to those from other deep subsurface environments.

  2. Sedimentation in the Kane fracture zone, western North Atlantic

    DOE Office of Scientific and Technical Information (OSTI.GOV)

    Jaroslow, G.E.

    1991-03-01

    The Kane fracture zone, a deep narrow trough in oceanic crust, has provided an ideal depocenter for reservation on the seismic stratigraphic record of the North Atlantic basin. The acoustic stratigraphy in single-channel and multichannel seismic reflection profiles crossing the Kane fracture zone in the western North Atlantic has been examined in order to scrutinize age processes within a fracture zone. Maps of total sediment thickness have provided insight into overall sediment distribution and the influence of topography on sedimentation. Eight reflectors have been traced and correlated with lithostratigraphy at Deep Sea Drilling Project (DSDP) sites. The Bermuda Rise, amore » prominent topographic feature, has had a profound effect on the distribution of sediments within the fracture zone. Since late Eocene, the rise has blocked transport by turbidity currents of terrigenous sediments to distal portions of the fracture valley. A 1,000-m-thick turbidite pond within the fracture zone east of the Bermuda Rise has been determined to have been derived from local sources. Within the ponded sequence a seismic discontinuity is estimated to be early Oligocene and postdates the emergence of the Bermuda Rise, adding an independent age constraint on the development of the rise. The pond terminates against a structural dam at 55{degree}20W, east of which the fracture zone is essentially sediment starved.« less

  3. High-frequency sediment-level oscillations in the swash zone

    USGS Publications Warehouse

    Sallenger, A.H.; Richmond, B.M.

    1984-01-01

    Sediment-level oscillations with heights of about 6 cm and shore-normal lengths of order 10 m have been measured in the swash zone of a high-energy, coarse-sand beach. Crests of oscillations were shore parallel and continuous alongshore. The oscillations were of such low steepness (height-to-length ratio approximately 0.006) that they were difficult to detect visually. The period of oscillation ranged between 6 and 15 min and decreased landward across the swash zone. The sediment-level oscillations were progressive landward with an average migration rate in the middle to upper swash zone of 0.8 m min-1. Migration was caused mostly by erosion on the seaward flank of the crest of an oscillation during a period of net seaward sediment transport. Thus, the observed migration was a form migration landward rather than a migration involving net landward sediment transport. The observed sediment-level oscillations were different than sand waves or other swash-zone bedforms previously described. ?? 1984.

  4. Frictional behavior of carbonate-rich incoming sediment in the Hikurangi subduction zone

    NASA Astrophysics Data System (ADS)

    Rabinowitz, H. S.; Savage, H. M.; Carpenter, B.; Ikari, M.; Collettini, C.

    2017-12-01

    In recent years, the traditional view of the seismogenic zone has been challenged by observations of a range of seismic behaviors both above and below the depths previously considered capable of nucleating earthquakes. The Hikurangi trench is one of the few subduction zones where this transitional seismic behavior has been observed at the shallowest portions of the subduction zone, providing an opportunity to investigate the mechanical controls on seismic behavior through measurements of directly sampled sediment. To this end, an IODP cruise (March-May, 2018; Exp. 375) will recover sample from the faults that participate in this shallow seismic behavior. In order to obtain preliminary frictional characterization of the sedimentary inputs to the Hikurangi Trench, we conducted deformation experiments on samples from an ocean drill core through the incoming sediments (ODP Site 1124). The sedimentary package subducting at Hikurangi contains carbonate-rich lithologies, which have been shown to be more frictionally unstable (velocity-weakening, high healing rates) than the clays that comprise the majority of the sedimentary inputs to global subduction zones. Such frictional properties could promote seismic behavior in the shallower reaches of the subduction zone. We focus on a section of ODP Site 1124 which has a carbonate content of 40 wt% to investigate the effect of this lithology. Samples were saturated with distilled water mixed with 35 g/l sea salt. Velocity-stepping and slide-hold-slide tests were performed in multiple biaxial and triaxial deformation apparatus to investigate a range of pressures, temperatures and velocities relevant to the shallow subduction zone (σeff = 1-150 MPa, sliding velocities of 1.7 nm/s-300 μm/s, hold times of 1-1000 s, and T = 20-100 ºC). We observe transitions from velocity-strengthening to velocity-weakening behavior over these conditions which could contribute to shallow seismic behavior in the Hikurangi trench.

  5. High fungal diversity and abundance recovered in the deep-sea sediments of the Pacific Ocean.

    PubMed

    Xu, Wei; Pang, Ka-Lai; Luo, Zhu-Hua

    2014-11-01

    Knowledge about the presence and ecological significance of bacteria and archaea in the deep-sea environments has been well recognized, but the eukaryotic microorganisms, such as fungi, have rarely been reported. The present study investigated the composition and abundance of fungal community in the deep-sea sediments of the Pacific Ocean. In this study, a total of 1,947 internal transcribed spacer (ITS) regions of fungal rRNA gene clones were recovered from five sediment samples at the Pacific Ocean (water depths ranging from 5,017 to 6,986 m) using three different PCR primer sets. There were 16, 17, and 15 different operational taxonomic units (OTUs) identified from fungal-universal, Ascomycota-, and Basidiomycota-specific clone libraries, respectively. Majority of the recovered sequences belonged to diverse phylotypes of Ascomycota (25 phylotypes) and Basidiomycota (18 phylotypes). The multiple primer approach totally recovered 27 phylotypes which showed low similarities (≤97 %) with available fungal sequences in the GenBank, suggesting possible new fungal taxa occurring in the deep-sea environments or belonging to taxa not represented in the GenBank. Our results also recovered high fungal LSU rRNA gene copy numbers (3.52 × 10(6) to 5.23 × 10(7)copies/g wet sediment) from the Pacific Ocean sediment samples, suggesting that the fungi might be involved in important ecological functions in the deep-sea environments.

  6. Approximate Model of Zone Sedimentation

    NASA Astrophysics Data System (ADS)

    Dzianik, František

    2011-12-01

    The process of zone sedimentation is affected by many factors that are not possible to express analytically. For this reason, the zone settling is evaluated in practice experimentally or by application of an empirical mathematical description of the process. The paper presents the development of approximate model of zone settling, i.e. the general function which should properly approximate the behaviour of the settling process within its entire range and at the various conditions. Furthermore, the specification of the model parameters by the regression analysis of settling test results is shown. The suitability of the model is reviewed by graphical dependencies and by statistical coefficients of correlation. The approximate model could by also useful on the simplification of process design of continual settling tanks and thickeners.

  7. High-resolution chronology of sediment below CCD based on Holocene paleomagnetic secular variations in the Tohoku-oki earthquake rupture zone

    NASA Astrophysics Data System (ADS)

    Kanamatsu, Toshiya; Usami, Kazuko; McHugh, Cecilia M. G.; Ikehara, Ken

    2017-08-01

    Using high-resolution paleomagnetic data, we examined the potential for obtaining precise ages from sediment core samples recovered from deep-sea basins close to rupture zones of the 2011 and earlier earthquakes off Tohoku, Japan. Obtaining detailed stratigraphic ages from deep-sea sediments below the calcium compensation depth (CCD) is difficult, but we found that the samples contain excellent paleomagnetic secular variation records to constrain age models. Variations in paleomagnetic directions obtained from the sediments reveal systematic changes in the cores. A stacked paleomagnetic profile closely matches the Lake Biwa data sets in southwest Japan for the past 7000 years, one can establish age models based on secular variations of the geomagnetic field on sediments recovered uniquely below the CCD. Comparison of paleomagnetic directions near a tephra and a paleomagnetic direction of contemporaneous pyroclastic flow deposits acquired by different magnetization processes shows precise depositional ages reflecting the magnetization delay of the marine sediment record.Plain Language SummaryGenerally obtaining detailed ages from deep-sea <span class="hlt">sediments</span> is difficult, because available dating method is very limited. We found that the deep-see <span class="hlt">sediment</span> off North Japan recorded past sequential geomagnetic directions. If those records correlate well with the reference record in past 7000 years, then we could estimate age of <span class="hlt">sediment</span> by pattern matching. Additionally a volcanic ash emitted in 915 A.D., which was intercalated in our samples, indicates a time lag in our age model. This observation makes our age model more precise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=235359&keyword=dead&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=235359&keyword=dead&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Analysis of archaeal communities in Gulf of Mexico dead <span class="hlt">zone</span> <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><span class="hlt">Sediments</span> may contribute significantly to Louisiana continental shelf “dead zone” hypoxia but limited information hinders comparison of <span class="hlt">sediment</span> biogeochemistry between norm-oxic and hypoxic seasons. Dead <span class="hlt">zone</span> <span class="hlt">sediment</span> cores collected during hypoxia (September 2006) had higher l...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSHE44C1519S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSHE44C1519S"><span>In-situ Geotechnical Investigation of Arctic Nearshore <span class="hlt">Zone</span> <span class="hlt">Sediments</span>, Herschel Island, Yukon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stark, N.; Quinn, B.; Radosavljevic, B.; Lantuit, H.</p> <p>2016-02-01</p> <p>The Arctic is currently undergoing rapid changes with regard to ice coverage, permafrost retreat and coastal erosion. In addition to hydrodynamic processes, the <span class="hlt">sediments</span> in the Arctic nearshore <span class="hlt">zone</span> are affected by potential variations in freeze-thaw cycles, as well as an increase of abundant suspended <span class="hlt">sediment</span> introduced by active retrogressive thaw slumps and increased river discharge. During the YUKON14 expedition to Herschel Island, Yukon, in-situ geotechnical testing of nearshore <span class="hlt">zone</span> <span class="hlt">sediments</span> was conducted using a portable free fall penetrometer. The research goals were mapping of <span class="hlt">sediment</span> types, identification of surficial <span class="hlt">sediment</span> stratification related to recent <span class="hlt">sediment</span> remobilization or deposition processes, and the investigation of the soil mechanical characteristics of the uppermost seabed surface in the nearshore <span class="hlt">zone</span>. Approximately 200 sites were tested using the portable free fall penetrometer, and five different geotechnical signatures identified and grouped. Most locations were characterized by a soft <span class="hlt">sediment</span> top layer that exhibited a noticeably lower <span class="hlt">sediment</span> strength than the underlying <span class="hlt">sediment</span>. The results were correlated to existing <span class="hlt">sediment</span> grain size records and a <span class="hlt">sediment</span> type interpretation based on side scan sonar backscatter information. Strong spatial variations in <span class="hlt">sediment</span> type and stiffness were observed, as well as in abundance and thickness of a top layer of very soft and loose <span class="hlt">sediment</span>. It was attempted to relate the geotechnical signature to site-specific hydrodynamic energy, morphology, and vicinity to thaw slumps. The results will contribute to a detailed investigation of Arctic coastal erosion in the region, and the investigation of the role of geotechnical parameters for Arctic coastal erosion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.T21D2844R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.T21D2844R"><span>Frictional behavior of carbonate-rich <span class="hlt">sediments</span> in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabinowitz, H. S.; Savage, H. M.; Carpenter, B. M.; Collettini, C.</p> <p>2016-12-01</p> <p>Deformation in rocks and <span class="hlt">sediments</span> is controlled by multiple mechanisms, each governed by its own pressure- (P), temperature- (T), and slip velocity- (v) dependent kinetics. Frictional behavior depends on which of these mechanisms are dominant, and, thus, varies with P, T, and v. Carbonates are a useful material with which to interrogate the PTv controls on friction due to the fact that a wide range of mechanisms can be easily accessed in the lab at geologically relevant conditions. In addition, carbonate-rich layers make up a significant component of subducting <span class="hlt">sediments</span> around the world and may impact the frictional behavior of shallow subduction <span class="hlt">zones</span>. In order to investigate the effect of carbonate subduction and the evolution of friction at subduction <span class="hlt">zone</span> conditions, we conducted deformation experiments on input <span class="hlt">sediments</span> for two subduction <span class="hlt">zones</span>, the Hikurangi trench, New Zealand (ODP Site 1124) and the Peru trench (DSDP Site 321), which have carbonate/clay contents of 40/60 wt% and 80/20 wt%, respectively. Samples were saturated with distilled water mixed with 35g/l sea salt and deformed at room temperature. Experiments were conducted at σeff = 1-100 MPa and T = 20-100 °C with sliding velocities of 1-300 μm/s and hold times of 1-1000 s. We test the changes in velocity dependence and healing over these PT conditions to elucidate the frictional behavior of carbonates in subduction <span class="hlt">zone</span> settings. The mechanical results are complemented by microstructural analysis. In lower stress experiments, there is no obvious shear localization; however, by 25 MPa, pervasive boundary-parallel shears become dominant, particularly in the Peru samples. Optical observations of these shear <span class="hlt">zones</span> under cross-polarized light show evidence of plastic deformation (CPO development) while SEM-EDS observations indicate phase segregation in the boundary shears. Degree of microstructural localization appears to correspond with the trends observed in velocity-dependence. Our</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.U53A0050G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.U53A0050G"><span>Permeability-Porosity Relationships of Subduction <span class="hlt">Zone</span> <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gamage, K.; Screaton, E.; Bekins, B.; Aiello, I.</p> <p>2008-12-01</p> <p>Permeability-porosity relationships for <span class="hlt">sediments</span> from Northern Barbados, Costa Rica, Nankai, and Peru subduction <span class="hlt">zones</span> were examined based on their <span class="hlt">sediment</span> type and grain size distribution. Greater correlation was observed between permeability and porosity for siliciclastic <span class="hlt">sediments</span>, diatom oozes, and nannofossil chalk than for nannofossil oozes. For siliciclastic <span class="hlt">sediments</span>, grouping of <span class="hlt">sediments</span> by clay content yields relationships that are generally consistent with results from other marine settings and suggest decreasing permeability for a given porosity as clay content increases. Correction of measured porosities for smectite content generally improves the quality of permeability-porosity relationships. The relationship between permeability and porosity for diatom oozes may be controlled by the amount of clay present in the ooze, causing diatom oozes to behave similarly to siliciclastic <span class="hlt">sediments</span>. For a given porosity the nannofossil oozes have higher permeability values by 1.5 orders of magnitude than the siliciclastic <span class="hlt">sediments</span>. However, the use of a permeability-porosity relation may not be appropriate for unconsolidated carbonates such as nannofossil oozes. This study provided insight to the effects of porosity correction for smectite, variations in lithology and grain size in permeability-porosity relationships. However, further progress in delineating controls on permeability will require more careful and better documented permeability tests on characterized samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036049','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036049"><span>Permeability-porosity relationships of subduction <span class="hlt">zone</span> <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gamage, Kusali; Screaton, Elizabeth; Bekins, B.; Aiello, I.</p> <p>2011-01-01</p> <p>Permeability-porosity relationships for <span class="hlt">sediments</span> from the northern Barbados, Costa Rica, Nankai, and Peru subduction <span class="hlt">zones</span> were examined based on <span class="hlt">sediment</span> type, grain size distribution, and general mechanical and chemical compaction history. Greater correlation was observed between permeability and porosity in siliciclastic <span class="hlt">sediments</span>, diatom oozes, and nannofossil chalks than in nannofossil oozes. For siliciclastic <span class="hlt">sediments</span>, grouping of <span class="hlt">sediments</span> by percentage of clay-sized material yields relationships that are generally consistent with results from other marine settings and suggests decreasing permeability as percentage of clay-sized material increases. Correction of measured porosities for smectite content improved the correlation of permeability-porosity relationships for siliciclastic <span class="hlt">sediments</span> and diatom oozes. The relationship between permeability and porosity for diatom oozes is very similar to the relationship in siliciclastic <span class="hlt">sediments</span>, and permeabilities of both <span class="hlt">sediment</span> types are related to the amount of clay-size particles. In contrast, nannofossil oozes have higher permeability values by 1.5 orders of magnitude than siliciclastic <span class="hlt">sediments</span> of the same porosity and show poor correlation between permeability and porosity. More indurated calcareous <span class="hlt">sediments</span>, nannofossil chalks, overlap siliciclastic permeabilities at the lower end of their measured permeability range, suggesting similar consolidation patterns at depth. Thus, the lack of correlation between permeability and porosity for nannofossil oozes is likely related to variations in mechanical and chemical compaction at shallow depths. This study provides the foundation for a much-needed global database with fundamental properties that relate to permeability in marine settings. Further progress in delineating controls on permeability requires additional carefully documented permeability measurements on well-characterized samples. ?? 2010 Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.B51A0482A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.B51A0482A"><span>New procedure for <span class="hlt">recovering</span> extra- and intracellular DNA from marine <span class="hlt">sediment</span> samples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alawi, M.; Kallmeyer, J.</p> <p>2012-12-01</p> <p> evaluate the new extraction method two <span class="hlt">sediments</span> with rather opposing composition were analyzed. <span class="hlt">Sediment</span> from the South Pacific Gyre, the most oligotrophic oceanic region on earth and organic-rich Baltic Sea <span class="hlt">sediment</span> (Northern Germany) were processed. Using this new procedure high purity genomic iDNA and eDNA with a molecular size range between 20 bp and 50k bp can be simultaneously <span class="hlt">recovered</span> even from very oligotrophic <span class="hlt">sediment</span> with very low cell abundances. The main fraction of <span class="hlt">recovered</span> eDNA was suitable for downstream applications like PCR and had a molecular size that indicates minimal shearing. Despite about two decades of research many questions about deep subsurface life remain unanswered. The fact that microbes can be found even in deep oligotrophic marine <span class="hlt">sediment</span> raises the fundamental questions of the types and availability of substrates and their biogeochemical cycling. This is the first study that provides evidence that eDNA is an important potential substrate for microorganisms in the deep biosphere. Also, our results show a link between cell counts and eDNA content, indicating that the eDNA pool in the investigated <span class="hlt">sediment</span> consist mainly of microbial DNA. Comparative sequence analysis of extracted iDNA and eDNA will provide deeper insights into the origin and turnover of eDNA and the apparent microbial community composition in the deep biosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S54C..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S54C..07M"><span>Effect of <span class="hlt">Sediments</span> on Rupture Dynamics of Shallow Subduction <span class="hlt">Zone</span> Earthquakes and Tsunami Generation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, S.</p> <p>2011-12-01</p> <p>Low-velocity fault <span class="hlt">zones</span> have long been recognized for crustal earthquakes by using fault-<span class="hlt">zone</span> trapped waves and geodetic observations on land. However, the most pronounced low-velocity fault <span class="hlt">zones</span> are probably in the subduction <span class="hlt">zones</span> where <span class="hlt">sediments</span> on the seafloor are being continuously subducted. In this study I focus on shallow subduction <span class="hlt">zone</span> earthquakes; these earthquakes pose a serious threat to human society in their ability in generating large tsunamis. Numerous observations indicate that these earthquakes have unusually long rupture durations, low rupture velocities, and/or small stress drops near the trench. However, the underlying physics is unclear. I will use dynamic rupture simulations with a finite-element method to investigate the dynamic stress evolution on faults induced by both <span class="hlt">sediments</span> and free surface, and its relations with rupture velocity and slip. I will also explore the effect of off-fault yielding of <span class="hlt">sediments</span> on the rupture characteristics and seafloor deformation. As shown in Ma and Beroza (2008), the more compliant hanging wall combined with free surface greatly increases the strength drop and slip near the trench. <span class="hlt">Sediments</span> in the subduction <span class="hlt">zone</span> likely have a significant role in the rupture dynamics of shallow subduction <span class="hlt">zone</span> earthquakes and tsunami generation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T31G2600J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T31G2600J"><span>Sharp Permeability Transitions due to Shallow Diagenesis of Subduction <span class="hlt">Zone</span> <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>James, S.; Screaton, E.</p> <p>2013-12-01</p> <p>The permeability of hemipelagic <span class="hlt">sediments</span> is an important factor in fluid flow in subduction <span class="hlt">zones</span> and can be affected by porosity changes and cementation-dissolution processes acting during diagenesis. Anomalously high porosities have been observed in cores from the Shikoku Basin <span class="hlt">sediments</span> approaching the Nankai Trough subduction <span class="hlt">zone</span>. These high porosities have been attributed to the presence of minor amounts of amorphous silica cement that strengthen the <span class="hlt">sediment</span> and inhibit consolidation. The porosity rapidly drops from 66-68% to 54-56% at a diagenetic boundary where the amorphous silica cement dissolves. Although the anomalous porosity profiles at Nankai have received attention, the magnitude of the corresponding permeability change has not been addressed. In this study, permeability profiles were constructed using permeability-porosity relationships from previous studies, to estimate the magnitude and rate of permeability changes with depth. The predicted permeability profiles for the Nankai Trough <span class="hlt">sediment</span> cores indicate that permeability drops by almost one order of magnitude across the diagenetic boundary. This abrupt drop in permeability has the potential to facilitate significant changes in pore fluid pressures and thus to influence the deformation of the <span class="hlt">sediment</span> onto the accretionary prism. At the Costa Rica subduction <span class="hlt">zone</span>, results vary with location. Site U1414 offshore the Osa Peninsula shows porosities stable at 69% above 145 mbsf and then decrease to 54% over a 40 m interval. A porosity drop of that magnitude is predicted to correlate to an order of magnitude permeability decrease. In contrast, porosity profiles from Site 1039 offshore the Nicoya Peninsula and Site U1381 offshore the Osa Peninsula show anomalously high porosities but no sharp drop. It is likely that <span class="hlt">sediments</span> do not cross the diagenetic boundary due to the extremely low (<10°C/km) thermal gradient at Site 1039 and the thin (<100 m) <span class="hlt">sediment</span> cover at Site U1381. At these locations</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.jstor.org/stable/25737049','USGSPUBS'); return false;" href="http://www.jstor.org/stable/25737049"><span>Geologic framework, evolution, and <span class="hlt">sediment</span> resources for restoration of the Louisiana Coastal <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kulp, Mark; Penland, Shea; Williams, S. Jeffress; Jenkins, Chris; Flocks, Jim; Kindinger, Jack</p> <p>2005-01-01</p> <p>The Louisiana Coastal <span class="hlt">Zone</span> along the north-central Gulf of Mexico represents one of America's most important coastal ecosystems in terms of natural resources, human infrastructure, and cultural heritage. This <span class="hlt">zone</span> also has the highest rates of coastal erosion and wetland loss in the nation because of a complex combination of natural processes and anthropogenic activities during the past century. In response to the dramatic land loss, regional-scale restoration plans are being developed through a partnership of federal and state agencies. One objective is to maintain the barrier island and tidal inlet systems, thereby reducing the impact of storm surge and interior wetland loss. Proposed shore line restoration work relies primarily upon the use of large volumes of sand-rich <span class="hlt">sediment</span> for shoreline stabilization and the implementation of the shoreline projects. Although sand-rich <span class="hlt">sediment</span> is required for the Louisiana restoration projects, it is of limited availability within the generally clay to silt-rich, shallow strata of the Louisiana Coastal <span class="hlt">Zone</span>. Locating volumetrically significant quantities of sand-rich <span class="hlt">sediment</span> presents a challenge and requires detailed field investigations using direct sampling and geophysical sensing methods. Consequently, there is a fundamental need to thoroughly understand and map the distribution and textural character {e.g., sandiness) of <span class="hlt">sediment</span> resources within the Coastal <span class="hlt">Zone</span> for the most cost-effective design and completion of restoration projects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040088314&hterms=APICAL&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DAPICAL','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040088314&hterms=APICAL&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DAPICAL"><span>Conservation of the plastid <span class="hlt">sedimentation</span> <span class="hlt">zone</span> in all moss genera with known gravitropic protonemata</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schwuchow, J. M.; Kern, V. D.; White, N. J.; Sack, F. D.</p> <p>2002-01-01</p> <p>Moss protonemata from several species are known to be gravitropic. The characterization of additional gravitropic species would be valuable to identify conserved traits that may relate to the mechanism of gravitropism. In this study, four new species were found to have gravitropic protonemata, Fissidens adianthoides, Fissidens cristatus, Physcomitrium pyriforme, and Barbula unguiculata. Comparison of upright and inverted apical cells of P. pyriforme and Fissidens species showed clear axial <span class="hlt">sedimentation</span>. This <span class="hlt">sedimentation</span> is highly regulated and not solely dependent on amyloplast size. Additionally, the protonemal tip cells of these species contained broad subapical <span class="hlt">zones</span> that displayed lateral amyloplast <span class="hlt">sedimentation</span>. The conservation of a <span class="hlt">zone</span> of lateral <span class="hlt">sedimentation</span> in a total of nine gravitropic moss species from five different orders supports the idea that this <span class="hlt">sedimentation</span> serves a specialized and conserved function in gravitropism, probably in gravity sensing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5030832','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5030832"><span>Differences in the Composition of Archaeal Communities in <span class="hlt">Sediments</span> from Contrasting <span class="hlt">Zones</span> of Lake Taihu</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Fan, Xianfang; Xing, Peng</p> <p>2016-01-01</p> <p>In shallow lakes, different primary producers might impact the physiochemical characteristics of the <span class="hlt">sediment</span> and the associated microbial communities. Until now, little was known about the features of <span class="hlt">sediment</span> Archaea and their variation across different primary producer-dominated ecosystems. Lake Taihu provides a suitable study area with cyanobacteria- and macrophyte-dominated <span class="hlt">zones</span> co-occurring in one ecosystem. The composition of the <span class="hlt">sediment</span> archaeal community was assessed using 16S rRNA gene amplicon sequencing technology, based on which the potential variation with respect to the physiochemical characteristics of the <span class="hlt">sediment</span> was analyzed. Euryarchaeota (30.19% of total archaeal sequences) and Bathyarchaeota (28.00%) were the two most abundant phyla, followed by Crenarchaeota (11.37%), Aigarchaeota (10.24%) and Thaumarchaeota (5.98%). The differences found in the composition of the archaeal communities between the two <span class="hlt">zones</span> was significant (p = 0.005). <span class="hlt">Sediment</span> from macrophyte-dominated <span class="hlt">zones</span> had high TOC and TN content and an abundance of archaeal lineages potentially involved in the degradation of complex organic compounds, such as the order Thermoplasmatales. In the area dominated by Cyanobacteria, archaeal lineages related to sulfur metabolism, for example, Sulfolobales and Desulfurococcales, were significantly enriched. Among Bathyarchaeota, subgroups MCG-6 and MCG-15 were significantly accumulated in the <span class="hlt">sediment</span> of areas dominated by macrophytes whereas MCG-4 was consistently dominant in both type of <span class="hlt">sediments</span>. The present study contributes to the knowledge of <span class="hlt">sediment</span> archaeal communities with different primary producers and their possible biogeochemical functions in <span class="hlt">sediment</span> habitats. PMID:27708641</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089458&hterms=stein&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3Dstein','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089458&hterms=stein&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D60%26Ntt%3Dstein"><span>Organelle <span class="hlt">sedimentation</span> in gravitropic roots of Limnobium is restricted to the elongation <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sack, F. D.; Kim, D.; Stein, B.</p> <p>1994-01-01</p> <p>Roots of the aquatic angiosperm Limnobium spongia (Bosc) Steud. were evaluated by light and electron microscopy to determine the distribution of organelle <span class="hlt">sedimentation</span> towards gravity. Roots of Limnobium are strongly gravitropic. The rootcap consists of only two layers of cells. Although small amyloplasts are present in the central cap cells, no <span class="hlt">sedimentation</span> of any organelle, including amyloplasts, was found. In contrast, both amyloplasts and nuclei <span class="hlt">sediment</span> consistently and completely in cells of the elongation <span class="hlt">zone</span>. <span class="hlt">Sedimentation</span> occurs in one cell layer of the cortex just outside the endodermis. <span class="hlt">Sedimentation</span> of both amyloplasts and nuclei begins in cells that are in their initial stages of elongation and persists at least to the level of the root where root hairs emerge. This is the first modern report of the presence of <span class="hlt">sedimentation</span> away from, but not in, the rootcap. It shows that <span class="hlt">sedimentation</span> in the rootcap is not necessary for gravitropic sensing in at least one angiosperm. If amyloplast <span class="hlt">sedimentation</span> is responsible for gravitropic sensing, then the site of sensing in Limnobium roots is the elongation <span class="hlt">zone</span> and not the rootcap. These data do not necessarily conflict with the hypothesis that sensing occurs in the cap in other roots, since Limnobium roots are exceptional in rootcap origin and structure, as well as in the distribution of organelle <span class="hlt">sedimentation</span>. Similarly, if nuclear <span class="hlt">sedimentation</span> is involved in gravitropic sensing, then nuclear mass would function in addition to, not instead of, that of amyloplasts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22306311','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22306311"><span>Contamination of port <span class="hlt">zone</span> <span class="hlt">sediments</span> by metals from Large Marine Ecosystems of Brazil.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Buruaem, Lucas M; Hortellani, Marcos A; Sarkis, Jorge E; Costa-Lotufo, Leticia V; Abessa, Denis M S</p> <p>2012-03-01</p> <p><span class="hlt">Sediment</span> contamination by metals poses risks to coastal ecosystems and is considered to be problematic to dredging operations. In Brazil, there are differences in sedimentology along the Large Marine Ecosystems in relation to the metal distributions. We aimed to assess the extent of Al, Fe, Hg, Cd, Cr, Cu, Ni, Pb and Zn contamination in <span class="hlt">sediments</span> from port <span class="hlt">zones</span> in northeast (Mucuripe and Pecém) and southeast (Santos) Brazil through geochemical analyses and <span class="hlt">sediment</span> quality ratings. The metal concentrations found in these port <span class="hlt">zones</span> were higher than those observed in the continental shelf or the background values in both regions. In the northeast, metals were associated with carbonate, while in Santos, they were associated with mud. Geochemical analyses showed enrichments in Hg, Cd, Cu, Ni and Zn, and a simple application of international <span class="hlt">sediment</span> quality guidelines failed to predict their impacts, whereas the use of site-specific values that were derived by geochemical and ecotoxicological approaches seemed to be more appropriate in the management of the dredged <span class="hlt">sediments</span>. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li class="active"><span>1</span></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_1 --> <div id="page_2" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="21"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AdWR...33..277B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AdWR...33..277B"><span>Numerical simulation of two-phase flow for <span class="hlt">sediment</span> transport in the inner-surf and swash <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bakhtyar, R.; Barry, D. A.; Yeganeh-Bakhtiary, A.; Li, L.; Parlange, J.-Y.; Sander, G. C.</p> <p>2010-03-01</p> <p>A two-dimensional two-phase flow framework for fluid-<span class="hlt">sediment</span> flow simulation in the surf and swash <span class="hlt">zones</span> was described. Propagation, breaking, uprush and backwash of waves on sloping beaches were studied numerically with an emphasis on fluid hydrodynamics and <span class="hlt">sediment</span> transport characteristics. The model includes interactive fluid-solid forces and intergranular stresses in the moving <span class="hlt">sediment</span> layer. In the Euler-Euler approach adopted, two phases were defined using the Navier-Stokes equations with interphase coupling for momentum conservation. The k-ɛ closure model and volume of fluid approach were used to describe the turbulence and tracking of the free surface, respectively. Numerical simulations explored incident wave conditions, specifically spilling and plunging breakers, on both dissipative and intermediate beaches. It was found that the spatial variation of <span class="hlt">sediment</span> concentration in the swash <span class="hlt">zone</span> is asymmetric, while the temporal behavior is characterized by maximum <span class="hlt">sediment</span> concentrations at the start and end of the swash cycle. The numerical results also indicated that the maximum turbulent kinetic energy and <span class="hlt">sediment</span> flux occurs near the wave-breaking point. These predictions are in general agreement with previous observations, while the model describes the fluid and <span class="hlt">sediment</span> phase characteristics in much more detail than existing measurements. With direct quantifications of velocity, turbulent kinetic energy, <span class="hlt">sediment</span> concentration and flux, the model provides a useful approach to improve mechanistic understanding of hydrodynamic and <span class="hlt">sediment</span> transport in the nearshore <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS23B1185C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS23B1185C"><span>In-situ Observations of Swash-<span class="hlt">zone</span> Flow Velocities and <span class="hlt">Sediment</span> Transport on a Steep Beach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chardon-Maldonado, P.; Puleo, J. A.; Figlus, J.</p> <p>2014-12-01</p> <p>A 45 m scaffolding frame containing an array of instruments was installed at South Bethany Beach, Delaware, to obtain in-situ measurements in the swash <span class="hlt">zone</span>. Six cross-shore stations were established to simultaneously measure near-bed velocity profiles, <span class="hlt">sediment</span> concentration and water level fluctuations on a steep beach. Measurements of swash-<span class="hlt">zone</span> hydrodynamics and morphological change were collected from February 12 to 25, 2014, following a large Nor'easter storm with surf <span class="hlt">zone</span> significant wave height exceeding 5 m. Swash-<span class="hlt">zone</span> flow velocities (u,v,w) were measured at each cross-shore location using a Nortek Vectrino profiling velocimeter that measured a 30 mm velocity profile at 1 mm vertical increments at 100 Hz. These velocity profiles were used to quantify the vertical flow structure over the foreshore and estimate hydrodynamic parameters such as bed shear stress and turbulent kinetic energy dissipation. <span class="hlt">Sediment</span> concentrations were measured using optical backscatter sensors (OBS) to obtain spatio-temporal measurements during both uprush and backwash phases of the swash cycle. Cross-shore <span class="hlt">sediment</span> transport rates at each station were estimated by taking the product of cross-shore velocity and <span class="hlt">sediment</span> concentration. Foreshore elevations were sampled every low tide using a Leica GPS system with RTK capability. Cross-shore <span class="hlt">sediment</span> transport rates and gradients derived from the velocities and bed shear stress estimates will be related to the observed morphological change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28978732','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28978732"><span>Diatoms dominate the eukaryotic metatranscriptome during spring in coastal 'dead <span class="hlt">zone</span>' <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Broman, Elias; Sachpazidou, Varvara; Dopson, Mark; Hylander, Samuel</p> <p>2017-10-11</p> <p>An important characteristic of marine <span class="hlt">sediments</span> is the oxygen concentration that affects many central metabolic processes. There has been a widespread increase in hypoxia in coastal systems (referred to as 'dead <span class="hlt">zones</span>') mainly caused by eutrophication. Hence, it is central to understand the metabolism and ecology of eukaryotic life in <span class="hlt">sediments</span> during changing oxygen conditions. Therefore, we sampled coastal 'dead <span class="hlt">zone</span>' Baltic Sea <span class="hlt">sediment</span> during autumn and spring, and analysed the eukaryotic metatranscriptome from field samples and after incubation in the dark under oxic or anoxic conditions. Bacillariophyta (diatoms) dominated the eukaryotic metatranscriptome in spring and were also abundant during autumn. A large fraction of the diatom RNA reads was associated with the photosystems suggesting a constitutive expression in darkness. Microscope observation showed intact diatom cells and these would, if hatched, represent a significant part of the pelagic phytoplankton biomass. Oxygenation did not significantly change the relative proportion of diatoms nor resulted in any major shifts in metabolic 'signatures'. By contrast, diatoms rapidly responded when exposed to light suggesting that light is limiting diatom development in hypoxic <span class="hlt">sediments</span>. Hence, it is suggested that diatoms in hypoxic <span class="hlt">sediments</span> are on 'standby' to exploit the environment if they reach suitable habitats. © 2017 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdWR..110...59O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdWR..110...59O"><span>Vortex-induced suspension of <span class="hlt">sediment</span> in the surf <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Otsuka, Junichi; Saruwatari, Ayumi; Watanabe, Yasunori</p> <p>2017-12-01</p> <p>A major mechanism of <span class="hlt">sediment</span> suspension by organized vortices produced under violent breaking waves in the surf <span class="hlt">zone</span> was identified through physical and computational experiments. Counter-rotating flows within obliquely descending eddies produced between adjacent primary roller vortices induce transverse convergent near-bed flows, driving bed load transport to form regular patterns of transverse depositions. The deposited <span class="hlt">sediment</span> is then rapidly ejected by upward carrier flows induced between the vortices. This mechanism of vortex-induced suspension is supported by experimental evidence that coherent <span class="hlt">sediment</span> clouds are ejected where the obliquely descending eddies reach the sea bed after the breaking wave front has passed. In addition to the effects of settling and turbulent diffusion caused by breaking waves, the effect of the vortex-induced flows was incorporated into a suspension model on the basis of vorticity dynamics and parametric characteristics of transverse flows in breaking waves. The model proposed here reasonably predicts an exponential attenuation of the measured <span class="hlt">sediment</span> concentration due to violent plunging waves and significantly improves the underprediction of the concentration produced by previous models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1064617-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquife','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1064617-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquife"><span>Geochemical, mineralogical and microbiological characteristics of <span class="hlt">sediment</span> from a naturally reduced <span class="hlt">zone</span> in a uranium-contaminated aquife</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Campbell, K M; K Kukkadapu, R K; Qafoku, N P</p> <p>2012-05-23</p> <p>Localized <span class="hlt">zones</span> or lenses of naturally reduced <span class="hlt">sediments</span> have the potential to play a significant role in the fate and transport of redox-sensitive metals and metalloids in aquifers. To assess the mineralogy, microbiology and redox processes that occur in these <span class="hlt">zones</span>, several cores from a region of naturally occurring reducing conditions in a U-contaminated aquifer (Rifle, CO) were examined. <span class="hlt">Sediment</span> samples from a transect of cores ranging from oxic/suboxic Rifle aquifer <span class="hlt">sediment</span> to naturally reduced <span class="hlt">sediment</span> were analyzed for U and Fe content, oxidation state, and mineralogy; reduced S phases; and solid-phase organic C content using a suite of analyticalmore » and spectroscopic techniques on bulk <span class="hlt">sediment</span> and size fractions. Solid-phase U concentrations were higher in the naturally reduced <span class="hlt">zone</span>, with a high proportion of the U present as U(IV). The <span class="hlt">sediments</span> were also elevated in reduced S phases and Fe(II), indicating it is very likely that U(VI), Fe(III), and SO4 reduction has occurred or is occurring in the <span class="hlt">sediment</span>. The microbial community was assessed using lipid- and DNA-based techniques, and statistical redundancy analysis was performed to determine correlations between the microbial community and the geochemistry. Increased concentrations of solid-phase organic C and biomass in the naturally reduced <span class="hlt">sediment</span> suggests that natural bioreduction is stimulated by a <span class="hlt">zone</span> of increased organic C concentration associated with fine-grained material and lower permeability to groundwater flow. Characterization of the naturally bioreduced <span class="hlt">sediment</span> provides an understanding of the natural processes that occur in the <span class="hlt">sediment</span> under reducing conditions and how they may impact natural attenuation of radionuclides and other redox sensitive materials. Results also suggest the importance of recalcitrant organic C for maintaining reducing conditions and U immobilization.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1047358-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquifer','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1047358-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquifer"><span>Geochemical, mineralogical and microbiological characteristics of <span class="hlt">sediment</span> from a naturally reduced <span class="hlt">zone</span> in a uranium-contaminated aquifer</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Campbell, Kate M.; Kukkadapu, Ravi K.; Qafoku, Nikolla</p> <p>2012-05-23</p> <p>Localized <span class="hlt">zones</span> or lenses of naturally reduced <span class="hlt">sediments</span> have the potential to play a significant role in the fate and transport of redox-sensitive metals and metalloids in aquifers. To assess the mineralogy, microbiology, and redox processes that occur in these <span class="hlt">zones</span>, we examined several cores from a region of naturally occurring reducing conditions in a uranium-contaminated aquifer (Rifle, CO). <span class="hlt">Sediment</span> samples from a transect of cores ranging from oxic/suboxic Rifle aquifer <span class="hlt">sediment</span> to naturally reduced <span class="hlt">sediment</span> were analyzed for uranium and iron content, oxidation state, and mineralogy, reduced sulfur phases, and solid phase organic carbon content using a suite ofmore » analytical and spectroscopic techniques on bulk <span class="hlt">sediment</span> and size fractions. Solid-phase uranium concentrations were higher in the naturally reduced <span class="hlt">zone</span>, with a high proportion of the uranium present as reduced U(IV). The <span class="hlt">sediments</span> were also elevated in reduced sulfur phases and Fe(II), indicating it is very likely that U(VI), Fe(III), and sulfate reduction occurred or is occurring in the <span class="hlt">sediment</span>. The microbial community was assessed using lipid- and DNA-based techniques, and statistical redundancy analysis was performed to determine correlations between the microbial community and the geochemistry. Increased concentration of solid phase organic carbon and biomass in the naturally reduced <span class="hlt">sediment</span> suggests that natural bioreduction is stimulated by a <span class="hlt">zone</span> of increased organic carbon concentration associated with fine-grained material and lower permeability to groundwater flow. Characterization of the naturally bioreduced <span class="hlt">sediment</span> provides an understanding of the natural processes that occur in the <span class="hlt">sediment</span> under reducing conditions and how they may impact natural attenuation of radionuclides and other redox sensitive materials. Results also suggest the importance of recalcitrant organic carbon for maintaining reducing conditions and uranium immobilization.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1064451-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquifer','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1064451-geochemical-mineralogical-microbiological-characteristics-sediment-from-naturally-reduced-zone-uranium-contaminated-aquifer"><span>Geochemical, mineralogical and microbiological characteristics of <span class="hlt">sediment</span> from a naturally reduced <span class="hlt">zone</span> in a uranium-contaminated aquifer</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Campbell, K. M.; Kukkadapu, R. K.; Qafoku, N. P.</p> <p>2012-08-01</p> <p>Localized <span class="hlt">zones</span> or lenses of naturally reduced <span class="hlt">sediments</span> have the potential to play a significant role in the fate and transport of redox-sensitive metals and metalloids in aquifers. To assess the mineralogy, microbiology and redox processes that occur in these <span class="hlt">zones</span>, several cores from a region of naturally occurring reducing conditions in a U-contaminated aquifer (Rifle, CO) were examined. <span class="hlt">Sediment</span> samples from a transect of cores ranging from oxic/suboxic Rifle aquifer <span class="hlt">sediment</span> to naturally reduced <span class="hlt">sediment</span> were analyzed for U and Fe content, oxidation state, and mineralogy; reduced S phases; and solid-phase organic C content using a suite of analyticalmore » and spectroscopic techniques on bulk <span class="hlt">sediment</span> and size fractions. Solid-phase U concentrations were higher in the naturally reduced <span class="hlt">zone</span>, with a high proportion of the U present as U(IV). The <span class="hlt">sediments</span> were also elevated in reduced S phases and Fe(II), indicating it is very likely that U(VI), Fe(III), and SO 4 reduction has occurred or is occurring in the <span class="hlt">sediment</span>. The microbial community was assessed using lipid- and DNA-based techniques, and statistical redundancy analysis was performed to determine correlations between the microbial community and the geochemistry. Increased concentrations of solid-phase organic C and biomass in the naturally reduced <span class="hlt">sediment</span> suggests that natural bioreduction is stimulated by a <span class="hlt">zone</span> of increased organic C concentration associated with fine-grained material and lower permeability to groundwater flow. Characterization of the naturally bioreduced <span class="hlt">sediment</span> provides an understanding of the natural processes that occur in the <span class="hlt">sediment</span> under reducing conditions and how they may impact natural attenuation of radionuclides and other redox sensitive materials. Results also suggest the importance of recalcitrant organic C for maintaining reducing conditions and U immobilization.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015162','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015162"><span>Observations of gas hydrates in marine <span class="hlt">sediments</span>, offshore northern California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brooks, J.M.; Field, M.E.; Kennicutt, M.C.</p> <p>1991-01-01</p> <p>Biogenic gas hydrates were <span class="hlt">recovered</span> in shallow cores (< 6 m deep) from the Eel River basin in offshore northern California between 40??38??? and 40??56???N. The gas hydrates contained primarily methane (??13C = -57.6 to -69.1???) and occurred as dispersed crystals, small (2-20 mm) nodules, and layered bands within the <span class="hlt">sediment</span>. These hydrates, <span class="hlt">recovered</span> in <span class="hlt">sediment</span> at water depths between 510 and 642 m, coincide nearly, but not exactly, with areas showing bottom-simulating reflectors (BSRs) on seismic-reflection records. This study confirms indirect geophysical and geologic observations that gas hydrates are present north of the Mendocino Fracture <span class="hlt">Zone</span> in <span class="hlt">sediment</span> of the Eel River basin but probably are absent to the south in the Point Arena basin. This discovery extends the confirmed sites of gas hydrates in the eastern Pacific region beyond the Peruvian and Central American margins to the northern California margin. ?? 1991.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JAESc..29..508V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JAESc..29..508V"><span>Water and <span class="hlt">sediment</span> dynamics in the Red River mouth and adjacent coastal <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Maren, D. S.</p> <p>2007-02-01</p> <p>The coastline of the Red River Delta is characterized by alternating patterns of rapid accretion and severe erosion. The main branch of the Red River, the Ba Lat, is presently expanding seaward with a main depositional area several km downstream and offshore the Ba Lat River mouth. <span class="hlt">Sediment</span> deposition rates are approximately 6 m in the past 50 years. Field measurements were done to determine the processes that regulate marine dispersal and deposition of <span class="hlt">sediment</span> supplied by the Ba Lat. These measurements reveal that the waters surrounding the Ba Lat delta are strongly stratified with a pronounced southward-flowing surface layer. This southward-flowing surface layer is a coastal current which is generated by river plumes that flow into the coastal <span class="hlt">zone</span> north of the Ba Lat. However, outflow of turbid river water is not continuous and most <span class="hlt">sediment</span> enters the coastal <span class="hlt">zone</span> when the alongshore surface velocities are low. As a consequence, most <span class="hlt">sediment</span> settles from suspension close to the river mouth. In addition to the southward surface flow, the southward near-bottom currents are also stronger than northward currents. Contrasting with the residual flow near-surface, this southward flow component near-bottom is caused by tidal asymmetry. Because most <span class="hlt">sediment</span> is supplied by the Ba Lat when wave heights are low, <span class="hlt">sediment</span> is able to consolidate and therefore the long-term deposition is southward of, but still close to, the Ba Lat mouth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991llmm.conf..451B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991llmm.conf..451B"><span>Retardation and <span class="hlt">Sedimentation</span> of Chernobyl-derived Radiocesium in the Photic <span class="hlt">Zone</span> Sedimenttrap Deployment Studies in the Norwegian Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baumann, Marion</p> <p></p> <p>One long-term and three short-term sedimenttrap-deployments have been installed in the Norwegian Sea shortly after the reactor-accident at Chernobyl in April 1986. Radiocesium investigations of the sedimenttrap material were combined with detailed biological investigations on <span class="hlt">sedimentation</span> processes in the photic <span class="hlt">Zone</span>. Lacking efficient export processes in the photic <span class="hlt">Zone</span>, radiocesium first was retained in the photic <span class="hlt">Zone</span> for several weeks. Then the break down and successive <span class="hlt">sedimentation</span> of the heterotrophic community exported about 10 % of surface deposition of radiocesium to larger water depths and to the seafloor at 1450 m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1089107','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1089107"><span>Use of Polyphosphate to Decrease Uranium Leaching in Hanford 300 Area Smear <span class="hlt">Zone</span> <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Szecsody, James E.; Zhong, Lirong; Oostrom, Martinus</p> <p>2012-09-30</p> <p>The primary objective of this study is to summarize the laboratory investigations performed to evaluate short- and long-term effects of phosphate treatment on uranium leaching from 300 area smear <span class="hlt">zone</span> <span class="hlt">sediments</span>. Column studies were used to compare uranium leaching in phosphate-treated to untreated <span class="hlt">sediments</span> over a year with multiple stop flow events to evaluate longevity of the uranium leaching rate and mass. A secondary objective was to compare polyphosphate injection, polyphosphate/xanthan injection, and polyphosphate infiltration technologies that deliver phosphate to <span class="hlt">sediment</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/37771','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/37771"><span><span class="hlt">Sediment</span> trapping by streamside management <span class="hlt">zones</span> of various widths after forest harvest and site preparation</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>William Lakel; Wallace Aust; M. Aust; Chad Bolding; C. Dolloff; Patrick Keyser; Robert Feldt</p> <p>2010-01-01</p> <p>Recommended widths for streamside management <span class="hlt">zones</span> (SMZs) for <span class="hlt">sediment</span> protection vary. The objectives of this study were to compare the effects of SMZ widths and thinning levels on <span class="hlt">sediment</span> moving through SMZs. Four SMZ treatments were installed within 16 harvested watersheds where intermittent streams graded into small perennial streams. Sites were clearcut,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRII.125..117W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRII.125..117W"><span>Repeated occurrences of methanogenic <span class="hlt">zones</span>, diagenetic dolomite formation and linked silicate alteration in southern Bering Sea <span class="hlt">sediments</span> (Bowers Ridge, IODP Exp. 323 Site U1341)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wehrmann, L. M.; Ockert, C.; Mix, A. C.; Gussone, N.; Teichert, B. M. A.; Meister, P.</p> <p>2016-03-01</p> <p>Diagenetic precipitates, such as dolomite, and the chemistry of residual deeply buried porewater often represent the only traces of past biogeochemical activity in marine <span class="hlt">sediments</span>. A 600 m thick sedimentary section, recently drilled at Integrated Ocean Drilling Program (IODP) Site U1341 on Bowers Ridge (southern Bering Sea), provides insight into such a 4.3 Ma old paleo-diagenetic archive. Hard-lithified calcite-dolomite layers, and laminae of disseminated carbonate, were <span class="hlt">recovered</span> in diatom-rich <span class="hlt">sediments</span> over a depth range of 400 m. Carbon isotope values of the diagenetic carbonates between -16.6 and -14.4‰ (VPDB) and strontium isotope ratios of dolomites close to past seawater values suggest carbonate precipitation induced by the production of dissolved inorganic carbon (DIC) during elevated rates of organic carbon mineralization, primarily via sulfate reduction, at shallow <span class="hlt">sediment</span> depth below the paleo-seafloor. Diagenetic carbonates at 280-440 m below seafloor were likely also produced by the intermittent onset of sulfate reduction coupled to the anaerobic oxidation of methane (AOM) at sulfate-methane transition <span class="hlt">zones</span> (SMTZ). These microbially mediated processes do not occur in the <span class="hlt">sediment</span> at this site at present but were likely connected to the presence of a methanogenic <span class="hlt">zone</span> at 2.58-2.51 Ma. A minimum in sulfate concentrations in modern porewaters and low sedimentary Ba/Al ratios resulting from former sulfate depletion are reminiscent of the presence of this large methanogenic <span class="hlt">zone</span>. The minimum in sulfate concentrations is reflected in a minimum in magnesium concentrations, less radiogenic strontium and isotopically light calcium in the porewater. It is proposed that magnesium was removed from the porewater during carbonate precipitation and volcanic ash alteration which occurred in the former methanogenic <span class="hlt">zone</span> and also released strontium with a less radiogenic isotope ratio and isotopically light calcium into the porewater. The isotopic composition of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=183561','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=183561"><span>Biodegradation of organic compounds in vadose <span class="hlt">zone</span> and aquifer <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Konopka, A; Turco, R</p> <p>1991-01-01</p> <p>The microbial processes that occur in the subsurface under a typical Midwest agricultural soil were studied. A 26-m bore was installed in November of 1988 at a site of the Purdue University Agronomy Research Center. Aseptic collections of soil materials were made at 17 different depths. Physical analysis indicated that the site contained up to 14 different strata. The site materials were primarily glacial tills with a high carbonate content. The N, P, and organic C contents of <span class="hlt">sediments</span> tended to decrease with depth. Ambient water content was generally less than the water content, which corresponds to a -0.3-bar equivalent. No pesticides were detected in the samples, and degradation of added 14C-labeled pesticides (atrazine and metolachlor) was not detected in slurry incubations of up to 128 days. The sorption of atrazine and metolachlor was correlated with the clay content of the <span class="hlt">sediments</span>. Microbial biomass (determined by direct microscopic count, viable count, and phospholipid assay) in the tills was lower than in either the surface materials or the aquifer located at 25 m. The biodegradation of glucose and phenol occurred rapidly and without a lag in samples from the aquifer capillary fringe, saturated <span class="hlt">zone</span>, and surface soils. In contrast, lag periods and smaller biodegradation rates were found in the till samples. Subsurface <span class="hlt">sediments</span> are rich in microbial numbers and activity. The most active strata appear to be transmissive layers in the saturated <span class="hlt">zone</span>. This implies that the availability of water may limit activity in the profile. PMID:1768098</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1129864-microbial-distributions-detected-oligonucleotide-microarray-across-geochemical-zones-associated-methane-marine-sediments-from-ulleung-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1129864-microbial-distributions-detected-oligonucleotide-microarray-across-geochemical-zones-associated-methane-marine-sediments-from-ulleung-basin"><span>Microbial distributions detected by an oligonucleotide microarray across geochemical <span class="hlt">zones</span> associated with methane in marine <span class="hlt">sediments</span> from the Ulleung Basin</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Briggs, Brandon R; Graw, Michael; Brodie, Eoin L</p> <p>2013-11-01</p> <p>The biogeochemical processes that occur in marine <span class="hlt">sediments</span> on continental margins are complex; however, from one perspective they can be considered with respect to three geochemical <span class="hlt">zones</span> based on the presence and form of methane: sulfate–methane transition (SMTZ), gas hydrate stability <span class="hlt">zone</span> (GHSZ), and free gas <span class="hlt">zone</span> (FGZ). These geochemical <span class="hlt">zones</span> may harbor distinct microbial communities that are important in biogeochemical carbon cycles. The objective of this study was to describe the microbial communities in <span class="hlt">sediments</span> from the SMTZ, GHSZ, and FGZ using molecular ecology methods (i.e. PhyloChip microarray analysis and terminal restriction fragment length polymorphism (T-RFLP)) and examining themore » results in the context of non-biological parameters in the <span class="hlt">sediments</span>. Non-metric multidimensional scaling and multi-response permutation procedures were used to determine whether microbial community compositions were significantly different in the three geochemical <span class="hlt">zones</span> and to correlate samples with abiotic characteristics of the <span class="hlt">sediments</span>. This analysis indicated that microbial communities from all three <span class="hlt">zones</span> were distinct from one another and that variables such as sulfate concentration, hydrate saturation of the nearest gas hydrate layer, and depth (or unmeasured variables associated with depth e.g. temperature, pressure) were correlated to differences between the three <span class="hlt">zones</span>. The archaeal anaerobic methanotrophs typically attributed to performing anaerobic oxidation of methane were not detected in the SMTZ; however, the marine benthic group-B, which is often found in SMTZ, was detected. Within the GHSZ, samples that were typically closer to layers that contained higher hydrate saturation had indicator sequences related to Vibrio-type taxa. These results suggest that the biogeographic patterns of microbial communities in marine <span class="hlt">sediments</span> are distinct based on geochemical <span class="hlt">zones</span> defined by methane.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26937632','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26937632"><span>Agar <span class="hlt">Sediment</span> Test for Assessing the Suitability of Organic Waste Streams for <span class="hlt">Recovering</span> Nutrients by the Aquatic Worm Lumbriculus variegatus.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Laarhoven, Bob; Elissen, H J H; Temmink, H; Buisman, C J N</p> <p>2016-01-01</p> <p>An agar <span class="hlt">sediment</span> test was developed to evaluate the suitability of organic waste streams from the food industry for <span class="hlt">recovering</span> nutrients by the aquatic worm Lumbriculus variegatus (Lv). The effects of agar gel, sand, and food quantities in the <span class="hlt">sediment</span> test on worm growth, reproduction, and water quality were studied. Agar gel addition ameliorated growth conditions by reducing food hydrolysis and altering <span class="hlt">sediment</span> structure. Best results for combined reproduction and growth were obtained with 0.6% agar-gel (20 ml), 10 g. fine sand, 40 g. coarse sand, and 105 mg fish food (Tetramin). With agar gel, ingestion and growth is more the result of addition of food in its original quality. Final tests with secondary potato starch sludge and wheat bran demonstrated that this test is appropriate for the comparison of solid feedstuffs and suspended organic waste streams. This test method is expected to be suitable for organic waste studies using other <span class="hlt">sediment</span> dwelling invertebrates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4777450','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4777450"><span>Agar <span class="hlt">Sediment</span> Test for Assessing the Suitability of Organic Waste Streams for <span class="hlt">Recovering</span> Nutrients by the Aquatic Worm Lumbriculus variegatus</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Laarhoven, Bob; Elissen, H. J. H.; Temmink, H.; Buisman, C. J. N.</p> <p>2016-01-01</p> <p>An agar <span class="hlt">sediment</span> test was developed to evaluate the suitability of organic waste streams from the food industry for <span class="hlt">recovering</span> nutrients by the aquatic worm Lumbriculus variegatus (Lv). The effects of agar gel, sand, and food quantities in the <span class="hlt">sediment</span> test on worm growth, reproduction, and water quality were studied. Agar gel addition ameliorated growth conditions by reducing food hydrolysis and altering <span class="hlt">sediment</span> structure. Best results for combined reproduction and growth were obtained with 0.6% agar-gel (20 ml), 10 g. fine sand, 40 g. coarse sand, and 105 mg fish food (Tetramin). With agar gel, ingestion and growth is more the result of addition of food in its original quality. Final tests with secondary potato starch sludge and wheat bran demonstrated that this test is appropriate for the comparison of solid feedstuffs and suspended organic waste streams. This test method is expected to be suitable for organic waste studies using other <span class="hlt">sediment</span> dwelling invertebrates. PMID:26937632</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24379809','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24379809"><span>Fe-phyllosilicate redox cycling organisms from a redox transition <span class="hlt">zone</span> in Hanford 300 Area <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Benzine, Jason; Shelobolina, Evgenya; Xiong, Mai Yia; Kennedy, David W; McKinley, James P; Lin, Xueju; Roden, Eric E</p> <p>2013-01-01</p> <p>Microorganisms capable of reducing or oxidizing structural iron (Fe) in Fe-bearing phyllosilicate minerals were enriched and isolated from a subsurface redox transition <span class="hlt">zone</span> at the Hanford 300 Area site in eastern Washington, USA. Both conventional and in situ "i-chip" enrichment strategies were employed. One Fe(III)-reducing Geobacter (G. bremensis strain R1, Deltaproteobacteria) and six Fe(II) phyllosilicate-oxidizing isolates from the Alphaproteobacteria (Bradyrhizobium japonicum strains 22, is5, and in8p8), Betaproteobacteria (Cupriavidus necator strain A5-1, Dechloromonas agitata strain is5), and Actinobacteria (Nocardioides sp. strain in31) were <span class="hlt">recovered</span>. The G. bremensis isolate grew by oxidizing acetate with the oxidized form of NAu-2 smectite as the electron acceptor. The Fe(II)-oxidizers grew by oxidation of chemically reduced smectite as the energy source with nitrate as the electron acceptor. The Bradyrhizobium isolates could also carry out aerobic oxidation of biotite. This is the first report of the recovery of a Fe(II)-oxidizing Nocardioides, and to date only one other Fe(II)-oxidizing Bradyrhizobium is known. The 16S rRNA gene sequences of the isolates were similar to ones found in clone libraries from Hanford 300 <span class="hlt">sediments</span> and groundwater, suggesting that such organisms may be present and active in situ. Whole genome sequencing of the isolates is underway, the results of which will enable comparative genomic analysis of mechanisms of extracellular phyllosilicate Fe redox metabolism, and facilitate development of techniques to detect the presence and expression of genes associated with microbial phyllosilicate Fe redox cycling in <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3863755','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3863755"><span>Fe-phyllosilicate redox cycling organisms from a redox transition <span class="hlt">zone</span> in Hanford 300 Area <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Benzine, Jason; Xiong, Mai Yia; Kennedy, David W.; McKinley, James P.; Lin, Xueju; Roden, Eric E.</p> <p>2013-01-01</p> <p>Microorganisms capable of reducing or oxidizing structural iron (Fe) in Fe-bearing phyllosilicate minerals were enriched and isolated from a subsurface redox transition <span class="hlt">zone</span> at the Hanford 300 Area site in eastern Washington, USA. Both conventional and in situ “i-chip” enrichment strategies were employed. One Fe(III)-reducing Geobacter (G. bremensis strain R1, Deltaproteobacteria) and six Fe(II) phyllosilicate-oxidizing isolates from the Alphaproteobacteria (Bradyrhizobium japonicum strains 22, is5, and in8p8), Betaproteobacteria (Cupriavidus necator strain A5-1, Dechloromonas agitata strain is5), and Actinobacteria (Nocardioides sp. strain in31) were <span class="hlt">recovered</span>. The G. bremensis isolate grew by oxidizing acetate with the oxidized form of NAu-2 smectite as the electron acceptor. The Fe(II)-oxidizers grew by oxidation of chemically reduced smectite as the energy source with nitrate as the electron acceptor. The Bradyrhizobium isolates could also carry out aerobic oxidation of biotite. This is the first report of the recovery of a Fe(II)-oxidizing Nocardioides, and to date only one other Fe(II)-oxidizing Bradyrhizobium is known. The 16S rRNA gene sequences of the isolates were similar to ones found in clone libraries from Hanford 300 <span class="hlt">sediments</span> and groundwater, suggesting that such organisms may be present and active in situ. Whole genome sequencing of the isolates is underway, the results of which will enable comparative genomic analysis of mechanisms of extracellular phyllosilicate Fe redox metabolism, and facilitate development of techniques to detect the presence and expression of genes associated with microbial phyllosilicate Fe redox cycling in <span class="hlt">sediments</span>. PMID:24379809</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24561931','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24561931"><span><span class="hlt">Sedimentation</span> and associated trace metal enrichment in the riparian <span class="hlt">zone</span> of the Three Gorges Reservoir, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tang, Qiang; Bao, Yuhai; He, Xiubin; Zhou, Huaidong; Cao, Zhijing; Gao, Peng; Zhong, Ronghua; Hu, Yunhua; Zhang, Xinbao</p> <p>2014-05-01</p> <p>Impoundment of the Three Gorges Reservoir has created an artificial riparian <span class="hlt">zone</span> with a vertical height of 30 m and a total area of 349 km(2), which has been subjected to seasonal inundation and exposure due to regular reservoir impoundment and the occurrence of natural floods. The significant alteration of hydrologic regime has caused numerous environmental changes. The present study investigated the magnitude and spatial pattern of <span class="hlt">sedimentation</span> and metal enrichment in a typical section of the riparian <span class="hlt">zone</span>, composed of bench terraces with previous agricultural land uses, and explored their links to the changed hydrologic regime. In particular, we measured the total <span class="hlt">sediment</span> depths and collected surface riparian <span class="hlt">sediments</span> and down-profile sectioned riparian soils (at 5 cm intervals) for trace metal determination. Our analysis showed that the annual average <span class="hlt">sedimentation</span> rates varied from 0.5 to 10 cm·yr(-1) and they decreased significantly with increasing elevation. This lateral distribution was principally attributed to seasonal variations in water levels and suspended <span class="hlt">sediment</span> concentrations. Enriched concentrations of trace metals were found both in the riparian <span class="hlt">sediments</span> and soils, but they were generally higher in the riparian <span class="hlt">sediments</span> than in riparian soils and followed a similar lateral decreasing trend. Metal contamination assessment showed that the riparian <span class="hlt">sediments</span> were slightly contaminated by Ni, Zn, and Pb, moderately contaminated by Cu, and moderately to strongly contaminated by Cd; while riparian soils were slightly contaminated by As, and moderately contaminated by Cd. Trace metal enrichment in the riparian <span class="hlt">sediments</span> may be attributed to external input of contaminated <span class="hlt">sediments</span> produced from upstream anthropogenic sources and chemical adsorption from dissolved fractions during pure <span class="hlt">sediment</span> mobilization and after sink for a prolonged flooding period due to reservoir impoundment. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_2 --> <div id="page_3" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="41"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B22B..04Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B22B..04Y"><span>Investigation of mechanical properties of hydrate-bearing pressure core <span class="hlt">sediments</span> <span class="hlt">recovered</span> from the Eastern Nankai Trough using transparent acrylic cell triaxial testing system (TACTT-system)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoneda, J.; Masui, A.; Konno, Y.; Jin, Y.; Kida, M.; Suzuki, K.; Nakatsuka, Y.; Tenma, N.; Nagao, J.</p> <p>2014-12-01</p> <p>Natural gas hydrate-bearing pressure core <span class="hlt">sediments</span> have been sheared in compression using a newly developed Transparent Acrylic Cell Triaxial Testing (TACTT) system to investigate the geophysical and geomechanical behavior of <span class="hlt">sediments</span> <span class="hlt">recovered</span> from the deep seabed in the Eastern Nankai Trough, the first Japanese offshore production test region. The <span class="hlt">sediments</span> were <span class="hlt">recovered</span> by hybrid pressure core system (hybrid PCS) and pressure cores were cut by pressure core analysis tools (PCATs) on board. These pressure cores were transferred to the AIST Hokkaido centre and trimmed by pressure core non-destructive analysis tools (PNATs) for TACTT system which maintained the pressure and temperature conditions within the hydrate stability boundary, through the entire process of core handling from drilling to the end of laboratory testing. An image processing technique was used to capture the motion of <span class="hlt">sediment</span> in a transparent acrylic cell, and digital photographs were obtained at every 0.1% of vertical strain during the test. Analysis of the optical images showed that <span class="hlt">sediments</span> with 63% hydrate saturation exhibited brittle failure, although nonhydrate-bearing <span class="hlt">sediments</span> exhibited ductile failure. In addition, the increase in shear strength with hydrate saturation increase of natural gas hydrate is in agreement with previous data from synthetic gas hydrate. This research was financially supported by the Research Consortium for Methane Hydrate Resources in Japan (MH21 Research Consortium) that carries out Japan's Methane Hydrate R&D Program by the Ministry of Economy, Trade and Industry (METI).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T43G..05R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T43G..05R"><span>Frictional behavior of carbonate-rich <span class="hlt">sediments</span> in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabinowitz, H. S.; Savage, H. M.; Carpenter, B. M.; Collettini, C.</p> <p>2015-12-01</p> <p>Carbonate-rich layers make up a significant component of subducting <span class="hlt">sediments</span> around the world and may impact the frictional behavior of subduction <span class="hlt">zones</span>. In order to investigate the effect of carbonate subduction, we conducted biaxial deformation experiments within a pressure vessel using the Brittle Rock deformAtion Versatile Apparatus (BRAVA) at INGV. We obtained input <span class="hlt">sediments</span> for two subduction <span class="hlt">zones</span>, the Hikurangi trench, New Zealand (ODP Site 1124) and the Peru trench (DSDP Site 321), which have carbonate/clay contents of ~40/60 wt% and ~80/20 wt%, respectively. Samples were saturated with distilled water mixed with 35g/l sea salt and deformed at room temperature. Experiments were conducted at σN = 1-50 MPa with sliding velocities of 1-300 μm/s and hold times of 1-1000 s. Frictional strength of Hikurangi gouge is 0.35-0.55 and Peru gouge is 0.55-0.65. Velocity-stepping tests show that the Hikurangi gouge is consistently velocity strengthening (friction rate parameter (a-b) > 0). The Peru gouge is mostly velocity strengthening but exhibits a minimum in a-b at the 3-10 μm/s velocity step (with velocity weakening behavior at 25 MPa, indicating the potential for earthquake nucleation). Slide-hold-slide tests show that the healing rate (β) of the Hikurangi gouge is 1x10-4-1x10-3 /decade which is comparable to that of clays (β~0.002 /decade) while the healing rate of Peru gouge (β~6x10-3-7x10-3 /decade) is closer to that of carbonate gouge (β~0.01 /decade). The mechanical results are complemented by microstructural analysis. In lower stress experiments, there is no obvious shear localization. At 25 and 50 MPa, pervasive boundary-parallel shears become dominant, particularly in the Peru samples. Degree of microstructural localization appears to correspond with the trends observed in velocity-dependence. Our preliminary results indicate that carbonate/clay compositions could have a significant impact on the frictional behavior of subducting <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24637449','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24637449"><span><span class="hlt">Recovering</span> low-turbidity cutting liquid from silicon slurry waste.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tsai, Tzu-Hsuan; Shih, Yu-Pei</p> <p>2014-04-30</p> <p>In order to <span class="hlt">recover</span> a low-turbidity polyalkylene glycol (PAG) liquid from silicon slurry waste by <span class="hlt">sedimentation</span>, temperatures were adjusted, and acetone, ethanol or water was used as a diluent. The experimental results show that the particles in the waste would aggregate and settle readily by using water as a diluent. This is because particle surfaces had lower surface potential value and weaker steric stabilization in PAG-water than in PAG-ethanol or PAG-acetone solutions. Therefore, water is the suggested diluent for <span class="hlt">recovering</span> a low-turbidity PAG (<100 NTU) by <span class="hlt">sedimentation</span>. After 50 wt.% water-assisted <span class="hlt">sedimentation</span> for 21 days, the solid content of the upper liquid reduced to 0.122 g/L, and the turbidity decreased to 44 NTU. The obtained upper liquid was then vacuum-distillated to remove water. The final <span class="hlt">recovered</span> PAG with 0.37 NTU had similar viscosity and density to the unused PAG and could be reused in the cutting process. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H14F..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H14F..04M"><span>Investigating the development of less-mobile porosity in realistic hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span> with COMSOL Multiphysics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MahmoodPoorDehkordy, F.; Briggs, M. A.; Day-Lewis, F. D.; Bagtzoglou, A. C.</p> <p>2017-12-01</p> <p>Although hyporheic <span class="hlt">zones</span> are often modeled at the reach scale as homogeneous "boxes" of exchange, heterogeneity caused by variations of pore sizes and connectivity is not uncommon. This heterogeneity leads to the creation of more- and less-mobile <span class="hlt">zones</span> of hydraulic exchange that influence reactive solute transport processes. Whereas fluid sampling is generally sensitive to more-mobile <span class="hlt">zones</span>, geoelectrical measurement is sensitive to ionic tracer dynamics in both less- and more-mobile <span class="hlt">zones</span>. Heterogeneity in pore connectivity leads to a lag between fluid and bulk electrical conductivity (EC) resulting in a hysteresis loop, observed during tracer breakthrough tests, that contains information about the less-mobile porosity attributes of the medium. Here, we present a macro-scale model of solute transport and electrical conduction developed using COMSOL Multiphysics. The model is used to simulate geoelectrical monitoring of ionic transport for bed <span class="hlt">sediments</span> based on (1) a stochastic sand-and-cobble mixture and (2) a dune feature with strong permeability layering. In both of these disparate <span class="hlt">sediment</span> types, hysteresis between fluid and bulk EC is observed, and depends in part on fluid flux rate through the model domain. Using the hysteresis loop, the ratio of less-mobile to mobile porosity and mass-transfer coefficient are estimated graphically. The results indicate the presence and significance of less-mobile porosity in the hyporheic <span class="hlt">zones</span> and demonstrate the capability of the proposed model to detect heterogeneity in flow processes and estimate less-mobile <span class="hlt">zone</span> parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004GeCoA..68.2649X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004GeCoA..68.2649X"><span>Speciation of strontium in particulates and <span class="hlt">sediments</span> from the Mississippi River mixing <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Yingfeng; Marcantonio, Franco</p> <p>2004-06-01</p> <p>Sequential extractions were performed on small amounts of particulate and <span class="hlt">sediment</span> samples (6 to10 mg) from the Mississippi River mixing <span class="hlt">zone</span>. The leachates were analyzed for Sr concentration and 87Sr/ 86Sr isotope ratio. Mn and Fe contents were also measured as their oxyhydroxides are potential carrier phases for Sr. The largest fraction of Sr in the solid phase (particulates and <span class="hlt">sediments</span>) was found to be present in the residual, refractory fraction (>70% of total). By comparison with the corresponding <span class="hlt">sediment</span>, particulates appear to have higher concentrations of nonresidual, labile Sr (30% vs. 15%). Carbonate components seem to play an important role as carriers for labile Sr in particulates and <span class="hlt">sediments</span>. Changes in the composition and content of the solid phase may significantly modify both the 87Sr/ 86Sr isotope ratio of the total labile fractions and that of the bulk components. However, such modifications, under normal conditions, exert little measurable influence on the Sr isotope composition of the dissolved phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014207','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014207"><span><span class="hlt">Sedimentation</span> across the central California oxygen minimum <span class="hlt">zone</span>: an alternative coastal upwelling sequence.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vercoutere, T.L.; Mullins, H.T.; McDougall, K.; Thompson, J.B.</p> <p>1987-01-01</p> <p>Distribution, abundance, and diversity of terrigenous, authigenous, and biogenous material provide evidence of the effect of bottom currents and oxygen minimum <span class="hlt">zone</span> (OMZ) on continental slope <span class="hlt">sedimentation</span> offshore central California. Three major OMZ facies are identified, along the upper and lower edges of OMZ and one at its core.-from Authors</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.S31C4407C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.S31C4407C"><span>Comparisons of Low-Strain Amplification at Soft-<span class="hlt">Sediment</span>, Hard-Rock, Topographic, and Fault-<span class="hlt">Zone</span> Sites in the Hayward Fault <span class="hlt">Zone</span>, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Catchings, R.; Strayer, L. M.; Goldman, M.</p> <p>2014-12-01</p> <p>We used a temporary network of approximately 600 seismographs to record a seismic source generated by the collapse of a 13-story building near the active trace of the Hayward Fault. These data allow us to evaluate variations in ground shaking across a series of 30 2-km-long radial arrays centered on the seismic source. Individual seismographs were spaced at 200-m intervals, forming a series of 360°concentric arrays around the seismic source. The data show variations in amplification caused by (1) soft <span class="hlt">sediments</span> within the East Bay alluvial plain (EBAP), (2) hard rocks within the East Bay hills (EBH), (3) low-velocity rocks within the Hayward Fault <span class="hlt">zone</span> (HFZ), and (4) topography. Given that ground shaking varies strongly with distance from the source, the concentric arrays allowed us to measure variations in ground shaking as a function of azimuth at fixed distances from the source. On individual linear profiles within the concentric arrays, we observed decreases in peak ground velocity (PGV) across the HFZ and other faults within the EBH. However, for a given distance from the source, we observe four to five fold amplification from the EBAP sites compared to most sites in the EBH. Topographic and fault-<span class="hlt">zone</span> amplification effects within the EBH, however, are greater than the EBAP <span class="hlt">sediment</span> amplification. Thus, for future earthquakes, shaking at many sites within the EBH may be significantly stronger than many sites within the EBAP. These observations suggest amplification can be expected in unconsolidated <span class="hlt">sediments</span>, but topographic and fault-<span class="hlt">zone</span> amplification can be larger. This confirms the importance of site effects for hazard mitigation and in interpreting MMI for future and historical earthquakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1172449-fe-ii-sulfide-facilitated-reduction-vii-o4-microbially-reduced-hyporheic-zone-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1172449-fe-ii-sulfide-facilitated-reduction-vii-o4-microbially-reduced-hyporheic-zone-sediments"><span>Fe(II)- and Sulfide-Facilitated Reduction of 99Tc(VII)O4- in Microbially Reduced Hyporheic <span class="hlt">Zone</span> <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Lee, Ji-Hoon; Zachara, John M.; Fredrickson, Jim K.</p> <p></p> <p>Redox-reactive, biogeochemical phases generated by reductive microbial activity in hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span> from a dynamic groundwater-river interaction <span class="hlt">zone</span> were evaluated for their ability to reduce soluble pertechnetate [99Tc(VII)O4-] to less soluble Tc(IV). The <span class="hlt">sediments</span> were bioreduced by indigenous microorganisms that were stimulated by organic substrate addition in synthetic groundwater with or without sulfate. In most treatments, 20 µmol L-1 initial aqueous Tc(VII) was reduced to near or below detection (3.82×10-9 mol L-1) over periods of days to months in suspensions of variable solids concentrations. Native <span class="hlt">sediments</span> containing significant lithogenic Fe(II) in various phases were, in contrast, unreactive with Tc(VII). Themore » reduction rates in the bioreduced <span class="hlt">sediments</span> increased with increases in <span class="hlt">sediment</span> mass, in proportion to weak acid-extractable Fe(II) and <span class="hlt">sediment</span>-associated sulfide (AVS). The rate of Tc(VII) reduction was first order with respect to both aqueous Tc(VII) concentration and <span class="hlt">sediment</span> mass, but correlations between specific reductant concentrations and reaction rate were not found. X-ray microprobe measurements revealed a strong correlation between Tc hot spots and Fe-containing mineral particles in the <span class="hlt">sediment</span>. However, only a portion of Fe-containing particles were Tc-hosts. The Tc-hot spots displayed a chemical signature (by EDXRF) similar to pyroxene. The application of autoradiography and electron microprobe allowed further isolation of Tc-containing particles that were invariably found to be ca 100 µm aggregates of primary mineral material embedded within a fine-grained phyllosilicate matrix. EXAFS spectroscopy revealed that the Tc(IV) within these were a combination of a Tc(IV)O2-like phase and Tc(IV)-Fe surface clusters, with a significant fraction of a TcSx-like phase in <span class="hlt">sediments</span> incubated with SO42-. AVS was implicated as a more selective reductant at low solids concentration even though its concentration was below</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeCoA.136..247L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeCoA.136..247L"><span>Fe(II)- and sulfide-facilitated reduction of 99Tc(VII)O4- in microbially reduced hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Ji-Hoon; Zachara, John M.; Fredrickson, James K.; Heald, Steve M.; McKinley, James P.; Plymale, Andrew E.; Resch, Charles T.; Moore, Dean A.</p> <p>2014-07-01</p> <p>Redox-reactive, biogeochemical phases generated by reductive microbial activity in hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span> from a dynamic groundwater-river interaction <span class="hlt">zone</span> were evaluated for their ability to reduce soluble pertechnetate [99Tc(VII)O4-] to less soluble Tc(IV). The <span class="hlt">sediments</span> were bioreduced by indigenous microorganisms that were stimulated by organic substrate addition in synthetic groundwater with or without sulfate. In most treatments, 20 μmol L-1 initial aqueous Tc(VII) was reduced to near or below detection (3.82 × 10-9 mol L-1) over periods of days to months in suspensions of variable solids concentrations. Native <span class="hlt">sediments</span> containing significant lithogenic Fe(II) in various phases were, in contrast, unreactive with Tc(VII). The reduction rates in the bioreduced <span class="hlt">sediments</span> increased with increases in <span class="hlt">sediment</span> mass, in proportion to weak acid-extractable Fe(II) and <span class="hlt">sediment</span>-associated sulfide (AVS). The rate of Tc(VII) reduction was first order with respect to both aqueous Tc(VII) concentration and <span class="hlt">sediment</span> mass, but correlations between specific reductant concentrations and reaction rate were not found. X-ray microprobe measurements revealed a strong correlation between Tc hot spots and Fe-containing mineral particles in the <span class="hlt">sediment</span>. However, only a portion of Fe-containing particles were Tc-hosts. The Tc-hot spots displayed a chemical signature (by EDXRF) similar to pyroxene. The application of autoradiography and electron microprobe allowed further isolation of Tc-containing particles that were invariably found to be ca 100 μm aggregates of primary mineral material embedded within a fine-grained phyllosilicate matrix. EXAFS spectroscopy revealed that the Tc(IV) within these were a combination of a Tc(IV)O2-like phase and Tc(IV)-Fe surface clusters, with a significant fraction of a TcSx-like phase in <span class="hlt">sediments</span> incubated with SO42-. AVS was implicated as a more selective reductant at low solids concentration even though its concentration was below that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015253','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015253"><span>The chemistry and mineralogy of haloed burrows in pelagic <span class="hlt">sediment</span> at DOMES Site A: The equatorial North Pacific</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Piper, D.Z.; Rude, P.D.; Monteith, S.</p> <p>1987-01-01</p> <p>The chemical and mineralogical composition of burrowed <span class="hlt">sediment</span>, <span class="hlt">recovered</span> in 66 box cores at latitude 9??25???N and longitude 151??15???W in the equatorial Pacific, demonstrates the important role of infauna in determining the geochemistry of pelagic <span class="hlt">sediment</span>. Haloed burrows, approximately 3 cm across, were present in many of the cores. Within early Tertiary <span class="hlt">sediment</span> that was covered by less than 5 cm of surface Quaternary <span class="hlt">sediment</span> in several cores, the burrows in cross-section consist of three units: (1) a dark yellowish-brown central <span class="hlt">zone</span> of Quaternary <span class="hlt">sediment</span> surrounded, by (2) a pale yellowish-orange <span class="hlt">zone</span> (the halo) of Tertiary <span class="hlt">sediment</span>, which is surrounded by (3) a metal-oxide precipitate; the enclosing Tertiary <span class="hlt">sediment</span> is dusky brown. Several elements - Mn, Ni, Cu, Co, Zn, Sb and Ce - have been leached from the light-colored halo, whereas Cr, Cs, Hf, Rb, Sc, Ta, Th, U, the rare earth elements exclusive of Ce, and the major oxides have not been leached. The metal-oxide <span class="hlt">zone</span>, 1-5 mm thick, contains as much as 16% MnO2, as the mineral todorokite. The composition of the todorokite, exclusive of the admixed Tertiary <span class="hlt">sediment</span>, resembles the composition of the metal deficit of the halo and also the composition of surface ferromanganese nodules that have been interpreted as having a predominantly diagenetic origin. Thus bioturbation contributes not only to the redistribution of metals within pelagic <span class="hlt">sediment</span>, but also to the accretion of ferromanganese nodules on the sea floor. ?? 1987.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1060656-experimental-study-diffusivity-technetium-hanford-vadose-zone-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1060656-experimental-study-diffusivity-technetium-hanford-vadose-zone-sediments"><span>An Experimental Study of Diffusivity of Technetium-99 in Hanford Vadose <span class="hlt">Zone</span> <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Mattigod, Shas V.; Bovaird, Chase C.; Wellman, Dawn M.</p> <p>2012-11-01</p> <p>One of the methods being considered at the Hanford site in Washington for safely disposing of low-level radioactive wastes (LLW) is to encase the waste in concrete and entomb the packages in the Hanford vadose <span class="hlt">zone</span> <span class="hlt">sediments</span>. The current plan for waste isolation consists of stacking low-level waste packages on a trench floor, surrounding the stacks with reinforced steel, and encasing these packages with concrete. Any failure of the concrete encasement may result in water intrusion and consequent mobilization of radionuclides from the waste packages. The mobilized radionuclides may escape from the encased concrete by mass flow and/or diffusion andmore » move into the surrounding subsurface <span class="hlt">sediments</span>. It is therefore necessary to conduct an assessment of the performance of the concrete encasement structure and the surrounding soil’s ability to retard radionuclide migration. The retardation factors for radionuclides contained in the waste packages can be determined from measurements of diffusion coefficients for these contaminants through concrete and fill material. Because of their anionic nature in aqueous solutions, the radionuclides, 99Tc and 129I were identified as long-term dose contributors in LLW. The leachability and/or diffusion of these radionuclide species must be measured in order to assess the long-term performance of waste grouts when contacted with vadose-<span class="hlt">zone</span> porewater or groundwater. To measure the diffusivity, a set of experiments were conducted using 99Tc-spiked concrete (with 0 and 4% metallic iron additions) in contact with unsaturated soil half-cells that reflected the typical moisture contents of Hanford vadose <span class="hlt">zone</span> <span class="hlt">sediments</span>. The 99Tc diffusion profiles in the soil half cells were measured after a time lapse of ~1.9 yr. Using the concentration profiles, the 99Tc diffusivity coefficients were calculated based on Fick’s Second Law.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP11A1994Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP11A1994Z"><span>Microbial Communities Associated with Phosphorite-bearing <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zoss, R.; Bailey, J.; Flood, B.; Jones, D. S.</p> <p>2016-12-01</p> <p>Phosphorus is a limiting nutrient in the environment and is an important component of many biological molecules. Calcium phosphate mineral deposits known as phosphorites, are also the primary source of P for agriculture. Understanding phosphorite formation may improve management of P resources. However, the processes that mediate calcium phosphate mineral precipitation in certain marine pore waters remain poorly understood. Phosphogenesis occurs in <span class="hlt">sediments</span> beneath some oceanic upwelling <span class="hlt">zones</span> that harbor polyphosphate-accumulating giant sulfur bacteria (GSB). These bacteria may concentrate phosphate in <span class="hlt">sediment</span> pore waters - creating supersaturated conditions with respect to apatite. However, the relationship between microbes and phosphogenesis is not fully resolved. To further study this relationship, we examined microbial communities from two sources: <span class="hlt">sediment</span> cores <span class="hlt">recovered</span> from the shelf of the Benguela region, and DNA extracted from washed phosphorites <span class="hlt">recovered</span> from those same <span class="hlt">sediments</span>. We used itag and clone library sequencing of the 16S rRNA gene to examine the microbial communities and their relationship with the environment. We found that many of our <span class="hlt">sediments</span> shared large numbers of phylotypes with one another, and that the same metabolic guilds were represented at localities across the shelf. Sulfur-reducing bacteria and sulfur-oxidizing bacteria were abundant in our datasets. Phylotypes that are known to carry out nitrification and/or anammox (anaerobic ammonia oxidation) were also well-represented. Our phosphorite extraction, however, contained a distinct microbial community from those observed in the modern <span class="hlt">sediments</span>. We observed both an enrichment of certain common microbial classes and a complete absence of others. These results could represent an ancient microbial assemblage that was present when the apatite precipitated. While these taxa may or may not have contributed to apatite precipitation, several groups represented in the phosphorite</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70157102','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70157102"><span>The role of suspension events in cross-shore and longshore suspended <span class="hlt">sediment</span> transport in the surf <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jaffe, Bruce E.</p> <p>2015-01-01</p> <p>Suspension of sand in the surf <span class="hlt">zone</span> is intermittent. Especially striking in a time series of concentration are periods of intense suspension, suspension events, when the water column suspended <span class="hlt">sediment</span> concentration is an order of magnitude greater than the mean concentration. The prevalence, timing, and contribution of suspension events to cross-shore and longshore suspended <span class="hlt">sediment</span> transport are explored using field data collected in the inner half of the surf <span class="hlt">zone</span> during a large storm at Duck, NC. Suspension events are defined as periods when the concentration is above a threshold. Events tended to occur during onshore flow under the wave crest, resulting in an onshore contribution to the suspended <span class="hlt">sediment</span> transport. Even though large events occurred less than 10 percent of the total time, at some locations onshore transport associated with suspension events was greater than mean-current driven offshore-directed transport during non-event periods, causing the net suspended <span class="hlt">sediment</span> transport to be onshore. Events and fluctuations in longshore velocity were not correlated. However, events did increase the longshore suspended <span class="hlt">sediment</span> transport by approximately the amount they increase the mean concentration, which can be up to 35%. Because of the lack of correlation, the longshore suspended <span class="hlt">sediment</span> transport can be modeled without considering the details of the intensity and time of events as the vertical integration of the product of the time-averaged longshore velocity and an event-augmented time-averaged concentration. However, to accurately model cross-shore suspended <span class="hlt">sediment</span> transport, the timing and intensity of suspension events must be reproduced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28965061','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28965061"><span>Bioavailability of trace metals in <span class="hlt">sediments</span> of a <span class="hlt">recovering</span> freshwater coastal wetland in China's Yellow River Delta, and risk assessment for the macrobenthic community.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Wei; Li, Xiaoxiao; Pei, Jun; Sun, Tao; Shao, Dongdong; Bai, Junhong; Li, Yanxia</p> <p>2017-12-01</p> <p>We investigated the speciation of trace metals and their ecological risks to macrobenthic communities in a <span class="hlt">recovering</span> coastal wetland of China's Yellow River Delta during the freshwater release project. We established 16 sampling sites in three restoration areas and one intertidal reference area, and collected <span class="hlt">sediments</span> and macrobenthos four times from 2014 to 2015. The instability index for the trace metals showed a moderate risk for Mn and a high risk for Cd. For both Mn and Cd, the carbonate and FeMn-bound fractions appear to contribute mostly to the instability and bioavailability indexes, but for Cd, the exchangeable fraction also have a much higher contribution. The bioavailability index indicated higher bioavailability of trace metals in freshwater restoration areas than that in the intertidal area. The single-factor contamination index indicated that most trace metal concentrations in the macrobenthos were in excess of the national standard. The biota-<span class="hlt">sediment</span> accumulation factor suggested that the macrobenthos accumulated most As, Cd, and Cu. Redundancy analysis showed clear relationships between the macrobenthos and <span class="hlt">sediment</span> metal concentrations. Our results will help wetland managers to assess the bioaccumulation risks based on metal speciation, and to improve management of these <span class="hlt">recovering</span> freshwater wetland ecosystems. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20337706','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20337706"><span>Prokaryotic functional diversity in different biogeochemical depth <span class="hlt">zones</span> in tidal <span class="hlt">sediments</span> of the Severn Estuary, UK, revealed by stable-isotope probing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Webster, Gordon; Rinna, Joachim; Roussel, Erwan G; Fry, John C; Weightman, Andrew J; Parkes, R John</p> <p>2010-05-01</p> <p>Stable isotope probing of prokaryotic DNA was used to determine active prokaryotes using (13)C-labelled substrates (glucose, acetate, CO(2)) in <span class="hlt">sediment</span> slurries from different biogeochemical <span class="hlt">zones</span> of the Severn Estuary, UK. Multiple, low concentrations (5 x 100 microM) of (13)C-substrate additions and short-term incubations (7 days) were used to minimize changes in the prokaryotic community, while achieving significant (13)C-incorporation. Analysis demonstrated clear metabolic activity within all slurries, although neither the net sulphate removal nor CH(4) production occurred in the anaerobic sulphate reduction and methanogenesis <span class="hlt">zone</span> slurries. Some similarities occurred in the prokaryotic populations that developed in different <span class="hlt">sediment</span> slurries, particularly in the aerobic and dysaerobic <span class="hlt">zone</span> slurries with (13)C-glucose, which were dominated by Gammaproteobacteria and Marine Group 1 Archaea, whereas both anaerobic <span class="hlt">sediment</span> slurries incubated with (13)C-acetate showed incorporation into Epsilonproteobacteria and other bacteria, with the sulphate reduction <span class="hlt">zone</span> slurry also showing (13)C-acetate utilization by Miscellaneous Crenarchaeotic Group Archaea. The lower potential energy methanogenesis <span class="hlt">zone</span> slurries were the only conditions where no (13)C-incorporation into Archaea occurred, despite Bacteria being labelled; this was surprising because Archaea have been suggested to be adapted to low-energy conditions. Overall, our results highlight that uncultured prokaryotes play important ecological roles in tidal <span class="hlt">sediments</span> of the Severn Estuary, providing new metabolic information for novel groups of Archaea and suggesting broader metabolisms for largely uncultivated Bacteria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18..858O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18..858O"><span>The undatables: Quantifying uncertainty in a highly expanded Late Glacial-Holocene <span class="hlt">sediment</span> sequence <span class="hlt">recovered</span> from the deepest Baltic Sea basin—IODP Site M0063</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Obrochta, S. P.; Andrén, T.; Fazekas, S. Z.; Lougheed, B. C.; Snowball, I.; Yokoyama, Y.; Miyairi, Y.; Kondo, R.; Kotilainen, A. T.; Hyttinen, O.; Fehr, A.</p> <p>2017-03-01</p> <p>Laminated, organic-rich silts and clays with high dissolved gas content characterize <span class="hlt">sediments</span> at IODP Site M0063 in the Landsort Deep, which at 459 m is the deepest basin in the Baltic Sea. Cores <span class="hlt">recovered</span> from Hole M0063A experienced significant expansion as gas was released during the recovery process, resulting in high <span class="hlt">sediment</span> loss. Therefore, during operations at subsequent holes, penetration was reduced to 2 m per 3.3 m core, permitting expansion into 1.3 m of initially empty liner. Fully filled liners were <span class="hlt">recovered</span> from Holes B through E, indicating that the length of <span class="hlt">recovered</span> intervals exceeded the penetrated distance by a factor of >1.5. A typical down-core logarithmic trend in gamma density profiles, with anomalously low-density values within the upper ˜1 m of each core, suggests that expansion primarily occurred in this upper interval. Thus, we suggest that a simple linear correction is inappropriate. This interpretation is supported by anisotropy of magnetic susceptibility data that indicate vertical stretching in the upper ˜1.5 m of expanded cores. Based on the mean gamma density profiles of cores from Holes M0063C and D, we obtain an expansion function that is used to adjust the depth of each core to conform to its known penetration. The variance in these profiles allows for quantification of uncertainty in the adjusted depth scale. Using a number of bulk 14C dates, we explore how the presence of multiple carbon source pathways leads to poorly constrained radiocarbon reservoir age variability that significantly affects age and <span class="hlt">sedimentation</span> rate calculations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19943108','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19943108"><span>Harmonised framework for ecological risk assessment of <span class="hlt">sediments</span> from ports and estuarine <span class="hlt">zones</span> of North and South Atlantic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choueri, R B; Cesar, A; Abessa, D M S; Torres, R J; Riba, I; Pereira, C D S; Nascimento, M R L; Morais, R D; Mozeto, A A; DelValls, T A</p> <p>2010-04-01</p> <p>This paper presents a harmonised framework of <span class="hlt">sediment</span> quality assessment and dredging material characterisation for estuaries and port <span class="hlt">zones</span> of North and South Atlantic. This framework, based on the weight-of-evidence approach, provides a structure and a process for conducting <span class="hlt">sediment</span>/dredging material assessment that leads to a decision. The main structure consists of "step 1" (examination of available data); "step 2" (chemical characterisation and toxicity assessment); "decision 1" (any chemical level higher than reference values? are <span class="hlt">sediments</span> toxic?); "step 3" (assessment of benthic community structure); "step 4" (integration of the results); "decision 2" (are <span class="hlt">sediments</span> toxic or benthic community impaired?); "step 5" (construction of the decision matrix) and "decision 3" (is there environmental risk?). The sequence of assessments may be interrupted when the information obtained is judged to be sufficient for a correct characterisation of the risk posed by the <span class="hlt">sediments</span>/dredging material. This framework brought novel features compared to other <span class="hlt">sediment</span>/dredging material risk assessment frameworks: data integration through multivariate analysis allows the identification of which samples are toxic and/or related to impaired benthic communities; it also discriminates the chemicals responsible for negative biological effects; and the framework dispenses the use of a reference area. We demonstrated the successful application of this framework in different port and estuarine <span class="hlt">zones</span> of the North (Gulf of Cádiz) and South Atlantic (Santos and Paranaguá Estuarine Systems).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS44A..07Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS44A..07Y"><span>Hydro-mechanical properties of pressure core <span class="hlt">sediments</span> <span class="hlt">recovered</span> from the Krishna-Godavari Basin during India's National Gas Hydrate Program Expedition NGHP-02</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yoneda, J.; Oshima, M.; Kida, M.; Kato, A.; Konno, Y.; Jin, Y.; Waite, W. F.; Jang, J.; Kumar, P.; Tenma, N.</p> <p>2017-12-01</p> <p>Pressure coring and analysis technology allows for gas hydrate to be <span class="hlt">recovered</span> from the deep seabed, transferred to the laboratory and characterized while continuously maintaining gas hydrate stability. For this study, dozens of hydrate-bearing pressure core <span class="hlt">sediment</span> subsections <span class="hlt">recovered</span> from the Krishna-Godavari Basin during India's National Gas Hydrate Program Expedition NGHP-02 were tested with Pressure Core Non-destructive Analysis Tools (PNATs) through a collaboration between Japan and India. PNATs, originally developed by AIST as a part of the Japanese National hydrate research program (MH21, funded by METI) conducted permeability, compression and consolidation tests under various effective stress conditions, including the in situ stress state estimated from downhole bulk density measurements. At the in situ effective stress, gas hydrate-bearing <span class="hlt">sediments</span> had an effective permeability range of 0.01-10mD even at pore-space hydrate saturations above 60%. Permeability increased by 10 to 100 times after hydrate dissociation at the same effective stress, but these post-dissociation gains were erased when effective stress was increased from in situ values ( 1 MPa) to 10MPa in a simulation of the depressurization method for methane extraction from hydrate. Vertical-to-horizontal permeability anisotropy was also investigated. First-ever multi-stage loading tests and strain-rate alternation compression tests were successfully conducted for evaluating <span class="hlt">sediment</span> strengthening dependence on the rate and magnitude of effective confining stress changes. In addition, oedometer tests were performed up to 40MPa of consolidation stress to simulate the depressurization method in ultra-deep sea environments. Consolidation curves measured with and without gas hydrate were investigated over a wide range of effective confining stresses. Compression curves for gas hydrate-bearing <span class="hlt">sediments</span> were convex downward due to high hydrate saturations. Consolidation tests show that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.B11B0015M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.B11B0015M"><span>Simultaneous measurement for thermal conductivity, diffusivity, and specific heat of methane hydrate bearing <span class="hlt">sediments</span> <span class="hlt">recovered</span> from Nankai-Trough wells</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muraoka, M.; Ohtake, M.; Susuki, N.; Yamamoto, Y.; Suzuki, K.; Tsuji, T.</p> <p>2014-12-01</p> <p>This study presents the results of the measurements of the thermal constants of natural methane-hydrate-bearing <span class="hlt">sediments</span> samples <span class="hlt">recovered</span> from the Tokai-oki test wells (Nankai-Trough, Japan) in 2004. The thermal conductivity, thermal diffusivity, and specific heat of the samples were simultaneously determined using the hot-disk transient method. The thermal conductivity of natural hydrate-bearing <span class="hlt">sediments</span> decreases slightly with increasing porosity. In addition, the thermal diffusivity of hydrate-bearing <span class="hlt">sediment</span> decrease as porosity increases. We also used simple models to calculate the thermal conductivity and thermal diffusivity. The results of the distribution model (geometric-mean model) are relatively consistent with the measurement results. In addition, the measurement results are consistent with the thermal diffusivity, which is estimated by dividing the thermal conductivity obtained from the distribution model by the specific heat obtained from the arithmetic mean. In addition, we discuss the relation between the thermal conductivity and mineral composition of core samples in conference. Acknowledgments. This work was financially supported by MH21 Research Consortium for Methane Hydrate Resources in Japan on the National Methane Hydrate Exploitation Program planned by the Ministry of Economy, Trade and Industry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034394','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034394"><span>The dark side of the hyporheic <span class="hlt">zone</span>: Depth profiles of nitrogen and its processing in stream <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stelzer, R.S.; Bartsch, L.A.; Richardson, W.B.; Strauss, E.A.</p> <p>2011-01-01</p> <p>1.Although it is well known that <span class="hlt">sediments</span> can be hot spots for nitrogen transformation in streams, many previous studies have confined measurements of denitrification and nitrate retention to shallow <span class="hlt">sediments</span> (<5cm deep). We determined the extent of nitrate processing in deeper <span class="hlt">sediments</span> of a sand plains stream (Emmons Creek) by measuring denitrification in core sections to a depth of 25cm and by assessing vertical nitrate profiles, with peepers and piezometers, to a depth of 70cm. 2.Denitrification rates of <span class="hlt">sediment</span> slurries based on acetylene block were higher in shallower core sections. However, core sections deeper than 5cm accounted for 68% of the mean depth-integrated denitrification rate. 3.Vertical hydraulic gradient and vertical profiles of pore water chloride concentration suggested that deep ground water upwelled through shallow <span class="hlt">sediments</span> before discharging to the stream channel. The results of a two-source mixing model based on chloride concentrations suggested that the hyporheic <span class="hlt">zone</span> was very shallow (<5cm) in Emmons Creek. 4.Vertical profiles showed that nitrate concentration in shallow ground water was about 10-60% of the nitrate concentration of deep ground water. The mean nitrate concentrations of deep and shallow ground water were 2.17 and 0.73mgNO3-NL-1, respectively. 5.Deep ground water tended to be oxic (6.9mgO2L-1) but approached anoxia (0.8mgO2L-1) after passing through shallow, organic carbon-rich <span class="hlt">sediments</span>, which suggests that the decline in the nitrate concentrations of upwelling ground water was because of denitrification. 6.Collectively, our results suggest that there is substantial nitrate removal occurring in deep <span class="hlt">sediments</span>, below the hyporheic <span class="hlt">zone</span>, in Emmons Creek. Our findings suggest that not accounting for nitrate removal in deep <span class="hlt">sediments</span> could lead to underestimates of nitrogen processing in streams and catchments. ?? 2011 Blackwell Publishing Ltd.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..122a2101W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..122a2101W"><span>The relation of <span class="hlt">sediment</span> texture to macro- and microplastic abundance in intertidal <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wahyuningsih, H.; Bangun, A. P.; Muhtadi, A.</p> <p>2018-02-01</p> <p>The intertidal <span class="hlt">zone</span> is a waters area directly affected by the contamination of plastic debris from land and sea. The aim of this research were to analyze the relation of <span class="hlt">sediment</span> texture to macro- and micro plastic abundance and also to determine appropriate management strategy. This research was conducted in intertidal <span class="hlt">zone</span> Jaring Halus Village Langkat Regency North Sumatera Province on February-April 2017. Plastic debris was collected using quadrat transect. <span class="hlt">Sediment</span> was collected with correct, up to a depth of least 30 cm. Abundance of micro plastic in Station 1 were positively tolerated with clay (0.509), and silt (0.787) and negatively correlations with sand (0.709) Station 2 were positively correlations with sand (0.645) and negatively correlations with clay (0.575), and silt (0.626) Station 3 were positively correlations with clay (0.435), and silt (0.466) and negatively correlations with sand (0.599). The abundance of microplastic was positively correlations with the abundance of microplastic (0.765). Microplastic density is directly proportional to the content of clay and dust. The higher the clay and dust content the higher the micro plastic density.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=275176&Lab=NHEERL&keyword=recycling&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=275176&Lab=NHEERL&keyword=recycling&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Microbial respiration and extracellular enzyme activity in <span class="hlt">sediments</span> from the Gulf of Mexico hypoxic <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>This study explores the relationship between <span class="hlt">sediment</span> chemistry (TC, TN, TP) and microbial respiration (DHA) and extracellular enzyme activity (EEA) across the Gulf of Mexico (GOM) hypoxic <span class="hlt">zone</span>. TC, TN, and TP were all positively correlated with each other (r=0.19-0.68). DHA was ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1427927-redox-transformation-reductive-immobilization-cr-vi-columbia-river-hyporheic-zone-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1427927-redox-transformation-reductive-immobilization-cr-vi-columbia-river-hyporheic-zone-sediments"><span>Redox transformation and reductive immobilization of Cr(VI) in the Columbia River hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Xu, Fen; Liu, Yuanyuan; Zachara, John</p> <p></p> <p>An experimental and modeling study was conducted to investigate the redox transformation and reductive immobilization of groundwater contaminant Cr in hyporheic <span class="hlt">zone</span> (HZ) <span class="hlt">sediments</span> from U.S. Department of Energy’s Hanford site, where groundwater Cr(VI) is migrating and discharging to the nearby Columbia River. Experimental results revealed that Cr(VI) can be reduced to immobile reduced Cr by the HZ <span class="hlt">sediments</span> in the presence/absence of O2. Anaerobic pre-incubation of the <span class="hlt">sediments</span> increased the effective rate of Cr reduction that was correlated with the increase in HCl-extractable Fe(II) content in the <span class="hlt">sediments</span>. The reduced Cr was stable in exposure to O2 under field-relevantmore » pH (~7.5) and Mn-containing (~0.02% w/w) conditions. The Cr(VI) reduction rate showed a multi-rate behavior, apparently reflecting the presence of reductants with different reactivity in the <span class="hlt">sediments</span>. The results from this study indicated that the HZ <span class="hlt">sediments</span> can reductively immobilize Cr and the <span class="hlt">sediment</span> redox capacity can be recharged through microbial activities. The results implied that HZ can play a role as a natural permeable redox barrier for removing groundwater Cr before it discharges into a river system.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JHyd..555..278X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JHyd..555..278X"><span>Redox transformation and reductive immobilization of Cr(VI) in the Columbia River hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Fen; Liu, Yuanyuan; Zachara, John; Bowden, Mark; Kennedy, David; Plymale, Andrew E.; Liu, Chongxuan</p> <p>2017-12-01</p> <p>An experimental and modeling study was conducted to investigate the redox transformation and reductive immobilization of groundwater contaminant Cr in hyporheic <span class="hlt">zone</span> (HZ) <span class="hlt">sediments</span> from U.S. DOE's Hanford Site, where groundwater Cr(VI) is migrating and discharging to the nearby Columbia River. Experimental results revealed that Cr(VI) can be reduced and immobilized by the HZ <span class="hlt">sediments</span> in the presence/absence of O2. Anaerobic pre-incubation of the <span class="hlt">sediments</span> increased the effective rate of Cr reduction that was correlated with the increase in HCl-extractable Fe(II) content in the <span class="hlt">sediments</span>. The reduced Cr was stable when exposed to O2 under field-relevant pH (7.5) with and without dissolved Mn(II), which might be oxidized to form Mn(III/IV) oxides that may oxidize reduced Cr. The Cr(VI) reduction rate showed a multi-rate behavior, apparently reflecting the presence of reductants with different reactivity in the <span class="hlt">sediments</span>. The results from this study indicated that the HZ <span class="hlt">sediments</span> can reductively immobilize Cr and the <span class="hlt">sediment</span> redox capacity can be recharged through microbial activities. The results implied that HZ can play a role as a natural permeable redox barrier for removing groundwater Cr before it discharges into a river system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51D2900H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51D2900H"><span>Seismic velocity structure of the <span class="hlt">sediment</span> seaward of Cascadia Subduction <span class="hlt">Zone</span> deformation front</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, S.; Gibson, J. C.; Carbotte, S. M.; Canales, J. P.; Nedimovic, M. R.; Carton, H. D.</p> <p>2015-12-01</p> <p>We present seismic velocity structure of the <span class="hlt">sediment</span> section seaward of the Cascadia Subduction <span class="hlt">Zone</span> deformation front (DF), derived from multichannel seismic data acquired during the 2012 Juan de Fuca Ridge to Trench experiment. Detailed velocity analyses are conducted on every 100th prestack-time-migrated common reflection point gather (625 m spacing) within 45 km seaward of the DF along two ridge-to-trench transects offshore Oregon at 44.6˚N and Washington at 47.4˚N respectively, and on every 200th common mid-point gather (1250 m spacing) along a ~400 km-long trench-parallel transect ~15 km from the DF. We observe a landward increase of <span class="hlt">sediment</span> velocity starting from ~15-20 km from the DF on both Oregon and Washington transects, which may result from increased horizontal compressive tectonic stress within the accretionary wedge and thermally induced dehydration processes in the <span class="hlt">sediment</span> column. Although the velocity of near-basement <span class="hlt">sediments</span> at 30 km from the DF is similar (~3.1 km/s) on both transects, the velocity increases are larger on the Washington transect, to ~4.0 km/s beneath the DF (<span class="hlt">sediment</span> thickness ~3.2 km), than on the Oregon transect, to ~3.6 km/s beneath the DF (<span class="hlt">sediment</span> thickness ~3.5 km). The long-wavelength <span class="hlt">sediment</span> velocity structure on the trench-parallel transect confirms this regional difference in deep <span class="hlt">sediment</span> velocity and also highlights variations related to a group of WNW-trending strike-slip faults along the margin. Offshore Washington, where higher <span class="hlt">sediment</span> velocity seaward of the DF is observed, the accretionary wedge is wide with a decollement located close to the basement and landward-verging thrust faults. By contrast, offshore Oregon, the lower <span class="hlt">sediment</span> velocity seaward of the DF is associated with a narrow accretionary wedge, a shallow decollement ~1 km above the basement, and seaward-verging thrust faults. The regional differences in deep <span class="hlt">sediment</span> velocity may be related to the along-strike variation in <span class="hlt">sediment</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011GeCoA..75.3581H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011GeCoA..75.3581H"><span>A cryptic sulfur cycle driven by iron in the methane <span class="hlt">zone</span> of marine <span class="hlt">sediment</span> (Aarhus Bay, Denmark)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holmkvist, Lars; Ferdelman, Timothy G.; Jørgensen, Bo Barker</p> <p>2011-06-01</p> <p>Sulfate reduction and sulfur-iron geochemistry were studied in 5-6 m deep gravity cores of Holocene mud from Aarhus Bay (Denmark). A goal was to understand whether sulfate is generated by re-oxidation of sulfide throughout the sulfate and methane <span class="hlt">zones</span>, which might explain the abundance of active sulfate reducers deep below the main sulfate <span class="hlt">zone</span>. Sulfate penetrated down to 130 cm where methane started to build up and where the concentration of free sulfide peaked at 5.5 mM. Below this sulfate-methane transition, sulfide diffused downwards to a sulfidization front at 520 cm depth, below which dissolved iron, Fe 2+, accumulated in the pore water. Sulfate reduction rates measured by 35S-tracer incubations in the sulfate <span class="hlt">zone</span> were high due to high concentrations of reactive organic matter. Within the sulfate-methane transition, sulfate reduction was distinctly stimulated by the anaerobic oxidation of methane. In the methane <span class="hlt">zone</span> below, sulfate remained at positive "background" concentrations of <0.5 mM down to the sulfidization front. Sulfate reduction decreased steeply to rates which at 300-500 cm depth were 0.2-1 pmol SO 42- cm -3 d -1, i.e., 4-5 orders of magnitude lower than rates measured near the <span class="hlt">sediment</span> surface. The turn-over time of sulfate increased from 3 years at 12 cm depth to 100-1000 years down in the methane <span class="hlt">zone</span>. Sulfate reduction in the methane <span class="hlt">zone</span> accounted for only 0.1% of sulfate reduction in the entire <span class="hlt">sediment</span> column and was apparently limited by the low pore water concentration of sulfate and the low availability of organic substrates. Amendment of the <span class="hlt">sediment</span> with both sulfate and organic substrates immediately caused a 10- to 40-fold higher, "potential sulfate reduction" which showed that a physiologically intact community of sulfate reducing bacteria was present. The "background" sulfate concentration appears to be generated from the reaction of downwards diffusing sulfide with deeply buried Fe(III) species, such as poorly-reactive iron</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27802871','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27802871"><span>Nutrient fluxes across <span class="hlt">sediment</span>-water interface in Bohai Bay Coastal <span class="hlt">Zone</span>, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mu, Di; Yuan, Dekui; Feng, Huan; Xing, Fangwei; Teo, Fang Yenn; Li, Shuangzhao</p> <p>2017-01-30</p> <p><span class="hlt">Sediment</span> cores and overlying water samples were collected at four sites in Tianjin Coastal <span class="hlt">Zone</span>, Bohai Bay, to investigate nutrient (N, P and Si) exchanges across the <span class="hlt">sediment</span>-water interface. The exchange fluxes of each nutrient species were estimated based on the porewater profiles and laboratory incubation experiments. The results showed significant differences between the two methods, which implied that molecular diffusion alone was not the dominant process controlling nutrient exchanges at these sites. The impacts of redox conditions and bioturbation on the nutrient fluxes were confirmed by the laboratory incubation experiments. The results from this study showed that the nutrient fluxes measured directly from the incubation experiment were more reliable than that predicted from the porewater profiles. The possible impacts causing variations in the nutrient fluxes include sewage discharge and land reclamation. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4427P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4427P"><span>Hyporheic <span class="hlt">zone</span> as a bioreactor: <span class="hlt">sediment</span> heterogeneity influencing biogeochemical processes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Perujo, Nuria; Romani, Anna M.; Sanchez-Vila, Xavier</p> <p>2017-04-01</p> <p>Mediterranean fluvial systems are characterized by frequent periods of low flow or even drought. During low flow periods, water from wastewater treatment plants (WWTPs) is proportionally large in fluvial systems. River water might be vertically transported through the hyporheic <span class="hlt">zone</span>, and then porous medium acts as a complementary treatment system since, as water infiltrates, a suite of biogeochemical processes occurs. Subsurface <span class="hlt">sediment</span> heterogeneity plays an important role since it influences the interstitial fluxes of the medium and drives biomass growing, determining biogeochemical reactions. In this study, WWTP water was continuously infiltrated for 3 months through two porous medium tanks: one consisting of 40 cm of fine <span class="hlt">sediment</span> (homogeneous); and another comprised of two layers of different grain size <span class="hlt">sediments</span> (heterogeneous), 20 cm of coarse <span class="hlt">sediment</span> in the upper part and 20 cm of fine one in the bottom. Several hydrological, physicochemical and biological parameters were measured periodically (weekly at the start of the experiment and biweekly at the end). Analysed parameters include dissolved nitrogen, phosphorus, organic carbon, and oxygen all measured at the surface, and at 5, 20 and 40 cm depth. Variations in hydraulic conductivity with time were evaluated. <span class="hlt">Sediment</span> samples were also analysed at three depths (surface, 20 and 40 cm) to determine bacterial density, chlorophyll content, extracellular polymeric substances, and biofilm function (extracellular enzyme activities and carbon substrate utilization profiles). Preliminary results suggest hydraulic conductivity to be the main driver of the differences in the biogeochemical processes occurring in the subsurface. At the heterogeneous tank, a low nutrient reduction throughout the whole medium is measured. In this medium, high hydraulic conductivity allows for a large amount of infiltrating water, but with a small residence time. Since some biological processes are largely time-dependent, small water</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014QSRv..102..149N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014QSRv..102..149N"><span>Lithology of the long <span class="hlt">sediment</span> record <span class="hlt">recovered</span> by the ICDP Dead Sea Deep Drilling Project (DSDDP)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neugebauer, Ina; Brauer, Achim; Schwab, Markus J.; Waldmann, Nicolas D.; Enzel, Yehouda; Kitagawa, Hiroyuki; Torfstein, Adi; Frank, Ute; Dulski, Peter; Agnon, Amotz; Ariztegui, Daniel; Ben-Avraham, Zvi; Goldstein, Steven L.; Stein, Mordechai</p> <p>2014-10-01</p> <p>The sedimentary sections that were deposited from the Holocene Dead Sea and its Pleistocene precursors are excellent archives of the climatic, environmental and seismic history of the Levant region. Yet, most of the previous work has been carried out on sequences of lacustrine <span class="hlt">sediments</span> exposed at the margins of the present-day Dead Sea, which were deposited only when the lake surface level rose above these terraces (e.g. during the Last Glacial period) and typically are discontinuous due to major lake level variations in the past. Continuous <span class="hlt">sedimentation</span> can only be expected in the deepest part of the basin and, therefore, a deep drilling has been accomplished in the northern basin of the Dead Sea during winter of 2010-2011 within the Dead Sea Deep Drilling Project (DSDDP) in the framework of the ICDP program. Approximately 720 m of <span class="hlt">sediment</span> cores have been retrieved from two deep and several short boreholes. The longest profile (5017-1), revealed at a water depth of ˜300 m, reaches 455 m below the lake floor (blf, i.e. to ˜1175 m below global mean sea level) and comprises approximately the last 220-240 ka. The record covers the upper part of the Amora (penultimate glacial), the Last Interglacial Samra, the Last Glacial Lisan and the Holocene Ze'elim Formations and, therewith, two entire glacial-interglacial cycles. Thereby, for the first time, consecutive <span class="hlt">sediments</span> deposited during the MIS 6/5, 5/4 and 2/1 transitions were <span class="hlt">recovered</span> from the Dead Sea basin, which are not represented in <span class="hlt">sediments</span> outcropping on the present-day lake shores. In this paper, we present essential lithological data including continuous magnetic susceptibility and geochemical scanning data and the basic stratigraphy including first chronological data of the long profile (5017-1) from the deep basin. The results presented here (a) focus on the correlation of the deep basin deposits with main on-shore stratigraphic units, thus providing a unique comprehensive stratigraphic framework for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGP51A1315K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGP51A1315K"><span>Rock Magnetic Study in the Methanogenesis <span class="hlt">Zone</span>, Site U1437, IODP Exp 350, Izu Rear Arc</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kars, M. A. C.; Musgrave, R. J.; Kodama, K.; Jonas, A. S.</p> <p>2015-12-01</p> <p>In 2014, IODP Expedition 350 drilled a 1806.5 m deep hole at Site U1437 in the Izu Bonin rear arc. The Site presents an unusual deep methanogenesis <span class="hlt">zone</span> because of a release of sulfate below the sulfate reduction <span class="hlt">zone</span> (27-83 mbsf) which may buffer methanogenesis by anaerobic methanogens. Methane abundance gradually increases with depth, with significant abundance at ~750-1459 mbsf with a maximum value at 920 mbsf. The rock magnetic study carried out in Hole U1437D from ~775 to ~1000 mbsf shows a drastic change of the magnetic properties at ~850 mbsf coincidently with a stronger release of methane from < 60 ppm at 841 mbsf to ~300 ppm at 854 mbsf. That also corresponds to a depth interval where no core was <span class="hlt">recovered</span> (~846-854 mbsf). For the sake of clarity, we call hereafter <span class="hlt">zone</span> A the depth interval above this non-<span class="hlt">recovered</span> interval (775-846 mbsf) and <span class="hlt">zone</span> B the interval below (854-1000 mbsf). Both belong to the same lithostratigraphic unit composed of tuffaceous mudstones intercalated with volcanoclastics. In the <span class="hlt">zone</span> A, NRM, magnetic susceptibility, ARM, SIRM, HIRM display high values. In the <span class="hlt">zone</span> B, these parameters show much lower values of one order of magnitude less, except for the interval 936-950 mbsf that corresponds to a local maximum (but still lower values than the <span class="hlt">zone</span> A). Besides, the rock magnetic parameters for grain size and coercivity, such as ARM/χ, S-ratio and Bcr do not show any variations throughout the entire studied interval, although S-ratio displays slightly lower values from ~850 to ~930 mbsf. Grains are low coercivity pseudo-single domain sized. According to the present data, two preliminary hypotheses can be proposed to explain the observations. 1) The non-<span class="hlt">recovered</span> interval between the <span class="hlt">zones</span> A and B can be caused by the presence of a sedimentary hiatus and/or a fault, which may be consistent with the observed change in <span class="hlt">sedimentation</span> rate. 2) No hiatus in the <span class="hlt">sedimentation</span>. The changes in the magnetic properties can be explained by a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..180..111S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..180..111S"><span>Terminal <span class="hlt">zone</span> glacial <span class="hlt">sediment</span> transfer at a temperate overdeepened glacier system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swift, D. A.; Cook, S. J.; Graham, D. J.; Midgley, N. G.; Fallick, A. E.; Storrar, R.; Toubes Rodrigo, M.; Evans, D. J. A.</p> <p>2018-01-01</p> <p>Continuity of <span class="hlt">sediment</span> transfer through glacial systems is essential to maintain subglacial bedrock erosion, yet transfer at temperate glaciers with overdeepened beds, where subglacial fluvial <span class="hlt">sediment</span> transport should be greatly limited by adverse slopes, remains poorly understood. Complex multiple transfer processes in temperate overdeepened systems has been indicated by the presence of large frontal moraine systems, supraglacial debris of mixed transport origin, thick basal ice sequences, and englacial thrusts and eskers. At Svínafellsjökull, thrusts comprising decimetre-thick debris-rich bands of stratified facies ice of basal origin, with a coarser size distribution and higher clast content than that observed in basal ice layers, contribute substantially to the transfer of subglacial material in the terminal <span class="hlt">zone</span>. Entrainment and transfer of material occurs by simple shear along the upper surface of bands and by strain-induced deformation of stratified and firnified glacier ice below. Thrust material includes rounded and well-rounded clasts that are also striated, indicating that fluvial bedload is deposited as subglacial channels approach the overdeepening and then entrained along thrusts. Substantial transfer also occurs within basal ice, with facies type and debris content dependent on the hydrological connectedness of the adverse slope. A process model of transfer at glaciers with terminal overdeepenings is proposed, in which the geometry of the overdeepening influences spatial patterns of ice deformation, hydrology, and basal ice formation. We conclude that the significance of thrusting in maintaining <span class="hlt">sediment</span> transfer continuity has likely been overlooked by glacier <span class="hlt">sediment</span> budgets and glacial landscape evolution studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGP51A1371G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGP51A1371G"><span>Resolution Study of Marine CSEM Imaging of Subduction <span class="hlt">Zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gustafson, C.; Key, K.</p> <p>2016-12-01</p> <p>Marine controlled source electromagnetic (CSEM) data allow us to image seafloor electrical resistivity from which we can constrain the porosity and fluid content of the subsurface. In subduction <span class="hlt">zones</span>, CSEM data can be used to constrain geologic structure, hydrogeology and fluid-tectonic processes. The scales of features we are interested in <span class="hlt">recovering</span> with CSEM data range from large-scale features such as the incoming tectonic plate and subducting slab, to the narrow dipping plate boundary interface where slip occurs, to thin faults that cut the overriding forearc crust and shallow fluid seeps and mounds on the seafloor. Thus electrical structure is expected to vary on scales ranging from scales of meters to tens of kilometers. CSEM data collected by Scripps at the Middle America Trench in 2010 is the first and to-date the only application of the method for studying a subduction <span class="hlt">zone</span>. The results from this pioneering data set highlight the types of new discoveries that are possible with CSEM data, such as imaging conductive bending faults and a water-rich channel of subducting <span class="hlt">sediments</span>. In this work we explore the magnitude and scale of 2D resistivity structures that can be resolved with CSEM data through a suite of synthetic inversion studies. We build resistivity models that are representative of various known and hypothesized subduction <span class="hlt">zone</span> plate boundary structures. We generate synthetic noisy data for these models and invert them using the freely available MARE2DEM inversion code. We compare the <span class="hlt">recovered</span> models to the original models in order to determine which resistivity structures may be successfully identified using CSEM. We explore the potential effects of receiver spacing, frequency bandwidth and system noise levels on the ability of CSEM to <span class="hlt">recover</span> these different subduction <span class="hlt">zone</span> structures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=65373&keyword=nitrous+AND+oxide&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=65373&keyword=nitrous+AND+oxide&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>SOIL NITROUS OXIDE, NITRIC OXIDE, AND AMMONIA EMISSIONS FROM A <span class="hlt">RECOVERING</span> RIPARIAN ECOSYSTEM IN SOUTHERN APPALACHIA</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>The paper presents two years of seasonal nitric oxide, ammonia, and nitrous oxide trace gas fluxes measured in a <span class="hlt">recovering</span> riparian <span class="hlt">zone</span> with cattle excluded and in an adjacent riparian <span class="hlt">zone</span> grazed by cattle. In the <span class="hlt">recovering</span> riparian <span class="hlt">zone</span>, average nitric oxide, ammonia, and ni...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC51F1148R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC51F1148R"><span>Trace Element Mobility in Water and <span class="hlt">Sediments</span> in a Hyporheic <span class="hlt">Zone</span> Adjacent to an Abandoned Uranium Mine</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roldan, C.; Blake, J.; Cerrato, J.; Ali, A.; Cabaniss, S.</p> <p>2015-12-01</p> <p>The legacy of abandoned uranium mines lead to community concerns about environmental and health effects. This study focuses on a cross section of the Rio Paguate, adjacent to the Jackpile Mine on the Laguna Reservation, west-central New Mexico. Often, the geochemical interactions that occur in the hyporheic <span class="hlt">zone</span> adjacent to these abandoned mines play an important role in trace element mobility. In order to understand the mobility of uranium (U), arsenic (As), and vanadium (V) in the Rio Paguate; surface water, hyporheic <span class="hlt">zone</span> water, and core <span class="hlt">sediment</span> samples were analyzed using inductively coupled plasma mass spectroscopy (ICP-MS). All water samples were filtered through 0.45μm and 0.22μm filters and analyzed. The results show that there is no major difference in concentrations of U (378-496μg/L), As (0.872-6.78μg/L), and V (2.94-5.01μg/L) between the filter sizes or with depth (8cm and 15cm) in the hyporheic <span class="hlt">zone</span>. The unfiltered hyporheic <span class="hlt">zone</span> water samples were analyzed after acid digestion to assess the particulate fraction. These results show a decrease in U concentration (153-202μg/L) and an increase in As (33.2-219μg/L) and V (169-1130μg/L) concentrations compared to the filtered waters. Surface water concentrations of U(171-184μg/L) are lower than the filtered hyporheic <span class="hlt">zone</span> waters while As(1.32-8.68μg/L) and V(1.75-2.38μg/L) are significantly lower than the hyporheic <span class="hlt">zone</span> waters and particulates combined. Concentrations of As in the <span class="hlt">sediment</span> core samples are higher in the first 15cm below the water-<span class="hlt">sediment</span> interface (14.3-3.82μg/L) and decrease (0.382μg/L) with depth. Uranium concentrations are consistent (0.047-0.050μg/L) at all depths. The over all data suggest that U is mobile in the dissolved phase and both As and V are mobile in the particular phase as they travel through the system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRG..123..902N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRG..123..902N"><span>Influence of Hydrological Perturbations and Riverbed <span class="hlt">Sediment</span> Characteristics on Hyporheic <span class="hlt">Zone</span> Respiration of CO2 and N2</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Newcomer, Michelle E.; Hubbard, Susan S.; Fleckenstein, Jan H.; Maier, Ulrich; Schmidt, Christian; Thullner, Martin; Ulrich, Craig; Flipo, Nicolas; Rubin, Yoram</p> <p>2018-03-01</p> <p>Rivers in climatic <span class="hlt">zones</span> characterized by dry and wet seasons often experience periodic transitions between losing and gaining conditions across the river-aquifer continuum. Infiltration shifts can stimulate hyporheic microbial biomass growth and cycling of riverine carbon and nitrogen leading to major exports of biogenic CO2 and N2 to rivers. In this study, we develop and test a numerical model that simulates biological-physical feedback in the hyporheic <span class="hlt">zone</span>. We used the model to explore different initial conditions in terms of dissolved organic carbon availability, <span class="hlt">sediment</span> characteristics, and stochastic variability in aerobic and anaerobic conditions from water table fluctuations. Our results show that while highly losing rivers have greater hyporheic CO2 and N2 production, gaining rivers allowed the greatest fraction of CO2 and N2 production to return to the river. Hyporheic aerobic respiration and denitrification contributed 0.1-2 g/m2/d of CO2 and 0.01-0.2 g/m2/d of N2; however, the suite of potential microbial behaviors varied greatly among <span class="hlt">sediment</span> characteristics. We found that losing rivers that consistently lacked an exit pathway can store up to 100% of the entering C/N as subsurface biomass and dissolved gas. Our results demonstrate the importance of subsurface feedbacks whereby microbes and hydrology jointly control fate of C and N and are strongly linked to wet-season control of initial <span class="hlt">sediment</span> conditions and hydrologic control of seepage direction. These results provide a new understanding of hydrobiological and <span class="hlt">sediment</span>-based controls on hyporheic <span class="hlt">zone</span> respiration, including a new explanation for the occurrence of anoxic microzones and large denitrification rates in gravelly riverbeds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036030','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036030"><span>Hurricane Katrina <span class="hlt">sediment</span> slowed elevation loss in subsiding brackish marshes of the Mississippi River delta</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McKee, K.L.; Cherry, J.A.</p> <p>2009-01-01</p> <p>Although hurricanes can damage or destroy coastal wetlands, they may play a beneficial role in reinvigorating marshes by delivering <span class="hlt">sediments</span> that raise soil elevations and stimulate organic matter production. Hurricane Katrina altered elevation dynamics of two subsiding brackish marshes in the Mississippi River deltaic plain by adding 3 to 8 cm of <span class="hlt">sediment</span> to the soil surface in August 2005. Soil elevations at both sites subsequently declined due to continued subsidence, but net elevation gain was still positive at both Pearl River (+1.7 cm) and Big Branch (+0.7 cm) marshes two years after the hurricane. At Big Branch where storm <span class="hlt">sediments</span> had higher organic matter and water contents, post-storm elevation loss was more rapid due to initial compaction of the storm layer in combination with root-<span class="hlt">zone</span> collapse. In contrast, elevation loss was slower at Pearl River where the storm deposit (high sand content) did not compact and the root <span class="hlt">zone</span> did not collapse. Vegetation at both sites fully <span class="hlt">recovered</span> within one year, and accumulation of root matter at Big Branch increased 10-fold from 2005 to 2006, suggesting that the hurricane stimulated belowground productivity. Results of this study imply that hurricane <span class="hlt">sediment</span> may benefit subsiding marshes by slowing elevation loss. However, long-term effects of hurricane <span class="hlt">sediment</span> on elevation dynamics will depend not only on the amount of <span class="hlt">sediment</span> deposited, but on <span class="hlt">sediment</span> texture and resistance to compaction as well as on changes in organic matter accumulation in the years following the hurricane.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003AGUFMOS51B0855N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003AGUFMOS51B0855N"><span>Methane Hydrate <span class="hlt">Recovered</span> From A Mud Volcano in Santa Monica Basin, Offshore Southern California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Normark, W. R.; Hein, J. R.; Powell, C. L.; Lorenson, T. D.; Lee, H. J.; Edwards, B. D.</p> <p>2003-12-01</p> <p>In July 2003, a short (2.1 m) piston core from the summit of a mud volcano <span class="hlt">recovered</span> methane hydrate at a water depth of 813 m in Santa Monica Basin. The discovery core penetrated into in the hydrate as evidenced by chunks of ice and violent degassing of the core section between 162 and 212 cm depth. The core consists of shell hash and carbonate clasts (to 7-cm long) in silty mud. The methanogenic carbonates are of two types: massive, recrystallized nodular masses with an outer mm-thick sugary patina and a bivalve coquina with carbonate cement. Living clams including the genus Vesicomya, commonly found at cold-seep sites elsewhere, were <span class="hlt">recovered</span> from the top of the core. Further sampling attempts using piston, gravity, and box corers, all of which were obtained within 15 m of the discovery core, <span class="hlt">recovered</span> olive-brown silty mud with variable amounts of whole and fragmented bivalve shells and methanogenic carbonate fragments characteristic of cold-seep environments. Gases collected in cores adjacent to the discovery core contain elevated amounts of methane and trace amounts of heavier hydrocarbon gases, indicating some component from thermogenic sources. Hydrogen sulfide was also detected in these <span class="hlt">sediment</span> samples. Vertical channels in one core may have served as fluid pathways. The existence of hydrate at such a shallow depth in the <span class="hlt">sediment</span> was unexpected, however, the presence of Vesicomya and hydrogen sulfide indicate that the mud volcano is a site of active methane venting. The mud volcano, which is about 24 km west-southwest of Redondo Beach, is about 300 m in diameter at the base. No internal structure is resolved on either high resolution deep-tow boomer or single-channel air-gun profiles, most likely as a result of the gas content and <span class="hlt">sediment</span> deformation. The diapiric structure has ascended through well-bedded <span class="hlt">sediment</span> on the lower slope of the basin, producing as much as 30 m of bathymetric relief. It is located in an area where strike-slip motion along</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=83744&keyword=phone&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=83744&keyword=phone&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span><span class="hlt">SEDIMENT</span> TOXICITY AND COMMUNITY COMPOSITION OF BENTHOS AND COLONIZED PERIPHYTON IN THE EVERGLADES - FLORIDA BAY TRANSITIONAL <span class="hlt">ZONE</span>.</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Lewis, Michael A., Larry R. Goodman, John M. Macauley and James C. Moore. 2004. <span class="hlt">Sediment</span> Toxicity and Community Composition of Benthos and Colonized Periphyton in the Everglades-Florida Bay Transitional <span class="hlt">Zone</span>. Ecotoxicology. 13(3):231-244. (ERL,GB 1164). <br><br>This survey provid...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869745','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869745"><span>Method for continuously <span class="hlt">recovering</span> metals using a dual <span class="hlt">zone</span> chemical reactor</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bronson, Mark C.</p> <p>1995-01-01</p> <p>A dual <span class="hlt">zone</span> chemical reactor continuously processes metal-containing materials while regenerating and circulating a liquid carrier. The starting materials are fed into a first reaction <span class="hlt">zone</span> of a vessel containing a molten salt carrier. The starting materials react to form a metal product and a by-product that dissolves in the molten salt that flows to a second reaction <span class="hlt">zone</span> in the reaction vessel. The second reaction <span class="hlt">zone</span> is partitioned from, but in fluid communication with, the first reaction <span class="hlt">zone</span>. The liquid carrier continuously circulates along a pathway between the first reaction <span class="hlt">zone</span> and the second reaction <span class="hlt">zone</span>. A reactive gas is introduced into the second reaction <span class="hlt">zone</span> to react with the reaction by-product to generate the molten salt. The metal product, the gaseous waste products, and the excess liquid carrier are removed without interrupting the operation of the reactor. The design of the dual <span class="hlt">zone</span> reactor can be adapted to combine a plurality of liquid carrier regeneration <span class="hlt">zones</span> in a multiple dual <span class="hlt">zone</span> chemical reactor for production scale processing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/27711','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/27711"><span>Method for continuously <span class="hlt">recovering</span> metals using a dual <span class="hlt">zone</span> chemical reactor</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Bronson, M.C.</p> <p>1995-02-14</p> <p>A dual <span class="hlt">zone</span> chemical reactor continuously processes metal-containing materials while regenerating and circulating a liquid carrier. The starting materials are fed into a first reaction <span class="hlt">zone</span> of a vessel containing a molten salt carrier. The starting materials react to form a metal product and a by-product that dissolves in the molten salt that flows to a second reaction <span class="hlt">zone</span> in the reaction vessel. The second reaction <span class="hlt">zone</span> is partitioned from, but in fluid communication with, the first reaction <span class="hlt">zone</span>. The liquid carrier continuously circulates along a pathway between the first reaction <span class="hlt">zone</span> and the second reaction <span class="hlt">zone</span>. A reactive gas is introduced into the second reaction <span class="hlt">zone</span> to react with the reaction by-product to generate the molten salt. The metal product, the gaseous waste products, and the excess liquid carrier are removed without interrupting the operation of the reactor. The design of the dual <span class="hlt">zone</span> reactor can be adapted to combine a plurality of liquid carrier regeneration <span class="hlt">zones</span> in a multiple dual <span class="hlt">zone</span> chemical reactor for production scale processing. 6 figs.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFMOS11A0196S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFMOS11A0196S"><span>Strontium Isotope Dating of Metalliferous <span class="hlt">Sediment</span> in the SW Pacific Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stancin, A. M.; Gleason, J. D.; Owen, B. M.; Rea, D. K.; Moore, T. C.; Hendy, I. L.; Lyle, M. W.; Blum, J. D.</p> <p>2007-12-01</p> <p>A 2 million km2 region virtually devoid of <span class="hlt">sediment</span> was identified in the remote SW Pacific Basin during the TUIM- 3 2005 drill site survey cruise. This region, termed the "South Pacific Bare <span class="hlt">Zone</span>", comprises ocean floor dating back to the Late Cretaceous. Within the Bare <span class="hlt">Zone</span>, a small (1km2) abyssal valley containing <span class="hlt">sediment</span> to a depth of 24 m was sampled using a large diameter piston core (MV0502-15JC, 31 ° 42.194'S, 143 ° 30.331'W), leading to recovery of 8.35 m of metalliferous <span class="hlt">sediment</span> at 5082 m water depth. Fish-teeth Sr-isotope stratigraphy reveals a continuous record of <span class="hlt">sedimentation</span> from 31 Ma to present at this site. The fish teeth age-depth profile and INAA geochemistry reveal an exponentially decreasing hydrothermal flux, with <span class="hlt">sedimentation</span> rates approaching 0.05 mm/kyr after 20 Ma. The source of hydrothermal activity at this site was likely the Pacific- Farallon Ridge, which went extinct at 20 Ma. A second piston core (MV0502-16JC; 28 ° 05.151'S, 140 ° 14.140'W) was collected near MacDonald Seamounts located on the southeastern end of the Cook-Austral island chain outside the Bare <span class="hlt">Zone</span> and <span class="hlt">recovered</span> 10.5 m of hydrothermal <span class="hlt">sediment</span> and biogenic ooze. The lower 65 cm of the core consists of a coccolith ooze. From 10 mbsf depth to 1.5 mbsf depth, the core contians reddish black zeolitic clay, while the upper 1.5 mbsf contains biogenic ooze associated with abundant Late Pleistocene foraminifera remains. Concordant nannofossil and fish teeth ages at the base of the core (27-28 Ma), and Pleistocene ages near the top of the core reinforce the validity of the Sr fish teeth method for dating hydrothermal cores. These independent records suggest that regional hydrothermal activity during the Oligocene may have been related to a series of late Eocene/early Oligocene ridge jumps, propagating rifts and seafloor spreading centers that accompanied large-scale plate tectonic reorganization of South Pacific seafloor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18441804','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18441804"><span>Advective removal of intraparticle uranium from contaminated vadose <span class="hlt">zone</span> <span class="hlt">sediments</span>, Hanford, U.S.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ilton, Eugene S; Qafoku, Nikolla P; Liu, Chongxuan; Moore, Dean A; Zachara, John M</p> <p>2008-03-01</p> <p>A column study on U(VI)-contaminated vadose <span class="hlt">zone</span> <span class="hlt">sediments</span> from the Hanford Site, WA, was performed to investigate U(VI) release kinetics with water advection and variable geochemical conditions. The <span class="hlt">sediments</span> were collected from an area adjacent to and below tank BX-102 that was contaminated as a result of a radioactive tank waste overfill event. The primary reservoir for U(VI) in the <span class="hlt">sediments</span> are micrometer-size precipitates composed of nanocrystallite aggregates of a Na-U-Silicate phase, most likely Na-boltwoodite, that nucleated and grew within microfractures of the plagioclase component of sand-sized granitic clasts. Two <span class="hlt">sediment</span> samples, with different U(VI) concentrations and intraparticle mass transfer properties, were leached with advective flows of three different solutions. The influent solutions were all calcite-saturated and in equilibrium with atmospheric CO2. One solution was prepared from DI water, the second was a synthetic groundwater (SGW) with elevated Na that mimicked groundwater at the Hanford site, and the third was the same SGW but with both elevated Na and Si. The latter two solutions were employed, in part, to test the effect of saturation state on U(VI) release. For both <span class="hlt">sediments</span>, and all three electrolytes, there was an initial rapid release of U(VI) to the advecting solution followed by slower near steady-state release. U(VI)aq concentrations increased during subsequent stop-flow events. The electrolytes with elevated Na and Si depressed U(VL)aq concentrations in effluent solutions. Effluent U(VI)aq concentrations for both <span class="hlt">sediments</span> and all three electrolytes were simulated reasonably well by a three domain model (the advecting fluid, fractures, and matrix) that coupled U(VI) dissolution, intraparticle U(VI)aq diffusion, and interparticle advection, where diffusion and dissolution properties were parameterized in a previous batch study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4999275','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4999275"><span>Rapid <span class="hlt">Sediment</span> Accumulation Results in High Methane Effluxes from Coastal <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lenstra, Wytze; Jong, Dirk; Meysman, Filip J. R.; Sapart, Célia J.; van der Veen, Carina; Röckmann, Thomas; Gonzalez, Santiago; Slomp, Caroline P.</p> <p>2016-01-01</p> <p>Globally, the methane (CH4) efflux from the ocean to the atmosphere is small, despite high rates of CH4 production in continental shelf and slope environments. This low efflux results from the biological removal of CH4 through anaerobic oxidation with sulfate in marine <span class="hlt">sediments</span>. In some settings, however, pore water CH4 is found throughout the sulfate-bearing <span class="hlt">zone</span>, indicating an apparently inefficient oxidation barrier for CH4. Here we demonstrate that rapid <span class="hlt">sediment</span> accumulation can explain this limited capacity for CH4 removal in coastal <span class="hlt">sediments</span>. In a saline coastal reservoir (Lake Grevelingen, The Netherlands), we observed high diffusive CH4 effluxes from the <span class="hlt">sediment</span> into the overlying water column (0.2–0.8 mol m-2 yr-1) during multiple years. Linear pore water CH4 profiles and the absence of an isotopic enrichment commonly associated with CH4 oxidation in a <span class="hlt">zone</span> with high rates of sulfate reduction (50–170 nmol cm-3 d-1) both suggest that CH4 is bypassing the <span class="hlt">zone</span> of sulfate reduction. We propose that the rapid <span class="hlt">sediment</span> accumulation at this site (~ 13 cm yr-1) reduces the residence time of the CH4 oxidizing microorganisms in the sulfate/methane transition <span class="hlt">zone</span> (< 5 years), thus making it difficult for these slow growing methanotrophic communities to build-up sufficient biomass to efficiently remove pore water CH4. In addition, our results indicate that the high input of organic matter (~ 91 mol C m-2 yr-1) allows for the co-occurrence of different dissimilatory respiration processes, such as (acetotrophic) methanogenesis and sulfate reduction in the surface <span class="hlt">sediments</span> by providing abundant substrate. We conclude that anthropogenic eutrophication and rapid <span class="hlt">sediment</span> accumulation likely increase the release of CH4 from coastal <span class="hlt">sediments</span>. PMID:27560511</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T12A..05K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T12A..05K"><span>Effects of stress paths on physical properties of <span class="hlt">sediments</span> at the Nankai Trough subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitajima, H.; Saffer, D. M.</p> <p>2011-12-01</p> <p>Stress states are one of the most important factors governing deformation modes and fault strength. In subduction systems where tectonic stress is large, <span class="hlt">sediments</span> are subjected to complicated stress conditions in time and space. Because direct measurements of stress are very limited, stress conditions at depths have been estimated by combining seismic reflection data with empirical relations between compressional-wave, porosity, and effective stress [Tsuji et al., 2008; Tobin and Saffer, 2009]. However, most of the empirical relations are derived from experiments conducted under isotropic conditions, and do not account for the more complicated stress states expected in active subduction-accretion complexes. In this study, we aim to derive relations between physical properties and stress states from triaxial deformation experiments on <span class="hlt">sediments</span>. During the Integrated Ocean Drilling Program (IODP) Nankai Trough Seismogenic <span class="hlt">Zone</span> Experiment (NanTroSEIZE) Expeditions 314, 315, 319, 322, and 333, core samples were <span class="hlt">recovered</span> from shallow boreholes into the accretionary prism and two sites seaward of the deformation front (reference sites). We used core samples from reference sites (Sites C0011 and C0012) for this study because they represent input material for the subduction system, and have not been subjected to tectonic compression in the accretionary wedge. In our deformation tests, samples are loaded under a range of different stress paths including isotropic loading, triaxial compression, and triaxial extension by controlling axial stress (up to 100 MPa), confining pressure (up to 100 MPa), and pore pressure (0.5-28 MPa). During tests, all pressures, axial displacement, and pore volume change were monitored. Permeability, and ultrasonic velocity were also measured during the tests. Two experiments have been conducted on samples taken from the core 322-C0011B-19R-5 (Lower Shikoku Basin hemipelagic mudstone, initial porosity of 43 %). The first test was conducted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70100648','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70100648"><span>Dispersal of fine <span class="hlt">sediment</span> in nearshore coastal waters</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Warrick, Jonathan A.</p> <p>2013-01-01</p> <p>Fine <span class="hlt">sediment</span> (silt and clay) plays an important role in the physical, ecological, and environmental conditions of coastal systems, yet little is known about the dispersal and fate of fine <span class="hlt">sediment</span> across coastal margin settings outside of river mouths. Here I provide simple physical scaling and detailed monitoring of a beach nourishment project near Imperial Beach, California, with a high portion of fines (40% silt and clay by weight). These results provide insights into the pathways and residence times of fine <span class="hlt">sediment</span> transport across a wave-dominated coastal margin. Monitoring of the project used physical, optical, acoustic, and remote sensing techniques to track the fine portion of the nourishment <span class="hlt">sediment</span>. The initial transport of fine <span class="hlt">sediment</span> from the beach was influenced strongly by longshore currents of the surf <span class="hlt">zone</span> that were established in response to the approach angles of the waves. The mean residence time of fine <span class="hlt">sediment</span> in the surf zone—once it was suspended—was approximately 1 hour, and rapid decreases in surf <span class="hlt">zone</span> fine <span class="hlt">sediment</span> concentrations along the beach resulted from mixing and offshore transport in turbid rip heads. For example, during a day with oblique wave directions and surf <span class="hlt">zone</span> longshore currents of approximately 25 cm/s, the offshore losses of fine <span class="hlt">sediment</span> in rips resulted in a 95% reduction in alongshore surf <span class="hlt">zone</span> fine <span class="hlt">sediment</span> flux within 1 km of the nourishment site. However, because of the direct placement of nourishment <span class="hlt">sediment</span> on the beach, fine suspended-<span class="hlt">sediment</span> concentrations in the swash <span class="hlt">zone</span> remained elevated for several days after nourishment, while fine <span class="hlt">sediment</span> was winnowed from the beach. Once offshore of the surf <span class="hlt">zone</span>, fine <span class="hlt">sediment</span> settled downward in the water column and was observed to transport along and across the inner shelf. Vertically sheared currents influenced the directions and rates of fine <span class="hlt">sediment</span> transport on the shelf. <span class="hlt">Sedimentation</span> of fine <span class="hlt">sediment</span> was greatest on the seafloor directly offshore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ECSS..205....1A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ECSS..205....1A"><span>Microplastics in <span class="hlt">sediments</span> from the littoral <span class="hlt">zone</span> of the north Tunisian coast (Mediterranean Sea)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abidli, Sami; Antunes, Joana C.; Ferreira, Joana L.; Lahbib, Youssef; Sobral, Paula; Trigui El Menif, Najoua</p> <p>2018-05-01</p> <p>The distribution of microplastics (MPs) was investigated in the <span class="hlt">sediments</span> of five sampling sites from the northern Tunisian coast during June 2017. MPs were categorized according to type, colour and size. Representative MPs from the five sites were isolated for polymer identification using Fourier Transformed Infrared Spectroscopy in attenuated total reflectance mode (FTIR-ATR). Results showed that MPs were <span class="hlt">recovered</span>, from all <span class="hlt">sediment</span> samples, indicating for the first time, their extensive distribution in Tunisian coast. Concentrations varied from 141.20 ± 25.98 to 461.25 ± 29.74 items kg-1 dry weight. Fibres, fragments, Styrofoam®, pellets and films were the types registered in this study. With the exception of Menzel Bourguiba (MB), fibres significantly outnumbered plastic particles followed by fragments, Styrofoam®, films and pellets. The predominant colours are as follows: black > clear > white > red > blue > green for fibres, blue > white > clear > red > green > yellow > black for fragments, blue > white > black > clear for films while only white pellets and Styrofoam® were found. MPs particles ranged from 0.1 to 5 mm in length. A total of three polymer types were identified, polyethylene (PE), polypropylene (PP) and polystyrene (PS). Except for industrial pellets, the presence of MPs is likely due to the degradation of marine plastic debris accumulating in each site. This work provides original data of the presence of MPs in coastal <span class="hlt">sediments</span> from Northern Tunisian coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018689','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018689"><span>Using nonlinear forecasting to learn the magnitude and phasing of time-varying <span class="hlt">sediment</span> suspension in the surf <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Jaffe, B.E.; Rubin, D.M.</p> <p>1996-01-01</p> <p>The time-dependent response of <span class="hlt">sediment</span> suspension to flow velocity was explored by modeling field measurements collected in the surf <span class="hlt">zone</span> during a large storm. Linear and nonlinear models were created and tested using flow velocity as input and suspended-<span class="hlt">sediment</span> concentration as output. A sequence of past velocities (velocity history), as well as velocity from the same instant as the suspended-<span class="hlt">sediment</span> concentration, was used as input; this velocity history length was allowed to vary. The models also allowed for a lag between input (instantaneous velocity or end of velocity sequence) and output (suspended-<span class="hlt">sediment</span> concentration). Predictions of concentration from instantaneous velocity or instantaneous velocity raised to a power (up to 8) using linear models were poor (correlation coefficients between predicted and observed concentrations were less than 0.10). Allowing a lag between velocity and concentration improved linear models (correlation coefficient of 0.30), with optimum lag time increasing with elevation above the seabed (from 1.5 s at 13 cm to 8.5 s at 60 cm). These lags are largely due to the time for an observed flow event to effect the bed and mix <span class="hlt">sediment</span> upward. Using a velocity history further improved linear models (correlation coefficient of 0.43). The best linear model used 12.5 s of velocity history (approximately one wave period) to predict concentration. Nonlinear models gave better predictions than linear models, and, as with linear models, nonlinear models using a velocity history performed better than models using only instantaneous velocity as input. Including a lag time between the velocity and concentration also improved the predictions. The best model (correlation coefficient of 0.58) used 3 s (approximately a quarter wave period) of the cross-shore velocity squared, starting at 4.5 s before the observed concentration, to predict concentration. Using a velocity history increases the performance of the models by specifying a more</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T31G2599V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T31G2599V"><span>Physical properties and Consolidation behavior of <span class="hlt">sediments</span> from the N. Japan subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Valdez, R. D., II; Lauer, R. M.; Ikari, M.; Kitajima, H.; Saffer, D. M.</p> <p>2013-12-01</p> <p><span class="hlt">Sediment</span> hydraulic properties, consolidation state, and ambient pore pressure development are key parameters that affect fluid migration, deformation, and the slip behavior and mechanical strength of subduction <span class="hlt">zone</span> megathrusts. In order to better understand the dynamics and mechanisms of large subduction earthquakes, Integrated Oceanic Drilling Program (IODP) Expedition 343, drilled into the toe of the Japan Trench subduction <span class="hlt">zone</span> in a region of large shallow slip in the M 9.0 Tohoku earthquake, as part of the Japan Trench Fast Drilling Project (J-FAST). Here, we report on two constant rate of strain (CRS) uniaxial consolidation experiments and two triaxial deformation experiments on bedded claystone and clayey mudstone core samples collected from the frontal prism and subducted <span class="hlt">sediment</span> section cored at Site C0019, 2.5 km landward of the Japan Trench, from depths of 697.18 and 831.45 mbsf. The goals of our experiments were: (1) to define the hydraulic and acoustic properties of <span class="hlt">sediments</span> that host the subduction megathrust fault that slipped in the M 9.0 Tohoku earthquake; and (2) to constrain in-situ consolidation state and its implications for in-situ stress. The permeability-porosity trends are similar for the two samples, and both exhibit permeability that decreases systematically with increasing effective stress and decreasing porosity, and which varies log-linearly with porosity. Permeabilities of material from the frontal prism decrease from 5×10-18 m2 at 5 MPa effective stress, to 3.0×10-19 m2 at 70 MPa, and porosities decrease from 51% to 29%, while permeabilities of the subducted <span class="hlt">sediment</span> sample decrease from 5×10-18 m2 at 5 MPa to 3.6×10-19 m2 at 90 MPa, and porosities decrease from 49% to 36%. In-situ permeabilities for the prism and underthrust <span class="hlt">sediment</span> samples, estimated using laboratory defined permeability-porosity relationships, are 4.9×10-18 m2 and 3.7×10-18 m2, respectively. Elastic wavespeeds increase systematically with increasing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H33I0949K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H33I0949K"><span>The Dynamics of <span class="hlt">Sediment</span> Oxygenation in Marsh Rhizospheres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koop-Jakobsen, K.</p> <p>2014-12-01</p> <p>Many marsh grasses are capable of internal oxygen transport from aboveground sources to belowground roots and rhizomes, where oxygen may leak across the rhizodermis and oxygenate the surrounding <span class="hlt">sediment</span>. In the field, the extent of <span class="hlt">sediment</span> oxygenation in marshes was assessed in the rhizosphere of the marsh grass; Spartina anglica, inserting 70 optical fiber oxygen sensors into the rhizosphere. Two locations with S. anglica growing in different <span class="hlt">sediment</span> types were investigated. No oxygen was detected in the rhizospheres indicating that belowground <span class="hlt">sediment</span> oxygenation in S. anglica has a limited effect on the bulk anoxic <span class="hlt">sediment</span> and is restricted to <span class="hlt">sediment</span> in the immediate vicinity of the roots. In the laboratory, the presence of 1.5mm wide and 16mm long oxic root <span class="hlt">zones</span> was demonstrated around root tips of S. anglica growing in permeable sandy <span class="hlt">sediment</span> using planar optodes recording 2D-images of the oxygen distribution. Oxic root <span class="hlt">zones</span> in S. anglica growing in tidal flat deposits were significantly smaller. The size of oxic roots <span class="hlt">zones</span> was highly dynamic and affected by tidal inundations as well as light availability. Atmospheric air was the primary oxygen source for belowground <span class="hlt">sediment</span> oxygenation, whereas photosynthetic oxygen production only played a minor role for the size of the oxic root <span class="hlt">zones</span> during air-exposure of the aboveground biomass. During tidal inundations (1.5 h) completely submerging the aboveground biomass cutting off access to atmospheric oxygen, the size of oxic root <span class="hlt">zones</span> were reduced significantly in the light and oxic root <span class="hlt">zones</span> were completely eliminated in darkness. <span class="hlt">Sediment</span> oxygenation in the rhizospheres of marsh grasses is of significant importance for marshes ability to retain inorganic nitrogen before it reaches the coastal waters. The presence of oxic roots <span class="hlt">zones</span> promotes coupled nitrification-denitrification at depth in the <span class="hlt">sediment</span>, which can account for more than 80% of the total denitrification in marshes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912967S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912967S"><span><span class="hlt">Sediment</span> features at the grounding <span class="hlt">zone</span> and beneath Ekström Ice Shelf, East Antarctica, imaged using on-ice vibroseis.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, Emma C.; Eisen, Olaf; Hofstede, Coen; Lambrecht, Astrid; Mayer, Christoph</p> <p>2017-04-01</p> <p>The grounding <span class="hlt">zone</span>, where an ice sheet becomes a floating ice shelf, is known to be a key threshold region for ice flow and stability. A better understanding of ice dynamics and <span class="hlt">sediment</span> transport across such <span class="hlt">zones</span> will improve knowledge about contemporary and palaeo ice flow, as well as past ice extent. Here we present a set of seismic reflection profiles crossing the grounding <span class="hlt">zone</span> and continuing to the shelf edge of Ekström Ice Shelf, East Antarctica. Using an on-ice vibroseis source combined with a snowstreamer we have imaged a range of sub-glacial and sub-shelf sedimentary and geomorphological features; from layered <span class="hlt">sediment</span> deposits to elongated flow features. The acoustic properties of the features as well as their morphology allow us to draw conclusions as to their material properties and origin. These results will eventually be integrated with numerical models of ice dynamics to quantify past and present interactions between ice and the solid Earth in East Antarctica; leading to a better understanding of future contributions of this region to sea-level rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24825508','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24825508"><span>Freeze shoe sampler for the collection of hyporheic <span class="hlt">zone</span> <span class="hlt">sediments</span> and porewater.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bianchin, M; Smith, L; Beckie, R</p> <p>2015-01-01</p> <p>The Starr and Ingleton (1992) drive point piston sampler (DPPS) design was modified by fitting it with a Murphy and Herkelrath (1996) type sample-freezing drive shoe (SFDS), which uses liquid carbon dioxide as a cryogen. Liquid carbon dioxide was used to freeze <span class="hlt">sediments</span> in the lower 0.1 m of the core and the drive-point piston sealed the core at the top preserving the reductive-oxidation (redox) sensitive <span class="hlt">sediments</span> from the atmosphere and maintaining natural stratigraphy. The use of nitrogen gas to provide positive pressure on the gas system blocked the ingress of water which froze on contact with the cryogen thus blocking the gas lines with ice. With this adaptation to the gas system cores could be collected at greater depths beneath the static water level. This tool was used to collect intact saturated <span class="hlt">sediment</span> cores from the hyporheic <span class="hlt">zone</span> of the tidally influenced Fraser River in Vancouver, British Columbia, Canada where steep geochemical and microbial gradients develop within the interface between discharging anaerobic groundwater and recharging aerobic river water. In total, 25 cores driven through a 1.5 m sampling interval were collected from the river bed with a mean core recovery of 75%. The ability to deploy this method from a fishing vessel makes the tool more cost effective than traditional marine-based drilling operations which often use barges, tug boats, and drilling rigs. © 2014, National Ground Water Association.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050060957','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050060957"><span>Recent Monitoring of Suspended <span class="hlt">Sediment</span> Patterns along Louisiana's Coastal <span class="hlt">Zone</span> using ER-2 based MAS Data and Terra Based MODIS Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moeller, Christopher C.; Gunshor, M. M.; Menzel, W. P.; Huh, O. K.; Walker, N. D.; Rouse, L. J.</p> <p>2001-01-01</p> <p>The University nf Wisconsin and Louisiana State University have teamed to study the forcing of winter season cold frontal wind systems on <span class="hlt">sediment</span> distribution patterns and geomorphology in the Louisiana coastal <span class="hlt">zone</span>. Wind systems associated with cold fronts have been shown to model coastal circulation and resuspend <span class="hlt">sediments</span> along the micro tidal Louisiana coast (Roberts et at. 1987, Moeller et al. 1993). Remote sensing data is being used to map and track <span class="hlt">sediment</span> distribution patterns for various wind conditions. Suspended <span class="hlt">sediment</span> is a building material for coastal progradation and wetlands renewal, but also restricts access to marine nursery environments and impacts oyster bed health. Transferring a suspended <span class="hlt">sediment</span> concentration (SSC) algorithm to EOS MODerate resolution Imaging Spectroradiometer (MODIS; Barnes et al. 1998) observations may enable estimates of SSC globally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ofr/2017/1024/ofr20171024.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ofr/2017/1024/ofr20171024.pdf"><span>Nearshore <span class="hlt">sediment</span> thickness, Fire Island, New York</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Locker, Stanley D.; Miselis, Jennifer L.; Buster, Noreen A.; Hapke, Cheryl J.; Wadman, Heidi M.; McNinch, Jesse E.; Forde, Arnell S.; Stalk, Chelsea A.</p> <p>2017-04-03</p> <p>Investigations of coastal change at Fire Island, New York (N.Y.), sought to characterize <span class="hlt">sediment</span> budgets and determine geologic framework controls on coastal processes. Nearshore <span class="hlt">sediment</span> thickness is critical for assessing coastal system <span class="hlt">sediment</span> availability, but it is largely unquantified due to the difficulty of conducting geological or geophysical surveys across the nearshore. This study used an amphibious vessel to acquire chirp subbottom profiles. These profiles were used to characterize nearshore geology and provide an assessment of nearshore <span class="hlt">sediment</span> volume. Two resulting <span class="hlt">sediment</span>-thickness maps are provided: total Holocene <span class="hlt">sediment</span> thickness and the thickness of the active shoreface. The Holocene <span class="hlt">sediment</span> section represents deposition above the maximum flooding surface that is related to the most recent marine transgression. The active shoreface section is the uppermost Holocene <span class="hlt">sediment</span>, which is interpreted to represent the portion of the shoreface thought to contribute to present and future coastal behavior. The <span class="hlt">sediment</span> distribution patterns correspond to previously defined <span class="hlt">zones</span> of erosion, accretion, and stability along the island, demonstrating the importance of <span class="hlt">sediment</span> availability in the coastal response to storms and seasonal variability. The eastern <span class="hlt">zone</span> has a thin nearshore <span class="hlt">sediment</span> thickness, except for an ebb-tidal deposit at the wilderness breach caused by Hurricane Sandy. Thicker <span class="hlt">sediment</span> is found along a central <span class="hlt">zone</span> that includes shoreface-attached sand ridges, which is consistent with a stable or accretional coastline in this area. The thickest overall Holocene section is found in the western <span class="hlt">zone</span> of the study, where a thicker lower section of Holocene <span class="hlt">sediment</span> appears related to the westward migration of Fire Island Inlet over several hundred years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.T34C..04C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.T34C..04C"><span>Mineralogy and fluid content of <span class="hlt">sediments</span> entering the Costa Rica subduction <span class="hlt">zone</span> - Results from Site U1414, IODP Expedition 344</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Charpentier, D.; Buatier, M.; Kutterolf, S.; Straub, S. M.; Nascimento, D.; Millan, C.</p> <p>2013-12-01</p> <p>Subduction <span class="hlt">zones</span> are characterized by the largest thrust earthquakes, as quantified by both rupture area and seismic moment release. Offshore Costa Rica, the oceanic Cocos Plate subducts under the Caribbean plate forming the southern end of the Middle America trench. A high convergence rate and almost complete subduction of incoming <span class="hlt">sediments</span> make the Costa Rica convergent margin an extremely dynamic environment. The Costa Rica Seismogenesis Project (CRISP) is designed to understand the processes that control nucleation and seismic rupture of large earthquakes at erosional subduction <span class="hlt">zones</span>. Site U1414 of IODP Exp.344 was drilled to investigate the material from the incoming Cocos Plate. A key parameter of incoming plate is fluid content and release because it impacts deformation within the subduction complex. The deposition, compaction and diagenesis of sedimentary rocks control the distribution of fluids, fluid pressures and fluid flow patterns within subduction <span class="hlt">zones</span>. We therefore decided to characterize <span class="hlt">sediment</span> composition and quantify the different types of water at Site U1414. Mineralogical investigations were performed using optical and electronic microscope observations, X Ray Diffraction (on bulk and clay fractions), Cation Exchange Capacity measurements, carbon analyses (to determine carbonate contents), and sequenced extractions in NaOH (to quantify the biogenic opal content). Fluid characteristics were approached by thermal gravimetric analyses. The entire sedimentary sequence was <span class="hlt">recovered</span> at Site U1414 and can be divided into three major sedimentary units. The first one is a hemipelagic silty clay to clay with a gradual increase of calcareous nannofossils. The dominant mineral is smectite associated in the clay fractions with kaolinite and zeolites. Small amounts of biogenic opal have been analyzed. Other minerals like quartz, feldspar and calcite are also present. The second unit is composed of nannofossil-rich calcareous ooze. The proportion of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29523543','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29523543"><span>Isoprenoid quinones resolve the stratification of microbial redox processes in a biogeochemical continuum from the photic <span class="hlt">zone</span> to deep anoxic <span class="hlt">sediments</span> of the Black Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Becker, Kevin W; Elling, Felix J; Schröder, Jan M; Lipp, Julius S; Goldhammer, Tobias; Zabel, Matthias; Elvert, Marcus; Overmann, Jörg; Hinrichs, Kai-Uwe</p> <p>2018-03-09</p> <p>The stratified water column of the Black Sea serves as a model ecosystem for studying the interactions of microorganisms with major biogeochemical cycles. Here we provide detailed analysis of isoprenoid quinones to study microbial redox processes in the ocean. In a continuum from the photic <span class="hlt">zone</span> through the chemocline into deep anoxic <span class="hlt">sediments</span> of the southern Black Sea, diagnostic quinones and inorganic geochemical parameters indicate niche segregation between redox processes and corresponding shifts in microbial community composition. Quinones specific for oxygenic photosynthesis and aerobic respiration dominate oxic waters, while quinones associated with thaumarchaeal ammonia-oxidation and bacterial methanotrophy, respectively, dominate a narrow interval in suboxic waters. Quinone distributions indicate highest metabolic diversity within the anoxic <span class="hlt">zone</span>, with anoxygenic photosynthesis being a major process in its photic layer. In the dark anoxic layer, quinone profiles indicate occurrence of bacterial sulfur and nitrogen cycling, archaeal methanogenesis, and archaeal methanotrophy. Multiple novel ubiquinone isomers, possibly originating from unidentified intra-aerobic anaerobes, occur in this <span class="hlt">zone</span>. The respiration modes found in the anoxic <span class="hlt">zone</span> continue into shallow subsurface <span class="hlt">sediments</span>, but quinone abundances rapidly decrease within the upper 50 cm below sea floor, reflecting the transition to lower energy availability. In the deep subseafloor <span class="hlt">sediments</span>, quinone distributions and geochemical profiles indicate archaeal methanogenesis/methanotrophy and potentially bacterial fermentative metabolisms. We observed that sedimentary quinone distributions track lithology, which supports prior hypotheses that deep biosphere community composition and metabolisms are determined by environmental conditions during <span class="hlt">sediment</span> deposition. Importance Microorganisms play crucial roles in global biogeochemical cycles. Yet, we have only a fragmentary understanding of the diversity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..107a2022S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..107a2022S"><span>Preliminary estimating the contemporary <span class="hlt">sedimentation</span> trend in dry valley bottoms of first-order catchments of different landscape <span class="hlt">zones</span> of the Russian Plain using the 137Cs as a chronomarker</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sharifullin, A.; Gusarov, A.; Gafurov, A.; Essuman-Quainoo, B.</p> <p>2018-01-01</p> <p>A general trend of erosion processes over the last 50-60 years can be estimated by dating <span class="hlt">sediments</span> washed off from arable lands and accumulated in the first-order dry valleys bottoms. Three small (first-order) catchments were chosen as objects of the study. They are located, respectively, in the southern part of the taiga <span class="hlt">zone</span>, the <span class="hlt">zone</span> of temperate broad-leaf forests and the forest-steppe <span class="hlt">zone</span> of the Russian Plain. To date the <span class="hlt">sediments</span> accumulated in the bottoms the radioactive caesium-137 (137Cs) of global (since 1954) and Chernobyl origin (1986) had been used as a chronomarker. The average (for all the catchments) <span class="hlt">sedimentation</span> rates during the global 137Cs fallout period (1963(1954)-1986) are at least 0.88-2.71 cm per year.For the period that has passed since the Chernobyl accident (1986-2015(2016)) the average rates were 0.15-1.07 cm per year. The greatest reduction in the <span class="hlt">sedimentation</span> rates is observed in the subzone of the southern taiga, the lowest one is in the forest-steppe <span class="hlt">zone</span> of the Russian Plain. The main reason for such significant reduction in the rates of <span class="hlt">sedimentation</span> of the soil erosion products in the dry valley bottoms was a reduction of surface runoff within the catchments during a snowmelt period, as well as crop-rotation changes there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3638456','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3638456"><span>Distribution of dehalogenation activity in subseafloor <span class="hlt">sediments</span> of the Nankai Trough subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Futagami, Taiki; Morono, Yuki; Terada, Takeshi; Kaksonen, Anna H.; Inagaki, Fumio</p> <p>2013-01-01</p> <p>Halogenated organic matter buried in marine subsurface <span class="hlt">sediment</span> may serve as a source of electron acceptors for anaerobic respiration of subseafloor microbes. Detection of a diverse array of reductive dehalogenase-homologous (rdhA) genes suggests that subseafloor organohalide-respiring microbial communities may play significant ecological roles in the biogeochemical carbon and halogen cycle in the subseafloor biosphere. We report here the spatial distribution of dehalogenation activity in the Nankai Trough plate-subduction <span class="hlt">zone</span> of the northwest Pacific off the Kii Peninsula of Japan. Incubation experiments with slurries of <span class="hlt">sediment</span> collected at various depths and locations showed that degradation of several organohalides tested only occurred in the shallow sedimentary basin, down to 4.7 metres below the seafloor, despite detection of rdhA in the deeper <span class="hlt">sediments</span>. We studied the phylogenetic diversity of the metabolically active microbes in positive enrichment cultures by extracting RNA, and found that Desulfuromonadales bacteria predominate. In addition, for the isolation of genes involved in the dehalogenation reaction, we performed a substrate-induced gene expression screening on DNA extracted from the enrichment cultures. Diverse DNA fragments were obtained and some of them showed best BLAST hit to known organohalide respirers such as Dehalococcoides, whereas no functionally known dehalogenation-related genes such as rdhA were found, indicating the need to improve the molecular approach to assess functional genes for organohalide respiration. PMID:23479745</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23479745','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23479745"><span>Distribution of dehalogenation activity in subseafloor <span class="hlt">sediments</span> of the Nankai Trough subduction <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Futagami, Taiki; Morono, Yuki; Terada, Takeshi; Kaksonen, Anna H; Inagaki, Fumio</p> <p>2013-04-19</p> <p>Halogenated organic matter buried in marine subsurface <span class="hlt">sediment</span> may serve as a source of electron acceptors for anaerobic respiration of subseafloor microbes. Detection of a diverse array of reductive dehalogenase-homologous (rdhA) genes suggests that subseafloor organohalide-respiring microbial communities may play significant ecological roles in the biogeochemical carbon and halogen cycle in the subseafloor biosphere. We report here the spatial distribution of dehalogenation activity in the Nankai Trough plate-subduction <span class="hlt">zone</span> of the northwest Pacific off the Kii Peninsula of Japan. Incubation experiments with slurries of <span class="hlt">sediment</span> collected at various depths and locations showed that degradation of several organohalides tested only occurred in the shallow sedimentary basin, down to 4.7 metres below the seafloor, despite detection of rdhA in the deeper <span class="hlt">sediments</span>. We studied the phylogenetic diversity of the metabolically active microbes in positive enrichment cultures by extracting RNA, and found that Desulfuromonadales bacteria predominate. In addition, for the isolation of genes involved in the dehalogenation reaction, we performed a substrate-induced gene expression screening on DNA extracted from the enrichment cultures. Diverse DNA fragments were obtained and some of them showed best BLAST hit to known organohalide respirers such as Dehalococcoides, whereas no functionally known dehalogenation-related genes such as rdhA were found, indicating the need to improve the molecular approach to assess functional genes for organohalide respiration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMEP31B1003C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMEP31B1003C"><span>River Suspended <span class="hlt">Sediment</span> and Particulate Organic Carbon Transport in Two Montane Catchments in the Luquillo Critical <span class="hlt">Zone</span> Observatory of Puerto Rico over 25 years: 1989 to 2014</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, K. E.; Plante, A. F.; Willenbring, J. K.; Jerolmack, D. J.; Gonzalez, G.; Stallard, R. F.; Murphy, S. F.; Vann, D. R.; Leon, M.; McDowell, W. H.</p> <p>2015-12-01</p> <p>Physical erosion in mountain catchments mobilizes large amounts of <span class="hlt">sediment</span>, while exporting carbon and nutrients from forest ecosystems. This study expands from previous studies quantifying river suspended <span class="hlt">sediment</span> and particulate organic carbon loads in the Luquillo Critical <span class="hlt">Zone</span> Observatory, in Puerto Rico. We evaluate the influences on river suspended load due to i) underlying basin geology, ii) hillslope debris and biomass supply, and iii) hurricanes and large storms. In the Mameyes and Icacos catchments of the Luquillo Mountains, we estimate suspended <span class="hlt">sediment</span> and particulate organic carbon yields over a 25-year period using streamflow discharge determined from stage measurements at 15-intervals, with estimates of discharge replacing gaps in data, and over 3000 suspended <span class="hlt">sediment</span> samples. We estimate variation in suspended <span class="hlt">sediment</span> loads over time, and examine variation in particulate organic carbon loads. Mass spectrometry was used to determine organic carbon concentrations. We confirm that higher suspended <span class="hlt">sediment</span> fluxes occurred i) in the highly weathered quartz diorite catchment rather than the predominantly volcaniclastic catchment, ii) on the rising limb of the hydrograph once a threshold discharge had been reached, and iii) during hurricanes and other storm events, and we explore these influences on particulate organic carbon transport. Transport of suspended <span class="hlt">sediment</span> and particulate organic carbon in the rivers shows considerable hysteresis, and we evaluate the extent to which hysteresis affects particulate fluxes over time and between catchments. Because particulate organic carbon is derived from the critical <span class="hlt">zone</span> and transported during high flow, our research highlights the role of major tropical storms in controlling carbon storage in the critical <span class="hlt">zone</span> and the coastal ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMPP11B1312V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMPP11B1312V"><span>The <span class="hlt">sediment</span> record of Lake Ohrid (Albania/Macedonia)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vogel, H.; Wagner, B.; Sulpizio, R.; Zanchetta, G.; Schouten, S.; Leng, M. J.; Wessels, M.; Nowaczyk, N.; Hilgers, A.</p> <p>2009-12-01</p> <p>Lake Ohrid, a transboundary lake shared by the former Yugoslav Republic of Macedonia and the Republic of Albania is with its likely Pliocene age, considered to be the oldest existing lake in Europe. Since 2004 numerous <span class="hlt">sediment</span> successions have been <span class="hlt">recovered</span> from Lake Ohrid in order to investigate modern and past <span class="hlt">sedimentation</span> patterns, to establish a tephrostratigraphic and chronological framework, and to infer past climatic and environmental changes. Frequent occurrences of well-dated tephra and cryptotephra layers as well as radiocarbon, electron spin resonance, and luminescence dating allowed the establishment of a chronological framework for the <span class="hlt">recovered</span> <span class="hlt">sediment</span> successions. These data revealed that the <span class="hlt">sediment</span> successions <span class="hlt">recovered</span> so far in part reach well back into MIS 6. Despite distinct spatial heterogeneity in <span class="hlt">sediment</span> composition, Lake Ohrid appears to have reacted uniformly to climatic forcing on changes in catchment configuration, limnology and hydrology in the past as evidenced by contemporaneous changes in <span class="hlt">sediment</span> composition in successions from different parts of the lake basin. The interplay of climatic forced factors has varied significantly in the course of the last glacial-interglacial cycle and led to distinctly different <span class="hlt">sediment</span> characteristics during glacial and interglacial phases at Lake Ohrid. Beside this general pattern tied to high amplitude climate fluctuations, short-term climatic fluctuations of reduced amplitude are also recorded in the <span class="hlt">sediment</span> successions and generally well correlated to other paleoclimate records in the Mediterranean. Initial quantitative inferences of past lake surface temperatures using the TEX86 paleothermometer revealed c. 5-6°C lower temperatures in the glacial compared with the interglacial periods. The reconstructed glacial and interglacial temperatures from Lake Ohrid correspond relatively well with temperature anomalies derived from sea surface temperature reconstructions in the marine (-4°C) and</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021161','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021161"><span>Chemistry, isotopic composition, and origin of a methane-hydrogen sulfide hydrate at the Cascadia subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kastner, M.; Kvenvolden, K.A.; Lorenson, T.D.</p> <p>1998-01-01</p> <p>Although the presence of extensive gas hydrate on the Cascadia margin, offshore from the western U.S. and Canada, has been inferred from marine seismic records and pore water chemistry, solid gas hydrate has only been found at one location. At Ocean Drilling Program (ODP) Site 892, offshore from central Oregon, gas hydrate was <span class="hlt">recovered</span> close to the <span class="hlt">sediment</span> - water interface at 2-19 m below the seafloor, (mbsf) at 670 m water depth. The gas hydrate occurs as elongated platy crystals or crystal aggregates, mostly disseminated irregularly, with higher concentrations occurring in discrete <span class="hlt">zones</span>, thin layers, and/or veinlets parallel or oblique to the bedding. A 2-to 3-cm thick massive gas hydrate layer, parallel to bedding, was <span class="hlt">recovered</span> at ???17 mbsf. Gas from a sample of this layer was composed of both CH4 and H2S. This sample is the first mixed-gas hydrate of CH4-H2S documented in ODP; it also contains ethane and minor amounts of CO2. Measured temperature of the <span class="hlt">recovered</span> core ranged from 2 to - 18??C and are 6 to 8 degrees lower than in-situ temperatures. These temperature anomalies were caused by the partial dissociation of the CH4-H2S hydrate during recovery without a pressure core sampler. During this dissociation, toxic levels of H2S (??34S, +27.4???) were released. The ??13C values of the CH4 in the gas hydrate, -64.5 to -67.5???(PDB), together with ??D values of - 197 to - 199???(SMOW) indicate a primarily microbial source for the CH4. The ??18O value of the hydrate H2O is +2.9???(SMOW), comparable with the experimental fractionation factor for sea-ice. The unusual composition (CH4-H2S) and depth distribution (2-19 mbsf) of this gas hydrate indicate mixing between a methane-rich fluid with a pore fluid enriched in sulfide; at this site the former is advecting along an inclined fault into the active sulfate reduction <span class="hlt">zone</span>. The facts that the CH4-H2S hydrate is primarily confined to the present day active sulfate reduction <span class="hlt">zone</span> (2-19 mbsf), and that from here</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24798421','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24798421"><span>Concentration, composition and sources of PAHs in the coastal <span class="hlt">sediments</span> of the exclusive economic <span class="hlt">zone</span> (EEZ) of Qatar, Arabian Gulf.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Soliman, Y S; Al Ansari, E M S; Wade, T L</p> <p>2014-08-30</p> <p>Surface <span class="hlt">sediments</span> were collected from sixteen locations in order to assess levels and sources of polycyclic aromatic hydrocarbons (PAHs) in <span class="hlt">sediments</span> of Qatar exclusive economic <span class="hlt">zone</span> (EEZ). Samples were analyzed for 16 parent PAHs, 18 alkyl homologs and for dibenzothiophenes. Total PAHs concentration (∑PAHs) ranged from 2.6 ng g(-1) to 1025 ng g(-1). The highest PAHs concentrations were in <span class="hlt">sediments</span> in and adjacent to harbors. Alkylated PAHs predominated most of the sampling locations reaching up to 80% in offshore locations. Parent PAHs and parent high molecular weight PAHs dominated location adjacent to industrial activities and urban areas. The origin of PAHs sources to the <span class="hlt">sediments</span> was elucidated using ternary plot, indices, and molecular ratios of specific compounds such as (Ant/Phe+Ant), (Flt/Flt+Pyr). PAHs inputs to most coastal sites consisted of mixture of petroleum and combustion derived sources. However, inputs to the offshore <span class="hlt">sediments</span> were mainly of petroleum origin. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25976635','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25976635"><span>Evaluation of Baermann apparatus <span class="hlt">sedimentation</span> time on recovery of Strongylus vulgaris and S. edentatus third stage larvae from equine coprocultures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bellaw, Jennifer L; Nielsen, Martin K</p> <p>2015-06-30</p> <p>Traditional methods of diagnosing equine Strongylinae infections require culturing feces, <span class="hlt">sedimenting</span> the culture media in Baermann apparatuses, collecting the <span class="hlt">sediment</span>, and morphologically identifying <span class="hlt">recovered</span> third stage larvae. However, this method is plagued by low negative predictive values. This study evaluated <span class="hlt">sedimentation</span> time within the Baermann apparatus by comparing larval recovery from the traditionally collected <span class="hlt">sediment</span>, "<span class="hlt">sediment</span> 1", and from the usually discarded remaining fluid contents, "<span class="hlt">sediment</span> 2", of the Baermann apparatus after 12, 24, and 48 h. A grand total of 147,482 larvae were <span class="hlt">recovered</span> and examined. <span class="hlt">Sedimentation</span> time did not significantly influence total larval recovery. At all three durations, significantly more Cyathostominae and Strongylus vulgaris larvae were covered from <span class="hlt">sediment</span> 1 than from <span class="hlt">sediment</span> 2. However, less than 60% of all <span class="hlt">recovered</span> Strongylus edentatus were <span class="hlt">recovered</span> from <span class="hlt">sediment</span> 1. As 95% of S. vulgaris larvae were always <span class="hlt">recovered</span> from <span class="hlt">sediment</span> 1, the need for collection and examination of the remaining fluid contents of the Baermann apparatus is obviated when performing coprocultures for diagnosis of S. vulgaris infections, and <span class="hlt">sedimentation</span> for 12h is adequate. Approximately 70% of Cyathostominae were <span class="hlt">recovered</span> in <span class="hlt">sediment</span> 1 at all durations, suggesting that 12h of <span class="hlt">sedimentation</span> is adequate, although there is a need for future research to evaluate the risk of selection bias at differing <span class="hlt">sedimentation</span> times among individual cyathostomin species. In contrast to S. vulgaris, collecting and examining the entire contents of the Baermann apparatus may be necessary when an increased diagnostic sensitivity and negative predictive value is desired in diagnosing S. edentatus infections as only 38-61% of larvae were <span class="hlt">recovered</span> from <span class="hlt">sediment</span> 1 portion of the Baermann apparatus. This information will allow researchers and practitioners to make more informed decisions in choosing appropriate larval recovery techniques, balancing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22980125','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22980125"><span>UV filters, ethylhexyl methoxycinnamate, octocrylene and ethylhexyl dimethyl PABA from untreated wastewater in <span class="hlt">sediment</span> from eastern Mediterranean river transition and coastal <span class="hlt">zones</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Amine, Helmieh; Gomez, Elena; Halwani, Jalal; Casellas, Claude; Fenet, Hélène</p> <p>2012-11-01</p> <p>UVF may occur in the aquatic environment through two principal sources: direct inputs from recreational activities and indirect wastewater- and river-borne inputs. The aim of this study was to obtain a first overview of levels of three UVF (EHMC, OC and OD-PABA) in coastal areas subjected to river inputs, untreated wastewater discharges and dumpsite leachates. We selected three eastern Mediterranean rivers that have been impacted for decades by untreated wastewater release and collected <span class="hlt">sediment</span> in the coastal <span class="hlt">zone</span> during the hot and humid seasons. Western Mediterranean sites receiving treated wastewaters were analyzed for comparison. The results gave an overview of <span class="hlt">sediment</span> contamination under these two contrasted situations representative of Mediterranean coastal areas without bathing activities. The analysis of the three UVF revealed the ubiquity and high point source contamination by EHMC and OC in transition and coastal <span class="hlt">zones</span>, with levels as high as 128 ng g(-1)d.w. OD-PABA was also frequently detected, but at lower concentrations (<LOD-17 ng g(-1)d.w.). A temporal trend was observed, with a higher <span class="hlt">sediment</span> concentration in the dry period (August and October). Based on these results, we conclude that there is background contamination from river input that could be exacerbated by the direct contribution in coastal bathing <span class="hlt">zones</span>. Copyright © 2012. Published by Elsevier Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037625','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037625"><span>Late Hesperian plains formation and degradation in a low <span class="hlt">sedimentation</span> <span class="hlt">zone</span> of the northern lowlands of Mars</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rodriguez, J.A.P.; Tanaka, K.L.; Berman, D.C.; Kargel, J.S.</p> <p>2010-01-01</p> <p>The plains materials that form the martian northern lowlands suggest large-scale <span class="hlt">sedimentation</span> in this part of the planet. The general view is that these sedimentary materials were transported from <span class="hlt">zones</span> of highland erosion via outflow channels and other fluvial systems. The study region, the northern circum-polar plains south of Gemini Scopuli on Planum Boreum, comprises the only extensive <span class="hlt">zone</span> in the martian northern lowlands that does not include sub-basin floors nor is downstream from outflow channel systems. Therefore, within this <span class="hlt">zone</span>, the ponding of fluids and fluidized <span class="hlt">sediments</span> associated with outflow channel discharges is less likely to have taken place relative to sub-basin areas that form the other northern circum-polar plains surrounding Planum Boreum. Our findings indicate that during the Late Hesperian sedimentary deposits produced by the erosion of an ancient cratered landscape, as well as via sedimentary volcanism, were regionally emplaced to form extensive plains materials within the study region. The distribution and magnitude of surface degradation suggest that groundwater emergence from an aquifer that extended from the Arabia Terra cratered highlands to the northern lowlands took place non-catastrophically and regionally within the study region through faulted upper crustal materials. In our model the margin of the Utopia basin adjacent to the study region may have acted as a boundary to this aquifer. Partial destruction and dehydration of these Late Hesperian plains, perhaps induced by high thermal anomalies resulting from the low thermal conductivity of these materials, led to the formation of extensive knobby fields and pedestal craters. During the Early Amazonian, the rates of regional resurfacing within the study region decreased significantly; perhaps because the knobby ridges forming the eroded impact crater rims and contractional ridges consisted of thermally conductive indurated materials, thereby inducing freezing of the tectonically</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020521','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020521"><span>Organic carbon accumulation and preservation in surface <span class="hlt">sediments</span> on the Peru margin</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Arthur, M.A.; Dean, W.E.; Laarkamp, K.</p> <p>1998-01-01</p> <p>Concentrations and characteristics of organic matter in surface <span class="hlt">sediments</span> deposited under an intense oxygen-minimum <span class="hlt">zone</span> on the Peru margin were studied in samples from deck-deployed box cores and push cores acquired by submersible on two transects spanning depths of 75 to 1000 m at 12??and 13.5??S. The source of organic matter to the seafloor in these areas is almost entirely marine material as confirmed by the narrow range of ??13C of organic carbon obtained in the present study (-20.3 to -21.6???; PDB) and the lack of any relationship between pyrolysis hydrogen index and carbon isotope composition. Organic carbon contents are highest (up to 16%) on the slope at depths between 75 and 350 m in <span class="hlt">sediments</span> deposited under intermediate water masses with low dissolved oxygen concentrations (< 5 ??mol/kg). Even at these low concentrations of dissolved oxygen, however, the surface <span class="hlt">sediments</span> that were <span class="hlt">recovered</span> from these depths are dominantly unlaminated. Strong currents (up to 30 cm/s) associated with the poleward-flowing Peru Undercurrent were measured at depths between 160 and 300 m on both transects. The seafloor in this range of water depths is characterized by bedforms stabilized by bacterial mats, extensive authigenic mineral crusts, and (or) thick organic flocs. Constant advection of dissolved oxygen, although in low concentrations, active resuspension of surficial organic matter, activity of organisms, and transport of fine-grained <span class="hlt">sediment</span> to and from more oxygenated <span class="hlt">zones</span> all contribute to greater degradation and poorer initial preservation of organic matter than might be expected under oxygen-deficient conditions. Dissolved-oxygen concentrations ultimately may be the dominant affect on organic matter characteristics, but reworking of fine-grained <span class="hlt">sediment</span> and organic matter by strong bottom currents and redeposition on the seafloor in areas of lower energy also exert important controls on organic carbon concentration and degree of oxidation in this region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JSG....33.1554L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JSG....33.1554L"><span>Fault architecture and deformation processes within poorly lithified rift <span class="hlt">sediments</span>, Central Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loveless, Sian; Bense, Victor; Turner, Jenni</p> <p>2011-11-01</p> <p>Deformation mechanisms and resultant fault architecture are primary controls on the permeability of faults in poorly lithified <span class="hlt">sediments</span>. We characterise fault architecture using outcrop studies, hand samples, thin sections and grain-size data from a minor (1-10 m displacement) normal-fault array exposed within Gulf of Corinth rift <span class="hlt">sediments</span>, Central Greece. These faults are dominated by mixed <span class="hlt">zones</span> with poorly developed fault cores and damage <span class="hlt">zones</span>. In poorly lithified <span class="hlt">sediment</span> deformation is distributed across the mixed <span class="hlt">zone</span> as beds are entrained and smeared. We find particulate flow aided by limited distributed cataclasis to be the primary deformation mechanism. Deformation may be localised in more competent <span class="hlt">sediments</span>. Stratigraphic variations in <span class="hlt">sediment</span> competency, and the subsequent alternating distributed and localised strain causes complexities within the mixed <span class="hlt">zone</span> such as undeformed blocks or lenses of cohesive <span class="hlt">sediment</span>, or asperities at the mixed <span class="hlt">zone</span>/protolith boundary. Fault tip bifurcation and asperity removal are important processes in the evolution of these fault <span class="hlt">zones</span>. Our results indicate that fault <span class="hlt">zone</span> architecture and thus permeability is controlled by a range of factors including lithology, stratigraphy, cementation history and fault evolution, and that minor faults in poorly lithified <span class="hlt">sediment</span> may significantly impact subsurface fluid flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004GeCoA..68.4429B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004GeCoA..68.4429B"><span>Geochemistry of Peruvian near-surface <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Böning, Philipp; Brumsack, Hans-Jürgen; Böttcher, Michael E.; Schnetger, Bernhard; Kriete, Cornelia; Kallmeyer, Jens; Borchers, Sven Lars</p> <p>2004-11-01</p> <p>Sixteen short <span class="hlt">sediment</span> cores were <span class="hlt">recovered</span> from the upper edge (UEO), within (WO) and below (BO) the oxygen minimum <span class="hlt">zone</span> (OMZ) off Peru during cruise 147 of R/V Sonne. Solids were analyzed for major/trace elements, total organic carbon, total inorganic carbon, total sulfur, the stable sulfur isotope composition (δ 34S) of pyrite, and sulfate reduction rates (SRR). Pore waters were analyzed for dissolved sulfate/sulfide and δ 34S of sulfate. In all cores highest SRR were observed in the top 5 cm where pore water sulfate concentrations varied little due to resupply of sulfate by sulfide oxidation and/or diffusion of sulfate from bottom water. δ 34S of dissolved sulfate showed only minor downcore increases. Strong 32S enrichments in sedimentary pyrite (to -48‰ vs. V-CDT) are due to processes in the oxidative part of the sulfur cycle in addition to sulfate reduction. Manganese and Co are significantly depleted in Peruvian upwelling <span class="hlt">sediments</span> most likely due to mobilization from particles settling through the OMZ, whereas release of both elements from reducing <span class="hlt">sediments</span> only seems to occur in near-coastal sites. Cadmium, Mo and Re are exceptionally enriched in WO <span class="hlt">sediments</span> (<600 m water depth). High Re and moderate Cd and Mo enrichments are seen in BO <span class="hlt">sediments</span> (>600 m water depth). Re/Mo ratios indicate anoxic and suboxic conditions for WO and BO <span class="hlt">sediments</span>, respectively. Cadmium and Mo downcore profiles suggest considerable contribution to UEO/WO <span class="hlt">sediments</span> by a biodetrital phase, whereas Re presumably accumulates via diffusion across the <span class="hlt">sediment</span>-water interface to precipitation depth. Uranium is distinctly enriched in WO <span class="hlt">sediments</span> (due to sulfidic conditions) and in some BO <span class="hlt">sediments</span> (due to phosphorites). Silver transfer to suboxic BO <span class="hlt">sediments</span> is likely governed by diatomaceous matter input, whereas in anoxic WO <span class="hlt">sediments</span> Ag is presumably trapped due to sulfide precipitation. Cadmium, Cu, Zn, Ni, Cr, Ag, and T1 predominantly accumulate via biogenic pre</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFMOS71B0279S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFMOS71B0279S"><span>Relationship of Hotspots to the Distribution of Surficial Surf-<span class="hlt">Zone</span> <span class="hlt">Sediments</span> along the Outer Banks of North Carolina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schupp, C. A.; McNinch, J. E.; List, J. H.; Farris, A. S.</p> <p>2002-12-01</p> <p>The formation and behavior of hotspots, or sections of the beach that exhibit markedly higher shoreline change rates than adjacent regions, are poorly understood. Several hotspots have been identified on the Outer Banks, a developed barrier island in North Carolina. To better understand hotspot dynamics and the potential relationship to the geologic framework in which they occur, the surf <span class="hlt">zone</span> between Duck and Bodie Island was surveyed in June 2002 as part of a research effort supported by the U.S. Geological Survey and U.S. Army Corps of Engineers. Swath bathymetry, sidescan sonar, and chirp seismic were used to characterize a region 40 km long and1 km wide. Hotspot locations were pinpointed using standard deviation values for shoreline position as determined by monthly SWASH buggy surveys of the mean high water contour between October 1999 and September 2002. Observational data and sidescan images were mapped to delineate regions of surficial <span class="hlt">sediment</span> distributions, and regions of interest were ground-truthed via grab samples or visual inspection. General kilometer-scale correlation between acoustic backscatter and high shoreline standard deviation is evident. Acoustic returns are uniform in a region of Duck where standard deviation is low, but backscatter is patchy around the Kitty Hawk hotspot, where standard deviation is higher. Based on ground-truthing of an area further north, these patches are believed to be an older ravinement surface of fine <span class="hlt">sediment</span>. More detailed analyses of the correlation between acoustic data, standard deviation, and hotspot locations will be presented. Future work will include integration of seismic, bathymetric, and sidescan data to better understand the links between sub-bottom geology, temporal changes in surficial <span class="hlt">sediments</span>, surf-<span class="hlt">zone</span> <span class="hlt">sediment</span> budgets, and short-term changes in shoreline position and morphology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70178100','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70178100"><span>Physical properties of repressurized samples <span class="hlt">recovered</span> during the 2006 National Gas Hydrate Program expedition offshore India</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Winters, William J.; Waite, William F.; Mason, David H.; Kumar, P.</p> <p>2008-01-01</p> <p>As part of an international cooperative research program, the U.S. Geological Survey (USGS) and researchers from the National Gas Hydrate Program (NGHP) of India are studying the physical properties of <span class="hlt">sediment</span> <span class="hlt">recovered</span> during the NGHP-01 cruise conducted offshore India during 2006. Here we report on index property, acoustic velocity, and triaxial shear test results for samples <span class="hlt">recovered</span> from the Krishna-Godavari Basin. In addition, we discuss the effects of sample storage temperature, handling, and change in structure of fine-grained <span class="hlt">sediment</span>. Although complex, sub-vertical planar gas-hydrate structures were observed in the silty clay to clayey silt samples prior to entering the Gas Hydrate And <span class="hlt">Sediment</span> Test Laboratory Instrument (GHASTLI), the samples yielded little gas post test. This suggests most, if not all, gas hydrate dissociated during sample transfer. Mechanical properties of hydrate-bearing marine <span class="hlt">sediment</span> are best measured by avoiding sample depressurization. By contrast, mechanical properties of hydrate-free <span class="hlt">sediments</span>, that are shipped and stored at atmospheric pressure can be approximated by consolidating core material to the original in situ effective stress.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H51H..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H51H..01M"><span>Tackling the Challenge of Deep Vadose <span class="hlt">Zone</span> Remediation at the Hanford Site</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morse, J. G.; Wellman, D. M.; Gephart, R.</p> <p>2010-12-01</p> <p>The Central Plateau of the Hanford Site in Washington State contains some 800 waste disposal sites where 1.7 trillion liters of contaminated water was once discharged into the subsurface. Most of these sites received liquids from the chemical reprocessing of spent uranium fuel to <span class="hlt">recover</span> plutonium. In addition, 67 single shell tanks have leaked or are suspected to have leaked 3.8 million liters of high alkali and aluminate rich cesium-contaminated liquids into the <span class="hlt">sediment</span>. Today, this inventory of subsurface contamination contains an estimated 550,000 curies of radioactivity and 150 million kg (165,000 tons) of metals and hazardous chemicals. Radionuclides range from mobile 99Tc to more immobilized 137Cs, 241Am, uranium, and plutonium. A significant fraction of these contaminants likely remain within the deep vadose <span class="hlt">zone</span>. Plumes of groundwater containing tritium, nitrate, 129I and other contaminants have migrated through the vadose <span class="hlt">zone</span> and now extend outward from the Central Plateau to the Columbia River. During most of Hanford Site history, subsurface studies focused on groundwater monitoring and characterization to support waste management decisions. Deep vadose <span class="hlt">zone</span> studies were not a priority because waste practices relied upon that <span class="hlt">zone</span> to buffer contaminant releases into the underlying aquifer. Remediation of the deep vadose <span class="hlt">zone</span> is now central to Hanford Site cleanup because these <span class="hlt">sediments</span> can provide an ongoing source of contamination to the aquifer and therefore to the Columbia River. However, characterization and remediation of the deep vadose <span class="hlt">zone</span> pose some unique challenges. These include <span class="hlt">sediment</span> thickness; contaminant depth; coupled geohydrologic, geochemical, and microbial processes controlling contaminant spread; limited availability and effectiveness of traditional characterization tools and cleanup remedies; and predicting contaminant behavior and remediation performance over long time periods and across molecular to field scales. The U</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5170918-process-recovering-products-from-oil-shale','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5170918-process-recovering-products-from-oil-shale"><span>Process for <span class="hlt">recovering</span> products from oil shale</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Jacobs, H.R.; Udell, K.S.</p> <p></p> <p>A process is claimed for <span class="hlt">recovering</span> hydrocarbon products from a body of fragmented or rubblized oil shale. The process includes initiating a combustion <span class="hlt">zone</span> adjacent the lower end of a body of oil shale and using the thermal energy therefrom for volatilizing the shale oil from the oil shale above the combustion front. Improved recovery of hydrocarbon products is realized by refluxing the heavier fractions in the volatilized shale oil. The heavier fractions are refluxed by condensing the heavier fractions and allowing the resulting condensate to flow downwardly toward the combustion front. Thermal energy from the combustion <span class="hlt">zone</span> cracks themore » condensate producing additional lower molecular weight fractions and a carbonaceous residue. The carbonaceous residue is burned in the combustion front to supply the thermal energy. The temperature of the combustion front is maintained by regulating input of oxygen to the combustion <span class="hlt">zone</span>. The process also includes sweeping the volatilized products from the rubblized oil shale with a noncombustible gas. The flow rate of sweep gas is also controlled to regulate the temperature of the combustion front. The <span class="hlt">recovered</span> products can be enriched with hydrogen by using water vapor as part of the noncombustible sweep gas and cracking the water vapor with the hot carbon in the combustion front to produce hydrogen and an oxide of carbon.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1983ECSS...17..547A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983ECSS...17..547A"><span><span class="hlt">Sediment</span> transport by fishes in Harrington Sound, Bermuda</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alheit, Jürgen</p> <p>1983-11-01</p> <p>Harrington Sound, Bermuda, is a shallow subtropical lagoon with carbonate <span class="hlt">sediments</span>. The most important fishes in this lagoon, in terms of biomass, are grunts (Haemulon aurolineatum, H. flavolineatum, H. sciurus) and a sea-bream (Diplodus bermudensis). These undertake diel feeding migrations from the shallow rocky <span class="hlt">zone</span> towards the deeper sand and mud <span class="hlt">zones</span>. When feeding on zoobenthos they cannot avoid swallowing carbonate <span class="hlt">sediment</span> particles. These <span class="hlt">sediment</span> particles pass through the alimentary canal of the fishes and are deposited again, after digestion of the food, as faeces in the shallow <span class="hlt">zones</span>. Thus, the fishes transport the <span class="hlt">sediment</span> in an unusual direction, from the deep to the shallow <span class="hlt">zones</span>, in effect against the force of gravity. By recording the fish stock densities, digestion rates, and calcium carbonate content of fish stomach and guts, it was possible to estimate the amount of <span class="hlt">sediment</span> transported by the fishes. In Harrington Sound, this amounts annually to 4530 kg calcium carbonate, 40% of which is deposited in the very shallow areas. The pH-values measured in fish stomachs seem to be acidic enough for the dissolution of carbonate <span class="hlt">sediment</span> particles when transported by fishes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS44B..08O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS44B..08O"><span>Contrasts in <span class="hlt">Sediment</span> Delivery and Dispersal from River Mouth to Accumulation <span class="hlt">Zones</span> in High <span class="hlt">Sediment</span> Load Systems: Fly River, Papua New Guinea and Waipaoa River, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogston, A. S.; Walsh, J. P.; Hale, R. P.</p> <p>2011-12-01</p> <p>The relationships between <span class="hlt">sediment</span>-transport processes, short-term sedimentary deposition, subsequent burial, and long-term accumulation are critical to understanding the morphological development of the continental margin. This study focuses on processes involved in formation and evolution of the clinoform in the Gulf of Papua, Papua New Guinea in which much of the riverine <span class="hlt">sediment</span> accumulates, and comparison to those processes active off the Waipaoa River, New Zealand that form mid-shelf deposits and export <span class="hlt">sediment</span> to the slope. In tidally dominated deltas, <span class="hlt">sediment</span> discharged from the river sources must transit through an estuarine region located within the distributary channels, where particle pathways can undergo significant transformations. Within the distributaries of the Fly River tidally dominated delta, near-bed fluid-mud concentrations were observed at the estuarine turbidity maximum and <span class="hlt">sediment</span> delivery to the nearshore was controlled by the morphology and gradient of the distributary. El Niño results in anonymously low flow and <span class="hlt">sediment</span> discharge conditions, which limits transport of <span class="hlt">sediment</span> from the distributaries to the nearshore <span class="hlt">zone</span> of temporary storage. Because the <span class="hlt">sediment</span> stored nearshore feeds the prograding clinoform, this perturbation propagates throughout the dispersal system. In wave-dominated regions, transport mechanisms actively move <span class="hlt">sediment</span> away from the river source, separating the site of deposition and accumulation from the river mouth. River-flood and storm-wave events each create discrete deposits on the Waipaoa River shelf and data has been collected to determine their form, distribution, and relationship to factors such as flood magnitude or wave energy. In this case, transport pathways appear to be influenced by structurally controlled shelf bathymetry. In both cases, the combined fluvial and marine processes can initiate and maintain gravity-driven density flows, and although their triggers and controls differ vastly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25989857','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25989857"><span>Trace element fluxes in <span class="hlt">sediments</span> of an environmentally impacted river from a coastal <span class="hlt">zone</span> of Brazil.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>da Silva, Yuri Jacques Agra Bezerra; Cantalice, José Ramon Barros; Singh, Vijay P; do Nascimento, Clístenes Williams Araújo; Piscoya, Victor Casimiro; Guerra, Sérgio M S</p> <p>2015-10-01</p> <p>Data regarding trace element concentrations and fluxes in suspended <span class="hlt">sediments</span> and bedload are scarce. To fill this gap and meet the international need to include polluted rivers in future world estimation of trace element fluxes, this study aimed to determine the trace element fluxes in suspended <span class="hlt">sediment</span> and bedload of an environmentally impacted river in Brazil. Water, suspended <span class="hlt">sediment</span>, and bedload from both the upstream and the downstream cross sections were collected. To collect both the suspended <span class="hlt">sediment</span> and water samples, we used the US DH-48. Bedload measurements were carried out using the US BLH 84 sampler. Concentrations of Cd, Cr, Cu, Fe, Mn, Ni, Pb, and Zn were determined by inductively coupled plasma (ICP-OES). As and Hg were determined by an atomic absorption spectrophotometer (AA-FIAS). The suspended <span class="hlt">sediments</span> contributed more than 99 % of the trace element flux. By far Pb and to a less extent Zn at the downstream site represents major concerns. The yields of Pb and Zn in suspended <span class="hlt">sediments</span> were 4.20 and 2.93 kg km(2) year(-1), respectively. These yields were higher than the values reported for Pb and Zn for Tuul River (highly impacted by mining activities), 1.60 and 1.30 kg km(2) year(-1), respectively, as well as the Pb yield (suspended + dissolved) to the sea of some Mediterranean rivers equal to 3.4 kg km(2) year(-1). Therefore, the highest flux and yield of Pb and Zn in Ipojuca River highlighted the importance to include medium and small rivers-often overlooked in global and regional studies-in the future estimation of world trace element fluxes in order to protect estuaries and coastal <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/7860','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/7860"><span>The volume of fine <span class="hlt">sediment</span> in pools: An index of <span class="hlt">sediment</span> supply in gravel-bed streams</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Thomas E. Lisle; Sue Hilton</p> <p>1992-01-01</p> <p>Abstract - During waning flood flows in gravel-bed streams, fine-grained bedload <span class="hlt">sediment</span> (sand and fine gravel) is commonly winnowed from <span class="hlt">zones</span> of high shear stress, such as riffles, and deposited in pools, where it mantles an underlying coarse layer. As <span class="hlt">sediment</span> load increases, more fine <span class="hlt">sediment</span> becomes availabe to fill pools. The volume of fine <span class="hlt">sediment</span> in pools...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910135P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910135P"><span>Structural architecture and petrophysical properties of the Rocca di Neto extensional fault <span class="hlt">zone</span> developed in the shallow marine <span class="hlt">sediments</span> of the Crotone Basin (Southern Apennines, Italy).</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pizzati, Mattia; Balsamo, Fabrizio; Iacumin, Paola; Swennen, Rudy; Storti, Fabrizio</p> <p>2017-04-01</p> <p>In this contribution we describe the architecture and petrophysical properties of the Rocca di Neto extensional fault <span class="hlt">zone</span> in loose and poorly lithified <span class="hlt">sediments</span>, located in the Crotone forearc basin (south Italy). To this end, we combined fieldwork with microstructural observations, grain size analysis, and in situ permeability measurements. The studied fault <span class="hlt">zone</span> has an estimated maximum displacement of 80-90 m and separates early Pleistocene age (Gelasian) sands in the footwall from middle Pleistocene (Calabrian) silty clay in the hangingwall. The analysed outcrop consists of about 70 m section through the fault <span class="hlt">zone</span> mostly developed in the footwall block. Fault <span class="hlt">zone</span> consists of four different structural domains characterized by distinctive features: (1) <1 m-thick fault core (where the majority of the displacement is accommodated) in which bedding is transposed into foliation imparted by grain preferential orientation and some black gouges decorate the main slip surfaces; (2) <span class="hlt">zone</span> of tectonic mixing characterized by a set of closely spaced and anastomosed deformation bands parallel to the main slip surface; (3) about 8 m-thick footwall damage <span class="hlt">zone</span> characterized by synthetic and antithetic sets of deformation bands; (4) <span class="hlt">zone</span> of background deformation with a few, widely-spaced conjugate minor faults and deformation bands. The boundary between the relatively undeformed <span class="hlt">sediments</span> and the damage <span class="hlt">zone</span> is not sharp and it is characterized by a progressive decrease in deformation intensity. The silty clay in the hangingwall damage <span class="hlt">zone</span> is characterized by minor faults. Grain size and microstructural data indicate that particulate flow with little amount of cataclasis is the dominant deformation mechanism in both fault core rocks and deformation bands. Permeability of undeformed <span class="hlt">sediments</span> is about 70000 mD, whereas the permeability in deformation bands ranges from 1000 to 18000 mD; within the fault core rocks permeability is reduced up to 3-4 orders of magnitude</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS41A1386C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS41A1386C"><span>Glacially-derived overpressure in the northeastern Alaskan subduction <span class="hlt">zone</span>: combined tomographic and morphometric analysis of shallow <span class="hlt">sediments</span> on the Yakutat shelf and slope, Gulf of Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clary, W. A.; Worthington, L. L.; Scuderi, L. A.; Daigle, H.; Swartz, J. M.</p> <p>2017-12-01</p> <p>The Pamplona <span class="hlt">zone</span> fold and thrust belt is the offshore expression of convergence and shallow subduction of the Yakutat microplate beneath North America in the northeastern Alaska subduction <span class="hlt">zone</span>. The combination of convergent tectonics and glaciomarine sedimentary processes create patterns of deformation and deposition resulting in a shallow sedimentary sequence with varying compaction, fluid pressure, and fault activity. We propose that velocity variations observed in our tomographic analysis represent long-lived fluid overpressure due to loading by ice sheets and <span class="hlt">sediments</span>. Regions with bathymetric and stratigraphic evidence of recent ice sheets and associated <span class="hlt">sedimentation</span> should be collocated with evidence of overpressure (seismic low velocity <span class="hlt">zones</span>) in the shallow <span class="hlt">sediments</span>. Here, we compare a velocity model with shelf seismic stratigraphic facies and modern seafloor morphology. To document glacially derived morphology we use high resolution bathymetry to identify channel and gully networks on the western Yakutat shelf-slope then analyze cross-channel shape indices across the study area. We use channel shape index measurements as a proxy of recent ice-proximal <span class="hlt">sedimentation</span> based on previously published results that proposed a close correlation. Profiles taken at many locations were fitted with a power function and assigned a shape - U-shape channels likely formed proximal to recent ice advances. Detailed velocity models were created by a combination of streamer tomography and pre-stack depth migration velocities with seismic data including: a 2008 R/V Langseth dataset from the St. Elias Erosion and Tectonics Project (STEEP); and a 2004 high-resolution R/V Ewing dataset. Velocity-porosity-permeability relationships developed using IODP Expedition 341 drilling data inform interpretation and physical properties analyses of the shallow <span class="hlt">sediments</span>. Initial results from a 35 km profile extending SE seaward of the Bering glacier and subparallel to the Bering trough</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T44C..05R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T44C..05R"><span>Neogene <span class="hlt">Sediment</span> Transport, Deposition, and Exhumation from the Southern Alaska Syntaxis to the Eastern Aleutian Subduction <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ridgway, K. D.; Witmer, J. W.; Enkelmann, E.; Plafker, G.; Brennan, P. R.</p> <p>2011-12-01</p> <p>Over 5 km of Neogene sedimentary strata are well exposed in the Chugach-St. Elias Ranges within the southern Alaska syntaxis. This syntaxis forms where the Pacific-North America plate boundary changes from the northwest-trending Queen Charlotte-Fairweather transform system to the southwest-trending Alaska-Aleutian subduction <span class="hlt">zone</span>. Active collision and subduction of the buoyant Yakutat microplate in the syntaxis results in a wide collisional <span class="hlt">zone</span> defined by active mountain belts, extensive glaciation, and thick packages of synorogenic strata. New stratigraphic and U-Th/He thermochronologic data from Neogene synorogenic strata, named the Yakataga and Redwood Formations, provide insights on collisional tectonics, glacial erosion, and <span class="hlt">sediment</span> transport, deposition, burial, and exhumation from the onshore Chugach and St. Elias Ranges to the exposed accretionary prism of the Aleutian trench. Stratigraphic analyses show that along the southeastern part of the syntaxis, Neogene strata are characterized by deposition in braid delta, shallow marine, and glaciomarine slope apron depositional systems that resulted in construction of a broad continental shelf. In the central part of the syntaxis, marine shelf and upper slope environments deposited thick-bedded sandstone and mudstone in a thrust belt/foreland basin system. Along the southwestern part of the syntaxis, Neogene strata were deposited in a regional submarine fan system that filled the easternmost part of the Aleutian trench. Geologic mapping of the contact between the Yakataga Formation and underlying strata along the syntaxis document an angular unconformity with maximum stratigraphic separation (> 5 km) in the central part of the syntaxis. Along strike, this unconformity becomes conformable along both the southwestern and southeastern parts of the syntaxis. The regional angular unconformity and facies transitions both point to the importance of the central part of the syntaxis in the generation and distribution of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010GGG....11.AD05H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010GGG....11.AD05H"><span>Velocity-porosity relationships for slope apron and accreted <span class="hlt">sediments</span> in the Nankai Trough Seismogenic <span class="hlt">Zone</span> Experiment, Integrated Ocean Drilling Program Expedition 315 Site C0001</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hashimoto, Y.; Tobin, H. J.; Knuth, M.</p> <p>2010-12-01</p> <p>In this study, we focused on the porosity and compressional wave velocity of marine <span class="hlt">sediments</span> to examine the physical properties of the slope apron and the accreted <span class="hlt">sediments</span>. This approach allows us to identify characteristic variations between <span class="hlt">sediments</span> being deposited onto the active prism and those deposited on the oceanic plate and then carried into the prism during subduction. For this purpose we conducted ultrasonic compressional wave velocity measurements on the obtained core samples with pore pressure control. Site C0001 in the Nankai Trough Seismogenic <span class="hlt">Zone</span> Experiment transect of the Integrated Ocean Drilling Program is located in the hanging wall of the midslope megasplay thrust fault in the Nankai subduction <span class="hlt">zone</span> offshore of the Kii peninsula (SW Japan), penetrating an unconformity at ˜200 m depth between slope apron <span class="hlt">sediments</span> and the underlying accreted <span class="hlt">sediments</span>. We used samples from Site C0001. Compressional wave velocity from laboratory measurements ranges from ˜1.6 to ˜2.0 km/s at hydrostatic pore pressure conditions estimated from sample depth. The compressional wave velocity-porosity relationship for the slope apron <span class="hlt">sediments</span> shows a slope almost parallel to the slope for global empirical relationships. In contrast, the velocity-porosity relationship for the accreted <span class="hlt">sediments</span> shows a slightly steeper slope than that of the slope apron <span class="hlt">sediments</span> at 0.55 of porosity. This higher slope in the velocity-porosity relationship is found to be characteristic of the accreted <span class="hlt">sediments</span>. Textural analysis was also conducted to examine the relationship between microstructural texture and acoustic properties. Images from micro-X-ray CT indicated a homogeneous and well-sorted distribution of small pores both in shallow and in deeper sections. Other mechanisms such as lithology, clay fraction, and abnormal fluid pressure were found to be insufficient to explain the higher velocity for accreted <span class="hlt">sediments</span>. The higher slope in velocity-porosity relationship for</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_6 --> <div id="page_7" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="121"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033980','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033980"><span>Paleomagnetism and environmental magnetism of GLAD800 <span class="hlt">sediment</span> cores from Bear Lake, Utah and Idaho</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Heil, C.W.; King, J.W.; Rosenbaum, J.G.; Reynolds, R.L.; Colman, Steven M.</p> <p>2009-01-01</p> <p>A ???220,000-year record <span class="hlt">recovered</span> in a 120-m-long <span class="hlt">sediment</span> core from Bear Lake, Utah and Idaho, provides an opportunity to reconstruct climate change in the Great Basin and compare it with global climate records. Paleomagnetic data exhibit a geomagnetic feature that possibly occurred during the Laschamp excursion (ca. 40 ka). Although the feature does not exhibit excursional behavior (???40?? departure from the expected value), it might provide an additional age constraint for the sequence. Temporal changes in salinity, which are likely related to changes in freshwater input (mainly through the Bear River) or evaporation, are indicated by variations in mineral magnetic properties. These changes are represented by intervals with preserved detrital Fe-oxide minerals and with varying degrees of diagenetic alteration, including sulfidization. On the basis of these changes, the Bear Lake sequence is divided into seven mineral magnetic <span class="hlt">zones</span>. The differing magnetic mineralogies among these <span class="hlt">zones</span> reflect changes in deposition, preservation, and formation of magnetic phases related to factors such as lake level, river input, and water chemistry. The occurrence of greigite and pyrite in the lake <span class="hlt">sediments</span> corresponds to periods of higher salinity. Pyrite is most abundant in intervals of highest salinity, suggesting that the extent of sulfidization is limited by the availability of SO42-. During MIS 2 (<span class="hlt">zone</span> II), Bear Lake transgressed to capture the Bear River, resulting in deposition of glacially derived hematite-rich detritus from the Uinta Mountains. Millennial-scale variations in the hematite content of Bear Lake <span class="hlt">sediments</span> during the last glacial maximum (<span class="hlt">zone</span> II) resemble Dansgaard-Oeschger (D-O) oscillations and Heinrich events (within dating uncertainties), suggesting that the influence of millennial-scale climate oscillations can extend beyond the North Atlantic and influence climate of the Great Basin. The magnetic mineralogy of <span class="hlt">zones</span> IV-VII (MIS 5, 6, and 7</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6866218-sedimentation-central-segment-aleutian-trench-sources-transport-depositional-style','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6866218-sedimentation-central-segment-aleutian-trench-sources-transport-depositional-style"><span><span class="hlt">Sedimentation</span> in the central segment of the Aleutian Trench: Sources, transport, and depositional style</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Stevenson, A.J.; Scholl, D.W.; Vallier, T.L.</p> <p>1990-05-01</p> <p>The central segment of the Aleutian Trench (162{degree}W to 175{degree}E) is an intraoceanic subduction <span class="hlt">zone</span> that contains an anomalously thick sedimentary fill (4 km maximum). The fill is an arcward-thickening and slightly tilted wedge of <span class="hlt">sediment</span> characterized acoustically by laterally continuous, closely spaced, parallel reflectors. These relations are indicative of turbidite deposition. The trench floor and reflection horizons are planar, showing no evidence of an axial channel or any transverse fan bodies. Cores of surface <span class="hlt">sediment</span> <span class="hlt">recover</span> turbidite layers, implying that <span class="hlt">sediment</span> transport and deposition occur via diffuse, sheetlike, fine-grained turbidite flows that occupy the full width of the trench.more » The mineralogy of Holocene trench <span class="hlt">sediments</span> document a mixture of island-arc (dominant) and continental source terranes. GLORIA side-scan sonar images reveal a westward-flowing axial trench channel that conducts <span class="hlt">sediment</span> to the eastern margin of the central segment, where channelized flow cases. Much of the <span class="hlt">sediment</span> transported in this channel is derived from glaciated drainages surrounding the Gulf of Alaska which empty into the eastern trench segment via deep-sea channel systems (Surveyor and others) and submarine canyons (Hinchinbrook and others). Insular <span class="hlt">sediment</span> transport is more difficult to define. GLORIA images show the efficiency with which the actively growing accretionary wedge impounds <span class="hlt">sediment</span> that manages to cross a broad fore-arc terrace. It is likely that island-arc <span class="hlt">sediment</span> reaches the trench either directly via air fall, via recycling of the accretionary prism, or via overtopping of the accretionary ridges by the upper parts of thick turbidite flows.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613135D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613135D"><span>Frictional behaviour of exhumed subduction <span class="hlt">zone</span> <span class="hlt">sediments</span> from the Shimanto Belt, Japan, at in-situ P-T conditions and implications for megathrust seismogenesis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>den Hartog, Sabine; Niemeijer, Andre; Saffer, Demian; Marone, Chris</p> <p>2014-05-01</p> <p>Seismogenesis on subduction <span class="hlt">zone</span> megathrusts is generally thought to be limited to a region between the ~100-150°C isotherms, at ~5-15 km depth, and the ~350°C isotherm, typically at ~40 km depth. This <span class="hlt">zone</span> is bounded at its up-dip and down-dip limits by aseismic <span class="hlt">zones</span>. However, in recent years it has been discovered that very low frequency earthquakes (VLFE) and non-destructive Slow Slip Events (SSEs) or slow earthquakes nucleate in these presumed aseismic regions. Slip on megathrusts is likely to localize in the weak subducted <span class="hlt">sediments</span> along the plate interface, which implies that the fault material is derived at least in part from these <span class="hlt">sediments</span>. Therefore, understanding the depth distribution of seismicity and SSEs on megathrusts requires knowledge of the frictional behaviour of metapelites. We investigated such behaviour by performing shear experiments on natural megathrust fault gouges, derived from exhumed subduction <span class="hlt">zone</span> <span class="hlt">sediments</span> and faults exposed in the Shimanto Belt on Shikoku Island, Japan. These gouges correspond to peak paleo-temperatures of 105°C to 280°C, representing different stages in the diagenetic and metamorphic evolution of the subducted <span class="hlt">sediments</span>, covering the shallow aseismic <span class="hlt">zone</span> as well as the seismogenic <span class="hlt">zone</span>. The composition of all gouges was dominated by illite/muscovite, with smaller amounts of quartz, feldspar and chlorite. We sheared these gouges at low displacement rates (0.1-100 micron/s) to address the nucleation of megathrust earthquakes and SSEs, using either a double-direct (biaxial) shear machine or a rotary shear machine. The double-direct shear experiments were performed at room temperature, 5% relative humidity and 50 MPa normal stress. The rotary shear experiments, in turn, were conducted at the sample-specific, approximate peak in-situ P-T conditions, i.e. the P-T conditions corresponding to the maximum burial depth of these samples. At room temperature, samples from different peak paleo-temperatures showed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGP14C..08C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGP14C..08C"><span>Paleomagnetism of late Quaternary drift <span class="hlt">sediments</span> off the west Antarctica Peninsula</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Channell, J. E. T.; Xuan, C.; Hillenbrand, C. D.; Larter, R. D.</p> <p>2016-12-01</p> <p>Natural remanant magnetization of a series of piston cores (typically 10 m in lengtth) collected during the JR298 Expedition (January-March 2015) to the west Antarctica Peninsula shows well-defined magnetic components (maximum angular deviations 1°-3°) that potentially record paleomagnetic changes at high southern latitudes. Rock magnetic experiments on the <span class="hlt">sediments</span> conducted at room and high (up to 700°C) temperatures demonstrate the presence of a low- and a high-coercivity component (mean coercivity of 50-60 mT and 130-140 mT respectively). Paleomagnetic directions from the piston cores are primarily carried by the low-coercivity detrital (titano)magnetite, and are affected by authigenic growth of the high-coercivity maghemite. Maghematization in these <span class="hlt">sediments</span> is attributed to the low concentrations of labile organic matter and lack of sulfate reduction in an extended oxic <span class="hlt">zone</span> not penetrated by the piston cores. Despite the varying degree of maghematization, some of the <span class="hlt">recovered</span> cores yield relative paleointensity (RPI) records that can be matched to a reference RPI record constructed mainly from North Atlantic cores. The resulting age models yield mean <span class="hlt">sedimentation</span> rates of 4-12 cm/kyr for the JR298 piston cores. RPI may serve as a stratigraphic tool to date <span class="hlt">sediment</span> cores from the region where traditional isotope stratigraphy is challenging due to the rarity of foraminiferal carbonate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011810','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011810"><span>Holocene <span class="hlt">sedimentation</span> in the shallow nearshore <span class="hlt">zone</span> off Nauset Inlet, Cape Cod, Massachusetts</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Aubrey, D.G.; Twichell, D.C.; Pfirman, S.L.</p> <p>1982-01-01</p> <p>Present conditions and sedimentary evolution of the shallow offshore region near Nauset Inlet on Cape Cod, Massachusetts were clarified using high-resolution seismic-reflection profiles, sidescan-sonar records, surface grab samples and current meter measurements. The study area contains three provinces: (1) a nearshore province (shallower than 18 m) with a relatively steep slope (0.6°) and a cover of medium sand; (2) a northern offshore province covered with coarse sand, gravel, and boulders, interpreted to be glacial drift; and (3) a southern offshore province with a gentle seaward-dipping slope (0.3°) and a surface <span class="hlt">sediment</span> of coarse sand. The glacial drift exposed in the northern offshore province can be traced southward under the coarse sand province. The overlying fill is comprised of either outwash <span class="hlt">sediment</span> derived from the Pleistocene South Channel ice lobe to the east or Holocene-aged marine <span class="hlt">sediments</span> eroded from seacliffs to the north. Latest Holocene <span class="hlt">sediment</span> appears to be limited to the <span class="hlt">zone</span> shoreward of 18 m where the medium sand occurs.Near-bottom mean flows (measured over two winter months in 10 m water depth) average 6 cm sec−1 to the south. Mean flows exceeded 20 cm sec−1approx. 23% of the time. Ninety percent of the flows exceeding 20 cm sec−1were directed to the south, reflecting the dominant atmospheric forcing during these winter months. Waves had an average variance of 650 cm2 with variance exceeding 5000 cm2, 3% of the time, indicating moderate wave activity.Present processes are actively reshaping the nearshore province, which is characterized by many east to northeast-trending shore-oblique channels that do not extend seaward of the 18-m contour. Coarse sand in the floors of these channels suggests they may be erosional features, and the presence of megaripples oriented perpendicular to the channel axes indicates active transport in these channels. Megaripple orientation and the current and wave regime of the study area support a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP13B1616O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP13B1616O"><span>Deciphering Equatorial Pacific Deep Sea <span class="hlt">Sediment</span> Transport Regimes by Core-Log-Seismic Integration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ortiz, E.; Tominaga, M.; Marcantonio, F.</p> <p>2017-12-01</p> <p>Investigating deep-sea <span class="hlt">sediment</span> transportation and deposition regimes is a key to accurately understand implications from geological information recorded by pelagic <span class="hlt">sediments</span>, e.g. climate signals. However, except for physical oceanographic particle trap experiments, geochemical analyses of in situsediments, and theoretical modeling of the relation between the bottom currents and <span class="hlt">sediment</span> particle flux, it has remained a challenging task to document the movement of deep sea <span class="hlt">sediments</span>, that takes place over time. We utilized high-resolution, multichannel reflection seismic data from the eastern equatorial Pacific region with drilling and logging results from two Integrated Ocean Drilling Program (IODP) sites, the Pacific Equatorial Age Transect (PEAT) 7 (Site U1337) and 8 (Site U1338), to characterize <span class="hlt">sediment</span> transportation regimes on 18-24 Ma oceanic crust. Site U1337, constructed by a series of distinct abyssal hills and abyssal basins; Site U1338, located 570 km SE from Site U1337 site and constructed by a series of ridges, seamounts, and abyssal hills. These sites are of particular interest due to their proximity to the equatorial productivity <span class="hlt">zone</span>, areas with high <span class="hlt">sedimentation</span> rates and preservation of carbonate-bearing <span class="hlt">sediment</span> that provide invaluable insights on equatorial Pacific ecosystems and carbon cycle. We integrate downhole geophysical logging data as well as geochemistry and physical properties measurements on <span class="hlt">recovered</span> cores from IODP Sites U1337 and U1338 to comprehensively examine the mobility of deep-sea <span class="hlt">sediments</span> and <span class="hlt">sediment</span> diagenesis over times in a quasi-3D manner. We also examine 1100 km of high resolution underway seismic surveys from site survey lines in between PEAT 7 and 8 in order to investigate changes in <span class="hlt">sediment</span> transportation between both sites. Integrating detailed seismic interpretations, high resolution core data, and 230Th flux measurements we aim to create a detailed chronological <span class="hlt">sedimentation</span> and <span class="hlt">sediment</span> diagenesis history</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26PSL.447...95K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26PSL.447...95K"><span>Molybdenum isotope systematics in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>König, Stephan; Wille, Martin; Voegelin, Andrea; Schoenberg, Ronny</p> <p>2016-08-01</p> <p>This study presents Mo isotope data for arc lavas from different subduction <span class="hlt">zones</span> that range between δ 98 / 95 Mo = - 0.72 and + 0.07 ‰. Heaviest isotope values are observed for the most slab fluid dominated samples. Isotopically lighter signatures are related to increasing relevance of terrigenous <span class="hlt">sediment</span> subduction and <span class="hlt">sediment</span> melt components. Our observation complements previous conclusions that an isotopically heavy Mo fluid flux likely mirrors selective incorporation of isotopically light Mo in secondary minerals within the subducting slab. Analogue to this interpretation, low δ 98 / 95 Mo flux that coincides with terrigenous <span class="hlt">sediment</span> subduction and <span class="hlt">sediment</span> melting cannot be simply related to a recycled input signature. Instead, breakdown of the controlling secondary minerals during <span class="hlt">sediment</span> melting may release the light component and lead to decreasing δ 98 / 95 Mo influx into subarc mantle sources. The natural range between slab dehydration and hydrous <span class="hlt">sediment</span> melting may thus cause a large spread of δ 98 / 95 Mo in global subduction <span class="hlt">zone</span> magmas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS21A1348F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS21A1348F"><span>Enhanced Sulfate Reduction and Carbon Sequestration in <span class="hlt">Sediments</span> Underlying the Core of the Arabian Sea Oxygen Minimum <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernandes, S. Q.; Mazumdar, A.; Peketi, A.; Bhattacharya, S.; Carvalho, M.; Da Silva, R.; Roy, R.; Mapder, T.; Roy, C.; Banik, S. K.; Ghosh, W.</p> <p>2017-12-01</p> <p>The oxygen minimum <span class="hlt">zone</span> (OMZ) of the Arabian Sea in the northern Indian Ocean is one of the three major global sites of open ocean denitrification. The functionally anoxic water column between 150 to 1200 mbsl plays host to unique biogeochemical processes and organism interactions. Little is known, however, about the consequence of the low dissolved oxygen on the underlying sedimentary biogeochemical processes. Here we present, for the first time, a comprehensive investigation of <span class="hlt">sediment</span> biogeochemistry of the Arabian Sea OMZ by coupling pore fluid analyses with microbial diversity data in eight <span class="hlt">sediment</span> cores collected across a transect off the west coast of India in the Eastern Arabian Sea. We observed that in <span class="hlt">sediments</span> underlying the core of the OMZ, high organic carbon sequestration coincides with a high diversity of all bacteria (the majority of which are complex organic matter hydrolyzers) and sulfate reducing bacteria (simple organic compound utilizers). Depth-integrated sulfate reduction rate also intensifies in this territory. These biogeochemical features, together with the detected shallowing of the sulfate-methane interface and buildup of pore-water sulfide, are all reflective of heightened carbon-sulfur cycling in the <span class="hlt">sediments</span> underlying the OMZ core. Our data suggests that the <span class="hlt">sediment</span> biogeochemistry of the OMZ is sensitive to minute changes in bottom water dissolved oxygen, and is dictated by the potential abundance and bioavailability of complex to simple carbon compounds which can stimulate a cascade of geomicrobial activities pertaining to the carbon-sulfur cycle. Our findings hold implications in benthic ecology and <span class="hlt">sediment</span> diagenesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70187315','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70187315"><span>Site 765: <span class="hlt">Sediment</span> Lithostratigraphy</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>,</p> <p>1990-01-01</p> <p>A 935-m-thick succession of Quaternary through Lower Cretaceous <span class="hlt">sediments</span> was <span class="hlt">recovered</span> at Site 765 (Fig. 10). A single core of Quaternary <span class="hlt">sediment</span> was obtained from Hole 765A; drilling terminated and a new hole was drilled in an attempt to establish the mud line. Quaternary through middle Miocene <span class="hlt">sediments</span> were cored in Hole 765B down to a depth of 395.6 mbsf. Middle Miocene through Lower Cretaceous <span class="hlt">sediments</span> were cored in Hole 765C, after washing the interval between 0 and 350.2 mbsf. Exact lithologic correlation of the basal cores from Hole 765B with the upper cores from Hole 765C is not possible because of poor recovery; hence, correlation is based solely on matching sub-bottom depths.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFM.T31D..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFM.T31D..02B"><span>Constraints on Subduction <span class="hlt">Zone</span> Temperatures and Chemical Fluxes from Accessory Phase Saturation in Subducted <span class="hlt">Sediments</span> (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Blundy, J.; Skora, S.</p> <p>2009-12-01</p> <p>. For the case of 7 wt% added H2O, monazite is exhausted at 825 °C; it disappears at 780 °C with 15 wt% added H2O. In our experiments monazite fractionates LREE from Th, such that fluids preserving the original sedimentary ratio must be generated at or above monazite-out temperatures in subducted slabs where red clay is the dominant sedimentary lithology. We propose that the subducted sedimentary signature is imparted by fluxing of H2O derived from hydrated (e.g. serpentinised) portions of the deeper subducting slab, triggering copious “flash melting” of the <span class="hlt">sediment</span> at the point were its temperature exceeds ~800 °C. Without the addition of H2O <span class="hlt">sediment</span> melting is too restricted to allow any appreciable fluid release into the overlying mantle. Moreover, under such conditions the Th/LREE ratio is strongly fractionated due to the abundance of residual monazite. The availability of H2O in hydrated portions of subducted slabs, e.g. in the vicinity of fracture <span class="hlt">zones</span>, may exercise an important control on the spatial distribution of subduction <span class="hlt">zone</span> magmatism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4707442','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4707442"><span>Methane Emission in a Specific Riparian-<span class="hlt">Zone</span> <span class="hlt">Sediment</span> Decreased with Bioelectrochemical Manipulation and Corresponded to the Microbial Community Dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Friedman, Elliot S.; McPhillips, Lauren E.; Werner, Jeffrey J.; Poole, Angela C.; Ley, Ruth E.; Walter, M. Todd; Angenent, Largus T.</p> <p>2016-01-01</p> <p>Dissimilatory metal-reducing bacteria are widespread in terrestrial ecosystems, especially in anaerobic soils and <span class="hlt">sediments</span>. Thermodynamically, dissimilatory metal reduction is more favorable than sulfate reduction and methanogenesis but less favorable than denitrification and aerobic respiration. It is critical to understand the complex relationships, including the absence or presence of terminal electron acceptors, that govern microbial competition and coexistence in anaerobic soils and <span class="hlt">sediments</span>, because subsurface microbial processes can effect greenhouse gas emissions from soils, possibly resulting in impacts at the global scale. Here, we elucidated the effect of an inexhaustible, ferrous-iron and humic-substance mimicking terminal electron acceptor by deploying potentiostatically poised electrodes in the <span class="hlt">sediment</span> of a very specific stream riparian <span class="hlt">zone</span> in Upstate New York state. At two sites within the same stream riparian <span class="hlt">zone</span> during the course of 6 weeks in the spring of 2013, we measured CH4 and N2/N2O emissions from soil chambers containing either poised or unpoised electrodes, and we harvested biofilms from the electrodes to quantify microbial community dynamics. At the upstream site, which had a lower vegetation cover and highest soil temperatures, the poised electrodes inhibited CH4 emissions by ∼45% (when normalized to remove temporal effects). CH4 emissions were not significantly impacted at the downstream site. N2/N2O emissions were generally low at both sites and were not impacted by poised electrodes. We did not find a direct link between bioelectrochemical treatment and microbial community membership; however, we did find a correspondence between environment/function and microbial community dynamics. PMID:26793170</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15..137M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15..137M"><span>Microbial methanogenesis in the sulfate-reducing <span class="hlt">zone</span> of <span class="hlt">sediments</span> in the Eckernförde Bay, SW Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maltby, Johanna; Steinle, Lea; Löscher, Carolin R.; Bange, Hermann W.; Fischer, Martin A.; Schmidt, Mark; Treude, Tina</p> <p>2018-01-01</p> <p>Benthic microbial methanogenesis is a known source of methane in marine systems. In most <span class="hlt">sediments</span>, the majority of methanogenesis is located below the sulfate-reducing <span class="hlt">zone</span>, as sulfate reducers outcompete methanogens for the major substrates hydrogen and acetate. The coexistence of methanogenesis and sulfate reduction has been shown before and is possible through the usage of noncompetitive substrates by methanogens such as methanol or methylated amines. However, knowledge about the magnitude, seasonality, and environmental controls of this noncompetitive methane production is sparse. In the present study, the presence of methanogenesis within the sulfate reduction <span class="hlt">zone</span> (SRZ methanogenesis) was investigated in <span class="hlt">sediments</span> (0-30 cm below seafloor, cm b.s.f.) of the seasonally hypoxic Eckernförde Bay in the southwestern Baltic Sea. Water column parameters such as oxygen, temperature, and salinity together with porewater geochemistry and benthic methanogenesis rates were determined in the sampling area <q>Boknis Eck</q> quarterly from March 2013 to September 2014 to investigate the effect of seasonal environmental changes on the rate and distribution of SRZ methanogenesis, to estimate its potential contribution to benthic methane emissions, and to identify the potential methanogenic groups responsible for SRZ methanogenesis. The metabolic pathway of methanogenesis in the presence or absence of sulfate reducers, which after the addition of a noncompetitive substrate was studied in four experimental setups: (1) unaltered <span class="hlt">sediment</span> batch incubations (net methanogenesis), (2) 14C-bicarbonate labeling experiments (hydrogenotrophic methanogenesis), (3) manipulated experiments with the addition of either molybdate (sulfate reducer inhibitor), 2-bromoethanesulfonate (methanogen inhibitor), or methanol (noncompetitive substrate, potential methanogenesis), and (4) the addition of 13C-labeled methanol (potential methylotrophic methanogenesis). After incubation with methanol</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021584','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021584"><span>Formation of natural gas hydrates in marine <span class="hlt">sediments</span> 1. Conceptual model of gas hydrate growth conditioned by host <span class="hlt">sediment</span> properties</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Clennell, M.B.; Hovland, M.; Booth, J.S.; Henry, P.; Winters, W.J.</p> <p>1999-01-01</p> <p>The stability of submarine gas hydrates is largely dictated by pressure and temperature, gas composition, and pore water salinity. However, the physical properties and surface chemistry of deep marine <span class="hlt">sediments</span> may also affect the thermodynamic state, growth kinetics, spatial distributions, and growth forms of clathrates. Our conceptual model presumes that gas hydrate behaves in a way analogous to ice in a freezing soil. Hydrate growth is inhibited within fine-grained <span class="hlt">sediments</span> by a combination of reduced pore water activity in the vicinity of hydrophilic mineral surfaces, and the excess internal energy of small crystals confined in pores. The excess energy can be thought of as a "capillary pressure" in the hydrate crystal, related to the pore size distribution and the state of stress in the <span class="hlt">sediment</span> framework. The base of gas hydrate stability in a sequence of fine <span class="hlt">sediments</span> is predicted by our model to occur at a lower temperature (nearer to the seabed) than would be calculated from bulk thermodynamic equilibrium. Capillary effects or a build up of salt in the system can expand the phase boundary between hydrate and free gas into a divariant field extending over a finite depth range dictated by total methane content and pore-size distribution. Hysteresis between the temperatures of crystallization and dissociation of the clathrate is also predicted. Growth forms commonly observed in hydrate samples <span class="hlt">recovered</span> from marine <span class="hlt">sediments</span> (nodules, and lenses in muds; cements in sands) can largely be explained by capillary effects, but kinetics of nucleation and growth are also important. The formation of concentrated gas hydrates in a partially closed system with respect to material transport, or where gas can flush through the system, may lead to water depletion in the host <span class="hlt">sediment</span>. This "freeze-drying" may be detectable through physical changes to the <span class="hlt">sediment</span> (low water content and overconsolidation) and/or chemical anomalies in the pore waters and metastable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Ocgy...52..780S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Ocgy...52..780S"><span>Distribution of metal concentrations in <span class="hlt">sediments</span> of the coastal <span class="hlt">zone</span> of the Gulf of Riga and open part of the Baltic Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seisuma, Z.; Kulikova, I.</p> <p>2012-11-01</p> <p>The comparison of spatial and temporal distribution of Hg, Cd, Pb, Cu, Ni, Zn, Mn and Fe concentrations in <span class="hlt">sediments</span> from the Gulf of Riga and open Baltic Sea along the coastal <span class="hlt">zone</span> is presented for the first time. There were considerable differences in Pb, Zn, Mn and Fe levels in <span class="hlt">sediment</span> at various stations of the Gulf of Riga. A significant difference of Cd, Pb, Cu, Ni, Zn levels was found in <span class="hlt">sediments</span> of various stations in the open Baltic coast. The amount of Cd, Pb, Cu, Ni, Zn and Fe levels also differed significantly in the <span class="hlt">sediments</span> of the Gulf of Riga in different years. A considerable yearly difference in amount of Hg, Cd, Pb, Cu, Ni and Mn levels was found in <span class="hlt">sediments</span> in the open Baltic coast. The essential highest values of Pb and Zn in coastal <span class="hlt">sediments</span> of the open Baltic Sea are stated in comparison with the Gulf of Riga. The concentrations of other metals have only a tendency to be higher in coastal <span class="hlt">sediments</span> of the open Baltic Sea in comparison with the Gulf of Riga. Natural and anthropogenic factors were proved to play an important role in determining resultant metals concentrations in the regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFM.T52A..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFM.T52A..07G"><span>Interplay of Structure and <span class="hlt">Sediment</span> Supply May Influence Subduction <span class="hlt">Zone</span> Rupture Patches and Propagation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goldfinger, C.; Wang, K.; Witter, R.; Baptista, A.; Zhang, Y.; Priest, G.; Nelson, H.; Morey, A.; Johnson, J.</p> <p>2007-12-01</p> <p>The question of whether there are universal controls on the genesis and maintenance of large slip and moment patches along strike on subduction megathrusts has proved remarkably elusive, in part due to the short temporal records we have of these great events around the globe. Many events this century are poorly constrained, and many subduction <span class="hlt">zones</span> only have one or a few events available for comparison. Long historical records and good structural constraints have made Nankai a leading case for basin centered asperities, yet the recent Sumatra Mw 9.2 rupture models show that slip and moment for the most part avoided basins and was centered under structural highs. In Cascadia, both deformation and tsunami models clearly fit the respective subsidence and runup data better if slip in past events was centered under or did not avoid these highs as opposed to basin centered model. Onshore and offshore paleoseismic evidence from 38 Cascadia earthquakes strongly suggest that structural segmentation plays a role only along the southernmost margin. These data do not provide information on moment or slip distribution, but do effectively constrain rupture lengths. Rupture lengths constrained by the paleoseismic data show that there is no Holocene segmentation for the northern margin, and that southern segments may be controlled by some of the obvious structural boundaries such as the Blanco Fracture <span class="hlt">zone</span>, and outer arc uplifts and forearc basins. Where resolution is adequate, these data also suggest that ruptures die out into the basins and are linked multi-segment ruptures of structural uplifts, similar to that observed in the 2004 and 2005 earthquakes from Sumatra where outer arc uplifts may mark segment boundaries, high slip patches and initiation points for great earthquakes. The difference between the rupture modes observed for Nankai and Sumatra, and suggested here for Cascadia may be linked to the <span class="hlt">sediment</span> supply for these systems. Cascadia and Sumatra are both systems</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..404N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..404N"><span>Anthropopression markers in lake bottom <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nadolna, Anna; Nowicka, Barbara</p> <p>2014-05-01</p> <p>Lakes are vulnerable to various types of anthropogenic disturbances. Responses of lake ecosystems to environmental stressors are varied and depend not only on the type of a factor but also on the lake natural resistance to degradation. Within the EULAKES project an evaluation of anthropogenic stress extent in a flow-through, postglacial, ribbon lake (Lake Charzykowskie) was carried out. It was assumed, that this impact manifests unevenly, depending on a type and degree of the pressure on the shore <span class="hlt">zones</span>, water quality of tributaries, lake basin shape and dynamics of a water movement. It was stated, that anthropogenic markers are substances accumulated in bottom <span class="hlt">sediments</span> as a result of allochthonous substances inflow from the catchment and atmosphere. Along the selected transects 105 samples from the top layer of <span class="hlt">sediments</span> (about 20 cm) was collected representing the contemporary accumulation (about 15 years). The content of selected chemical elements and compounds was examined, including nutrients (TN and TP), heavy metals (arsenic, cadmium, lead, chromium, nickel, copper, zinc, mercury, iron, and manganese) and pesticides (DDT, DDD, DDE, DMDT , γ-HCH). The research was conducted in the deepest points of each lake basin and along the research transects - while choosing the spots, the increased intensity of anthropogenic impact (ports, roads with heavy traffic, wastewater discharge <span class="hlt">zones</span>, built-up areas) was taken into consideration. The river outlets to the lake, where there are ecotonal <span class="hlt">zones</span> between limnic and fluvial environment, were also taken into account. Analysis of the markers distribution was carried out against the diversity of chemical characteristics of limnic <span class="hlt">sediments</span>. Ribbon shape of the lake basin and the dominant wind direction provide an opportunity of easy water mixing to a considerable depth. Intensive waving processes cause removal of the matter from the littoral <span class="hlt">zone</span> towards lake hollows (separated by the underwater tresholds), where the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.3910V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.3910V"><span>Extracting a Detailed Magnetostratigraphy From Weakly Magnetized, Oligocene to Early Miocene <span class="hlt">Sediment</span> Drifts <span class="hlt">Recovered</span> at IODP Site U1406 (Newfoundland Margin, Northwest Atlantic Ocean)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Peer, Tim E.; Xuan, Chuang; Lippert, Peter C.; Liebrand, Diederik; Agnini, Claudia; Wilson, Paul A.</p> <p>2017-11-01</p> <p>Fine-grained magnetic particles in deep-sea <span class="hlt">sediments</span> often statistically align with the ambient magnetic field during (and shortly after) deposition and can therefore record geomagnetic reversals. Correlation of these reversals to a geomagnetic polarity time scale is an important geochronological tool that facilitates precise stratigraphic correlation and dating of geological records globally. <span class="hlt">Sediments</span> often carry a remanence strong enough for confident identification of polarity reversals, but in some cases a low signal-to-noise ratio prevents the construction of a reliable and robust magnetostratigraphy. Here we implement a data-filtering protocol, which can be integrated with the UPmag software package, to automatically reduce the maximum angular deviation and statistically mask noisy data and outliers deemed unsuitable for magnetostratigraphic interpretation. This protocol thus extracts a clearer signal from weakly magnetized <span class="hlt">sediments</span> <span class="hlt">recovered</span> at Integrated Ocean Drilling Program (IODP) Expedition 342 Site U1406 (Newfoundland margin, northwest Atlantic Ocean). The resulting magnetostratigraphy, in combination with shipboard and shore-based biostratigraphy, provides an age model for the study interval from IODP Site U1406 between Chrons C6Ar and C9n (˜21-27 Ma). We identify rarely observed geomagnetic directional changes within Chrons C6Br, C7r, and C7Ar, and perhaps within Subchron C8n.1n. Our magnetostratigraphy dates three intervals of unusual stratigraphic behavior within the <span class="hlt">sediment</span> drifts at IODP Site U1406 on the Newfoundland margin. These lithostratigraphic changes are broadly concurrent with the coldest climatic phases of the middle Oligocene to early Miocene and we hypothesize that they reflect changes in bottom water circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JAfES..70...36J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JAfES..70...36J"><span>Lithostratigraphy, biostratigraphy and chemostratigraphy of Upper Cretaceous and Paleogene <span class="hlt">sediments</span> from southern Tanzania: Tanzania Drilling Project Sites 27-35</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jimènez Berrocoso, Àlvaro; Huber, Brian T.; MacLeod, Kenneth G.; Petrizzo, Maria Rose; Lees, Jacqueline A.; Wendler, Ines; Coxall, Helen; Mweneinda, Amina K.; Falzoni, Francesca; Birch, Heather; Singano, Joyce M.; Haynes, Shannon; Cotton, Laura; Wendler, Jens; Bown, Paul R.; Robinson, Stuart A.; Gould, Jeremy</p> <p>2012-07-01</p> <p>The 2008 Tanzania Drilling Project (TDP) expedition <span class="hlt">recovered</span> common planktonic foraminifera (PF), calcareous nannofossils (CN) and calcareous dinoflagellates with extraordinary shell preservation at multiple Cenomanian-Campanian sites that will be used for paleoclimatic, paleoceanographic, and biostratigraphic studies. New cores confirm the existence of a more expanded and continuous Upper Cretaceous sequence than had previously been documented in the Lindi and Kilwa regions of southeastern coastal Tanzania. This TDP expedition cored 684.02 m at eight Upper Cretaceous sites (TDP Sites 28-35) and a thin Paleocene section (TDP Site 27). TDP Sites 29, 30, 31 and 34 together span the lowermost Turonian to Coniacian (PF Whiteinella archaeocretacea to Dicarinella concavata <span class="hlt">Zones</span> and CN <span class="hlt">Zones</span> UC6a-9b), with TDP Site 31 being the most biostratigraphically complete Turonian section found during TDP drilling. A discontinuous section from the Santonian-upper Campanian (PF D. asymetrica to Radotruncana calcarata <span class="hlt">Zones</span> and CN <span class="hlt">Zones</span> UC12-16) was collectively <span class="hlt">recovered</span> at TDP Sites 28, 32 and 35, while thin sequences of the lower Cenomanian (PF Thalmanninella globotruncanoides <span class="hlt">Zone</span> and CN subzones UC3a-b) and middle Paleocene (Selandian; PF <span class="hlt">Zone</span> P3a and CN <span class="hlt">Zone</span> NP5) were cored in TDP Sites 33 and 27, respectively. Records of δ13Corg and δ13Ccarb from bulk <span class="hlt">sediments</span> generated for all the Cretaceous sites show largely stable values through the sections. Only a few parallel δ13Corg and δ13Ccarb shifts have been found and they are interpreted to reflect local processes. The δ18Ocarb record, however, is consistent with Late Cretaceous cooling trends from the Turonian into the Campanian. Lithologies of these sites include thick intervals of claystones and siltstones with locally abundant, finely-laminated fabrics, irregular occurrences of thin sandstone layers, and sporadic bioclastic debris (e.g., inoceramids, ammonites). Minor lithologies represent much thinner units of up to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1811923Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1811923Z"><span>Deep aquifer as driver for mineral authigenesis in Gulf of Alaska <span class="hlt">sediments</span> (IODP Expedition 341, Site U1417)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zindorf, Mark; März, Christian; Wagner, Thomas; Strauss, Harald; Gulick, Sean P. S.; Jaeger, John M.; LeVay, Leah J.</p> <p>2016-04-01</p> <p>Bacterial sulphate reduction plays a key role in authigenic mineral formation in marine <span class="hlt">sediments</span>. Usually, decomposition of organic matter follows a sequence of microbial metabolic pathways, where microbial sulphate reduction leads to sulphate depletion deeper in the <span class="hlt">sediment</span>. When sulphate is consumed completely from the pore waters, methanogenesis commences. The contact of sulphate- and methane-containing pore waters is a well-defined biogeochemical boundary (the sulphate-methane transition <span class="hlt">zone</span>, SMTZ). Here authigenic pyrite, barite and carbonates form. Pyrite formation is directly driven by bacterial sulphate reduction since pyrite precipitates from produced hydrogen sulphide. Barite and carbonate formation are secondary effects resulting from changes of the chemical milieu due to microbial activity. However, this mineral authigenesis is ultimately linked to abiotic processes that determine the living conditions for microorganisms. At IODP Site U1417 in the Gulf of Alaska, a remarkable diagenetic pattern has been observed: Between sulphate depletion and methane enrichment, a ~250 m wide gap exists. Consequently, no SMTZ can be found under present conditions, but enrichments of pyrite indicate that such <span class="hlt">zones</span> have existed in the past. Solid layers consisting of authigenic carbonate-cemented sand were partly <span class="hlt">recovered</span> right above the methane production <span class="hlt">zone</span>, likely preventing continued upward methane diffusion. At the bottom of the <span class="hlt">sediment</span> succession, the lower boundary of the methanogenic <span class="hlt">zone</span> is constrained by sulphate-rich pore waters that appear to originate from a deeper source. Here, a well-established SMTZ exists, but in reversed order (sulphate diffusing up, methane diffusing down). Sulphur isotopes of pyrite reveal that sulphate reduction here does not occur under closed system conditions. This indicates that a deep aquifer is actively recharging the deep sulphate pool. Similar deep SMTZs have been found at other sites, yet mostly in geologically</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24988362','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24988362"><span>Occurrence of halogenated flame retardants in <span class="hlt">sediment</span> off an urbanized coastal <span class="hlt">zone</span>: association with urbanization and industrialization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Hui-Hui; Hu, Yuan-Jie; Luo, Pei; Bao, Lian-Jun; Qiu, Jian-Wen; Leung, Kenneth M Y; Zeng, Eddy Y</p> <p>2014-01-01</p> <p>To examine the impacts of urbanization and industrialization on the coastal environment, <span class="hlt">sediment</span> samples were collected from an urbanized coastal <span class="hlt">zone</span> (i.e., Daya Bay and Hong Kong waters of South China) and analyzed for 20 polybrominated diphenyl ethers (PBDEs) and 10 alternative halogenated flame retardants (AHFRs). The sum concentration of PBDEs was in the range of 1.7-55 (mean: 17) ng g(-1), suggesting a moderate pollution level compared to the global range. The higher fractions of AHFRs (i.e., TBB+TBPH, BTBPE and DBDPE) than those of legacy PBDEs (i.e., penta-BDE, octa-BDE and deca-BDE) corresponded with the phasing out of PBDEs and increasing demand for AHFRs. Heavy contamination occurred at the estuary of Dan'ao River flowing through the Daya Bay Economic <span class="hlt">Zone</span>, home to a variety of petrochemicals and electronics manufacturing facilities. The concentrations of HFRs in surface <span class="hlt">sediments</span> of Hong Kong were the highest in Victoria Harbor, which receives around 1.4 million tons of primarily treated sewage daily, and a good relationship (r(2) = 0.80; p < 0.0001) between the HFR concentration and population density in each council district was observed, highlighting the effect of urbanization. Moreover, the AHFR concentrations were significantly correlated (r(2) > 0.73; p < 0.05) with the production volume of electronic devices, production value of electronic industries and population size, demonstrating the importance of industrializing and urbanizing processes in dictating the historical input patterns of AHFRs.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li class="active"><span>7</span></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_7 --> <div id="page_8" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="141"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP33A1915E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP33A1915E"><span>Sedimentology of cores <span class="hlt">recovered</span> from the Canada Basin of the Arctic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edwards, B. D.; Saint-Ange, F.; Pohlman, J.; Higgins, J.; Mosher, D. C.; Lorenson, T. D.; Hart, P.</p> <p>2011-12-01</p> <p>Researchers from the United States and Canada are collaborating to understand the tectonic and sedimentary history of the Arctic Ocean between Canada and Alaska. As part of this on-going study, a joint US-Canadian ice breaker expedition operated in parts of the Canada Basin during August 2010. Occasional interruptions of the seismic data acquisition provided the ship time to collect gravity and piston cores at five sites-of-opportunity throughout the basin. High-resolution multibeam bathymetry and chirp sub-bottom profiler data collected immediately prior to coring reveal the fine-scale morphology of each site. Core photographs, X-ray radiographs, and physical property data support the following descriptions. Two piston cores were collected from the Beaufort Sea continental margin in a region of known bottom simulating reflectors (BSRs). Site 1 (2538 m water depth): This core <span class="hlt">recovered</span> 5.72 m of gas-charged, gray sticky clay and silty-clay from an approximately 1100 m diameter, 130 m high conical mound overlying the crest of a buried anticline. Gas hydrate <span class="hlt">recovered</span> in the core catcher combined with cracks and voids, methane and other hydrocarbon gasses, pyrite concretions, chemosynthetic clams, carbonate nodules, and soft carbonate masses indicate the likely upward migration of deep-seated fluids. Site 2 (1157 m water depth): This core, positioned 40 km upslope from the gas hydrate core, <span class="hlt">recovered</span> 3 m of gray sticky silty clay and clayey silt near the base of an erosional scarp. Some voids and fracturing are apparent but carbonate masses and pyrite concretions are absent. Site 3 (3070 m water depth): This core from the top of a seamount discovered in 2009 in the north-central part of the Canada Basin <span class="hlt">recovered</span> 4.94 m of <span class="hlt">sediment</span>. More than 3 m of dark brown to yellowish brown, massive interbedded silty clays with sands and matrix-supported gravels (ice rafted debris [IRD]) occur in abrupt contact with underlying reddish yellow to brownish yellow silty clay and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSEC24B1098A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC24B1098A"><span>Surf <span class="hlt">Zone</span> <span class="hlt">Sediment</span> Size Variation, Morphodynamics, and Hydrodynamics During Sea/Land Breeze and El-Norte Storm in Sisal, Yucatan, Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alrushaid, T.; Figlus, J.; Torres-Freyermuth, A.; Puleo, J. A.; Dellapenna, T. M.</p> <p>2016-02-01</p> <p>Coastlines around the world are under ever-increasing pressure due to population trends, commerce, and geophysical processes like tropical storms and erosion. This multi-institutional field campaign was conducted to improve our understanding of complex nearshore processes under varying forcing conditions on a microtidal, sandy beach located in Sisal, Yucatan from 3/27 to 4/12/2014. Hydrodynamics, morphodynamics, and textural variability were investigated during: (1) a cold front event (referred to as El-Norte); (2) land breeze (LB); and (3) sea breeze (SB). The instrumentation layout included three surf/swash <span class="hlt">zone</span> cross-shore transects where water elevation, suspended <span class="hlt">sediment</span> concentration, bed load, and current velocities were measured, as well as several offshore ADCP for hydrodynamic measurements. TKE, τb, ɛ and were estimated using the data obtained from surf <span class="hlt">zone</span> ADV. In addition, Hs and Tsin the surf <span class="hlt">zone</span> were computed using measurements from ADV pressure sensors, while a separate pressure transducer was used to obtain water free-surface elevation within the swash <span class="hlt">zone</span>. During SB cycles the study area experienced wind velocities reaching up to 12ms-1, and 15ms-1 during El-Norte. Elevated wind stress during El-Norte resulted in Hs of 1.5m and 0.6m in water depths of 10m and 0.4m, respectively. Surface <span class="hlt">sediment</span> grab samples during SB/LB cycles showed that the swash <span class="hlt">zone</span> had a moderately well sorted distribution with a mean grain size of 0.5mm, while poor sorting and a mean grain size of 0.7mm were found during El-Norte. Additionally, measured bathymetry data showed evidence for offshore sandbar migration during strong offshore currents (0.4ms-1) during El-Norte, while onshore sandbar migration was evident during SB/LB periods (0.3ms-1 and 0.1ms-1, respectively). This study highlights how different weather forcing conditions affect hydrodynamics, morphodynamics, and textural variability on a sandy beach. Aside from furthering our knowledge on these complex</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRB..122.2457D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRB..122.2457D"><span>Rapid <span class="hlt">sedimentation</span> and overpressure in shallow <span class="hlt">sediments</span> of the Bering Trough, offshore southern Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daigle, Hugh; Worthington, Lindsay L.; Gulick, Sean P. S.; Van Avendonk, Harm J. A.</p> <p>2017-04-01</p> <p>Pore pressures in <span class="hlt">sediments</span> at convergent margins play an important role in driving chemical fluxes and controlling deformation styles and localization. In the Bering Trough offshore Southern Alaska, extreme <span class="hlt">sedimentation</span> rates over the last 140 kyr as a result of glacial advance/retreats on the continental shelf have resulted in elevated pore fluid pressures in slope <span class="hlt">sediments</span> overlying the Pamplona <span class="hlt">Zone</span> fold and thrust belt, the accretionary wedge resulting from subduction of the Yakutat microplate beneath the North American Plate. Based on laboratory experiments and downhole logs acquired at Integrated Ocean Drilling Program Site U1421, we predict that the overpressure in the slope <span class="hlt">sediments</span> may be as high as 92% of the lithostatic stress. Results of one-dimensional numerical modeling accounting for changes in <span class="hlt">sedimentation</span> rate over the last 130 kyr predicted overpressures that are consistent with our estimates, suggesting that the overpressure is a direct result of the rapid <span class="hlt">sedimentation</span> experienced on the Bering shelf and slope. Comparisons with other convergent margins indicate that such rapid <span class="hlt">sedimentation</span> and high overpressure are anomalous in <span class="hlt">sediments</span> overlying accretionary wedges. We hypothesize that the shallow overpressure on the Bering shelf/slope has fundamentally altered the deformation style within the Pamplona <span class="hlt">Zone</span> by suppressing development of faults and may inhibit seismicity by focusing faulting elsewhere or causing deformation on existing faults to be aseismic. These consequences are probably long-lived as it may take several million years for the excess pressure to dissipate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GCarp..68..130D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GCarp..68..130D"><span>The Campanian-Maastrichtian foraminiferal biostratigraphy of the basement <span class="hlt">sediments</span> from the southern Pannonian Basin (Vojvodina, northern Serbia): implications for the continuation of the Eastern Vardar and Sava <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dunčić, Milena; Dulić, Ivan; Popov, Olivera; Bogićević, Goran; Vranjković, Alan</p> <p>2017-04-01</p> <p>Micropalaeontological and biostratigraphical studies included Campanian-Maastrichtian complexes from five oil exploration wells drilled in northern Serbia (Vojvodina): the first is a carbonate-clastic complex and second is a complex containing ophiolites intercalated with hemipelagic and pelagic <span class="hlt">sediments</span>. Within the studied complexes, rich associations of planktonic and benthic foraminifera, calcareous nannoplankton, palynomorphs, as well as shallow and deep-water fossil detritus were determined. The presence of relatively rich associations of planktonic foraminifera allowed recognition of two biozones: the Globotruncana ventricosa <span class="hlt">Zone</span>, observed in the <span class="hlt">sediments</span> of the carbonate-clastic complex and the Gansserina gansseri <span class="hlt">Zone</span>, observed in both complexes. Except biozones, based on documented index species, for some units in both complexes, larger benthic foraminifera species had special biostratigraphical value, and in some of them, the calcareous nannoplankton <span class="hlt">zones</span> were recognized. The studied complexes represent deep-water formations, generated in oceanic island arc and trough <span class="hlt">zones</span>. The presence of limestones, which originate from destroyed rudist reefs, is explained by transfer by means of gravitational transport mechanisms of shallow-water <span class="hlt">sediments</span> to deep-water depositional environments. In this paper, the results of more detailed biostratigraphical and palaeo-ecological studies of foraminifera associations in Campanian-Maastrichtian complexes in Vojvodina are presented. Combined with lithological studies, seven units were determined within the complexes. The obtained results are important as a part of multidisciplinary, regional exploration of both complexes, generated in specific geological conditions, that today constitute a part of the pre-Neogene basement complex in the southeastern part of the Pannonian Basin. The Campanian- Maastrichtian carbonate-clastic complex represents sedimentary cover of the Eastern Vardar Ophiolitic Unit, while the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA269869','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA269869"><span>Chronic Sublethal Effects of San Francisco Bay <span class="hlt">Sediments</span> on Nereis (Neanthes) arenaceodentata; Bioaccumulation from Bedded <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1993-09-01</p> <p><span class="hlt">Sediments</span> were also analyzed for tributyltins . dibutyltins, and monobutyltins ( TBT , DBT, and MBT) by the Naval Command and Con- trol and Ocean...outlined in USEPA SW-846 (USEPA 1986). Tissues were also analyzed tor tributyltins , dibutyltins and monobutyltins by the NRaD in San Diego, CA, using... tributyltin were significantly higher in the tissues of animals <span class="hlt">recovered</span> from OC <span class="hlt">sediment</span> relative to the SC sedi- ment. A number of metals (i.e</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27595942','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27595942"><span>Temporal variation on environmental variables and pollution indicators in marine <span class="hlt">sediments</span> under sea Salmon farming cages in protected and exposed <span class="hlt">zones</span> in the Chilean inland Southern Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Urbina, Mauricio A</p> <p>2016-12-15</p> <p>The impacts of any activity on marine ecosystems will depend on the characteristics of the receptor medium and its resilience to external pressures. Salmon farming industry develops along a constant gradient of hydrodynamic conditions in the south of Chile. However, the influence of the hydrodynamic characteristics (weak or strong) on the impacts of intensive salmon farming is still poorly understood. This one year study evaluates the impacts of salmon farming on the marine <span class="hlt">sediments</span> of both protected and exposed marine <span class="hlt">zones</span> differing in their hydrodynamic characteristics. Six physico-chemical, five biological variables and seven indexes of marine <span class="hlt">sediments</span> status were evaluated under the salmon farming cages and control sites. Our results identified a few key variables and indexes necessary to accurately evaluate the salmon farming impacts on both protected and exposed <span class="hlt">zones</span>. Interestingly, the ranking of importance of the variables and the temporality of the observed changes, varied depending on the hydrodynamic characteristics. Biological variables (nematodes abundance) and environmental indexes (Simpson's dominance, Shannon's diversity and Pielou evenness) are the first to reflect detrimental impacts under the salmon farming cages. Then the physico-chemical variables such as redox, sulphurs and phosphorus in both <span class="hlt">zones</span> also show detrimental impacts. Based on the present results we propose that the hydrodynamic regime is an important driver of the magnitude and temporality of the effects of salmon farming on marine <span class="hlt">sediments</span>. The variables and indexes that best reflect the effects of salmon farming, in both protected and exposed <span class="hlt">zones</span>, are also described. Copyright © 2016. Published by Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28664369','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28664369"><span>Rapid and efficient method to extract metagenomic DNA from estuarine <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Shamim, Kashif; Sharma, Jaya; Dubey, Santosh Kumar</p> <p>2017-07-01</p> <p>Metagenomic DNA from <span class="hlt">sediments</span> of selective estuaries of Goa, India was extracted using a simple, fast, efficient and environment friendly method. The recovery of pure metagenomic DNA from our method was significantly high as compared to other well-known methods since the concentration of <span class="hlt">recovered</span> metagenomic DNA ranged from 1185.1 to 4579.7 µg/g of <span class="hlt">sediment</span>. The purity of metagenomic DNA was also considerably high as the ratio of absorbance at 260 and 280 nm ranged from 1.88 to 1.94. Therefore, the <span class="hlt">recovered</span> metagenomic DNA was directly used to perform various molecular biology experiments viz. restriction digestion, PCR amplification, cloning and metagenomic library construction. This clearly proved that our protocol for metagenomic DNA extraction using silica gel efficiently removed the contaminants and prevented shearing of the metagenomic DNA. Thus, this modified method can be used to <span class="hlt">recover</span> pure metagenomic DNA from various estuarine <span class="hlt">sediments</span> in a rapid, efficient and eco-friendly manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70009866','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70009866"><span>Determining earthquake recurrence intervals from deformational structures in young lacustrine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sims, John D.</p> <p>1975-01-01</p> <p>Examination of the silty <span class="hlt">sediments</span> in the lower Van Normal reservoir after the 1971 San Fernando, California earthquake revealed three <span class="hlt">zones</span> of deformational structures in the 1-m-thick sequence of <span class="hlt">sediments</span> exposed over about 2 km2 of the reservoir bottom. These <span class="hlt">zones</span> are correlated with moderate earthquakes that shook the San Fernando area in 1930, 1952, and 1971. The success of this study, coupled with the experimental formation of deformational structures similar to those of the Van Norman reservoir, led to a search for similar structures in Pleistocene and Holocene lakes and lake <span class="hlt">sediments</span> in other seismically active areas. Thus, studies have been started in Pleistocene and Holocene silty and sandy lake <span class="hlt">sediments</span> in the Imperial Valley, southeastern California; Clear Lake, in northern California; and the Puget Sound area of Washington. The Imperial Valley study has yielded spectacular results: five <span class="hlt">zones</span> of structures in the upper 10 m of Late Holocene <span class="hlt">sediments</span> near Brawley have been correlated over an area of approximately 100 km2, using natural outcrops. These structures are similar to those of the Van Norman reservoir and are interpreted to represent at least five moderate to large earthquakes that affected the southern Imperial Valley area during Late Holocene time. The Clear Lake study has provided ambiguous results with respect to determination of earthquake recurrence intervals because the cores studied are in clayey rich in organic material <span class="hlt">sediments</span> that have low liquefaction potential. A study of Late Pleistocene varved glacio-lacustrine <span class="hlt">sediments</span> has been started in the Puget Sound area of Washington, and thirteen sites have been examined. One has yielded 18.75 m of <span class="hlt">sediments</span> that contains 1,804 varves and fourteen deformed <span class="hlt">zones</span> interpreted as being caused by earthquake, because they are identical to structures formed experimentally by simulated seismic shaking. Correlation of deformational structures with seismic events is based on:(1) proximity</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24411518','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24411518"><span>Organic contamination of surface <span class="hlt">sediments</span> in the metropolitan coastal <span class="hlt">zone</span> of Athens, Greece: sources, degree, and ecological risk.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kapsimalis, V; Panagiotopoulos, I P; Talagani, P; Hatzianestis, I; Kaberi, H; Rousakis, G; Kanellopoulos, T D; Hatiris, G A</p> <p>2014-03-15</p> <p>Bottom <span class="hlt">sediments</span> represent a crucial component of the marine environment, since they constitute a habitat, a trophic resource, and a spawning place for various organisms. Unfortunately, the <span class="hlt">sediments</span> of urban coastal areas are deeply impacted by anthropogenic activities that degrade their quality. In the Drapetsona-Keratsini metropolitan coastal <span class="hlt">zone</span> of Athens, current industrial and shipping activities together with the effluents from a sewage outfall, which was in operation in the past, have resulted in one of the most contaminated sedimentary environments, in terms of organic compound loads, in Mediterranean. Exceptionally high concentrations of aliphatic hydrocarbons (up to 4457 μg g⁻¹), carcinogenic PAHs (up to 7284 ng g⁻¹), and organochlorines (up to 544 ng g⁻¹ for PCBs; up to 208 ng g⁻¹ for DDTs) constitute a major threat to the marine life of the associated Saronikos Gulf. Copyright © 2013 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T23A0591Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T23A0591Y"><span>Structural characteristics of the décollement <span class="hlt">zone</span> and underthrust <span class="hlt">sediments</span> in the Nankai accretionary prism: Geologic architectures in the Site C0023, IODP Expedition 370</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamamoto, Y.; Okutsu, N.; Yamada, Y.; Bowden, S.; Tonai, S.; Yang, K.; Tsang, M. Y.; Hirose, T.; Kamiya, N.</p> <p>2017-12-01</p> <p>Expedition 370 penetrated the accretionary prism, plate boundary décollement <span class="hlt">zone</span>, and underthrust <span class="hlt">sediment</span> and touched the basement basalt on the Philippine Sea Plate. The drilling site (C0023) is located 4 km NE from the legacy sites, Sites 808 and 1174. Compared to the legacy sites, the décollement <span class="hlt">zone</span> is characterized by weak and intermittent negative reflectors in the seismic profile. Onboard physical properties, e.g. porosity and P-wave velocity data, indeed show the smaller gaps at the top of the décollement <span class="hlt">zone</span>. The nature of the deformation along the décollement <span class="hlt">zone</span> represented 40 m thick phacoidal deformation <span class="hlt">zone</span> composed of fragmented mudstone with slickenlines on the surfaces in the Sites 808 and 1174. Compare with this, décollement <span class="hlt">zone</span> in Site C0023 represented the weaker and non-localized deformation <span class="hlt">zone</span> comprised of alternating <span class="hlt">zone</span> of 1 m thick phacoidal deformation <span class="hlt">zones</span> and a few 10 m of intact intervals in the Site C0023. Many normal faults striking parallel to the trench were identified just below the décollement <span class="hlt">zone</span>, which is indicative of non-localized deformations along the décollement <span class="hlt">zone</span>. Many of these faults were accompanied with calcite and sulphate mineral veins (anhydrite and barite), indicative of high-temperature fluid migration just above the ridge-spreading center. Based on the paleomagnetic restoration of structure to the geologic coordinate, attitudes of the bedding and fault planes in the Site C0023 are controlled by two factors: 1) subduction/accretion producing the trench-parallel bedding strikes and trench-perpendicular principal stress and 2) ridge spreading that produces ridge-parallel bedding and vein strikes. The former developed in the accretionary prism and the upper part of the underthrust <span class="hlt">sediment</span> (<900 mbsf), whereas the latter occurs in the lower part (>900 mbsf). These tectonic variations might affect fluid migration pathways.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030064','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030064"><span>Spectroscopic evidence for uranium bearing precipitates in vadose <span class="hlt">zone</span> <span class="hlt">sediments</span> at the Hanford 300-area site</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Arai, Y.; Marcus, M.A.; Tamura, N.; Davis, J.A.; Zachara, J.M.</p> <p>2007-01-01</p> <p>Uranium (U) solid-state speciation in vadose <span class="hlt">zone</span> <span class="hlt">sediments</span> collected beneath the former North Process Pond (NPP) in the 300 Area of the Hanford site (Washington) was investigated using multi-scale techniques. In 30 day batch experiments, only a small fraction of total U (???7.4%) was released to artificial groundwater solutions equilibrated with 1% pCO2. Synchrotron-based micro-X-ray fluorescence spectroscopy analyses showed that U was distributed among at least two types of species: (i) U discrete grains associated with Cu and (ii) areas with intermediate U concentrations on grains and grain coatings. Metatorbernite (Cu[UO2]2[PO 4]2??8H2O) and uranophane (Ca[UO 2]2[SiO3(OH)]2?? 5H 2O) at some U discrete grains, and muscovite at U intermediate concentration areas, were identified in synchrotron-based micro-X-ray diffraction. Scanning electron microscopy/energy dispersive X-ray analyses revealed 8-10 ??m size metatorbernite particles that were embedded in C-, Al-, and Si-rich coatings on quartz and albite grains. In ??- and bulk-X-ray absorption structure (??-XAS and XAS) spectroscopy analyses, the structure of metatorbernite with additional U-C and U-U coordination environments was consistently observed at U discrete grains with high U concentrations. The consistency of the ??- and bulk-XAS analyses suggests that metatorbernite may comprise a significant fraction of the total U in the sample. The entrapped, micrometer-sized metatorbernite particles in C-, Al-, and Si-rich coatings, along with the more soluble precipitated uranyl carbonates and uranophane, likely control the long-term release of U to water associated with the vadose <span class="hlt">zone</span> <span class="hlt">sediments</span>. ?? 2007 American Chemical Society.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-10-01/pdf/2013-23859.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-10-01/pdf/2013-23859.pdf"><span>78 FR 60218 - Safety <span class="hlt">Zone</span>; Old Mormon Slough, Stockton, CA</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-10-01</p> <p>... decontaminate soil, groundwater, and <span class="hlt">sediment</span> in Old Mormon Slough and the surrounding basin. This safety <span class="hlt">zone</span>... safety <span class="hlt">zone</span> in Old Mormon Slough to further the efforts of the EPA to rehabilitate soil, <span class="hlt">sediment</span>, and... water collection ponds. The unlined oily waste ponds were closed in 1981. Sampling has shown that soils...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUFMOS53A0980C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUFMOS53A0980C"><span>The Study of Geotechnical Properties of <span class="hlt">Sediment</span> in C-C <span class="hlt">Zone</span> in the Northeastern Pacific for Deep-sea Mining</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chi, S.; Kim, K.; Lee, H.; Ju, S.; Yoo, C.</p> <p>2007-12-01</p> <p>Recently the market price of valuable metals are rapidly increased due to the high demand and limited resources. Therefore, manganese (Mn)-nodules (Polymetallic nodules) in the Clarion-Clipperton fracture <span class="hlt">zone</span> have stimulated economic interest. Nickel, copper, cobalt and manganese are the economically most interesting metals of Mn-nodules. In order to mine Mn-nodules from sea floor, understanding the geotechnical properties of surface <span class="hlt">sediment</span> are very important for two major reasons. First, geotechnical data are required to design and build the stable and environmentally acceptable mining vehicles. Second, deep-sea mining activity could significantly effect on the surface layer of deep sea floor. For example, surface <span class="hlt">sediments</span> will be redistributed through the resuspension and redeposition. Reliable sedimentological and soil mechanical baseline data of the undisturbed benthic environment are essential to assess and evaluate these environmental impacts by mining activity using physical and numerical modeling. The 225 times deployments of the multiple corer guaranteed undisturbed <span class="hlt">sediment</span> samples in which geotechnical parameters were measured including <span class="hlt">sediment</span> grain size, density, water content, shear strength. The sea floor <span class="hlt">sediments</span> in this study area are generally characterized into three different types as follow. The seabed of the middle part (8-12° N) of this study area is mainly covered with biogenic siliceous <span class="hlt">sediment</span> compared with pelagic red clays in the northern part (16-17° N). However, the southern part (5-6° N) is dominant with calcareous <span class="hlt">sediments</span> because its water depth is shallower than the carbonate compensation depth (CCD). This result suggests that middle area, covered with siliceous <span class="hlt">sediment</span>, is more feasible for commercial mining than northern area, covered with pelagic red clay, with the consideration of the nodule miner maneuverability and the environmental impact. Especially, middle part with the highest nodule abundance and valuable</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176518','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176518"><span>Balanced <span class="hlt">sediment</span> fluxes in southern California’s Mediterranean-climate <span class="hlt">zone</span> salt marshes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rosencranz, Jordan A.; Ganju, Neil K.; Ambrose, Richard F.; Brosnahan, Sandra M.; Dickhudt, Patrick J.; Guntenspergen, Glenn R.; MacDonald, Glen M.; Takekawa, John Y.; Thorne, Karen M.</p> <p>2016-01-01</p> <p>Salt marsh elevation and geomorphic stability depends on mineral <span class="hlt">sedimentation</span>. Many Mediterranean-climate salt marshes along southern California, USA coast import <span class="hlt">sediment</span> during El Niño storm events, but <span class="hlt">sediment</span> fluxes and mechanisms during dry weather are potentially important for marsh stability. We calculated tidal creek <span class="hlt">sediment</span> fluxes within a highly modified, <span class="hlt">sediment</span>-starved, 1.5-km2 salt marsh (Seal Beach) and a less modified 1-km2marsh (Mugu) with fluvial <span class="hlt">sediment</span> supply. We measured salt marsh plain suspended <span class="hlt">sediment</span> concentration and vertical accretion using single stage samplers and marker horizons. At Seal Beach, a 2014 storm yielded 39 and 28 g/s mean <span class="hlt">sediment</span> fluxes and imported 12,000 and 8800 kg in a western and eastern channel. Western channel storm imports offset 8700 kg exported during 2 months of dry weather, while eastern channel storm imports augmented 9200 kg imported during dry weather. During the storm at Mugu, suspended <span class="hlt">sediment</span> concentrations on the marsh plain increased by a factor of four; accretion was 1–2 mm near creek levees. An exceptionally high tide sequence yielded 4.4 g/s mean <span class="hlt">sediment</span> flux, importing 1700 kg: 20 % of Mugu’s dry weather fluxes. Overall, low <span class="hlt">sediment</span> fluxes were observed, suggesting that these salt marshes are geomorphically stable during dry weather conditions. Results suggest storms and high lunar tides may play large roles, importing <span class="hlt">sediment</span> and maintaining dry weather <span class="hlt">sediment</span> flux balances for southern California salt marshes. However, under future climate change and sea level rise scenarios, results suggest that balanced <span class="hlt">sediment</span> fluxes lead to marsh elevational instability based on estimated mineral <span class="hlt">sediment</span> deficits.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..121..143W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..121..143W"><span>Biogeochemical flux and phytoplankton succession: A year-long <span class="hlt">sediment</span> trap record in the Australian sector of the Subantarctic <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilks, Jessica V.; Rigual-Hernández, Andrés S.; Trull, Thomas W.; Bray, Stephen G.; Flores, José-Abel; Armand, Leanne K.</p> <p>2017-03-01</p> <p>The Subantarctic <span class="hlt">Zone</span> (SAZ) plays a crucial role in global carbon cycling as a significant sink for atmospheric CO2. In the Australian sector, the SAZ exports large quantities of organic carbon from the surface ocean, despite lower algal biomass accumulation in surface waters than other Southern Ocean sectors. We present the first analysis of diatom and coccolithophore assemblages and seasonality, as well as the first annual quantification of bulk organic components of captured material at the base of the mixed layer (500 m depth) in the SAZ. <span class="hlt">Sediment</span> traps were moored in the SAZ southwest of Tasmania as part of the long-term SAZ Project for one year (September 2003 to September 2004). Annual mass flux at 500 m and 2000 m was composed mainly of calcium carbonate, while biogenic silica made up on average <10% of material captured in the traps. Organic carbon flux was estimated at 1.1 g m-2 y-1 at 500 m, close to the estimated global mean carbon flux. Low diatom fluxes and high fluxes of coccoliths were consistent with low biogenic silica and high calcium carbonate fluxes, respectively. Diatoms and coccoliths were identified to species level. Diatom and coccolithophore sinking assemblages reflected some seasonal ecological succession. A theoretical scheme of diatom succession in live assemblages is compared to successional patterns presented in <span class="hlt">sediment</span> traps. This study provides a unique, direct measurement of the biogeochemical fluxes and their main biological carbon vectors just below the winter mixed layer depth at which effective sequestration of carbon occurs. Comparison of these results with previous <span class="hlt">sediment</span> trap deployments at the same site at deeper depths (i.e. 1000, 2000 and 3800 m) documents the changes particle fluxes experience in the lower "twilight <span class="hlt">zone</span>" where biological processes and remineralisation of carbon reduce the efficiency of carbon sequestration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3317506','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3317506"><span>Characterization of Metabolically Active Bacterial Populations in Subseafloor Nankai Trough <span class="hlt">Sediments</span> above, within, and below the Sulfate–Methane Transition <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mills, Heath J.; Reese, Brandi Kiel; Shepard, Alicia K.; Riedinger, Natascha; Dowd, Scot E.; Morono, Yuki; Inagaki, Fumio</p> <p>2012-01-01</p> <p>A remarkable number of microbial cells have been enumerated within subseafloor <span class="hlt">sediments</span>, suggesting a biological impact on geochemical processes in the subseafloor habitat. However, the metabolically active fraction of these populations is largely uncharacterized. In this study, an RNA-based molecular approach was used to determine the diversity and community structure of metabolically active bacterial populations in the upper sedimentary formation of the Nankai Trough seismogenic <span class="hlt">zone</span>. Samples used in this study were collected from the slope apron <span class="hlt">sediment</span> overlying the accretionary prism at Site C0004 during the Integrated Ocean Drilling Program Expedition 316. The <span class="hlt">sediments</span> represented microbial habitats above, within, and below the sulfate–methane transition <span class="hlt">zone</span> (SMTZ), which was observed approximately 20 m below the seafloor (mbsf). Small subunit ribosomal RNA were extracted, quantified, amplified, and sequenced using high-throughput 454 pyrosequencing, indicating the occurrence of metabolically active bacterial populations to a depth of 57 mbsf. Transcript abundance and bacterial diversity decreased with increasing depth. The two communities below the SMTZ were similar at the phylum level, however only a 24% overlap was observed at the genus level. Active bacterial community composition was not confined to geochemically predicted redox stratification despite the deepest sample being more than 50 m below the oxic/anoxic interface. Genus-level classification suggested that the metabolically active subseafloor bacterial populations had similarities to previously cultured organisms. This allowed predictions of physiological potential, expanding understanding of the subseafloor microbial ecosystem. Unique community structures suggest very diverse active populations compared to previous DNA-based diversity estimates, providing more support for enhancing community characterizations using more advanced sequencing techniques. PMID:22485111</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4141734','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4141734"><span>Barrier Island Morphology and <span class="hlt">Sediment</span> Characteristics Affect the Recovery of Dune Building Grasses following Storm-Induced Overwash</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Brantley, Steven T.; Bissett, Spencer N.; Young, Donald R.; Wolner, Catherine W. V.; Moore, Laura J.</p> <p>2014-01-01</p> <p>Barrier islands are complex and dynamic systems that provide critical ecosystem services to coastal populations. Stability of these systems is threatened by rising sea level and the potential for coastal storms to increase in frequency and intensity. Recovery of dune-building grasses following storms is an important process that promotes topographic heterogeneity and long-term stability of barrier islands, yet factors that drive dune recovery are poorly understood. We examined vegetation recovery in overwash <span class="hlt">zones</span> on two geomorphically distinct (undisturbed vs. frequently overwashed) barrier islands on the Virginia coast, USA. We hypothesized that vegetation recovery in overwash <span class="hlt">zones</span> would be driven primarily by environmental characteristics, especially elevation and beach width. We sampled species composition and environmental characteristics along a continuum of disturbance from active overwash <span class="hlt">zones</span> to relict overwash <span class="hlt">zones</span> and in adjacent undisturbed environments. We compared species assemblages along the disturbance chronosequence and between islands and we analyzed species composition data and environmental measurements with Canonical Correspondence Analysis to link community composition with environmental characteristics. <span class="hlt">Recovering</span> and geomorphically stable dunes were dominated by Ammophila breviligulata Fernaud (Poaceae) on both islands while active overwash <span class="hlt">zones</span> were dominated by Spartina patens (Aiton) Muhl. (Poaceae) on the frequently disturbed island and bare sand on the less disturbed island. Species composition was associated with environmental characteristics only on the frequently disturbed island (p = 0.005) where A. breviligulata was associated with higher elevation and greater beach width. Spartina patens, the second most abundant species, was associated with larger <span class="hlt">sediment</span> grain size and greater <span class="hlt">sediment</span> size distribution. On the less frequently disturbed island, time since disturbance was the only factor that affected community</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28883417','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28883417"><span>The Deposition and Accumulation of Microplastics in Marine <span class="hlt">Sediments</span> and Bottom Water from the Irish Continental Shelf.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martin, Jake; Lusher, Amy; Thompson, Richard C; Morley, Audrey</p> <p>2017-09-07</p> <p>Microplastics are widely dispersed throughout the marine environment. An understanding of the distribution and accumulation of this form of pollution is crucial for gauging environmental risk. Presented here is the first record of plastic contamination, in the 5 mm-250 μm size range, of Irish continental shelf <span class="hlt">sediments</span>. Sixty-two microplastics were <span class="hlt">recovered</span> from 10 of 11 stations using box cores. 97% of <span class="hlt">recovered</span> microplastics were found to reside shallower than 2.5 cm <span class="hlt">sediment</span> depth, with the area of highest microplastic concentration being the water-<span class="hlt">sediment</span> interface and top 0.5 cm of <span class="hlt">sediments</span> (66%). Microplastics were not found deeper than 3.5 ± 0.5 cm. These findings demonstrate that microplastic contamination is ubiquitous within superficial <span class="hlt">sediments</span> and bottom water along the western Irish continental shelf. Results highlight that cores need to be at least 4-5 cm deep to quantify the standing stock of microplastics within marine <span class="hlt">sediments</span>. All <span class="hlt">recovered</span> microplastics were classified as secondary microplastics as they appear to be remnants of larger items; fibres being the principal form of microplastic pollution (85%), followed by broken fragments (15%). The range of polymer types, colours and physical forms <span class="hlt">recovered</span> suggests a variety of sources. Further research is needed to understand the mechanisms influencing microplastic transport, deposition, resuspension and subsequent interactions with biota.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70189705','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70189705"><span>Eruptive and environmental processes recorded by diatoms in volcanically-dispersed lake <span class="hlt">sediments</span> from the Taupo Volcanic <span class="hlt">Zone</span>, New Zealand</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harper, Margaret A.; Pledger, Shirley A.; Smith, Euan G. C.; Van Eaton, Alexa; Wilson, Colin J. N.</p> <p>2015-01-01</p> <p>Late Pleistocene diatomaceous <span class="hlt">sediment</span> was widely dispersed along with volcanic ash (tephra) across and beyond New Zealand by the 25.4 ka Oruanui supereruption from Taupo volcano. We present a detailed analysis of the diatom populations in the Oruanui tephra and the newly discovered floras in two other eruptions from the same volcano: the 28.6 ka Okaia and 1.8 ka Taupo eruptions. For comparison, the diatoms were also examined in Late Pleistocene and Holocene lake <span class="hlt">sediments</span> from the Taupo Volcanic <span class="hlt">Zone</span> (TVZ). Our study demonstrates how these microfossils provide insights into the lake history of the TVZ since the Last Glacial Maximum. Morphometric analysis of Aulacoseira valve dimensions provides a useful quantitative tool to distinguish environmental and eruptive processes within and between individual tephras. The Oruanui and Okaia diatom species and valve dimensions are highly consistent with a shared volcanic source, paleolake and eruption style (involving large-scale magma-water interaction). They are distinct from lacustrine <span class="hlt">sediments</span> sourced elsewhere in the TVZ. Correspondence analysis shows that small, intact samples of erupted lake <span class="hlt">sediment</span> (i.e., lithic clasts in ignimbrite) contain heterogeneous diatom populations, reflecting local variability in species composition of the paleolake and its shallowly-buried <span class="hlt">sediments</span>. Our analysis also shows a dramatic post-Oruanui supereruption decline in Cyclostephanos novaezelandiae, which likely reflects a combination of (1) reorganisation of the watershed in the aftermath of the eruption, and (2) overall climate warming following the Last Glacial Maximum. This decline is reflected in substantially lower proportions of C. novaezelandiae in the 1.8 ka Taupo eruption deposits, and even fewer in post-1.8 ka <span class="hlt">sediments</span> from modern (Holocene) Lake Taupo. Our analysis highlights how the excellent preservation of siliceous microfossils in volcanic tephra may fingerprint the volcanic source region and retain a valuable record</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=198546&Lab=NRMRL&keyword=marine+AND+pollution&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=198546&Lab=NRMRL&keyword=marine+AND+pollution&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>USE OF <span class="hlt">SEDIMENT</span> CORE PROFILING IN ASSESSING EFFECTIVENESS OF MONITORED NATURAL RECOVERY</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>The <span class="hlt">Sediment</span> Issue summarizes two studies conducted by the National Risk Management Research Laboratory of U.S. EPA to evaluate the natural recovery of surface <span class="hlt">sediments</span> contaminated with polycyclic aromatic hydrocarbons (PAHs) an polychlorinated biphenyls (PCBs). Natural <span class="hlt">recove</span>...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T33C2953S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T33C2953S"><span>Nature and Role of Subducting <span class="hlt">Sediments</span> on the Megathrust and Forearc Evolution in the 2004 Great Sumatra Earthquake Rupture <span class="hlt">Zone</span>: Results from Full Waveform Inversion of Long Offset Seismic Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, S. C.; Qin, Y.</p> <p>2015-12-01</p> <p>On active accretionary margins, the nature of incoming <span class="hlt">sediments</span> defines the locking mechanism on the megathrust, and the development and evolution of the accretionary wedge. Drilling is the most direct method to characterise the nature of these <span class="hlt">sediments</span>, but the drilling is very expensive, and provide information at only a few locations. In north Sumatra, an IODP drilling is programmed to take place in July-August 2016. We have performed seismic full waveform inversion of 12 km long offset seismic reflection data acquired by WesternGeco in 2006 over a 35 km <span class="hlt">zone</span> near the subduction front in the 2004 earthquake rupture <span class="hlt">zone</span> area that provide detailed quantitative information on the characteristics of the incoming <span class="hlt">sediments</span>. We first downward continue the surface streamer data to the seafloor, which removes the effect of deep water (~5 km) and brings out the refraction arrivals as the first arrivals. We carry out travel time tomography, and then performed full waveform inversion of seismic refraction data followed by the full waveform inversion of reflection data providing detailed (10-20 m) velocity structure. The <span class="hlt">sediments</span> in this area are 3-5 km thick where the P-wave velocity increases from 1.6 km/s near the seafloor to more than 4.5 km/s above the oceanic crust. The high velocity of <span class="hlt">sediments</span> above the basement suggests that the <span class="hlt">sediments</span> are highly compacted, strengthened the coupling near the subduction front, which might have been responsible for 2004 earthquake rupture propagation up to the subduction front, enhancing the tsunami. We also find several thin velocity layers within the <span class="hlt">sediments</span>, which might be due to high pore-pressure fluid or free gas. These layers might be responsible for the formation of pseudo-decollement within the forearc <span class="hlt">sediments</span> that acts as a conveyer belt between highly compacted subducting lower <span class="hlt">sediments</span> and accreted <span class="hlt">sediments</span> above. The presence of well intact <span class="hlt">sediments</span> on the accretionary prism supports this interpretation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70175367','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70175367"><span>Mihi Breccia: A stack of lacustrine <span class="hlt">sediments</span> and subaqueous pyroclastic flows within the Taupo Volcanic <span class="hlt">Zone</span>, New Zealand</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Downs, Drew</p> <p>2016-01-01</p> <p>The Taupo Volcanic <span class="hlt">Zone</span> (TVZ), New Zealand, encompasses a wide variety of arc-related strata, although most of its small-volume (non-caldera-forming) eruptions are poorly-exposed and extensively hydrothermally altered. The Mihi Breccia is a stratigraphic sequence consisting of interbedded rhyolitic pyroclastic flows and lacustrine <span class="hlt">sediments</span> with eruption ages of 281 ± 18 to at least 239 ± 6 ka (uncertainties at 2σ). In contrast to other small-volume rhyolitic eruptions within the TVZ, Mihi Breccia is relatively well-exposed within the Paeroa fault block, and contains minimal hydrothermal alteration. Pyroclastic flow characteristics and textures including: 1) breadcrusted juvenile clasts, 2) lack of welding, 3) abundant ash-rich matrix, 4) lack of fiamme and eutaxitic textures, 5) lack of thermal oxidation colors, 6) lack of cooling joints, 7) exclusive lacustrine <span class="hlt">sediment</span> lithic clasts, and 8) interbedding with lacustrine <span class="hlt">sediments</span>, all indicating that Mihi Breccia strata originated in a paleo-lake system. This ephemeral paleo-lake system is inferred to have lasted for > 50 kyr (based on Mihi Breccia age constraints), and referred to as Huka Lake. Mihi Breccia pyroclastic flow juvenile clast geochemistry and petrography correspond with similar-aged (264 ± 8, 263 ± 10, and 247 ± 4 ka) intra-caldera rhyolite domes filling the Reporoa caldera (source of the 281 ± 81 Kaingaroa Formation ignimbrite). These exposed intra-caldera rhyolite domes (as well as geophysically inferred subsurface domes) are proposed to be source vents for the Mihi Breccia pyroclastic flows. Soft-<span class="hlt">sediment</span> deformation associated with Mihi Breccia strata indicate either seismic shock, rapid <span class="hlt">sediment</span> loading during pyroclastic flow emplacement, or both. Thus, the Mihi Breccia reflects a prolonged series of subaqueous rhyolite dome building and associated pyroclastic flows, accompanied by seismic activity, emplaced into a large paleo-lake system within the TVZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JVGR..327..180D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JVGR..327..180D"><span>Mihi Breccia: A stack of lacustrine <span class="hlt">sediments</span> and subaqueous pyroclastic flows within the Taupo Volcanic <span class="hlt">Zone</span>, New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Downs, Drew T.</p> <p>2016-11-01</p> <p>The Taupo Volcanic <span class="hlt">Zone</span> (TVZ), New Zealand, encompasses a wide variety of arc-related strata, although most of its small-volume (non-caldera-forming) eruptions are poorly-exposed and extensively hydrothermally altered. The Mihi Breccia is a stratigraphic sequence consisting of interbedded rhyolitic pyroclastic flows and lacustrine <span class="hlt">sediments</span> with eruption ages of 281 ± 18 to at least 239 ± 6 ka (uncertainties at 2σ). In contrast to other small-volume rhyolitic eruptions within the TVZ, Mihi Breccia is relatively well-exposed within the Paeroa fault block, and contains minimal hydrothermal alteration. Pyroclastic flow characteristics and textures include: 1) prismatically jointed juvenile clasts, 2) lack of welding, 3) abundant ash-rich matrix, 4) lack of fiamme and eutaxitic textures, 5) lack of thermal oxidation colors, 6) lack of cooling joints, 7) exclusive lacustrine <span class="hlt">sediment</span> lithic clasts, and 8) interbedding with lacustrine <span class="hlt">sediments</span>, all indicating that Mihi Breccia strata originated in a paleo-lake system. This ephemeral paleo-lake system is inferred to have lasted for > 50 kyr (based on Mihi Breccia age constraints), and referred to as Huka Lake. Mihi Breccia pyroclastic flow juvenile clast geochemistry and petrography correspond with similar-aged (264 ± 8, 263 ± 10, and 247 ± 4 ka) intra-caldera rhyolite domes filling the Reporoa caldera (source of the 281 ka Kaingaroa Formation ignimbrite). These exposed intra-caldera rhyolite domes (as well as geophysically inferred subsurface domes) are proposed to be source vents for the Mihi Breccia pyroclastic flows. Soft-<span class="hlt">sediment</span> deformation associated with Mihi Breccia strata indicates either seismic shock, rapid <span class="hlt">sediment</span> loading during pyroclastic flow emplacement, or both. Thus, the Mihi Breccia reflects a prolonged series of subaqueous rhyolite dome building and associated pyroclastic flows, accompanied by seismic activity, emplaced into a large paleo-lake system within the TVZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MinPe.109..679B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MinPe.109..679B"><span>Morphogenesis and grain size variation of alluvial gold <span class="hlt">recovered</span> in auriferous <span class="hlt">sediments</span> of the Tormes Basin (Iberian Peninsula) using a simple correspondence analysis</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barrios, S.; Merinero, R.; Lozano, R.; Orea, I.</p> <p>2015-12-01</p> <p>With present techniques it is difficult to determine whether the gold particles present at fluvial placers have come from one or multiple sources. Knowledge of this would be useful in prospecting for larger gold deposits. The aim of the present work was to test the potential of a technique based on modern visual and classic statistical methods to determine the single or multisource origin of gold particles at different sites in the Tormes Basin (Central Iberian <span class="hlt">Zone</span> of the Iberian Massif, Iberian Peninsula). This basin contains numerous lode and placer gold deposits that have been exploited since ancient times. Today, gold nuggets (usually associated with quartz, 0.2-6 g in weight, 0.53-3.74 cm long and mostly discoidal in shape and of intermediate roundness) can be <span class="hlt">recovered</span> from the <span class="hlt">sediments</span> of the upper reaches of the River Tormes. These nuggets, as well as small gold particles collected at three gravel pits from across the basin (all of which showed abrasion marks) were examined by optical and/or environmental scanning electron microscopy, and the differences in their dimensions and morphological features noted. Simple correspondence analysis of the sphericity and roundness of the nuggets and particles was used to morphologically classify the gold samples collected at each location. The gold nuggets were best classified as elongated rods of intermediate roundness. Surprisingly, the gold particles from the most upstream and downstream gravel pits were best described as discs/sub-discs of rounded appearance, while those from the intermediate gravel pit were discs of intermediate roundness. Analysis of the variance followed by the Tukey honest significant differences test revealed the particles from the most upstream gravel pit to be significantly more flattened and smaller. These were therefore transported further from their source than the particles collected at the other two pits. These results suggest that multiple sources of sedimentary gold exist in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23479889','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23479889"><span>[Ciliate diversity and spatiotemporal variation in surface <span class="hlt">sediments</span> of Yangtze River estuary hypoxic <span class="hlt">zone</span>].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Feng, Zhao; Kui-Dong, Xu; Zhao-Cui, Meng</p> <p>2012-12-01</p> <p>By using denaturing gradient gel electrophoresis (DGGE) and sequencing as well as Ludox-QPS method, an investigation was made on the ciliate diversity and its spatiotemporal variation in the surface <span class="hlt">sediments</span> at three sites of Yangtze River estuary hypoxic <span class="hlt">zone</span> in April and August 2011. The ANOSIM analysis indicated that the ciliate diversity had significant difference among the sites (R = 0.896, P = 0.0001), but less difference among seasons (R = 0.043, P = 0.207). The sequencing of 18S rDNA DGGE bands revealed that the most predominant groups were planktonic Choreotrichia and Oligotrichia. The detection by Ludox-QPS method showed that the species number and abundance of active ciliates were maintained at a higher level, and increased by 2-5 times in summer, as compared with those in spring. Both the Ludox-QPS method and the DGGE technique detected that the ciliate diversity at the three sites had the similar variation trend, and the Ludox-QPS method detected that there was a significant variation in the ciliate species number and abundance between different seasons. The species number detected by Ludox-QPS method was higher than that detected by DGGE bands. Our study indicated that the ciliates in Yangtze River estuary hypoxic <span class="hlt">zone</span> had higher diversity and abundance, with the potential to supply food for the polyps of jellyfish.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1052525','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1052525"><span>Effects of remediation amendments on vadose <span class="hlt">zone</span> microorganisms</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Miller, Hannah M.; Tilton, Fred A.</p> <p>2012-08-10</p> <p>Surfactant-based foam delivery technology has been studied to remediate Hanford 200 area deep vadose <span class="hlt">zone</span> <span class="hlt">sediment</span>. However, the surfactants and remediation amendments have an unknown effect on indigenous subsurface microorganisms. Microbial populations are important factors to consider in remediation efforts due to their potential to alter soil geochemistry. This project focuses on measuring microbial metabolic responses to remediation amendments in batch and column studies using Deep Vadose <span class="hlt">Zone</span> <span class="hlt">Sediments</span>. Initial studies of the microbes from Hanford 200 area deep vadose <span class="hlt">zone</span> <span class="hlt">sediment</span> showed surfactants sodium dodecyl sulfate (SDS) and cocamidopropyl betaine (CAPB) and remediation amendment calcium polysulfide (CPS) had nomore » affect on microbial growth using BiologTM Ecoplates. To move towards a more realistic field analog, soil columns were packed with Hanford 200 Area <span class="hlt">sediment</span>. Once microbial growth in the column was verified by observing growth of the effluent solution on tryptic soy agar plates, remedial surfactants were injected into the columns, and the resulting metabolic diversity was measured. Results suggest surfactant sodium dodecyl sulfate (SDS) stimulates microbial growth. The soil columns were also visualized using X-ray microtomography to inspect soil packing and possibly probe for evidence of biofilms. Overall, BiologTM Ecoplates provide a rapid assay to predict effects of remediation amendments on Hanford 200 area deep vadose <span class="hlt">zone</span> microorganisms.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA047235','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA047235"><span>Suspended <span class="hlt">Sediments</span> Measured in the Surf <span class="hlt">Zone</span>.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1977-09-01</p> <p>order that a comparison of the two methods could be made. During these <span class="hlt">sediment</span> transport studies, Lagrangian floats made from wine bottles...1 J \\J \\ I ÜU! 40 - - - irM ....... ^_^^. -- - — - plWVtl . .11 ---*»— •.’...— / UJ m 27 z: C3 - IT i Spectra</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMOS43A0530M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMOS43A0530M"><span>Trace Metal Distribution and Speciation in Pore Water of Hydrothermal <span class="hlt">Sediments</span> From the Guaymas Basin, Gulf of California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morales-Villafuerte, M.; Ortega-Osorio, A.; Wheat, G.; Seewald, J.</p> <p>2004-12-01</p> <p>Thirteen <span class="hlt">sediment</span> cores were collected through out direct sampling with the MBARI/ ROV "Tiburon" in the southern trough of the Guaymas Basin in March 2003. Pore water samples from regular 2.5 cm intervals of <span class="hlt">sediment</span> cores were extracted onboard by centrifugation. The supernatants were collected in clean polystyrene vials and stored at 4° C until analytical work on shore. Dissolved Fe, Mn, Cu, Pb, Zn and Ni concentrations in extracted fluid samples were analyzed by direct injection of atomic absorption spectrometry. Four <span class="hlt">zones</span> in the hydrothermal field were classified according to their physical characteristics. A core located away from the influence of active vents was <span class="hlt">recovered</span> as a background site. The second <span class="hlt">zone</span> is characterized by low temperatures (4.2-80° C) and <span class="hlt">sediments</span> saturated in hydrocarbons. Sulfides formation and higher temperatures (4-166° C) were observed in the third <span class="hlt">zone</span>. Precipitation of carbonates on top of the <span class="hlt">sediment</span> characterizes the fourth <span class="hlt">zone</span>. Concentration of trace metals at the water-<span class="hlt">sediment</span> interface appears to be the highest, probably due to metal precipitation from the hydrothermal plume, followed by diffusion into the pore water. A decrease in concentration is observed between 5-12 cm depth, suggesting that biological activity is consuming essential metals (<span class="hlt">zone</span> of bioturbation). Metal concentrations in <span class="hlt">zones</span> where sulfide phases are rich, exhibit smaller values in pore water (Fe=2.4-3.8 μ mol/kg, Cu=0.6-0.8 μ mol/kg, Pb=1.2-1.5 μ mol/kg, Zn=0.4-0.5 μ mol/kg and Ni= 3.4-4.4 μ mol/kg) relative to samples located at hydrocarbon sites (Fe= 2.7-11.4, Cu= 0.7-1.0 μ mol/kg, Pb= 1.2-2.2 μ mol/kg, Zn= 0.4-0.7 μ mol/kg and Ni= 3.4-5.2 μ mol/kg). At sulfide <span class="hlt">zones</span>, pH and Eh conditions help to precipitate their stable sulfides as opposed to the hydrocarbon areas, where conditions are not favorable for sulfide formation due to the absence of H2S. In general, Fe concentrations in pore water are lower than that of Mn, very likely</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=325323','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=325323"><span>Arid <span class="hlt">Zone</span> Hydrology</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Arid <span class="hlt">zone</span> hydrology encompasses a wide range of topics and hydro-meteorological and ecological characteristics. Although arid and semi-arid watersheds perform the same functions as those in humid environments, their hydrology and <span class="hlt">sediment</span> transport characteristics cannot be readily predicted by inf...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H51D1298L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H51D1298L"><span>Nitrogen fluxes across hydrogeomorphic <span class="hlt">zones</span> in coastal deltaic floodplain using flow-through technique</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, S.; Twilley, R.; Christensen, A.</p> <p>2017-12-01</p> <p>Coastal floodplain deltas are the region of continental margins of major river basins that can remove excess nitrogen before entering the coastal ocean. We propose that the processing of nitrogen in active deltaic wetlands varies with soil organic content in response to different hydrogeomorphic <span class="hlt">zones</span>. Continuous flow-through core system was used to incubate <span class="hlt">sediment</span> cores from supratidal, intertidal, and subtidal hydrogeomorphic <span class="hlt">zones</span> along a chronosequence in Wax Lake Delta during summer of 2017. Ambient water from Wax Lake Outlet was continuously pumped through sealed cores to estimate fluxes of inorganic nitrogen and phosphorus across the <span class="hlt">sediment</span>-water interface by calculating the difference between inflow and outflow concentrations. The average respiration rate of <span class="hlt">sediment</span> cores from intertidal <span class="hlt">zone</span> was about 1.5 g m-2 d-1 while the rate in supratidal <span class="hlt">zone</span> was more than doubled to 3.7 g m-2 d-1. Under the constant inflow concentration of nitrate (about 107.1 umol/L), <span class="hlt">sediment</span> cores in supratidal <span class="hlt">zone</span> exhibited greater NO3- uptake (1329.7 umol m-2 h-1) and N2 release (499.0 umol N m-2 h-1) than that in intertidal <span class="hlt">zone</span> (421.5 umol m-2 h-1 of NO3- uptake and 67.6 umol N m-2 h-1 of N2 flux respectively). These results indicate greater rate of net denitrification in supratidal <span class="hlt">zone</span> than intertidal <span class="hlt">zone</span> in the older chronosequence of the active delta (which formed approximately in 1980). Also, lower NH4 flux (mean 70.0 umol m-2 h-1) from <span class="hlt">sediment</span> to water column in supratidal <span class="hlt">zone</span> together with higher NO2- flux (mean 94.2 umol m-2 h-1) illustrated strong signal of nitrification. In conclusion, <span class="hlt">sediment</span> cores at the intertidal <span class="hlt">zone</span> helped to remove 12% of NO3- from the water column while cores at supratidal <span class="hlt">zone</span> removed 35% of NO3-. Based on the correlation between NO3- and N2 fluxes, about 60% of NO3- removed could be converted to N2 under <span class="hlt">sediment</span> organic concentrations of about 12%. Comparisons of NO3 removal and conversion to N2 by denitrification will be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H41H1337J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H41H1337J"><span>Porosity and Organic Carbon Controls on Naturally Reduced <span class="hlt">Zone</span> (NRZ) Formation Creating Microbial ';Hotspots' for Fe, S, and U Cycling in Subsurface <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jones, M. E.; Janot, N.; Bargar, J.; Fendorf, S. E.</p> <p>2013-12-01</p> <p>Previous studies have illustrated the importance of Naturally Reduced <span class="hlt">Zones</span> (NRZs) within saturated <span class="hlt">sediments</span> for the cycling of metals and redox sensitive contaminants. NRZs can provide a source of reducing equivalents such as reduced organic compounds or hydrogen to stimulate subsurface microbial communities. These NRZ's are typically characterized by low permeability and elevated concentrations of organic carbon and trace metals. However, both the formation of NRZs and their importance to the overall aquifer carbon remineralization is not fully understood. Within NRZs the hydrolysis of particulate organic carbon (POC) and subsequent fermentation of dissolved organic carbon (DOC) to form low molecular weight dissolved organic carbon (LMW-DOC) provides electron donors necessary for the respiration of Fe, S, and in the case of the Rifle aquifer, U. Rates of POC hydrolysis and subsequent fermentation have been poorly constrained and rates in excess and deficit to the rates of subsurface anaerobic respiratory processes have been suggested. In this study, we simulate the development of NRZ <span class="hlt">sediments</span> in diffusion-limited aggregates to investigate the physical and chemical conditions required for NRZ formation. Effects of <span class="hlt">sediment</span> porosity and POC loading on Fe, S, and U cycling on molecular and nanoscale are investigated with synchrotron-based Near Edge X-ray Absorption Fine Structure Spectroscopy (NEXAFS). Fourier Transform Ion Cyclotron Resonance Mass Spectrometry (FT-ICR-MS) and Fourier Transform Infrared spectroscopy (FTIR) are used to characterize the transformations in POC and DOC. <span class="hlt">Sediment</span> aggregates are inoculated with the natural microbial biota from the Rifle aquifer and population dynamics are monitored by 16S RNA analysis. Overall, establishment of low permeability NRZs within the aquifer stimulate microbial respiration beyond the diffusion-limited <span class="hlt">zones</span> and can limit the transport of U through a contaminated aquifer. However, the long-term stability of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019106','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019106"><span>Faulting of gas-hydrate-bearing marine <span class="hlt">sediments</span> - contribution to permeability</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dillon, William P.; Holbrook, W.S.; Drury, Rebecca; Gettrust, Joseph; Hutchinson, Deborah; Booth, James; Taylor, Michael</p> <p>1997-01-01</p> <p>Extensive faulting is observed in <span class="hlt">sediments</span> containing high concentrations of methane hydrate off the southeastern coast of the United States. Faults that break the sea floor show evidence of both extension and shortening; mud diapirs are also present. The <span class="hlt">zone</span> of recent faulting apparently extends from the ocean floor down to the base of gas-hydrate stability. We infer that the faulting resulted from excess pore pressure in gas trapped beneath the gas hydrate-beating layer and/or weakening and mobilization of <span class="hlt">sediments</span> in the region just below the gas-hydrate stability <span class="hlt">zone</span>. In addition to the <span class="hlt">zone</span> of surface faults, we identified two buried <span class="hlt">zones</span> of faulting, that may have similar origins. Subsurface faulted <span class="hlt">zones</span> appear to act as gas traps.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=43183&Lab=ORD&keyword=methodological+AND+method&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=43183&Lab=ORD&keyword=methodological+AND+method&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>RECOVERY OF DNA FROM SOILS AND <span class="hlt">SEDIMENTS</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Experiments were performed to evaluate the effectiveness of different methodological approaches for <span class="hlt">recovering</span> DNA from soil and <span class="hlt">sediment</span> bacterial communities; cell extraction followed by lysis and DNA recovery (cell extraction method) versus direct cell lysis and alkaline extra...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP41C..02K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP41C..02K"><span>Diffusive Transfer of Oxygen From Seamount Basaltic Crust Into Overlying <span class="hlt">Sediments</span>: an Example From the Clarion-Clipperton Fracture <span class="hlt">Zone</span>, Equatorial Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kasten, S.; Mewes, K.; Mogollón, J.; Picard, A.; Rühlemann, C.; Eisenhauer, A.; Kuhn, T.; Ziebis, W.</p> <p>2015-12-01</p> <p>Within the Clarion-Clipperton Fracture <span class="hlt">Zone</span> (CCFZ) located in the equatorial Pacific Ocean numerous seamounts, with diameters ranging from 3 to 30 km and varying heights above the surrounding seafloor of up to 2500 m, occur throughout the deep-sea plain. There is evidence that these may serve as conduits for low-temperature hydrothermal circulation of seawater through the oceanic crust. During RV SONNE cruise SO205 in April/May 2010 and BIONOD cruise with RV ĹATALANTE in spring 2012 we took piston and gravity cores for geochemical analyses, as well as for high-resolution pore-water oxygen and nutrient measurements. Specifically, we took cores along a transect at three sites, located 400, 700 and 1000 m away from the foot of a 240 m high seamount, called 'Teddy Bare'. At all 3 sites oxygen penetrates the entire <span class="hlt">sediment</span> column of the organic carbon-poor <span class="hlt">sediment</span>. More importantly, oxygen concentrations initially decrease with <span class="hlt">sediment</span> depth but increase again at depths of 3 m and 7 m above the basaltic basement, suggesting an upward diffusion of oxygen from seawater circulating within the seamount crust into the overlying basal <span class="hlt">sediments</span>. This is the first time this has been shown for the deep subsurface in the Pacific Ocean. Mirroring the oxygen concentrations nitrate concentrations accumulate with <span class="hlt">sediment</span> depth but decrease towards the basement. Transport-reaction modeling revealed that (1) the diffusive flux of oxygen from the basaltic basement exceeds the oxygen consumption through organic matter oxidation and nitrification in the basal <span class="hlt">sediments</span> and (2) the nutrient exchange between the <span class="hlt">sediment</span> and the underlying basaltic crust occurs at orders-of-magnitude lower rates than between the <span class="hlt">sediment</span> surface and the overlying bottom water. We furthermore show that the upward diffusion of oxygen from the basaltic basement affects the preservation of organic compounds within the oxic <span class="hlt">sediment</span> column at all 3 sites. Our investigations indicate that an upward</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27321802','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27321802"><span>Artificial soft <span class="hlt">sediment</span> resuspension and high density opportunistic macroalgal mat fragmentation as method for increasing <span class="hlt">sediment</span> zoobenthic assemblage diversity in a eutrophic lagoon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Martelloni, Tatiana; Tomassetti, Paolo; Gennaro, Paola; Vani, Danilo; Persia, Emma; Persiano, Marco; Falchi, Riccardo; Porrello, Salvatore; Lenzi, Mauro</p> <p>2016-09-15</p> <p>Superficial soft <span class="hlt">sediment</span> resuspension and partial fragmentation of high density opportunistic macroalgal mats were investigated by boat to determine the impact on zoobenthic assemblages in a eutrophic Mediterranean lagoon. <span class="hlt">Sediment</span> resuspension was used to oxidise superficial organic <span class="hlt">sediments</span> as a method to counteract the effects of eutrophication. Likewise, artificial decay of macroalgal mat was calculated to reduce a permanent source of <span class="hlt">sediment</span> organic matter. An area of 9ha was disturbed (<span class="hlt">zone</span> D) and two other areas of the same size were left undisturbed (<span class="hlt">zones</span> U). We measured chemical-physical variables, estimated algal biomass and sedimentary organic matter, and conducted qualitative and quantitative determinations of the zoobenthic species detected in <span class="hlt">sediment</span> and among algal mats. The results showed a constant major reduction in labile organic matter (LOM) and algal biomass in D, whereas values in U remained stable or increased. In the three <span class="hlt">zones</span>, however, bare patches of lagoon bed increased in size, either by direct effect of the boats in D or by anaerobic decay of the algal mass in U. Zoobenthic assemblages in algal mats reduced the number of species in D, probably due to the sharp reduction in biomass, but remained stable in U, whereas in all three areas abundance increased. <span class="hlt">Sediment</span> zoobenthic assemblages increased the number of species in D, as expected, due to drastic reduction in LOM, whereas values in U remained stable and again abundance increased in all three <span class="hlt">zones</span>. In conclusion, we confirmed that reduction of <span class="hlt">sediment</span> organic load enabled an increase in the number of species, while the algal mats proved to be an important substrate in the lagoon environment for zoobenthic assemblages, especially when mat alternated with bare intermat areas of lagoon bed. <span class="hlt">Sediment</span> resuspension is confirmed as a management criterion for counteracting the effects of eutrophication and improving the biodiversity of zoobenthic assemblages in eutrophic lagoon</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS33B1708W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS33B1708W"><span>The Lithological Constraint To Gas Hydrate Formation: Evidence OF Grain Size Of <span class="hlt">Sediments</span> From IODP 311 On CASCADIA Margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, J.</p> <p>2006-12-01</p> <p>A total of 614 <span class="hlt">sediment</span> samples at intervals of about 1.5 m from all 5 sites of the Integrated Ocean Drilling Program (IODP) Expedition 311 on Cascadia Margin were analyzed using a Beckman Coulter LS-230 Particle Analyzer. The grain-size data were then plotted in depth and compared with other proxies of gas hydrate- occurrence such as soupy/mousse-like structures in <span class="hlt">sediments</span>, gas hydrate concentration (Sh) derived from LWD data using Archie's relation, IR core images (infrared image) and the <span class="hlt">recovered</span> samples of gas hydrate¨Cbearing <span class="hlt">sediments</span>. A good relationship between the distribution of coarse grains in size of 31-63¦Ìm and 63-125¦Ìm <span class="hlt">sediments</span> and the potential occurrence of gas hydrate was found across the entire gas hydrate stability <span class="hlt">zone</span>. The depth distribution of grain size from the Site U1326 shows clear excursions at depths of 5-8, 21-26, 50- 123, 132-140, 167-180, 195-206 and 220-240 mbsf, which coincide with the potential occurrence of gas hydrate suggested by soupy/mousse-like structures, logging-derived gas hydrate concentrations (Sh) and the <span class="hlt">recovered</span> samples of the gas hydrate¨Cbearing sand layers. The lithology of <span class="hlt">sediments</span> significantly affects the formation of gas hydrate. Gas hydrate forms preferentially within relatively coarse grain-size <span class="hlt">sediments</span> above 31 ¦Ìm. Key words: grain size of <span class="hlt">sediments</span>, constraint, occurrence of gas hydrate, IODP 311 IODP Expedition 311 Scientists: Michael Riedel (Co-chief Scientist), Timothy S. Collett (Co-chief Scientist), Mitchell Malone (Expedition Project Manager/Staff Scientist), Gilles Gu¨¨rin, Fumio Akiba, Marie-Madeleine Blanc-Valleron, Michelle Ellis, Yoshitaka Hashimoto, Verena Heuer, Yosuke Higashi, Melanie Holland, Peter D. Jackson, Masanori Kaneko, Miriam Kastner, Ji-Hoon Kim, Hiroko Kitajima, Philip E. Long, Alberto Malinverno, Greg Myers, Leena D. Palekar, John Pohlman, Peter Schultheiss, Barbara Teichert, Marta E. Torres, Anne M. Tr¨¦hu, Jiasheng Wang, Ulrich G. Wortmann, Hideyoshi</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014CorRe..33..733P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014CorRe..33..733P"><span>Historic impact of watershed change and <span class="hlt">sedimentation</span> to reefs along west-central Guam</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prouty, Nancy G.; Storlazzi, Curt D.; McCutcheon, Amanda L.; Jenson, John W.</p> <p>2014-09-01</p> <p>Using coral growth parameters (extension, density, calcification rates, and luminescence) and geochemical measurements (barium to calcium rations; Ba/Ca) from coral cores collected in west-central Guam, we provide a historic perspective on <span class="hlt">sediment</span> input to coral reefs adjacent to the Piti-Asan watershed. The months of August through December are dominated by increased coral Ba/Ca values, corresponding to the rainy season. With river water enriched in barium related to nearshore seawater, coral Ba/Ca ratios are presented as a proxy for input of fine-grained terrigenous <span class="hlt">sediment</span> to the nearshore environment. The century-long Ba/Ca coral record indicates that the Asan fore reef is within the <span class="hlt">zone</span> of impact from discharged <span class="hlt">sediments</span> transported from the Piti-Asan watershed and has experienced increased terrestrial <span class="hlt">sedimentation</span> since the 1940s. This abrupt shift in <span class="hlt">sedimentation</span> occurred at the same time as both the sudden denudation of the landscape by military ordinance and the immediate subsequent development of the Asan area through the end of the war, from 1944 through 1945. In response to rapid input of <span class="hlt">sediment</span>, as determined from coral Ba/Ca values, coral growth rates were reduced for almost two decades, while calcification rates <span class="hlt">recovered</span> much more quickly. Furthermore, coral luminescence is decoupled from the Ba/Ca record, which is consistent with degradation of soil organic matter through disturbance by forest fires, suggesting a potential index of fire history and degradation of soil organic matter. These patterns were not seen in the cores from nearby reefs associated with watersheds that have not undergone the same degree of landscape denudation. Taken together, these records provide a valuable tool for understanding the compounding effects of land-use change on coral reef health.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70104144','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70104144"><span>Historic impact of watershed change and <span class="hlt">sedimentation</span> to reefs along west-central Guam</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prouty, Nancy G.; Storlazzi, Curt D.; McCutcheon, Amanda L.; Jenson, John W.</p> <p>2014-01-01</p> <p>Using coral growth parameters (extension, density, calcification rates, and luminescence) and geochemical measurements (barium to calcium rations; Ba/Ca) from coral cores collected in west-central Guam, we provide a historic perspective on <span class="hlt">sediment</span> input to coral reefs adjacent to the Piti-Asan watershed. The months of August through December are dominated by increased coral Ba/Ca values, corresponding to the rainy season. With river water enriched in barium related to nearshore seawater, coral Ba/Ca ratios are presented as a proxy for input of fine-grained terrigenous <span class="hlt">sediment</span> to the nearshore environment. The century-long Ba/Ca coral record indicates that the Asan fore reef is within the <span class="hlt">zone</span> of impact from discharged <span class="hlt">sediments</span> transported from the Piti-Asan watershed and has experienced increased terrestrial <span class="hlt">sedimentation</span> since the 1940s. This abrupt shift in <span class="hlt">sedimentation</span> occurred at the same time as both the sudden denudation of the landscape by military ordinance and the immediate subsequent development of the Asan area through the end of the war, from 1944 through 1945. In response to rapid input of <span class="hlt">sediment</span>, as determined from coral Ba/Ca values, coral growth rates were reduced for almost two decades, while calcification rates <span class="hlt">recovered</span> much more quickly. Furthermore, coral luminescence is decoupled from the Ba/Ca record, which is consistent with degradation of soil organic matter through disturbance by forest fires, suggesting a potential index of fire history and degradation of soil organic matter. These patterns were not seen in the cores from nearby reefs associated with watersheds that have not undergone the same degree of landscape denudation. Taken together, these records provide a valuable tool for understanding the compounding effects of land-use change on coral reef health.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1000651-vadose-zone-microbiology','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1000651-vadose-zone-microbiology"><span>Vadose <span class="hlt">zone</span> microbiology</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kieft, Thomas L.; Brockman, Fred J.</p> <p>2001-01-17</p> <p>The vadose <span class="hlt">zone</span> is defined as the portion of the terrestrial subsurface that extends from the land surface downward to the water table. As such, it comprises the surface soil (the rooting <span class="hlt">zone</span>), the underlying subsoil, and the capillary fringe that directly overlies the water table. The unsaturated <span class="hlt">zone</span> between the rooting <span class="hlt">zone</span> and the capillary fringe is termed the "intermediate <span class="hlt">zone</span>" (Chapelle, 1993). The vadose <span class="hlt">zone</span> has also been defined as the unsaturated <span class="hlt">zone</span>, since the <span class="hlt">sediment</span> pores and/or rock fractures are generally not completely water filled, but instead contain both water and air. The latter characteristic results inmore » the term "<span class="hlt">zone</span> of aeration" to describe the vadose <span class="hlt">zone</span>. The terms "vadose <span class="hlt">zone</span>," "unsaturated <span class="hlt">zone</span>", and "<span class="hlt">zone</span> of aeration" are nearly synonymous, except that the vadose <span class="hlt">zone</span> may contain regions of perched water that are actually saturated. The term "subsoil" has also been used for studies of shallow areas of the subsurface immediately below the rooting <span class="hlt">zone</span>. This review focuses almost exclusively on the unsaturated region beneath the soil layer since there is already an extensive body of literature on surface soil microbial communities and process, e.g., Paul and Clark (1989), Metting (1993), Richter and Markowitz, (1995), and Sylvia et al. (1998); whereas the deeper strata of the unsaturated <span class="hlt">zone</span> have only recently come under scrutiny for their microbiological properties.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23987916','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23987916"><span>Benthic exchange and biogeochemical cycling in permeable <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huettel, Markus; Berg, Peter; Kostka, Joel E</p> <p>2014-01-01</p> <p>The sandy <span class="hlt">sediments</span> that blanket the inner shelf are situated in a <span class="hlt">zone</span> where nutrient input from land and strong mixing produce maximum primary production and tight coupling between water column and sedimentary processes. The high permeability of the shelf sands renders them susceptible to pressure gradients generated by hydrodynamic and biological forces that modulate spatial and temporal patterns of water circulation through these <span class="hlt">sediments</span>. The resulting dynamic three-dimensional patterns of particle and solute distribution generate a broad spectrum of biogeochemical reaction <span class="hlt">zones</span> that facilitate effective decomposition of the pelagic and benthic primary production products. The intricate coupling between the water column and <span class="hlt">sediment</span> makes it challenging to quantify the production and decomposition processes and the resultant fluxes in permeable shelf sands. Recent technical developments have led to insights into the high biogeochemical and biological activity of these permeable <span class="hlt">sediments</span> and their role in the global cycles of matter.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_9 --> <div id="page_10" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="181"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMEP24B..07A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMEP24B..07A"><span>Numerical Model of Turbulence, <span class="hlt">Sediment</span> Transport, and <span class="hlt">Sediment</span> Cover in a Large Canyon-Bound River</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alvarez, L. V.; Schmeeckle, M. W.</p> <p>2013-12-01</p> <p> during the High Flow Experiment (HFE) of 2008. The model accurately reproduces the size and position of the major recirculation currents, and the error in velocity magnitude was found to be less than 17% or 0.22 m/s absolute error. The mean deviation of the direction of velocity with respect to the measured velocity was found to be 20 degrees. Large-scale turbulence structures with vorticity predominantly in the vertical direction are produced at the shear layer between the main channel and the separation <span class="hlt">zone</span>. However, these structures rapidly become three-dimensional with no preferred orientation of vorticity. Surprisingly, cross-stream velocities, into the main recirculation <span class="hlt">zone</span> just upstream of the point of reattachment and out of the main recirculation region just downstream of the point of separation, are highest near the bed. Lateral separation eddies are more efficient at storing and exporting <span class="hlt">sediment</span> than previously modeled. The input of <span class="hlt">sediment</span> to the eddy recirculation <span class="hlt">zone</span> occurs near the reattachment <span class="hlt">zone</span> and is relatively continuous in time. While, the export of <span class="hlt">sediment</span> to the main channel by the return current occurs in pulses. Pulsation of the strength of the return current becomes a key factor to determine the rates of erosion and deposition in the main recirculation <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27267721','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27267721"><span>Effects of bottom water dissolved oxygen variability on copper and lead fractionation in the <span class="hlt">sediments</span> across the oxygen minimum <span class="hlt">zone</span>, western continental margin of India.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chakraborty, Parthasarathi; Chakraborty, Sucharita; Jayachandran, Saranya; Madan, Ritu; Sarkar, Arindam; Linsy, P; Nath, B Nagender</p> <p>2016-10-01</p> <p>This study describes the effect of varying bottom-water oxygen concentration on geochemical fractionation (operational speciation) of Cu and Pb in the underneath <span class="hlt">sediments</span> across the oxygen minimum <span class="hlt">zone</span> (Arabian Sea) in the west coast of India. Both, Cu and Pb were redistributed among the different binding phases of the <span class="hlt">sediments</span> with changing dissolved oxygen level (from oxic to hypoxic and close to suboxic) in the bottom water. The average lability of Cu-<span class="hlt">sediment</span> complexes gradually decreased (i.e., stability increased) with the decreasing dissolved oxygen concentrations of the bottom water. Decreasing bottom-water oxygen concentration increased Cu association with sedimentary organic matter. However, Pb association with Fe/Mn-oxyhydroxide phases in the <span class="hlt">sediments</span> gradually decreased with the decreasing dissolved oxygen concentration of the overlying bottom water (due to dissolution of Fe/Mn oxyhydroxide phase). The lability of Pb-<span class="hlt">sediment</span> complexes increased with the decreasing bottom-water oxygen concentration. This study suggests that bottom-water oxygen concentration is one of the key factors governing stability and lability of Cu and Pb complexes in the underneath <span class="hlt">sediment</span>. Sedimentary organic matter and Fe/Mn oxyhydroxide binding phases were the major hosting phases for Cu and Pb respectively in the study area. Increasing lability of Pb-complexes in bottom <span class="hlt">sediments</span> may lead to positive benthic fluxes of Pb at low oxygen environment. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Ocgy...58..240P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Ocgy...58..240P"><span><span class="hlt">Sediment</span> Flux of Particulate Organic Phosphorus in the Open Black Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parkhomenko, A. V.; Kukushkin, A. S.</p> <p>2018-03-01</p> <p>The interannual variation of the monthly average (weighted average) concentrations of particulate organic phosphorus (PPOM) in the photosynthetic layer, oxycline, redox <span class="hlt">zone</span>, and H2S <span class="hlt">zone</span> in the open Black Sea is estimated based on long-term observation data. The suspension <span class="hlt">sedimentation</span> rates from the studied layers are assessed using model calculations and published data. The annual variation of PPOM <span class="hlt">sediment</span> fluxes from the photosynthetic layer, oxycline, redox <span class="hlt">zone</span>, and upper H2S <span class="hlt">zone</span> to the anaerobic <span class="hlt">zone</span> of the sea and the correspondingly annual average values are estimated for the first time. A regular decrease in the PPOM annual average flux with depth in the upper active layer is demonstrated. A correlation between the annual average values of PPOM <span class="hlt">sediment</span> flux from the photosynthetic layer and ascending phosphate flux to this layer is shown, which suggests their balance in the open sea. The results are discussed in terms of the phosphorus biogeochemical cycle and the concept of new and regenerative primary production in the open Black Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAESc.160..200B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAESc.160..200B"><span>Unravelling the stratigraphy and <span class="hlt">sedimentation</span> history of the uppermost Cretaceous to Eocene <span class="hlt">sediments</span> of the Kuching <span class="hlt">Zone</span> in West Sarawak (Malaysia), Borneo</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Breitfeld, H. Tim; Hall, Robert; Galin, Thomson; BouDagher-Fadel, Marcelle K.</p> <p>2018-07-01</p> <p>The Kuching <span class="hlt">Zone</span> in West Sarawak consists of two different sedimentary basins, the Kayan and Ketungau Basins. The sedimentary successions in the basins are part of the Kuching Supergroup that extends into Kalimantan. The uppermost Cretaceous (Maastrichtian) to Lower Eocene Kayan Group forms the sedimentary deposits directly above a major unconformity, the Pedawan Unconformity, which marks the cessation of subduction-related magmatism beneath SW Borneo and the Schwaner Mountains, due to termination of the Paleo-Pacific subduction. The successions consist of the Kayan and Penrissen Sandstones and are dominated by fluvial channels, alluvial fans and floodplain deposits with some deltaic to tidally-influenced sections in the Kayan Sandstone. In the late Early or early Middle Eocene, <span class="hlt">sedimentation</span> in this basin ceased and a new basin, the Ketungau Basin, developed to the east. This change is marked by the Kayan Unconformity. <span class="hlt">Sedimentation</span> resumed in the Middle Eocene (Lutetian) with the marginal marine, tidal to deltaic Ngili Sandstone and Silantek Formation. Upsequence, the Silantek Formation is dominated by floodplain and subsidiary fluvial deposits. The Bako-Mintu Sandstone, a potential lateral equivalent of the Silantek Formation, is formed of major fluvial channels. The top of the Ketungau Group in West Sarawak is formed by the fluvially-dominated Tutoop Sandstone. This shows a transition of the Ketungau Group in time towards terrestrial/fluvially-dominated deposits. Paleocurrent measurements show river systems were complex, but reveal a dominant southern source. This suggests uplift of southern Borneo initiated in the region of the present-day Schwaner Mountains from the latest Cretaceous onwards. Additional sources were local sources in the West Borneo province, Mesozoic melanges to the east and potentially the Malay Peninsula. The Ketungau Group also includes reworked deposits of the Kayan Group. The <span class="hlt">sediments</span> of the Kuching Supergroup are predominantly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43.7114M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43.7114M"><span>Quantifying manganese and nitrogen cycle coupling in manganese-rich, organic carbon-starved marine <span class="hlt">sediments</span>: Examples from the Clarion-Clipperton fracture <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mogollón, José M.; Mewes, Konstantin; Kasten, Sabine</p> <p>2016-07-01</p> <p>Extensive deep-sea sedimentary areas are characterized by low organic carbon contents and thus harbor suboxic sedimentary environments where secondary (autotrophic) redox cycling becomes important for microbial metabolic processes. Simulation results for three stations in the Eastern Equatorial Pacific with low organic carbon content (<0.5 dry wt %) and low <span class="hlt">sedimentation</span> rates (10-1-100 mm ky-1) show that ammonium generated during organic matter degradation may act as a reducing agent for manganese oxides below the oxic <span class="hlt">zone</span>. Likewise, at these sedimentary depths, dissolved reduced manganese may act as a reducing agent for oxidized nitrogen species. These manganese-coupled transformations provide a suboxic conversion pathway of ammonium and nitrate to dinitrogen. These manganese-nitrogen interactions further explain the presence and production of dissolved reduced manganese (up to tens of μM concentration) in <span class="hlt">sediments</span> with high nitrate (>20 μM) concentrations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1991GeCoA..55.2067K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991GeCoA..55.2067K"><span>Novel pyropheophorbide steryl esters in Black Sea <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>King, Linda L.; Repeta, Daniel J.</p> <p>1991-07-01</p> <p>A series of non-polar chlorophyll degradation products (NPCs) with greater than 10 components has been isolated from Black Sea <span class="hlt">sediment</span> and identified as pyropheophorbide steryl esters by visible and mass spectrometry. These compounds have been previously observed in seawater and <span class="hlt">sediment</span> trap samples, and may be formed during grazing of phytoplankton by zooplanktonic herbivores. In Black Sea <span class="hlt">sediments</span>, NPCs constitute 14% of the total phorbins determined spectroscopically at 660 nm, and 39% of the total chlorophyll degradation products measured by high pressure liquid chromatography. NPCs therefore constitute a significant sedimentary sink for chlorophyll. The distribution of sterols released by hydrolysis of NPCs most closely resembles sterols in suspended particulate matter collected from the euphotic <span class="hlt">zone</span> and is quite different from the distribution of solvent-extractable sterols in <span class="hlt">sediments</span>. Sterols extracted from <span class="hlt">sediments</span> have high concentrations of 4-methylsterols and high stanol/stenol ratios. NPC-derived sterols have very low concentrations of 4-methylsterols and low stanol/stenol ratios. We suggest that these differences reflect an enhanced preservation of NPCs in <span class="hlt">sediments</span> relative to free sterols and phorbins. As a result, the original production of sterols in the euphotic <span class="hlt">zone</span> may be more closely approximated by the distribution of NPC-derived sterols than by the distribution of free sterols in <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033196','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033196"><span>Metalliferous <span class="hlt">sediment</span> and a silica-hematite deposit within the Blanco fracture <span class="hlt">zone</span>, Northeast Pacific</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hein, J.R.; Clague, D.A.; Koski, R.A.; Embley, R.W.; Dunham, R.E.</p> <p>2008-01-01</p> <p>A Tiburon ROV dive within the East Blanco Depression (EBD) increased the mapped extent of a known hydrothermal field by an order of magnitude. In addition, a unique opal-CT (cristobalite-tridymite)-hematite mound was discovered, and mineralized <span class="hlt">sediments</span> and rock were collected and analyzed. Silica-hematite mounds have not previously been found on the deep ocean floor. The light-weight rock of the porous mound consists predominantly of opal-CT and hematite filaments, rods, and strands, and averages 77.8% SiO2 and 11.8% Fe2O3. The hematite and opal-CT precipitated from a low-temperature (???115?? C), strongly oxidized, silica- and iron-rich, sulfur-poor hydrothermal fluid; a bacterial mat provided the framework for precipitation. Samples collected from a volcaniclastic rock outcrop consist primarily of quartz with lesser plagioclase, smectite, pyroxene, and sulfides; SiO2 content averages 72.5%. Formation of these quartz-rich samples is best explained by cooling in an up-flow <span class="hlt">zone</span> of silica-rich hydrothermal fluids within a low permeability system. Opal-A, opal-CT, and quartz mineralization found in different places within the EBD hydrothermal field likely reflects decreasing silica saturation and increasing temperature of the mineralizing fluid with increasing silica crystallinity. Six push cores <span class="hlt">recovered</span> gravel, coarse sand, and mud mineralized variously by Fe or Mn oxides, silica, and sulfides. Total rare-earth element concentrations are low for both the rock and push core samples. Ce and Eu anomalies reflect high and low temperature hydrothermal components and detrital phases. A remarkable variety of types of mineralization occur within the EBD field, yet a consistent suite of elements is enriched (relative to basalt and unmineralized cores) in all samples analyzed: Ag, Au, S, Mo, Hg, As, Sb, Sr, and U; most samples are also enriched in Cu, Pb, Cd, and Zn. On the basis of these element enrichments, the EBD hydrothermal field might best be described as a base</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001AGUFMGP41A0238K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001AGUFMGP41A0238K"><span>Magnetic Hysteresis of Deep-Sea <span class="hlt">Sediments</span> in Korea Deep Ocean Study(KODOS) Area, NE Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, K.; Park, C.; Yoo, C.</p> <p>2001-12-01</p> <p>The KODOS area within the Clarion-Clipperton fracture <span class="hlt">zone</span> (C-C <span class="hlt">zone</span>) is surrounded by the Hawaiian and Line Island Ridges to the west and the central American continent to the east. Topography of the seafloor consists of flat-topped abyssal hills and adjacent abyssal troughs, both of which run parallel in N-S direction. <span class="hlt">Sediments</span> from the study area consist mainly of biogenic <span class="hlt">sediments</span>. Latitudinal zonation of sedimentary facies was caused by the accumulation of biogenic materials associated with the equatorial current system and movement of the Pacific plate toward the north or northwest. The KODOS area belongs to the latitudinal transition <span class="hlt">zone</span> having depositional characteristics between non-fossiliferous pelagic clay-dominated <span class="hlt">zone</span> and calcareous <span class="hlt">sediment</span>-dominated <span class="hlt">zone</span>. The box core <span class="hlt">sediments</span> of the KODOS area are analyzed in an attempt to obtain magnetic hysteresis information and to elucidate the relationship between hysteresis property and lithological facies. Variations in magnetic hysteresis parameters with unit layers reflect the magnetic grain-size and concentrations within the <span class="hlt">sediments</span>. The ratios of remanant coercivity/coercive force (Hcr/Hc) and saturation remnance/saturation magnetization (Mrs/Ms) indicate that coarse magnetic grains are mainly distributed in dark brown <span class="hlt">sediments</span> (lower part of the <span class="hlt">sediment</span> core samples) reflecting high Hcr/Hc and low Mrs/Ms ratios. These results are mainly caused by dissolution differences with core depth. From the plotting of the ratios of hyteresis parameters, it is indicated that magnetic minerals in cubic samples are in pseudo-single domain (PSD) state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP21A1825G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP21A1825G"><span>The spatial distribution of major and trace elements in the surface <span class="hlt">sediments</span> from the northeastern Beibu Gulf, South China Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ge, Q.; Xue, Z. G.</p> <p>2017-12-01</p> <p>Major and trace elements contents and grain size were analyzed for surface <span class="hlt">sediments</span> retrieved from the northeastern Beibu (Tonkin) Gulf. The study area was divided into four <span class="hlt">zones</span>: <span class="hlt">Zone</span> I locates in the northeastern coastal area of the gulf, which received large amount of the fluvial materials from local rivers; <span class="hlt">Zone</span> II locates in the center of the study area, where surface <span class="hlt">sediments</span> is from multiple sources; <span class="hlt">Zone</span> III locates in the Qiongzhou Strait, which is dominated by material from the Pearl River and Hainan Island; <span class="hlt">Zone</span> IV locates in the southwest of the study area, and the <span class="hlt">sediments</span> mainly originated from the Red River. Statistical analyses of <span class="hlt">sediment</span> geochemical characteristics reveal that grain size is the leading factor for elementary distribution, which is also influenced by hydrodynamics, mineral composition of terrigenous <span class="hlt">sediments</span>, anthropogenic activity, and authigenic components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032961','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032961"><span>Methane hydrate formation in turbidite <span class="hlt">sediments</span> of northern Cascadia, IODP Expedition 311</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Torres, M.E.; Trehu, A.M.; Cespedes, N.; Kastner, M.; Wortmann, U.G.; Kim, J.-H.; Long, P.; Malinverno, A.; Pohlman, J.W.; Riedel, M.; Collett, T.</p> <p>2008-01-01</p> <p>Expedition 311 of the Integrated Ocean Drilling Program (IODP) to northern Cascadia <span class="hlt">recovered</span> gas-hydrate bearing <span class="hlt">sediments</span> along a SW-NE transect from the first ridge of the accretionary margin to the eastward limit of gas-hydrate stability. In this study we contrast the gas gas-hydrate distribution from two sites drilled ~ 8??km apart in different tectonic settings. At Site U1325, drilled on a depositional basin with nearly horizontal sedimentary sequences, the gas-hydrate distribution shows a trend of increasing saturation toward the base of gas-hydrate stability, consistent with several model simulations in the literature. Site U1326 was drilled on an uplifted ridge characterized by faulting, which has likely experienced some mass wasting events. Here the gas hydrate does not show a clear depth-distribution trend, the highest gas-hydrate saturation occurs well within the gas-hydrate stability <span class="hlt">zone</span> at the shallow depth of ~ 49??mbsf. <span class="hlt">Sediments</span> at both sites are characterized by abundant coarse-grained (sand) layers up to 23??cm in thickness, and are interspaced within fine-grained (clay and silty clay) detrital <span class="hlt">sediments</span>. The gas-hydrate distribution is punctuated by localized depth intervals of high gas-hydrate saturation, which preferentially occur in the coarse-grained horizons and occupy up to 60% of the pore space at Site U1325 and > 80% at Site U1326. Detailed analyses of contiguous samples of different lithologies show that when enough methane is present, about 90% of the variance in gas-hydrate saturation can be explained by the sand (> 63????m) content of the <span class="hlt">sediments</span>. The variability in gas-hydrate occupancy of sandy horizons at Site U1326 reflects an insufficient methane supply to the <span class="hlt">sediment</span> section between 190 and 245??mbsf. ?? 2008 Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29934827','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29934827"><span>Modeling of <span class="hlt">sediment</span> transport in a saltwater lake with supplemental sandy freshwater.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liang, Li; Deng, Yun; Li, Ran; Li, Jia</p> <p>2018-06-22</p> <p>Considering the highly complex flow structure of saltwater lakes during freshwater supplementation, a three-dimensional numerical model was developed to simulate suspended <span class="hlt">sediment</span> transport in saltwater lakes. The model was validated using measurements of the salinity and <span class="hlt">sediment</span> concentration during a pumping test at Yamdrok Lake. The simulation results were in quantitative agreement with the measured data. The observed and simulated results also indicated that the wind stress and vertical salinity gradient have a significant influence on salinity and <span class="hlt">sediment</span> transport in a saltwater lake. The validated model was then used to predict and analyze the contributions of wind, the supplement flow rate and salinity stratification to the <span class="hlt">sediment</span> transport process in Yamdrok Lake during continuous river water supplementation. The simulation results showed that after the sandy river water was continuously discharged into the saltwater lake, the lateral diffusion trends of the <span class="hlt">sediment</span> exhibited three stages: linear growth in the inflow direction, logarithmic growth in the wind direction, and stabilization. Furthermore, wind was the dominant factor in driving the lake flow pattern and <span class="hlt">sediment</span> transport. Specifically, wind can effectively reduce the area of the <span class="hlt">sediment</span> diffusion <span class="hlt">zone</span> by increasing the lateral <span class="hlt">sediment</span> carrying and dilution capacities. The effect of inflow on the lake current is negligible, but the extent of the <span class="hlt">sediment</span> turbidity <span class="hlt">zone</span> mainly depends on the inflow. Reducing the inflow discharge can decrease the area of the <span class="hlt">sediment</span> turbidity <span class="hlt">zone</span> to proportions that far exceed the proportions of inflow discharge reductions. In addition, the high-salinity lake water can support the supplemented freshwater via buoyancy forces, which weaken vertical mixing and <span class="hlt">sediment</span> settlement and increase lake currents and <span class="hlt">sediment</span> diffusion near the surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMEP53A0925W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMEP53A0925W"><span>Characteristics of Holocene <span class="hlt">sediments</span> in the Gunsan Basin, central Yellow Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Woo, H. J.; Huh, S.; Jeong, K. S.; Lee, J. H.; Ham, A.; Kang, J.</p> <p>2016-12-01</p> <p>The Gunsan Basin, in the eastern part of the South Yellow Sea Basin, is filled by terrestrial sedimentary rocks, maximally up to 8 km deep on the basement of metamorphic rocks that constitutes the Yangtze Platform. The uppermost sedimentary layer (generally less than 1 km) appears to have formed experiencing the repeated marine environments since the middle Miocene. This study is to investigate the characteristics of Holocene <span class="hlt">sediments</span> in the Gunsan Basin, based on interpretation of core <span class="hlt">sediments</span> and high-resolution shallow (Sparker and Chirp) seismic profiles. The surface <span class="hlt">sediments</span> in the basin consist of sand (56.6% on the average), silt (18.4%), and clay (25.0%) with a mean grain size of 1.5 to 7.8 Ø. Sand is prevalent (63.8 to 98.3%) in and around the Yellow Sea Trough lying in the eastern part of the basin. The sandy <span class="hlt">sediments</span> are regarded as relict <span class="hlt">sediments</span> deposited in the last glacial maximum (LGM). The sedimentary environments are classified, based on the acoustic and morphological characters of high-resolution shallow (Sparker and Chirp) seismic profiles, into mud <span class="hlt">zone</span>, deformed <span class="hlt">zone</span>, and sand ridges with sand waves <span class="hlt">zone</span> from the west to the east in the Gunsan Basin. The deformed <span class="hlt">zone</span> in the central Yellow Sea is a mixing area of <span class="hlt">sediments</span> derived from China and Korea, where there are a number of paleochannels and erosional surfaces in the direction of northwest-southeast. The deformed <span class="hlt">zone</span> represents non-deposition or erosion in the central Yellow Sea during the Holocene. Tidal sand ridges and sand waves are well developed along the coast of Korea. Modern sand ridges are generally moving in the northeast-southwest direction, which coincide with dominant tidal current direction. Fifteen piston cores were collected in the basin to investigate the general geological characters of the marine sedimentary sequence. In comparison with three cores in the southern basin, the sand contents tend to increase in the direction of east. 14C dates from three cores</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1337875-stability-normal-zone-propagation-ybco-corc-cables','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1337875-stability-normal-zone-propagation-ybco-corc-cables"><span>Stability and normal <span class="hlt">zone</span> propagation in YBCO CORC cables</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Majoros, M.; Sumption, M. D.; Collings, E. W.; ...</p> <p>2016-03-11</p> <p>In this study, a two layer conductor on round core cable was tested for stability and normal <span class="hlt">zone</span> propagation at 77 K in a liquid nitrogen bath. The cable was instrumented with voltage taps and wires on each strand over the cable’s central portion (i.e. excluding the end connections of the cable with the outside world). A heater was placed in the central <span class="hlt">zone</span> on the surface of the cable, which allowed pulses of various powers and durations to be generated. Shrinking (<span class="hlt">recovering</span>) and expanding (not <span class="hlt">recovering</span>) normal <span class="hlt">zones</span> have been detected, as well as stationary <span class="hlt">zones</span> which were inmore » thermal equilibrium. Such stationary thermal equilibrium <span class="hlt">zones</span> did not expand or contract, and hit a constant upper temperature while the heater current persisted; they are essentially a form of Stekly stability. Overall, the cable showed a high degree of stability. Notably, it was able to carry a current of 0.45I c cable with maximum temperature of 123 K for one minute without damage.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1415086-effect-water-chemistry-hydrodynamics-nitrogen-transformation-activity-microbial-community-functional-potential-hyporheic-zone-sediment-columns','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1415086-effect-water-chemistry-hydrodynamics-nitrogen-transformation-activity-microbial-community-functional-potential-hyporheic-zone-sediment-columns"><span>Effect of Water Chemistry and Hydrodynamics on Nitrogen Transformation Activity and Microbial Community Functional Potential in Hyporheic <span class="hlt">Zone</span> <span class="hlt">Sediment</span> Columns</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Liu, Yuanyuan; Liu, Chongxuan; Nelson, William C.</p> <p></p> <p>Nitrogen (N) transformation in hyporheic <span class="hlt">zone</span> (HZ) is an important component in N-cycling in ecosystems. A column study was conducted to investigate N transformation in a HZ <span class="hlt">sediment</span> with a focus on how characteristic HZ properties including water chemistry, fluid residence time, and dynamic groundwater and surface water exchange affect on N transformation. Metagenomic and quantitative polymerase chain reaction (qPCR) analyses were performed to evaluate the dynamic changes in microbial community structure and its function in response to N transformation. The results indicated that N transformation in the HZ <span class="hlt">sediment</span> was collectively controlled by microbial community functions including: denitrification, dissimilatorymore » nitrate reduction to ammonium (DNRA), nitrification, and anaerobic ammonium oxidation (anammox). However, the spatial distribution of the microbial community functions and associated biogeochemical reaction rates and products changed quickly in response to experimental perturbation, and was influenced by various factors including water chemistry (dissolved O2 and N species), desorption of <span class="hlt">sediment</span> associated organic carbon, ion exchange reactions of NH4+, and fluid residence time. The results of this study implied that the microbial community in the HZ would exhibit strong function zonation along N and O gradients, which in turn would control the rates and products of N transformation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913823H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913823H"><span>Is DOM driver of the microbial carrying capacity in pristine porous groundwater ecosystems? - lab-scale experiments in 2D <span class="hlt">sediment</span> flow-through microcosms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hofmann, Roland; Griebler, Christian</p> <p>2017-04-01</p> <p>Groundwater ecosystems are an essential resource for drinking water and at the same time constitute fascinating habitats subject to increasing (anthropogenic) disturbances. In our research, we look for ways to qualitatively and quantitatively access, and predict the resistance and resilience (potential) of groundwater ecosystems in consequence of selected disturbances. As a central goal we hope to identify and quantify the underlying biological and ecological key drivers of the microbial Carrying Capacity (mCC) - an ecological concept established in macro-ecology - we assume directly connected to the ecosystem's productivity and the resistance and resilience of aquifers. We further hypothesize, that the ecosystems' mCC is a result of available energy and constitutes a promising proxy for the potential of groundwater ecosystems to withstand impacts and <span class="hlt">recover</span> from it. In a first approach we studied the dynamics of the microbial standing stock (biomass) and growth (productivity) productivity of a natural groundwater microbial community in parallel 2-D <span class="hlt">sediment</span> flow-through systems. Selected <span class="hlt">zones</span> of the model aquifers were disturbed by elevated DOM concentrations. Both the 'mobile' (free floating) and 'sessile' (<span class="hlt">sediment</span> attached) microbial components were followed over time in terms of biomass, growth, and specific activities (ATP, carbon use efficiency) and taxonomic composition. <span class="hlt">Sediment</span> regions supplied with elevated concentrations of natural DOM showed increased biomass, activities and taxonomic richness with the <span class="hlt">sediment</span> community, while differences in the mobile microbial were marginal. Specifically, the carbon use efficiency was significantly increased in the DOM amended <span class="hlt">sediment</span> <span class="hlt">zones</span>. In contrast, the microbial community that received the mainly refractory natural background DOM was able to metabolize polymers more efficiently in substrate use tests (ECOLOG), seen as an adaptation to the energy-poor subsurface. Quasi-stationary conditions were reached in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918342H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918342H"><span>Glacimarine <span class="hlt">sedimentation</span> in Petermann Fjord and Nares Strait, NW Greenland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hogan, Kelly; Jakobsson, Martin; Mayer, Larry; Mix, Alan; Nielsen, Tove; Kamla, Elina; Reilly, Brendan; Heirman, Katrina An; Stranne, Christian; Mohammed, Rezwan; Eriksson, Bjorn; Jerram, Kevin</p> <p>2017-04-01</p> <p>Here we build on preliminary results from 6500 line-km of high-resolution chirp sub-bottom profiles (2-7 kHz) acquired in Petermann Fjord and Nares Strait during the Petermann 2015 Expedition of the Swedish icebreaker Oden. We map the unlithified <span class="hlt">sediment</span> cover in Peterman Fjord, which consists of up to 3 conformable "drape" units and calculate volumes of this assumed "post-glacial" fill. In Nares Strait we have mapped <span class="hlt">sediment</span> volumes in local basins just beyond the sill at the Petermann Fjord-mouth: do these <span class="hlt">sediments</span> represent material flushed out from the grounding <span class="hlt">zone</span> of Petermann Glacier when it was grounded at the sill? In this vein, and interestingly, some of the thickest <span class="hlt">sediments</span> that we observe are found close to a grounding-<span class="hlt">zone</span> wedge (GZW) in Nares Strait that represents a former grounding <span class="hlt">zone</span> of ice retreating southwards through the strait. We also map conformable units across Nares Strait and consider the similarities between these and the <span class="hlt">sediment</span> units in the fjord. Do the strong reflections between the units represent the same climatic, oceanographic or process-shift both inside and outside the fjord? We also aim to tie our new acoustic stratigraphy to <span class="hlt">sediment</span>-core data (lithofacies, dates) and, therefore, to comment on the age of the mapped <span class="hlt">sediment</span> units and present ideas on the glacimarine flux of material to the Petermann-Nares system. Primary <span class="hlt">sediment</span> delivery to the seafloor in this environment is thought to be predominantly through <span class="hlt">sedimentation</span> from meltwater plumes but also of iceberg-rafted debris (IRD). However, <span class="hlt">sediment</span> redeposition by slope failures on a variety of scales also occurs and has focussed <span class="hlt">sediments</span> into discrete basins where the seafloor is rugged. This work - which aims to relate past <span class="hlt">sediment</span>, meltwater and iceberg fluxes to changes in climate - will help us to identify how the system has responded to a past global warming event, namely the last deglaciation. This is particularly relevant in light of the recent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28503172','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28503172"><span>Hydrocarbon Degradation in Caspian Sea <span class="hlt">Sediment</span> Cores Subjected to Simulated Petroleum Seepage in a Newly Designed <span class="hlt">Sediment</span>-Oil-Flow-Through System.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mishra, Sonakshi; Wefers, Peggy; Schmidt, Mark; Knittel, Katrin; Krüger, Martin; Stagars, Marion H; Treude, Tina</p> <p>2017-01-01</p> <p>The microbial community response to petroleum seepage was investigated in a whole round <span class="hlt">sediment</span> core (16 cm length) collected nearby natural hydrocarbon seepage structures in the Caspian Sea, using a newly developed <span class="hlt">Sediment</span>-Oil-Flow-Through (SOFT) system. Distinct redox <span class="hlt">zones</span> established and migrated vertically in the core during the 190 days-long simulated petroleum seepage. Methanogenic petroleum degradation was indicated by an increase in methane concentration from 8 μM in an untreated core compared to 2300 μM in the lower sulfate-free <span class="hlt">zone</span> of the SOFT core at the end of the experiment, accompanied by a respective decrease in the δ 13 C signal of methane from -33.7 to -49.5‰. The involvement of methanogens in petroleum degradation was further confirmed by methane production in enrichment cultures from SOFT <span class="hlt">sediment</span> after the addition of hexadecane, methylnapthalene, toluene, and ethylbenzene. Petroleum degradation coupled to sulfate reduction was indicated by the increase of integrated sulfate reduction rates from 2.8 SO 4 2- m -2 day -1 in untreated cores to 5.7 mmol SO 4 2- m -2 day -1 in the SOFT core at the end of the experiment, accompanied by a respective accumulation of sulfide from 30 to 447 μM. Volatile hydrocarbons (C2-C6 n -alkanes) passed through the methanogenic <span class="hlt">zone</span> mostly unchanged and were depleted within the sulfate-reducing <span class="hlt">zone</span>. The amount of heavier n -alkanes (C10-C38) decreased step-wise toward the top of the <span class="hlt">sediment</span> core and a preferential degradation of shorter (<C14) and longer chain n -alkanes (>C30) was seen during the seepage. This study illustrates, to the best of our knowledge, for the first time the development of methanogenic petroleum degradation and the succession of benthic microbial processes during petroleum passage in a whole round <span class="hlt">sediment</span> core.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5409261','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5409261"><span>Hydrocarbon Degradation in Caspian Sea <span class="hlt">Sediment</span> Cores Subjected to Simulated Petroleum Seepage in a Newly Designed <span class="hlt">Sediment</span>-Oil-Flow-Through System</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Mishra, Sonakshi; Wefers, Peggy; Schmidt, Mark; Knittel, Katrin; Krüger, Martin; Stagars, Marion H.; Treude, Tina</p> <p>2017-01-01</p> <p>The microbial community response to petroleum seepage was investigated in a whole round <span class="hlt">sediment</span> core (16 cm length) collected nearby natural hydrocarbon seepage structures in the Caspian Sea, using a newly developed <span class="hlt">Sediment</span>-Oil-Flow-Through (SOFT) system. Distinct redox <span class="hlt">zones</span> established and migrated vertically in the core during the 190 days-long simulated petroleum seepage. Methanogenic petroleum degradation was indicated by an increase in methane concentration from 8 μM in an untreated core compared to 2300 μM in the lower sulfate-free <span class="hlt">zone</span> of the SOFT core at the end of the experiment, accompanied by a respective decrease in the δ13C signal of methane from -33.7 to -49.5‰. The involvement of methanogens in petroleum degradation was further confirmed by methane production in enrichment cultures from SOFT <span class="hlt">sediment</span> after the addition of hexadecane, methylnapthalene, toluene, and ethylbenzene. Petroleum degradation coupled to sulfate reduction was indicated by the increase of integrated sulfate reduction rates from 2.8 SO42-m-2 day-1 in untreated cores to 5.7 mmol SO42-m-2 day-1 in the SOFT core at the end of the experiment, accompanied by a respective accumulation of sulfide from 30 to 447 μM. Volatile hydrocarbons (C2–C6 n-alkanes) passed through the methanogenic <span class="hlt">zone</span> mostly unchanged and were depleted within the sulfate-reducing <span class="hlt">zone</span>. The amount of heavier n-alkanes (C10–C38) decreased step-wise toward the top of the <span class="hlt">sediment</span> core and a preferential degradation of shorter (<C14) and longer chain n-alkanes (>C30) was seen during the seepage. This study illustrates, to the best of our knowledge, for the first time the development of methanogenic petroleum degradation and the succession of benthic microbial processes during petroleum passage in a whole round <span class="hlt">sediment</span> core. PMID:28503172</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T51A4564J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T51A4564J"><span>Elastic Properties of Subduction <span class="hlt">Zone</span> Materials in the Large Shallow Slip Environment for the Tohoku 2011 Earthquake: Laboratory data from JFAST Core Samples</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeppson, T.; Tobin, H. J.</p> <p>2014-12-01</p> <p>The 11 March 2011 Tohoku-Oki earthquake (Mw=9.0) produced large displacements of ~50 meters near the Japan Trench. In order to understand earthquake propagation and slip stabilization in this environment, quantitative values of the real elastic properties of fault <span class="hlt">zones</span> and their surrounding wall rock material is crucial. Because elastic and mechanical properties of faults and wallrocks are controlling factors in fault strength, earthquake generation and propagation, and slip stabilization, an understanding of these properties and their depth dependence is essential to understanding and accurately modeling earthquake rupture. In particular, quantitatively measured S-wave speeds, needed for estimation of elastic properties, are scarce in the literature. We report laboratory ultrasonic velocity measurements performed at elevated pressures, as well as the calculated dynamic elastic moduli, for samples of the rock surrounding the Tohoku earthquake principal fault <span class="hlt">zone</span> <span class="hlt">recovered</span> by drilling during IODP Expedition 343, Japan Trench Fast Drilling Project (JFAST). We performed measurements on five samples of gray mudstone from the hanging wall and one sample of underthrust brown mudstone from the footwall. We find P- and S-wave velocities of 2.0 to 2.4 km/s and 0.7 to 1.0 km/s, respectively, at 5 MPa effective pressure. At the same effective pressure, the hanging wall samples have shear moduli ranging from 1.4 to 2.2 GPa and the footwall sample has a shear modulus of 1.0 GPa. While these values are perhaps not surprising for shallow, clay-rich subduction <span class="hlt">zone</span> <span class="hlt">sediments</span>, they are substantially lower than the 30 GPa commonly assumed for rigidity in earthquake rupture and propagation models [e.g., Ide et al., 1993; Liu and Rice, 2005; Loveless and Meade, 2011]. In order to better understand the elastic properties of shallow subduction <span class="hlt">zone</span> <span class="hlt">sediments</span>, our measurements from the Japan Trench are compared to similar shallow drill core samples from the Nankai Trough, Costa Rica</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1715841C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715841C"><span>Seasonal herbicide monitoring in soil, runoff and <span class="hlt">sediments</span> of an olive orchard under conventional tillage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calderón, Maria Jesus; de Luna, Elena; Gómez, José Alfonso; Cornejo, Juan; Hermosín, M. Carmen</p> <p>2015-04-01</p> <p>Several pollution episodes in surface and groundwaters with pesticides have occurred in areas where olive crops are established. For that reason, it is necessary to know the evolution of some pesticides in olive trees plantation depending on their seasonal application. This is especially important when conventional tillage is used. A monitoring of two herbicides (terbuthylazine and oxyfluorfen)in the first cm of soil and, in runoff and <span class="hlt">sediment</span> yield was carried out after several rainfall events. The rainfall occurred during the study was higher in winter than in spring giving rise more runoff in winter. However, no differences in <span class="hlt">sediment</span> yields were observed between spring and winter. Terbuthylazine depletion from soil is associated to the first important rainfall events in both seasons (41 mm in spring and 30 mm in winter). At the end of the experiment, no terbuthylazine soil residues were <span class="hlt">recovered</span> in winter whereas 15% of terbuthylazine applied remained in spring. Oxyfluorfen showed a character more persistent than terbuthylazine remaining 48% of the applied at the end of the experiment due to its low water solubility. Higher percentage from the applied of terbuthylazine was <span class="hlt">recovered</span> in runoff in winter (0.55%) than in spring (0.17%). Nevertheless, no differences in terbuthylazine <span class="hlt">sediments</span> yields between both seasons were observed. That is in agreement with the values of runoff and <span class="hlt">sediment</span> yields accumulated in tanks in both seasons. Due to the low water solubility of oxyfluorfen very low amount of this herbicide was <span class="hlt">recovered</span> in runoff. Whereas, in <span class="hlt">sediment</span> yields the 39.5% of the total applied was <span class="hlt">recovered</span>. These data show that the dissipation of terbuthylazine from soil is closely related with leaching processes and in less extent with runoff. However, oxyfluorfen dissipation is more affected by runoff processes since this herbicide is co-transported in <span class="hlt">sediment</span> yields. Keywords: olive crop, pesticide, runoff, <span class="hlt">sediments</span>, surface water, groundwater</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B21C0463K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B21C0463K"><span>Identifying and Quantifying Chemical Forms of <span class="hlt">Sediment</span>-Bound Ferrous Iron.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kohler, M.; Kent, D. B.; Bekins, B. A.; Cozzarelli, I.; Ng, G. H. C.</p> <p>2015-12-01</p> <p>Aqueous Fe(II) produced by dissimilatory iron reduction comprises only a small fraction of total biogenic Fe(II) within an aquifer. Most biogenic Fe(II) is bound to <span class="hlt">sediments</span> on ion exchange sites; as surface complexes and, possibly, surface precipitates; or incorporated into solid phases (e.g., siderite, magnetite). Different chemical forms of <span class="hlt">sediment</span>-bound Fe(II) have different reactivities (e.g., with dissolved oxygen) and their formation or destruction by sorption/desorption and precipitation/dissolution is coupled to different solutes (e.g., major cations, H+, carbonate). We are quantifying chemical forms of <span class="hlt">sediment</span>-bound Fe(II) using previously published extractions, novel extractions, and experimental studies (e.g., Fe isotopic exchange). <span class="hlt">Sediments</span> are from Bemidji, Minnesota, where biodegradation of hydrocarbons from a burst oil pipeline has driven extensive dissimilatory Fe(III) reduction, and sites potentially impacted by unconventional oil and gas development. Generally, minimal Fe(II) was mobilized from ion exchange sites (batch desorption with MgCl2 and repeated desorption with NH4Cl). A < 2mm <span class="hlt">sediment</span> fraction from the iron-reducing <span class="hlt">zone</span> at Bemidji had 1.8umol/g Fe(II) as surface complexes or carbonate phases (sodium acetate at pH 5) of which ca. 13% was present as surface complexes (FerroZine extractions). Total bioavailable Fe(III) and biogenic Fe(II) (HCl extractions) was 40-50 umole/g on both background and iron-reducing <span class="hlt">zone</span> <span class="hlt">sediments</span> . Approximately half of the HCl-extractable Fe from Fe-reducing <span class="hlt">zone</span> <span class="hlt">sediments</span> was Fe(II) whereas 12 - 15% of Fe extracted from background <span class="hlt">sediments</span> was present as Fe(II). One-third to one-half of the total biogenic Fe(II) extracted from <span class="hlt">sediments</span> collected from a Montana prairie pothole located downgradient from a produced-water disposal pit was present as surface-complexed Fe(II).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3504103','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3504103"><span>Organism-<span class="hlt">Sediment</span> Interactions Govern Post-Hypoxia Recovery of Ecosystem Functioning</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Van Colen, Carl; Rossi, Francesca; Montserrat, Francesc; Andersson, Maria G. I.; Gribsholt, Britta; Herman, Peter M. J.; Degraer, Steven; Vincx, Magda; Ysebaert, Tom; Middelburg, Jack J.</p> <p>2012-01-01</p> <p>Hypoxia represents one of the major causes of biodiversity and ecosystem functioning loss for coastal waters. Since eutrophication-induced hypoxic events are becoming increasingly frequent and intense, understanding the response of ecosystems to hypoxia is of primary importance to understand and predict the stability of ecosystem functioning. Such ecological stability may greatly depend on the recovery patterns of communities and the return time of the system properties associated to these patterns. Here, we have examined how the reassembly of a benthic community contributed to the recovery of ecosystem functioning following experimentally-induced hypoxia in a tidal flat. We demonstrate that organism-<span class="hlt">sediment</span> interactions that depend on organism size and relate to mobility traits and <span class="hlt">sediment</span> reworking capacities are generally more important than <span class="hlt">recovering</span> species richness to set the return time of the measured <span class="hlt">sediment</span> processes and properties. Specifically, increasing macrofauna bioturbation potential during community reassembly significantly contributed to the recovery of <span class="hlt">sediment</span> processes and properties such as denitrification, bedload <span class="hlt">sediment</span> transport, primary production and deep pore water ammonium concentration. Such bioturbation potential was due to the replacement of the small-sized organisms that recolonised at early stages by large-sized bioturbating organisms, which had a disproportionately stronger influence on <span class="hlt">sediment</span>. This study suggests that the complete recovery of organism-<span class="hlt">sediment</span> interactions is a necessary condition for ecosystem functioning recovery, and that such process requires long periods after disturbance due to the slow growth of juveniles into adult stages involved in these interactions. Consequently, repeated episodes of disturbance at intervals smaller than the time needed for the system to fully <span class="hlt">recover</span> organism-<span class="hlt">sediment</span> interactions may greatly impair the resilience of ecosystem functioning. PMID:23185440</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/8683','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/8683"><span>Effect of logging on streamflow, <span class="hlt">sedimentation</span>, and fish habitat</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Robert R. Ziemer</p> <p>1968-01-01</p> <p>Cooperative Watershed Management research in the Lower Conifer <span class="hlt">Zone</span> of California started in 1961. Research in the Lower Conifer <span class="hlt">Zone</span> was designed to obtain information and develop principles about the effect of land management in the <span class="hlt">Zone</span> upon water quality, floods and <span class="hlt">sedimentation</span>, water timing, and water yield. The research was conducted by the Pacific Southwest...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23641239','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23641239"><span>Spatial variation of <span class="hlt">sediment</span> mineralization supports differential CO2 emissions from a tropical hydroelectric reservoir.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cardoso, Simone J; Vidal, Luciana O; Mendonça, Raquel F; Tranvik, Lars J; Sobek, Sebastian; Fábio, Roland</p> <p>2013-01-01</p> <p>Substantial amounts of organic matter (OM) from terrestrial ecosystems are buried as <span class="hlt">sediments</span> in inland waters. It is still unclear to what extent this OM constitutes a sink of carbon, and how much of it is returned to the atmosphere upon mineralization to carbon dioxide (CO2). The construction of reservoirs affects the carbon cycle by increasing OM <span class="hlt">sedimentation</span> at the regional scale. In this study we determine the OM mineralization in the <span class="hlt">sediment</span> of three <span class="hlt">zones</span> (river, transition, and dam) of a tropical hydroelectric reservoir in Brazil as well as identify the composition of the carbon pool available for mineralization. We measured <span class="hlt">sediment</span> organic carbon mineralization rates and related them to the composition of the OM, bacterial abundance and pCO2 of the surface water of the reservoir. Terrestrial OM was an important substrate for the mineralization. In the river and transition <span class="hlt">zones</span> most of the OM was allochthonous (56 and 48%, respectively) while the dam <span class="hlt">zone</span> had the lowest allochthonous contribution (7%). The highest mineralization rates were found in the transition <span class="hlt">zone</span> (154.80 ± 33.50 mg C m(-) (2) d(-) (1)) and the lowest in the dam (51.60 ± 26.80 mg C m(-) (2) d(-) (1)). Moreover, mineralization rates were significantly related to bacterial abundance (r (2) = 0.50, p < 0.001) and pCO2 in the surface water of the reservoir (r (2) = 0.73, p < 0.001). The results indicate that allochthonous OM has different contributions to <span class="hlt">sediment</span> mineralization in the three <span class="hlt">zones</span> of the reservoir. Further, the <span class="hlt">sediment</span> mineralization, mediated by heterotrophic bacteria metabolism, significantly contributes to CO2 supersaturation in the water column, resulting in higher pCO2 in the river and transition <span class="hlt">zones</span> in comparison with the dam <span class="hlt">zone</span>, affecting greenhouse gas emission estimations from hydroelectric reservoirs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=92781','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=92781"><span>Biogeochemical and Molecular Signatures of Anaerobic Methane Oxidation in a Marine <span class="hlt">Sediment</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Thomsen, Trine R.; Finster, Kai; Ramsing, Niels B.</p> <p>2001-01-01</p> <p>Anaerobic methane oxidation was investigated in 6-m-long cores of marine <span class="hlt">sediment</span> from Aarhus Bay, Denmark. Measured concentration profiles for methane and sulfate, as well as in situ rates determined with isotope tracers, indicated that there was a narrow <span class="hlt">zone</span> of anaerobic methane oxidation about 150 cm below the <span class="hlt">sediment</span> surface. Methane could account for 52% of the electron donor requirement for the peak sulfate reduction rate detected in the sulfate-methane transition <span class="hlt">zone</span>. Molecular signatures of organisms present in the transition <span class="hlt">zone</span> were detected by using selective PCR primers for sulfate-reducing bacteria and for Archaea. One primer pair amplified the dissimilatory sulfite reductase (DSR) gene of sulfate-reducing bacteria, whereas another primer (ANME) was designed to amplify archaeal sequences found in a recent study of <span class="hlt">sediments</span> from the Eel River Basin, as these bacteria have been suggested to be anaerobic methane oxidizers (K. U. Hinrichs, J. M. Hayes, S. P. Sylva, P. G. Brewer, and E. F. DeLong, Nature 398:802–805, 1999). Amplification with the primer pairs produced more amplificate of both target genes with samples from the sulfate-methane transition <span class="hlt">zone</span> than with samples from the surrounding <span class="hlt">sediment</span>. Phylogenetic analysis of the DSR gene sequences retrieved from the transition <span class="hlt">zone</span> revealed that they all belonged to a novel deeply branching lineage of diverse DSR gene sequences not related to any previously described DSR gene sequence. In contrast, DSR gene sequences found in the top <span class="hlt">sediment</span> were related to environmental sequences from other estuarine <span class="hlt">sediments</span> and to sequences of members of the genera Desulfonema, Desulfococcus, and Desulfosarcina. Phylogenetic analysis of 16S rRNA sequences obtained with the primers targeting the archaeal group of possible anaerobic methane oxidizers revealed two clusters of ANME sequences, both of which were affiliated with sequences from the Eel River Basin. PMID:11282617</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11282617','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11282617"><span>Biogeochemical and molecular signatures of anaerobic methane oxidation in a marine <span class="hlt">sediment</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thomsen, T R; Finster, K; Ramsing, N B</p> <p>2001-04-01</p> <p>Anaerobic methane oxidation was investigated in 6-m-long cores of marine <span class="hlt">sediment</span> from Aarhus Bay, Denmark. Measured concentration profiles for methane and sulfate, as well as in situ rates determined with isotope tracers, indicated that there was a narrow <span class="hlt">zone</span> of anaerobic methane oxidation about 150 cm below the <span class="hlt">sediment</span> surface. Methane could account for 52% of the electron donor requirement for the peak sulfate reduction rate detected in the sulfate-methane transition <span class="hlt">zone</span>. Molecular signatures of organisms present in the transition <span class="hlt">zone</span> were detected by using selective PCR primers for sulfate-reducing bacteria and for Archaea. One primer pair amplified the dissimilatory sulfite reductase (DSR) gene of sulfate-reducing bacteria, whereas another primer (ANME) was designed to amplify archaeal sequences found in a recent study of <span class="hlt">sediments</span> from the Eel River Basin, as these bacteria have been suggested to be anaerobic methane oxidizers (K. U. Hinrichs, J. M. Hayes, S. P. Sylva, P. G. Brewer, and E. F. DeLong, Nature 398:802-805, 1999). Amplification with the primer pairs produced more amplificate of both target genes with samples from the sulfate-methane transition <span class="hlt">zone</span> than with samples from the surrounding <span class="hlt">sediment</span>. Phylogenetic analysis of the DSR gene sequences retrieved from the transition <span class="hlt">zone</span> revealed that they all belonged to a novel deeply branching lineage of diverse DSR gene sequences not related to any previously described DSR gene sequence. In contrast, DSR gene sequences found in the top <span class="hlt">sediment</span> were related to environmental sequences from other estuarine <span class="hlt">sediments</span> and to sequences of members of the genera Desulfonema, Desulfococcus, and Desulfosarcina. Phylogenetic analysis of 16S rRNA sequences obtained with the primers targeting the archaeal group of possible anaerobic methane oxidizers revealed two clusters of ANME sequences, both of which were affiliated with sequences from the Eel River Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5864061-ordovician-chitinozoan-zones-great-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5864061-ordovician-chitinozoan-zones-great-basin"><span>Ordovician chitinozoan <span class="hlt">zones</span> of Great Basin</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Hutter, T.J.</p> <p></p> <p>Within the Basin and Range province of the Great Basin of the western US, Ordovician chitinozoans have been <span class="hlt">recovered</span> in two major lithic facies; the western eugeosynclinal facies and the eastern miogeosynclinal facies. Chitinozoans <span class="hlt">recovered</span> from these facies range in age from Arenig to Ashgill. Extensive collections from this area make possible the establishment of chitinozoan faunal interval <span class="hlt">zones</span> from the Ordovician of this area. Selected species of biostratigraphic value include, in chronostratigraphic order, Lagenochitina ovoidea Benoit and Taugourdeau, 1961, Conochitina langei Combaz and Peniguel, 1972, Conochitinia poumoti Combaz and Penique, Desmochitina cf. nodosa Eisenack, 1931, Conochitina maclartii Combaz andmore » Peniguel, 1972, Conochitina robusta Eisenack, 1959, Angochitina capitallata Eisenack, 1937, Sphaerochitina lepta Jenkins. 1970, and Ancyrochitina merga Jenkins, 1970. In many cases, these <span class="hlt">zones</span> can be divided into additional sub-<span class="hlt">zones</span> using chitinozoans and acritarchs. In all cases, these chitinozoan faunal <span class="hlt">zones</span> are contrasted with established American graptolite <span class="hlt">zones</span> of the area, as well as correlated with British standard graptolite <span class="hlt">zones</span>. The composition of these faunas of the western US Great Basin is similar to that of the Marathon region of west Texas and the Basin Ranges of Arizona and New Mexico, to which direct comparisons have been made. There also appears to be a great similarity with the microfaunas and microfloras of the Ordovician of the Canning basin of western Australia. The Ordovician chitinozoan faunal interval <span class="hlt">zones</span> established for the Basin and Range province of the Great Basin of the western US also appear to be applicable to the Marathon region of west Texas and the Basin Ranges of Arizona and New Mexico.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatGe..10..954H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatGe..10..954H"><span>Links between <span class="hlt">sediment</span> consolidation and Cascadia megathrust slip behaviour</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Shuoshuo; Bangs, Nathan L.; Carbotte, Suzanne M.; Saffer, Demian M.; Gibson, James C.</p> <p>2017-12-01</p> <p>At <span class="hlt">sediment</span>-rich subduction <span class="hlt">zones</span>, megathrust slip behaviour and forearc deformation are tightly linked to the physical properties and in situ stresses within underthrust and accreted <span class="hlt">sediments</span>. Yet the role of <span class="hlt">sediment</span> consolidation at the onset of subduction in controlling the downdip evolution and along-strike variation in megathrust fault properties and accretionary wedge structure is poorly known. Here we use controlled-source seismic data combined with ocean drilling data to constrain the <span class="hlt">sediment</span> consolidation and in situ stress state near the deformation front of the Cascadia subduction <span class="hlt">zone</span>. Offshore Washington where the megathrust is inferred to be strongly locked, we find over-consolidated <span class="hlt">sediments</span> near the deformation front that are incorporated into a strong outer wedge, with little <span class="hlt">sediment</span> subducted. These conditions are favourable for strain accumulation on the megathrust and potential earthquake rupture close to the trench. In contrast, offshore Central Oregon, a thick under-consolidated <span class="hlt">sediment</span> sequence is subducting, and is probably associated with elevated pore fluid pressures on the megathrust in a region where reduced locking is inferred. Our results suggest that the consolidation state of the <span class="hlt">sediments</span> near the deformation front is a key factor contributing to megathrust slip behaviour and its along-strike variation, and it may also have a significant role in the deformation style of the accretionary wedge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA614647','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA614647"><span>Conceptual Regional <span class="hlt">Sediment</span> Budget for USACE North Atlantic Division</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-03-01</p> <p><span class="hlt">sediment</span> budget is the first phase in development of the working budget and is intended to provide a general framework based on existing transport ...existing literature and databases were reviewed and analyzed to characterize <span class="hlt">sediment</span> transport pathways and magnitudes, and morphologic <span class="hlt">zones</span> of...net <span class="hlt">sediment</span> transport pathways for Region 1 (includes NACCS planning regions VA1 through VA6 and MD2 through MD5</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMEP21A0665D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMEP21A0665D"><span>Analysis of the <span class="hlt">Sediment</span> Hydrograph of the alluvial deltas in the Apalachicola River, Florida</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daranpob, A.; Hagen, S.; Passeri, D.; Smar, D. E.</p> <p>2011-12-01</p> <p>Channel and alluvial characteristics in lowlands are the products of boundary conditions and driving forces. The boundary conditions normally include materials and land cover types, such as soil type and vegetation cover. General driving forces include discharge rate, <span class="hlt">sediment</span> loadings, tides and waves. Deltas built up of river-transported <span class="hlt">sediment</span> occur in depositional <span class="hlt">zones</span> of the river mouth in flat terrains and slow currents. Total <span class="hlt">sediment</span> load depends on two major abilities of the river, the river shear stress and capacity. The shear stress determines transport of a given <span class="hlt">sediment</span> grain size, normally expressed as tractive force. The river capacity determines the total load or quantity of total <span class="hlt">sediments</span> transported across a section of the river, generally expressed as the <span class="hlt">sediment</span> loading rate. The shear stress and <span class="hlt">sediment</span> loading rate are relatively easy to measure in the headwater and transfer <span class="hlt">zones</span> where streams form a v-shape valley and the river begins to form defined banks compared to the deposition <span class="hlt">zone</span> where rivers broaden across lower elevation landscapes creating alluvial forms such as deltas. Determinations of deposition and re-suspension of <span class="hlt">sediment</span> in fluvial systems are complicated due to exerting tidal, wind, and wave forces. Cyclic forces of tides and waves repeatedly change the <span class="hlt">sediment</span> transport and deposition rate spatially and temporally in alluvial fans. However, the influence decreases with water depth. Understanding the transport, deposition, and re-suspension of <span class="hlt">sediments</span> in the fluvial <span class="hlt">zone</span> would provide a better understanding of the morphology of landscape in lowland estuaries such as the Apalachicola Bay and its estuary systems. The Apalachicola River system is located in the Florida Panhandle. Shelf <span class="hlt">sedimentation</span> process is not a strong influence in this region because it is protected by barrier islands from direct ocean forces of the Gulf of Mexico. This research explores the characteristic of suspended <span class="hlt">sediment</span> loadings in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS23A1372M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS23A1372M"><span>Texture, mineralogy and geochemistry of the continental slope <span class="hlt">sediments</span> in front of Los Tuxtlas, Gulf of Mexico, Mexico: implications on weathering, origin and depositional environments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marca-Castillo, M. E.; Armstrong-Altrin, J.</p> <p>2017-12-01</p> <p>The textural analysis, mineralogy and geochemistry of two <span class="hlt">sediment</span> cores <span class="hlt">recovered</span> from the deep water <span class="hlt">zone</span> of the southwestern part of the Gulf of Mexico ( 1666 and 1672 m water depth) were studied to infer the provenance and depositional behavior. The textural analysis revealed that both cores are dominated by silt, which occupy more than 50% in both samples and the clay occupy 40%. The petrographic analysis revealed remains of biogenic origin <span class="hlt">sediments</span> and lithic fragments with an angular shape and low sphericity, indicating a low energy environment and therefore a low level of weathering in the <span class="hlt">sediment</span>, which suggests that the <span class="hlt">sediments</span> were not affected by transport and derived from a nearby source rock. In both cores quartz fragments were identified; also volcanic lithic and pyroxenes fragments, which are rocks of intermediate composition and are generally associated with the volcanic activity of the continental margins. SEM-EDS studies showed that the analysed samples have concentrations of minerals such as barite, gibbsite, kaolinite, grossular, magnetite, plagioclase and chlorite, which are probably derived from the mainland to the deep sea <span class="hlt">zone</span>. In the trace element analysis it was observed a low Sc content, while Co, Ni, V and Cu are slightly enriched with respect to the upper continental crust; this enrichment is related to <span class="hlt">sediments</span> from intermediate sources. The <span class="hlt">sediments</span> are classified as shale in the log (SiO2 / Al2O3) - log (Fe2O / K2O) diagram. The fine particles of the shale indicate that a deposit occurred as a result of the gradual <span class="hlt">sedimentation</span> due to relatively non-turbulent currents, which is consistent with the petrographic analysis. The geochemical features of major and trace elements suggest <span class="hlt">sediments</span> were derived largely from the natural andesite erosion of coastal regions along the Gulf of Mexico. High values of Fe2O3 and MnO are observed in the upper intervals, reflecting the influence of volcanic <span class="hlt">sediments</span>. The major element</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC53D0927L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC53D0927L"><span>Thermokarst lake dynamics and its influence on biogeochemical <span class="hlt">sediment</span> characteristics: A case study from the discontinuous permafrost <span class="hlt">zone</span> in Interior Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenz, J.; Walter Anthony, K. M.; Maio, C. V.; Matuszewski, F.; Grosse, G.</p> <p>2017-12-01</p> <p>Under currently projected scenarios of climate warming, discontinuous warm permafrost in Interior Alaska is expected to experience widespread disappearance. Thermokarst ponds and lakes are evidence for rapid permafrost thaw and amplify deep thaw by talik development. During the thawing process, previously preserved organic matter is made available for decomposition and former permafrost carbon is potentially released as greenhouse gases carbon dioxide and methane. In the course of lake development and shoreline expansion, both, younger near-surface and older organic matter from slumping shores are potentially deposited in the lake basin. Lake internal bioproductivity is complementing carbon accumulation in lacustrine deposits and provides an additional source of young carbon. This study presents results of two intersecting, limnolithological transects of 5 <span class="hlt">sediment</span> cores from Goldstream Lake, a typical small, boreal thermokarst lake in Interior Alaska. We here distinguish external terrestrial and internal aquatic carbon contributions to <span class="hlt">sediments</span> based on <span class="hlt">sediment</span> samples that were analyzed for the total organic carbon/total nitrogen ratio (C/N) as well as stable carbon isotopes. The littoral <span class="hlt">zone</span> with actively eroding shorelines is characterized by methane seeps produced from anaerobic microbial decomposition; however, near-shore <span class="hlt">sediments</span> have surprisingly low total organic carbon contents with a mean of 1.5 wt%; the low C/N ratio of 8.7 indicate a dominance of lacustrine plant material. Very similar results were found for <span class="hlt">sediments</span> in the central basin, but here a clear shift to a terrestrial carbon signal (C/N of 22) with total organic carbon content of almost 30 wt% is presumably indicating the presence of a trash layer featuring largely terrestrial plants submerged during the initial lake phase. The talik <span class="hlt">sediments</span> have carbon storage similar to the lake <span class="hlt">sediments</span> but in contrast are not layered. Subarctic aquatic environments such as Goldstream Lake</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14526546','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14526546"><span>[Microbial sulfate reduction in <span class="hlt">sediments</span> of the coastal <span class="hlt">zone</span> and littoral of the Kandalaksha bay of the White sea].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Savvichev, A S; Rusanov, I I; Iusupov, S K; Baĭramov, I T; Pimenov, N V; Lein, A Iu; Ivanov, M V</p> <p>2003-01-01</p> <p>Microbiological and biogeochemical investigations of the coastal <span class="hlt">zone</span> and the littoral of the Kandalaksha Bay of the White Sea were carried out. The material for investigations was obtained in the series of expeditions of the Institute of Microbiology, Russian Academy of Sciences, in August 1999, 2000, 2001, and in March 2003. The studies were conducted on the littoral and in the water area of the Kandalaksha Preserve, the Moscow University Belomorsk Biological Station, and the Zoological Institute Biological Station, Russian Academy of Sciences, <span class="hlt">Sediment</span> sampling on the littoral was carried out in the typical microlandscapes differing in the <span class="hlt">sediment</span> properties and macrobenthos distribution. The maximal sulfate reduction rate (SRR) was shown for the shallow part of the Chemorechenskaya Bay (up to 2550 micrograms S/(dm3 day)) and in the Bab'ye More Bay (up to 3191 micrograms S/(dm3 day)). During the winter season, at a temperature of -0.5-0.5 degrees C, the SRR in the <span class="hlt">sediments</span> of the Kartesh Bay was 7.9-13 micrograms S/(dm3 day). In the widest limits, the SRR values varied in the <span class="hlt">sediment</span> cores sampled on the littoral. The minimal values (11 mu]g S/(dm3 day)) were obtained in the core samples on the silt-sandy littoral. The littoral finely dispersed <span class="hlt">sediments</span> rich in organic matter were characterized by high SRR values (524-1413 micrograms S/(dm3 day)). The maximal SRR values were shown for the <span class="hlt">sediments</span> present within the stretch of decomposing macrophytes, in local pits at the lower littoral waterline, and in the mouth of a freshwater stream (51-159 mg S/(dm3 day)). A sharp difference in the level of H2S production in the type microlandscapes was shown. The average hydrogen sulfide production in finely dispersed <span class="hlt">sediments</span> constituted 125 mg S/(m2 day); in stormy discharge deposits, 1950 mg S/(m2 day); in depressions under stones and in silted pits, 4300 mg S/(m2 day). A calculation made with regard to the area of microlandscapes with increased productivity shows</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916110B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916110B"><span>Evaluation of ship-based <span class="hlt">sediment</span> flux measurements by ADCPs in tidal flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Becker, Marius; Maushake, Christian; Grünler, Steffen; Winter, Christian</p> <p>2017-04-01</p> <p>In the past decades acoustic backscatter calibration developed into a frequently applied technique to measure fluxes of suspended <span class="hlt">sediments</span> in rivers and estuaries. Data is mainly acquired using single-frequency profiling devices, such as ADCPs. In this case, variations of acoustic particle properties may have a significant impact on the calibration with respect to suspended <span class="hlt">sediment</span> concentration, but associated effects are rarely considered. Further challenges regarding flux determination arise from incomplete vertical and lateral coverage of the cross-section, and the small ratio of the residual transport to the tidal transport, depending on the tidal prism. We analyzed four sets of 13h cross-sectional ADCP data, collected at different locations in the range of the turbidity <span class="hlt">zone</span> of the Weser estuary, North Sea, Germany. Vertical LISST, OBS and CTD measurements were taken very hour. During the calibration <span class="hlt">sediment</span> absorption was taken into account. First, acoustic properties were estimated using LISST particle size distributions. Due to the tidal excursion and displacement of the turbidity <span class="hlt">zone</span>, acoustic properties of particles changed during the tidal cycle, at all locations. Applying empirical functions, the lowest backscattering cross-section and highest <span class="hlt">sediment</span> absorption coefficient were found in the center of the turbidity <span class="hlt">zone</span>. Outside the tidally averaged location of the turbidity <span class="hlt">zone</span>, changes of acoustic parameters were caused mainly by advection. In the turbidity <span class="hlt">zone</span>, these properties were also affected by settling and entrainment, inducing vertical differences and systematic errors in concentration. In general, due to the iterative correction of <span class="hlt">sediment</span> absorption along the acoustic path, local errors in concentration propagate and amplify exponentially. Based on reference concentration obtained from water samples and OBS data, we quantified these errors and their effect on cross-sectional averaged concentration and <span class="hlt">sediment</span> flux. We found that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5691419','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5691419"><span>Depth Distribution and Assembly of Sulfate-Reducing Microbial Communities in Marine <span class="hlt">Sediments</span> of Aarhus Bay</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jochum, Lara M.; Chen, Xihan; Lever, Mark A.; Loy, Alexander; Jørgensen, Bo Barker; Schramm, Andreas</p> <p>2017-01-01</p> <p>ABSTRACT Most sulfate-reducing microorganisms (SRMs) present in subsurface marine <span class="hlt">sediments</span> belong to uncultured groups only distantly related to known SRMs, and it remains unclear how changing geochemical <span class="hlt">zones</span> and <span class="hlt">sediment</span> depth influence their community structure. We mapped the community composition and abundance of SRMs by amplicon sequencing and quantifying the dsrB gene, which encodes dissimilatory sulfite reductase subunit beta, in <span class="hlt">sediment</span> samples covering different vertical geochemical <span class="hlt">zones</span> ranging from the surface <span class="hlt">sediment</span> to the deep sulfate-depleted subsurface at four locations in Aarhus Bay, Denmark. SRMs were present in all geochemical <span class="hlt">zones</span>, including sulfate-depleted methanogenic <span class="hlt">sediment</span>. The biggest shift in SRM community composition and abundance occurred across the transition from bioturbated surface <span class="hlt">sediments</span> to nonbioturbated <span class="hlt">sediments</span> below, where redox fluctuations and the input of fresh organic matter due to macrofaunal activity are absent. SRM abundance correlated with sulfate reduction rates determined for the same <span class="hlt">sediments</span>. Sulfate availability showed a weaker correlation with SRM abundances and no significant correlation with the composition of the SRM community. The overall SRM species diversity decreased with depth, yet we identified a subset of highly abundant community members that persists across all vertical geochemical <span class="hlt">zones</span> of all stations. We conclude that subsurface SRM communities assemble by the persistence of members of the surface community and that the transition from the bioturbated surface <span class="hlt">sediment</span> to the unmixed <span class="hlt">sediment</span> below is a main site of assembly of the subsurface SRM community. IMPORTANCE Sulfate-reducing microorganisms (SRMs) are key players in the marine carbon and sulfur cycles, especially in coastal <span class="hlt">sediments</span>, yet little is understood about the environmental factors controlling their depth distribution. Our results suggest that macrofaunal activity is a key driver of SRM abundance and community structure</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/873640','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/873640"><span>Marine clathrate mining and <span class="hlt">sediment</span> separation</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Borns, David J.; Hinkebein, Thomas E.; Lynch, Richard W.; Northrop, David A.</p> <p>2001-01-01</p> <p>A method and apparatus for mining of hydrocarbons from a hydrocarbon-containing clathrate such as is found on the ocean floor. The hydrocarbon containing clathrate is disaggregated from <span class="hlt">sediment</span> by first disrupting clathrate-containing strata using continuous mining means such as a rotary tilling drum, a fluid injector, or a drill. The clathrate-rich portion of <span class="hlt">sediment</span> thus disrupted from the sea floor strata are carried through the apparatus to regions of relative lower pressure and/or relative higher temperature where the clathrate further dissociates into component hydrocarbons and water. The hydrocarbon is <span class="hlt">recovered</span> with the assistance of a gas that is injected and buoys the hydrocarbon containing clathrate helping it to rise to regions of lower pressure and temperature where hydrocarbon is released. The <span class="hlt">sediment</span> separated from the hydrocarbon returns to the ocean floor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T44C..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T44C..04S"><span>Dispersed Volcanic Ash in <span class="hlt">Sediment</span> Entering NW Pacific Ocean Subduction <span class="hlt">Zones</span>: Towards a Regional Perspective</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scudder, R. P.; Murray, R. W.; Underwood, M.; Kutterolf, S.; Plank, T.; Dyonisius, M.; Arshad, M. A.</p> <p>2011-12-01</p> <p>Volcanic ash has long been recognized to be an important component of the global sedimentary system. Ash figures prominently in a number of sedimentary and petrophysical investigations, including how the fluid budget of subducting <span class="hlt">sediment</span> will be affected by hydration/dehydration reactions. Additionally, many studies focus on discrete ash layers, and how to link their presence with volcanism, climate, arc evolution, biological productivity, and other processes. Less widely recognized is the ash that is mixed into the bulk <span class="hlt">sediment</span>, or "dispersed" ash. Dispersed ash is quantitatively significant and is an under-utilized source of critical geochemical and tectonic information. Based on geochemical studies of ODP Site 1149, a composite of DSDP Sites 579 & 581, as well as IODP Sites C0011 & C0012 drilled during Expedition 322, we will show the importance of dispersed ash to the Izu-Bonin-Marianas, Kurile-Kamchatka and Nankai subduction <span class="hlt">zones</span>. Initial geochemical analyses of the bulk <span class="hlt">sediment</span>, as related to dispersed ash entering these subduction systems are presented here. Geochemical analysis shows that the characteristics of the three sites exhibit some variability consistent with observed lithological variations. For example, the average SiO2/Al2O3 ratios at Site 1149, Site C0011 and Site C0012 average 3.7. The composite of Sites 579 & 581 exhibits a higher average of 4.6. There are contrasts between other key major elemental indicators as well (e.g., Fe2O3). Ternary diagrams such as K2O-Na2O-CaO show that there are at least two distinct geochemical fields with Sites 1149, C0011 and C0012 clustering in one and Sites 579 & 581 in the other. Q-mode Factor Analysis was performed on the bulk <span class="hlt">sediment</span> chemical data in order to determine the composition of potential end members of these sites. The multivariate statistics indicate that Site 1149 has 3-4 end members, consistent with the results of Scudder et al. (2009, EPSL, v. 284, pp 639), while each of the other sites</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26803740','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26803740"><span>Flow regulation manipulates contemporary seasonal sedimentary dynamics in the reservoir fluctuation <span class="hlt">zone</span> of the Three Gorges Reservoir, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tang, Qiang; Bao, Yuhai; He, Xiubin; Fu, Bojie; Collins, Adrian L; Zhang, Xinbao</p> <p>2016-04-01</p> <p>Since the launch of the Three Gorges Dam on the Yangtze River, a distinctive reservoir fluctuation <span class="hlt">zone</span> has been created and significantly modified by regular dam operations. <span class="hlt">Sediment</span> redistribution within this artificial landscape differs substantially from that in natural fluvial riparian <span class="hlt">zones</span>, due to a specific hydrological regime comprising steps of water impoundment with increasing magnitudes and seasonal water level fluctuation holding a range of <span class="hlt">sediment</span> fluxes. This study reinterpreted post-dam sedimentary dynamics in the reservoir fluctuation <span class="hlt">zone</span> by stratigraphy determination of a 345-cm long <span class="hlt">sediment</span> core, and related it to impact of the hydrological regime. Seasonality in absolute grain-size composition of suspended <span class="hlt">sediment</span> was applied as a methodological basis for stratigraphic differentiation. Sedimentary laminations with relatively higher proportions of sandy fractions were ascribed to <span class="hlt">sedimentation</span> during the dry season when proximal subsurface bank erosion dominates source contributions, while stratigraphy with a lower proportion of sandy fractions is possibly contributed by <span class="hlt">sedimentation</span> during the wet season when distal upstream surface erosion prevails. Chronology determination revealed non-linear and high annual <span class="hlt">sedimentation</span> rates ranging from 21.7 to 152.1cm/yr. Although channel geomorphology may primarily determine the spatial extent of <span class="hlt">sedimentation</span>, seasonal sedimentary dynamics was predominantly governed by the frequency, magnitude, and duration of flooding. Summer inundation by natural floods with enhanced <span class="hlt">sediment</span> loads produced from upstream basins induced higher <span class="hlt">sedimentation</span> rates than water impoundment during the dry season when distal <span class="hlt">sediment</span> supply was limited. We thus conclude that flow regulation manipulates contemporary seasonal sedimentary dynamics in the reservoir fluctuation <span class="hlt">zone</span>, though little impact on total <span class="hlt">sediment</span> retention rate was detected. Ongoing reductions in flow and <span class="hlt">sediment</span> supply under human disturbance may</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP21D1871L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP21D1871L"><span>Tropical Cyclones as a Driver of Global <span class="hlt">Sediment</span> Flux</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leyland, J.; Darby, S. E.; Cohen, S.</p> <p>2017-12-01</p> <p>The world's rivers deliver 19 billion tonnes of <span class="hlt">sediment</span> to the coastal <span class="hlt">zone</span> annually. The <span class="hlt">sediment</span> supplied to the coastal <span class="hlt">zone</span> is of significant importance for a variety of reasons, for example in acting as a vector for nutrients as well as in supplying <span class="hlt">sediment</span> to coastal landforms such as deltas and beaches that can buffer those landforms from erosion and flooding. A greater understanding of the factors governing <span class="hlt">sediment</span> flux to the oceans is therefore a key research gap. The non-linear relationship between river discharge and <span class="hlt">sediment</span> flux implies that the global <span class="hlt">sediment</span> flux may be disproportionately driven by large floods. Indeed, in our recent empirical research we have demonstrated that changes in the track locations, frequency and intensity of tropical storms in recent decades exert a significant control on the <span class="hlt">sediment</span> flux emanating from the Mekong River. Since other large rivers potentially affected by tropical storms are known to make a significant contribution to the global <span class="hlt">sediment</span> flux, this raises the question of the extent to which such storms play a significant role in controlling <span class="hlt">sediment</span> loads at the global scale. In this paper we address that question by employing a global hydrological model (WBMsed) in order to predict runoff and <span class="hlt">sediment</span> load forced by recent historical climate scenarios `with' and `without' tropical cyclones. We compare the two scenarios to (i) make the first estimate of the global contribution of <span class="hlt">sediment</span> load forced by tropical storms; (ii) evaluate how that contribution has varied in recent decades and to (iii) explore variations in tropical-storm driven <span class="hlt">sediment</span> loads in selected major river basins that are significantly affected by such storms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.3090Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.3090Q"><span>Detailed seismic velocity of the incoming subducting <span class="hlt">sediments</span> in the 2004 great Sumatra earthquake rupture <span class="hlt">zone</span> from full waveform inversion of long offset seismic data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qin, Yanfang; Singh, Satish C.</p> <p>2017-04-01</p> <p>The nature of incoming <span class="hlt">sediments</span> defines the locking mechanism on the megathrust, and the development and evolution of the accretionary wedge. Here we present results from seismic full waveform inversion of 12 km long offset seismic reflection data within the trench in the 2004 Sumatra earthquake rupture <span class="hlt">zone</span> area that provide detailed quantitative information on the incoming oceanic <span class="hlt">sediments</span> and the trench-fill <span class="hlt">sediments</span>. The thickness of <span class="hlt">sediments</span> in this area is 3-4 km, and P wave velocity is as much as 4.5 km/s just above the oceanic crust, suggesting the presence of silica-rich highly compacted and lithified <span class="hlt">sediments</span> leading to a strong coupling up to the subduction front. We also find an 70-80 m thick low-velocity layer, capped by a high-velocity layer, at 0.8 km above the subducting plate. This low-velocity layer, previously identified as high-amplitude negative polarity reflection, could have porosity of up to 30% containing overpressured fluids, which could act as a protodécollement seaward from the accretionary prism and décollement beneath the forearc. This weak protodécollement combined with the high-velocity indurated <span class="hlt">sediments</span> above the basement possibly facilitated the rupture propagating up to the front during the 2004 earthquake and enhancing the tsunami. We also find another low-velocity layer within the <span class="hlt">sediments</span> that may act as a secondary décollement observed offshore central Sumatra, forming bivergent pop-up structures and acting as a conveyer belt in preserving these pop-up structures in the forearc region.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS53B1192V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS53B1192V"><span>Fe-C-S systematics in Bengal Fan <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volvoikar, S. P.; Mazumdar, A.; Goswami, H.; Pujari, S.; Peketi, A.</p> <p>2017-12-01</p> <p>Global biogeochemical cycles of iron, carbon and sulfur (Fe-C-S) are interrelated. Sulfate reduction in marine <span class="hlt">sediments</span> is the major factor controlling the cycling and burial of carbon, sulfur and iron. Organoclastic sulfate reduction and anaerobic oxidation of methane (AOM) are the two main processes responsible for sulfate reduction in marine <span class="hlt">sediments</span>. The amount and reactivity of organic matter, iron minerals and concentrations of dissolved sulfide in pore water control the burial of iron sulfide and organic bound sulfur in marine <span class="hlt">sediments</span>. Here we investigate the sulfidization process in a <span class="hlt">sediment</span> core from the western part of upper Bay of Bengal fan characterized by efficient burial of organic matter with siliclastic load. A 30 m long <span class="hlt">sediment</span> core (MD 161/29, Lat. 170 18.04' N, Long. 870 22.56' E, water depth: 2434m) was collected onboard Marion Dufresne (May, 2007) and studied for Fe-S speciation and organic matter characterization. Buffered dithionite extractable iron (FeD) varies from 0.71 to 1.43 wt % (Avg. 0.79 wt %). FeD represents Fe oxides and oxyhydroxides mainly, ferrihydrite, lepidocrocite, goethite and hematite. Acid volatile sulfur (AVS) varies from 0.0015 to 0.63 wt % (avg: 0.058 wt %), while chromium reducible sulfur (CRS) varies from 0.00047 to 0.29 wt % (avg. 0.054 wt %). Based on the vertical distribution patterns of FeD, AVS and CRS, the core is divided into three <span class="hlt">zones</span>, the lower (3000 to 1833 cm), middle (1833 to 398 cm) and upper (398 cm to surface) <span class="hlt">zones</span>. FeD shows higher concentration in the lower <span class="hlt">zone</span>. FeTR (FeOx + FeD + FeCRS + FeAVS) also exhibit higher concentration in this <span class="hlt">zone</span>, suggesting higher availability of reactive iron for iron sulfide precipitation. AVS, elemental sulfur, spikes of CRS and gradual enrichment of δ34SAVS and δ34SCRS with sharp peaks in-between is noted in the lower <span class="hlt">zone</span>. The gradual enrichment of δ34SAVS and δ34SCRS is the outcome of late diagenetic pyritization with higher availability of sulfide</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeCoA.223..198B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeCoA.223..198B"><span>Chromium isotope fractionation in ferruginous <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bauer, Kohen W.; Gueguen, Bleuenn; Cole, Devon B.; Francois, Roger; Kallmeyer, Jens; Planavsky, Noah; Crowe, Sean A.</p> <p>2018-02-01</p> <p>Ferrous Fe is a potent reductant of Cr(VI), and while a number of laboratory studies have characterized Cr isotope fractionation associated with Cr(VI) reduction by ferrous iron, the expression of this fractionation in real-world ferrous Fe-rich environments remains unconstrained. Here we determine the isotope fractionation associated with Cr(VI) reduction in modern ferrous Fe-rich <span class="hlt">sediments</span> obtained from the previously well studied Lake Matano, Indonesia. Whole core incubations demonstrate that reduction of Cr(VI) within ferruginous <span class="hlt">sediments</span> provides a sink for Cr(VI) leading to Cr(VI) concentration gradients and diffusive Cr(VI) fluxes across the <span class="hlt">sediment</span> water interface. As reduction proceeded, Cr(VI) remaining in the overlying lake water became progressively enriched in the heavy isotope (53Cr), increasing δ53Cr by 2.0 ± 0.1‰ at the end of the incubation. Rayleigh distillation modelling of the evolution of Cr isotope ratios and Cr(VI) concentrations in the overlying water yields an effective isotope fractionation of εeff = 1.1 ± 0.2‰ (53Cr/52Cr), whereas more detailed diagenetic modelling implies an intrinsic isotope fractionation of εint = 1.80 ± 0.04‰. Parallel slurry experiments performed using anoxic ferruginous <span class="hlt">sediment</span> yield an intrinsic isotope fractionation of εint = 2.2 ± 0.1‰. These modelled isotope fractionations are corroborated by direct measurement of the δ53Cr composition on the upper 0.5 cm of Lake Matano <span class="hlt">sediment</span>, revealing an isotopic offset from the lake water of Δ53Cr = 0.21-1.81‰. The data and models reveal that effective isotope fractionations depend on the depth at which Cr(VI) reduction takes place below the <span class="hlt">sediment</span> water interface-the deeper the oxic non-reactive <span class="hlt">zone</span>, the smaller the effective fractionation relative to the intrinsic fractionation. Based on the geochemistry of the <span class="hlt">sediment</span> we suggest the electron donors responsible for reduction are a combination of dissolved Fe(II) and 0.5 M HCl extractable (solid</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70148276','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70148276"><span>Influence of the Amlia fracture <span class="hlt">zone</span> on the evolution of the Aleutian Terrace forearc basin, central Aleutian subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ryan, Holly F.; Draut, Amy E.; Keranen, Katie M.; Scholl, David W.</p> <p>2012-01-01</p> <p>During Pliocene to Quaternary time, the central Aleutian forearc basin evolved in response to a combination of tectonic and climatic factors. Initially, along-trench transport of <span class="hlt">sediment</span> and accretion of a frontal prism created the accommodation space to allow forearc basin deposition. Transport of sufficient <span class="hlt">sediment</span> to overtop the bathymetrically high Amlia fracture <span class="hlt">zone</span> and reach the central Aleutian arc began with glaciation of continental Alaska in the Pliocene. As the obliquely subducting Amlia fracture <span class="hlt">zone</span> swept along the central Aleutian arc, it further affected the structural evolution of the forearc basins. The subduction of the Amlia fracture <span class="hlt">zone</span> resulted in basin inversion and loss of accommodation space east of the migrating fracture <span class="hlt">zone</span>. Conversely, west of Amlia fracture <span class="hlt">zone</span>, accommodation space increased arcward of a large outer-arc high that formed, in part, by a thickening of arc basement. This difference in deformation is interpreted to be the result of a variation in interplate coupling across the Amlia fracture <span class="hlt">zone</span> that was facilitated by increasing subduction obliquity, a change in orientation of the subducting Amlia fracture <span class="hlt">zone</span>, and late Quaternary intensification of glaciation. The change in coupling is manifested by a possible tear in the subducting slab along the Amlia fracture <span class="hlt">zone</span>. Differences in coupling across the Amlia fracture <span class="hlt">zone</span> have important implications for the location of maximum slip during future great earthquakes. In addition, shaking during a great earthquake could trigger large mass failures of the summit platform, as evidenced by the presence of thick mass transport deposits of primarily Quaternary age that are found in the forearc basin west of the Amlia fracture <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3198393','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3198393"><span>High Levels of <span class="hlt">Sediment</span> Contamination Have Little Influence on Estuarine Beach Fish Communities</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>McKinley, Andrew C.; Dafforn, Katherine A.; Taylor, Matthew D.; Johnston, Emma L.</p> <p>2011-01-01</p> <p>While contaminants are predicted to have measurable impacts on fish assemblages, studies have rarely assessed this potential in the context of natural variability in physico-chemical conditions within and between estuaries. We investigated links between the distribution of <span class="hlt">sediment</span> contamination (metals and PAHs), physico-chemical variables (pH, salinity, temperature, turbidity) and beach fish assemblages in estuarine environments. Fish communities were sampled using a beach seine within the inner and outer <span class="hlt">zones</span> of six estuaries that were either heavily modified or relatively unmodified by urbanization and industrial activity. All sampling was replicated over two years with two periods sampled each year. Shannon diversity, biomass and abundance were all significantly higher in the inner <span class="hlt">zone</span> of estuaries while fish were larger on average in the outer <span class="hlt">zone</span>. Strong differences in community composition were also detected between the inner and outer <span class="hlt">zones</span>. Few differences were detected between fish assemblages in heavily modified versus relatively unmodified estuaries despite high concentrations of <span class="hlt">sediment</span> contaminants in the inner <span class="hlt">zones</span> of modified estuaries that exceeded recognized <span class="hlt">sediment</span> quality guidelines. Trends in species distributions, community composition, abundance, Shannon diversity, and average fish weight were strongly correlated to physico-chemical variables and showed a weaker relationship to <span class="hlt">sediment</span> metal contamination. <span class="hlt">Sediment</span> PAH concentrations were not significantly related to the fish assemblage. These findings suggest that variation in some physico-chemical factors (salinity, temperature, pH) or variables that co-vary with these factors (e.g., wave activity or grain size) have a much greater influence on this fish assemblage than anthropogenic stressors such as contamination. PMID:22039470</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1999/0237/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1999/0237/report.pdf"><span>Survey of Lake Ontario bottom <span class="hlt">sediment</span> off Rochester, New York, to define the extent of jettisoned World War II material and its potential for <span class="hlt">sediment</span> contamination</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kennedy, Gregory; Kappel, William M.</p> <p>2000-01-01</p> <p>Military-type mat??riel was <span class="hlt">recovered</span> from the bottom of Lake Ontario near Rochester, N.Y., during bottom-trawl, fish-stock surveys at depths of 75 to 180 feet each year from 1978 through 1996. The <span class="hlt">recovered</span> mat??riel included many shell-detonator nose cones (2 inches in diameter by about 3.5 inches long); several electronic components; one corroded box of detonators; a corrugated container of mercury-filled capsules; and corroded batteries. Most of the <span class="hlt">recovered</span> mat??riel has been identified as defective components of shell detonators (proximity-fuze assemblies) that were jettisoned in the lake to protect them from discovery during World War II. Side-scan SONAR, metal-detector, and ROV (remotely-operated-vehicle) surveys found no evidence of any large piles of mat??riel containing potentially hazardous, toxic, or polluting materials within the 17-square-mile study site. Many scattered magnetic anomalies were detected in this area, but chemical analysis of bottom <span class="hlt">sediment</span> and of zebra- and quagga-mussel (Dreissena spp.) tissue indicate that the concentrations of mercury and other heavy metals are within the previously documented ranges for Lake Ontario <span class="hlt">sediment</span>. The failure of ROV videos and of SCUBA-diver surveys and probes of the lake bottom to locate any debris indicates that most, if not all, of the debris is scattered and buried under a layer of fine-grained <span class="hlt">sediment</span> and, possibly, mussels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5750861-novel-pyropheophorbide-steryl-esters-black-sea-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5750861-novel-pyropheophorbide-steryl-esters-black-sea-sediments"><span>Novel pyropheophorbide steryl esters in Black Sea <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>King, L.L.; Repeta, D.J.</p> <p>1991-07-01</p> <p>A series of non-polar chlorophyll degradation products (NPCs) with greater than 10 components has been isolated from Black Sea <span class="hlt">sediment</span> and identified as pyropheophorbide steryl esters by visible and mass spectrometry. These compounds have been previously observed in seawater and <span class="hlt">sediment</span> trap samples, and may be formed during grazing of phytoplankton by zooplanktonic herbivores. In Black Sea <span class="hlt">sediments</span>, NPCs constitute 14% of the total phorbins determined spectroscopically at 660 nm, and 39% of the total chlorophyll degradation products measured by high pressure liquid chromatography. NPCs therefore constitute a significant sedimentary sink for chlorophyll. The distribution of sterols released by hydrolysismore » of NPCs most closely resembles sterols in suspended particulate matter collected from the euphotic <span class="hlt">zone</span> and is quite different from the distribution of solvent-extractable sterols in <span class="hlt">sediments</span>. Sterols extracted from sediemtns have high concentrations of 4-methylsterols and high stanol/stenol ratios. BNPC-derived sterols have very low concentrations of 4-methylsterols and low stanol/stenol ratios. The authors suggest that these differences reflect an enhanced preservation of HPCs in <span class="hlt">sediments</span> relative to free sterols and phorbins. As a result, the original production of sterols in the euphotic <span class="hlt">zone</span> may be more closely approximated by the distribution of NPC-derived sterols than by the distribution of free sterols in <span class="hlt">sediments</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS43B..06Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS43B..06Y"><span>Methane Recycling During Burial of Methane Hydrate-Bearing <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>You, K.; Flemings, P. B.</p> <p>2017-12-01</p> <p>We quantitatively investigate the integral processes of methane hydrate formation from local microbial methane generation, burial of methane hydrate with <span class="hlt">sedimentation</span>, and methane recycling at the base of the hydrate stability <span class="hlt">zone</span> (BHSZ) with a multiphase multicomponent numerical model. Methane recycling happens in cycles, and there is not a steady state. Each cycle starts with free gas accumulation from hydrate dissociation below the BHSZ. This free gas flows upward under buoyancy, elevates the hydrate saturation and capillary entry pressure at the BHSZ, and this prevents more free gas flowing in. Later as this layer with elevated hydrate saturation is buried and dissociated, the large amount of free gas newly released and accumulated below rapidly intrudes into the hydrate stability <span class="hlt">zone</span>, drives rapid hydrate formation and creates three-phase (gas, liquid and hydrate) equilibrium above the BHSZ. The gas front retreats to below the BHSZ until all the free gas is depleted. The shallowest depth that the free gas reaches in one cycle moves toward seafloor as more and more methane is accumulated to the BHSZ with time. More methane is stored above the BHSZ in the form of concentrated hydrate in <span class="hlt">sediments</span> with relatively uniform pore throat, and/or with greater compressibility. It is more difficult to initiate methane recycling in passive continental margins where the <span class="hlt">sedimentation</span> rate is low, and in <span class="hlt">sediments</span> with low organic matter content and/or methanogenesis reaction rate. The presence of a permeable layer can store methane for significant periods of time without recycling. In a 2D system where the seafloor dips rapidly, the updip gas flow along the BHSZ transports more methane toward topographic highs where methane gas and elevated hydrate saturation intrude deeper into the hydrate stability <span class="hlt">zone</span> within one cycle. This could lead to intermittent gas venting at seafloor at the topographic highs. This study provides insights on many phenomenon associated with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS23B1191S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS23B1191S"><span>Acoustic measurement of <span class="hlt">sediment</span> dynamics in the coastal <span class="hlt">zones</span> using wireless sensor networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sudhakaran, A., II; Paramasivam, A.; Seshachalam, S.; A, C.</p> <p>2014-12-01</p> <p>Analyzing of the impact of constructive or low energy waves and deconstructive or high energy waves in the ocean are very much significant since they deform the geometry of seashore. The deformation may lead to productive result and also to the end of deteriorate damage. Constructive waves results deposition of <span class="hlt">sediment</span> which widens the beach where as deconstructive waves results erosion which narrows the beach. Validation of historic <span class="hlt">sediment</span> transportation and prediction of the direction of movement of seashore is essential to prevent unrecoverable damages by incorporating precautionary measurements to identify the factors that influence <span class="hlt">sediment</span> transportation if feasible. The objective of this study is to propose a more reliable and energy efficient Information and communication system to model the Coastal <span class="hlt">Sediment</span> Dynamics. Various factors influencing the <span class="hlt">sediment</span> drift at a particular region is identified. Consequence of source depth and frequency dependencies of spread pattern in the presence of <span class="hlt">sediments</span> is modeled. Property of source depth and frequency on sensitivity to values of model parameters are determined. Fundamental physical reasons for these <span class="hlt">sediment</span> interaction effects are given. Shallow to deep water and internal and external wave model of ocean is obtained intended to get acoustic data assimilation (ADA). Signal processing algorithms are used over the observed data to form a full field acoustic propagation model and construct sound speed profile (SSP). The inversions of data due to uncertainties at various depths are compared. The impact of <span class="hlt">sediment</span> drift over acoustic data is identified. An energy efficient multipath routing scheme Wireless sensor networks (WSN) is deployed for the well-organized communication of data. The WSN is designed considering increased life time, decreased power consumption, free of threats and attacks. The practical data obtained from the efficient system to model the ocean <span class="hlt">sediment</span> dynamics are evaluated with remote</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP31B1277S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP31B1277S"><span>Preliminary Nearshore <span class="hlt">Sedimentation</span> Rate Analysis of the Tuungane Project Northern Mahale Conservation Area, Lake Tanganyika (Tanzania)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smiley, R. A.; McGlue, M. M.; Yeager, K. M.; Soreghan, M. J.; Lucas, J.; Kimirei, I.; Mbonde, A.; Limbu, P.; Apse, C.</p> <p>2017-12-01</p> <p>The combined effects of climate change, overfishing, and <span class="hlt">sediment</span> pollution are altering Lake Tanganyika's littoral fisheries in profoundly negative ways. One method for conserving critical fish resources and safeguarding biodiversity in Lake Tanganyika is by establishing small-scale nearshore protected <span class="hlt">zones</span>, which can be administrated by lakeshore villagers organized into beach management units (BMUs). Each BMU endeavors to manage offshore "no-catch" protected <span class="hlt">zones</span>, prohibit the use of illegal fishing gear, and promote sustainable agriculture that abates erosion in the lake watershed, in order to mitigate <span class="hlt">sediment</span> pollution in the lake. We adopted a limnogeological approach to assist in characterizing the littoral <span class="hlt">zone</span> associated with BMUs in the northern Mahale region of Lake Tanganyika (Tanzania), a critical conservation area for the Nature Conservancy's Tuungane Project (https://www.nature.org/ourinitiatives/regions/africa/wherewework/tuungane-project.xml). We hypothesized that BMUs with heavy onshore agricultural activity would experience relatively high offshore <span class="hlt">sedimentation</span> rates, due to enhanced <span class="hlt">sediment</span>-laden runoff in the wet season. Such changes are predicted to alter benthic substrates and degrade habitat available for fish spawning. We mapped bathymetry and <span class="hlt">sediment</span> types along a 29 km2 area of the littoral <span class="hlt">zone</span> using high-resolution geophysical tools, and assessed short-term <span class="hlt">sedimentation</span> rates using <span class="hlt">sediment</span> cores and radionuclide geochronology (210Pb). Initial results from 210Pb analyses show that <span class="hlt">sedimentation</span> rates at the mud-line ( 85-100 m water depth) are relatively slow but spatially variable in the northern Mahale area. Offshore of the Kalilani village BMU, linear <span class="hlt">sedimentation</span> rates are 0.50 mm/yr. By contrast, <span class="hlt">sedimentation</span> rates offshore from the Igualula village BMU are 0.90-1.30 mm/yr. Higher <span class="hlt">sedimentation</span> rates near Igualula are consistent with greater <span class="hlt">sediment</span> inputs from the nearby Lagosa River and its watershed, which has been</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70148113','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70148113"><span>Response of crayfish to hyporheic water availability and excess <span class="hlt">sedimentation</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dyer, Joseph J.; Worthington, Thomas A.; Brewer, Shannon K.</p> <p>2015-01-01</p> <p>Crayfish in many headwater streams regularly cope with seasonal drought. However, it is unclear how landscape changes affect the long-term persistence of crayfish populations. We designed two laboratory experiments to investigate the acute effects of common landscape stressors on crayfish: water withdrawal and <span class="hlt">sedimentation</span>. The first experiment tested the interaction among water withdrawals (four 24-h water reductions of 0, 15, 30, or 45 cm) and two substrate treatments (pebble and cobble) on the burrowing depth of crayfish. The second experiment evaluated the effects of excess fine <span class="hlt">sediment</span> (three treatments of 0, 45, and 90% <span class="hlt">sediment</span>) and substrate type (cobble and pebble) on crayfish burrowing depth. Crayfish were able to burrow deeper into the simulated hyporheic <span class="hlt">zone</span> in cobble substrate when compared to pebble. Crayfish subjected to greater water withdrawals in the pebble treatment were not able to reach the simulated hyporheic <span class="hlt">zone</span>. Excess fine <span class="hlt">sediment</span> reduced the depth that crayfish burrowed, regardless of substrate type. Results from this study suggest excess fine <span class="hlt">sediment</span> may reduce crayfish persistence, particularly when seeking refuge during prolonged dry conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17400350','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17400350"><span>Influence of hydropower dams on the composition of the suspended and riverbank <span class="hlt">sediments</span> in the Danube.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Klaver, Gerard; van Os, Bertil; Negrel, Philippe; Petelet-Giraud, Emmanuelle</p> <p>2007-08-01</p> <p>Large hydropower dams have major impacts on flow regime, <span class="hlt">sediment</span> transport and the characteristics of water and <span class="hlt">sediment</span> in downstream rivers. The Gabcikovo and Iron Gate dams divide the studied Danube transect (rkm 1895-795) into three parts. In the Gabcikovo Reservoir (length of 40km) only a part of the incoming suspended <span class="hlt">sediments</span> were deposited. Contrary to this, in the much larger Iron Gate backwater <span class="hlt">zone</span> and reservoir (length of 310km) all riverine suspended <span class="hlt">sediments</span> were deposited within the reservoir. Subsequently, suspended <span class="hlt">sediments</span> were transported by tributaries into the Iron Gate backwater <span class="hlt">zone</span>. Here they were modified by fractional <span class="hlt">sedimentation</span> before they transgressed downstream via the dams. Compared with undammed Danube sections, Iron Gate reservoir <span class="hlt">sediment</span> and suspended matter showed higher clay contents and different K/Ga and Metal/Ga ratios. These findings emphasize the importance of reservoir-river <span class="hlt">sediment</span>-fractionation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS21A1113T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS21A1113T"><span>A Non-Steady-State Condition in <span class="hlt">Sediments</span> at the Gashydrate Stability Boundary off West Spitsbergen: Evidence for Gashydrate Dissociation or Just Dynamic Methane Transport?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Treude, T.; Krause, S.; Bertics, V. J.; Steinle, L.; Niemann, H.; Liebetrau, V.; Feseker, T.; Burwicz, E.; Krastel, S.; Berndt, C.</p> <p>2014-12-01</p> <p>In 2008, a large area with several hundred methane plumes was discovered along the West Spitsbergen continental margin at water depths between 150 and 400 m (Westbrook et al. 2009, GRL 36, doi:10.1029/2009GL039191). Many of the observed plumes were located at the boundary of gas hydrate stability (~400 m water depth). It was speculated that the methane escape at this depth was correlated with gas hydrate destabilization caused by recent increases in water temperatures recorded in this region. In a later study, geochemical analyses of authigenic carbonates and modeling of heat flow data combined with seasonal changes in water temperature demonstrated that the methane seeps were active already prior to industrial warming but that the gas hydrate system nevertheless reacts very sensitive to even seasonal temperature changes (Berndt et al. 2014, Science 343: 284-287). Here, we report about a methane seep site at the gas hydrate stability boundary (394 m water depth) that features unusual geochemical profiles indicative for non-steady state conditions. <span class="hlt">Sediment</span> was <span class="hlt">recovered</span> with a gravity corer (core length 210 cm) and samples were analyzed to study porewater geochemistry, methane concentration, authigenic carbonates, and microbial activity. Porewater profiles revealed two <span class="hlt">zones</span> of sulfate-methane transition at 50 and 200 cm <span class="hlt">sediment</span> depth. The twin <span class="hlt">zones</span> were confirmed by a double peaking in sulfide, total alkalinity, anaerobic oxidation of methane, and sulfate reduction. δ18O values sharply increased from around -2.8 ‰ between 0 and 126 cm to -1.2 ‰ below 126 cm <span class="hlt">sediment</span> depth. While U/Th isotope measurements of authigenic seep carbonates that were collected from different depths of the core illustrated that methane seepage must be occurring at this site since at least 3000 years, the biogeochemical profiles suggest that methane flux must have been altered recently. By applying a multi-phase reaction-transport model using known initial parameters from the study</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018616','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018616"><span>Hydrothermal mineralization along submarine rift <span class="hlt">zones</span>, Hawaii</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hein, J.R.; Gibbs, A.E.; Clague, D.A.; Torresan, M.</p> <p>1996-01-01</p> <p>Describes mineralization of midplate submarine rift <span class="hlt">zones</span> and hydrothermal manganese oxide mineralization of midplate volcanic edifices. Hydrothermal Mn oxides were <span class="hlt">recovered</span> from submarine extensions of two Hawaiian rift <span class="hlt">zones</span>, along Haleakala and Puna Ridges. These Mn oxides form two types of deposits, metallic stratiform layers in volcaniclastic rocks and cement for clastic rocks; both deposit types are composed of todorokite and birnessite. Unlike most other hydrothermal Mn oxide deposits, those from Hawaiian rift <span class="hlt">zones</span> are enriched in the trace metals Zn, Co, Ba, Mo, Sr, V, and especially Ni. Metals are derived from three sources: mafic and ultramafic rocks leached by circulating hydrothermal fluids, clastic material (in Mn-cemented sandstone), and seawater that mixed with the hydrothermal fluids. Precipitation of Mn oxide below the seafloor is indicated by its occurrence as cement, growth textures that show mineralizing fluids were introduced from below, and pervasive replacement of original matrix of clastic rocks.Hydrothermal Mn oxides were <span class="hlt">recovered</span> from submarine extensions of two Hawaiian rift <span class="hlt">zones</span>, along Haleakala and Puna Ridges. These Mn oxides form two types of deposits, metallic stratiform layers in volcaniclastic rocks and cement for clastic rocks. Both deposit types are composed of todorokite and birnessite. This article describes in detail the specific characteristics of these Mn oxides.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24026206','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24026206"><span>Organotin compounds in surface <span class="hlt">sediments</span> of the Southern Baltic coastal <span class="hlt">zone</span>: a study on the main factors for their accumulation and degradation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Filipkowska, Anna; Kowalewska, Grażyna; Pavoni, Bruno</p> <p>2014-02-01</p> <p><span class="hlt">Sediment</span> samples were collected in the Gulf of Gdańsk, and the Vistula and Szczecin Lagoons-all located in the coastal <span class="hlt">zone</span> of the Southern Baltic Sea-just after the total ban on using harmful organotins in antifouling paints on ships came into force, to assess their butyltin and phenyltin contamination extent. Altogether, 26 sampling stations were chosen to account for different potential exposure to organotin pollution and environmental conditions: from shallow and well-oxygenated waters, shipping routes and river mouths, to deep and anoxic sites. Additionally, the organic carbon content, pigment content, and grain size of all the <span class="hlt">sediment</span> samples were determined, and some parameters of the near-bottom water (oxygen content, salinity, temperature) were measured as well. Total concentrations of butyltin compounds ranged between 2 and 182 ng Sn g(-1) d.w., whereas phenyltins were below the detection limit. <span class="hlt">Sediments</span> from the Gulf of Gdańsk and Vistula Lagoon were found moderately contaminated with tributyltin, whereas those from the Szczecin Lagoon were ranked as highly contaminated. Butyltin degradation indices prove a recent tributyltin input into the <span class="hlt">sediments</span> adjacent to sites used for dumping for dredged harbor materials and for anchorage in the Gulf of Gdańsk (where two big international ports are located), and into those collected in the Szczecin Lagoon. Essential factors affecting the degradation and distribution of organotins, based on significant correlations between butyltins and environmental variables, were found in the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19766465','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19766465"><span>The mechanism of erythrocyte <span class="hlt">sedimentation</span>. Part 1: Channeling in <span class="hlt">sedimenting</span> blood.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pribush, A; Meyerstein, D; Meyerstein, N</p> <p>2010-01-01</p> <p>Despite extensive efforts to elucidate the mechanism of erythrocyte <span class="hlt">sedimentation</span>, the understanding of this mechanism still remains obscure. In attempt to clarify this issue, we studied the effect of hematocrit (Hct) on the complex admittance of quiescent blood measured at different axial positions of the 2 mm x 2 mm cross-section chambers. It was found that after the aggregation process is completed, the admittance reveals delayed changes caused by the formation of cell-free <span class="hlt">zones</span> within the settling dispersed phase. The delay time (tau(d)) correlates positively with Hct and the distance between the axial position where measurements were performed and the bottom and is unaffected by the gravitational load. These findings and literature reports for colloidal gels suggest that erythrocytes in aggregating media form a network followed by the formation of plasma channels within it. The cell-free <span class="hlt">zones</span> form initially near the bottom and then propagate toward the top until they reach the plasma/blood interface. These channels increase the permeability of a network and, as a result, accelerate the <span class="hlt">sedimentation</span> velocity. The energy of the flow field in channels is sufficiently strong to erode their walls. The upward movement of network fragments in channels is manifested by erratic fluctuations of the conductivity. The main conclusion, which may be drawn from the results of this study, is that the phase separation of blood is associated with the formation of plasma channels within the <span class="hlt">sedimenting</span> dispersed phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25975438','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25975438"><span><span class="hlt">Sediment</span> Dynamics Within Buffer <span class="hlt">Zone</span> and Sinkhole Splay Areas Under Extreme Soil Disturbance Conditions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schoonover, Jon E; Crim, Jackie F; Williard, Karl W J; Groninger, John W; Zaczek, James J; Pattumma, Klairoong</p> <p>2015-09-01</p> <p><span class="hlt">Sedimentation</span> dynamics were assessed in sinkholes within training areas at Ft. Knox Military Installation, a karst landscape subjected to decades of tracked vehicle use and extreme soil disturbance. Sinkholes sampled were <span class="hlt">sediment</span>-laden and behaved as intermittent ponds. Dendrogeomorphic analyses were conducted using willow trees (Salix spp.) located around the edge of 18 sinkholes to estimate historical <span class="hlt">sedimentation</span> rates, and buried bottles were installed in 20 sinkholes at the center, outer edge, and at the midpoint between the center and edge to estimate annual <span class="hlt">sedimentation</span> rates. <span class="hlt">Sedimentation</span> data were coupled with vegetation characteristics of sinkhole buffers to determine relationships among these variables. The dendrogeomorphic method estimated an average accumulation rate of 1.27 cm year(-1) translating to a <span class="hlt">sediment</span> loss rate of 46.1 metric ton year(-1) from the training areas. However, <span class="hlt">sediment</span> export to sinkholes was estimated to be much greater (118.6 metric ton year(-1)) via the bottle method. These data suggest that the latter method provided a more accurate estimate since accumulation was greater in the center of sinkholes compared to the periphery where dendrogeomorphic data were collected. Vegetation data were not tightly correlated with <span class="hlt">sedimentation</span> rates, suggesting that further research is needed to identify a viable proxy for direct measures of <span class="hlt">sediment</span> accumulation in this extreme deposition environment. Mitigation activities for the sinkholes at Ft. Knox's tank training area, and other heavily disturbed karst environments where extreme <span class="hlt">sedimentation</span> exists, should consider focusing on flow path and splay area management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009Geomo.113..129C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009Geomo.113..129C"><span>Diagnostic heavy minerals in Plio-Pleistocene <span class="hlt">sediments</span> of the Yangtze Coast, China with special reference to the Yangtze River connection into the sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Jing; Wang, Zhanghua; Chen, Zhongyuan; Wei, Zixin; Wei, Taoyuan; Wei, Wei</p> <p>2009-12-01</p> <p>This present study revealed five heavy mineral <span class="hlt">zones</span> in the Yangtze coastal borehole <span class="hlt">sediments</span>. Ilmenite, garnet and zircon suite of <span class="hlt">Zone</span> I of the Pliocene characterizes the derivation of basaltic bedrock and local andesitic-granitic rocks. Indicative limonite in the <span class="hlt">Zone</span> I <span class="hlt">sediments</span> formed as alluvial fan facies shows strong chemical weathering. The assemblage of amphibole, straurolite, kyanite and idocrase of metamorphic derivation, together with a few zircon and tourmaline of andesitic-granitic origin in <span class="hlt">Zone</span> II, represents the extension of <span class="hlt">sediment</span> sources to the lower and middle Yangtze basin in Early Pleistocene as the study area subsided. Also, the braided to meandering riverine facies demonstrates a longer distance <span class="hlt">sediment</span> transport. Few heavy minerals remained in <span class="hlt">Zone</span> III of Mid-Pleistocene, when mottled thicker stiff mud occurred as the lacustrine facies, suggesting a quasi-coastal floodplain with lower capability of <span class="hlt">sediment</span> transport. Heavy minerals appeared significant and continuous in <span class="hlt">Zone</span> IV of Late Pleistocene, when changing to the shallow marine facies, inferring much extended <span class="hlt">sediment</span> sources to the upper Yangtze. Hypersthene, identified primarily in <span class="hlt">Zone</span> IV, was closely associated with the Er-Mei Mountain tholeiite basalt of the upper Yangtze. Heavy minerals of <span class="hlt">Zone</span> V remained almost the same as IV during Holocene, when the modern delta evolved. The heavy minerals suggested the timing of the Yangtze connection to the sea at ca 0.12 Ma BP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H11H..05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H11H..05L"><span>Size matters: The effects of displacement magnitude on the fluid flow properties of faults in poorly lithified <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loveless, S. E.; Bense, V.; Turner, J.</p> <p>2011-12-01</p> <p>Many aquifers worldwide occur in poorly lithified <span class="hlt">sediments</span>, often in regions that experience active tectonic deformation. Faulting of these <span class="hlt">sediments</span> introduces heterogeneities that may affect aquifer porosity and permeability, and consequently subsurface fluid flow and groundwater storage. The specific hydrogeological effects of faults depend upon the fault architecture and deformation mechanisms. These are controlled by factors such as rheology, stratigraphy and burial depth. Here, we analyse fault permeability in poorly lithified <span class="hlt">sediments</span> as a function of fault displacement. We have carried out detailed outcrop studies of minor normal faults at five study sites within the rapidly extending Corinth rift, Central Greece. Gravel conglomerates of giant Gilbert delta facies form productive but localised shallow aquifers within the region. Exposures reveal dense (average 20 faults per 100 m) networks of minor (0.1 to 50 m displacement) normal faults within the uplifted sequences, proximal to many of the crustal-scale normal faults. Analysis of 42 faults shows that fault <span class="hlt">zones</span> are primarily composed of smeared beds that can either retain their definition or mix with surrounding <span class="hlt">sediment</span>. Lenses or blocks of <span class="hlt">sediment</span> are common in fault <span class="hlt">zones</span> that cut beds with contrasting rheology, and a few faults have a clay core and/or damage <span class="hlt">zone</span>. Fault thickness increases at a rate of about 0.4 m per 10 m increase in displacement. Comparison of <span class="hlt">sediment</span> micro-structures from the field, hand samples and thin sections show grain-scale <span class="hlt">sediment</span> mixing, fracturing of clasts, and in some cases cementation, within fault <span class="hlt">zones</span>. In faults with displacements >12 m we also find a number of roughly parallel, highly indurated shear planes, up to 20 mm in thickness, composed of highly fragmented clasts and a fine grained matrix. Image analysis of thin sections from hand samples collected in the field was used to quantify the porosity of fault <span class="hlt">zones</span> and adjacent undeformed <span class="hlt">sediment</span>. These</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70156063','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70156063"><span>Recovery of <span class="hlt">sediment</span> characteristics in moraine, headwater streams of northern Minnesota after forest harvest</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vondracek, Bruce C.; Merten, Eric C.; Hemstad, Nathaniel A.; Kolka, Randall K.; Newman, Raymond M.; Verry, Elon S.</p> <p>2010-01-01</p> <p>We investigated the recovery of <span class="hlt">sediment</span> characteristics in four moraine, headwater streams in north-central Minnesota after forest harvest. We examined changes in fine <span class="hlt">sediment</span> levels from 1997 (preharvest) to 2007 (10 years postharvest) at study plots with upland clear felling and riparian thinning, using canopy cover, proportion of unstable banks, surficial fine substrates, residual pool depth, and streambed depth of refusal as response variables. Basin-scale year effects were significant (p < 0.001) for all responses when evaluated by repeated-measures ANOVAs. Throughout the study area, unstable banks increased for several years postharvest, coinciding with an increase in windthrow and fine <span class="hlt">sediment</span>. Increased unstable banks may have been caused by forest harvest equipment, increased windthrow and exposure of rootwads, or increased discharge and bank scour. Fine <span class="hlt">sediment</span> in the channels did not <span class="hlt">recover</span> by summer 2007, even though canopy cover and unstable banks had returned to 1997 levels. After several storm events in fall 2007, 10 years after the initial <span class="hlt">sediment</span> input, fine <span class="hlt">sediment</span> was flushed from the channels and returned to 1997 levels. Although our study design did not discern the source of the initial <span class="hlt">sediment</span> inputs (e.g., forest harvest, road crossings, other natural causes), we have shown that moraine, headwater streams can require an extended period (up to 10 years) and enabling event (e.g., high storm flows) to <span class="hlt">recover</span> from large inputs of fine <span class="hlt">sediment</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037293','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037293"><span>Recovery of <span class="hlt">sediment</span> characteristics in moraine, headwater streams of Northern Minnesota after forest harvest</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Merten, Eric C.; Hemstad, Nathaniel A.; Kolka, Randall K.; Newman, Raymond M.; Verry, Elon S.; Vondracek, Bruce C.</p> <p>2010-01-01</p> <p>We investigated the recovery of <span class="hlt">sediment</span> characteristics in four moraine, headwater streams in north-central Minnesota after forest harvest. We examined changes in fine <span class="hlt">sediment</span> levels from 1997 (preharvest) to 2007 (10 years postharvest) at study plots with upland clear felling and riparian thinning, using canopy cover, proportion of unstable banks, surficial fine substrates, residual pool depth, and streambed depth of refusal as response variables. Basin-scale year effects were significant (p < 0.001) for all responses when evaluated by repeated-measures ANOVAs. Throughout the study area, unstable banks increased for several years postharvest, coinciding with an increase in windthrow and fine <span class="hlt">sediment</span>. Increased unstable banks may have been caused by forest harvest equipment, increased windthrow and exposure of rootwads, or increased discharge and bank scour. Fine <span class="hlt">sediment</span> in the channels did not <span class="hlt">recover</span> by summer 2007, even though canopy cover and unstable banks had returned to 1997 levels. After several storm events in fall 2007, 10 years after the initial <span class="hlt">sediment</span> input, fine <span class="hlt">sediment</span> was flushed from the channels and returned to 1997 levels. Although our study design did not discern the source of the initial <span class="hlt">sediment</span> inputs (e.g., forest harvest, road crossings, other natural causes), we have shown that moraine, headwater streams can require an extended period (up to 10 years) and enabling event (e.g., high storm flows) to <span class="hlt">recover</span> from large inputs of fine <span class="hlt">sediment</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20390851','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20390851"><span>Evaluation of toxicity of polluted marine <span class="hlt">sediments</span> from Bahia Salina Cruz, Mexico.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gonzalez-Lozano, Maria Cristina; Mendez-Rodriguez, Lia C; Maeda-Martinez, Alejandro M; Murugan, Gopal; Vazquez-Botello, Alfonso</p> <p>2010-01-01</p> <p>Bahia Salina Cruz, Oaxaca, Mexico is a major center of oil and refined product distribution on the Mexican Pacific coast. From the start of oil industry operations in 1979, negative effects from discharges of treated effluents in the bay have been a constant concern for local communities. We analyzed 28 surface <span class="hlt">sediment</span> samples obtained in June, 2002 to evaluate the level of toxicity in the littoral <span class="hlt">zone</span>, port-harbor, and La Ventosa estuary in Bahia Salina Cruz. The extractable organic matter concentration was high (1,213 to 7,505 micro g g(-1)) in 5 of 7 stations from the port and harbor, whereas it was low in 12 of 16 stations in the littoral <span class="hlt">zone</span> (36 to 98 micro g g(-1)). The total aromatic hydrocarbon concentration was highest (57 to 142 micro g g(-1)) in the port and harbor compared to the La Ventosa estuary and the littoral <span class="hlt">zone</span>. Among the heavy metals analyzed, cadmium exceeded the effects range-low values associated with adverse biological effects. The geo-accumulation index of <span class="hlt">sediments</span> was moderate to strong contamination at 5 stations in the nonlittoral and 6 stations in the littoral <span class="hlt">zone</span>. The enrichment of lead, zinc, and cadmium at 5 stations from the littoral, port, and harbor suggest that these metals are of anthropogenic origin. Bioassay tests of elutriates of <span class="hlt">sediments</span> on nauplii of Artemia franciscana and Artemia sp. showed that the port and harbor were more toxic than the La Ventosa estuary and the coastal <span class="hlt">zone</span>. The Microtox test (Vibrio fischeri) did not show a similar response with the solid phase of the <span class="hlt">sediments</span>. The results of this study indicate that the high levels of organic content and metals in the <span class="hlt">sediments</span> of port-harbor and the La Ventosa estuary are mainly caused by anthropogenic activities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFM.T22B1144W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFM.T22B1144W"><span>Physical Properties of <span class="hlt">Sediment</span> Related to Gas Hydrate in the Northern Gulf of Mexico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winters, W. J.; Novosel, I.; Boldina, O. M.; Waite, W. F.; Lorenson, T. D.; Paull, C. K.; Bryant, W.</p> <p>2002-12-01</p> <p>Eighteen giant piston cores, up to 38-m long, were <span class="hlt">recovered</span> during July 2002 to determine the distribution of gas hydrate in widely different geologic environments of the Northern Gulf of Mexico. Physical properties, including electrical resistivity, three different shear strengths, P-wave velocity, and thermal conductivity were measured on split and whole-round cores at sea. Water content, grain density, and related properties are being determined in a shore-based laboratory from shipboard-acquired subsamples. These physical property data are important for two primary reasons: (1) to relate the presence of gas hydrate to the natural host <span class="hlt">sediment</span>; and (2) to correlate with shallow seismic reflection records so they can be interpreted more accurately within and below the depth of coring. Preliminary results indicate that porosity and water content typically decrease rapidly to a subbottom depth of about 8 to 9 m, but then decrease at a much lower rate to the base of the core - often 30 or more mbsf. Although higher water contents are measured in the <span class="hlt">sediments</span> that were <span class="hlt">recovered</span> in association with gas hydrates, they are probably an artifact of post-sampling hydrate dissociation rather than an in-situ characteristic. The hydrate <span class="hlt">recovered</span> during the cruise, was present either as particles distributed throughout the <span class="hlt">sediment</span> or as massive chunks that filled the entire 10-cm diameter of the core liner. The <span class="hlt">sediments</span> immediately adjacent to the <span class="hlt">recovered</span> gas hydrates are visually similar to surrounding <span class="hlt">sediments</span>, and thus primary lithologic differences do not appear to control the distribution of these gas hydrates. Vane shear strength measurements correlate better to subbottom depth than to water content. The strength values typically increase from less than 10 kPa near the seafloor to as much as 80 to 90 kPa at the base of some cores. Electrical resistivity appears to be related to water content (and probably porewater salinity) since a break in slope with depth is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JVGR..341...84K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JVGR..341...84K"><span>Fluidization of host <span class="hlt">sediments</span> and its impacts on peperites-forming processes, the Cretaceous Buan Volcanics, Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kwon, Chang Woo; Gihm, Yong Sik</p> <p>2017-07-01</p> <p>In the Cretaceous Buan Volcanics (SW Korea), blocky and fluidal peperites are developed in a bed of poorly sorted, massive pumiceous lapilli tuff (hot <span class="hlt">sediments</span>) as a result of the vertical to subvertical intrusion of the trachyandesitic dikes into the bed. Blocky peperites are composed of polyhedral or platy juvenile clasts with a jigsaw-crack texture. Fluidal peperites are characterized by fluidal or globular juvenile clasts with irregular or ragged margins. The blocky peperites are ubiquitous in the host <span class="hlt">sediments</span>, whereas the fluidal peperites only occur in fine-grained <span class="hlt">zone</span> (well sorted fine to very fine ash) that are aligned parallel to the dike margin. The development of the fine-grained <span class="hlt">zone</span> within the poorly sorted host <span class="hlt">sediments</span> is interpreted to form by grain size segregation caused by upward moving pore water (fluidization) that has resulted from heat transfer from intruding magma toward the waterlogged host <span class="hlt">sediments</span> during intrusion. With the release of pore water and the selective entrainment of fine-grained ash, the fine-grained <span class="hlt">zone</span> formed within the host <span class="hlt">sediments</span>. Subsequent interactions between the fine-grained <span class="hlt">zone</span> and the intruding magma resulted in ductile deformation of the magma, which generated fluidal peperites. Outside the fine-grained <span class="hlt">zone</span>, because of the relative deficiency of both pore water and fine-grained ash, intruding magma fragmented in a brittle manner, resulting in the formation of blocky peperites. The results of this study suggest that redistribution of constituent particles (ash) and interstitial fluids during fluidization resulted in heterogeneous physical conditions of the host <span class="hlt">sediments</span>, which influenced peperite-forming processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/15010322','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/15010322"><span>Characterization of Vadose <span class="hlt">Zone</span> <span class="hlt">Sediment</span>: Borehole 299-E33-46 Near Tank B-110 in the B-BX-BY Waste Management Area.</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Serne, R. Jeffrey; Bjornstad, Bruce N.; Gee, Glendon W.</p> <p>2002-12-15</p> <p>This report presents vadose <span class="hlt">sediment</span> characterization data that improves understanding of the nature and extent of past releases in the B tank farm. A vertical borehole, located approximately 15 ft (5 m) from the northeast edge of single-shell tank 241-B-110 was drilled to a total depth of 264.4 ft bgs, the groundwater table was encountered at 255.8 ft bgs. During drilling, a total of 3 two-ft long, 4-inch diameter split-spoon core samples were collected between 10 and 254 ft bgs-an average of every 7.5 ft. Grab samples were collected between these core sample intervals to yield near continuous samples tomore » a depth of 78.3 m (257 ft). Geologic logging occurred after each core segment was emptied into an open plastic container, followed by photographing and sub-sampling for physical and chemical characterization. In addition, 54 out of a total of 120 composite grab samples were opened, sub-sampled, logged, and photographed. Immediately following the geologic examination, the core and selected grab samples were sub-sampled for moisture content, gamma-emission radiocounting, tritium and strontium-90 determinations, total carbon and inorganic carbon content, and 8 M nitric acid extracts (which provide a measure of the total leachable <span class="hlt">sediment</span> content of contaminants) and one-to-one <span class="hlt">sediment</span> to water extracts (which provide soil pH, electrical conductivity, cation, and anion data and water soluble contaminant data. Later, additional aliquots of selected sleeves or grab samples were removed to measure particle size distribution and mineralogy and to squeeze porewater. Major conclusions follow. Vadose <span class="hlt">zone</span> contamination levels were lower than generally anticipated prior to the initiation of the field investigation. Strong evidence of extensive vadose <span class="hlt">zone</span> lateral migration in WMA BBXBY exists. There are indications that such lateral migration may have extended into WMA B-BX-BY from adjacent past practice discharge sites. Ponding of runoff from natural precipitation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999QSRv...18.1445D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999QSRv...18.1445D"><span>Recent <span class="hlt">sediment</span> remolding on a deep shelf, Ross Sea: implications for radiocarbon dating of Antarctic marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Domack, Eugene W.; Taviani, Marco; Rodriguez, Anthonio</p> <p>1999-11-01</p> <p>Coarse, bioclastic rich sands have been widely reported from the banks of the Antarctic continental shelf but their origin is still poorly known. We report on a suite of coarse <span class="hlt">sediments</span> <span class="hlt">recovered</span> from the top of the Mawson Bank in the northwestern Ross Sea. Radiocarbon ages of biogenic calcite, for modern and apparently late Pleistocene deposits, range from 1085±45 to 20,895±250 yr B.P.. Discovery of soft tissue (Ascidian) preserved as an incrustation on a pebble at 2 m depth indicates aggregation of the <span class="hlt">sediment</span> within several months or a year of core recovery. Radiocarbon ages of acid insoluble organic matter (aiom) are less than those of the foraminifera calcite. The aiom ages are also reversed in sequence, indicating reworking of the <span class="hlt">sediment</span> during deposition. These observations and a review of recently published literature suggest that much of the bank top <span class="hlt">sediment</span> in Antarctica is presently undergoing remobilization, under the influence of strong currents and/or icebergs even under interglacical (high-stand) sea levels. These observations point out the need for careful, integrated studies on high latitude marine <span class="hlt">sediment</span> cores before resultant "ages" alone are used as the foundation for paleoglacial reconstructions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011GCarp..62..233I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011GCarp..62..233I"><span>Biostratigraphy and paleoecology of the Burdigalian-Serravallian <span class="hlt">sediments</span> in Wadi Sudr (Gulf of Suez, Egypt): comparison with the Central Paratethys evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ied, Ibrahim M.; Holcová, Katarína; Abd-Elshafy, Ezzat</p> <p>2011-06-01</p> <p>Two main Miocene facies were recorded in the Gulf of Suez area: a deep marine and a coastal facies. The analysed sections in the Wadi Sudr area belong to the marine facies. The Lower Miocene (Burdigalian) is represented by coastal, shallow marine <span class="hlt">sediments</span>, rich in coral, algae, gastropods and large pectinids followed by Langhian open marine <span class="hlt">sediments</span> and Serravallian lagoonal carbonates. The open marine <span class="hlt">sediments</span> contain well preserved planktonic and benthic foraminifers and abundant ostracods. The parts of the sections containing foraminifers have been correlated with three planktonic foraminiferal <span class="hlt">zones</span> (<italic>Praeorbulina glomerosa <span class="hlt">Zone</span>, Orbulina <span class="hlt">Zone</span></italic> and <italic>Globorotalia praemenardii-Globorotalia peripheroronda</italic> <span class="hlt">Zone</span>). Two benthic ecozones were defined (<italic>Heterolepa dutemplei-Laevidentalina elegans <span class="hlt">Zone</span></italic> and <italic>Bolivina compressa-Elphidium</italic> spp. <span class="hlt">Zone</span>). Two cycles of sea-level changes can be distinguished and correlated with global sea-level cycles Bur5/Lan1 and Ser1. The first (Langhian) cycle culminated in open marine sublittoral to upper bathyal well aerated <span class="hlt">sediments</span>. The second (Serravallian) cycle was shallower, littoral suboxic <span class="hlt">sediments</span> were overlaid by euryhaline carbonates. The studied foraminifera-bearing <span class="hlt">sediments</span> can be correlated with the lower and Middle Badenian of the Central Paratethys. Though the area of the Gulf of Suez and the Central Paratethys were situated in different climatic <span class="hlt">zones</span>, and influenced by different tectonic events, the main paleoenvironmental events (sea-level changes, oxygen decrease, salinity changes) are comparable. This correspondence shows that the decisive factors triggering these events were global climatic events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70148294','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70148294"><span>Bacterial dominance in subseafloor <span class="hlt">sediments</span> characterized by methane hydrates</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Briggs, Brandon R.; Inagaki, Fumio; Morono, Yuki; Futagami, Taiki; Huguet, Carme; Rosell-Mele, Antoni; Lorenson, T.D.; Colwell, Frederick S.</p> <p>2015-01-01</p> <p>The degradation of organic carbon in subseafloor <span class="hlt">sediments</span> on continental margins contributes to the largest reservoir of methane on Earth. <span class="hlt">Sediments</span> in the Andaman Sea are composed of ~ 1% marine-derived organic carbon and biogenic methane is present. Our objective was to determine microbial abundance and diversity in <span class="hlt">sediments</span> that transition the gas hydrate occurrence <span class="hlt">zone</span> (GHOZ) in the Andaman Sea. Microscopic cell enumeration revealed that most <span class="hlt">sediment</span> layers harbored relatively low microbial abundance (103–105 cells cm−3). Archaea were never detected despite the use of both DNA- and lipid-based methods. Statistical analysis of terminal restriction fragment length polymorphisms revealed distinct microbial communities from above, within, and below the GHOZ, and GHOZ samples were correlated with a decrease in organic carbon. Primer-tagged pyrosequences of bacterial 16S rRNA genes showed that members of the phylum Firmicutes are predominant in all <span class="hlt">zones</span>. Compared with other seafloor settings that contain biogenic methane, this deep subseafloor habitat has a unique microbial community and the low cell abundance detected can help to refine global subseafloor microbial abundance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS44A..08H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS44A..08H"><span><span class="hlt">Sediment</span>-pore water interactions controlling cementation in the NanTroSEIZE drilling transects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hong, W.; Spinelli, G. A.; Torres, M. E.</p> <p>2012-12-01</p> <p>One goal of the Nankai Trough Seismogenic <span class="hlt">Zone</span> Experiment (NanTroSEIZE) is to understand how changes in subducting <span class="hlt">sediment</span> control the transition from aseismic to seismogenic behavior in subduction <span class="hlt">zones</span>. In the <span class="hlt">sediment</span> entering the Nankai subduction <span class="hlt">zone</span>, dramatic changes in physical and chemical properties occur across a diagenetic boundary; they are thought to affect <span class="hlt">sediment</span> strength and deformation. The dissolution of disseminated volcanic ash and precipitation of silica cement may be responsible for these changes in physical properties, but the mechanism controlling cementation was unclear (Spinelli et al., 2007). In this study, we used CrunchFlow (Steefel, 2009) to simulate chemical reactions and fluid flow through 1-D <span class="hlt">sediment</span> columns at Integrated Ocean Drilling Program (IODP) sites on the incoming plate in Nankai Trough. The simulations include the thermodynamics and kinetics of <span class="hlt">sediment</span>-water interactions, advection of pore water and <span class="hlt">sediment</span> due to compaction, and multi-component diffusion in an accumulating <span class="hlt">sediment</span> column. Key reactions in the simulations are: ash dissolution, amorphous silica precipitation and dissolution, and zeolite precipitation. The rate of ash decomposition was constrained using Sr isotope data of Joseph et al. (2012). Our model reproduces the distinct diagenetic boundary observed in <span class="hlt">sediment</span> and pore water chemistry, which defines two <span class="hlt">zones</span>. Above this boundary (<span class="hlt">zone</span> 1), dissolved and amorphous silicate contents are high and the potassium concentration remains near seawater values or gradually decreases toward the boundary. Below the boundary, both dissolved and amorphous silicate content drop rapidly, concomitant with a decrease in dissolved potassium. Our model shows that these changes in the system are driven by formation of clinoptilolite in response to changes in pore fluid pH. The low pH values (<7.6) above the diagenetic boundary accelerate ash decomposition and maintain clinoptilolite slightly undersaturated. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=308452&Lab=NRMRL&keyword=State+AND+flow&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=308452&Lab=NRMRL&keyword=State+AND+flow&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Quantifying Seepage Flux using <span class="hlt">Sediment</span> Temperatures</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>This report provides a demonstration of different modeling approaches that use <span class="hlt">sediment</span> temperatures to estimate the magnitude and direction of water flux across the groundwater-surface water transition <span class="hlt">zone</span>. Analytical models based on steady-state or transient temperature solut...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S43C2250H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S43C2250H"><span><span class="hlt">Recovering</span> the slip history of a scenario earthquake in the Mexican subduction <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hjorleifsdottir, V.; Perez-Campos, X.; Iglesias, A.; Cruz-Atienza, V.; Ji, C.; Legrand, D.; Husker, A. L.; Kostoglodov, V.; Valdes Gonzalez, C.</p> <p>2011-12-01</p> <p>The Guerrero segment of the Mexican subduction <span class="hlt">zone</span> has not experienced a large earthquake for almost 100 years (Singh et al., 1981). Due to its proximity to Mexico City, which was devastated by an earthquake in the more distant Michoacan segment in 1985, it has been studied extensively in recent years. Silent slip events have been observed by a local GPS network (Kostoglodov et al. 2003) and seismic observations from a dense linear array of broadband seismometers (MASE) have provided detailed images of the crustal structure of this part of the subduction <span class="hlt">zone</span> (see for example Pérez-Campos et al., 2008, Iglesias et al., 2010). Interestingly the part of the fault <span class="hlt">zone</span> that is locked during the inter-seismic period is thought to reach up to or inland from the coast line. In the event of a large megathrust earthquake, this geometry could allow recordings from above the fault interface. These types of recordings can be critical to resolve the history of slip as a function of time on the fault plane during the earthquake. A well constrained model of slip-time history, together with other observations as mentioned above, could provide very valuable insights into earthquake physics and the earthquake cycle. In order to prepare the scientific response for such an event we generate a scenario earthquake in the Guerrero segment of the subduction <span class="hlt">zone</span>. We calculate synthetic strong motion records, seismograms for global stations and static offsets on the Earth's surface. To simulate the real data available we add real noise, recorded during times of no earthquake, to the synthetic data. We use a simulated annealing inversion algorithm (Ji et al., 1999) to invert the different datasets and combinations thereof for the time-history of slip on the fault plane. We present the recovery of the slip model using the different datasets, as well as idealized datasets, investigating the expected and best possible levels of recovery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29100638','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29100638"><span>Presence, concentrations and risk assessment of selected antibiotic residues in <span class="hlt">sediments</span> and near-bottom waters collected from the Polish coastal <span class="hlt">zone</span> in the southern Baltic Sea - Summary of 3years of studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siedlewicz, Grzegorz; Białk-Bielińska, Anna; Borecka, Marta; Winogradow, Aleksandra; Stepnowski, Piotr; Pazdro, Ksenia</p> <p>2018-04-01</p> <p>Concentrations of selected antibiotic compounds from different groups were measured in <span class="hlt">sediment</span> samples (14 analytes) and in near-bottom water samples (12 analytes) collected in 2011-2013 from the southern Baltic Sea (Polish coastal <span class="hlt">zone</span>). Antibiotics were determined at concentration levels of a few to hundreds of ng g -1 d.w. in <span class="hlt">sediments</span> and ng L -1 in near-bottom waters. The most frequently detected compounds were sulfamethoxazole, trimethoprim, oxytetracycline in <span class="hlt">sediments</span> and sulfamethoxazole and trimethoprim in near-bottom waters. The occurrence of the identified antibiotics was characterized by spatial and temporal variability. A statistically important correlation was observed between <span class="hlt">sediment</span> organic matter content and the concentrations of sulfachloropyridazine and oxytetracycline. Risk assessment analyses revealed a potential high risk of sulfamethoxazole contamination in near-bottom waters and of contamination by sulfamethoxazole, trimethoprim and tetracyclines in <span class="hlt">sediments</span>. Both chemical and risk assessment analyses show that the coastal area of the southern Baltic Sea is highly exposed to antibiotic residues. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T11H..04P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T11H..04P"><span>Variations in fluid transport and seismogenic properties in the Lesser Antilles subduction <span class="hlt">zone</span>: constraints from joint active-source and local earthquake tomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Paulatto, M.; Laigle, M.; Charvis, P.; Galve, A.</p> <p>2015-12-01</p> <p>The degree of coupling and the seismogenic properties of the plate interface at subduction <span class="hlt">zones</span> are affected by the abundance of slab fluids and subducted <span class="hlt">sediments</span>. High fluid input can cause high pore-fluid pressures in the subduction channel and decrease coupling leading to aseismic behaviour. Constraining fluid input and transfer is therefore important for understanding plate coupling and large earthquake hazard, particularly in places where geodetic and seismological constraints are scarce. We use P-wave traveltimes from several active source seismic experiments and P- and S-wave traveltimes from shallow and intermediate depth (< 150 km) local earthquakes recorded on a vast amphibious array of OBSs and land stations to <span class="hlt">recover</span> the Vp and Vp/Vs structure of the central Lesser Antilles subduction <span class="hlt">zone</span>. Our model extends between Martinique and Antigua from the prism to the arc and from the surface to a depth of 160 km. We find low Vp and high Vp/Vs ratio (> 1.80) on the top of the slab, at depths of up to 100 km. We interpret this high Vp/Vs ratio anomaly as evidence of elevated fluid content either as free fluids or as bound fluids in hydrated minerals (e.g. serpentinite). The strength and depth extent of the anomaly varies strongly from south to north along the subduction <span class="hlt">zone</span> and correlates with variations in forearc morphology and with <span class="hlt">sediment</span> input constrained by multi-channel seismic reflection profiles. The anomaly is stronger and extends to greater depth in the south, offshore Martinique, where <span class="hlt">sediment</span> input is elevated due to the vicinity of the Orinoco delta. The gently dipping forearc slope observed in this region may be the result of weak coupling of the plate interface. A high Vp/Vs ratio is also observed in the forearc likely indicating a fractured and water-saturated overriding plate. On the other hand the anomaly is weaker and shallower offshore Guadeloupe, where <span class="hlt">sediment</span> input is low due to subduction of the Barracuda ridge. Here a strong</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA629218','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA629218"><span>Flow and Suspended <span class="hlt">Sediment</span> Events in the Near-Coastal <span class="hlt">Zone</span> off Corpus Christi, Texas</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2003-09-30</p> <p>redistribution of preexisting shelf <span class="hlt">sediments</span> during storms and (2) transportation of suspended <span class="hlt">sediment</span> from the adjacent bay- lagoon system. Snedden et al...and K.E. Schmedes. (1983). Submerged lands of Texas, Corpus Christi area: <span class="hlt">sediments</span>, geochemistry, benthic macroinvertebrates and associated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7085B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7085B"><span>Temperature, productivity and <span class="hlt">sediment</span> characteristics as drivers of seasonal and spatial variations of dissolved methane in the near-shore coastal areas (Belgian coastal <span class="hlt">zone</span>, North Sea)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Borges, Alberto V.; Speeckaert, Gaëlle; Champenois, Willy; Scranton, Mary I.; Gypens, Nathalie</p> <p>2017-04-01</p> <p>The open ocean is a modest source of CH4 to the atmosphere compared to other natural and anthropogenic CH4 emissions. Coastal regions are more intense sources of CH4 to the atmosphere than open oceanic waters, in particular estuarine <span class="hlt">zones</span>. The CH4 emission to the atmosphere from coastal areas is sustained by riverine inputs and methanogenesis in the <span class="hlt">sediments</span> due to high organic matter (OM) deposition. Additionally, natural gas seeps are sources of CH4 to bottom waters leading to high dissolved CH4 concentrations in bottom waters (from tenths of nmol L-1 up to several µmol L-1). We report a data set of dissolved CH4 concentrations obtained at nine fixed stations in the Belgian coastal <span class="hlt">zone</span> (Southern North Sea), during one yearly cycle, with a bi-monthly frequency in spring, and a monthly frequency during the rest of the year. This is a coastal area with multiple possible sources of CH4 such as from rivers and gassy <span class="hlt">sediments</span>, and where intense phytoplankton blooms are dominated by the high dimethylsulfoniopropionate (DMSP) producing micro-algae Phaeocystis globosa, leading to DMSP and dimethylsulfide (DMS) concentrations. Furthermore, the BCZ is a site of important OM <span class="hlt">sedimentation</span> and accumulation unlike the rest of the North Sea. Spatial variations of dissolved CH4 concentrations were very marked with a minimum yearly average of 9 nmol L-1 in one of the most off-shore stations and maximum yearly average of 139 nmol L-1 at one of the most near-shore stations. The spatial variations of dissolved CH4 concentrations were related to the organic matter (OM) content of <span class="hlt">sediments</span>, although the highest concentrations seemed to also be related to inputs of CH4 from gassy <span class="hlt">sediments</span> associated to submerged peat. In the near-shore stations with fine sand or muddy <span class="hlt">sediments</span> with a high OM content, the seasonal cycle of dissolved CH4 concentration closely followed the seasonal cycle of water temperature, suggesting the control of methanogenesis by temperature in these OM</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.4117D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4117D"><span>Optimization of remediation strategies using vadose <span class="hlt">zone</span> monitoring systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dahan, Ofer</p> <p>2016-04-01</p> <p>In-situ bio-remediation of the vadose <span class="hlt">zone</span> depends mainly on the ability to change the subsurface hydrological, physical and chemical conditions in order to enable development of specific, indigenous, pollutants degrading bacteria. As such the remediation efficiency is much dependent on the ability to implement optimal hydraulic and chemical conditions in deep sections of the vadose <span class="hlt">zone</span>. These conditions are usually determined in laboratory experiments where parameters such as the chemical composition of the soil water solution, redox potential and water content of the <span class="hlt">sediment</span> are fully controlled. Usually, implementation of desired optimal degradation conditions in deep vadose <span class="hlt">zone</span> at full scale field setups is achieved through infiltration of water enriched with chemical additives on the land surface. It is assumed that deep percolation into the vadose <span class="hlt">zone</span> would create chemical conditions that promote biodegradation of specific compounds. However, application of water with specific chemical conditions near land surface dose not necessarily results in promoting of desired chemical and hydraulic conditions in deep sections of the vadose <span class="hlt">zone</span>. A vadose-<span class="hlt">zone</span> monitoring system (VMS) that was recently developed allows continuous monitoring of the hydrological and chemical properties of deep sections of the unsaturated <span class="hlt">zone</span>. The VMS includes flexible time-domain reflectometry (FTDR) probes which allow continuous monitoring of the temporal variation of the vadose <span class="hlt">zone</span> water content, and vadose-<span class="hlt">zone</span> sampling ports (VSPs) which are designed to allow frequent sampling of the <span class="hlt">sediment</span> pore-water and gas at multiple depths. Implementation of the vadose <span class="hlt">zone</span> monitoring system in sites that undergoes active remediation provides real time information on the actual chemical and hydrological conditions in the vadose <span class="hlt">zone</span> as the remediation process progresses. Up-to-date the system has been successfully implemented in several studies on water flow and contaminant transport in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25412274','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25412274"><span>Iron-mediated anaerobic oxidation of methane in brackish coastal <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Egger, Matthias; Rasigraf, Olivia; Sapart, Célia J; Jilbert, Tom; Jetten, Mike S M; Röckmann, Thomas; van der Veen, Carina; Bândă, Narcisa; Kartal, Boran; Ettwig, Katharina F; Slomp, Caroline P</p> <p>2015-01-06</p> <p>Methane is a powerful greenhouse gas and its biological conversion in marine <span class="hlt">sediments</span>, largely controlled by anaerobic oxidation of methane (AOM), is a crucial part of the global carbon cycle. However, little is known about the role of iron oxides as an oxidant for AOM. Here we provide the first field evidence for iron-dependent AOM in brackish coastal surface <span class="hlt">sediments</span> and show that methane produced in Bothnian Sea <span class="hlt">sediments</span> is oxidized in distinct <span class="hlt">zones</span> of iron- and sulfate-dependent AOM. At our study site, anthropogenic eutrophication over recent decades has led to an upward migration of the sulfate/methane transition <span class="hlt">zone</span> in the <span class="hlt">sediment</span>. Abundant iron oxides and high dissolved ferrous iron indicate iron reduction in the methanogenic <span class="hlt">sediments</span> below the newly established sulfate/methane transition. Laboratory incubation studies of these <span class="hlt">sediments</span> strongly suggest that the in situ microbial community is capable of linking methane oxidation to iron oxide reduction. Eutrophication of coastal environments may therefore create geochemical conditions favorable for iron-mediated AOM and thus increase the relevance of iron-dependent methane oxidation in the future. Besides its role in mitigating methane emissions, iron-dependent AOM strongly impacts sedimentary iron cycling and related biogeochemical processes through the reduction of large quantities of iron oxides.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/25043','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/25043"><span>Dicamptodon tenebrosus larvae within hyporheic <span class="hlt">zones</span> of intermittent streams in California</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>David Feral; Michael A. Camann; Hartwell H. Welsh Jr.</p> <p>2005-01-01</p> <p>Lotic ecosystems are increasingly viewed as having three interactive spatial compartments, i.e., channel <span class="hlt">sediments</span>, the hyporheic <span class="hlt">zone</span>, and flood plains or riparian areas (Cummins et al. 1983; Ward 1989). The hyporheic <span class="hlt">zone</span> is the sub-benthic habitat of interstitial spaces between substrate particles in the stream bed, and is the transition <span class="hlt">zone</span> between surface flow...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24377871','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24377871"><span>Seasonal arsenic accumulation in stream <span class="hlt">sediments</span> at a groundwater discharge <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>MacKay, Allison A; Gan, Ping; Yu, Ran; Smets, Barth F</p> <p>2014-01-21</p> <p>Seasonal changes in arsenic and iron accumulation rates were examined in the <span class="hlt">sediments</span> of a brook that receives groundwater discharges of arsenic and reduced iron. Clean glass bead columns were deployed in <span class="hlt">sediments</span> for known periods over the annual hydrologic cycle to monitor changes in arsenic and iron concentrations in bead coatings. The highest accumulation rates occurred during the dry summer period (July-October) when groundwater discharges were likely greatest at the sample locations. The intermediate flow period (October-March), with higher surface water levels, was associated with losses of arsenic and iron from bead column coatings at depths below 2-6 cm. Batch incubations indicated iron releases from solids to be induced by biological reduction of iron (oxy)hydroxide solids. Congruent arsenic releases during incubation were limited by the high arsenic sorption capacity (0.536 mg(As)/mg(Fe)) of unreacted iron oxide solids. The flooded spring (March-June) with high surface water flows showed the lowest arsenic and iron accumulation rates in the <span class="hlt">sediments</span>. Comparisons of accumulation rates across a shoreline transect were consistent with greater rates at regions exposed above surface water levels for longer times and greater losses at locations submerged below surface water. Iron (oxy)hydroxide solids in the shallowest <span class="hlt">sediments</span> likely serve as a passive barrier to sorb arsenic released to pore water at depth by biological iron reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.5284D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.5284D"><span>New data concerning the geochemistry of unconsolidated <span class="hlt">sediments</span> collected from the anoxic <span class="hlt">zone</span> of the Black Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duliu, Octavian G.; Cristache, Carmen; Florea, Nelida; Oaie, Gheorghe; Culicov, Otilia A.; Frontasyeva, Marina V.</p> <p>2010-05-01</p> <p>The content of eight major, rock forming elements (Na, Cl, Al, Si, K, Ca, Ti, Fe) and 34 trace elements (B, S, Sc, V, Cr, Mn, Co, Ni, Zn, As, Se, Br, Rb, Sr, Zr, Mo, Sn, Sb, Cs, Ba, La, Ce, Nd, Sm, Eu, Gd, Tb, Dy, Yb, Hf, Ta, W, Th and U) were determined by Prompt Gamma and Epithermal Neutron Activation Analysis in 45 samples of the uppermost 50 cm of undisturbed <span class="hlt">sediments</span> collected from an anoxic continental <span class="hlt">zone</span> of the Black Sea at a depth of 600 m, off the City of Constanta. 137Cs geochronology has evidenced a <span class="hlt">sedimentation</span> ratio of 0,42 ± 0,12 mm/y which, by extrapolation to the entire 50 cm column gave an age of 1300 ± 300 y for the oldest <span class="hlt">sediments</span>. Principal Component Analysis (PCA), Sc-La-Th and Co-Hf-Th ternary diagrams as well as La/Th ratio were used to interpret these data in correlation with the corresponding ones for the Upper Continental Crust (UCC), North American Shale Composite (NASC), as well as Atlantic, Pacific and Indian MORBs. At the same time the Se/Al, Se/Sc, Se/Mn, Mo/Al, Mo/Sc and Mo/Mn, ratios were used as indicators for anoxic conditions along sedimentary core. Major components distribution showed, that excepting CaO, their contents are very close to UCC and NASC, while the Principal Component Analysis evidenced three clusters consisting of Na, K and Cl, Al, Ti and Fe and respectively Ca, in concordance with the <span class="hlt">sediments</span>' mineralogical composition. The Trace Elements Distribution was also close to UCC except for redox sensitive metals Se and Mo whose contents were 10 to 100 times higher than the corresponding UCC ones, this fact reflecting the anoxic conditions along the entire column of <span class="hlt">sediments</span>. Moreover, by using Se and Mo as proxies for an anoxic environment, we estimated a relative consistency of the local conditions for a period between 350 ± 60 and 1300 ± 300 BP followed by a more fluctuant one during the last 300 years, this peculiarity also being confirmed by PCA, as well as by the vertical distribution of La/Th ratio. A</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22990811','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22990811"><span>Effect of <span class="hlt">sediment</span> composition on methane concentration and production in the transition <span class="hlt">zone</span> of a mangrove (Sepetiba Bay, Rio de Janeiro, Brazil).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marinho, C C; Campos, E A; Guimarães, J R D; Esteves, F A</p> <p>2012-08-01</p> <p>The aim of this research was to evaluate the effect of <span class="hlt">sediment</span> composition on methane (CH4) dynamics in <span class="hlt">sediments</span> of different areas in the transition <span class="hlt">zone</span> between a mangrove and the sea. This research was conducted in a mangrove at Coroa Grande, on the southern coast of Rio de Janeiro. Samples were collected at three stations: (1) region colonised by Rhizophora mangle L. on the edge of the mangrove, (2) region colonised by seagrasses and (3) infra-littoral region without vegetation. Samples were collected from the surface layer of the <span class="hlt">sediment</span> to determine the concentrations of nutrients (C, N and P) and CH4 concentration and production. We observed that concentrations of CH4 and carbon (C) were significantly higher (p < 0.05) in station 1 than station 3. The molar ratios (C:N, C:P and N:P) suggest that the origin of the substrate is mainly autochthonous. Methanogenesis was initially low, possibly due to competition between methanogens and sulfate reducers, and increased significantly (p < 0.05) on the twenty-sixth day in the <span class="hlt">sediment</span> of station 1, probably due to higher organic matter (OM) availability in this region. Results indicate that methanogenic activity observed herein is not regulated by the amount or quality of OM, but by other factors. The concentration of CH4 in the sea-land ecotone at Mangrove Coroa Grande is a function of available OM suggesting a possible inhibition of methanotrophy by intense oxygen consumption in the soil surface covered by detritus of Rhizophora mangle vegetation.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1861c0045M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1861c0045M"><span>Magnetic properties of Surabaya river <span class="hlt">sediments</span>, East Java, Indonesia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mariyanto, Bijaksana, Satria</p> <p>2017-07-01</p> <p>Surabaya river is one of urban rivers in East Java Province, Indonesia that is a part of Brantas river that flows in four urban and industrial cities of Mojokerto, Gresik, Sidoarjo, and Surabaya. The urban populations and industries along the river pose serious threat to the river mainly for their anthropogenic pollutants. This study aims to characterize the magnetic properties of <span class="hlt">sediments</span> in various locations along Surabaya river and correlate these magnetic properties to the level of pollution along the river. Samples are taken and measured through a series of magnetic measurements. The mass-specific magnetic susceptibility of <span class="hlt">sediments</span> ranges from 259.4 to 1134.8 × 10-8 m3kg-1. The magnetic minerals are predominantly PSD to MD magnetite with the grain size range from 6 to 14 μm. The mass-specific magnetic susceptibility tends to decreases downstream as accumulation of magnetic minerals in <span class="hlt">sediments</span> is affected not only by the amount of household and industrial wastes but also by <span class="hlt">sediment</span> dredging, construction of embankments, and extensive erosion arround the river. <span class="hlt">Sediments</span> located in the industrial <span class="hlt">zone</span> on the upstream area tend to have higher mass-specific magnetic susceptibility than in the non-industrial <span class="hlt">zones</span> on the downstream area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035563','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035563"><span>Geomorphic evolution of the Le Sueur River, Minnesota, USA, and implications for current <span class="hlt">sediment</span> loading</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Gran, K.B.; Belmont, P.; Day, S.S.; Jennings, C.; Johnson, Aaron H.; Perg, L.; Wilcock, P.R.</p> <p>2009-01-01</p> <p>There is clear evidence that the Minnesota River is the major <span class="hlt">sediment</span> source for Lake Pepin and that the Le Sueur River is a major source to the Minnesota River. Turbidity levels are high enough to require management actions. We take advantage of the well-constrained Holocene history of the Le Sueur basin and use a combination of remote sensing, fi eld, and stream gauge observations to constrain the contributions of different <span class="hlt">sediment</span> sources to the Le Sueur River. Understanding the type, location, and magnitude of <span class="hlt">sediment</span> sources is essential for unraveling the Holocene development of the basin as well as for guiding management decisions about investments to reduce <span class="hlt">sediment</span> loads. Rapid base-level fall at the outlet of the Le Sueur River 11,500 yr B.P. triggered up to 70 m of channel incision at the mouth. Slope-area analyses of river longitudinal profi les show that knickpoints have migrated 30-35 km upstream on all three major branches of the river, eroding 1.2-2.6 ?? 109 Mg of <span class="hlt">sediment</span> from the lower valleys in the process. The knick <span class="hlt">zones</span> separate the basin into an upper watershed, receiving <span class="hlt">sediment</span> primarily from uplands and streambanks, and a lower, incised <span class="hlt">zone</span>, which receives additional <span class="hlt">sediment</span> from high bluffs and ravines. Stream gauges installed above and below knick <span class="hlt">zones</span> show dramatic increases in <span class="hlt">sediment</span> loading above that expected from increases in drainage area, indicating substantial inputs from bluffs and ravines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017WRR....53..799K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017WRR....53..799K"><span>Tidal controls on riverbed denitrification along a tidal freshwater <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Knights, Deon; Sawyer, Audrey H.; Barnes, Rebecca T.; Musial, Cole T.; Bray, Samuel</p> <p>2017-01-01</p> <p>In coastal rivers, tidal pumping enhances the exchange of oxygen-rich river water across the <span class="hlt">sediment</span>-water interface, controlling nitrogen cycling in riverbed <span class="hlt">sediment</span>. We developed a one-dimensional, fluid flow and solute transport model that quantifies the influence of tidal pumping on nitrate removal and applied it to the tidal freshwater <span class="hlt">zone</span> (TFZ) of White Clay Creek (Delaware, USA). In field observations and models, both oxygenated river water and anoxic groundwater deliver nitrate to carbon-rich riverbed <span class="hlt">sediment</span>. A <span class="hlt">zone</span> of nitrate removal forms beneath the aerobic interval, which expands and contracts over daily timescales due to tidal pumping. At high tide when oxygen-rich river water infiltrates into the bed, denitrification rates decrease by 25% relative to low tide. In the absence of tidal pumping, our model predicts that the aerobic <span class="hlt">zone</span> would be thinner, and denitrification rates would increase by 10%. As tidal amplitude increases toward the coast, nitrate removal rates should decrease due to enhanced oxygen exchange across the <span class="hlt">sediment</span>-water interface, based on sensitivity analysis. Denitrification hot spots in TFZs are more likely to occur in less permeable <span class="hlt">sediment</span> under lower tidal ranges and higher rates of ambient groundwater discharge. Our models suggest that tidal pumping is not efficient at removing surface water nitrate but can remove up to 81% of nitrate from discharging groundwater in the TFZ of White Clay Creek. Given the high population densities of coastal watersheds, the reactive riverbeds of TFZs play a critical role in mitigating new nitrogen loads to coasts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016043','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016043"><span>Extraction and speciation of arsenic in lacustrine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ficklin, W.H.</p> <p>1990-01-01</p> <p>Arsenic was partially extracted with 4.OM hydrochloric acid, from samples collected at 25-cm intervals in a 350-cm column of <span class="hlt">sediment</span> at Milltown Reservoir, Montana and from a 60-cm core of <span class="hlt">sediment</span> collected at the Cheyenne River Embayment of Lake Oahe, South Dakota. The <span class="hlt">sediment</span> in both reservoirs is highly contaminated with arsenic. The extracted arsenic was separated into As(III) and As(V) on acetate form Dowex 1-X8 ion-exchange resin with 0.12M HCl eluent. Residual arsenic was sequentially extracted with KClO3 and HCl. Arsenic was determined by graphite-furnace atomic-absorption spectrometry. The analytical results define oxidized and reduced <span class="hlt">zones</span> in the <span class="hlt">sediment</span> columns. ?? 1990.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70031244','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70031244"><span>Changes in ice-margin processes and <span class="hlt">sediment</span> routing during ice-sheet advance across a marginal moraine</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Knight, P.G.; Jennings, C.E.; Waller, R.I.; Robinson, Z.P.</p> <p>2007-01-01</p> <p>Advance of part of the margin of the Greenland ice sheet across a proglacial moraine ridge between 1968 and 2002 caused progressive changes in moraine morphology, basal ice formation, debris release, ice-marginal <span class="hlt">sediment</span> storage, and <span class="hlt">sediment</span> transfer to the distal proglacial <span class="hlt">zone</span>. When the ice margin is behind the moraine, most of the <span class="hlt">sediment</span> released from the glacier is stored close to the ice margin. As the margin advances across the moraine the potential for ice-proximal <span class="hlt">sediment</span> storage decreases and distal <span class="hlt">sediment</span> flux is augmented by reactivation of moraine <span class="hlt">sediment</span>. For six stages of advance associated with distinctive glacial and sedimentary processes we describe the ice margin, the debris-rich basal ice, debris release from the glacier, <span class="hlt">sediment</span> routing into the proglacial <span class="hlt">zone</span>, and geomorphic processes on the moraine. The overtopping of a moraine ridge is a significant glaciological, geomorphological and sedimentological threshold in glacier advance, likely to cause a distinctive pulse in distal <span class="hlt">sediment</span> accumulation rates that should be taken into account when glacial <span class="hlt">sediments</span> are interpreted to reconstruct glacier fluctuations. ?? 2007 Swedish Society for Anthropology and Geography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001Geo....29...43R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001Geo....29...43R"><span>Internal architecture, permeability structure, and hydrologic significance of contrasting fault-<span class="hlt">zone</span> types</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rawling, Geoffrey C.; Goodwin, Laurel B.; Wilson, John L.</p> <p>2001-01-01</p> <p>The Sand Hill fault is a steeply dipping, large-displacement normal fault that cuts poorly lithified Tertiary <span class="hlt">sediments</span> of the Albuquerque basin, New Mexico, United States. The fault <span class="hlt">zone</span> does not contain macroscopic fractures; the basic structural element is the deformation band. The fault core is composed of foliated clay flanked by structurally and lithologically heterogeneous mixed <span class="hlt">zones</span>, in turn flanked by damage <span class="hlt">zones</span>. Structures present within these fault-<span class="hlt">zone</span> architectural elements are different from those in brittle faults formed in lithified sedimentary and crystalline rocks that do contain fractures. These differences are reflected in the permeability structure of the Sand Hill fault. Equivalent permeability calculations indicate that large-displacement faults in poorly lithified <span class="hlt">sediments</span> have little potential to act as vertical-flow conduits and have a much greater effect on horizontal flow than faults with fractures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2013/3023/fs2013-3023.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2013/3023/fs2013-3023.pdf"><span>Fine-grained <span class="hlt">sediment</span> dispersal along the California coast</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Warrick, Jonathan A.; Storlazzi, Curt D.</p> <p>2013-01-01</p> <p>Fine-grained <span class="hlt">sediment</span> (silt and clay) enters coastal waters from rivers, eroding coastal bluffs, resuspension of seabed <span class="hlt">sediment</span>, and human activities such as dredging and beach nourishment. The amount of <span class="hlt">sediment</span> in coastal waters is an important factor in ocean ecosystem health, but little information exists on both the natural and human-driven magnitudes of fine-grained <span class="hlt">sediment</span> delivery to the coastal <span class="hlt">zone</span>, its residence time there, and its transport out of the system—information upon which to base environmental assessments. To help fill these information gaps, the U.S. Geological Survey has partnered with Federal, State, and local agencies to monitor fine-grained <span class="hlt">sediment</span> dispersal patterns and fate in the coastal regions of California. Results of these studies suggest that the waves and currents of many of the nearshore coastal settings of California are adequately energetic to transport fine-grained <span class="hlt">sediment</span> quickly through coastal systems. These findings will help with the management and regulation of fine-grained <span class="hlt">sediment</span> along the U.S. west coast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70022693','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70022693"><span>Formation of natural gas hydrates in marine <span class="hlt">sediments</span>. Gas hydrate growth and stability conditioned by host <span class="hlt">sediment</span> properties</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Clennell, M.B.; Henry, P.; Hovland, M.; Booth, J.S.; Winters, W.J.; Thomas, M.</p> <p>2000-01-01</p> <p>The stability conditions of submarine gas hydrates (methane clathrates) are largely dictated by pressure, temperature, gas composition, and pore water salinity. However, the physical properties and surface chemistry of the host <span class="hlt">sediments</span> also affect the thermodynamic state, growth kinetics, spatial distributions, and growth forms of clathrates. Our model presumes that gas hydrate behaves in a way analogous to ice in the pores of a freezing soil, where capillary forces influence the energy balance. Hydrate growth is inhibited within fine-grained <span class="hlt">sediments</span> because of the excess internal phase pressure of small crystals with high surface curvature that coexist with liquid water in small pores. Therefore, the base of gas hydrate stability in a sequence of fine <span class="hlt">sediments</span> is predicted by our model to occur at a lower temperature, and so nearer to the seabed than would be calculated from bulk thermodynamic equilibrium. The growth forms commonly observed in hydrate samples <span class="hlt">recovered</span> from marine <span class="hlt">sediments</span> (nodules, sheets, and lenses in muds; cements in sand and ash layers) can be explained by a requirement to minimize the excess of mechanical and surface energy in the system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/43653','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/43653"><span>Influence of forest road buffer <span class="hlt">zones</span> on <span class="hlt">sediment</span> transport in the Southern Appalachian Region</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Johnny M. Grace; Stanley J. Zarnoch</p> <p>2013-01-01</p> <p>A gap exists in the understanding of the effectiveness of forest road best management practices (BMP) in controlling <span class="hlt">sediment</span> movement and minimizing risks of <span class="hlt">sediment</span> delivery to forest streams. The objective of this paper is to report the findings of investigations to assess <span class="hlt">sediment</span> travel distances downslope of forest roads in the Appalachian region, relate...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMEP13F..06N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMEP13F..06N"><span>Role of <span class="hlt">Sediments</span> and Nutrients in the Condition of a Coral Reef Under Tourist Pressure: Akumal México.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naranjo-Garcia, M. J.; Vadés Lozano, D. S.; Real-De-Leon, E.; Lopez-Aguiar, K.; Garza-Perez, J. R.</p> <p>2014-12-01</p> <p>Akumal, Mexico, was the first tourist resort in the Mexican Caribbean mainland, its highly developed coastal <span class="hlt">zone</span> lies directly above the phreatic, and it is directly connected to the sub-littoral waters. Akumal is also known as a well-developed fringing coral reef, now in a critical condition. The main objective of this study was to explore the relationship between two of the main indicators of human pressure (nutrients and <span class="hlt">sedimentation</span>, linked to coastal development and water run-offs) and the condition of the reef benthos, during a year. The sampling design used four transects perpendicular to shore, associated to different tourist and water run-off exposure, for a total of 12 stations distributed in three different reef <span class="hlt">zones</span> (transition <span class="hlt">zone</span>, shallow and deep spurs and grooves). Monthly samples were collected: water samples close to the reef lagoon drain channels and at bottom depth at each station, and <span class="hlt">sediment</span> traps were <span class="hlt">recovered</span> and replaced also at each station. Reef Benthos videotransects were recorded bi-monthly at each station to assess its condition. Macroalgae and filamentous algae dominate benthic cover (up to 50%), hard-coral cover ranges from 5-9%. Five coral-diseases were recorded, affecting 10.16% of the coral colonies: Caribbean Ciliate Infection, White Band, Purple Spots, White Spots and Yellow Band. The <span class="hlt">sedimentation</span> rate -sr- ranged from 0.13 to 83.7 mg/cm2/day during the year; 86% of the samples had a sr ≤ 10 mg/cm2/day (reefs not stressed); 13% of the samples had a sr ranging from 10 to 50 mg/cm2/day (stressed reefs); and 1% of the samples were over the critical threshold (>50 mg/cm2/day). Dissolved Inorganic Nitrogen concentrations during the year were above those recorded previously in Caribbean reefs. The most abundant fraction was ammonium, surpassing both Mexican norms: For protection of aquatic life in coastal <span class="hlt">zones</span> (0.01 mg/L), and the critical threshold for aquatic life (0.4 mg/L). These concentration limits are considered as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=91219','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=91219"><span>Microbiological and Geochemical Characterization of Fluvially Deposited Sulfidic Mine Tailings</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wielinga, Bruce; Lucy, Juliette K.; Moore, Johnnie N.; Seastone, October F.; Gannon, James E.</p> <p>1999-01-01</p> <p>The fluvial deposition of mine tailings generated from historic mining operations near Butte, Montana, has resulted in substantial surface and shallow groundwater contamination along Silver Bow Creek. Biogeochemical processes in the <span class="hlt">sediment</span> and underlying hyporheic <span class="hlt">zone</span> were studied in an attempt to characterize interactions consequential to heavy-metal contamination of shallow groundwater. <span class="hlt">Sediment</span> cores were extracted and fractionated based on <span class="hlt">sediment</span> stratification. Subsamples of each fraction were assayed for culturable heterotrophic microbiota, specific microbial guilds involved in metal redox transformations, and both aqueous- and solid-phase geochemistry. Populations of cultivable Fe(III)-reducing bacteria were most prominent in the anoxic, circumneutral pH regions associated with a ferricrete layer or in an oxic <span class="hlt">zone</span> high in organic carbon and soluble iron. Sulfur- and iron-oxidizing bacteria were distributed in discrete <span class="hlt">zones</span> throughout the tailings and were often <span class="hlt">recovered</span> from sections at and below the anoxic groundwater interface. Sulfate-reducing bacteria were also widely distributed in the cores and often occurred in <span class="hlt">zones</span> overlapping iron and sulfur oxidizers. Sulfate-reducing bacteria were consistently <span class="hlt">recovered</span> from oxic <span class="hlt">zones</span> that contained high concentrations of metals in the oxidizable fraction. Altogether, these results suggest a highly varied and complex microbial ecology within a very heterogeneous geochemical environment. Such physical and biological heterogeneity has often been overlooked when remediation strategies for metal contaminated environments are formulated. PMID:10103249</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023164','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023164"><span>Gas content and composition of gas hydrate from <span class="hlt">sediments</span> of the southeastern North American continental margin</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lorenson, T.D.; Collett, T.S.</p> <p>2000-01-01</p> <p>Gas hydrate samples were <span class="hlt">recovered</span> from four sites (Sites 994, 995, 996, and 997) along the crest of the Blake Ridge during Ocean Drilling Program (ODP) Leg 164. At Site 996, an area of active gas venting, pockmarks, and chemosynthetic communities, vein-like gas hydrate was <span class="hlt">recovered</span> from less than 1 meter below seafloor (mbsf) and intermittently through the maximum cored depth of 63 mbsf. In contrast, massive gas hydrate, probably fault filling and/or stratigraphically controlled, was <span class="hlt">recovered</span> from depths of 260 mbsf at Site 994, and from 331 mbsf at Site 997. Downhole-logging data, along with geochemical and core temperature profiles, indicate that gas hydrate at Sites 994, 995, and 997 occurs from about 180 to 450 mbsf and is dispersed in <span class="hlt">sediment</span> as 5- to 30-m-thick <span class="hlt">zones</span> of up to about 15% bulk volume gas hydrate. Selected gas hydrate samples were placed in a sealed chamber and allowed to dissociate. Evolved gas to water volumetric ratios measured on seven samples from Site 996 ranged from 20 to 143 mL gas/mL water to 154 mL gas/mL water in one sample from Site 994, and to 139 mL gas/mL water in one sample from Site 997, which can be compared to the theoretical maximum gas to water ratio of 216. These ratios are minimum gas/water ratios for gas hydrate because of partial dissociation during core recovery and potential contamination with pore waters. Nonetheless, the maximum measured volumetric ratio indicates that at least 71% of the cages in this gas hydrate were filled with gas molecules. When corrections for pore-water contamination are made, these volumetric ratios range from 29 to 204, suggesting that cages in some natural gas hydrate are nearly filled. Methane comprises the bulk of the evolved gas from all sites (98.4%-99.9% methane and 0%-1.5% CO2). Site 996 hydrate contained little CO2 (0%-0.56%). Ethane concentrations differed significantly from Site 996, where they ranged from 720 to 1010 parts per million by volume (ppmv), to Sites 994 and 997</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2014/1220/ofr2014-1220-title_page.html','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2014/1220/ofr2014-1220-title_page.html"><span>Shallow geology, sea-floor texture, and physiographic <span class="hlt">zones</span> of Buzzards Bay, Massachusetts</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Foster, David S.; Baldwin, Wayne E.; Barnhardt, Walter A.; Schwab, William C.; Ackerman, Seth D.; Andrews, Brian D.; Pendleton, Elizabeth A.</p> <p>2015-01-07</p> <p>Geologic, <span class="hlt">sediment</span> texture, and physiographic <span class="hlt">zone</span> maps characterize the sea floor of Buzzards Bay, Massachusetts. These maps were derived from interpretations of seismic-reflection profiles, high-resolution bathymetry, acoustic-backscatter intensity, bottom photographs, and surficial <span class="hlt">sediment</span> samples. The interpretation of the seismic stratigraphy and mapping of glacial and Holocene marine units provided a foundation on which the surficial maps were created. This mapping is a result of a collaborative effort between the U.S. Geological Survey and the Massachusetts Office of Coastal <span class="hlt">Zone</span> Management to characterize the surface and subsurface geologic framework offshore of Massachusetts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1399394-natural-attenuation-streambed-sediment-receiving-chlorinated-solvents-from-underlying-fracture-networks','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1399394-natural-attenuation-streambed-sediment-receiving-chlorinated-solvents-from-underlying-fracture-networks"><span>Natural Attenuation in Streambed <span class="hlt">Sediment</span> Receiving Chlorinated Solvents from Underlying Fracture Networks</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Şimşir, Burcu; Yan, Jun; Im, Jeongdae; ...</p> <p>2017-03-22</p> <p>Contaminant discharge from fractured bedrock formations remains a remediation challenge. Here, we applied an integrated approach to assess the natural attenuation potential of <span class="hlt">sediment</span> that forms the transition <span class="hlt">zone</span> between upwelling groundwater from a chlorinated solvent-contaminated fractured bedrock aquifer and the receiving surface water. In situ measurements demonstrated that reductive dechlorination in the <span class="hlt">sediment</span> attenuated chlorinated compounds before reaching the water column. Microcosms established with creek <span class="hlt">sediment</span> or in situ incubated Bio-Sep beads degraded C 1-C 3 chlorinated solvents to less-chlorinated or innocuous products. Quantitative PCR and 16S rRNA gene amplicon sequencing revealed the abundance and spatial distribution of knownmore » dechlorinator biomarker genes within the creek <span class="hlt">sediment</span> and demonstrated that multiple dechlorinator populations degrading chlorinatedC 1-C 3 alkanes and alkenes co-inhabit the <span class="hlt">sediment</span>. Phylogenetic classification of bacterial and archaeal sequences indicated a relatively uniform distribution over spatial (300 m horizontally) scale, but Dehalococcoides and Dehalobacter were more abundant in deeper <span class="hlt">sediment</span>, where 5.7 ± 0.4 × 10 5 and 5.4 ± 0.9 × 10 6 16S rRNA gene copies per g of <span class="hlt">sediment</span>, respectively, were measured. The microbiological and hydrogeological characterization demonstrated that microbial processes at the fractured bedrock-<span class="hlt">sediment</span> interface were crucial for preventing contaminants reaching the water column, emphasizing the relevance of this critical <span class="hlt">zone</span> environment for contaminant attenuation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1399394','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1399394"><span>Natural Attenuation in Streambed <span class="hlt">Sediment</span> Receiving Chlorinated Solvents from Underlying Fracture Networks</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Şimşir, Burcu; Yan, Jun; Im, Jeongdae</p> <p></p> <p>Contaminant discharge from fractured bedrock formations remains a remediation challenge. Here, we applied an integrated approach to assess the natural attenuation potential of <span class="hlt">sediment</span> that forms the transition <span class="hlt">zone</span> between upwelling groundwater from a chlorinated solvent-contaminated fractured bedrock aquifer and the receiving surface water. In situ measurements demonstrated that reductive dechlorination in the <span class="hlt">sediment</span> attenuated chlorinated compounds before reaching the water column. Microcosms established with creek <span class="hlt">sediment</span> or in situ incubated Bio-Sep beads degraded C 1-C 3 chlorinated solvents to less-chlorinated or innocuous products. Quantitative PCR and 16S rRNA gene amplicon sequencing revealed the abundance and spatial distribution of knownmore » dechlorinator biomarker genes within the creek <span class="hlt">sediment</span> and demonstrated that multiple dechlorinator populations degrading chlorinatedC 1-C 3 alkanes and alkenes co-inhabit the <span class="hlt">sediment</span>. Phylogenetic classification of bacterial and archaeal sequences indicated a relatively uniform distribution over spatial (300 m horizontally) scale, but Dehalococcoides and Dehalobacter were more abundant in deeper <span class="hlt">sediment</span>, where 5.7 ± 0.4 × 10 5 and 5.4 ± 0.9 × 10 6 16S rRNA gene copies per g of <span class="hlt">sediment</span>, respectively, were measured. The microbiological and hydrogeological characterization demonstrated that microbial processes at the fractured bedrock-<span class="hlt">sediment</span> interface were crucial for preventing contaminants reaching the water column, emphasizing the relevance of this critical <span class="hlt">zone</span> environment for contaminant attenuation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999E%26PSL.173..205S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999E%26PSL.173..205S"><span>Variations of oxygen-minimum and primary productivity recorded in <span class="hlt">sediments</span> of the Arabian Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schulte, Sonja; Rostek, Frauke; Bard, Edouard; Rullkötter, Jürgen; Marchal, Olivier</p> <p>1999-11-01</p> <p>Two deep-sea <span class="hlt">sediment</span> cores from the northeastern and the southeastern Arabian Sea were studied in order to reconstruct the palaeoenvironments of the past glacial cycles. Core 136KL was <span class="hlt">recovered</span> from the high-productivity area off Pakistan within the modern oxygen-minimum <span class="hlt">zone</span> (OMZ). By contrast, modern primary productivity at the site of MD900963 close to Maldives is moderate and bottom waters are today well oxygenated. For both cores, we reconstructed the changes in palaeoproductivity using a set of biomarkers (alkenones, dinosterol and brassicasterol); the main result is that primary productivity is enhanced during glacial stages and lowered during interstadials. The proxies associated with productivity show a 23 kyr cyclicity corresponding to the precession-related insolation cycle. Palaeoredox conditions were studied in both cores using a new organic geochemical parameter (C 35/C 31- n-alkane ratio) developed by analysing surface <span class="hlt">sediments</span> from a transect across the OMZ off Pakistan. The value of this ratio in core 136KL shows many variations during the last 65 kyr, indicating that the OMZ was not stable during this time: it disappeared completely during Heinrich- and the Younger Dryas events, pointing to a connection between global oceanic circulation and the stability of the OMZ. The C 35/C 31 ratio determined in <span class="hlt">sediments</span> of core MD900963 shows that bottom waters remained rather well oxygenated over the last 330 kyr, which is confirmed by comparison with authigenic metal concentrations in the same <span class="hlt">sediments</span>. A zonally averaged, circulation-biogeochemical ocean model was used to explore how the intermediate Indian Ocean responds to a freshwater flux anomaly at the surface of the North Atlantic. As suggested by the geochemical time series, both the abundance of Southern Ocean Water and the oxygen concentration are significantly increased in response to this freshwater perturbation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70197120','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70197120"><span>Middle Pleistocene infill of Hinkley Valley by Mojave River <span class="hlt">sediment</span> and associated lake <span class="hlt">sediment</span>: Depositional architecture and deformation by strike-slip faults</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, David; Haddon, Elizabeth; Langenheim, Victoria; Cyr, Andrew J.; Wan, Elmira; Walkup, Laura; Starratt, Scott W.</p> <p>2018-01-01</p> <p>Hinkley Valley in the Mojave Desert, near Barstow about 140 km northeast of Los Angeles and midway between Victorville Valley and the Lake Manix basin, contains a thick sedimentary sequence delivered by the Mojave River. Our study of <span class="hlt">sediment</span> cores drilled in the valley indicates that Hinkley Valley was probably a closed playa basin with stream inflow from four directions prior to Mojave River inflow. The Mojave River deposited thick and laterally extensive clastic wedges originating from the southern valley that rapidly filled much of Hinkley Valley. Sedimentary facies representing braided stream, wetland, delta, and lacustrine depositional environments all are found in the basin fill; in some places, the sequence is greater than 74 m (245 ft) thick. The <span class="hlt">sediment</span> is dated in part by the presence of the ~631 ka Lava Creek B ash bed low in the section, and thus represents <span class="hlt">sediment</span> deposition after Victorville basin was overtopped by <span class="hlt">sediment</span> and before the Manix basin began to be filled. Evidently, upstream Victorville basin filled with <span class="hlt">sediment</span> by about 650 ka, causing the ancestral Mojave River to spill to the Harper and Hinkley basins, and later to Manix basin.Initial river <span class="hlt">sediment</span> overran wetland deposits in many places in southern Hinkley Valley, indicating a rapidly encroaching river system. These <span class="hlt">sediments</span> were succeeded by a widespread lake (“blue” clay) that includes the Lava Creek B ash bed. Above the lake <span class="hlt">sediment</span> lies a thick section of interlayered stream <span class="hlt">sediment</span>, delta and nearshore lake <span class="hlt">sediment</span>, mudflat and/or playa <span class="hlt">sediment</span>, and minor lake <span class="hlt">sediment</span>. This stratigraphic architecture is found throughout the valley, and positions of lake <span class="hlt">sediment</span> layers indicate a successive northward progression in the closed basin. A thin overlapping sequence at the north end of the valley contains evidence for a younger late Pleistocene lake episode. This late lake episode, and bracketing braided stream deposits of the Mojave River, indicate that the river</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/911766','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/911766"><span>Idaho National Laboratory Vadose <span class="hlt">Zone</span> Research Park Geohydrological Monitoring Results</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kristine Baker</p> <p>2006-01-01</p> <p>Vadose <span class="hlt">zone</span> lithology, hydrological characterization of interbed <span class="hlt">sediments</span>, and hydrological data from subsurface monitoring of Idaho Nuclear Technology and Engineering Center wastewater infiltration are presented. Three-dimensional subsurface lithology of the vadose <span class="hlt">zone</span> beneath the Vadose <span class="hlt">Zone</span> Research Park is represented in a 2 dimensional (2 D) diagram showing interpolated lithology between monitoring wells. Laboratory-measured values for saturated hydraulic conductivity and porosity are given for three major interbeds, denoted as the B BC interbed (20 to 35 m bls), the C D interbed (40 to 45 m bls), and the DE 1 2 interbed (55 to 65 m bls), along withmore » an overall physical description of the <span class="hlt">sediments</span> and geologic depositional environments. Pre-operational pore water pressure conditions are presented to show the presence and location of perched water <span class="hlt">zones</span> before pond discharge at the New Percolation Ponds. Subsurface infiltration conditions during initial high-volume discharge are presented to show water arrival times and arrival sequences. Steady-state conditions are then presented to show formation and locations of perched water <span class="hlt">zones</span> and recharge sources after several months of discharge to the New Percolation Ponds.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910040011&hterms=coastal+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcoastal%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910040011&hterms=coastal+zone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dcoastal%2Bzone"><span>Multipolarization P-, L-, and C-band radar for coastal <span class="hlt">zone</span> mapping - The Louisiana example</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wu, Shih-Tseng</p> <p>1989-01-01</p> <p>Multipolarization P-, L-, and C-band airborne SAR data sets were acquired over a coastal <span class="hlt">zone</span> and a forested wetland of southern Louisiana. The data sets were used with field-collected surface-parameter data in order to determine the value of SAR systems in assessing and mapping coastal-<span class="hlt">zone</span> surface features. The coastal-<span class="hlt">zone</span> surface features in this study are <span class="hlt">sediments</span>, <span class="hlt">sediment</span> distribution, and the formation of new isles and banks. Results of the data analysis indicate that the P-band radar with 68-cm wavelength is capable of detecting the submerged <span class="hlt">sediment</span> if the area is very shallow (i.e., a water depth of less than one meter). The penetration capability of P-band radar is also demonstrated in the forested wetland area. The composition and condition of the ground surface can be detected, as well as the standing water beneath dense tree leaves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613800F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613800F"><span>Subduction <span class="hlt">zone</span> earthquake probably triggered submarine hydrocarbon seepage offshore Pakistan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fischer, David; José M., Mogollón; Michael, Strasser; Thomas, Pape; Gerhard, Bohrmann; Noemi, Fekete; Volkhard, Spiess; Sabine, Kasten</p> <p>2014-05-01</p> <p>Seepage of methane-dominated hydrocarbons is heterogeneous in space and time, and trigger mechanisms of episodic seep events are not well constrained. It is generally found that free hydrocarbon gas entering the local gas hydrate stability field in marine <span class="hlt">sediments</span> is sequestered in gas hydrates. In this manner, gas hydrates can act as a buffer for carbon transport from the <span class="hlt">sediment</span> into the ocean. However, the efficiency of gas hydrate-bearing <span class="hlt">sediments</span> for retaining hydrocarbons may be corrupted: Hypothesized mechanisms include critical gas/fluid pressures beneath gas hydrate-bearing <span class="hlt">sediments</span>, implying that these are susceptible to mechanical failure and subsequent gas release. Although gas hydrates often occur in seismically active regions, e.g., subduction <span class="hlt">zones</span>, the role of earthquakes as potential triggers of hydrocarbon transport through gas hydrate-bearing <span class="hlt">sediments</span> has hardly been explored. Based on a recent publication (Fischer et al., 2013), we present geochemical and transport/reaction-modelling data suggesting a substantial increase in upward gas flux and hydrocarbon emission into the water column following a major earthquake that occurred near the study sites in 1945. Calculating the formation time of authigenic barite enrichments identified in two <span class="hlt">sediment</span> cores obtained from an anticlinal structure called "Nascent Ridge", we find they formed 38-91 years before sampling, which corresponds well to the time elapsed since the earthquake (62 years). Furthermore, applying a numerical model, we show that the local sulfate/methane transition <span class="hlt">zone</span> shifted upward by several meters due to the increased methane flux and simulated sulfate profiles very closely match measured ones in a comparable time frame of 50-70 years. We thus propose a causal relation between the earthquake and the amplified gas flux and present reflection seismic data supporting our hypothesis that co-seismic ground shaking induced mechanical fracturing of gas hydrate-bearing <span class="hlt">sediments</span></p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GeCoA.124..328D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GeCoA.124..328D"><span>CO2 solubility and speciation in rhyolitic <span class="hlt">sediment</span> partial melts at 1.5-3.0 GPa - Implications for carbon flux in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duncan, Megan S.; Dasgupta, Rajdeep</p> <p>2014-01-01</p> <p> much as 2.6-5.5 wt.% CO2 to the sub-arc mantle source regions. At saturation, 1.6-3.3 wt.% <span class="hlt">sediment</span> partial melt relative to the mantle wedge is therefore sufficient to bring up the carbon budget of the mantle wedge to produce primary arc basalts with 0.3 wt.% CO2. <span class="hlt">Sediment</span> plumes in mantle wedge: <span class="hlt">Sediment</span> plumes or diapirs may form from the downgoing slab because the <span class="hlt">sediment</span> layer atop the slab is buoyant relative to the overlying, hanging wall mantle (Currie et al., 2007; Behn et al., 2011). Via this process, <span class="hlt">sediment</span> layers with carbonates would carry CO2 to the arc source region. Owing to the higher temperature in the mantle wedge, carbonate can breakdown. Behn et al. (2011) suggested that <span class="hlt">sediment</span> layers as thin as 100 m, appropriate for modern arcs, could form <span class="hlt">sediment</span> diapirs. They predicted that diapirs would form from the slab in the sub-arc region for most subduction <span class="hlt">zones</span> today without requiring hydrous melting. H2O-rich fluid driven carbonate breakdown: Hydrous fluid flushing of the slab owing to the breakdown of hydrous minerals could drive carbonate breakdown (Kerrick and Connolly, 2001b; Grove et al., 2002; Gorman et al., 2006). The addition of water would cause decarbonation creating an H2O-CO2-rich fluid that would then flux through the overlying <span class="hlt">sediment</span> layer, lower the solidus temperature, and trigger melting. Recent geochemical (Cooper et al., 2012) and geodynamic (van Keken, 2003; Syracuse et al., 2010) constraints suggest that the sub-arc slab top temperatures are above the hydrous fluid-present <span class="hlt">sediment</span> solidus, thus in the presence of excess fluid, both infiltration induced decarbonation and <span class="hlt">sediment</span> melting may occur. Hot subduction: This is relevant for subduction <span class="hlt">zones</span> such as Cascadia and Mexico, where slab-surface temperatures are estimated to be higher (Syracuse et al., 2010). A higher temperature could cause carbonate breakdown and <span class="hlt">sediment</span> partial melting without requiring a hydrous fluid flux. In this case a relatively dry silicate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15952347','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15952347"><span>Colloid-facilitated transport of cesium in variably saturated Hanford <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Gang; Flury, Markus; Harsh, James B; Lichtner, Peter C</p> <p>2005-05-15</p> <p>Radioactive 137Cs has leaked from underground waste tanks into the vadose <span class="hlt">zone</span> at the Hanford Reservation in south-central Washington State. There is concern that 137Cs, currently located in the vadose <span class="hlt">zone</span>, can reach the groundwater. In this study, we investigated whether, and to what extent, colloidal particles can facilitate the transport of 137Cs at Hanford. We used colloidal materials isolated from Hanford <span class="hlt">sediments</span>. Transport experiments were conducted under variably saturated, steady-state flow conditions in repacked, 20 cm long Hanford <span class="hlt">sediment</span> columns, with effective water saturations ranging from 0.2 to 1.0. Cesium, pre-associated with colloids, was stripped off during transport through the <span class="hlt">sediments</span>. The higher the flow rates, the less Cs was stripped off, indicating in part that Cs desorption from carrying colloids was a residence-time-dependent process. Depending on the flow rate, up to 70% of the initially sorbed Cs desorbed from colloidal carriers and was captured in the stationary <span class="hlt">sediments</span>. Less Cs was stripped off colloids under unsaturated than under saturated flow conditions at similar flow rates. This phenomenon was likely due to the reduced availability of sorption sites for Cs on the <span class="hlt">sediments</span> as the water content decreased and water flow was divided between mobile and immobile regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22138990','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22138990"><span>Distribution of microbial biomass and potential for anaerobic respiration in Hanford Site 300 Area subsurface <span class="hlt">sediment</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lin, Xueju; Kennedy, David; Peacock, Aaron; McKinley, James; Resch, Charles T; Fredrickson, James; Konopka, Allan</p> <p>2012-02-01</p> <p>Subsurface <span class="hlt">sediments</span> were <span class="hlt">recovered</span> from a 52-m-deep borehole cored in the 300 Area of the Hanford Site in southeastern Washington State to assess the potential for biogeochemical transformation of radionuclide contaminants. Microbial analyses were made on 17 <span class="hlt">sediment</span> samples traversing multiple geological units: the oxic coarse-grained Hanford formation (9 to 17.4 m), the oxic fine-grained upper Ringold formation (17.7 to 18.1 m), and the reduced Ringold formation (18.3 to 52 m). Microbial biomass (measured as phospholipid fatty acids) ranged from 7 to 974 pmols per g in discrete samples, with the highest numbers found in the Hanford formation. On average, strata below 17.4 m had 13-fold less biomass than those from shallower strata. The nosZ gene that encodes nitrous oxide reductase (measured by quantitative real-time PCR) had an abundance of 5 to 17 relative to that of total 16S rRNA genes below 18.3 m and <5 above 18.1 m. Most nosZ sequences were affiliated with Ochrobactrum anthropi (97 sequence similarity) or had a nearest neighbor of Achromobacter xylosoxidans (90 similarity). Passive multilevel sampling of groundwater geochemistry demonstrated a redox gradient in the 1.5-m region between the Hanford-Ringold formation contact and the Ringold oxic-anoxic interface. Within this <span class="hlt">zone</span>, copies of the dsrA gene and Geobacteraceae had the highest relative abundance. The majority of dsrA genes detected near the interface were related to Desulfotomaculum spp. These analyses indicate that the region just below the contact between the Hanford and Ringold formations is a <span class="hlt">zone</span> of active biogeochemical redox cycling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3264105','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3264105"><span>Distribution of Microbial Biomass and Potential for Anaerobic Respiration in Hanford Site 300 Area Subsurface <span class="hlt">Sediment</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lin, Xueju; Kennedy, David; Peacock, Aaron; McKinley, James; Resch, Charles T.; Fredrickson, James</p> <p>2012-01-01</p> <p>Subsurface <span class="hlt">sediments</span> were <span class="hlt">recovered</span> from a 52-m-deep borehole cored in the 300 Area of the Hanford Site in southeastern Washington State to assess the potential for biogeochemical transformation of radionuclide contaminants. Microbial analyses were made on 17 <span class="hlt">sediment</span> samples traversing multiple geological units: the oxic coarse-grained Hanford formation (9 to 17.4 m), the oxic fine-grained upper Ringold formation (17.7 to 18.1 m), and the reduced Ringold formation (18.3 to 52 m). Microbial biomass (measured as phospholipid fatty acids) ranged from 7 to 974 pmols per g in discrete samples, with the highest numbers found in the Hanford formation. On average, strata below 17.4 m had 13-fold less biomass than those from shallower strata. The nosZ gene that encodes nitrous oxide reductase (measured by quantitative real-time PCR) had an abundance of 5 to 17 relative to that of total 16S rRNA genes below 18.3 m and <5 above 18.1 m. Most nosZ sequences were affiliated with Ochrobactrum anthropi (97 sequence similarity) or had a nearest neighbor of Achromobacter xylosoxidans (90 similarity). Passive multilevel sampling of groundwater geochemistry demonstrated a redox gradient in the 1.5-m region between the Hanford-Ringold formation contact and the Ringold oxic-anoxic interface. Within this <span class="hlt">zone</span>, copies of the dsrA gene and Geobacteraceae had the highest relative abundance. The majority of dsrA genes detected near the interface were related to Desulfotomaculum spp. These analyses indicate that the region just below the contact between the Hanford and Ringold formations is a <span class="hlt">zone</span> of active biogeochemical redox cycling. PMID:22138990</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25603259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25603259"><span>Spatial characterization of riparian buffer effects on <span class="hlt">sediment</span> loads from watershed systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Momm, Henrique G; Bingner, Ronald L; Yuan, Yongping; Locke, Martin A; Wells, Robert R</p> <p>2014-09-01</p> <p>Understanding all watershed systems and their interactions is a complex, but critical, undertaking when developing practices designed to reduce topsoil loss and chemical/nutrient transport from agricultural fields. The presence of riparian buffer vegetation in agricultural landscapes can modify the characteristics of overland flow, promoting <span class="hlt">sediment</span> deposition and nutrient filtering. Watershed simulation tools, such as the USDA-Annualized Agricultural Non-Point Source (AnnAGNPS) pollution model, typically require detailed information for each riparian buffer <span class="hlt">zone</span> throughout the watershed describing the location, width, vegetation type, topography, and possible presence of concentrated flow paths through the riparian buffer <span class="hlt">zone</span>. Research was conducted to develop GIS-based technology designed to spatially characterize riparian buffers and to estimate buffer efficiency in reducing <span class="hlt">sediment</span> loads in a semiautomated fashion at watershed scale. The methodology combines modeling technology at different scales, at individual concentrated flow paths passing through the riparian <span class="hlt">zone</span>, and at watershed scales. At the concentrated flow path scale, vegetative filter strip models are applied to estimate the <span class="hlt">sediment</span>-trapping efficiency for each individual flow path, which are aggregated based on the watershed subdivision and used in the determination of the overall impact of the riparian vegetation at the watershed scale. This GIS-based technology is combined with AnnAGNPS to demonstrate the effect of riparian vegetation on <span class="hlt">sediment</span> loadings from sheet and rill and ephemeral gully sources. The effects of variability in basic input parameters used to characterize riparian buffers, onto generated outputs at field scale (<span class="hlt">sediment</span> trapping efficiency) and at watershed scale (<span class="hlt">sediment</span> loadings from different sources) were evaluated and quantified. The AnnAGNPS riparian buffer component represents an important step in understanding and accounting for the effect of riparian</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMMR33B0457D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMMR33B0457D"><span>Earthquake rupture dynamics in poorly lithified <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Paola, N.; Bullock, R. J.; Holdsworth, R.; Marco, S.; Nielsen, S. B.</p> <p>2017-12-01</p> <p>Several recent large earthquakes have generated anomalously large slip patches when propagating through fluid-saturated, clay-rich <span class="hlt">sediments</span> near the surface. Friction experiments at seismic slip rates show that such <span class="hlt">sediments</span> are extremely weak and deform with very little energy dissipation, which facilitates rupture propagation. Although dynamic weakening may explain the ease of rupture propagation through such <span class="hlt">sediments</span>, it cannot account for the peculiar slow rupture velocity and low radiation efficiency exhibited by some large, shallow ruptures. Here, we integrate field and experimental datasets to describe on- and off-fault deformation in natural syn-depositional seismogenic faults (< 35 ka) in shallow, clay-rich, poorly lithified <span class="hlt">sediments</span> from the Dead Sea Fault system, Israel. The data are then used to estimate the energy dissipated by on- and off-fault damage during earthquake rupture through shallow, clay-rich <span class="hlt">sediments</span>. Our mechanical and field data show localised principal slip <span class="hlt">zones</span> (PSZs) that deform by particulate flow, with little energy dissipated by brittle fracturing with cataclasis. Conversely, we show that coseismic brittle and ductile deformation in the damage <span class="hlt">zones</span> outwith the PSZ, which cannot be replicated in small-scale laboratory experiments, is a significant energy sink, contributing to an energy dissipation that is one order of magnitude greater than that estimated from laboratory experiments alone. In particular, a greater proportion of dissipated energy would result in lower radiation efficiency, due to a reduced proportion of radiated energy, plus slower rupture velocity and more energy radiation in the low frequency range than might be anticipated from laboratory experiments alone. This result is in better agreement with seismological estimates of fracture energy, implying that off-fault damage can account for the geophysical characteristics of earthquake ruptures as they pass through clay-rich <span class="hlt">sediments</span> in the shallow crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IJEaS.tmp..221B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IJEaS.tmp..221B"><span>From an ocean floor wrench <span class="hlt">zone</span> origin to transpressional tectonic emplacement of the Sithonia ophiolite, eastern Vardar Suture <span class="hlt">Zone</span>, northern Greece</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bonev, Nikolay; Filipov, Petyo</p> <p>2017-12-01</p> <p>In the Hellenides of northern Greece, the Sithonia back-arc ophiolite constitute an element of the Vardar suture <span class="hlt">zone</span> against the Chortiatis island arc magmatic suite, the Melissochori Formation and the Serbo-Macedonian Massif further north at the Mesozoic continental margin of Eurasia. A granodiorite from the Chortiatis island arc magmatic suite crystallized at 160 Ma as derived from new U-Pb zircon geochronology and confirms the end of arc magmatic activity that started at around 173 Ma. Located southerly of the Chortiatis island arc magmatic suite, the Sithonia ophiolite had igneous life from 159 to 149 Ma, and the ophiolite interfinger with clastic-carbonate Kimmeridgian <span class="hlt">sediments</span>. Magmatic structures (i.e., sheeted dykes) in the ophiolite witness for NE-trending rift axis, while the transform faults and fracture <span class="hlt">zones</span> sketch NW-SE transcurrent transtension-like propagation of the rift-spreading center at Sithonia that is consistent with a dextral wrench corridor already proposed for the ophiolite origin in the eastern Vardar <span class="hlt">zone</span>. The tectonic emplacement of the Sithonia ophiolite involved dextral ENE to SE strike-slip sense of shear and SW and NE reverse thrust sense of shear on mostly steep foliation S1, subhorizontal lineation L1 and associated variably inclined F1 fold axes. This structural grain and kinematics are shared by adjacent Chortiatis island arc magmatic suite and the Melissochori Formation. The coexistence of strike-parallel and thrust components of displacement along discrete dextral strike-slip shear <span class="hlt">zones</span> and internal deformation of the mentioned units is interpreted to result from a bulk dextral transpressive deformation regime developed in greenschist-facies metamorphic conditions. The back-arc ocean floor previous structural architecture with faults and fracture <span class="hlt">zones</span> where Kimmeridgian <span class="hlt">sediments</span> deposited in troughs was used by discrete strike-slip shear <span class="hlt">zones</span> in which these <span class="hlt">sediments</span> involved, and the shear <span class="hlt">zones</span> become the sites for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032965','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032965"><span>DIN retention-transport through four hydrologically connected <span class="hlt">zones</span> in a headwater catchment of the Upper Mississippi River</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Triska, F.J.; Duff, J.H.; Sheibley, R.W.; Jackman, A.P.; Avanzino, R.J.</p> <p>2007-01-01</p> <p>Dissolved inorganic nitrogen (DIN) retention-transport through a headwater catchment was synthesized from studies encompassing four distinct hydrologic <span class="hlt">zones</span> of the Shingobee River Headwaters near the origin of the Mississippi River. The hydrologic <span class="hlt">zones</span> included: (1) hillslope ground water (ridge to bankside riparian); (2) alluvial riparian ground water; (3) ground water discharged through subchannel <span class="hlt">sediments</span> (hyporheic <span class="hlt">zone</span>); and (4) channel surface water. During subsurface hillslope transport through <span class="hlt">Zone</span> 1, DIN, primarily nitrate, decreased from ???3 mg-N/l to <0.1 mg-N/l. Ambient seasonal nitrate:chloride ratios in hillslope flow paths indicated both dilution and biotic processing caused nitrate loss. Biologically available organic carbon controlled biotic nitrate retention during hillslope transport. In the alluvial riparian <span class="hlt">zone</span> (<span class="hlt">Zone</span> 2) biologically available organic carbon controlled nitrate depletion although processing of both ambient and amended nitrate was faster during the summer than winter. In the hyporheic <span class="hlt">zone</span> (<span class="hlt">Zone</span> 3) and stream surface water (<span class="hlt">Zone</span> 4) DIN retention was primarily controlled by temperature. Perfusion core studies using hyporheic <span class="hlt">sediment</span> indicated sufficient organic carbon in bed <span class="hlt">sediments</span> to retain ground water DIN via coupled nitrification-denitrification. Numerical simulations of seasonal hyporheic <span class="hlt">sediment</span> nitrification-denitrification rates from perfusion cores adequately predicted surface water ammonium but not nitrate when compared to 5 years of monthly field data (1989-93). Mass balance studies in stream surface water indicated proportionally higher summer than winter N retention. Watershed DIN retention was effective during summer under the current land use of intermittently grazed pasture. However, more intensive land use such as row crop agriculture would decrease nitrate retention efficiency and increase loads to surface water. Understanding DIN retention capacity throughout the system, including special channel</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001DSRII..48.3523M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001DSRII..48.3523M"><span>Compositional changes of surface <span class="hlt">sediments</span> and variability of manganese nodules in the Peru Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marchig, Vesna; von Stackelberg, Ulrich; Hufnagel, Heinz; Durn, Goran</p> <p></p> <p>Two types of manganese nodules were observed in the Peru Basin: large botryoidal nodules in basins and small ellipsoidal nodules on slope positions. The <span class="hlt">sediment</span> in areas with large botryoidal nodules contains a thinner and weaker oxidation <span class="hlt">zone</span> than the <span class="hlt">sediment</span> under small ellipsoidal nodules, indicating that diagenetic processes in the <span class="hlt">sediment</span>, which supply manganese nodules with metals for their growth, are stronger in <span class="hlt">sediments</span> on which large botryoidal nodules grow. Organic matter, which activates remobilization of metals, occurs mostly in the form of refractory lipidic compounds in the inner capsule of radiolaria. This material needs bacterial degradation to act as a reducing agent. Easily oxidizable organic components could not be found in the <span class="hlt">sediments</span>. Other changes in <span class="hlt">sediment</span> composition do not have a link to manganese nodule growth. Biogenous components (radiolarians, organogenic barite and apatite) increase towards the equatorial high-productivity <span class="hlt">zone</span>. Authigenous clay minerals (nontronite as well as montmorillonite with high Fe +3 incorporation on positions of ochtaedral Al) increase with distance from the continent. The assessment of environmental impacts will have to take into account the regional differences in <span class="hlt">sediment</span> composition and the small-scale variability of manganese nodules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS23B..04H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS23B..04H"><span>Analyses of outcrop and <span class="hlt">sediment</span> grains observed and collected from the Sirena Deep and Middle Pond of the Mariana Trench</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hand, K. P.; Bartlett, D. H.; Fryer, P.</p> <p>2012-12-01</p> <p>During a March 2012 expedition we <span class="hlt">recovered</span> <span class="hlt">sediments</span> from two locales within the Marina Trench - Middle Pond and Sirena Deep. Samples were <span class="hlt">recovered</span> from a Niskin bottle deployed on a passive lander platform that released an arm after touching down on the seafloor. The impact of the arm holding the Niskin bottle caused <span class="hlt">sediments</span> to enter the bottle; this process was seen in images and on video captured by the lander. The combination of imagery and preliminary analyses of the <span class="hlt">sediments</span> indicates that the Sirena Deep locale is a region of serpentinization and active microbial communities. Images show several outcrops consistent with serpentinization, some of which are coated with filamentous microbial mats. Results and analyses of these samples will be presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=308597&keyword=chao&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=308597&keyword=chao&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Changes in northern Gulf of Mexico <span class="hlt">sediment</span> bacterial and archaeal communities exposed to hypoxia</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Biogeochemical changes in marine <span class="hlt">sediments</span> during coastal water hypoxia are well described, but less is known about underlying changes in microbial communities. Bacterial and archaeal communities in Louisiana continental shelf (LCS) hypoxic <span class="hlt">zone</span> <span class="hlt">sediments</span> were characterized by py...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28024210','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28024210"><span>Microplastics in the surface <span class="hlt">sediments</span> from the Beijiang River littoral <span class="hlt">zone</span>: Composition, abundance, surface textures and interaction with heavy metals.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Jundong; Peng, Jinping; Tan, Zhi; Gao, Yifan; Zhan, Zhiwei; Chen, Qiuqiang; Cai, Liqi</p> <p>2017-03-01</p> <p>While large quantities of studies on microplastics in the marine environment have been widely carried out, few were available in the freshwater environment. The occurrence and characteristics, including composition, abundance, surface texture and interaction with heavy metals, of microplastics in the surface <span class="hlt">sediments</span> from Beijiang River littoral <span class="hlt">zone</span> were investigated. The concentrations of microplastics ranged from 178 ± 69 to 544 ± 107 items/kg <span class="hlt">sediment</span>. SEM images illustrated that pits, fractures, flakes and adhering particles were the common patterns of degradation. Chemical weathering of microplastics was also observed and confirmed by μ-FTIR. EDS spectra displayed difference in the elemental types of metals on the different surface sites of individual microplastic, indicating that some metals carried by microplastics were not inherent but were derived from the environment. The content of metals (Ni, Cd, Pb, Cu, Zn and Ti) in microplastics after ultrasonic cleaning has been analyzed by ICP-MS. Based on data from the long-term sorption of metals by microplastics and a comparison of metal burden between microplastics, macroplastics and fresh plastic products, we suggested that the majority of heavy metals carried by microplastics were derived from inherent load. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSEC14C1001C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSEC14C1001C"><span>Field Observations of Swash-<span class="hlt">Zone</span> Dynamics on a Sea-Breeze Dominated Beach at the Yucatán Peninsula, México</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chardon-Maldonado, P.; Puleo, J. A.; Torres-Freyermuth, A.</p> <p>2016-02-01</p> <p>Sea breezes can modify the nearshore processes and alter beach morphology depending on the geographical location. Prior studies have shown that surf <span class="hlt">zone</span> wave energy intensifies during strong sea-breeze conditions (wind speeds > 10 ms-1) and the impact on the coast can be similar to a small storm. However, few research efforts have investigated the coastal dynamics on sea-breeze dominated beaches (e.g., Masselink and Pattiaratchi, 1998, Mar. Geol.; Pattiaratchi et al., 1997, Cont. Shelf Res.) and, to the authors' knowledge, only one study has focused on swash-<span class="hlt">zone</span> processes (Sonu et al., 1973, EOS). A field study was performed on a microtidal, low wave energy, sea-breeze dominated sandy beach in order to investigate the effects of local (sea breeze) and synoptic (storm) scale meteorological events on swash-<span class="hlt">zone</span> dynamics. In-situ measurements of swash-<span class="hlt">zone</span> hydrodynamics and <span class="hlt">sediment</span> transport processes were collected from March 31st to April 12th, 2014 in Sisal, Yucatán located on the northern coast of the Yucatán Peninsula. Flow velocities and suspended <span class="hlt">sediment</span> concentrations were measured concurrently, at multiple cross-shore and alongshore locations, using Vectrino-II profiling velocimeters and optical backscatter sensors, respectively. The high resolution data allowed the quantification of bed shear stress, turbulent dissipation rate, <span class="hlt">sediment</span> loads and <span class="hlt">sediment</span> flux during a mesoscale frontal system (cold-front passage referred to as an El Norte) and local sea-breeze cycles. Field observations showed that strong swash-<span class="hlt">zone</span> bed shear stresses, turbulence intensity and <span class="hlt">sediment</span> suspension occur during energetic conditions (i.e., El Norte event). On the other hand, despite milder energy conditions during the sea-breeze events, the alongshore component of bed-shear stresses and velocities can be significant owing to the high incidence wave angle associated with the sea-breeze system in the study area. The increased forcing in the swash <span class="hlt">zone</span> induced <span class="hlt">sediment</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=544275','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=544275"><span>Simultaneous Recovery of Extracellular and Intracellular DNA Suitable for Molecular Studies from Marine <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Corinaldesi, Cinzia; Danovaro, Roberto; Dell'Anno, Antonio</p> <p>2005-01-01</p> <p>The occurrence of high extracellular DNA concentrations in aquatic <span class="hlt">sediments</span> (concentrations that are 3 to 4 orders of magnitude greater than those in the water column) might play an important role in biogeochemical cycling, as well as in horizontal gene transfer through natural transformation. Since isolation of extracellular DNA from <span class="hlt">sediments</span> is a difficult and unsolved task, in this study we developed an efficient procedure to <span class="hlt">recover</span> simultaneously DNA associated with microbial cells and extracellular DNA from the same <span class="hlt">sediment</span> sample. This procedure is specifically suitable for studying extracellular DNA because it avoids any contamination with DNA released by cell lysis during handling and extraction. Applying this procedure to different <span class="hlt">sediment</span> types, we obtained extracellular DNA concentrations that were about 10 to 70 times higher than the intracellular DNA concentrations. Using specific targeted prokaryotic primers, we obtained evidence that extracellular DNA <span class="hlt">recovered</span> from different <span class="hlt">sediments</span> did not contain amplifiable 16S rRNA genes. By contrast, using DNA extracted from microbial cells as the template, we always amplified 16S rRNA genes. Although 16S rRNA genes were not detected in extracellular DNA, analyses of the sizes of extracellular DNA indicated the presence of high-molecular-weight fragments that might have contained other gene sequences. This protocol allows investigation of extracellular DNA and its possible participation in natural transformation processes. PMID:15640168</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5155368-turboexpander-recovers-energy','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5155368-turboexpander-recovers-energy"><span>Turboexpander <span class="hlt">recovers</span> energy</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Moruzzi, L.; Righi, E.</p> <p>1989-10-01</p> <p>Turboexpanding natural gas in a decompression plant is a useful means to <span class="hlt">recover</span> energy. Italy's natural gas transmission system uses this method in which gas is expanded through a turbine to <span class="hlt">recover</span> the mechanical energy, rather than dissipate it as friction. The turbo expanding system is illustrated and thermodynamic aspects are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18409623','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18409623"><span>Effect of saline waste solution infiltration rates on uranium retention and spatial distribution in Hanford <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wan, Jiamin; Tokunaga, Tetsu K; Kim, Yongman; Wang, Zheming; Lanzirotti, Antonio; Saiz, Eduardo; Serne, R Jeffrey</p> <p>2008-03-15</p> <p>The accidental overfilling of waste liquid from tank BX-102 at the Hanford Site in 1951 put about 10 t of U(VI) into the vadose <span class="hlt">zone</span>. In order to understand the dominant geochemical reactions and transport processes that occurred during the initial infiltration and to help understand current spatial distribution, we simulated the waste liquid spilling event in laboratory <span class="hlt">sediment</span> columns using synthesized metal waste solution. We found that, as the plume propagated through <span class="hlt">sediments</span>, pH decreased greatly (as much as 4 units) at the moving plume front. Infiltration flow rates strongly affect U behavior. Slower flow rates resulted in higher <span class="hlt">sediment</span>-associated U concentrations, and higher flow rates (> or =5 cm/day) permitted practically unretarded U transport. Therefore, given the very high Ksat of most of Hanford formation, the low permeability <span class="hlt">zones</span> within the <span class="hlt">sediment</span> could have been most important in retaining high concentrations of U during initial release into the vadose <span class="hlt">zone</span>. Massive amount of colloids, including U-colloids, formed at the plume fronts. Total U concentrations (aqueous and colloid) within plume fronts exceeded the source concentration by up to 5-fold. Uranium colloid formation and accumulation at the neutralized plume front could be one mechanism responsible for highly heterogeneous U distribution observed in the contaminated Hanford vadose <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T21E2879M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T21E2879M"><span>Quaternary <span class="hlt">Sediment</span> Accumulation in the Aleutian Trench: Implications for Dehydration Reaction Progress and Pore Pressure Development Offshore Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meridth, L. N.; Screaton, E.; Jaeger, J. M.; James, S. R.; Villaseñor, T. G.</p> <p>2015-12-01</p> <p><span class="hlt">Sediment</span> inputs to subduction <span class="hlt">zones</span> impart a significant control on diagenetic reaction progress, fluid production and pore pressure development and thus affect hydrologic and tectonic behavior during subduction. Intensified glaciation following the mid-Pleistocene transition increased <span class="hlt">sediment</span> flux to the Gulf of Alaska. Rapid <span class="hlt">sediment</span> accumulation (>1 km/my) in the Aleutian Trench increases overburden and should accelerate dehydration of hydrous sedimentary components by elevating temperatures in the incoming <span class="hlt">sediment</span> column. These processes have the potential to generate fluid overpressures in the mud-dominated, low permeability <span class="hlt">sediments</span> deposited on the incoming plate, offshore SE Alaska. Mineralogical analyses on incoming <span class="hlt">sediments</span> from Deep Sea Drilling Project Leg 18 and Integrated Ocean Drilling Program Expedition 341 show that both smectite and Opal-A are present as hydrous mineral phases. A 1-D numerical model was developed to track dehydration reaction progress and pore pressures in the incoming <span class="hlt">sediment</span> column from the abyssal plain to the Aleutian Trench. Simulated temperatures in the incoming column increase due to the insulating effect of trench <span class="hlt">sediments</span>. As a result, trench <span class="hlt">sedimentation</span> causes smectite dehydration to begin and Opal-A dehydration to nearly reach completion at the deformation front. Simulated excess pore pressures in the proto-decollement <span class="hlt">zone</span> increase from nearly hydrostatic to almost half of lithostatic due to the rapid deposition of trench <span class="hlt">sediments</span>. The 1-D modeling results were incorporated into a 2-D model that follows the underthrust column at the deformation front into the subduction <span class="hlt">zone</span>. Simulated results of the 2-D flow model illustrate the effects of lateral flow on pore pressure distribution following subduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70174991','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70174991"><span>Methane and sulfate dynamics in <span class="hlt">sediments</span> from mangrove-dominated tropical coastal lagoons, Yucatan, Mexico</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chuang, P. C.; Young, Megan B.; Dale, Andrew W.; Miller, Laurence G.; Herrera-Silveira, Jorge A.; Paytan, Adina</p> <p>2016-01-01</p> <p>Porewater profiles in <span class="hlt">sediment</span> cores from mangrove-dominated coastal lagoons (Celestún and Chelem) on the Yucatán Peninsula, Mexico, reveal the widespread coexistence of dissolved methane and sulfate. This observation is interesting since dissolved methane in porewaters is typically oxidized anaerobically by sulfate. To explain the observations we used a numerical transport-reaction model that was constrained by the field observations. The model suggests that methane in the upper <span class="hlt">sediments</span> is produced in the sulfate reduction <span class="hlt">zone</span> at rates ranging between 0.012 and 31 mmol m−2 d−1, concurrent with sulfate reduction rates between 1.1 and 24 mmol SO42− m−2 d−1. These processes are supported by high organic matter content in the <span class="hlt">sediment</span> and the use of non-competitive substrates by methanogenic microorganisms. Indeed <span class="hlt">sediment</span> slurry incubation experiments show that non-competitive substrates such as trimethylamine (TMA) and methanol can be utilized for microbial methanogenesis at the study sites. The model also indicates that a significant fraction of methane is transported to the sulfate reduction <span class="hlt">zone</span> from deeper <span class="hlt">zones</span> within the sedimentary column by rising bubbles and gas dissolution. The shallow depths of methane production and the fast rising methane gas bubbles reduce the likelihood for oxidation, thereby allowing a large fraction of the methane formed in the <span class="hlt">sediments</span> to escape to the overlying water column.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ESRv..127..171B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ESRv..127..171B"><span>Fault <span class="hlt">zone</span> hydrogeology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bense, V. F.; Gleeson, T.; Loveless, S. E.; Bour, O.; Scibek, J.</p> <p>2013-12-01</p> <p>Deformation along faults in the shallow crust (< 1 km) introduces permeability heterogeneity and anisotropy, which has an important impact on processes such as regional groundwater flow, hydrocarbon migration, and hydrothermal fluid circulation. Fault <span class="hlt">zones</span> have the capacity to be hydraulic conduits connecting shallow and deep geological environments, but simultaneously the fault cores of many faults often form effective barriers to flow. The direct evaluation of the impact of faults to fluid flow patterns remains a challenge and requires a multidisciplinary research effort of structural geologists and hydrogeologists. However, we find that these disciplines often use different methods with little interaction between them. In this review, we document the current multi-disciplinary understanding of fault <span class="hlt">zone</span> hydrogeology. We discuss surface- and subsurface observations from diverse rock types from unlithified and lithified clastic <span class="hlt">sediments</span> through to carbonate, crystalline, and volcanic rocks. For each rock type, we evaluate geological deformation mechanisms, hydrogeologic observations and conceptual models of fault <span class="hlt">zone</span> hydrogeology. Outcrop observations indicate that fault <span class="hlt">zones</span> commonly have a permeability structure suggesting they should act as complex conduit-barrier systems in which along-fault flow is encouraged and across-fault flow is impeded. Hydrogeological observations of fault <span class="hlt">zones</span> reported in the literature show a broad qualitative agreement with outcrop-based conceptual models of fault <span class="hlt">zone</span> hydrogeology. Nevertheless, the specific impact of a particular fault permeability structure on fault <span class="hlt">zone</span> hydrogeology can only be assessed when the hydrogeological context of the fault <span class="hlt">zone</span> is considered and not from outcrop observations alone. To gain a more integrated, comprehensive understanding of fault <span class="hlt">zone</span> hydrogeology, we foresee numerous synergistic opportunities and challenges for the discipline of structural geology and hydrogeology to co-evolve and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JGRF..114.2005N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRF..114.2005N"><span>Response of bed surface patchiness to reductions in <span class="hlt">sediment</span> supply</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nelson, Peter A.; Venditti, Jeremy G.; Dietrich, William E.; Kirchner, James W.; Ikeda, Hiroshi; Iseya, Fujiko; Sklar, Leonard S.</p> <p>2009-06-01</p> <p>River beds are often arranged into patches of similar grain size and sorting. Patches can be distinguished into "free patches," which are <span class="hlt">zones</span> of sorted material that move freely, such as bed load sheets; "forced patches," which are areas of sorting forced by topographic controls; and "fixed patches" of bed material rendered immobile through localized coarsening that remain fairly persistent through time. Two sets of flume experiments (one using bimodal, sand-rich <span class="hlt">sediment</span> and the other using unimodal, sand-free <span class="hlt">sediment</span>) are used to explore how fixed and free patches respond to stepwise reductions in <span class="hlt">sediment</span> supply. At high <span class="hlt">sediment</span> supply, migrating bed load sheets formed even in unimodal, sand-free <span class="hlt">sediment</span>, yet grain interactions visibly played a central role in their formation. In both sets of experiments, reductions in supply led to the development of fixed coarse patches, which expanded at the expense of finer, more mobile patches, narrowing the <span class="hlt">zone</span> of active bed load transport and leading to the eventual disappearance of migrating bed load sheets. Reductions in <span class="hlt">sediment</span> supply decreased the migration rate of bed load sheets and increased the spacing between successive sheets. One-dimensional morphodynamic models of river channel beds generally are not designed to capture the observed variability, but should be capable of capturing the time-averaged character of the channel. When applied to our experiments, a 1-D morphodynamic model (RTe-bookAgDegNormGravMixPW.xls) predicted the bed load flux well, but overpredicted slope changes and was unable to predict the substantial variability in bed load flux (and load grain size) because of the migration of mobile patches. Our results suggest that (1) the distribution of free and fixed patches is primarily a function of <span class="hlt">sediment</span> supply, (2) the dynamics of bed load sheets are primarily scaled by <span class="hlt">sediment</span> supply, (3) channels with reduced <span class="hlt">sediment</span> supply may inherently be unable to transport <span class="hlt">sediment</span> uniformly</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025723','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025723"><span>Inorganic nitrogen transformations in the bed of the Shingobee River, Minnesota: Integrating hydrologic and biological processes using <span class="hlt">sediment</span> perfusion cores</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Sheibley, R.W.; Duff, J.H.; Jackman, A.P.; Triska, F.J.</p> <p>2003-01-01</p> <p>Inorganic N transformations were examined in streambed <span class="hlt">sediments</span> from the Shingobee River using <span class="hlt">sediment</span> perfusion cores. The experimental design simulated groundwater-stream water mixing within <span class="hlt">sediment</span> cores, which provided a well-defined one-dimensional representation of in situ hydrologic conditions. Two distinct hydrologic and chemical settings were preserved in the <span class="hlt">sediment</span> cores: the lowermost <span class="hlt">sediments</span>, perfused with groundwater, remained anaerobic during the incubations, whereas the uppermost <span class="hlt">sediments</span>, perfused with oxic water pumped from the overlying water column, simulated stream water penetration into the bed. The maintenance of oxic and anoxic <span class="hlt">zones</span> formed a biologically active aerobic-anaerobic interface. Ammonium (NH4+) dissolved in groundwater was transported conservatively through the lower core <span class="hlt">zone</span> but was removed as it mixed with aerated recycle water. Concurrently, a small quantity of nitrate (NO3-) equaling ???25% of the NH4+ loss was produced in the upper <span class="hlt">sediments</span>. The NH4+ and NO3- profiles in the uppermost <span class="hlt">sediments</span> resulted from coupled nitrification-denitrification, because assimilation and sorption were negligible. We hypothesize that anaerobic microsites within the aerated upper <span class="hlt">sediments</span> supported denitrification. Rates of nitrification and denitrification in the perfusion cores ranged 42-209 and 53-160 mg N m-2 day-1, respectively. The use of modified perfusion cores permitted the identification and quantification of N transformations and verified process control by surface water exchange into the shallow hyporheic <span class="hlt">zone</span> of the Shingobee River.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28987916','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28987916"><span>Sequential <span class="hlt">Sedimentation</span>-Biofiltration System for the purification of a small urban river (the Sokolowka, Lodz) supplied by stormwater.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Szklarek, S; Wagner, I; Jurczak, T; Zalewski, M</p> <p>2018-01-01</p> <p>The study analyses the efficiency of a Sequentional <span class="hlt">Sedimentation</span>-Biofiltration System (SSBS) built on the Sokolowka river in Lodz (Poland). It was constructed to purify a small urban river whose hydrological regime is dominated by stormwater and meltwater. The SSBS was constructed on a limited area as multi-<span class="hlt">zone</span> constructed wetlands. The SSBS consists of three <span class="hlt">zones</span>: <span class="hlt">sedimentation</span> <span class="hlt">zone</span> with structures added to improve <span class="hlt">sedimentation</span>, a geochemical barrier made of limestone deposit and biofiltration <span class="hlt">zone</span>. The purification processes of total suspended solids (TSS), total phosphorus (TP), total nitrogen (TP) and other nutrients: phosphates (PO 4 3- ), ammonium (NH 4 + ) and nitrates (NO 3 - ) of the SSBS were analyzed. Chloride (Cl - ) reduction was investigated. Monitoring conducted in the first two hydrological years after construction indicated that the SSBS removed 61.4% of TSS, 37.3% of TP, 30.4% of PO 4 3- , 46.1% of TN, 2.8% of NH4+, 44.8% of NO 3 - and 64.0% of Cl - . The <span class="hlt">sedimentation</span> <span class="hlt">zone</span> played a key role in removing TSS and nutrients. The geochemical barrier and biofiltration <span class="hlt">zone</span> each significantly improved overall efficiency by 4-10% for TSS, PO 4 3- , TN, NO 3 - and Cl - . Although the system reduced the concentration of chloride, further studies are needed to determine the circulation of Cl - in constructed wetlands (CWs), and to assess its impact on purification processes. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740021570','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740021570"><span>Dynamic behaviour of coastal <span class="hlt">sedimentation</span> in the Lions Gulf. [France</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Guy, M. (Principal Investigator)</p> <p>1974-01-01</p> <p>The author has identified the following significant results. A number of ERTS-1 images covering this geographical <span class="hlt">zone</span> were studied and compared with cartographic maps, air photographs, and thermal-IR images. Old and recent <span class="hlt">sediments</span> leave traces in the landscape which are decoded by interpreting the shapes of the clear <span class="hlt">zones</span> forming a network against the black background representing water and humid <span class="hlt">zones</span>. Current <span class="hlt">sedimentation</span> and its mechanism were investigated. It had been hoped that a regular sequence of images would make it possible to follow the dynamics of the Rhone and the coastal rivers in relation to meteorological conditions. In any event only a small number of images spread over a wide period of time were obtained, and a complete study was therefore impossible. However, in comparing some of the ERTS-1 images certain thermal-IR images and information on the flow of the Rhone provided some clarification of mechanisms associated with river dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70036063','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70036063"><span>Effect of grain-coating mineralogy on nitrate and sulfate storage in the unsaturated <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reilly, T.J.; Fishman, N.S.; Baehr, A.L.</p> <p>2009-01-01</p> <p>Unsaturated-<span class="hlt">zone</span> <span class="hlt">sediments</span> and the chemistry of shallow groundwater underlying a small (???8-km2) watershed were studied to identify the mechanisms responsible for anion storage within the Miocene Bridgeton Formation and weathered Coastal Plain deposits in southern New Jersey. Lower unsaturated-<span class="hlt">zone</span> <span class="hlt">sediments</span> and shallow groundwater samples were collected and concentrations of selected ions (including NO3- and SO42-) from 11 locations were determined. Grain size, sorting, and color of the lower unsaturated-<span class="hlt">zone</span> <span class="hlt">sediments</span> were determined and the mineralogy of these grains and the composition of coatings were analyzed by petrographic examination, scanning electron microscopy and energy dispersive analysis of x-rays, and quantitative whole-rock x-ray diffraction. The <span class="hlt">sediment</span> grains, largely quartz and chert (80-94% w/w), are coated with a very fine-grained (<20 ??m), complex mixture of kaolinite, halloysite, goethite, and possibly gibbsite and lepidocrocite. The mineral coatings are present as an open fabric, resulting in a large surface area in contact with pore water. Significant correlations between the amount of goethite in the grain coatings and the concentration of <span class="hlt">sediment</span>-bound SO42- were observed, indicative of anion sorption. Other mineral-chemical relations indicate that negatively charged surfaces and competition with SO 42- results in exclusion of NO3- from inner sphere exchange sites. The observed NO3- storage may be a result of matrix forces within the grain coatings and outer sphere complexation. The results of this study indicate that the mineralogy of grain coatings can have demonstrable effects on the storage of NO 3- and SO42- in the unsaturated <span class="hlt">zone</span>. ?? Soil Science Society of America. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029294','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029294"><span><span class="hlt">Sediments</span> in marsh ponds of the Gulf Coast Chenier Plain: Effects of structural marsh management and salinity</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Bolduc, F.; Afton, A.D.</p> <p>2005-01-01</p> <p>Physical characteristics of <span class="hlt">sediments</span> in coastal marsh ponds (flooded <span class="hlt">zones</span> of marsh associated with little vegetation) have important ecological consequences because they determine compositions of benthic invertebrate communities, which in turn influence compositions of waterbird communities. <span class="hlt">Sediments</span> in marsh ponds of the Gulf Coast Chenier Plain potentially are affected by (1) structural marsh management (levees, water control structures and impoundments; SMM), and (2) variation in salinity. Based on available literature concerning effects of SMM on <span class="hlt">sediments</span> in emergent plant <span class="hlt">zones</span> (<span class="hlt">zones</span> of marsh occasionally flooded and associated with dense vegetation) of coastal marshes, we predicted that SMM would increase <span class="hlt">sediment</span> carbon content and <span class="hlt">sediment</span> hardness, and decrease oxygen penetration (O2 depth) and the silt-clay fraction in marsh pond <span class="hlt">sediments</span>. Assuming that freshwater marshes are more productive than are saline marshes, we also predicted that <span class="hlt">sediments</span> of impounded freshwater marsh ponds would contain more carbon than those of impounded oligohaline and mesohaline marsh ponds, whereas C:N ratio, <span class="hlt">sediment</span> hardness, silt-clay fraction, and O2 depth would be similar among pond types. Accordingly, we measured <span class="hlt">sediment</span> variables within ponds of impounded and unimpounded marshes on Rockefeller State Wildlife Refuge, near Grand Chenier, Louisiana. To test the above predictions, we compared <span class="hlt">sediment</span> variables (1) between ponds of impounded (IM) and unimpounded mesohaline marshes (UM), and (2) among ponds of impounded freshwater (IF), oligohaline (IO), and mesohaline (IM) marshes. An a priori multivariate analysis of variance (MANOVA) contrast indicated that <span class="hlt">sediments</span> differed between IM and UM marsh ponds. As predicted, the silt-clay fraction and O2 depth were lower and carbon content, C:N ratio, and <span class="hlt">sediment</span> hardness were higher in IM than in UM marsh ponds. An a priori MANOVA contrast also indicated that <span class="hlt">sediments</span> differed among IF, IO, and IM marsh ponds. As</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JESS..126...37Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JESS..126...37Z"><span>Fault <span class="hlt">zone</span> architecture within Miocene-Pliocene syn-rift <span class="hlt">sediments</span>, Northwestern Red Sea, Egypt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zaky, Khairy S.</p> <p>2017-04-01</p> <p>The present study focusses on field description of small normal fault <span class="hlt">zones</span> in Upper Miocene-Pliocene sedimentary rocks on the northwestern side of the Red Sea, Egypt. The trend of these fault <span class="hlt">zones</span> is mainly NW-SE. Paleostress analysis of 17 fault planes and slickenlines indicate that the tension direction is NE-SW. The minimum ( σ3) and intermediate ( σ2) paleostress axes are generally sub-horizontal and the maximum paleostress axis ( σ1) is sub-vertical. The fault <span class="hlt">zones</span> are composed of damage <span class="hlt">zones</span> and fault core. The damage <span class="hlt">zone</span> is characterized by subsidiary faults and fractures that are asymmetrically developed on the hanging wall and footwall of the main fault. The width of the damage <span class="hlt">zone</span> varies for each fault depending on the lithology, amount of displacement and irregularity of the fault trace. The average ratio between the hanging wall and the footwall damage <span class="hlt">zones</span> width is about 3:1. The fault core consists of fault gouge and breccia. It is generally concentrated in a narrow <span class="hlt">zone</span> of ˜0.5 to ˜8 cm width. The overall pattern of the fault core indicates that the width increases with increasing displacement. The faults with displacement < 1 m have fault cores ranging from 0.5 to 4.0 cm, while the faults with displacements of > 2 m have fault cores ranging from 4.0 to 8.0 cm. The fault <span class="hlt">zones</span> are associated with sliver fault blocks, clay smear, segmented faults and fault lenses' structural features. These features are mechanically related to the growth and linkage of the fault arrays. The structural features may represent a neotectonic and indicate that the architecture of the fault <span class="hlt">zones</span> is developed as several tectonic phases.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12666796','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12666796"><span>In situ observation of the water-<span class="hlt">sediment</span> interface in combined sewers, using endoscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Oms, C; Gromaire, M C; Chebbo, G</p> <p>2003-01-01</p> <p>A new method for water-<span class="hlt">sediment</span> interface observation has been designed. This system is based on a small diameter endoscope protected by a graduated plastic tube. It makes it possible to visualise in a non-destructive manner the <span class="hlt">sediments</span> and the water-<span class="hlt">sediment</span> interface. The endoscope was used to investigate Le Marais catchment (Paris): an immobile organic layer was observed at the water-<span class="hlt">sediment</span> interface. This layer appears in pools of gross bed <span class="hlt">sediment</span>, at the upstream of collectors, in <span class="hlt">zones</span> where velocity is slow and where bed shear stress is less than 0.03 N/m2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1610588A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1610588A"><span>Distribution of heavy metals in riverine soils and <span class="hlt">sediments</span> of the Turia River basin.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andreu, Vicente; Gimeno-García, Eugenia; Pascual, Juan Antonio</p> <p>2014-05-01</p> <p>Water is a scarce and contested good, and a primary need for the population all over. Rivers are one of the mainsources of freshwater to people but, in the same way, receive both point source and difuse pollution, usually frorm wastewaters and agriculture. However, they are not independent bodies but they influence different associated ecosystems that compound the catchment. Soils of the river banks often acts as the last phase of the diffuse contamination pathways, favouring the contaminants input to the river waters. In this sense, the fluvial sedimentary phase usually acts as a sink of pollutants. <span class="hlt">Sediments</span> can work as resevoirs that accumulate contaminants fixing them or allowing their decomposition or metabolization. However, environmental or human induced, such as variations in water pH, increases in the turbulence or intensity of the water flow, etc.could favour their release to the environment. In this work, the incidence and distribution of seven heavy metals was monitored in riverine soils and <span class="hlt">sediments</span> of the Turia River. Along the river course, 22 <span class="hlt">zones</span> were selected for sampling according different lithologies, land uses, size of populations and the proximity to waste waters treatment plants (WWTPs), from the headwaters to the mouth. The selected metals (Cd, Co, Cr, Cu, Pb, Ni and Zn) were analysed to determine its total and extractable contents in the <span class="hlt">sediments</span>. Total content of metals was extracted by microwave acid digestion and the extractable fraction by treatment with EDTA. Atomic Absorption Spectrometry, using graphite furnace when necessary, was used for the determination of all metals. Highest values for <span class="hlt">sediments</span> were mainly observed in <span class="hlt">zones</span> 10 and 22, close to urban areas, reaching values of 172.86 mg/kg for Pb, or 58.34 mg/kg for Cr. However, <span class="hlt">zone</span> 2 near in the headwaters of the Alfambra River and supposedly of reference for the River authorities shows the highest values of zinc with 96.96 mg/kg. Regarding the available</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMEP33A1029D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMEP33A1029D"><span>Control of <span class="hlt">Sediment</span> Availability on the Path of Channel Recovery in Bedload-Dominated Rivers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Doyle, H.; Renshaw, C. E.; Magilligan, F. J.</p> <p>2015-12-01</p> <p>Following a disturbance, a channel can <span class="hlt">recover</span> to an equilibrium form by adjusting its slope, width, depth, grain size, or some combination of these dimensions that define the recovery path. In this study we relate the channel recovery path to the quantity and caliber of <span class="hlt">sediment</span> introduced due to dam construction/removal or erosion caused by flooding. We suggest that the recovery path of a channel depends on the availability of <span class="hlt">sediment</span> of a size that is transported as bedload during bankfull flows (the "mobile fraction"). We define a ratio, S*, of the <span class="hlt">sediment</span> volume added to the channel because of the disturbance to the average annual <span class="hlt">sediment</span> flux. We compare S* values to the recovery path of New England gravel-bedded streams following two dam emplacements and removals and flooding related to Tropical Storm Irene. Pelham Dam in Pelham, MA (removed 2012) and Kendrick Dam in Pittsford, VT (removed 2014) were on similar streams: drainage areas ~25 km2, slopes 1-2%, and bankfull widths ~10 m. <span class="hlt">Sediment</span> was excavated from both impoundments prior to removal, resulting in lower S* values. Irene-affected study sites are on ~10 gravel-bedded streams in VT, NH, and MA. <span class="hlt">Sediment</span> input at these sites is due to bank failures and landslides, many of which continue to supply <span class="hlt">sediment</span> to the channel four years after flooding. To track recovery we collected annual topographic and <span class="hlt">sediment</span> size data and calculated Shields numbers to determine if channels had reached an equilibrium form. We define equilibrium for bedload rivers as Shields numbers at bankfull discharge equal to that required to initiate bedload transport. Following dam emplacements the channels failed to <span class="hlt">recover</span> because mobile <span class="hlt">sediment</span> was unavailable. Fining dominated the recovery at Irene-affected sites (~10% reduction in <span class="hlt">sediment</span> size) and dam removal sites (up to 30-60% reduction) with little post-disturbance change in channel geometry, possibly due to the limited mobile fraction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BGeo...10.7161L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BGeo...10.7161L"><span>Macrofaunal colonization across the Indian margin oxygen minimum <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Levin, L. A.; McGregor, A. L.; Mendoza, G. F.; Woulds, C.; Cross, P.; Witte, U.; Gooday, A. J.; Cowie, G.; Kitazato, H.</p> <p>2013-11-01</p> <p>There is a growing need to understand the ability of bathyal assemblages to <span class="hlt">recover</span> from disturbance and oxygen stress, as human activities and expanding oxygen minimum <span class="hlt">zones</span> increasingly affect deep continental margins. The effects of a pronounced oxygen minimum <span class="hlt">zone</span> (OMZ) on slope benthic community structure have been studied on every major upwelling margin; however, little is known about the dynamics or resilience of these benthic populations. To examine the influence of oxygen and phytodetritus on short-term settlement patterns, we conducted colonization experiments at 3 depths on the West Indian continental margin. Four colonization trays were deployed at each depth for 4 days at 542 and 802 m (transect 1-16°58' N) and for 9 days at 817 and 1147 m (transect 2-17°31' N). Oxygen concentrations ranged from 0.9 μM (0.02 mL L-1) at 542 m to 22 μM (0.5 mL L-1) at 1147 m. All trays contained local defaunated <span class="hlt">sediments</span>; half of the trays at each depth also contained 13C/15N-labeled phytodetritus mixed into the <span class="hlt">sediments</span>. <span class="hlt">Sediment</span> cores were collected between 535 m and 1140 m from 2 cross-margin transects for analysis of ambient (source) macrofaunal (>300 μm) densities and composition. Ambient macrofaunal densities ranged from 0 ind m-2 (at 535-542 m) to 7400 ind m-2, with maximum values on both transects at 700-800 m. Macrofaunal colonizer densities ranged from 0 ind m-2 at 542 m, where oxygen was lowest, to average values of 142 ind m-2 at 800 m, and 3074 ind m-2 at 1147 m, where oxygen concentration was highest. These were equal to 4.3 and 151% of the ambient community at 800 m and 1147 m, respectively. Community structure of settlers showed no response to the presence of phytodetritus. Increasing depth and oxygen concentration, however, significantly influenced the community composition and abundance of colonizing macrofauna. Polychaetes constituted 92.4% of the total colonizers, followed by crustaceans (4.2%), mollusks (2.5%), and echinoderms (0.8%). The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050060920','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050060920"><span>Application of Remote Sensing to Assess the Impact of Short Term Climate Variability on Coastal <span class="hlt">Sedimentation</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Menzel, W. Paul; Huh, Oscar K.; Walker, Nan</p> <p>2004-01-01</p> <p>The purpose of this joint University of Wisconsin (UW) and Louisiana State University (LSU) project has been to relate short term climate variation to response in the coastal <span class="hlt">zone</span> of Louisiana in an attempt to better understand how the coastal <span class="hlt">zone</span> is shaped by climate variation. Climate variation in this case largely refers to variation in surface wind conditions that affect wave action and water currents in the coastal <span class="hlt">zone</span>. The primary region of focus was the Atchafalaya Bay and surrounding bays in the central coastal region of Louisiana. Suspended solids in the water column show response to wind systems both in quantity (through resuspension) and in the pattern of dispersement or transport. Wind systems associated with cold fronts are influenced by short term climate variation. Wind energy was used as the primary signature of climate variation in this study because winds are a significant influence on <span class="hlt">sediment</span> transport in the micro-tidal Gilf of Mexico coastal <span class="hlt">zone</span>. Using case studies, the project has been able to investigate the influence of short term climate variation on <span class="hlt">sediment</span> transport. Wind energy data, collected daily for National Weather Service (NWS) stations at Lake Charles and New Orleans, LA, were used as an indicator of short term climate variation influence on seasonal time scales. A goal was to relate wind energy to coastal impact through <span class="hlt">sediment</span> transport. This goal was partially accomplished by combining remote sensing and wind energy data. Daily high resolution remote sensing observations are needed to monitor the complex coastal <span class="hlt">zone</span> environment, where winds, tides, and water level all interact to influence <span class="hlt">sediment</span> transport. The NASA Earth Observing System (EOS) era brings hope for documenting and revealing response of the complex coastal transport mosaic through regular high spatial resolution observations from the Moderate resolution Imaging Spectrometer (MODIS) instrument. MODIS observations were sampled in this project for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.C11A1062U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.C11A1062U"><span>Origin Of Methane Gas And Migration Through The Gas Hydrate Stability <span class="hlt">Zone</span> Beneath The Permafrost <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Uchida, T.; Waseda, A.; Namikawa, T.</p> <p>2005-12-01</p> <p>In 1998 and 2002 Mallik wells were drilled at Mackenzie Delta in the Canadian Arctic that clarified the characteristics of gas hydrate-dominant sandy layers at depths from 890 to 1110 m beneath the permafrost <span class="hlt">zone</span>. Continuous downhole well log data as well as visible gas hydrates have confirmed pore-space hydrate as intergranular pore filling within sandy layers whose saturations are up to 80% in pore volume, but muddy <span class="hlt">sediments</span> scarcely contain. Plenty of gas hydrate-bearing sand core samples have been obtained from the Mallik wells. According to grain size distributions pore-space hydrate is dominant in medium- to very fine-grained sandy strata. Methane gas accumulation and original pore space large enough to occur within host <span class="hlt">sediments</span> may be required for forming highly saturated gas hydrate in pore system. The distribution of a porous and coarser-grained host rock should be one of the important factors to control the occurrence of gas hydrate, as well as physicochemical conditions. Subsequent analyses in sedimentology and geochemistry performed on gas hydrate-bearing sandy core samples also revealed important geologic and sedimentological controls on the formation and concentration of natural gas hydrate. This appears to be a similar mode for conventional oil and gas accumulations. It is necessary for investigating subsurface fluid flow behaviors to evaluate both porosity and permeability of gas hydrate-bearing sandy <span class="hlt">sediments</span>, and the measurements of water permeability for them indicate that highly saturated sands may have permeability of a few millidarcies. The isotopic data of methane show that hydrocarbon gas contained in gas hydrate is generated by thermogenic decomposition of kerogen in deep mature <span class="hlt">sediments</span>. Based on geochemical and geological data, methane is inferred to migrate upward closely associated with pore water hundreds of meters into and through the hydrate stability <span class="hlt">zone</span> partly up to the permafrost <span class="hlt">zone</span> and the surface along faults and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP43A2253Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP43A2253Z"><span>Microbial Nitrogen Cycling Associated with the Early Diagenesis of Organic Matter in Subseafloor <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, R.</p> <p>2015-12-01</p> <p>The early diagenesis of organic matter is the major energy source of marine sedimentary biosphere and thus controls its population size; however, the vertical distribution of any functional groups along with the diagenesis of organic matter is remained unclear, especially for those microbes involved in nitrogen transformation which serve as a major control on the nitrogen flux between reservoirs. Here we investigated the vertical distributions of various functional groups in five <span class="hlt">sediment</span> cores retrieved from Arctic Mid-Ocean Ridge (AMOR), with emphasis on the nitrifiers, denitrifiers and anaerobic ammonium oxidizing bacteria (anammox). We observed the clear geochemical zonation associated with organic matter diagenesis in the <span class="hlt">sediments</span> based on the pore water profiles of oxygen, nitrate, ammonium, manganese and sulfate, with distinct geochemical transition <span class="hlt">zones</span> at the boundaries of geochemical <span class="hlt">zones</span>, including oxic-anoxic transition <span class="hlt">zone</span> (OATZ) and nitrate-manganese reduction <span class="hlt">zone</span> (NMTZ). Nitrate was produced in surface oxygenated <span class="hlt">sediments</span> and nitrate consumption mainly took place at the NMTZ, splitted between re-oxidation of ammonium and manganese (II). Abundances of ammonia oxidizers, nitrite oxidizers, and denitrifiers, estimated through quantitative PCR targeting their respective functional genes, generally decrease with depth, but constantly elevated around the OATZ, NMTZ, and manganese-reduction <span class="hlt">zone</span> as well. Anammox bacteria were only detected around the NMTZ where both nitrate/nitrite and ammonium are available. These depth profiles of functional groups were also confirmed by the community structure profiling by prokaryotic 16S rRNA gene tag pyrosequencing. Cell-specific rates of nitrification and denitrification, calculated from the bulk net reaction rates divided by functional group abundances, were similar to those values from oligotrophic <span class="hlt">sediments</span> like North Pond and thus suggested that nitrifiers and denitirifiers populations were in maintenance</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012GGG....13.AD27K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012GGG....13.AD27K"><span>Mechanical and hydraulic properties of Nankai accretionary prism <span class="hlt">sediments</span>: Effect of stress path</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitajima, Hiroko; Chester, Frederick M.; Biscontin, Giovanna</p> <p>2012-10-01</p> <p>We have conducted triaxial deformation experiments along different loading paths on prism <span class="hlt">sediments</span> from the Nankai Trough. Different load paths of isotropic loading, uniaxial strain loading, triaxial compression (at constant confining pressure, Pc), undrained Pc reduction, drained Pc reduction, and triaxial unloading at constant Pc, were used to understand the evolution of mechanical and hydraulic properties under complicated stress states and loading histories in accretionary subduction <span class="hlt">zones</span>. Five deformation experiments were conducted on three <span class="hlt">sediment</span> core samples for the Nankai prism, specifically from older accreted <span class="hlt">sediments</span> at the forearc basin, underthrust slope <span class="hlt">sediments</span> beneath the megasplay fault, and overthrust Upper Shikoku Basin <span class="hlt">sediments</span> along the frontal thrust. Yield envelopes for each sample were constructed based on the stress paths of Pc-reduction using the modified Cam-clay model, and in situ stress states of the prism were constrained using the results from the other load paths and accounting for horizontal stress. Results suggest that the <span class="hlt">sediments</span> in the vicinity of the megasplay fault and frontal thrust are highly overconsolidated, and thus likely to deform brittle rather than ductile. The porosity of <span class="hlt">sediments</span> decreases as the yield envelope expands, while the reduction in permeability mainly depends on the effective mean stress before yield, and the differential stress after yield. An improved understanding of <span class="hlt">sediment</span> yield strength and hydromechanical properties along different load paths is necessary to treat accurately the coupling of deformation and fluid flow in accretionary subduction <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999GGG.....1..007J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999GGG.....1..007J"><span>Dehydration and melting experiments constrain the fate of subducted <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, Marie C.; Plank, Terry</p> <p>1999-12-01</p> <p>Geochemical tracers demonstrate that elements are cycled from subducted <span class="hlt">sediments</span> into the arc melting regime at subduction <span class="hlt">zones</span>, although the transfer mechanism is poorly understood. Are key elements (Th, Be, Rb) lost during <span class="hlt">sediment</span> dehydration or is <span class="hlt">sediment</span> melting required? To investigate this question, we conducted phase equilibria and trace element partitioning experiments on a pelagic red clay for conditions appropriate to the slab beneath arc volcanoes (2-4 GPa, 600°-1000°C). Using both piston cylinders and multianvils, we determined the solidus, phase stabilities, and major element compositions of coexisting phases. The solidus (H2O + Cl fluid-saturated) was located at 775 +/- 25°C at 2 GPa, 810 +/- 15°C at 3 GPa, and 1025 +/- 25°C at 4 GPa with noevidence for complete miscibility between melt and fluid. This <span class="hlt">sediment</span> composition produces a profusion of phases both above and below the solidus: garnet, jadeitic pyroxene, alkali-rich amphibole, phengite, biotite, magnetite, coesite, kyanite, apatite, zircon, Cl-rich fluids, and peraluminous to peralkaline granitic melts. At 2 GPa the phengite dehydration solidus is at 800°-825°C, while biotite breaks down between 850° and 900°C. To explore trace element partitioning across the solidus at 2 GPa, we used diamonds to trap fluids and melts. Both the bulk <span class="hlt">sediment</span> residues and diamond traps were analyzed postexperiment by inductively coupled plasma-mass spectrometry (ICP-MS) and inductively coupled plasma-atomic emission spectrometry (ICP-AES) for 40 elements for which we calculated bulk partition coefficients (D = Csolid/Cfluid). Below the solidus, Rb, Sr, Ba, and Pb showed the greatest mobility (D ~ 0.5-1.0), while at the solidus, Th and Be became notably partitioned into the melt (D values changing from >2.0 to <1.0). K and Rb D values fall below 1.0 when the micas breakdown. Only at the solidus do Th and Rb attain similar partition coefficients, a condition required by arc data. Taken together, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000GGG.....1.1007J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000GGG.....1.1007J"><span>Dehydration and melting experiments constrain the fate of subducted <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Johnson, Marie C.; Plank, Terry</p> <p>2000-12-01</p> <p>Geochemical tracers demonstrate that elements are cycled from subducted <span class="hlt">sediments</span> into the arc melting regime at subduction <span class="hlt">zones</span>, although the transfer mechanism is poorly understood. Are key elements (Th, Be, Rb) lost during <span class="hlt">sediment</span> dehydration or is <span class="hlt">sediment</span> melting required? To investigate this question, we conducted phase equilibria and trace element partitioning experiments on a pelagic red clay for conditions appropriate to the slab beneath arc volcanoes (2-4 GPa, 600°-1000°C). Using both piston cylinders and multianvils, we determined the solidus, phase stabilities, and major element compositions of coexisting phases. The solidus (H2O + Cl fluid-saturated) was located at 775 ± 25°C at 2 GPa, 810 ± 15°C at 3 GPa, and 1025 ± 25°C at 4 GPa with noevidence for complete miscibility between melt and fluid. This <span class="hlt">sediment</span> composition produces a profusion of phases both above and below the solidus: garnet, jadeitic pyroxene, alkali-rich amphibole, phengite, biotite, magnetite, coesite, kyanite, apatite, zircon, Cl-rich fluids, and peraluminous to peralkaline granitic melts. At 2 GPa the phengite dehydration solidus is at 800°-825°C, while biotite breaks down between 850° and 900°C. To explore trace element partitioning across the solidus at 2 GPa, we used diamonds to trap fluids and melts. Both the bulk <span class="hlt">sediment</span> residues and diamond traps were analyzed postexperiment by inductively coupled plasma-mass spectrometry (ICP-MS) and inductively coupled plasma-atomic emission spectrometry (ICP-AES) for 40 elements for which we calculated bulk partition coefficients (D = Csolid/Cfluid). Below the solidus, Rb, Sr, Ba, and Pb showed the greatest mobility (D ˜ 0.5-1.0), while at the solidus, Th and Be became notably partitioned into the melt (D values changing from >2.0 to <1.0). K and Rb D values fall below 1.0 when the micas breakdown. Only at the solidus do Th and Rb attain similar partition coefficients, a condition required by arc data. Taken together, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.B51B0403R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.B51B0403R"><span>Depositionally controlled recycling of iron and sulfur in marine <span class="hlt">sediments</span> and its isotopic consequences</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Riedinger, N.; Formolo, M.; Arnold, G. L.; Vossmeyer, A.; Henkel, S.; Sawicka, J.; Kasten, S.; Lyons, T. W.</p> <p>2011-12-01</p> <p>The continental margin off Uruguay and Argentina is characterized by highly dynamic depositional conditions. This variable depositional regime significantly impacts the biogeochemical cycles of iron and sulfur. Mass deposit related redeposition of reduced minerals can lead to the reoxidation of these phases and thus to an overprint of their geochemical primary signatures. Due to rapid burial these oxidized phases are still present in deeper subsurface <span class="hlt">sediments</span>. To study the effects of <span class="hlt">sediment</span> relocation on the sulfur and iron inventory we collected shallow and deep subsurface <span class="hlt">sediment</span> samples via multicorer and gravity cores, respectively, in the western Argentine Basin during the RV Meteor Expedition M78/3 in May-July 2009. The samples were retrieved from shelf, slope and deep basin sites. The concentration and sulfur isotope composition of acid volatile sulfur (AVS), chromium reducible sulfur (CRS), elemental sulfur and total organic sulfur were determined. Furthermore, sequential iron extraction techniques were applied assess the distribution of iron oxide phases within the <span class="hlt">sediment</span>. The investigated <span class="hlt">sediments</span> are dominated by terrigenous inputs, with high amounts of reactive ferric iron minerals and only low concentrations of calcium carbonate. Total organic carbon concentrations show strong variation in the shallow subsurface <span class="hlt">sediments</span> ranging between approximately 0.7 and 6.4 wt% for different sites. These concentrations do not correlate with water depths. Pore water accumulations of hydrogen sulfide are restricted to an interval at the sulfate-methane transition (SMT) <span class="hlt">zone</span> a few meters below the <span class="hlt">sediment</span> surface. In these deeper subsurface <span class="hlt">sediments</span> pyrite is precipitated in this <span class="hlt">zone</span> of hydrogen sulfide excess, whereas the accumulation of authigenic AVS and elemental sulfur (up to 2000 ppm) occurs at the upper and lower boundary of the sulfidic <span class="hlt">zone</span> due the reaction of iron oxides with limited amounts of sulfide. Furthermore, our preliminary results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSMM44B0495S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSMM44B0495S"><span>The nature and function of microbial enzymes in subsurface marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Steen, A. D.; Schmidt, J.</p> <p>2016-02-01</p> <p>Isotopic and genomic evidence indicates that marine <span class="hlt">sediments</span> contain populations of active heterotrophic microorganisms which appear to metabolize old, detrital, apparently recalcitrant organic matter. In surface communities, heterotrophs use extracellular enzymes to access complex organic matter. In subsurface <span class="hlt">sediments</span>, in which microbial doubling times can be on the order of hundreds or thousands of years, it is not clear whether extracellular enzymes could remain stable and active long enough to constitute a 'profitable' stragtegy for accessing complex organic carbon. Here we present evidence that a wide range of extracellular enzyme are active in subsurface <span class="hlt">sediments</span> from two different environments: the White Oak River, NC, and deep (up to 80 m) <span class="hlt">sediments</span> of the Baltic Sea Basin <span class="hlt">recovered</span> from IODP Expedition 347. In the White Oak River, enzymes from deeper <span class="hlt">sediments</span> appear to be better-adapted to highly-degraded organic matter than enzymes from surface <span class="hlt">sediments</span>. In the Baltic Sea, preliminary data suggest that enzymes related to nitrogen acquisition are preferentially expressed. By characterizing the extracellular enzymes present in marine <span class="hlt">sediments</span>, we hope to achieve a better understanding of the mechanisms that control sedimentary organic matter remineralization and preservation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5905238','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5905238"><span>Energy Gradients Structure Microbial Communities Across <span class="hlt">Sediment</span> Horizons in Deep Marine <span class="hlt">Sediments</span> of the South China Sea</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Graw, Michael F.; D'Angelo, Grace; Borchers, Matthew; Thurber, Andrew R.; Johnson, Joel E.; Zhang, Chuanlun; Liu, Haodong; Colwell, Frederick S.</p> <p>2018-01-01</p> <p>The deep marine subsurface is a heterogeneous environment in which the assembly of microbial communities is thought to be controlled by a combination of organic matter deposition, electron acceptor availability, and sedimentology. However, the relative importance of these factors in structuring microbial communities in marine <span class="hlt">sediments</span> remains unclear. The South China Sea (SCS) experiences significant variability in <span class="hlt">sedimentation</span> across the basin and features discrete changes in sedimentology as a result of episodic deposition of turbidites and volcanic ashes within lithogenic clays and siliceous or calcareous ooze deposits throughout the basin's history. Deep subsurface microbial communities were recently sampled by the International Ocean Discovery Program (IODP) at three locations in the SCS with <span class="hlt">sedimentation</span> rates of 5, 12, and 20 cm per thousand years. Here, we used Illumina sequencing of the 16S ribosomal RNA gene to characterize deep subsurface microbial communities from distinct <span class="hlt">sediment</span> types at these sites. Communities across all sites were dominated by several poorly characterized taxa implicated in organic matter degradation, including Atribacteria, Dehalococcoidia, and Aerophobetes. Sulfate-reducing bacteria comprised only 4% of the community across sulfate-bearing <span class="hlt">sediments</span> from multiple cores and did not change in abundance in <span class="hlt">sediments</span> from the methanogenic <span class="hlt">zone</span> at the site with the lowest <span class="hlt">sedimentation</span> rate. Microbial communities were significantly structured by <span class="hlt">sediment</span> age and the availability of sulfate as an electron acceptor in pore waters. However, microbial communities demonstrated no partitioning based on the <span class="hlt">sediment</span> type they inhabited. These results indicate that microbial communities in the SCS are structured by the availability of electron donors and acceptors rather than sedimentological characteristics. PMID:29696012</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=106118','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=106118"><span>Anaerobic Benzene Degradation in Petroleum-Contaminated Aquifer <span class="hlt">Sediments</span> after Inoculation with a Benzene-Oxidizing Enrichment</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Weiner, Jonathan M.; Lovley, Derek R.</p> <p>1998-01-01</p> <p><span class="hlt">Sediments</span> from the sulfate-reduction <span class="hlt">zone</span> of a petroleum-contaminated aquifer, in which benzene persisted, were inoculated with a benzene-oxidizing, sulfate-reducing enrichment from aquatic <span class="hlt">sediments</span>. Benzene was degraded, with apparent growth of the benzene-degrading population over time. These results suggest that the lack of benzene degradation in the sulfate-reduction <span class="hlt">zones</span> of some aquifers may result from the failure of the appropriate benzene-degrading sulfate reducers to colonize the aquifers rather than from environmental conditions that are adverse for anaerobic benzene degradation. PMID:9464422</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeCoA.224..171Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeCoA.224..171Z"><span>Relative importance of methylotrophic methanogenesis in <span class="hlt">sediments</span> of the Western Mediterranean Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhuang, Guang-Chao; Heuer, Verena B.; Lazar, Cassandre S.; Goldhammer, Tobias; Wendt, Jenny; Samarkin, Vladimir A.; Elvert, Marcus; Teske, Andreas P.; Joye, Samantha B.; Hinrichs, Kai-Uwe</p> <p>2018-03-01</p> <p>Microbial production of methane is an important terminal metabolic process during organic matter degradation in marine <span class="hlt">sediments</span>. It is generally acknowledged that hydrogenotrophic and acetoclastic methanogenesis constitute the dominant pathways of methane production; the importance of methanogenesis from methylated compounds remains poorly understood. We conducted various biogeochemical and molecular genetic analyses to characterize substrate availability, rates of methanogenesis, and methanogen community composition, and further evaluated the contribution of different substrates and pathways for methane production in deltaic surface and subsurface <span class="hlt">sediments</span> of the Western Mediterranean Sea. Major substrates representing three methanogenic pathways, including H2, acetate, and methanol, trimethylamine (TMA), and dimethylsulfide (DMS), were detected in the pore waters and <span class="hlt">sediments</span>, and exhibited variability over depth and between sites. In accompanying incubation experiments, methanogenesis rates from various 14C labeled substrates varied as well, suggesting that environmental factors, such as sulfate concentration and organic matter quality, could significantly influence the relative importance of individual pathway. In particular, methylotrophic and hydrogenotrophic methanogenesis contributed to the presence of micromolar methane concentrations in the sulfate reduction <span class="hlt">zone</span>, with methanogenesis from methanol accounting for up to 98% of the total methane production in the topmost surface <span class="hlt">sediment</span>. In the sulfate-depleted <span class="hlt">zone</span>, hydrogenotrophic methanogenesis was the dominant methanogenic pathway (67-98%), and enhanced methane production from acetate was observed in organic-rich <span class="hlt">sediment</span> (up to 31%). Methyl coenzyme M reductase gene (mcrA) analysis revealed that the composition of methanogenic communities was generally consistent with the distribution of methanogenic activity from different substrates. This study provides the first quantitative assessment of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30c0702A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30c0702A"><span>Numerical and experimental analysis of the <span class="hlt">sedimentation</span> of spherical colloidal suspensions under centrifugal force</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Antonopoulou, Evangelia; Rohmann-Shaw, Connor F.; Sykes, Thomas C.; Cayre, Olivier J.; Hunter, Timothy N.; Jimack, Peter K.</p> <p>2018-03-01</p> <p>Understanding the <span class="hlt">sedimentation</span> behaviour of colloidal suspensions is crucial in determining their stability. Since <span class="hlt">sedimentation</span> rates are often very slow, centrifugation is used to expedite <span class="hlt">sedimentation</span> experiments. The effect of centrifugal acceleration on <span class="hlt">sedimentation</span> behaviour is not fully understood. Furthermore, in <span class="hlt">sedimentation</span> models, interparticle interactions are usually omitted by using the hard-sphere assumption. This work proposes a one-dimensional model for <span class="hlt">sedimentation</span> using an effective maximum volume fraction, with an extension for <span class="hlt">sedimentation</span> under centrifugal force. A numerical implementation of the model using an adaptive finite difference solver is described. Experiments with silica suspensions are carried out using an analytical centrifuge. The model is shown to be a good fit with experimental data for 480 nm spherical silica, with the effects of centrifugation at 705 rpm studied. A conversion of data to Earth gravity conditions is proposed, which is shown to <span class="hlt">recover</span> Earth gravity <span class="hlt">sedimentation</span> rates well. This work suggests that the effective maximum volume fraction accurately captures interparticle interactions and provides insights into the effect of centrifugation on <span class="hlt">sedimentation</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1180/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1180/"><span>Organic Geochemistry of <span class="hlt">Sediments</span> in Nearshore Areas of the Mississippi and Atchafalaya Rivers: I. General Organic Characterization</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Orem, William H.; Rosenbauer, Robert J.; Swarzenski, Peter W.; Lerch, Harry E.; Corum, Margo D.; Bates, Anne L.</p> <p>2007-01-01</p> <p>This report presents results on the general organic characteristics of <span class="hlt">sediment</span> cores collected from the coastal <span class="hlt">zone</span> of the Mississippi River system, including distributions of the important nutrient elements (C, N, P, and S). This was part of a larger study conducted from 2001-2005 to examine the delivery of <span class="hlt">sediment</span>-associated contaminants to the Gulf of Mexico by the Mississippi River system, funded by the USGS Coastal and Marine Geology Program. Companion reports emphasize organic contaminants (Rosenbauer and others, 2006), and metals (Swarzenski and others, 2006). The level of contamination within the deltaic system of the Mississippi River system was determined through the collection of <span class="hlt">sediment</span> cores from interdistributary bays, and offshore in the Gulf of Mexico, including the <span class="hlt">zone</span> of hypoxia. Results provide the basis for reconstructing contaminant inventories from which to develop historic perspectives on nutrient loading and hypoxia, and to better understand how <span class="hlt">sediment</span>-hosted contaminants either directly or indirectly move through biota and ultimately affect ecosystem health. Concentrations of C, N, P, and S in <span class="hlt">sediments</span> varied by a factor of 10 between sites, and in down core profiles. Nearshore cores collected in 2001 proved to have erratic downcore C, N, P, and S profiles and <span class="hlt">sediment</span> deposition rates, suggesting a high energy regime controlled more by variability in river flow rather than by geochemical processes and reactions within the system. These results focused further coring activities further offshore. Atomic C/N ratios suggest that organic matter deposited at all sites is a mix of microbial (algal) and terrestrial (vascular plant) remains, but with algal material dominant. Concentrations of total sulfur in <span class="hlt">sediments</span> from cores in the <span class="hlt">zone</span> of hypoxia were often higher than those in nearby <span class="hlt">zones</span> with oxic water columns. Corresponding atomic C/S ratios were typically lower in <span class="hlt">sediments</span> from sites in the <span class="hlt">zone</span> of hypoxia compared to nearby</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021493','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021493"><span>Localized sulfate-reducing <span class="hlt">zones</span> in a coastal plain aquifer</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Brown, C.J.; Coates, J.D.; Schoonen, M.A.A.</p> <p>1999-01-01</p> <p>High concentrations of dissolved iron in ground water of coastal plain or alluvial aquifers contribute to the biofouling of public supply wells for which treatment and remediation is costly. Many of these aquifers, however, contain <span class="hlt">zones</span> in which microbial sulfate reduction and the associated precipitation of iron-sulfide minerals decreases iron mobility. The principal water-bearing aquifer (Magothy Aquifer of Cretaceous age) in Suffolk County, New York, contains localized sulfate-reducing <span class="hlt">zones</span> in and near lignite deposits, which generally are associated with clay lenses. Microbial analyses of core samples amended with [14C]-acetate indicate that microbial sulfate reduction is the predominant terminal-electron-accepting process (TEAP) in poorly permeable, lignite-rich <span class="hlt">sediments</span> at shallow depths and near the ground water divide. The sulfate-reducing <span class="hlt">zones</span> are characterized by abundant lignite and iron-sulfide minerals, low concentrations of Fe(III) oxyhydroxides, and by proximity to clay lenses that contain pore water with relatively high concentrations of sulfate and dissolved organic carbon. The low permeability of these <span class="hlt">zones</span> and, hence, the long residence time of ground water within them, permit the preservation and (or) allow the formation of iron-sulfide minerals, including pyrite and marcasite. Both sulfate-reducing bacteria (SRB) and iron-reducing bacteria (IRB) are present beneath and beyond the shallow sulfate-reducing <span class="hlt">zones</span>. A unique Fe(III)-reducing organism, MD-612, was found in core <span class="hlt">sediments</span> from a depth of 187 m near the southern shore of Long Island. The distribution of poorly permeable, lignite-rich, sulfate-reducing <span class="hlt">zones</span> with decreased iron concentration is varied within the principal aquifer and accounts for the observed distribution of dissolved sulfate, iron, and iron sulfides in the aquifer. Locating such <span class="hlt">zones</span> for the placement of production wells would be difficult, however, because these <span class="hlt">zones</span> are of limited aerial extent.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.B33B0399L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.B33B0399L"><span>Beach-dune dynamics: Spatio-temporal patterns of aeolian <span class="hlt">sediment</span> transport under complex offshore airflow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lynch, K.; Jackson, D.; Delgado-Fernandez, I.; Cooper, J. A.; Baas, A. C.; Beyers, M.</p> <p>2010-12-01</p> <p>This study examines sand transport and wind speed across a beach at Magilligan Strand, Northern Ireland, under offshore wind conditions. Traditionally the offshore component of local wind regimes has been ignored when quantifying beach-dune <span class="hlt">sediment</span> budgets, with the sheltering effect of the foredune assumed to prohibit grain entrainment on the adjoining beach. Recent investigations of secondary airflow patterns over coastal dunes have suggested this may not be the case, that the turbulent nature of the airflow in these <span class="hlt">zones</span> enhances <span class="hlt">sediment</span> transport potential. Beach <span class="hlt">sediment</span> may be delivered to the dune toe by re-circulating eddies under offshore winds in coastal areas, which may explain much of the dynamics of aeolian dunes on coasts where the dominant wind direction is offshore. The present study investigated aeolian <span class="hlt">sediment</span> transport patterns under an offshore wind event. Empirical data were collected using load cell traps, for aeolian <span class="hlt">sediment</span> transport, co-located with 3-D ultrasonic anemometers. The instrument positioning on the sub-aerial beach was informed by prior analysis of the airflow patterns using computational fluid dynamics. The array covered a total beach area of 90 m alongshore by 65 m cross-shore from the dune crest. Results confirm that <span class="hlt">sediment</span> transport occurred in the ‘sheltered’ area under offshore winds. Over short time and space scales the nature of the transport is highly complex; however, preferential <span class="hlt">zones</span> for sand entrainment may be identified. Alongshore spatial heterogeneity of <span class="hlt">sediment</span> transport seems to show a relationship to undulations in the dune crest, while temporal and spatial variations may also be related to the position of the airflow reattachment <span class="hlt">zone</span>. These results highlight the important feedbacks between flow characteristics and transport in a complex three dimensional surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/bul/b2214/+','USGSPUBS'); return false;" href="https://pubs.usgs.gov/bul/b2214/+"><span>Elastic properties of overpressured and unconsolidated <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lee, Myung W.</p> <p>2003-01-01</p> <p>Differential pressure affects elastic velocities and Poisson?s ratio of <span class="hlt">sediments</span> in such a way that velocities increase as differential pressure increases. Overpressured <span class="hlt">zones</span> in <span class="hlt">sediments</span> can be detected by observing an increase in Poisson?s ratio with a corresponding drop in elastic velocities. In highly overpressured sands, such as shallow water flow sands, the P-to S-wave velocity ratio (Vp/Vs) is very high, on the order of 10 or higher, due to the unconsolidated and uncemented nature of <span class="hlt">sediments</span>. In order to predict elastic characteristics of highly overpressured sands, Biot-Gassmann theory by Lee (BGTL) is used with a variable exponent n that depends on differential pressure and the degree of consolidation/compaction. The exponent n decreases as differential pressure and the degree of consolidation increases, and, as n decreases, velocity increases and Vp/Vs decreases. The predicted velocity ratio by BGTL agrees well with the measured velocity ratio at low differential pressure for unconsolidated <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC23D1266M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC23D1266M"><span>Modern <span class="hlt">Sedimentation</span> along the SE Bangladesh Coast Reveal Surprisingly Low Accumulation Rates</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McHugh, C.; Mustaque, S.; Mondal, D. R.; Akhter, S. H.; Iqbal, M.</p> <p>2016-12-01</p> <p>Recent <span class="hlt">sediments</span> <span class="hlt">recovered</span> along the SE coast of Bangladesh, from Teknaf to Cox's Bazar and drainage basin analyses reveal <span class="hlt">sediment</span> sources and very low <span class="hlt">sedimentation</span> rates of 1mm/year. These low rates are surprisingly low given that this coast is adjacent to the Ganges-Brahmaputra Delta with a yearly discharge of 1GT. The Teknaf anticline (elevation 200 m), part of the western Burma fold-thrust belt dominates the topography extending across and along the Teknaf peninsula. It is thought to have begun evolving since the Miocene (Alam et al. 2003 & Allen et al. 2008). Presently the anticline foothills on the west are flanked by uplifted terraces, the youngest linked to coseismic displacement during the 1762 earthquake (Mondal et al. 2015), and a narrow beach 60-200 m in width. Petrography, semi-quantitative bulk mineralogy and SEM/EDX analyses were conducted on <span class="hlt">sediments</span> <span class="hlt">recovered</span> along the west coast from 1-4 m deep trenches and three 4-8 m deep drill holes. GIS mapping of drainage basins and quartz-feldspar-lithic (QFL) ternary plots based on grain counting show mixing of <span class="hlt">sediments</span> from multiple sources: Himalayan provenance of metamorphic and igneous origin (garnet-mostly almandine, tourmaline, rutile, kyanite, zircon, sillimanite and clinopyroxene) similar to Uddin et al. (2007); Brahmaputra provenance of igneous and metamorphic origin (amphibole, epidote, plagioclase 40% Na and 60% Ca, apatite, ilmenite, magnetite, Cr-spinel and garnet-mostly grossular,) as indicated by Garzanti et al. (2010) & Rahman et al. (2016) and Burmese sources (cassiterite and wolframite) (Zaw 1990 & Searle et al. 2007). Low <span class="hlt">sedimentation</span> rates are the result of two main factors: 1. Strong longshore currents from the south-east that interact with high tidal ranges as evidenced by the morphology of sand waves and ridge and runnel landforms along the beach. 2. Streams draining the Teknaf anticline are dry during the winter and during summer monsoon rains, the <span class="hlt">sediments</span> bypass the narrow</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26538260','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26538260"><span>Vertical profile, source apportionment, and toxicity of PAHs in <span class="hlt">sediment</span> cores of a wharf near the coal-based steel refining industrial <span class="hlt">zone</span> in Kaohsiung, Taiwan.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Chih-Feng; Chen, Chiu-Wen; Ju, Yun-Ru; Dong, Cheng-Di</p> <p>2016-03-01</p> <p>Three <span class="hlt">sediment</span> cores were collected from a wharf near a coal-based steel refining industrial <span class="hlt">zone</span> in Kaohsiung, Taiwan. Analyses for 16 polycyclic aromatic hydrocarbons (PAHs) of the US Environmental Protection Agency priority list in the core <span class="hlt">sediment</span> samples were conducted using gas chromatography-mass spectrometry. The vertical profiles of PAHs in the core <span class="hlt">sediments</span> were assessed, possible sources and apportionment were identified, and the toxicity risk of the core <span class="hlt">sediments</span> was determined. The results from the <span class="hlt">sediment</span> analyses showed that total concentrations of the 16 PAHs varied from 11774 ± 4244 to 16755 ± 4593 ng/g dry weight (dw). Generally, the vertical profiles of the PAHs in the <span class="hlt">sediment</span> cores exhibited a decreasing trend from the top to the lower levels of the S1 core and an increasing trend of PAHs from the top to the lower levels of the S2 and S3 cores. Among the core <span class="hlt">sediment</span> samples, the five- and six-ring PAHs were predominantly in the S1 core, ranging from 42 to 54 %, whereas the composition of the PAHs in the S2 and S3 cores were distributed equally across three groups: two- and three-ring, four-ring, and five- and six-ring PAHs. The results indicated that PAH contamination at the site of the S1 core had a different source. The molecular indices and principal component analyses with multivariate linear regression were used to determine the source contributions, with the results showing that the contributions of coal, oil-related, and vehicle sources were 38.6, 35.9, and 25.5 %, respectively. A PAH toxicity assessment using the mean effect range-median quotient (m-ERM-q, 0.59-0.79), benzo[a]pyrene toxicity equivalent (TEQ(carc), 1466-1954 ng TEQ/g dw), and dioxin toxicity equivalent (TEQ(fish), 3036-4174 pg TEQ/g dw) identified the wharf as the most affected area. The results can be used for regular monitoring, and future pollution prevention and management should target the coal-based industries in this region for pollution reduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016DSRII.125..107L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016DSRII.125..107L"><span>Paleomagnetic field variability and chronostratigraphy of Brunhes-Chron deep-sea <span class="hlt">sediments</span> from the Bering Sea: IODP Expedition 323</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lund, Steve; Stoner, Joseph; Okada, Makoto; Mortazavi, Emily</p> <p>2016-03-01</p> <p>IODP Expedition 323 <span class="hlt">recovered</span> six complete and replicate records of Brunhes-Chron paleomagnetic field variability (0-780,000 years BP) in 2820 m core depth below sea floor (CSF) of deep-sea <span class="hlt">sediments</span>. On shipboard, we made more than 220,000 paleomagnetic measurements on the <span class="hlt">recovered</span> <span class="hlt">sediments</span>. Since then, we have u-channel sampled more than 300 m of Brunhes Chron <span class="hlt">sediments</span> to corroborate our shipboard measurements and improve our paleomagnetic and rock magnetic understanding of these <span class="hlt">sediments</span>. Several intervals of distinctive paleomagnetic secular variation (PSV) have been identified that appear to be correlatable among sites 1343, 1344, and 1345. One magnetic field excursion is recorded in <span class="hlt">sediments</span> of sites 1339, 1343, 1344, and 1345. We identify this to be excursion 7α/Iceland Basin Event (192,000 years BP), which is also seen in the high-latitude North Atlantic Ocean (Channell et al., 1997). We have verified in u-channels the placement of the Brunhes/Matuyama boundary (780,000 years BP) at sites 1341 and 1343. Finally, we have developed a medium-quality relative paleointensity record for these <span class="hlt">sediments</span> that is correlatable among the sites, even though it is still biased by large-amplitude environmental variability. On the basis of these observations we have built a magnetic chronostratigraphy of Expedition 323 <span class="hlt">sediments</span> suitable for regional correlation and dating over the last 1 million years, and compared this with oxygen-isotope chronostratigraphy from sites U1339 and U1345.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H42G..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H42G..07S"><span>Hydrologically Controlled Arsenic Release in Deltaic Wetlands and Coastal Riparian <span class="hlt">Zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stuckey, J.; LeMonte, J. J.; Yu, X.; Schaefer, M.; Kocar, B. D.; Benner, S. G.; Rinklebe, J.; Tappero, R.; Michael, H. A.; Fendorf, S. E.; Sparks, D. L.</p> <p>2016-12-01</p> <p>Wetland and riparian <span class="hlt">zone</span> hydrology exerts critical controls on the biogeochemical cycling of metal contaminants including arsenic. The role of wetlands in driving geogenic arsenic release to groundwater has been debated in the deltas of South and Southeast Asia where the largest impacted human population resides. In addition, groundwater in coastal areas worldwide, such as those in South and Southeast Asia and the Mid-Atlantic of the U.S., is at risk to largely unexplored biogeochemical and hydrologic impacts of projected sea level rise. First, we present data from fresh-<span class="hlt">sediment</span> incubations, in situ model <span class="hlt">sediment</span> incubations and a controlled field experiment with manipulated wetland hydrology and organic carbon inputs in the minimally disturbed upper Mekong Delta. Here we show that arsenic release is limited to near-surface <span class="hlt">sediments</span> of permanently saturated wetlands where both organic carbon and arsenic-bearing solids are sufficiently reactive for microbial oxidation of organic carbon and reduction of arsenic-bearing iron oxides. In contrast, within the deeper aquifer or seasonally saturated <span class="hlt">sediments</span>, reductive dissolution of iron oxides is observed only when either more reactive exogenous forms of iron oxides or organic carbon are added, revealing a potential thermodynamic restriction to microbial metabolism. Second, in order to assess the potential impacts of sea level rise on arsenic release to groundwater, we determined the changes in arsenic speciation and partitioning in <span class="hlt">sediment</span> collected from an anthropogenically contaminated coastal riparian <span class="hlt">zone</span> under controlled Eh regimes in both seawater and freshwater systems. Here we show greater arsenic release under anoxic/suboxic conditions in the freshwater system than in the seawater system, potentially due to high salinity induced microbial inhibition. Collectively, our work shows that shifting hydrologic conditions in deltaic wetlands and tidally influenced <span class="hlt">zones</span> impacts the extent of arsenic release to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21367375-hydrodynamic-motions-dead-zones','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21367375-hydrodynamic-motions-dead-zones"><span>ON HYDRODYNAMIC MOTIONS IN DEAD <span class="hlt">ZONES</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Oishi, Jeffrey S.; Mac Low, Mordecai-Mark, E-mail: jsoishi@astro.berkeley.ed, E-mail: mordecai@amnh.or</p> <p></p> <p>We investigate fluid motions near the midplane of vertically stratified accretion disks with highly resistive midplanes. In such disks, the magnetorotational instability drives turbulence in thin layers surrounding a resistive, stable dead <span class="hlt">zone</span>. The turbulent layers in turn drive motions in the dead <span class="hlt">zone</span>. We examine the properties of these motions using three-dimensional, stratified, local, shearing-box, non-ideal, magnetohydrodynamical simulations. Although the turbulence in the active <span class="hlt">zones</span> provides a source of vorticity to the midplane, no evidence for coherent vortices is found in our simulations. It appears that this is because of strong vertical oscillations in the dead <span class="hlt">zone</span>. By analyzingmore » time series of azimuthally averaged flow quantities, we identify an axisymmetric wave mode particular to models with dead <span class="hlt">zones</span>. This mode is reduced in amplitude, but not suppressed entirely, by changing the equation of state from isothermal to ideal. These waves are too low frequency to affect <span class="hlt">sedimentation</span> of dust to the midplane, but may have significance for the gravitational stability of the resulting midplane dust layers.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRB..112.7404H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRB..112.7404H"><span>Nondestructive continuous physical property measurements of core samples <span class="hlt">recovered</span> from hole B, Taiwan Chelungpu-Fault Drilling Project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hirono, Tetsuro; Yeh, En-Chao; Lin, Weiren; Sone, Hiroki; Mishima, Toshiaki; Soh, Wonn; Hashimoto, Yoshitaka; Matsubayashi, Osamu; Aoike, Kan; Ito, Hisao; Kinoshita, Masataka; Murayama, Masafumi; Song, Sheng-Rong; Ma, Kuo-Fong; Hung, Jih-Hao; Wang, Chien-Ying; Tsai, Yi-Ben; Kondo, Tomomi; Nishimura, Masahiro; Moriya, Soichi; Tanaka, Tomoyuki; Fujiki, Toru; Maeda, Lena; Muraki, Hiroaki; Kuramoto, Toshikatsu; Sugiyama, Kazuhiro; Sugawara, Toshikatsu</p> <p>2007-07-01</p> <p>The Taiwan Chelungpu-Fault Drilling Project was undertaken in 2002 to investigate the faulting mechanism of the 1999 Mw 7.6 Taiwan Chi-Chi earthquake. Hole B penetrated the Chelungpu fault, and core samples were <span class="hlt">recovered</span> from between 948.42- and 1352.60-m depth. Three major <span class="hlt">zones</span>, designated FZB1136 (fault <span class="hlt">zone</span> at 1136-m depth in hole B), FZB1194, and FZB1243, were recognized in the core samples as active fault <span class="hlt">zones</span> within the Chelungpu fault. Nondestructive continuous physical property measurements, conducted on all core samples, revealed that the three major fault <span class="hlt">zones</span> were characterized by low gamma ray attenuation (GRA) densities and high magnetic susceptibilities. Extensive fracturing and cracks within the fault <span class="hlt">zones</span> and/or loss of atoms with high atomic number, but not a measurement artifact, might have caused the low GRA densities, whereas the high magnetic susceptibility values might have resulted from the formation of magnetic minerals from paramagnetic minerals by frictional heating. Minor fault <span class="hlt">zones</span> were characterized by low GRA densities and no change in magnetic susceptibility, and the latter may indicate that these minor <span class="hlt">zones</span> experienced relatively low frictional heating. Magnetic susceptibility in a fault <span class="hlt">zone</span> may be key to the determination that frictional heating occurred during an earthquake on the fault.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28797670','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28797670"><span>The role of alluvial aquifer <span class="hlt">sediments</span> in attenuating a dissolved arsenic plume.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ziegler, Brady A; Schreiber, Madeline E; Cozzarelli, Isabelle M</p> <p>2017-09-01</p> <p>In a crude-oil-contaminated sandy aquifer at the Bemidji site in northern Minnesota, biodegradation of petroleum hydrocarbons has resulted in release of naturally occurring As to groundwater under Fe-reducing conditions. This study used chemical extractions of aquifer <span class="hlt">sediments</span> collected in 1993 and 2011-2014 to evaluate the relationship between Fe and As in different redox <span class="hlt">zones</span> (oxic, methanogenic, Fe-reducing, anoxic-suboxic transition) of the contaminated aquifer over a twenty-year period. Results show that 1) the aquifer has the capacity to naturally attenuate the plume of dissolved As, primarily through sorption; 2) Fe and As are linearly correlated in <span class="hlt">sediment</span> across all redox <span class="hlt">zones</span>, and a regression analysis between Fe and As reasonably predicted As concentrations in <span class="hlt">sediment</span> from 1993 using only Fe concentrations; 3) an As-rich "iron curtain," associated with the anoxic-suboxic transition <span class="hlt">zone</span>, migrated 30m downgradient between 1993 and 2013 as a result of the hydrocarbon plume evolution; and 4) silt lenses in the aquifer preferentially sequester dissolved As, though As is remobilized into groundwater from <span class="hlt">sediment</span> after reducing conditions are established. Using results of this study coupled with historical data, we develop a conceptual model which summarizes the natural attenuation of As and Fe over time and space that can be applied to other sites that experience As mobilization due to an influx of bioavailable organic matter. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190585','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190585"><span>The role of alluvial aquifer <span class="hlt">sediments</span> in attenuating a dissolved arsenic plume</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ziegler, Brady A.; Schreiber, Madeline E.; Cozzarelli, Isabelle M.</p> <p>2017-01-01</p> <p>In a crude-oil-contaminated sandy aquifer at the Bemidji site in northern Minnesota, biodegradation of petroleum hydrocarbons has resulted in release of naturally occurring As to groundwater under Fe-reducing conditions. This study used chemical extractions of aquifer <span class="hlt">sediments</span> collected in 1993 and 2011–2014 to evaluate the relationship between Fe and As in different redox <span class="hlt">zones</span> (oxic, methanogenic, Fe-reducing, anoxic-suboxic transition) of the contaminated aquifer over a twenty-year period. Results show that 1) the aquifer has the capacity to naturally attenuate the plume of dissolved As, primarily through sorption; 2) Fe and As are linearly correlated in <span class="hlt">sediment</span> across all redox <span class="hlt">zones</span>, and a regression analysis between Fe and As reasonably predicted As concentrations in <span class="hlt">sediment</span> from 1993 using only Fe concentrations; 3) an As-rich “iron curtain,” associated with the anoxic-suboxic transition <span class="hlt">zone</span>, migrated 30 m downgradient between 1993 and 2013 as a result of the hydrocarbon plume evolution; and 4) silt lenses in the aquifer preferentially sequester dissolved As, though As is remobilized into groundwater from <span class="hlt">sediment</span> after reducing conditions are established. Using results of this study coupled with historical data, we develop a conceptual model which summarizes the natural attenuation of As and Fe over time and space that can be applied to other sites that experience As mobilization due to an influx of bioavailable organic matter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089459&hterms=gravitropism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dgravitropism','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089459&hterms=gravitropism&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DTitle%26N%3D0%26No%3D50%26Ntt%3Dgravitropism"><span>Caulonemal gravitropism and amyloplast <span class="hlt">sedimentation</span> in the moss Funaria</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Schwuchow, J. M.; Kim, D.; Sack, F. D.</p> <p>1995-01-01</p> <p>Caulonemata of the moss Funaria were examined to determine whether they are gravitropic. Funaria and Physcomitrella were also evaluated to compare amyloplast <span class="hlt">sedimentation</span> with that of Ceratodon. Protonemata were either chemically fixed in place or examined alive using infrared timelapse videomicroscopy. Funaria caulonemata were found to be negatively gravitropic, i.e., they grew upwards in the dark. Upward curvature reversed temporarily before cytokinesis in Funaria, a phenomenon already known for Ceratodon and Physcomitrella. Most horizontal and upward-curving Funaria tip cells contained a broad subapical <span class="hlt">zone</span> where plastid <span class="hlt">sedimentation</span> occurred. In dark-grown Physcomitrella caulonemata, <span class="hlt">sedimentation</span> was detected by the presence of a thin, amyloplast-free strip of cytoplasm at the top of the cell. These results suggest that gravitropism and subapical amyloplast <span class="hlt">sedimentation</span> may be relatively common in moss caulonemata.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.6323F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.6323F"><span>Predicting Martian dune shape and orientation from wind directional variability and <span class="hlt">sediment</span> availability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernandez-Cascales, Laura; Lucas, Antoine; Rodriguez, Sébastien; Narteau, Clément; Spiga, Aymeric; Allemand, Pascal</p> <p>2016-04-01</p> <p>Dunes provide a unique set of information to constrain local climatic regimes on planetary bodies where there is no direct meteorological data. Wind directional variability and <span class="hlt">sediment</span> availability are known to control the dune growth mechanism (i.e. the bed instability or fingering modes) and the subsequent dune shape and orientation (Courrech du Pont at al., 2014; Gao et al., 2015). Here we provide a quantitative analysis of these dependences on Mars using the output of the Martian General Circulation Models (GCM) and satellite imagery such as the Mars Reconnaissance Orbiter (MRO) Context Camera (CTX) images, at a selection of places where there is a high contrast between the dune material and the non-erodible ground. Dunes, mostly composed of unweathered basaltic and andesitic grains, appear dark, whereas the non-erodible ground has a higher albedo. Such a systematic contrast permits to link dune morphology to the local <span class="hlt">sediment</span> cover. Dune shape, crest orientation and local <span class="hlt">sediment</span> cover are extracted from CTX images using an automatic linear segment detection method and the local distribution in albedo. In <span class="hlt">zones</span> of high <span class="hlt">sediment</span> supply, dune crest alignments are close to the orientation of the bed instability mode predicted from the local winds from the Martian Climate Database (MCD) where is stored the outputs of the IPSL-GCM for Mars (Millour et al., 2014). Using the same wind data, in <span class="hlt">zones</span> of low <span class="hlt">sediment</span> supply, the crest angle is close to the orientation of the fingering mode. In addition, there are continuous transitions in dune shape and orientation as the dunes migrate from <span class="hlt">zone</span> of high to low <span class="hlt">sediment</span> availability. These results indicate that the prediction of the IPSL-GCM are in good agreement with the present dune shapes and orientations and shed new light on the dynamics of complex dune fields along sand flow path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27427199','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27427199"><span>Composition and temporal stability of turf <span class="hlt">sediments</span> on inner-shelf coral reefs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gordon, Sophie E; Goatley, Christopher H R; Bellwood, David R</p> <p>2016-10-15</p> <p>Elevated <span class="hlt">sediment</span> loads within the epilithic algal matrix (EAM) of coral reefs can increase coral mortality and inhibit herbivory. Yet the composition, distribution and temporal variability of EAM <span class="hlt">sediment</span> loads are poorly known, especially on inshore reefs. This study quantified EAM <span class="hlt">sediment</span> loads (including organic particulates) and algal length across the reef profile of two bays at Orpheus Island (inner-shelf Great Barrier Reef) over a six month period. We examined the total <span class="hlt">sediment</span> mass, organic load, carbonate and silicate content, and the particle sizes of EAM <span class="hlt">sediments</span>. Throughout the study period, all EAM <span class="hlt">sediment</span> variables exhibited marked variation among reef <span class="hlt">zones</span>. However, EAM <span class="hlt">sediment</span> loads and algal length were consistent between bays and over time, despite major seasonal variation in climate including a severe tropical cyclone. This study provides a comprehensive description of EAM <span class="hlt">sediments</span> on inshore reefs and highlights the exceptional temporal stability of EAM <span class="hlt">sediments</span> on coral reefs. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMEP23E..01S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMEP23E..01S"><span>Watershed <span class="hlt">sediment</span> source fingerprinting: a view under the hood</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, H.</p> <p>2015-12-01</p> <p><span class="hlt">Sediment</span> source fingerprinting procedures involve the discrimination of <span class="hlt">sediment</span> sources based on physical and chemical properties and estimation of the contributions from those sources to mixtures of fine-grained <span class="hlt">sediment</span> transported within watersheds. Sources of <span class="hlt">sediment</span> widely considered include agricultural land uses, channel banks and geological <span class="hlt">zones</span>. There has been a tendency in the literature for <span class="hlt">sediment</span> fingerprinting to be presented as a technique that can deliver accurate and precise information on source contributions to <span class="hlt">sediment</span> across a range of environments. However, recent research indicates that such a view of <span class="hlt">sediment</span> fingerprinting cannot presently be supported. Furthermore, many past papers lack transparency in data processing and presentation that prevents the critical assessment of results and hinders wider uptake of the technique. Therefore, this contribution aims to delve 'under the hood' of <span class="hlt">sediment</span> fingerprinting to promote further discussion and debate over future research needs and method limitations. It draws on important developments from the last two years concerning the effect of (i) tracer selection, (ii) tracer behaviour during transport, (iii) corrections to tracer datasets and (iv) the choice of mixing model on predictions of <span class="hlt">sediment</span> source contributions. <span class="hlt">Sediment</span> fingerprinting has the potential to make a very significant contribution to the measurement of contemporary <span class="hlt">sediment</span> sources in watersheds, but cannot be viewed as an 'off-the-shelf' technique for widespread application until important challenges have been addressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004SedG..163..165L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004SedG..163..165L"><span>Eogenetic siderite as an indicator for fluctuations in <span class="hlt">sedimentation</span> rate in the Oligocene Boom Clay Formation (Belgium)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laenen, B.; De Craen, M.</p> <p>2004-01-01</p> <p>Horizons with septarian concretions are a salient feature of the marine Boom Clay Formation. At most horizons, the concretions consist of ferroan calcite with variable amounts of pyrite, but at stratigraphic level S60 they also contain siderite. S60 is situated at the centre of an intensely bioturbated <span class="hlt">zone</span> that is underlain by a pyrite-rich layer. Furthermore, the enclosing clay is strongly enriched in iron, manganese and phosphorous. The sedimentological and chemical <span class="hlt">zoning</span> is indicative for low <span class="hlt">sedimentation</span> rates, which allowed the concentration of iron in the aerobic <span class="hlt">zone</span> of the <span class="hlt">sediment</span>. Concentration of iron was the prerequisite for the formation of the siderite-containing concretions. The co-precipitation with pyrite is an argument for a formation in the sulphate reduction <span class="hlt">zone</span>, and is indicative for a high rate of iron-reduction. The latter was due to the rapid burial of the iron-enriched layer below the redox boundary. The abrupt fluctuations in <span class="hlt">sedimentation</span> rate were a response to the maximum flooding event of the second Rupelian third-order relative sea-level cycle, which caused a brief pushback of the detrital <span class="hlt">sediment</span> wedge to its source areas. As this response is logically explained by the general sequence stratigraphic model [Spec. Publ.-Soc. Econ. Paleontol. Mineral. 42 (1988) 109], early diagenetic siderite may be widespread at maximum flooding surfaces in rapidly prograding marine mudstones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.2699K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.2699K"><span>Subduction, erosion and the <span class="hlt">sediment</span> record: Insights from Miocene <span class="hlt">sediments</span>, Hengchun Peninsula, Taiwan</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kirstein, Linda; Carter, Andrew; Chen, Yue-Gau</p> <p>2010-05-01</p> <p>Detrital sedimentary records include vast archives of material that have been removed from developing tectonically active regions. These archives have been used to investigate challenging questions on continental deformation, exhumation and palaeodrainage using a variety of different techniques including heavy minerals, fission-track dating and palaeocurrent reconstructions. The Hengchun Peninsula of southern Taiwan and offshore Hengchun Ridge form a present day accretionary prism, with accretionary wedge growth occurring both by frontal accretion, with <span class="hlt">sediments</span> from the continental margin scraped up into the accretionary wedge and by underplating. Miocene <span class="hlt">sediments</span> in Hengchun include foreland basin deposits, deep marine turbidites and forearc basin deposits. As a result the detrital <span class="hlt">sediments</span> record details of accretionary prism growth associated with continued Luzon arc-continent collision. Diametrically opposite palaeocurrents are preserved in the Miocene sandstones of the Hengchun Peninsula, southern Taiwan. Controversial explanations include an exotic source terrane to the south and/or 180 ° rotation of a depositional basin. We document the tecto-thermal evolution of the Miocene <span class="hlt">sediment</span> source(s) using a double dating approach. U-Pb grain ages range from Miocene to Archaean, while zircon fission-tracks record thermal cooling primarily in the Cretaceous with minor peaks in the Miocene, Triassic, Jurassic and Permian. The primary source of the Miocene <span class="hlt">sediments</span> at the centre of the controversy was similar. Palaeocurrent data are influenced by local basin geometry and submarine topography and suggest that <span class="hlt">sediment</span> deposition in the Miocene was strongly controlled by incipient subduction, associated structural trends and submarine topography. A similar control on deposition in the modern Taiwan collision <span class="hlt">zone</span> is apparent in the offshore region today.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911762G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911762G"><span>Effects of fluidization of the host <span class="hlt">sediment</span> on peperite textures: A field example from the Cretaceous Buan Volcanics, SW Korea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gihm, Yong Sik; Kwon, Chang Woo</p> <p>2017-04-01</p> <p>In the Cretaceous Buan Volcanics (SW Korea), blocky and fluidal peperites are hosted in a massive pumiceous lapilli tuff intruded by intermediate dikes. Blocky peperites, the most abundant species, are characterized by polyhedral or platy juvenile clasts and a jigsaw-crack texture. Fluidal peperites occur only along dike margins, where the host <span class="hlt">sediments</span> are composed of well sorted, fine to very fine ash (fine-grained <span class="hlt">zone</span>), and are characterized by fluidal or globular juvenile clasts with irregular or ragged margins. The fine-grained <span class="hlt">zone</span> is interpreted to form by grain size segregation caused by upward moving pore water (fluidization) that has resulted from heat transfer from intruding magma toward waterlogged host <span class="hlt">sediments</span> during intrusion. With the release of pore water and the selective entrainment of fine-grained ash, fine-grained <span class="hlt">zones</span> formed within the host <span class="hlt">sediments</span>. Subsequent interactions between the fine-grained <span class="hlt">zone</span> and the intruding magma resulted in ductile deformation of the magma before fragmentation, which generated fluidal peperites. Outside the fine-grained <span class="hlt">zone</span>, intruding magma fragmented in a brittle manner because of the relative deficiency of both pore water and fine-grained ash, resulting in the formation of blocky peperites. The results of this study suggest that redistribution of constituent particles (ash) and interstitial fluids during fluidization resulted in heterogeneous physical conditions of the host <span class="hlt">sediments</span>, which influenced peperite-forming processes, as reflected by the different peperite textures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/191303-recent-advances-use-estuarine-meiobenthos-assess-contaminated-sediment-effects-multi-species-whole-sediment-microcosms','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/191303-recent-advances-use-estuarine-meiobenthos-assess-contaminated-sediment-effects-multi-species-whole-sediment-microcosms"><span>Recent advances in the use of estuarine meiobenthos to assess contaminated <span class="hlt">sediment</span> effects in multi-species whole <span class="hlt">sediment</span> microcosms</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Chandler, G.T.; Coull, B.C.; Schizas, N.V.</p> <p>1995-12-31</p> <p>Many marine meiobenthic taxa (i.e. invertebrates passing a 1-mm sieve but retaining on a 0.063 mm sieve) are ideal for ``whole-<span class="hlt">sediment</span>`` and porewater bioassay of <span class="hlt">sedimented</span> pollutants. Annual production of meiobenthos is 5--10 times that of the more commonly studied macrobenthos, and > 95% of all meiobenthos live in the oxic <span class="hlt">zone</span> of muddy <span class="hlt">sediments</span> at densities of 4--12 million per M{sup 2}. Most spend their entire lifecycles, burrowing freely and feeding on/within the <span class="hlt">sediment</span>:porewater matrix, many taxa undergo 10--14 generations per year, most larval/juvenile stages are benthic, and many have easily quantifiable reproductive output. Furthermore, many meiobenthic taxa canmore » be cultured indefinitely over multiple life-cycles within simple <span class="hlt">sediment</span> microcosms consisting of sealed whole-<span class="hlt">sediment</span> cores collected intact from intertidal mudflats. The authors describe several recent technical developments exploiting meiofaunal <span class="hlt">sediment</span> culture for rapid contaminated <span class="hlt">sediment</span> bioassays of toxicant effects on survival, reproduction and population growth of meiobenthic taxa in whole-<span class="hlt">sediment</span> microcosms. Currently meiobenthic copepods, nematodes, foraminifers and polychaetes are being continuously cultured to study these parameters under exposure to model <span class="hlt">sediment</span>-associated toxicants (e.g. cadmium). Bioassays are run for 21-d under flowing seawater. With this approach, fertile benthic copepods (e.g. Amphiascus tenuiremis) can be added to core microcosms to assess survival and growth of a fixed population cohort. All other meiobenthic taxa are enumerated relative to controls and evaluated for toxicant effects on higher order community-level endpoints. This approach exploits meiobenthos` high abundance and rapid reproductive rates to yield on a micro scale better endpoints than much larger <span class="hlt">sediment</span> mesocosms targeted at macrofaunal endpoints.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B13G0725C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B13G0725C"><span>Methane-related metabolisms of deep-sea <span class="hlt">sediments</span> captured with a colonization experiment.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carr, S. A.; Wheat, C. G.; Orcutt, B.; Kopf, A.; Saffer, D. M.; Toczko, S.</p> <p>2016-12-01</p> <p>NanTroSEIZE is a multi-expedition project of the International Ocean Discovery Program (IODP) designed to investigate the Nankai Trough subduction <span class="hlt">zone</span>. In 2016, a long-term borehole instrument package known as the "GeniusPlug" was collected from Hole C0010A after a six-year deployment within the <span class="hlt">sediment</span> of a major fault <span class="hlt">zone</span>, at a depth of 400 mbsf. This GeniusPlug included a set of osmotically-driven pumps, which continuously pumped in situ deep seated, formation water through a microbiological colonization experiment (flow-through osmo colonization system (FLOCS)). This FLOCS experiment contained cassettes of olivine, barite, and <span class="hlt">sediment</span> collected from nearby Hole C0004D, to serve as colonization substrates. While similar FLOCS have been deployed within boreholes in the igneous oceanic crust, this FLOCS experiment represents the first to be deployed within a sedimentary environment, and thus represents the first opportunity to observe how pore water communities colonize <span class="hlt">sediment</span> and rock substrates. Initial geochemistry results suggest that conditions within the FLOCS experiment were similar to a methane-sulfate transition <span class="hlt">zone</span>, and initial enrichment cultures inoculated with the FLOCS substrates demonstrate methane production. Here, we will present integrated results of culturing experiments and culture-independent genomic investigations as a means to elucidate the methane-related metabolisms of these colonizing communities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..190..161B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..190..161B"><span>Geochemical provenance of <span class="hlt">sediments</span> from the northern East China Sea document a gradual migration of the Asian Monsoon belt over the past 400,000 years</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Beny, François; Toucanne, Samuel; Skonieczny, Charlotte; Bayon, Germain; Ziegler, Martin</p> <p>2018-06-01</p> <p>The reconstruction of the long-term evolution of the East Asian Monsoon remains controversial. In this study, we aim to give a new outlook on this evolution by studying a 400 kyr long <span class="hlt">sediment</span> record (U1429) from the northern East China Sea <span class="hlt">recovered</span> during IODP Expedition 346. Neodymium isotopic ratios and rare earth element concentrations of different grain-size fractions reveal significant provenance changes of the <span class="hlt">sediments</span> in the East China Sea between East Asian continental sources (mainly Yellow River) and <span class="hlt">sediment</span> contributions from the Japanese Archipelago. These provenance changes are interpreted as the direct impact of sea level changes, due to the reorganization of East Asian river mouth locations and ocean circulation on the East China Sea shelf, and latitudinal shifts of the intertropical convergence <span class="hlt">zone</span> (ITCZ) from the interior of Asia to the western North Pacific Ocean. Our data reveal the dominance of winter and summer monsoons during glacial and interglacial periods, respectively, except for glacial MIS 6d (∼150-180 ka) during which unexpected summer monsoon dominated conditions prevailed. Finally, our data suggests a possible strengthening of the interglacial summer monsoon rainfalls over the East Asian continent and Japan throughout the past 400 kyr, and between MIS 11 and MIS 5 in particular. This could result from a gradual northward migration of the ITCZ.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ECSS..130..179B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ECSS..130..179B"><span>Integrated quality assessment of <span class="hlt">sediments</span> from harbour areas in Santos-São Vicente Estuarine System, Southern Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buruaem, Lucas Moreira; de Castro, Ítalo Braga; Hortellani, Marcos Antonio; Taniguchi, Satie; Fillmann, Gilberto; Sasaki, Silvio Tarou; Varella Petti, Mônica Angélica; Sarkis, Jorge Eduardo de Souza; Bícego, Márcia Caruso; Maranho, Luciane Alves; Davanso, Marcela Bergo; Nonato, Edmundo Ferraz; Cesar, Augusto; Costa-Lotufo, Leticia Veras; Abessa, Denis Moledo de Souza</p> <p>2013-09-01</p> <p>Santos-São Vicente Estuarine System is a highly populated coastal <span class="hlt">zone</span> in Brazil and where it is located the major port of Latin America. Historically, port activities, industrial and domestic effluents discharges have constituted the main sources of contaminants to estuarine system. This study aimed to assess the recent status of <span class="hlt">sediment</span> quality from 5 <span class="hlt">zones</span> of Port of Santos by applying a lines-of-evidence approach through integrating results of: (1) acute toxicity of whole <span class="hlt">sediment</span> and chronic toxicity of liquid phases; (2) grain size, organic matter, organic carbon, nitrogen, phosphorus, trace metals, polycyclic aromatic hydrocarbons, linear alkylbenzenes and butyltins; (3) benthic community descriptors. Results revealed a gradient of increasing contamination for metals and organic compounds, alongside with their geochemical carriers. <span class="hlt">Sediment</span> liquid phases were more toxic compared to whole <span class="hlt">sediment</span>. Low number of species and individuals indicated the impoverishment of benthic community. The use of site-specific <span class="hlt">sediment</span> quality guidelines was more appropriate to predict <span class="hlt">sediment</span> toxicity. The integration of results through <span class="hlt">Sediment</span> Quality Triad approach and principal component analysis allowed observing the effects of natural stressors and dredging on <span class="hlt">sediment</span> quality and benthic distribution. Even with recent governmental efforts to control, pollution is still relevant in Port of Santos and a threat to local ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/14866','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/14866"><span>The Effectiveness of Permanent Highway Runoff Controls: <span class="hlt">Sedimentation</span>/Filtration Systems</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1998-09-01</p> <p>Original Report Date: October 1997. This study evaluates the performance of <span class="hlt">sedimentation</span>/filtration systems that are the most common control for treating highway runoff in the Edwards Aquifer recharge <span class="hlt">zone</span>. The study includes: 1) monitoring and eval...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SedG..364..228B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SedG..364..228B"><span>The Devils Mountain Fault <span class="hlt">zone</span>: An active Cascadia upper plate <span class="hlt">zone</span> of deformation, Pacific Northwest of North America</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barrie, J. Vaughn; Greene, H. Gary</p> <p>2018-02-01</p> <p>The Devils Mountain Fault <span class="hlt">Zone</span> (DMFZ) extends east to west from Washington State to just south of Victoria, British Columbia, in the northern Strait of Juan de Fuca of Canada and the USA. Recently collected geophysical data were used to map this fault <span class="hlt">zone</span> in detail, which show the main fault trace, and associated primary and secondary (conjugate) strands, and extensive northeast-southwest oriented folding that occurs within a 6 km wide deformation <span class="hlt">zone</span>. The fault <span class="hlt">zone</span> has been active in the Holocene as seen in the offset and disrupted upper Quaternary strata, seafloor displacement, and deformation within <span class="hlt">sediment</span> cores taken close to the seafloor expression of the faults. Data suggest that the present DMFZ and the re-activated Leech River Fault may be part of the same fault system. Based on the length and previously estimated slip rates of the fault <span class="hlt">zone</span> in Washington State, the DMFZ appears to have the potential of producing a strong earthquake, perhaps as large as magnitude 7.5 or greater, within 2 km of the city of Victoria.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Geomo.222..122M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Geomo.222..122M"><span>A detrital <span class="hlt">sediment</span> budget of a Maldivian reef platform</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morgan, K. M.; Kench, P. S.</p> <p>2014-10-01</p> <p><span class="hlt">Sediment</span> dynamics are an important control on the morphology and development of reef systems by actively removing and redistributing excess detrital <span class="hlt">sediment</span>. This study presents quantitative data from direct point measurements of <span class="hlt">sediment</span> transport on the platform surface and fore-reef slope of Vabbinfaru reef, North Malé Atoll, Maldives. A suite of <span class="hlt">sediment</span> traps were used to construct actual rates of platform <span class="hlt">sediment</span> fluxes and off-reef export over different spatial and temporal (seasonal) scales to establish key <span class="hlt">sediment</span> transport pathways. Findings showed that high <span class="hlt">sediment</span> fluxes occur on Vabbinfaru platform in the absence of major storm activity (up to 1905 g m- 1 d- 1), with 95% of annual transport occurring during the southwest monsoon as a result of increased wave energy. Climate-driven changes in the platform process regime caused a reversal of net <span class="hlt">sediment</span> transport pathways between each monsoon season. Off-reef export rates were high, reaching a maximum of 12.58 kg m- 1 y- 1 for gravel and 407 g m- 1 d- 1 for sand-sized <span class="hlt">sediment</span>. An estimated 127,120 kg is exported from the platform annually equating to a significant loss from the reef <span class="hlt">sediment</span> budget and contributing to the long-term geomorphic development of the fore-reef slope and atoll basin. Detrital <span class="hlt">sediment</span> reservoirs on Vabbinfaru are not purely depositional carbonate sinks, but rather temporary stores that are important in the transfer of <span class="hlt">sediment</span> between reef <span class="hlt">zones</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Geomo.193..112F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Geomo.193..112F"><span><span class="hlt">Sediment</span> tracing in the upper Hunter catchment using elemental and mineralogical compositions: Implications for catchment-scale suspended <span class="hlt">sediment</span> (dis)connectivity and management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fryirs, Kirstie; Gore, Damian</p> <p>2013-07-01</p> <p>River bed colmation layers clog the interstices of gravel-bed rivers, impeding the vertical exchange of water and nutrients that drives ecosystem function in the hyporheic <span class="hlt">zone</span>. In catchments where fine-grained <span class="hlt">sediment</span> supply has increased since human disturbance, understanding <span class="hlt">sediment</span> provenance and the (dis)connectivity of supply allows practitioners to target <span class="hlt">sediment</span> source problems and treat them within catchment management plans. Release of alluvial fine-grained <span class="hlt">sediment</span> from channel bank erosion since European settlement has resulted in the formation of a colmation layer along the upper Hunter River at Muswellbrook, eastern Australia. X-ray fluorescence spectrometry (XRF) and X-ray diffractometry (XRD) are used to determine the elemental and mineralogical signatures of colmation layer and floodplain <span class="hlt">sediment</span> sources across this 4480 km2 catchment. This <span class="hlt">sediment</span> tracing technique is used to construct a picture of how suspended <span class="hlt">sediment</span> supply and (dis)connectivity operates in this catchment. In this system, the primary source areas are subcatchments in which <span class="hlt">sediments</span> are stored largely in partly confined floodplain pockets, but from which <span class="hlt">sediment</span> supply is unimpeded and directly connected to the receiving reach. Subcatchments in which alluvial <span class="hlt">sediment</span> storage is significant — and which contain large, laterally unconfined valleys — are essentially 'switched off' or disconnected from the receiving reach. This is because large <span class="hlt">sediment</span> sinks act to trap fine-grained <span class="hlt">sediment</span> before it reaches the receiving reach, forming a buffer along the <span class="hlt">sediment</span> conveyor belt. Given the age structure of floodplains in the receiving reach, this pattern of source area contributions and (dis)connectivity must have occurred throughout the Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=244211&keyword=coral+AND+reef&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=244211&keyword=coral+AND+reef&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>EPA studies distribution of terrestrial <span class="hlt">sediment</span> in coastal <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Fundamental to the inter-Agency effort to protect coral reefs in southwestern Puerto Rico is the assumption that soil eroded from land in the Guánica/Rio Loco watershed is carried out of Guánica Bay and into coral reef <span class="hlt">zones</span> and may even be pushed by currents to the west, where i...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H31F1457S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H31F1457S"><span>Identifying Attributes of CO2 Leakage <span class="hlt">Zones</span> in Shallow Aquifers Using a Parametric Level Set Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sun, A. Y.; Islam, A.; Wheeler, M.</p> <p>2016-12-01</p> <p>Leakage through abandoned wells and geologic faults poses the greatest risk to CO2 storage permanence. For shallow aquifers, secondary CO2 plumes emanating from the leak <span class="hlt">zones</span> may go undetected for a sustained period of time and has the greatest potential to cause large-scale and long-term environmental impacts. Identification of the attributes of leak <span class="hlt">zones</span>, including their shape, location, and strength, is required for proper environmental risk assessment. This study applies a parametric level set (PaLS) method to characterize the leakage <span class="hlt">zone</span>. Level set methods are appealing for tracking topological changes and <span class="hlt">recovering</span> unknown shapes of objects. However, level set evolution using the conventional level set methods is challenging. In PaLS, the level set function is approximated using a weighted sum of basis functions and the level set evolution problem is replaced by an optimization problem. The efficacy of PaLS is demonstrated through <span class="hlt">recovering</span> the source <span class="hlt">zone</span> created by CO2 leakage into a carbonate aquifer. Our results show that PaLS is a robust source identification method that can <span class="hlt">recover</span> the approximate source locations in the presence of measurement errors, model parameter uncertainty, and inaccurate initial guesses of source flux strengths. The PaLS inversion framework introduced in this work is generic and can be adapted for any reactive transport model by switching the pre- and post-processing routines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMEP13B1027T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMEP13B1027T"><span>Stratigraphic Transfer Thresholds of <span class="hlt">Sediment</span> Supply Signals in Channelized Systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Toby, S. C.; De Angelis, S.; Duller, R.; Straub, K. M.</p> <p>2016-12-01</p> <p>The stratigraphic record is a unique physical archive for past climate and tectonic boundary conditions on Earth and other planetary bodies. These boundary and forcing conditions set the rate and volume of <span class="hlt">sediment</span> delivered to sedimentary basins, which can be, theoretically, linked back to the stratigraphic record. However for <span class="hlt">sediment</span> supply signals to make their way through to stratigraphy they must pass through the active layer of the Earth's surface, which is scaled to channel depth. For the long-term, the likelihood of this taking place can be evaluated using the vertical time-scale of autogenics. The current study tests whether or not cyclic <span class="hlt">sediment</span> supply to an experimental delta can influence morphodynamics and if so, can this be <span class="hlt">recovered</span> from synthetic and physical stratigraphic dataset collected during the experiments. Preliminary results suggest that short period <span class="hlt">sediment</span> supply signals are less likely to be transferred to the stratigraphic record, which is predicted by our theoretical framework for channelized systems. Once fully validated by the experiments the theoretical approach will be applied to field stratigraphy and used to guide more reliable interpretation of ancient <span class="hlt">sediment</span> supply signals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26531711','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26531711"><span>Response of invertebrates from the hyporheic <span class="hlt">zone</span> of chalk rivers to eutrophication and land use.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pacioglu, Octavian; Moldovan, Oana Teodora</p> <p>2016-03-01</p> <p>Whereas the response of lotic benthic macroinvertebrates to different environmental stressors is a widespread practice nowadays in assessing the water and habitat quality, the use of hyporheic <span class="hlt">zone</span> invertebrates is still in its infancy. In this study, classification and regression trees analysis were employed in order to assess the ecological requirements and the potential as bioindicators for the hyporheic <span class="hlt">zone</span> invertebrates inhabiting four lowland chalk rivers (south England) with contrasting eutrophication levels (based on surface nitrate concentrations) and magnitude of land use (based on percentage of fine <span class="hlt">sediments</span> load and median interstitial space). Samples of fauna, water and <span class="hlt">sediment</span> were sampled twice, during low (summer) and high (winter) groundwater level, at depths of 20 and 35 cm. Certain groups of invertebrates (Glossosomatidae and Psychomyiidae caddisflies, and riffle beetles) proved to be good indicators of rural catchments, moderately eutrophic and with high fine <span class="hlt">sediment</span> load. A diverse community dominated by microcrustaceans (copepods and ostracods) were found as good indicators of highly eutrophic urban streams, with moderate-high fine <span class="hlt">sediment</span> load. However, the use of other taxonomic groups (e.g. chironomids, oligochaetes, nematodes, water mites and the amphipod Gammarus pulex), very widespread in the hyporheic <span class="hlt">zone</span> of all sampled rivers, is of limited use because of their high tolerance to the analysed stressors. We recommend the use of certain taxonomic groups (comprising both meiofauna and macroinvertebrates) dwelling in the chalk hyporheic <span class="hlt">zone</span> as indicators of eutrophication and colmation and, along with routine benthic sampling protocols, for a more comprehensive water and habitat quality assessment of chalk rivers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24158459','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24158459"><span>Natural and anthropogenic controls on <span class="hlt">sediment</span> composition of an arid coastal environment: Sharm Obhur, Red Sea, Saudi Arabia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ghandour, I M; Basaham, A S; Basaham, S; Al-Washmi, H A; Al-Washmi, A; Masuda, H</p> <p>2014-03-01</p> <p>The present study investigated the natural and anthropogenic processes that control the composition of the bottom <span class="hlt">sediments</span> of Sharm Obhur, Red Sea. Mineralogical analysis using XRD indicated that the <span class="hlt">sediments</span> consist of carbonate and non-carbonate minerals. Elemental interrelationships allowed differentiating two groups of elements of different sources and origin. Elements that are in the same group are positively correlated, while they correlate negatively with elements of the other group. The first group includes silicon, Al, Fe, Mn, Mg, vanadium (V), chromium (Cr), Co, Ni, Cu, and Zn, whereas the other group includes Ca, Sr, and CaCO3. The highest concentration levels of the first group and the highest content of non-carbonate minerals were obtained from the <span class="hlt">sediments</span> near the head of the sharm (<span class="hlt">zone</span> A), whereas the <span class="hlt">sediments</span> near the mouth of the sharm (<span class="hlt">zone</span> B) yielded high concentrations of second group and carbonate minerals. Metal enrichment and contamination factors and pollution load index were calculated. The values of these indices differentiate two groups of metals: lithogenic and non-lithogenic. Except for lead (Pb) at one sampling site, metals in <span class="hlt">zone</span> A <span class="hlt">sediments</span> are of lithogenic source, supplied to the sharm either naturally by aeolian transportation and through Wadi Al-Kuraa'a during rare but major floods or by human activities such as dumping and shore protection. Non-lithogenic Cr, Pb, V, and Mn were documented from some sampling sites in <span class="hlt">zone</span> B, and their occurrences are related to waste disposal and fossil fuel combustion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008SGeo...29....1D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008SGeo...29....1D"><span>Advances in the Study of Moving <span class="hlt">Sediments</span> and Evolving Seabeds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davies, Alan G.; Thorne, Peter D.</p> <p>2008-01-01</p> <p>Sands and mud are continually being transported around the world’s coastal seas due to the action of tides, wind and waves. The transport of these <span class="hlt">sediments</span> modifies the boundary between the land and the sea, changing and reshaping its form. Sometimes the nearshore bathymetry evolves slowly over long time periods, at other times more rapidly due to natural episodic events or the introduction of manmade structures at the shoreline. For over half a century we have been trying to understand the physics of <span class="hlt">sediment</span> transport processes and formulate predictive models. Although significant progress has been made, our capability to forecast the future behaviour of the coastal <span class="hlt">zone</span> from basic principles is still relatively poor. However, innovative acoustic techniques for studying the fundamentals of <span class="hlt">sediment</span> movement experimentally are now providing new insights, and it is expected that such observations, coupled with developing theoretical works, will allow us to take further steps towards the goal of predicting the evolution of coastlines and coastal bathymetry. This paper presents an overview of our existing predictive capabilities, primarily in the field of non-cohesive <span class="hlt">sediment</span> transport, and highlights how new acoustic techniques are enabling our modelling efforts to achieve greater sophistication and accuracy. The paper is aimed at coastal scientists and managers seeking to understand how detailed physical studies can contribute to the improvement of coastal area models and, hence, inform coastal <span class="hlt">zone</span> management strategies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18...71R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18...71R"><span>Metagenomic analysis of nitrogen metabolism genes in the surface of marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reyes, Carolina; Schneider, Dominik; Thürmer, Andrea; Dellwig, Olaf; Lipka, Marko; Daniel, Rolf; Böttcher, Michael E.; Friedrich, Michael W.</p> <p>2016-04-01</p> <p>In this study, we analysed metagenomes along with biogeochemical profiles from Skagerrak (North Sea) and Bothnian Bay (Baltic Sea) <span class="hlt">sediments</span>, to trace the prevailing nitrogen pathways. NO3- was present in the top 5 cm below the <span class="hlt">sediment</span>-water interface at both sites. NH4+ increased with depth below 5 cm where it overlapped with the NO3- <span class="hlt">zone</span>. Steady state modelling of NO3- and NH4+ porewater profiles indicates <span class="hlt">zones</span> of net nitrogen species transformations. Protease, peptidase, urease and deaminase ammonification genes were detected in metagenomes. Genes involved in ammonia oxidation (amo, hao), nitrite oxidation (nxr), denitrification (nar, nir, nor) and dissimilatory NO3- reduction to NH4+ (nap, nfr and otr) were also present. 16S rRNA gene analysis showed that the nitrifying group Nitrosopumilales and other groups involved in nitrification and denitrification (Nitrobacter, Nitrosomonas, Nitrospira, Nitrosococcus, and Nitrosonomas) appeared less abundant in Skagerrak <span class="hlt">sediments</span> compared to Bothnian Bay <span class="hlt">sediments</span>. Beggiatoa and Thiothrix 16S rRNA genes were also present suggesting chemolithoautotrophic NO3- reduction to NO2- or NH4+ as a possible pathway. Although anammox planctomycetes 16S rRNA genes were present in metagenomes, anammox protein-coding genes were not detected. Our results show the metabolic potential for ammonification, nitrification, NO3- reduction, and denitrification activities in Skagerrak and Bothnian Bay <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMEP23D0859S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMEP23D0859S"><span>Numerical simulation of turbulence and <span class="hlt">sediment</span> transport of medium sand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmeeckle, M. W.</p> <p>2012-12-01</p> <p> particles are preferentially concentrated in <span class="hlt">zones</span> of upward fluid velocity. This may explain previous observations noting a rapid vertical rise at the beginning of saltation trajectories. The simulations described here have no lift forces. Because of the short particle time scales relative to that of the turbulent structures, high transport stage bedload entrainment <span class="hlt">zones</span> involve mutual interaction between turbulence structures and bed deformation. These deformation structures appear as depressed areas of the bed at the center of the sweep and raised areas of entraining particles at the edges of the sweep penetration. Suspended <span class="hlt">sediment</span> entrainment structures are similar to these bedload entrainment structures but have much larger scales. Preferential concentration of suspended grains in <span class="hlt">zones</span> of upward moving fluid dampens turbulence intensities and momentum transport. Much of the suspended transport takes place within this highly concentrated near-bed <span class="hlt">zone</span> of damped turbulence. Particle-fluid correlation coefficients are relatively low in the lower portion of this highly concentrated suspended <span class="hlt">sediment</span> <span class="hlt">zone</span>, owing to particle-particle interactions. As such, Rouse-like profiles utilizing eddy viscosity closures, adjusted according to flux Richardson numbers, do not adequately describe the physics of this <span class="hlt">zone</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017431','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017431"><span>Suspended <span class="hlt">sediments</span> of the modern Amazon and Orinoco rivers</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Meade, R.H.</p> <p>1994-01-01</p> <p>The Amazon and Orinoco Rivers are massive transcontinental conveyance systems for suspended <span class="hlt">sediment</span>. They derive about 90% of their <span class="hlt">sediment</span> from the Andes that support their western headwaters, transport it for thousands of kilometers across the breadth of the continent and deposit it in the coastal <span class="hlt">zones</span> of the Atlantic. At their points of maximum suspended-<span class="hlt">sediment</span> discharge, the Amazon transports an average of 1100-1300 ?? 106 tons per year and the Orinoco transports about 150 ?? 106 tons per year. Relations of <span class="hlt">sediment</span> discharge to water discharge are complicated by unusual patterns of seasonal storage and remobilization, increased storage and reduced transport of <span class="hlt">sediment</span> in the middle Orinoco during periods of peak water discharge, and storage of suspended <span class="hlt">sediment</span> in the lower Amazon during rising discharge and resuspension during falling discharge. Spatial distributions of suspended <span class="hlt">sediment</span> in cross-sections of both rivers are typically heterogeneous, not only in the vertical sense but also in the lateral. The cross-channel mixing of tributary inputs into the mainstem waters is a slow process that requires several hundred kilometers of downriver transport to complete. Considerable fine-grained <span class="hlt">sediment</span> is exchanged between rivers and floodplains by the combination of overbank deposition and bank erosion. ?? 1994.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10550047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10550047"><span>Fault slip rates in the modern new madrid seismic <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mueller; Champion; Guccione; Kelson</p> <p>1999-11-05</p> <p>Structural and geomorphic analysis of late Holocene <span class="hlt">sediments</span> in the Lake County region of the New Madrid seismic <span class="hlt">zone</span> indicates that they are deformed by fault-related folding above the blind Reelfoot thrust fault. The widths of narrow kink bands exposed in trenches were used to model the Reelfoot scarp as a forelimb on a fault-bend fold; this, coupled with the age of folded <span class="hlt">sediment</span>, yields a slip rate on the blind thrust of 6.1 +/- 0.7 mm/year for the past 2300 +/- 100 years. An alternative method used structural relief across the scarp and the estimated dip of the underlying blind thrust to calculate a slip rate of 4.8 +/- 0.2 mm/year. Geometric relations suggest that the right lateral slip rate on the New Madrid seismic <span class="hlt">zone</span> is 1.8 to 2.0 mm/year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70045584','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70045584"><span>Estimating floodplain <span class="hlt">sedimentation</span> in the Laguna de Santa Rosa, Sonoma County, CA</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Curtis, Jennifer A.; Flint, Lorraine E.; Hupp, Cliff R.</p> <p>2013-01-01</p> <p>We present a conceptual and analytical framework for predicting the spatial distribution of floodplain <span class="hlt">sedimentation</span> for the Laguna de Santa Rosa, Sonoma County, CA. We assess the role of the floodplain as a sink for fine-grained <span class="hlt">sediment</span> and investigate concerns regarding the potential loss of flood storage capacity due to historic <span class="hlt">sedimentation</span>. We characterized the spatial distribution of <span class="hlt">sedimentation</span> during a post-flood survey and developed a spatially distributed <span class="hlt">sediment</span> deposition potential map that highlights <span class="hlt">zones</span> of floodplain <span class="hlt">sedimentation</span>. The <span class="hlt">sediment</span> deposition potential map, built using raster files that describe the spatial distribution of relevant hydrologic and landscape variables, was calibrated using 2 years of measured overbank <span class="hlt">sedimentation</span> data and verified using longer-term rates determined using dendrochronology. The calibrated floodplain deposition potential relation was used to estimate an average annual floodplain <span class="hlt">sedimentation</span> rate (3.6 mm/year) for the ~11 km2 floodplain. This study documents the development of a conceptual model of overbank <span class="hlt">sedimentation</span>, describes a methodology to estimate the potential for various parts of a floodplain complex to accumulate <span class="hlt">sediment</span> over time, and provides estimates of short and long-term overbank <span class="hlt">sedimentation</span> rates that can be used for ecosystem management and prioritization of restoration activities.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_18 --> <div id="page_19" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="361"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMEP13A0862M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMEP13A0862M"><span>Decadal-scale Evolution of <span class="hlt">Sediment</span> Flux in the Aulne Estuary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moskalski, S. M.; Deschamps, A.; Floc'h, F.; Verney, R.; Piete, H.; Fromant, G.; Delacourt, C.</p> <p>2013-12-01</p> <p>Estuarine <span class="hlt">sediment</span> transport processes have the potential to evolve over time in response to alterations in various factors both internal and external to the estuary, such as <span class="hlt">sediment</span> supply, river discharge, tidal forcing, or changes to bathymetry. Changes in <span class="hlt">sediment</span> transport can affect many estuarine processes (e.g. budgets of <span class="hlt">sediment</span>-adsorbed contaminants or nutrients) and ecosystem services, such as aquaculture, primary production and the need to dredge shipping channels. Most studies of decadal-scale changes in estuaries focus on geomorphology or bathymetry, or are performed using models calibrated by a limited set of observational studies. Because of the potential for <span class="hlt">sediment</span> flux to both affect and be affected by geomorphology and bathymetry, observational studies oriented to <span class="hlt">sediment</span> flux evolution are needed. This study focuses on two intensive observational studies separated by 30 years to quantify change in suspended <span class="hlt">sediment</span> concentration (SSC) in the Aulne river, a shallow macrotidal estuary in western Brittany. Moored and vessel-mounted acoustic Doppler current profilers and YSIs were deployed over a three-week period in the winter of 2013 to examine hydrodynamic and <span class="hlt">sediment</span> transport processes. The results of the modern study were compared to a 1977 investigation of currents, suspended <span class="hlt">sediment</span> concentration, and erosion/deposition. The 1977 study found that SSC during spring tide and average river discharge was less than 30 mg/L near the mouth and above 300 mg/L landward, with near-bottom concentrations in the turbidity maximum <span class="hlt">zone</span> occasionally greater than 1000 mg/L. SSC was highest during low tide and remained elevated throughout, in the upstream part of the estuary. <span class="hlt">Sediment</span> deposition was stronger after flood tide due to a longer slack period, which implies landward <span class="hlt">sediment</span> transport in the estuary. In the 2013 study, near-bottom SSC during spring tide and average river discharge was also highest during low tide, but SSC was above 1000 mg</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP41C1784K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP41C1784K"><span>Black carbon in deep-sea <span class="hlt">sediments</span> from the northeastern equatorial Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, D.; Lee, Y.; Hyeong, K.; Yoo, C.</p> <p>2011-12-01</p> <p>Deep-sea <span class="hlt">sediment</span> core is a good archive for understanding the land-ocean interactions via atmosphere, due to it is little influenced by fluvial and continental shelf processes. This study dealt with black carbon(BC) in a 328 cm-long piston core collected from the northeastern equatorial Pacific Ocean (16°12'N, 125°59'W), covering the last 15 Ma (Hyeong at al., 2004). BC is a common name of carbon continuum formed by incomplete combustion of fossil fuels and plant materials. Though it may react with ozone and produce water-soluble organic carbon, BC has commonly refractory nature. Thus BC in preindustrial <span class="hlt">sediment</span> can be a tracer of forest-fire events. BC is purely terrestrial in origin, and is transported to marine environments by atmospheric and fluvial processes. Therefore, distribution of BC in deep-sea <span class="hlt">sediments</span> could be used to understand atmospheric circulation. Chemical oxidation was used to determine BC in this study following Lim and Cachier (1996). Concentration of BC varies from 0.010% to 0.233% of total <span class="hlt">sediments</span>. Mass accumulation rate (MAR) of BC ranged between 0.077 mg/cm^2/1000 yrs and 47.49 mg/cm^21000 yrs. It is noted that MAR in <span class="hlt">sediments</span> younger than 8 Ma (av. 9.0 mg/cm^2/1000 yrs) is higher than that in <span class="hlt">sediments</span> older than 8 Ma (av. 3.2 mg/cm^2/1000 yrs). Stable carbon isotope value of BC increases with time from the low δ13C value near 13 Ma until it reaches the highest value near 4 Ma. Change of MAR seems to be related to the meridional migration of Intertropical Convergence <span class="hlt">Zone</span> (ITCZ) at around 8 Ma in the study area (cf., Hyeong at al., 2004). Accordingly, higher BC content in <span class="hlt">sediment</span> younger than 8 Ma seems to be accounted for by its derivation from the Northern Hemisphere compared to that from the Southern Hemisphere in older <span class="hlt">sediment</span>. Increase of carbon isotope value with time seems to be related to expansion of C4 grassland. C4 grassland expansion might have been caused by change of atmosphreic cycle, which moved dry subtropical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25518648','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25518648"><span>[<span class="hlt">Sediment</span>-water flux and processes of nutrients and gaseous nitrogen release in a China River Reservoir].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Zhu-hong; Chen, Neng-wang; Wu, Yin-qi; Mo, Qiong-li; Zhou, Xing-peng; Lu, Ting; Tian, Yun</p> <p>2014-09-01</p> <p>The key processes and fluxes of nutrients (N and P) and gaseous N (N2 and N2O) across the <span class="hlt">sediment</span>-water interface in a river reservoir (Xipi) of the Jiulong River watershed in southeast China were studied. Intact core <span class="hlt">sediment</span> incubation of nutrients exchange, in-situ observation and lab incubation of excess dissolved N2 and N2O (products of nitrification, denitrification and Anammox), and determination of physiochemical and microbe parameters were carried out in 2013 for three representative sites along the lacustrine <span class="hlt">zone</span> of the reservoir. Results showed that ammonium and phosphate were generally released from <span class="hlt">sediment</span> to overlying water [with averaged fluxes of N (479.8 ± 675.4) mg. (m2. d)-1 and P (4. 56 ± 0.54) mg. (m2 d) -1] , while nitrate and nitrite diffused into the <span class="hlt">sediment</span>. Flood events in the wet season could introduce a large amount of particulate organic matter that would be trapped by the dam reservoir, resulting in the high release fluxes of ammonium and phosphate observed in the following low-flow season. No clear spatial variation of <span class="hlt">sediment</span> nutrient release was found in the lacustrine <span class="hlt">zone</span> of the reservoir. Gaseous N release was dominated by excess dissolved N2 (98% of total), and the N2 flux from <span class="hlt">sediment</span> was (15.8 ± 12. 5) mg (m2. d) -1. There was a longitudinal and vertical variation of excess dissolved N2, reflecting the combined results of denitrification and Anammox occurring in anoxic <span class="hlt">sediment</span> and fluvial transport. Nitrification mainly occurred in the lower lacustrine <span class="hlt">zone</span>, and the enrichment of N2O was likely regulated by the ratio of ammonium to DIN in water.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70000530','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70000530"><span>Spatial and temporal variability in <span class="hlt">sedimentation</span> rates associated with cutoff channel infill deposits: Ain River, France</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Piégay, H.; Hupp, C.R.; Citterio, A.; Dufour, S.; Moulin, B.; Walling, D.E.</p> <p>2008-01-01</p> <p>Floodplain development is associated with lateral accretion along stable channel geometry. Along shifting rivers, the floodplain <span class="hlt">sedimentation</span> is more complex because of changes in channel position but also cutoff channel presence, which exhibit specific overflow patterns. In this contribution, the spatial and temporal variability of <span class="hlt">sedimentation</span> rates in cutoff channel infill deposits is related to channel changes of a shifting gravel bed river (Ain River, France). The <span class="hlt">sedimentation</span> rates estimated from dendrogeomorphic analysis are compared between and within 14 cutoff channel infills. Detailed analyses along a single channel infill are performed to assess changes in the <span class="hlt">sedimentation</span> rates through time by analyzing activity profiles of the fallout radionuclides 137Cs and unsupported 210Pb. <span class="hlt">Sedimentation</span> rates are also compared within the channel infills with rates in other plots located in the adjacent floodplain. <span class="hlt">Sedimentation</span> rates range between 0.65 and 2.4 cm a−1 over a period of 10 to 40 years. The data provide additional information on the role of distance from the bank, overbank flow frequency, and channel geometry in controlling the <span class="hlt">sedimentation</span> rate. Channel infills, lower than adjacent floodplains, exhibit higher <span class="hlt">sedimentation</span> rates and convey overbank <span class="hlt">sediment</span> farther away within the floodplain. Additionally, channel degradation, aggradation, and bank erosion, which reduce or increase the distance between the main channel and the cutoff channel aquatic <span class="hlt">zone</span>, affect local overbank flow magnitude and frequency and therefore <span class="hlt">sedimentation</span> rates, thereby creating a complex mosaic of <span class="hlt">sedimentation</span> <span class="hlt">zones</span> within the floodplain and along the cutoff channel infills. Last, the dendrogeomorphic and 137Cs approaches are cross validated for estimating the <span class="hlt">sedimentation</span> rate within a channel infill.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/15731','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/15731"><span>Watershed scale assessment of the impact of forested riparian <span class="hlt">zones</span> on stream water quality</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>J. A. Webber; K. W. J. Williard; M. R. Whiles; M. L. Stone; J. J. Zaczek; D. K. Davie</p> <p>2003-01-01</p> <p>Federal and state land management agencies have been promoting forest and grass riparian <span class="hlt">zones</span> to combat non-point source nutrient and <span class="hlt">sediment</span> pollution of our nations' waters. The majority of research examining the effectiveness of riparian buffers at reducing nutrient and <span class="hlt">sediment</span> inputs to streams has been conducted at the field scale. This study took a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GPC...163....1I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GPC...163....1I"><span>Fluctuations in the East Asian monsoon recorded by pollen assemblages in <span class="hlt">sediments</span> from the Japan Sea off the southwestern coast of Hokkaido, Japan, from 4.3 Ma to the present</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Igarashi, Yaeko; Irino, Tomohisa; Sawada, Ken; Song, Lu; Furota, Satoshi</p> <p>2018-04-01</p> <p>We reconstructed fluctuations in the East Asian monsoon and vegetation in the Japan Sea region since the middle Pliocene based on pollen data obtained from <span class="hlt">sediments</span> collected by the Integrated Ocean Drilling Program off the southwestern coast of northern Japan. Taxodiaceae conifers Metasequoia and Cryptomeria and Sciadopityacere conifer Sciadopitys are excellent indicators of a humid climate during the monsoon. The pollen temperature index (Tp) can be used as a proxy for relative air temperature. Based on changes in vegetation and reconstructed climate over a period of 4.3 Ma, we classified the <span class="hlt">sediment</span> sequence into six pollen <span class="hlt">zones</span>. From 4.3 to 3.8 Ma (<span class="hlt">Zone</span> 1), the climate fluctuated between cool/moist and warm/moist climatic conditions. Vegetation changed between warm temperate mixed forest and cool temperate conifer forest. The Neogene type tree Carya <span class="hlt">recovered</span> under a warm/moist climate. The period from 3.8 to 2.5 Ma (<span class="hlt">Zone</span> 2) was characterized by increased Metasequoia pollen concentration. Warm temperate mixed forest vegetation developed under a cool/moist climate. The period from 2.5 to 2.2 Ma (<span class="hlt">Zone</span> 3) was characterized by an abrupt increase in Metasequoia and/or Cryptomeria pollen and a decrease in warm broadleaf tree pollen, indicating a cool/humid climate. The <span class="hlt">Zone</span> 4 period (2.2-1.7 Ma) was characterized by a decrease in Metasequoia and/or Cryptomeria pollen and an increase in cool temperate conifer Picea and Tsuga pollen, indicating a cool/moist climate. The period from 1.7 to 0.3 Ma (<span class="hlt">Zone</span> 5) was characterized by orbital-scale climate fluctuations. Cycles of abrupt increases and decreases in Cryptomeria and Picea pollen and in Tp values indicated changes between warm/humid and cold/dry climates. The alpine fern Selaginella selaginoides appeared as of 1.6 Ma. Vegetation alternated among warm mixed, cool mixed, and cool temperate conifer forests. <span class="hlt">Zone</span> 6 (0.3 Ma to present) was characterized by a decrease in Cryptomeria pollen. The warm temperate broadleaf</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PEPS....5...19T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PEPS....5...19T"><span>High-resolution and high-precision correlation of dark and light layers in the Quaternary hemipelagic <span class="hlt">sediments</span> of the Japan Sea <span class="hlt">recovered</span> during IODP Expedition 346</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tada, Ryuji; Irino, Tomohisa; Ikehara, Ken; Karasuda, Akinori; Sugisaki, Saiko; Xuan, Chuang; Sagawa, Takuya; Itaki, Takuya; Kubota, Yoshimi; Lu, Song; Seki, Arisa; Murray, Richard W.; Alvarez-Zarikian, Carlos; Anderson, William T.; Bassetti, Maria-Angela; Brace, Bobbi J.; Clemens, Steven C.; da Costa Gurgel, Marcio H.; Dickens, Gerald R.; Dunlea, Ann G.; Gallagher, Stephen J.; Giosan, Liviu; Henderson, Andrew C. G.; Holbourn, Ann E.; Kinsley, Christopher W.; Lee, Gwang Soo; Lee, Kyung Eun; Lofi, Johanna; Lopes, Christina I. C. D.; Saavedra-Pellitero, Mariem; Peterson, Larry C.; Singh, Raj K.; Toucanne, Samuel; Wan, Shiming; Zheng, Hongbo; Ziegler, Martin</p> <p>2018-12-01</p> <p>The Quaternary hemipelagic <span class="hlt">sediments</span> of the Japan Sea are characterized by centimeter- to decimeter-scale alternation of dark and light clay to silty clay, which are bio-siliceous and/or bio-calcareous to a various degree. Each of the dark and light layers are considered as deposited synchronously throughout the deeper (> 500 m) part of the sea. However, attempts for correlation and age estimation of individual layers are limited to the upper few tens of meters. In addition, the exact timing of the depositional onset of these dark and light layers and its synchronicity throughout the deeper part of the sea have not been explored previously, although the onset timing was roughly estimated as 1.5 Ma based on the result of Ocean Drilling Program legs 127/128. Consequently, it is not certain exactly when their deposition started, whether deposition of dark and light layers was synchronous and whether they are correlatable also in the earlier part of their depositional history. The Quaternary hemipelagic <span class="hlt">sediments</span> of the Japan Sea were drilled at seven sites during Integrated Ocean Drilling Program Expedition 346 in 2013. Alternation of dark and light layers was <span class="hlt">recovered</span> at six sites whose water depths are > 900 m, and continuous composite columns were constructed at each site. Here, we report our effort to correlate individual dark layers and estimate their ages based on a newly constructed age model at Site U1424 using the best available paleomagnetic datum and marker tephras. The age model is further tuned to LR04 δ18O curve using gamma ray attenuation density (GRA) since it reflects diatom contents that are higher during interglacial high-stands. The constructed age model for Site U1424 is projected to other sites using correlation of dark layers to form a high-resolution and high-precision paleo-observatory network that allows to reconstruct changes in material fluxes with high spatio-temporal resolutions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023002','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023002"><span>Examining differences between <span class="hlt">recovered</span> and declining endangered species</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Abbitt, Robbyn J.F.; Scott, J. Michael</p> <p>2001-01-01</p> <p>Between 1973 and 1999, 43 species in the United States were reclassified from endangered to threatened or removed entirely from the Endangered Species List. Of these, 23 were identified as <span class="hlt">recovered</span>. In 1999 the U.S. Fish and Wildlife Service ( USFWS) published a list of 33 additional species for possible reclassification and/or delisting. We initiated this study to examine why some endangered species <span class="hlt">recover</span> but others continue to decline and to identify differences in management activities between these two groups. We defined <span class="hlt">recovered/recovering</span> species as previously <span class="hlt">recovered</span> species and the additional <span class="hlt">recovered/recovering</span> species listed by the USFWS. We defined declining species as those identified as declining in the most recent USFWS Report to Congress. Information on <span class="hlt">recovered/recovering</span> and declining species was gathered from relevant literature, recovery plans, U.S. Federal Register documents, and individuals responsible for the recovery management of each species. We used this information to examine (1) the percentage of current and historic range covered by management activities; (2) threats affecting the species; (3) population sizes at the time of listing; (4) current versus historic range size; and (5) percentage of recovery management objectives completed. Although few statistical analyses provided significant results, those that did suggest the following differences between <span class="hlt">recovered/recovering</span> and declining species: (1) <span class="hlt">recovered/recovering</span> species face threats that are easier to address; (2) <span class="hlt">recovered/recovering</span> species occupy a greater percentage of their historic range; and (3) <span class="hlt">recovered/recovering</span> species have a greater percentage of their recovery management objectives completed. Those species with threats easier to address and that occupy a greater percentage of their historic range are <span class="hlt">recovered/recovering</span>. In contrast, declining species face threats more difficult to address and occupy significantly less of their historic range. If this</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1234549','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1234549"><span>Floodplain sedimentology and <span class="hlt">sediment</span> accumulation assessment – Savannah River Site</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Yeager, Kevin M.</p> <p>2016-01-03</p> <p>The primary goal of the larger research program, of which this work is one component, is to restore the hydrodynamics and energy gradients of targeted Savannah River Site (SRS) streams to a condition comparable to local natural streams or rivers of similar order, and to stabilize <span class="hlt">sediment</span> transport (net degradation/aggregation) with the assumption that the faunal components of these systems will quickly <span class="hlt">recover</span> on their own (e.g., Pen Branch; Lakly and McArthur, 2000). This work is specifically focused on the identification of near-stream floodplain areas that exhibit <span class="hlt">sediment</span> deposition or erosion, and the quantification of these processes over a historicalmore » time scale (last ~100 years).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25543244','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25543244"><span>Sulfide and methane production in sewer <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Yiwen; Ni, Bing-Jie; Ganigué, Ramon; Werner, Ursula; Sharma, Keshab R; Yuan, Zhiguo</p> <p>2015-03-01</p> <p>Recent studies have demonstrated significant sulfide and methane production by sewer biofilms, particularly in rising mains. Sewer <span class="hlt">sediments</span> in gravity sewers are also biologically active; however, their contribution to biological transformations in sewers is poorly understood at present. In this study, <span class="hlt">sediments</span> collected from a gravity sewer were cultivated in a laboratory reactor fed with real wastewater for more than one year to obtain intact <span class="hlt">sediments</span>. Batch test results show significant sulfide production with an average rate of 9.20 ± 0.39 g S/m(2)·d from the <span class="hlt">sediments</span>, which is significantly higher than the areal rate of sewer biofilms. In contrast, the average methane production rate is 1.56 ± 0.14 g CH4/m(2)·d at 20 °C, which is comparable to the areal rate of sewer biofilms. These results clearly show that the contributions of sewer <span class="hlt">sediments</span> to sulfide and methane production cannot be ignored when evaluating sewer emissions. Microsensor and pore water measurements of sulfide, sulfate and methane in the <span class="hlt">sediments</span>, microbial profiling along the depth of the <span class="hlt">sediments</span> and mathematical modelling reveal that sulfide production takes place near the <span class="hlt">sediment</span> surface due to the limited penetration of sulfate. In comparison, methane production occurs in a much deeper <span class="hlt">zone</span> below the surface likely due to the better penetration of soluble organic carbon. Modelling results illustrate the dependency of sulfide and methane productions on the bulk sulfate and soluble organic carbon concentrations can be well described with half-order kinetics. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024589','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024589"><span>Fluvial <span class="hlt">sediment</span> transport and deposition following the 1991 eruption of Mount Pinatubo</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hayes, S.K.; Montgomery, D.R.; Newhall, C.G.</p> <p>2002-01-01</p> <p>The 1991 eruption of Mount Pinatubo generated extreme <span class="hlt">sediment</span> yields from watersheds heavily impacted by pyroclastic flows. Bedload sampling in the Pasig-Potrero River, one of the most heavily impacted rivers, revealed negligible critical shear stress and very high transport rates that reflected an essentially unlimited <span class="hlt">sediment</span> supply and the enhanced mobility of particles moving over a smooth, fine-grained bed. Dimensionless bedload transport rates in the Pasig-Potrero River differed substantially from those previously reported for rivers in temperate regions for the same dimensionless shear stress, but were similar to rates identified in rivers on other volcanoes and ephemeral streams in arid environments. The similarity between volcanically disturbed and arid rivers appears to arise from the lack of an armored bed surface due to very high relative <span class="hlt">sediment</span> supply; in arid rivers, this is attributed to a flashy hydrograph, whereas volcanically disturbed rivers lack armoring due to sustained high rates of <span class="hlt">sediment</span> delivery. This work suggests that the increases in <span class="hlt">sediment</span> supply accompanying massive disturbance induce morphologic and hydrologic changes that temporarily enhance transport efficiency until the watershed <span class="hlt">recovers</span> and <span class="hlt">sediment</span> supply is reduced. ?? 2002 Elsevier Science B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15170244','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15170244"><span>Analysis of <span class="hlt">sediment</span> retention in western riverine wetlands: the Yampa River watershed, Colorado, USA.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arp, Christopher D; Cooper, David J</p> <p>2004-03-01</p> <p>We quantified annual <span class="hlt">sediment</span> deposition, bank erosion, and <span class="hlt">sediment</span> budgets in nine riverine wetlands that represented a watershed continuum for 1 year in the unregulated Yampa River drainage basin in Colorado. One site was studied for 2 years to compare responses to peak flow variability. Annual mean <span class="hlt">sediment</span> deposition ranged from 0.01 kg/m(2) along a first-order subalpine stream to 21.8 kg/m(2) at a sixth-order alluvial forest. Annual mean riverbank erosion ranged from 3 kg/m-of-bank at the first-order site to 1000 kg/m at the 6(th)-order site. Total <span class="hlt">sediment</span> budgets were nearly balanced at six sites, while net export from bank erosion occurred at three sites. Both total <span class="hlt">sediment</span> deposition (R(2) = 0.86, p < 0.01) and bank erosion (R(2) = 0.77, p < 0.01) were strongly related to bankfull height, and channel sinuosity and valley confinement helped to explain additional variability among sites. The texture and organic fraction of eroded and deposited <span class="hlt">sediment</span> were relatively similar in most sites and varied among sites by watershed position. Our results indicate that bank erosion generally balances <span class="hlt">sediment</span> deposition in riverine wetlands, and we found no distinct <span class="hlt">zones</span> of <span class="hlt">sediment</span> retention versus export on a watershed continuum. <span class="hlt">Zones</span> of apparent disequilibrium can occur in unregulated rivers due to factors such as incised channels, beaver activity, and cattle grazing. A primary function of many western riverine wetlands is <span class="hlt">sediment</span> exchange, not retention, which may operate by transforming materials and compounds in temporary <span class="hlt">sediment</span> pools on floodplains. These results are considered in the context of the Hydrogeomorphic approach being implemented by the U.S. government for wetland resource management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29502003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29502003"><span>Antibiotic and heavy metal resistance in enterococci from coastal marine <span class="hlt">sediment</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vignaroli, Carla; Pasquaroli, Sonia; Citterio, Barbara; Di Cesare, Andrea; Mangiaterra, Gianmarco; Fattorini, Daniele; Biavasco, Francesca</p> <p>2018-06-01</p> <p><span class="hlt">Sediment</span> samples from three coastal sites - two beach resorts (Beach 1 and Beach 2 sites) and an area lying between an oil refinery and a river estuary (Estuarine site) - were analyzed for antibiotic- and heavy metal (HM)-resistant enterococci. A total of 123 enterococci, 36 E. faecium, 34 E. casseliflavus, 33 E. hirae, 5 E. faecalis, 3 E. durans, 3 E. gallinarum, and 9 Enterococcus spp, were <span class="hlt">recovered</span>. Strains resistant to erythromycin, tetracycline and quinupristin/dalfopristin (Q/D) were <span class="hlt">recovered</span> from all sites, whereas multidrug-resistant isolates were <span class="hlt">recovered</span> only from "Beach 2" (14%) and "Estuarine" (3.7%). As regards HM resistance, the strains showed a high frequency (68%) of cadmium and/or copper resistance and uniform susceptibility to mercury. The prevalence of cadmium-resistant strains was significantly higher among erythromycin-resistant than among erythromycin-susceptible strains. A significant association between cadmium or copper resistance and Q/D resistance was also observed at "Estuarine" site. The levels of the two HMs in <span class="hlt">sediment</span> from all sites were fairly low, ranging from 0.070 to 0.126 μg/g, for cadmium and from 1.00 to 7.64 μg/g for copper. Mercury was always undetectable. These findings are consistent with reports that low HM concentrations may contribute to co-selection of antibiotic-resistant bacterial strains, including enterococci. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS51B2044M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS51B2044M"><span>Modeling the Formation of Hydrate-Filled Veins in Fine-Grained <span class="hlt">Sediments</span> from in Situ Microbial Methane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Malinverno, A.; Cook, A.; Daigle, H.</p> <p>2016-12-01</p> <p>Continental margin <span class="hlt">sediments</span> are dominantly fine-grained silt and clay, and methane hydrates in these <span class="hlt">sediments</span> are often found in semi-vertical veins and fractures. In several instances, these hydrate veins occupy discrete depth intervals that are a few tens of meters thick and are surrounded by hydrate-free <span class="hlt">sediments</span>. As they are not connected with gas sources beneath the base of the gas hydrate stability <span class="hlt">zone</span> (GHSZ), these isolated hydrate-bearing intervals have been interpreted as formed by in situ microbial methane. To investigate the formation of these hydrate deposits, we applied a time-dependent advection-diffusion-reaction model that includes the effects of <span class="hlt">sedimentation</span>, compaction, solute diffusion, and microbial methane generation. Microbial methane generation depends on the amount of metabolizable organic carbon deposited at the seafloor, whose progressive degradation produces methane beneath the sulfate reduction <span class="hlt">zone</span>. If the amount of organic carbon entering the methanogenic <span class="hlt">zone</span> is kept constant in time, we found that the computed amounts of hydrate formed in discrete intervals within the GHSZ are well below those estimated from observations. On the other hand, if the deposition of organic carbon is higher in a given time interval, methane generation during burial is more intense in the corresponding <span class="hlt">sediment</span> interval, resulting in enhanced hydrate formation. With variations in organic carbon deposition comparable to those generally observed in continental margins, our model was able to reproduce the methane hydrate contents that were estimated from drilling. These results support the suggestion that in situ microbial generation associated with transient organic carbon deposition is the source of methane that forms isolated intervals of hydrate-filled veins in fine-grained <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1338820','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1338820"><span>Modeling the Formation of Hydrate-Filled Veins in Fine-Grained <span class="hlt">Sediments</span> from in Situ Microbial Methane</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Malinverno, Alberto; Cook, Ann; Daigle, Hugh</p> <p></p> <p>Continental margin <span class="hlt">sediments</span> are dominantly fine-grained silt and clay, and methane hydrates in these <span class="hlt">sediments</span> are often found in semi-vertical veins and fractures. In several instances, these hydrate veins occupy discrete depth intervals that are a few tens of meters thick and are surrounded by hydrate-free <span class="hlt">sediments</span>. As they are not connected with gas sources beneath the base of the gas hydrate stability <span class="hlt">zone</span> (GHSZ), these isolated hydrate-bearing intervals have been interpreted as formed by in situ microbial methane. To investigate the formation of these hydrate deposits, we applied a time-dependent advection-diffusion-reaction model that includes the effects of <span class="hlt">sedimentation</span>, compaction,more » solute diffusion, and microbial methane generation. Microbial methane generation depends on the amount of metabolizable organic carbon deposited at the seafloor, whose progressive degradation produces methane beneath the sulfate reduction <span class="hlt">zone</span>. If the amount of organic carbon entering the methanogenic <span class="hlt">zone</span> is kept constant in time, we found that the computed amounts of hydrate formed in discrete intervals within the GHSZ are well below those estimated from observations. On the other hand, if the deposition of organic carbon is higher in a given time interval, methane generation during burial is more intense in the corresponding <span class="hlt">sediment</span> interval, resulting in enhanced hydrate formation. With variations in organic carbon deposition comparable to those generally observed in continental margins, our model was able to reproduce the methane hydrate contents that were estimated from drilling. These results support the suggestion that in situ microbial generation associated with transient organic carbon deposition is the source of methane that forms isolated intervals of hydrate-filled veins in fine-grained <span class="hlt">sediments</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15899267','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15899267"><span>Use of slow filtration columns to assess oxygen respiration, consumption of dissolved organic carbon, nitrogen transformations, and microbial parameters in hyporheic <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mermillod-Blondin, F; Mauclaire, L; Montuelle, B</p> <p>2005-05-01</p> <p>Biogeochemical processes mediated by microorganisms in river <span class="hlt">sediments</span> (hyporheic <span class="hlt">sediments</span>) play a key role in river metabolism. Because biogeochemical reactions in the hyporheic <span class="hlt">zone</span> are often limited to the top few decimetres of <span class="hlt">sediments</span> below the water-<span class="hlt">sediment</span> interface, slow filtration columns were used in the present study to quantify biogeochemical processes (uptakes of O2, DOC, and nitrate) and the associated microbial compartment (biomass, respiratory activity, and hydrolytic activity) at a centimetre scale in heterogeneous (gravel and sand) <span class="hlt">sediments</span>. The results indicated that slow filtration columns recreated properly the aerobic-anaerobic gradient classically observed in the hyporheic <span class="hlt">zone</span>. O2 and NO3- consumptions (256 +/- 13 microg of O2 per hour and 14.6 +/- 6.1 microg of N-NO3- per hour) measured in columns were in the range of values measured in different river <span class="hlt">sediments</span>. Slow filtration columns also reproduced the high heterogeneity of the hyporheic <span class="hlt">zone</span> with the presence of anaerobic pockets in <span class="hlt">sediments</span> where denitrification and fermentation processes occurred. The respiratory and hydrolytic activities of bacteria were strongly linked with the O2 consumption in the experimental system, highlighting the dominance of aerobic processes in our river <span class="hlt">sediments</span>. In comparison with these activities, the bacterial biomass (protein content) integrated both aerobic and anaerobic processes and could be used as a global microbial indicator in our system. Finally, slow filtration columns are an appropriate tool to quantify in situ rates of biogeochemical processes and to determine the relationship between the microbial compartment and the physico-chemical environment in coarse river <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4016307','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4016307"><span>Hard-Diet Feeding <span class="hlt">Recovers</span> Neurogenesis in the Subventricular <span class="hlt">Zone</span> and Olfactory Functions of Mice Impaired by Soft-Diet Feeding</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Utsugi, Chizuru; Miyazono, Sadaharu; Osada, Kazumi; Sasajima, Hitoshi; Noguchi, Tomohiro; Matsuda, Mitsuyoshi; Kashiwayanagi, Makoto</p> <p>2014-01-01</p> <p>The subventricular <span class="hlt">zone</span> (SVZ) generates an immense number of neurons even during adulthood. These neurons migrate to the olfactory bulb (OB) and differentiate into granule cells and periglomerular cells. The information broadcast by general odorants is received by the olfactory sensory neurons and transmitted to the OB. Recent studies have shown that a reduction of mastication impairs both neurogenesis in the hippocampus and brain functions. To examine these effects, we first measured the difference in Fos-immunoreactivity (Fos-ir) at the principal sensory trigeminal nucleus (Pr5), which receives intraoral touch information via the trigeminal nerve, when female adult mice ingested a hard or soft diet to explore whether soft-diet feeding could mimic impaired mastication. Ingestion of a hard diet induced greater expression of Fos-ir cells at the Pr5 than did a soft diet or no diet. Bromodeoxyuridine-immunoreactive (BrdU-ir) structures in sagittal sections of the SVZ and in the OB of mice fed a soft or hard diet were studied to explore the effects of changes in mastication on newly generated neurons. After 1 month, the density of BrdU-ir cells in the SVZ and OB was lower in the soft-diet-fed mice than in the hard-diet-fed mice. The odor preferences of individual female mice to butyric acid were tested in a Y-maze apparatus. Avoidance of butyric acid was reduced by the soft-diet feeding. We then explored the effects of the hard-diet feeding on olfactory functions and neurogenesis in the SVZ of mice impaired by soft-diet feeding. At 3 months of hard-diet feeding, avoidance of butyric acid was reversed and responses to odors and neurogenesis were <span class="hlt">recovered</span> in the SVZ. The present results suggest that feeding with a hard diet improves neurogenesis in the SVZ, which in turn enhances olfactory function at the OB. PMID:24817277</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMEP13F..02B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMEP13F..02B"><span>Fine <span class="hlt">Sediment</span> Erosion and Transport to the Near Coastal <span class="hlt">Zone</span> from Watersheds of St. Thomas, USVI</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Benoit, G.; Xuan, Z.</p> <p>2014-12-01</p> <p>The US Virgin Islands' landscape is characterized by steep slopes and short distances from ridge peaks to fringing reefs. Fine-grained <span class="hlt">sediments</span> eroded from predominantly thin soils may be transported rapidly by streams (locally called guts) to the sea and cause stress to corals. We have studied erosion and transport processes on St Thomas by three methods: (1) continuous monitoring of suspended matter in one of the island's few perennial streams, Dorothea Gut, (2) measurement of 137Cs inventories in soil cores taken across the landscape, and (3) evaluation of <span class="hlt">sediment</span> captured in most of the island's coastal ponds, through which a significant portion of runoff must pass. We find that, for areas that have not been recently disturbed, watersheds retain fine <span class="hlt">sediments</span> surprisingly well. On the other hand, small patches of land, like building lots that have been recently disturbed and poorly managed, can produce disproportionate amounts of fine <span class="hlt">sediment</span>. These results differ somewhat from nearby St John, USVI, where unpaved roads are the major source of eroded <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H23D1691S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H23D1691S"><span>Mixing-dependent Reactions in the Hyporheic <span class="hlt">Zone</span>: Laboratory and Numerical Experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Santizo, K. Y.; Eastes, L. A.; Hester, E. T.; Widdowson, M.</p> <p>2017-12-01</p> <p>The hyporheic <span class="hlt">zone</span> is the surface water-groundwater interface surrounding the river's perimeter. Prior research demonstrates the ability of the hyporheic <span class="hlt">zone</span> to attenuate pollutants when surface water cycles through reactive <span class="hlt">sediments</span> (non-mixing-dependent reactions). However, the colocation of both surface and ground water within hyporheic <span class="hlt">sediments</span> also allows mixing-dependent reactions that require mixing of reactants from these two water sources. Recent modeling studies show these mixing <span class="hlt">zones</span> can be small under steady state homogeneous conditions, but do not validate those results in the laboratory or explore the range of hydrological characteristics that control the extent of mixing. Our objective was to simulate the mixing <span class="hlt">zone</span>, quantify its thickness, and probe its hydrological controls using a "mix" of laboratory and numerical experiments. For the lab experiments, a hyporheic <span class="hlt">zone</span> was simulated in a sand mesocosm, and a mixing-dependent abiotic reaction of sodium sulfite and dissolved oxygen was induced. Oxygen concentration response and oxygen consumption were visualized via planar optodes. Sulfate production by the mixing-dependent reaction was measured by fluid samples and a spectrophometer. Key hydrologic controls varied in the mesocosm included head gradient driving hyporheic exchange and hydraulic conductivity/heterogeneity. Results show a clear mixing area, sulfate production, and oxygen gradient. Mixing <span class="hlt">zone</span> length (hyporheic flow cell size) and thickness both increase with the driving head gradient. For the numerical experiments, transient surface water boundary conditions were implemented together with heterogeneity of hydraulic conductivity. Results indicate that both fluctuating boundary conditions and heterogeneity increase mixing-dependent reaction. The hyporheic <span class="hlt">zone</span> is deemed an attenuation hotspot by multiple studies, but here we demonstrate its potential for mixing-dependent reactions and the influence of important hydrological</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014369','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014369"><span>The metal oxide fraction of pelagic <span class="hlt">sediment</span> in the equatorial North Pacific Ocean: A source of metals in ferromanganese nodules</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Piper, D.Z.</p> <p>1988-01-01</p> <p>Pelagic <span class="hlt">sediment</span> <span class="hlt">recovered</span> at DOMES Site A in the equatorial North Pacific (151??W, 9?? 15???N) consists of a surface homogeneous layer, approximately 10 cm thick, overlying a strongly mottled layer that is lighter in color. The radiolarian composition of both units is Quaternary. In areas where this <span class="hlt">sediment</span> was only a few centimeters thick, the underlying <span class="hlt">sediment</span> was early Tertiary. Clay mineralogy and major oxide composition of the two Quaternary <span class="hlt">sediments</span> are uniform. Their similarity to continental shale suggests that the <span class="hlt">sediment</span> has a terrigenous source. Clay mineralogy and major oxide composition of the Tertiary <span class="hlt">sediment</span> also are uniform, although they differ markedly from the Quarternary <span class="hlt">sediment</span>. In contrast to the major oxides, concentrations of Mn, Co, Cu, and Ni soluble in hydroxylamine hydrochlorideacetic acid are strongly different in the surface and subsurface Quaternary <span class="hlt">sediment</span>. Mn and Ni exhibit pronounced depletions in the subsurface <span class="hlt">sediment</span>, Ni slightly more than Mn. Cu is also depleted in the subsurface <span class="hlt">sediment</span>, but less than Mn. It is also depleted in the subsurface Tertiary <span class="hlt">sediment</span>, whereas the Mn concentration remains high. Concentration of Co relative to Mn increases into the subsurface Quaternary <span class="hlt">sediment</span> to a constant Co:Mn ratio of 3 ?? 10-2. The trivalent REE (the REE exclusive of Ce) and Fe exhibit little down-core variation. Distribution of elements in these <span class="hlt">sediments</span> is closely related to their concentration in associated surface ferromanganese nodules. The nodules are of two distinct types: those from the area where the Quaternary <span class="hlt">sediment</span> is relatively thick have ??-MnO2 as the dominant manganese mineral. The ratios of Ni:Mn, Cu:Mn, and Fe:Mn in these nodules approximate the corresponding ratios of the soluble fraction of surface <span class="hlt">sediment</span>. Todorokite is the dominant mineral of nodules <span class="hlt">recovered</span> from areas where the Quaternary <span class="hlt">sediment</span> is thin. Relatively high Cu/Mn, Ni/Mn, and low Fe/Mn ratios of these nodules mirror</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012CSR....35..129M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012CSR....35..129M"><span>Arsenic enrichment in shelf and coastal <span class="hlt">sediment</span> of the Brazilian subtropics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mirlean, N.; Medeanic, S.; Garcia, F. A.; Travassos, M. P.; Baisch, P.</p> <p>2012-03-01</p> <p>High levels of As (i.e., above the nationally legislated threshold of 70 mg kg-1) were found in shelf <span class="hlt">sediment</span> of the Espirito Santo state of Brazil. The elevated content of this metalloid propagated in the <span class="hlt">sediment</span> to a depth of approximately 1.5 m. The adjacent beach sands and mangrove <span class="hlt">sediments</span> were also enriched in As. The variation in As levels along the shelf <span class="hlt">sediment</span> profiles was acompained by calcareous-material distribution, which reflects the paleogeographical circumstances that promote local reef development during the corresponding intervals of <span class="hlt">sedimentation</span>. Arsenic-rich calcareous bioclast materials migrate to a beach from the surface horizon of nearby shelf <span class="hlt">sediment</span>, thereby replacing the part of the As that previously entered the marine environment with eroded material from the continent to the littoral <span class="hlt">zone</span>. The segment of the Brazilian tropical shelf that was studied clearly demonstrated that the As enrichment of the shelf <span class="hlt">sediment</span> is determined by the exposure of the Barreiras formation on the coast and the development of reefs, which are favorable sites for the settling of bodies of biogenic carbonates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58.2293H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58.2293H"><span>Distribution, abundance and seasonal flux of pteropods in the Sub-Antarctic <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Howard, W. R.; Roberts, D.; Moy, A. D.; Lindsay, M. C. M.; Hopcroft, R. R.; Trull, T. W.; Bray, S. G.</p> <p>2011-11-01</p> <p>Pteropods were identified from epipelagic net and trawl samples in the Sub-Antarctic <span class="hlt">Zone</span> during the 2007 mid-summer (January 17-February 20) Sub-Antarctic <span class="hlt">Zone</span> Sensitivity to Environmental Change (SAZ-Sense) voyage, as well as in a moored <span class="hlt">sediment</span> trap in the same region. Overall pteropod densities during SAZ-Sense were lower than those reported for higher-latitude Southern Ocean waters. The four major contributors to the Sub-Antarctic <span class="hlt">Zone</span> pteropod community during the SAZ-Sense voyage, Clio pyramidata forma antarctica, Clio recurva, Limacina helicina antarctica and Limacina retroversa australis, accounted for 93% of all pteropods observed. The distribution of the two dominant pteropods collected in the Sub-Antarctic <span class="hlt">Zone</span>, L. retroversa australis and C. pyramidata forma antarctica, is strongly related to latitude and depth. L. retroversa australis is typical of cold southern (50-54°S) polar waters and C. pyramidata forma antarctica is typical of shallow (top 20 m) Sub-Antarctic <span class="hlt">Zone</span> waters. A moored <span class="hlt">sediment</span> trap deployed to 2100 m at 47°S, 141°E in 2003/04 showed the pteropod flux in the Sub-Antarctic <span class="hlt">Zone</span> had late-Spring and mid-summer peaks. The diversity, abundance and distribution of pteropods collected during SAZ-Sense provide a timely benchmark against which to monitor future changes in SAZ ocean pteropod communities, particularly in light of predictions of declining aragonite saturation in the Southern Ocean by the end of the century.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.1987M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.1987M"><span>Catchment-scale environmental controls of <span class="hlt">sediment</span>-associated contaminant dispersal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macklin, Mark</p> <p>2010-05-01</p> <p>Globally river <span class="hlt">sediment</span> associated contaminants, most notably heavy metals, radionuclides, Polychlorinated Biphenyls (PCBs), Organochlorine pesticides (OCs) and phosphorous, constitute one the most significant long-term risks to ecosystems and human health. These can impact both urban and rural areas and, because of their prolonged environmental residence times, are major sources of secondary pollution if contaminated soil and <span class="hlt">sediment</span> are disturbed by human activity or by natural processes such as water or wind erosion. River catchments are also the primary source of <span class="hlt">sediment</span>-associated contaminants to the coastal <span class="hlt">zone</span>, and to the ocean, and an understanding of the factors that control contaminated <span class="hlt">sediment</span> fluxes and delivery in river systems is essential for effective environmental management and protection. In this paper the catchment-scale controls of <span class="hlt">sediment</span>-associated contaminant dispersal are reviewed, including climate-related variations in flooding regime, land-use change, channel engineering, restoration and flood defence. Drawing on case studies from metal mining impacted catchments in Bolivia (Río Pilcomayo), Spain (Río Guadiamar), Romania (River Tisa) and the UK (River Swale) some improved methodologies for identifying, tracing, modelling and managing contaminated river <span class="hlt">sediments</span> are proposed that could have more general application in similarly affected river systems worldwide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS53E1092M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS53E1092M"><span>The Influence of Coastal Wetland Zonation on Surface <span class="hlt">Sediment</span> and Porewater Mercury Speciation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marvin-DiPasquale, M. C.; Windham-Myers, L.; Wilson, A. M.; Buck, T.; Smith, E.</p> <p>2014-12-01</p> <p>An investigation of mercury (Hg) speciation in saltmarsh surface <span class="hlt">sediment</span> (top 0-2 cm) and porewater (integrated 0-50 cm) was conducted along two monitoring well transects established within North Inlet Estuary (S. Carolina, USA) as part of the NOAA sponsored National Estuarine Research Reserve (NERR) network. Transects were perpendicular to the shoreline, from the forested uplands to the edge of the tidal channel, and traversed a range of vegetated <span class="hlt">zones</span> from the high marsh (pickleweed, rush, and salt panne-dominated) to the low marsh (cordgrass dominated), as mediated by elevation and tidal inundation. <span class="hlt">Sediment</span> grain size and organic content explained 95% of the variability in the distribution of total Hg (THg) in surface <span class="hlt">sediment</span>. Tin-reducible 'reactive' mercury (HgR) concentration was 10X greater in the high marsh, compared to the low marsh, and increased sharply with decreasing <span class="hlt">sediment</span> pH values below pH=6. The percentage of THg as HgR decreased as <span class="hlt">sediment</span> redox conditions became more reducing. There were no significant differences in surface <span class="hlt">sediment</span> methylmercury (MeHg) concentrations between high and low marsh <span class="hlt">zones</span>. In contrast, porewater MeHg concentrations were 5X greater in the high marsh compared to the low marsh. As a percentage of THg, mean porewater %MeHg was 23% in the low marsh and 51% in the high marsh, reaching levels of 73-89% in a number of high marsh sites. Calculations of partitioning between porewater and the solid phase suggest stronger binding to particles in the low marsh and a shift towards the dissolved phase in the high marsh for both THg and MeHg. These results are consistent with a conceptual model for coastal wetlands where the less frequently inundated high marsh <span class="hlt">zone</span> may be important in terms of MeHg production and enhanced subsurface mobilization, partially due to the subsurface mixing of saline estuarine water and freshwater draining in from the uplands area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17111606','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17111606"><span>[Evaluating comprehensive quality of <span class="hlt">sediment</span> in Dianchi Lake using adjusted AHP method and 137Cs dating].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Yan; Deng, Xi-Hai; Peng, Bu-Zhuo</p> <p>2006-08-01</p> <p>It is difficult to evaluate comprehensive quality of <span class="hlt">sediment</span> and to understand development trend of pollution because of absence of monitoring data, especially history data. Combining the method of 137Cs dating with the ways of general sampling and measurement can easily resolve the problem of absence of data and also provide the possibility for calculating weighted environmental quality comprehensive index using the adjusted analytical hierarchy process (AHP) method. In order to overcome the willfulness the judgment matrix is formed objectively based on calculating monitoring data. Based on the monitoring data of <span class="hlt">sediment</span> pollution and the weights of various factors gained by adjusted AHP method the comprehensive quality of <span class="hlt">sediment</span> in each <span class="hlt">zone</span> of Dianchi Lake was evaluated and the results indicated that the pollution of <span class="hlt">sediments</span> in each <span class="hlt">zone</span> at the present be serious more than that in the history. The condition may be related to the industrial development and distribution of industries in Dianchi Lake basin. Therefore, in order to improve the comprehensive quality of <span class="hlt">sediment</span> in Dianchi Lake and to prevent the secondary pollution of heavy metals in <span class="hlt">sediment</span> from happening, it is necessary to control the pollutants discharge and to remove the pollutants with various ways.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15633038','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15633038"><span>Using <span class="hlt">sediment</span> budgets to investigate the pathogen flux through catchments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Whiteway, Tanya G; Laffan, Shawn W; Wasson, Robert J</p> <p>2004-10-01</p> <p>We demonstrate a materials budget approach to identify the main source areas and fluxes of pathogens through a landscape by using the flux of fine <span class="hlt">sediments</span> as a proxyfor pathogens. <span class="hlt">Sediment</span> budgets were created for three subcatchment tributaries of the Googong Reservoir in south-eastern New South Wales, Australia. Major inputs, sources, stores, and transport <span class="hlt">zones</span> were estimated using <span class="hlt">sediment</span> sampling, dam trap efficiency measures, and radionuclide tracing. Particle size analyses were used to quantify the fine-<span class="hlt">sediment</span> component of the total <span class="hlt">sediment</span> flux, from which the pathogen flux was inferred by considering the differences between the mobility and transportation of fine <span class="hlt">sediments</span> and pathogens. Gullies were identified as important sources of fine <span class="hlt">sediment</span>, and therefore of pathogens, with the pathogen risk compounded when cattle shelter in them during wet periods. The results also indicate that the degree of landscape modification influences both <span class="hlt">sediment</span> and pathogen mobilization. Farm dams, swampy meadows and glades along drainage paths lower the flux of fine <span class="hlt">sediment</span>, and therefore pathogens, in this landscape during low-flow periods. However, high-rainfall and high-flow events are likely to transport most of the fine <span class="hlt">sediment</span>, and therefore pathogen, flux from the Googong landscape to the reservoir. Materials budgets are a repeatable and comparatively low-cost method for investigating the pathogen flux through a landscape.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982Natur.297..139C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982Natur.297..139C"><span>Evolution of passive continental margins and initiation of subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cloetingh, S. A. P. L.; Wortel, M. J. R.; Vlaar, N. J.</p> <p>1982-05-01</p> <p>Although the initiation of subduction is a key element in plate tectonic schemes for evolution of lithospheric plates, the underlying mechanisms are not well understood. Plate rupture is an important aspect of the process of creating a new subduction <span class="hlt">zone</span>, as stresses of the order of kilobars are required to fracture oceanic lithosphere1. Therefore initiation of subduction could take place preferentially at pre-existing weakness <span class="hlt">zones</span> or in regions where the lithosphere is prestressed. As such, transform faults2,3 and passive margins4,5 where the lithosphere is downflexed under the influence of <span class="hlt">sediment</span> loading have been suggested. From a model study of passive margin evolution we found that ageing of passive margins alone does not make them more suitable sites for initiation of subduction. However, extensive <span class="hlt">sediment</span> loading on young lithosphere might be an effective mechanism for closure of small ocean basins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15092460','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15092460"><span>Organo-tins in <span class="hlt">sediments</span> and mussels from the Sado estuarine system (Portugal).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Quevauviller, P; Lavigne, R; Pinel, R; Astruc, M</p> <p>1989-01-01</p> <p>Analyses of methyl- and butyl-tin levels in freshwater, estuarine and marine <span class="hlt">sediments</span> from the Sado estuarine system, and in mussels (Mytilus galloprovincialis) from its adjacent coast, have been performed in order to detect the contaminated areas. The main inputs of tributyl-tin (TBT), along with degradation products di- and monobutyl-tin (DBT and MBT), were detected in the estuarine <span class="hlt">zone</span>, due to high discharge from shipyards located in this area. These levels are sometimes very high, ranging from 235 to 12,200 ng g(-1) total butyl-tins in <span class="hlt">sediments</span>. Such inputs lead to higher bioconcentration values in mussels in the estuarine <span class="hlt">zone</span>, as well as in a harbour located along the adjacent coast. The bioconcentration of organo-tins in mussel tissues could be enhanced in estuarine turbid waters, due to an ingestion of butyl-tins adsorbed onto fine particles, in comparison with non-turbid coastal waters. Debutylation processes occur in both <span class="hlt">sediments</span> and mussel tissues; in organisms, these processes may lead to the formation of inorganic tin, which may be methylated differently according to the period of the year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=194920','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=194920"><span>Differences in Hyporheic-<span class="hlt">Zone</span> Microbial Community Structure along a Heavy-Metal Contamination Gradient</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Feris, Kevin; Ramsey, Philip; Frazar, Chris; Moore, Johnnie N.; Gannon, James E.; Holben, William E.</p> <p>2003-01-01</p> <p>The hyporheic <span class="hlt">zone</span> of a river is nonphotic, has steep chemical and redox gradients, and has a heterotrophic food web based on the consumption of organic carbon entrained from downwelling surface water or from upwelling groundwater. The microbial communities in the hyporheic <span class="hlt">zone</span> are an important component of these heterotrophic food webs and perform essential functions in lotic ecosystems. Using a suite of methods (denaturing gradient gel electrophoresis, 16S rRNA phylogeny, phospholipid fatty acid analysis, direct microscopic enumeration, and quantitative PCR), we compared the microbial communities inhabiting the hyporheic <span class="hlt">zone</span> of six different river sites that encompass a wide range of <span class="hlt">sediment</span> metal loads resulting from large base-metal mining activity in the region. There was no correlation between <span class="hlt">sediment</span> metal content and the total hyporheic microbial biomass present within each site. However, microbial community structure showed a significant linear relationship with the <span class="hlt">sediment</span> metal loads. The abundances of four phylogenetic groups (groups I, II, III, and IV) most closely related to α-, β-, and γ-proteobacteria and the cyanobacteria, respectively, were determined. The <span class="hlt">sediment</span> metal content gradient was positively correlated with group III abundance and negatively correlated with group II abundance. No correlation was apparent with regard to group I or IV abundance. This is the first documentation of a relationship between fluvially deposited heavy-metal contamination and hyporheic microbial community structure. The information presented here may be useful in predicting long-term effects of heavy-metal contamination in streams and provides a basis for further studies of metal effects on hyporheic microbial communities. PMID:12957946</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.S51C2228S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.S51C2228S"><span>Soft-<span class="hlt">sediment</span> deformation in New Zealand: Structures resulting from the 2010/11 Christchurch earthquakes and comparison with Pleistocene <span class="hlt">sediments</span> of the Taupo Volcanic <span class="hlt">Zone</span> (TVZ)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Scholz, C.; Downs, D. T.; Gravley, D.; Quigley, M.; Rowland, J. V.</p> <p>2011-12-01</p> <p>The distinction between seismites and other event-related soft-<span class="hlt">sediment</span> deformation is a challenging problem. Recognition and interpretation is aided by comparison of recent examples produced during known seismic events and those generated experimentally. Seismites are important features, once recognized in a rock, for interpretations of paleotectonic environment, tectonic relationships of <span class="hlt">sediments</span> in basins, sedimentary facies analysis, evaluation of earthquake frequency and hazard and consequent land managment. Two examples of soft-<span class="hlt">sediment</span> deformation, potentially generated through ground shaking and associated liquefaction, are described from within the TVZ: 1) Near Matata on the western margin of the Whakatane Graben. This location has a complicated en-echelon fault history and large earthquakes occur from time to time (e.g., 1987 ML6.3 Edgecumbe event). The structures occur in ~550 ka volcanic <span class="hlt">sediments</span>, and represent soft-<span class="hlt">sediment</span> deformation within stratigraphically-bounded layers. Based on paleoenvironment, appearance, and diagnostic criteria described by other authors (Sims 1975; Hempton and Dewey 1983), we interpret these features to have formed by ground shaking related to an earthquake and/or possibly accompanying large volcanic eruptions, rather than by slope failure. 2) Near Taupo, 3 km from the active Kaiapo fault. Lakeward dipping, nearly horizontal lacustrine <span class="hlt">sediments</span> overlay Taupo Ignimbrite (1.8 ka). At one outcrop the lake beds have subsided into the underlying substrate resulting in kidney-shaped features. These structures formed as a result of liquefaction of the underlying substrate, which may have been caused by ground shaking related to either seismic or volcanic activity. However, inferred time relationships are more consistent with seismic-induced ground shaking. We compare and contrast the form and geometry of the above structures with seismites generated during the recent Christchurch earthquakes (Sep. 2010 and Feb. 2011). Hempton, M</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27485799','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27485799"><span>Pollution status of polycyclic aromatic hydrocarbons in surface <span class="hlt">sediments</span> from the Yangtze River Estuary and its adjacent coastal <span class="hlt">zone</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Chenglong; Zou, Xinqing; Gao, Jianhua; Zhao, Yifei; Yu, Wenwen; Li, Yali; Song, Qiaochu</p> <p>2016-11-01</p> <p>Polycyclic aromatic hydrocarbons (PAHs) are mainly produced by incomplete combustion and are used as indicators of anthropogenic activities on the environment. This study analyses the PAHs level in the Yangtze River Estuary (YRE), an important component of Yangtze River and a developed and populated region in China. Surface <span class="hlt">sediments</span> were collected from 77 sites at the YRE and its adjacent coastal <span class="hlt">zone</span> (IACZ) for a comprehensive study of PAHs. Kriging interpolation technology and Positive matrix factorization (PMF) model were applied to explore the spatial distribution and sources of PAHs. Concentrations of 16 PAHs (ΣPAHs) varied from 27.2 ng g(-1) to 621.6 ng g(-1) dry weight, with an average value of 158.2 ng g(-1). Spatially, ΣPAHs exhibited wide fluctuation and exhibited an increasing tendency from north to south. In addition, ΣPAHs exhibited a decreasing trend with increasing distance between the estuary and IACZ. The deposition flux of PAHs indicated that more than 107.8 t a(-1) PAHs was deposited in the study area annually. The results of the PMF model revealed that anthropogenic activities were the main sources of PAHs in the study area. Vehicle emissions and marine engines were the most important sources and accounted for 40.9% of the pollution. Coal combustion, petrogenic sources, and wood combustion were other sources that contributed 23.9%, 23.6%, and 11.5%, respectively. The distribution patterns of PAHs in the YRE and IACZ were influenced by many complicated factors such as <span class="hlt">sediment</span> grain size, hydrodynamics and so on. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Geomo.232..182Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Geomo.232..182Y"><span>Morphology, spatial pattern and <span class="hlt">sediment</span> of Nitraria tangutorum nebkhas in barchans interdune areas at the southeast margin of the Badain Jaran Desert, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, YanYan; Liu, LianYou; Shi, PeiJun; Zhang, GuoMing; Qu, ZhiQiang; Tang, Yan; Lei, Jie; Wen, HaiMing; Xiong, YiYing; Wang, JingPu; Shen, LingLing</p> <p>2015-03-01</p> <p>To understand the characteristics of the nebkhas in barchan interdune areas, isolated barchan dunes at the southeast margin of the Badain Jaran Desert in China and Nitraria tangutorun nebkhas in the interdune areas were selected, and the morphometric parameters, spatial patterns, and granulometric characteristics of the nebkhas in various interdune <span class="hlt">zones</span> were compared. According to the locations relative to barchan dunes, the interdune areas were divided into three <span class="hlt">zones</span>: the windward interdune <span class="hlt">zone</span> (Zw), the leeward interdune <span class="hlt">zone</span> (Zl), and the horn interdune <span class="hlt">zone</span> (Zh). The <span class="hlt">zone</span> that is proximal to barchan dunes and has never been disturbed by barchan dunes was also selected (Zi). The morphometric parameters were measured through a satellite image and field investigation. The population density and spatial patterns were analyzed using the satellite image, and surface <span class="hlt">sediment</span> samples of the nebkhas and barchan dunes were collected for grain size analysis. The morphometric parameters of Nitraria tangutorun nebkhas in the interdune <span class="hlt">zones</span> differ significantly. The nebkhas in Zh are larger than those observed in the other <span class="hlt">zones</span>, and the nebkhas are the smallest in Zl. In all of the <span class="hlt">zones</span>, the long-axis orientation of the nebkhas is perpendicular to the prevailing wind direction. The population density of the nebkhas in Zw is relatively higher, whereas the density in Zh and Zl becomes obviously lower. The spatial distribution of nebkhas in all of the <span class="hlt">zones</span> can be categorized as a dispersed pattern. The <span class="hlt">sediments</span> of the nebkhas are coarsest in Zh and finest in Zl. In addition, the <span class="hlt">sediments</span> of the nebkhas in all of the <span class="hlt">zones</span> are finer than those of barchan dunes. The amount of sand captured by the nebkhas in the interdune areas is approximately 20% of the volume of barchan dunes. The variations of the nebkhas' sizes, spatial pattern and <span class="hlt">sediment</span> are subjected to migration, flow field and sand transport of barchan dunes and sand accumulation with plant growth in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3597252','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3597252"><span>Increased freshwater discharge shifts the trophic balance in the coastal <span class="hlt">zone</span> of the northern Baltic Sea</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wikner, Johan; Andersson, Agneta</p> <p>2012-01-01</p> <p>Increased precipitation is one projected outcome of climate change that may enhance the discharge of freshwater to the coastal <span class="hlt">zone</span>. The resulting lower salinity, and associated discharge of both nutrients and dissolved organic carbon, may influence food web functioning. The scope of this study was to determine the net outcome of increased freshwater discharge on the balance between auto- and heterotrophic processes in the coastal <span class="hlt">zone</span>. By using long-term ecological time series data covering 13 years, we show that increased river discharge suppresses phytoplankton biomass production and shifts the carbon flow towards microbial heterotrophy. A 76% increase in freshwater discharge resulted in a 2.2 times higher ratio of bacterio- to phytoplankton production (Pb:Pp). The level of Pb:Pp is a function of riverine total organic carbon supply to the coastal <span class="hlt">zone</span>. This is mainly due to the negative effect of freshwater and total organic carbon discharge on phytoplankton growth, despite a concomitant increase in discharge of nitrogen and phosphorus. With a time lag of 2 years the bacterial production <span class="hlt">recovered</span> after an initial decline, further synergistically elevating the microbial heterotrophy. Current climate change projections suggesting increased precipitation may therefore lead to increased microbial heterotrophy, thereby decreasing the transfer efficiency of biomass to higher trophic levels. This prognosis would suggest reduced fish production and lower <span class="hlt">sedimentation</span> rates of phytoplankton, a factor of detriment to benthic fauna. Our findings show that discharge of freshwater and total organic carbon significantly contributes to the balance of coastal processes at large spatial and temporal scales, and that model's would be greatly augmented by the inclusion of these environmental drivers as regulators of coastal productivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA233120','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA233120"><span>Physical Properties and Microstructural Response of <span class="hlt">Sediments</span> to Accretion-Subduction: Barbados Forearc</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1991-01-01</p> <p>of major and minor stress directions ik associated with 40-m-thick <span class="hlt">zone</span>. The bedding-subparallel fabric results in accretion (Moran and Christian , 1990...Carson, B., and T.R. Bruns, 1980. Physical properties of <span class="hlt">sediments</span> from the Moran, K., and H.A. Christian , 1990. Strength and deformation behavior of...Geotechnical properties of lower Cowan, D.S., J.C. Moore, S.M. Roeske , N. Lundberg, and S.E. Lucas, 1984. trench inner slope <span class="hlt">sediments</span>. Tectonophysics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://pubs.usgs.gov/of/2016/1119/index.html','USGSPUBS'); return false;" href="http://pubs.usgs.gov/of/2016/1119/index.html"><span>Shallow geology, sea-floor texture, and physiographic <span class="hlt">zones</span> of Vineyard and western Nantucket Sounds, Massachusetts</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Baldwin, Wayne E.; Foster, David S.; Pendleton, Elizabeth A.; Barnhardt, Walter A.; Schwab, William C.; Andrews, Brian D.; Ackerman, Seth D.</p> <p>2016-09-02</p> <p>Geologic, <span class="hlt">sediment</span> texture, and physiographic <span class="hlt">zone</span> maps characterize the sea floor of Vineyard and western Nantucket Sounds, Massachusetts. These maps were derived from interpretations of seismic-reflection profiles, high-resolution bathymetry, acoustic-backscatter intensity, bottom photographs/video, and surficial <span class="hlt">sediment</span> samples collected within the 494-square-kilometer study area. Interpretations of seismic stratigraphy and mapping of glacial and Holocene marine units provided a foundation on which the surficial maps were created. This mapping is a result of a collaborative effort between the U.S. Geological Survey and the Massachusetts Office of Coastal <span class="hlt">Zone</span> Management to characterize the surface and subsurface geologic framework offshore of Massachusetts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.3283H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.3283H"><span>Sedimentary record of relay <span class="hlt">zone</span> evolution, Central Corinth Rift (Greece): Role of fault propagation and structural inheritance.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hemelsdaël, Romain; Ford, Mary; Meyer, Nicolas</p> <p>2013-04-01</p> <p>Relay <span class="hlt">zones</span> along rift border fault systems form topographic lows that are considered to allow the transfer of <span class="hlt">sediment</span> from the footwall into hanging wall depocentres. Present knowledge focuses on the modifications of drainage patterns and <span class="hlt">sediment</span> pathways across relay <span class="hlt">zones</span>, however their vertical motion during growth and interaction of faults segments is not well documented. 3D models of fault growth and linkage are also under debate. The Corinth rift (Greece) is an ideal natural laboratory for the study of fault system evolution. Fault activity and rift depocentres migrated northward during Pliocene to Recent N-S extension. We report on the evolution of a relay <span class="hlt">zone</span> in the currently active southern rift margin fault system from Pleistocene to present-day. The relay <span class="hlt">zone</span> lies between the E-W East Helike (EHF) and Derveni faults (DF) that lie just offshore and around the town of Akrata. During its evolution the relay <span class="hlt">zone</span> captured the antecedent Krathis river which continued to deposit Gilbert-type deltas across the relay <span class="hlt">zone</span> during fault interaction, breaching and post linkage phases. Moreover our work underlines the role that pre-existing structure in the location of the transfer <span class="hlt">zone</span>. Offshore fault geometry and kinematics, and <span class="hlt">sediment</span> distribution were defined by interpretation and depth conversion of high resolution seismic profiles (from Maurice Ewing 2001 geophysical survey). Early lateral propagation of the EHF is recorded by synsedimentary fault propagation folds while the DF records tilted block geometries since initiation. Within the relay <span class="hlt">zone</span> beds are gradually tilted toward the basin before breaching. These different styles of deformation highlight mechanical contrasts and upper crustal partition associated with the development of the Akrata relay <span class="hlt">zone</span>. Onshore detailed lithostratigraphy, structure and geomorphological features record <span class="hlt">sedimentation</span> across the subsiding relay ramp and subsequent footwall uplift after breaching. The area is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JGRB..114.7401S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRB..114.7401S"><span>Pore pressure development beneath the décollement at the Nankai subduction <span class="hlt">zone</span>: Implications for plate boundary fault strength and <span class="hlt">sediment</span> dewatering</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Skarbek, Robert M.; Saffer, Demian M.</p> <p>2009-07-01</p> <p>Despite its importance for plate boundary fault processes, quantitative constraints on pore pressure are rare, especially within fault <span class="hlt">zones</span>. Here, we combine laboratory permeability measurements from core samples with a model of loading and pore pressure diffusion to investigate pore fluid pressure evolution within underthrust <span class="hlt">sediment</span> at the Nankai subduction <span class="hlt">zone</span>. Independent estimates of pore pressure to ˜20 km from the trench, combined with permeability measurements conducted over a wide range of effective stresses and porosities, allow us to reliably simulate pore pressure development to greater depths than in previous studies and to directly quantify pore pressure within the plate boundary fault <span class="hlt">zone</span> itself, which acts as the upper boundary of the underthrusting section. Our results suggest that the time-averaged excess pore pressure (P*) along the décollement ranges from 1.7-2.1 MPa at the trench to 30.2-35.9 MPa by 40 km landward, corresponding to pore pressure ratios of λb = 0.68-0.77. For friction coefficients of 0.30-0.40, the resulting shear strength along the décollement remains <12 MPa over this region. When noncohesive critical taper theory is applied using these values, the required pore pressure ratios within the wedge are near hydrostatic (λw = 0.41-0.59), implying either that pore pressure throughout the wedge is low or that the fault slips only during transient pulses of elevated pore pressure. In addition, simulated downward migration of minima in effective stress during drainage provides a quantitative explanation for down stepping of the décollement that is consistent with observations at Nankai.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T11D4607I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T11D4607I"><span>Uemachi flexure <span class="hlt">zone</span> investigated by borehole database and numeical simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Inoue, N.; Kitada, N.; Takemura, K.</p> <p>2014-12-01</p> <p>The Uemachi fault <span class="hlt">zone</span> extending north and south, locates in the center of the Osaka City, in Japan. The Uemachi fault is a blind reverse fault and forms the flexure <span class="hlt">zone</span>. The effects of the Uemachi flexure <span class="hlt">zone</span> are considered in constructing of lifelines and buildings. In this region, the geomorphological survey is difficult because of the regression of transgression. Many organizations have carried out investigations of fault structures. Various surveys have been conducted, such as seismic reflection survey in and around Osaka. Many borehole data for construction conformations have been collected and the geotechnical borehole database has been constructed. The investigation with several geological borehole data provides the subsurface geological information to the geotechnical borehole database. Various numerical simulations have been carried out to investigate the growth of a blind reverse fault in unconsolidated <span class="hlt">sediments</span>. The displacement of the basement was given in two ways. One is based on the fault movement, such as dislocation model, the other is a movement of basement block of hanging wall. The Drucker-Prager and elastic model were used for the <span class="hlt">sediment</span> and basement, respectively. The simulation with low and high angle fault movements, show the good agree with the actual distribution of the marine clay inferred from borehole data in the northern and southern Uemachi fault flexure <span class="hlt">zone</span>, respectively. This research is partly funded by the Comprehensive Research on the Uemachi Fault <span class="hlt">Zone</span> (from FY2010 to FY2012) by The Ministry of Education, Culture, Sports, Science and Technology (MEXT).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26841598','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26841598"><span>[Exchange Fluxes and Coupling Relationship of Dissolved Inorganic Carbon and Dissolved Organic Carbon Across the Water-<span class="hlt">Sediment</span> Interface in Lakes].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Wei-ying; Lü, Chang-wei; He, Jiang; Zuo, Le; Yan, Dao-hao</p> <p>2015-10-01</p> <p>In this work, the exchange fluxes and coupling relationship of dissolved inorganic carbon (DIC) and dissolved organic carbon (DOC) were investigated across the water-<span class="hlt">sediment</span> interface in Lake Wuliangsuhai and Daihai by employing columnar simulation method. The results showed that the <span class="hlt">sediments</span> in non-Phragmitescommunis area from Lake Wuliangsuhai functioned as the sources of DIC and DOC for overlying water, whereas the <span class="hlt">sediments</span> from Lake Daihai as the sinks during the period of summer (90 days). In the experimental period, the average exchange rates of DIC and DOC were 71.07 mmol x (m2 x d)(-1) and 185.09 mmol x (m2 x d)(-1) in non-Phragmitescommunis area from Lake Wuliangsuhai, respectively; while in Lake Daihai, they were 155.75 mmol x (m2 x d)(-1) and -1478.08 mmol x (m2 x d)(-1) in shoal water <span class="hlt">zone</span>, and -486.53 mmol x (m2 x d)(-1) and -1274.02 mmol x (m2 x d)(-1) in deep water <span class="hlt">zone</span>, respectively. The coupling effects between DIC and DOC were governed by hydrobios, microbial uptake, abiotic and microbiological degradation in Lake Wuliangsuhai and in shoal water <span class="hlt">zone</span> of Lake Daihai; while they were closely related to the coprecipitation process of CaCO3 and the fraction distribution of inorganic carbon in <span class="hlt">sediments</span> in deep water <span class="hlt">zone</span> of Lake Daihai. In summary, the sink or source functions of <span class="hlt">sediments</span> could be considered as the results of synthetic action of lake types, offshore distance, geohydrochemistry and the fraction distribution of inorganic carbon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4693K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4693K"><span>Characterisation of organic matter source and <span class="hlt">sediment</span> distribution in Ashtamudi Estuary, southern India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Prem; Ankit, Yadav; Mishra, Praveen K.; Jha, Deepak Kumar; Anoop, Ambili</p> <p>2017-04-01</p> <p>In the present study we have focussed on the surface <span class="hlt">sediments</span> of Ashtamudi Estuary (southern India) to understand (i) the fate and sources of organic matter by investigating lipid biomarker (n-alkanes) distribution in modern <span class="hlt">sediments</span> and vegetation samples and (ii) the processes controlling the <span class="hlt">sediment</span> distribution into the lake basin using end-member modelling approach. The <span class="hlt">sediment</span> n-alkanes from the Ashtamudi Estuary exhibit a pronounced odd over even predominance with maxima at C29 and C31 chain length indicative of a dominant terrestrial contribution. A number of n-alkane indices have been calculated to illustrate the variability in space by considering separately the river dominated northern reaches and tidal influenced southern part of Ashtamudi Estuary. The highest terrigenous organic contents were found in <span class="hlt">sediments</span> from the river and upper bay sites, with smaller contributions to the lower parts of the estuary. The Paq and TAR (terrigenous/aquatic ratio) indices demonstrate maximum aquatic productivity (plankton growth and submerged macrophytes) in the tidal dominated region of the Ashtamudi Estuary. The carbon preference index (CPI) and average chain length (ACL) provide evidence for high petrogenic organic inputs in the tidal <span class="hlt">zone</span>, whereas dominant biogenic contribution have been observed in the riverine <span class="hlt">zone</span>. In addition, the end member modeling of the grain size distribution of the surface <span class="hlt">sediment</span> samples enabled us to decipher significant sedimentological processes affecting the <span class="hlt">sediment</span> distribution in the estuarine settings. The end-member distribution showing highest loading with the coarser fraction is maximum where estuary debouches into the sea. However, the samples near the mouth of the river shows finer fraction of the end-member.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814441W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814441W"><span>Environmental change at the southern Cape coast of South Africa as inferred from a high-resolution Holocene <span class="hlt">sediment</span> record from Eilandvlei</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wündsch, Michael; Haberzettl, Torsten; Meadows, Michael E.; Kirsten, Kelly L.; Meschner, Stephanie; Frenzel, Peter; Baade, Jussi; Daut, Gerhard; Mäusbacher, Roland; Kasper, Thomas; Quick, Lynne J.; Cawthra, Hayley C.; Zabel, Matthias</p> <p>2016-04-01</p> <p>The RAIN project (Regional Archives for Integrated iNvestigations), funded by the German Federal Ministry of Education and Research (BMBF), focuses on closely integrated investigations of terrestrial and marine geoarchives from southern Africa in order to assess environmental changes during the late Quaternary. For this purpose, various marine and terrestrial <span class="hlt">sediment</span> records from the three major rainfall <span class="hlt">zones</span> of South Africa (winter-, summer- and year-round rainfall <span class="hlt">zone</span>) were <span class="hlt">recovered</span> and analysed applying a wide range of methods (e.g., sedimentology, seismic stratigraphy, geochronology, organic and inorganic geochemistry, mineralogy, stable isotopes, micropalaeontology, palynology). In this contribution, we present results and interpretations obtained from a 30.5 m <span class="hlt">sediment</span> core retrieved from the coastal lake Eilandvlei located within the year-round rainfall <span class="hlt">zone</span>. Geochemical investigations (Ca, Sr, total inorganic carbon) indicate major changes in the <span class="hlt">sediment</span> carbonate contents which were linked to variations in the marine influence received at the site throughout the covered period. The interpretation of carbonates reflecting a varying marine influence is corroborated by micropalaeontological analyses (viz. ostracod and diatom assemblages) which reveal strong similarities with the geochemical data. In order to establish a reliable radiocarbon (14C) chronology for this record, it is of particular importance to consider the impact of 14C-depleted ("old") marine carbon contained in the measured samples causing reservoir effects. Therefore, two marine molluscan shells collected alive before AD 1950 ("pre-bomb") were analysed to determine the regional marine reservoir offset (ΔR). The obtained ΔR values of 134 ± 38 and 161 ± 38 14C yrs represent the first data available for the south coast of South Africa. However, the application of the resulting average ΔR = 148 ± 54 14C yrs for the calibration of the entire Eilandvlei record underestimates the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27582314','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27582314"><span>The Interplay between Carbon Availability and Growth in Different <span class="hlt">Zones</span> of the Growing Maize Leaf.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Czedik-Eysenberg, Angelika; Arrivault, Stéphanie; Lohse, Marc A; Feil, Regina; Krohn, Nicole; Encke, Beatrice; Nunes-Nesi, Adriano; Fernie, Alisdair R; Lunn, John E; Sulpice, Ronan; Stitt, Mark</p> <p>2016-10-01</p> <p>Plants assimilate carbon in their photosynthetic tissues in the light. However, carbon is required during the night and in nonphotosynthetic organs. It is therefore essential that plants manage their carbon resources spatially and temporally and coordinate growth with carbon availability. In growing maize (Zea mays) leaf blades, a defined developmental gradient facilitates analyses in the cell division, elongation, and mature <span class="hlt">zones</span>. We investigated the responses of the metabolome and transcriptome and polysome loading, as a qualitative proxy for protein synthesis, at dusk, dawn, and 6, 14, and 24 h into an extended night, and tracked whole-leaf elongation over this time course. Starch and sugars are depleted by dawn in the mature <span class="hlt">zone</span>, but only after an extension of the night in the elongation and division <span class="hlt">zones</span>. Sucrose (Suc) <span class="hlt">recovers</span> partially between 14 and 24 h into the extended night in the growth <span class="hlt">zones</span>, but not the mature <span class="hlt">zone</span>. The global metabolome and transcriptome track these <span class="hlt">zone</span>-specific changes in Suc. Leaf elongation and polysome loading in the growth <span class="hlt">zones</span> also remain high at dawn, decrease between 6 and 14 h into the extended night, and then partially <span class="hlt">recover</span>, indicating that growth processes are determined by local carbon status. The level of Suc-signaling metabolite trehalose-6-phosphate, and the trehalose-6-phosphate:Suc ratio are much higher in growth than mature <span class="hlt">zones</span> at dusk and dawn but fall in the extended night. Candidate genes were identified by searching for transcripts that show characteristic temporal response patterns or contrasting responses to carbon starvation in growth and mature <span class="hlt">zones</span>. © 2016 American Society of Plant Biologists. All Rights Reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/27967','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/27967"><span>Recovery of the Chaparral Riparian <span class="hlt">Zone</span> After Wildfire</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Frank W. Davis; Edward A. Keller; Anuja Parikh; Joan Florsheim</p> <p>1989-01-01</p> <p>After the Wheeler Fire in southern California in July 1985, we monitored <span class="hlt">sediment</span> deposition and vegetation recovery in a section of the severely burned chaparral riparian <span class="hlt">zone</span> of the North Fork of Matilija Creek, near Ojai, California. Increased runoff was accompanied by low magnitude debris flows and fluvial transport of gravel, most of which was added to the channel...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www-odp.tamu.edu/publications/204_SR/VOLUME/CHAPTERS/119.PDF','USGSPUBS'); return false;" href="http://www-odp.tamu.edu/publications/204_SR/VOLUME/CHAPTERS/119.PDF"><span>Physical properties of pressurized <span class="hlt">sediment</span> from hydrate ridge</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Winters, William J.; Waite, William F.; Mason, David H.; Gilbert, Lauren</p> <p>2006-01-01</p> <p>As part of an ongoing laboratory study, preliminary acoustic, triaxial strength, and electrical resistivity results are presented from a test performed on a clayey silt <span class="hlt">sediment</span> sample <span class="hlt">recovered</span> from Site 1249 at the summit of southern Hydrate Ridge during Ocean Drilling Program Leg 204. The test specimen was stored and transported in two different methane-charged pressure vessels until it was tested using the Gas Hydrate and <span class="hlt">Sediment</span> Test Laboratory Instrument (GHASTLI). Although gas hydrate may have existed in the core section immediately after recovery, little (if any) hydrate was present in the specimen during testing. We therefore present background physical property results for <span class="hlt">sediment</span> that may have hosted gas hydrate in situ. Because we consolidated the test specimen in increments beyond its in situ stress state, we are able to present properties representative of similar but deeper subbottom <span class="hlt">sediment</span>. The increased consolidation stress also helped to mitigate some, but not all, types of disturbance caused by the recovery process. P-wave velocities from 1.54 to 1.74 km/s varied linearly with consolidation stress, σ′c, up to 970 kPa (equivalent to ~160 meters below seafloor). Electrical resistivity was periodically measured by a Wenner array and varied between 1.0 and 2.8 Ωm. These values reflect both the pore water salinity and soft, fine-grained texture of the <span class="hlt">sediment</span>. Shear behavior is consistent with the induced normally consolidated behavior of clayey silt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S41C0788K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S41C0788K"><span>Experimental Investigation on Poro-Elasto-Plastic Behavior of the Inner Accretionary Wedge <span class="hlt">Sediments</span> at the Nankai Subduction <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuo, S. T.; Kitamura, M.; Kitajima, H.</p> <p>2017-12-01</p> <p>The Integrated Ocean Drilling Program (IODP) Nankai Trough Seismogenic <span class="hlt">Zone</span> Experiment (NanTroSEIZE) have installed borehole observatories to monitor the evolution of physical and hydrological properties caused by crustal deformation at various strain rates within earthquake cycles. The observatories have been installed at the base of a forearc basin above the megathrust fault (Site C0002) and near the shallow tip of the megasplay fault (Site C0010), and will be installed near the frontal thrust (Site C0006) next year. The observatory pore pressure data have shown the dynamic and post-seismic responses and are used to estimate volumetric strain (deformation) with poroelastic parameters (e.g., Wallace et al. 2016). The parameters of submarine <span class="hlt">sediments</span> are often computed theoretically from the porosity, compressibilities of matrix, solid, and pore fluid; however, few direct constraints on core samples have been made. To investigate the poro-elasto-plastic behavior of submarine <span class="hlt">sediments</span>, triaxial experiments with stress relaxation were conducted on the claystone cores (20% porosity) from 2185 meters below sea floor at Site C0002. Triaxial tests were conducted by applying an axial load at a constant displacement rate of 5×10-9m/s, while keeping confining pressure (Pc) at 42, 48, or 78 MPa and pore pressure (Pp) at 20 MPa. Stress relaxation tests were conducted periodically, in which neither axial displacement nor pore volume change was allowed. At lower effective pressure (Pe=Pc-Pp) of 22 and 28 MPa, the samples deform in a brittle manner, with a peak strength of 50 and 55 MPa and a residual strength of 36 and 46 MPa, respectively. At higher Pe of 58 MPa, the sample exhibits strain hardening. The relaxation tests at Pe = 22 MPa show an increase in Pp before yield and a decrease in Pp after yield, suggesting a transition from compaction to dilation. All of the relaxation tests at Pe = 58 MPa show an increase in Pp, suggesting compaction throughout the deformation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Geomo.277..210L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Geomo.277..210L"><span><span class="hlt">Sediment</span> export, transient landscape response and catchment-scale connectivity following rapid climate warming and Alpine glacier recession</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lane, Stuart N.; Bakker, Maarten; Gabbud, Chrystelle; Micheletti, Natan; Saugy, Jean-Noël</p> <p>2017-01-01</p> <p>In the face of rapid climate warming, rapid glacier recession should lead to a marked increase in the spatial extent of the paraglacial <span class="hlt">zone</span> in glaciated drainage basins. The extent of the paraglacial <span class="hlt">zone</span> has been well established to be transient but there are very few studies of this transient response and what it means for <span class="hlt">sediment</span> export. There is good reason to expect that glacier recession could increase basin-scale <span class="hlt">sediment</span> connectivity as: <span class="hlt">sediment</span> becomes less dependent on glacier surface transport; proglacial streams are more able to migrate laterally than subglacial streams and so access <span class="hlt">sediment</span> for transport; and glacier debuttressing may aid the development of gullies that can dissect moraines and so aid hillslope to proglacial <span class="hlt">zone</span> connectivity. By using records of the flushing of hydroelectric power installations we were able to develop a record of coarse <span class="hlt">sediment</span> (sand and gravel) export from a basin with a rapidly retreating valley glacier, the Haut Glacier d'Arolla, from 1977 to 2014. Modelling suggested that these data could only be partially controlled by transport capacity implying an important role for <span class="hlt">sediment</span> supply and potentially for the influence of changing <span class="hlt">sediment</span> connectivity. Indeed, there was evidence of the effects of glacial debuttressing upon gullying processes and hence a possible increase in the ease of connection of upstream basins to the proglacial area. More recently, we were able to show possible temperature control on <span class="hlt">sediment</span> export, which may only have become apparent because of the progressive development of better <span class="hlt">sediment</span> connectivity. However, whilst rapid glacier recession should result in theory in a progressive increase in connectivity of <span class="hlt">sediment</span> sources to the basin outlet, the supply to capacity ratio does not increase continually with glacier recession until maximum capacity is reached. We identified two possible examples of why. First, gullying was also accompanied by the <span class="hlt">sediment</span> accumulation at the base of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29751318','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29751318"><span>Characterizing the capacity of hyporheic <span class="hlt">sediments</span> to attenuate groundwater nitrate loads by adsorption.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Meghdadi, Aminreza</p> <p>2018-05-02</p> <p>Nitrate has been recognized as a global threat to environmental health. In this regard, the hyporheic <span class="hlt">zone</span> (saturated media beneath and adjacent to the stream bed) plays a crucial role in attenuating groundwater nitrate, prior to discharge into surface water. While different nitrate removal pathways have been investigated over recent decades, the adsorption capacity of hyporheic <span class="hlt">sediments</span> under natural conditions has not yet been identified. In this study, the natural attenuation capacity of the hyporheic-<span class="hlt">sediments</span> of the Ghezel-Ozan River, located in the north-west of Iran, was determined. The sampled <span class="hlt">sediments</span> (from 1 m below the stream bed) were characterized via XRD, FT-IR, BET, SEM, BJH, and Zeta potential. Nitrate adsorption was evaluated using a batch experiment with hyporheic pore-water from each study site. The study was performed in the hyporheic <span class="hlt">sediments</span> of two morphologically different <span class="hlt">zones</span>, including Z 1 located in the parafluvial <span class="hlt">zone</span> having the clay <span class="hlt">sediment</span> texture (57.8% clay) with smectite/Illite mixed layer clay type and Z 2 located in the river confluence area containing silty clay <span class="hlt">sediment</span> texture (47.6% clay) with smectite/kaolinite mixed layer clay type. Data obtained from the batch experiment were subjected to pseudo-first order, pseudo-second order, intra-particle diffusion, and Elovich mass transfer kinetic models to characterize the nitrate adsorption mechanism. Furthermore, to replicate nitrate removal efficiencies of the hyporheic <span class="hlt">sediments</span> under natural conditions, the sampled hyporheic pore-waters were applied as initial solutions to run the batch experiment. The results of the artificial nitrate solution correlated well with pseudo-second order (R 2 >95%; in both Z 1 and Z 2 ) and maximum removal efficiencies of 85.3% and 71.2% (adsorbent dosage 90 g/L, pH = 5.5, initial adsorbate concentration of 90 mg/L) were achieved in Z 1 and Z 2 , respectively. The results of the nitrate adsorption analysis revealed that the nitrate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18..442W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18..442W"><span>Wind influence on the course of <span class="hlt">sedimentation</span> processes of the laminated lacustrine <span class="hlt">sediments</span> of Lake Czechowskie</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wiśniewska, Daria; Kramkowski, Mateusz; Tyszkowski, Sebastian</p> <p>2016-04-01</p> <p>The studies of the laminated lacustrine <span class="hlt">sediments</span> play a very important role in the analysis of climate change. They provide valuable information related to the response of the ecosystem to changes in the environment. The condition for the development of the annual lamination is calm <span class="hlt">sedimentation</span>, which can be compromised by the movement of water caused by waving. The depth to which this movement affects depends on the shape of the lake basin as well as the velocity and direction of the wind. During the study of sedimentary processes of laminated deposits in Lake Czechowskie (Tuchola Forest, North Poland, 53°52'N, 18°14' E, 108 m asl), the following question arose: How strong was the influence of the wind on the processes of lacustrine <span class="hlt">sedimentation</span>? The key in getting the answers was the use of GIS techniques. Lake Czechowskie has an area of 76.6 hectares; it has two deeps separated by a threshold: a deeper one of 33 m (maximum depth of the basin) in the central-eastern part, and a shallower of 13 m in the western part. The speed of movement of water that is able to move <span class="hlt">sediment</span> from the bottom of the lake, called the orbital wave velocity, is the basis for the designation of areas where re-suspension takes place. To calculate the wave parameters, the process of mixing, as well as the designation of re-suspension <span class="hlt">zones</span>, the tool-script Wave Model (Rohweder et al. 2008) in the program ArsGIS 10.1 was used. The input data were wind direction and velocity from the meteorological station of Wirty about 15 km away, bathymetric data from acoustic profiling, and the Maximum Orbital Wave Velocity. The elements taken into account include maximum wind velocity of the multi-year 1996-2013, with particular emphasis on hurricanes Ksawery (December 2013) and Yoda (November 2011), during which wind velocity exceeded 120 km/h. In addition, maximum wind velocity ever recorded in the Polish Lowlands was considered. On the basis of the modelling, the authors delimited the areas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982DSRA...29...87D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982DSRA...29...87D"><span>Fish debris in <span class="hlt">sediments</span> of the upwelling <span class="hlt">zone</span> off central Peru: a late Quaternary record</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Vries, Thomas J.; Pearcy, William G.</p> <p>1982-01-01</p> <p>Scales of the anchoveta were abundantly represented among fish remains preserved in partly laminated marine <span class="hlt">sediments</span> on the upper continental slope of Peru. Hake scales were less common. Sardine scales occurred only sporadically. Recent accumulation rates of scales indicate that prior to exploitation the anchoveta standing stock off Peru was about five times that of northern anchovy off California. During glacial time, however, clupeoids were less abundant off Peru and were more evenly distributed among sardines and anchoveta. Evidence from fish scales and phytoplankton assemblages suggests that the coastal waters off Peru did not respond to continental glacial and neoglacial advances simply by cooling. High accumulation rates of scales from warm-water fishes and tests of cool-water phytoplankton preceded and succeeded an interval containing low numbers of dominantly warm-water taxa. This interval coincided with the second neoglacial advance (2000 to 2700 y B.P.). Similar but less well-defined warm-water and cool-water assemblages coincided with the third neoglacial advance (200 to 400 y B.P.) and the last glacial retreat. Upwelling intensity probably fluctuated more widely during early and late phases of glacial and neoglacial cooling episodes, accounting for the mix of distinctly warm-water and cool-water assemblages and perhaps for an enhanced productivity. A weakened Intertropical Convergence <span class="hlt">Zone</span> or strengthened coastal countercurrent may explain the warm-water marine faunas and floras and wet climates on the mainland of Peru inferred by others for neoglacial or glacial time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012082','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012082"><span>Structural characteristics of fulvic acids from Continental Shelf <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hatcher, P.G.; Breger, I.A.; Mattingly, M.A.</p> <p>1980-01-01</p> <p>Fulvic acids are those components of soil organic matter that remain soluble after a dilute alkaline extract of the soil is acidified to pH 2 (refs 1, 2). This extraction procedure has been applied to marine <span class="hlt">sediments</span>, and the organic compounds so <span class="hlt">recovered</span> have been called marine sedimentary fulvic acids. These fulvic acids are thought to form more complex humic substances in marine <span class="hlt">sediments</span> by condensation reactions3. However, the chemical structural compositions of marine fulvic acids have not been defined sufficiently to allow this precursor relationship to be made. Here NMR spectroscopy is used to identify more clearly the chemical structural components of some marine sedimentary fulvic acids, thus enabling a more useful examination of their relationship to more complex humic substances. ?? 1980 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26210588','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26210588"><span>Magnetic properties of <span class="hlt">sediments</span> in cores from the Mandovi estuary, western India: Inferences on provenance and pollution.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Prajith, A; Rao, V Purnachandra; Kessarkar, Pratima M</p> <p>2015-10-15</p> <p>Magnetic properties of <span class="hlt">sediments</span> were investigated in 7 gravity cores <span class="hlt">recovered</span> along a transect of the Mandovi estuary, western India to understand their provenance and pollution. The maximum magnetic susceptibility of <span class="hlt">sediments</span> was at least 6 times higher in the upper/middle estuary than in lower estuary/bay. The χfd% and χARM/SIRM of <span class="hlt">sediments</span> indicated coarse, multi-domain and pseudo-single domain magnetic grains, resembling ore material in the upper/middle estuary and coarse stable single domain (SSD) to fine SSD grains in the lower estuary/bay. Mineralogy parameters indicated hematite and goethite-dominated <span class="hlt">sediments</span> in the upper/middle estuary and magnetite-dominated <span class="hlt">sediments</span> in the lower estuary/bay. Two <span class="hlt">sediment</span> types were discernible because of deposition of abundant ore material in the upper/middle estuary and detrital <span class="hlt">sediment</span> in the lower estuary/bay. The enrichment factor and Index of geo-accumulation of metals indicated significant to strong pollution with respect to Fe and Mn in <span class="hlt">sediments</span> from the upper/middle estuary. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15..386W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15..386W"><span>Reactive and recoverable sorbents for halogenated organic compound remediation in <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Werner, David; Taggalou, Villy; Kordulis, Christos; Dolfing, Jan; Karapanagioti, Hrissi K.</p> <p>2013-04-01</p> <p>Activated carbon (AC) has been proposed as a <span class="hlt">sediment</span> amendment for aquatic systems polluted with hydrophobic organic compounds. AC acts as a strong binding agent that lowers the pollutant concentration and thus, its toxicity. A draw back of this in-situ remediation method is that although the pollutant will remain non-bioavailable for many years being sorbed into AC, it actually stays in the system. A reactive sorbent, a sorbent that would, at the same time, facilitate the degradation of the pollutant, would be better accepted by the public or the regulators than AC amendment. So far, catalysts supported on AC with zero valent iron and a reactive metal have been proposed for the dechlorination of chlorinated organic compounds. These reactive metals are usually expensive or toxic and thus, their addition to the environment is not desirable. In the present study, activated carbon modified with reduced iron(AC/Fe) is tested in batch systems in the presence of <span class="hlt">sediment</span> and DDT sorbed on polyethylene sheets. The batch systems are equilibrated for different contact times. Then, the DDT remaining in the polyethylene sheets is quantified along with DDD produced due to the dechlorination of DDT. A small percentage of DDT is degraded to DDD in the systems containing the AC/Fe material. No degradation of DDT is observed in the control systems containing the pollutant and the <span class="hlt">sediment</span> or the pollutant, the <span class="hlt">sediment</span> and AC. Thus, the addition of AC/Fe to the <span class="hlt">sediment</span> with the DDT is enough to cause the dechlorination of DDT. At the end of the experiments, a magnet rod is used to <span class="hlt">recover</span> the AC/Fe material from the batches with the <span class="hlt">sediment</span>. An average recovery of 83% is achieved. This is a high percentage suggesting that the material can be easily <span class="hlt">recovered</span>. Some drawbacks of the material preparation method are identified after the composite material characterization. For example, the AC/Fe surface area is decreased with the material preparation compared to the initial surface</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T23I..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T23I..02C"><span>Influence of <span class="hlt">sediment</span> recycling on the trace element composition of primitive arc lavas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Collinet, M.; Jagoutz, O. E.</p> <p>2017-12-01</p> <p>Primitive calc-alkaline lavas from continental arcs are, on average, enriched in incompatible elements compared to those from intra-oceanic arcs. This relative enrichment is observed in different groups of trace elements: LILE (e.g. K, Rb), LREE to MREE (La-Dy) and HFSE (e.g.Zr, Nb) and is thought to result from (1) a transfer of material from the subducting slab to the mantle wedge at higher temperature than in intra-oceanic margins and/or (2) lower average degrees of melting in the mantle wedge, as a consequence of thicker overlying crusts and higher average pressures of melting. In addition to thicker overlying crusts and generally higher slab temperatures, continental margins are characterized by larger volumes of rock exposed above sea level and enhanced erosion rates compared to intra-oceanic arcs. As several geochemical signatures of arc lavas attest to the importance of <span class="hlt">sediment</span> recycling in subduction <span class="hlt">zones</span>, we explore the possibility that the high concentrations of incompatible elements in primitive lavas from continental arcs directly reflect a larger input of <span class="hlt">sediment</span> to the subduction system. Previous efforts to quantify the <span class="hlt">sediment</span> flux to oceanic trenches focused on the thickness of pelagic and hemipelagic <span class="hlt">sediments</span> on top of the plate entering the subduction <span class="hlt">zone</span> (Plank and Langmuir, 1993, Nature). These estimates primarily relied on the <span class="hlt">sediment</span> layer drilled outboard from the subduction system and likely underestimate the volume of <span class="hlt">sediment</span> derived from the arc itself. Accordingly, we find that such estimates of <span class="hlt">sediment</span> flux do not correlate with the concentration of incompatible elements in primitive arc lavas. To account for regional contributions of coarser detrital <span class="hlt">sediments</span>, usually delivered to oceanic trenches by turbidity currents, we apply to arc segments a model that quantifies the <span class="hlt">sediment</span> load of rivers based on the average relief, area, temperature and runoff of their respective drainage areas (Syvitski et al., 2003, <span class="hlt">Sediment</span>. Geol</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016805','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016805"><span>Prospecting for <span class="hlt">zones</span> of contaminated ground-water discharge to streams using bottom-<span class="hlt">sediment</span> gas bubbles</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Vroblesky, Don A.; Lorah, Michelle M.</p> <p>1991-01-01</p> <p>Decomposition of organic-rich bottom <span class="hlt">sediment</span> in a tidal creek in Maryland results in production of gas bubbles in the bottom <span class="hlt">sediment</span> during summer and fall. In areas where volatile organic contaminants discharge from ground water, through the bottom <span class="hlt">sediment</span>, and into the creek, part of the volatile contamination diffuses into the gas bubbles and is released to the atmosphere by ebullition. Collection and analysis of gas bubbles for their volatile organic contaminant content indicate that relative concentrations of the volatile organic contaminants in the gas bubbles are substantially higher in areas where the same contaminants occur in the ground water that discharges to the streams. Analyses of the bubbles located an area of previously unknown ground-water contamination. The method developed for this study consisted of disturbing the bottom <span class="hlt">sediment</span> to release gas bubbles, and then capturing the bubbles in a polyethylene bag at the water-column surface. The captured gas was transferred either into sealable polyethylene bags for immediate analysis with a photoionization detector or by syringe to glass tubes containing wires coated with an activated-carbon adsorbent. Relative concentrations were determined by mass spectral analysis for chloroform and trichloroethylene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176619','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176619"><span>Estimation of historic flows and <span class="hlt">sediment</span> loads to San Francisco Bay,1849–2011</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Moftakhari, H.R.; Jay, D.A.; Talke, S.A.; Schoellhamer, David H.</p> <p>2015-01-01</p> <p>River flow and <span class="hlt">sediment</span> transport in estuaries influence morphological development over decadal and century time scales, but hydrological and sedimentological records are typically too short to adequately characterize long-term trends. In this study, we <span class="hlt">recover</span> archival records and apply a rating curve approach to develop the first instrumental estimates of daily delta inflow and <span class="hlt">sediment</span> loads to San Francisco Bay (1849–1929). The total <span class="hlt">sediment</span> load is constrained using <span class="hlt">sedimentation</span>/erosion estimated from bathymetric survey data to produce continuous daily <span class="hlt">sediment</span> transport estimates from 1849 to 1955, the time period prior to <span class="hlt">sediment</span> load measurements. We estimate that ∼55% (45–75%) of the ∼1500 ± 400 million tons (Mt) of <span class="hlt">sediment</span> delivered to the estuary between 1849 and 2011 was the result of anthropogenic alteration in the watershed that increased <span class="hlt">sediment</span> supply. Also, the seasonal timing of <span class="hlt">sediment</span> flux events has shifted because significant spring-melt floods have decreased, causing estimated springtime transport (April 1st to June 30th) to decrease from ∼25% to ∼15% of the annual total. By contrast, wintertime <span class="hlt">sediment</span> loads (December 1st to March 31st) have increased from ∼70% to ∼80%. A ∼35% reduction of annual flow since the 19th century along with decreased <span class="hlt">sediment</span> supply has resulted in a ∼50% reduction in annual <span class="hlt">sediment</span> delivery. The methods developed in this study can be applied to other systems for which unanalyzed historic data exist.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2011/1199/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2011/1199/"><span>Characterization of <span class="hlt">sediments</span> from the Gulf of Mexico and Atlantic shorelines, Texas to Florida</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lisle, John T.; Comer, Norris N.</p> <p>2011-01-01</p> <p>In response to the Deepwater Horizon oil spill, <span class="hlt">sediment</span> samples that were projected to have a high probability of being impacted by the oil were collected from shoreline <span class="hlt">zones</span> of Texas, Louisiana, Mississippi, Alabama, and Florida. Sixty-one sites were sampled and analyzed for hydraulic conductivity, porosity, and grain-size distribution. The objective of this effort was to provide a set of baseline data on <span class="hlt">sediment</span> characteristics known to directly influence (1) the penetration of oil into coastal <span class="hlt">sediments</span> and (2) the efficacy of chemical and (or) bioremediation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ECSS..202...87K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ECSS..202...87K"><span>Spatio-temporal scaling effects on longshore <span class="hlt">sediment</span> transport pattern along the nearshore <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khorram, Saeed; Ergil, Mustafa</p> <p>2018-03-01</p> <p>A measure of uncertainties, entropy has been employed in such different applications as coastal engineering probability inferences. Entropy <span class="hlt">sediment</span> transport integration theories present novel visions in coastal analyses/modeling the application and development of which are still far-reaching. Effort has been made in the present paper to propose a method that needs an entropy-power index for spatio-temporal patterns analyses. Results have shown that the index is suitable for marine/hydrological ecosystem components analyses based on a beach area case study. The method makes use of six Makran Coastal monthly data (1970-2015) and studies variables such as spatio-temporal patterns, LSTR (long-shore <span class="hlt">sediment</span> transport rate), wind speed, and wave height all of which are time-dependent and play considerable roles in terrestrial coastal investigations; the mentioned variables show meaningful spatio-temporal variability most of the time, but explanation of their combined performance is not easy. Accordingly, the use of an entropy-power index can show considerable signals that facilitate the evaluation of water resources and will provide an insight regarding hydrological parameters' interactions at scales as large as beach areas. Results have revealed that an STDDPI (entropy based spatio-temporal disorder dynamics power index) can simulate wave, long-shore <span class="hlt">sediment</span> transport rate, and wind when granulometry, concentration, and flow conditions vary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030352','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030352"><span>Mechanical and electromagnetic properties of northern Gulf of Mexico <span class="hlt">sediments</span> with and without THF hydrates</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lee, J.Y.; Santamarina, J.C.; Ruppel, C.</p> <p>2008-01-01</p> <p>Using an oedometer cell instrumented to measure the evolution of electromagnetic properties, small strain stiffness, and temperature, we conducted consolidation tests on <span class="hlt">sediments</span> <span class="hlt">recovered</span> during drilling in the northern Gulf of Mexico at the Atwater Valley and Keathley Canyon sites as part of the 2005 Chevron Joint Industry Project on Methane Hydrates. The tested specimens include both unremolded specimens (as <span class="hlt">recovered</span> from the original core liner) and remolded <span class="hlt">sediments</span> both without gas hydrate and with pore fluid exchanged to attain 100% synthetic (tetrahydrofuran) hydrate saturation at any stage of loading. Test results demonstrate the extent to which the electromagnetic and mechanical properties of hydrate-bearing marine <span class="hlt">sediments</span> are governed by the vertical effective stress, stress history, porosity, hydrate saturation, fabric, ionic concentration of the pore fluid, and temperature. We also show how permittivity and electrical conductivity data can be used to estimate the evolution of hydrate volume fraction during formation. The gradual evolution of geophysical properties during hydrate formation probably reflects the slow increase in ionic concentration in the pore fluid due to ion exclusion in closed systems and the gradual decrease in average pore size in which the hydrate forms. During hydrate formation, the increase in S-wave velocity is delayed with respect to the decrease in permittivity, consistent with hydrate formation on mineral surfaces and subsequent crystal growth toward the pore space. No significant decementation/debonding occurred in 100% THF hydrate-saturated <span class="hlt">sediments</span> during unloading, hence the probability of sampling hydrate-bearing <span class="hlt">sediments</span> without disturbing the original <span class="hlt">sediment</span> fabric is greatest for samples in which the gas hydrate is primarily responsible for maintaining the <span class="hlt">sediment</span> fabric and for which the time between core retrieval and restoration of in situ effective stress in the laboratory is minimized. In evaluating the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/10154578-reservoir-vital-signs-monitoring-physical-chemical-characteristics-water-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/10154578-reservoir-vital-signs-monitoring-physical-chemical-characteristics-water-sediments"><span>Reservoir vital signs monitoring, 1990: Physical and chemical characteristics of water and <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Meinert, D.L.</p> <p>1991-05-01</p> <p>As part of Tennessee Valley Authority`s (TVA`s) Reservoir Vital Signs Monitoring program, physical/chemical measurements of water and <span class="hlt">sediment</span> were made in 1990 on twelve TVA reservoirs (the nine main steam Tennessee river reservoirs - Kentucky through Fort Loudoun and three major tributary reservoirs - Cherokee, Douglas, and Norris). The objective of this monitoring program is to assess the health or integrity of these aquatic ecosystems. The physical/chemical water quality data collected in 1990 showed the water quality of these reservoirs to be very good. However, hypolimnetic anoxia during the summer months in Watts bars, Douglas, and Cherokee reservoir continues tomore » be a concern. High concentrations of nutrients were measured in the transition <span class="hlt">zones</span> of Cherokee and Douglas reservoirs, resulting in highly productive and eutrophic conditions in the transition <span class="hlt">zones</span> of these reservoirs. Fecal coliform organisms were frequently detected in the forebay area of Guntersville reservoir, and higher than expected ammonia nitrogen concentrations were found at the transition <span class="hlt">zone</span> of Wheeler reservoir. Elevated concentrations of mercury were found in Pickwick and Watts bar reservoir <span class="hlt">sediment</span>, and high lead concentrations were found in a <span class="hlt">sediment</span> sample collected from Guntersville reservoir. A TVA Reservoir Water Quality Index (RWQI) was developed and used to summarize water quality conditions on a scale from 0 (worst) to 100 (best).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5176693-reservoir-vital-signs-monitoring-physical-chemical-characteristics-water-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5176693-reservoir-vital-signs-monitoring-physical-chemical-characteristics-water-sediments"><span>Reservoir vital signs monitoring, 1990: Physical and chemical characteristics of water and <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Meinert, D.L.</p> <p>1991-05-01</p> <p>As part of Tennessee Valley Authority's (TVA's) Reservoir Vital Signs Monitoring program, physical/chemical measurements of water and <span class="hlt">sediment</span> were made in 1990 on twelve TVA reservoirs (the nine main steam Tennessee river reservoirs - Kentucky through Fort Loudoun and three major tributary reservoirs - Cherokee, Douglas, and Norris). The objective of this monitoring program is to assess the health or integrity of these aquatic ecosystems. The physical/chemical water quality data collected in 1990 showed the water quality of these reservoirs to be very good. However, hypolimnetic anoxia during the summer months in Watts bars, Douglas, and Cherokee reservoir continues tomore » be a concern. High concentrations of nutrients were measured in the transition <span class="hlt">zones</span> of Cherokee and Douglas reservoirs, resulting in highly productive and eutrophic conditions in the transition <span class="hlt">zones</span> of these reservoirs. Fecal coliform organisms were frequently detected in the forebay area of Guntersville reservoir, and higher than expected ammonia nitrogen concentrations were found at the transition <span class="hlt">zone</span> of Wheeler reservoir. Elevated concentrations of mercury were found in Pickwick and Watts bar reservoir <span class="hlt">sediment</span>, and high lead concentrations were found in a <span class="hlt">sediment</span> sample collected from Guntersville reservoir. A TVA Reservoir Water Quality Index (RWQI) was developed and used to summarize water quality conditions on a scale from 0 (worst) to 100 (best).« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17492316','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17492316"><span>Mangrove growth in New Zealand estuaries: the role of nutrient enrichment at sites with contrasting rates of <span class="hlt">sedimentation</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lovelock, Catherine E; Feller, Ilka C; Ellis, Joanne; Schwarz, Ann Maree; Hancock, Nicole; Nichols, Pip; Sorrell, Brian</p> <p>2007-09-01</p> <p>Mangrove forest coverage is increasing in the estuaries of the North Island of New Zealand, causing changes in estuarine ecosystem structure and function. <span class="hlt">Sedimentation</span> and associated nutrient enrichment have been proposed to be factors leading to increases in mangrove cover, but the relative importance of each of these factors is unknown. We conducted a fertilization study in estuaries with different <span class="hlt">sedimentation</span> histories in order to determine the role of nutrient enrichment in stimulating mangrove growth and forest development. We expected that if mangroves were nutrient-limited, nutrient enrichment would lead to increases in mangrove growth and forest structure and that nutrient enrichment of trees in our site with low <span class="hlt">sedimentation</span> would give rise to trees and <span class="hlt">sediments</span> that converged in terms of functional characteristics on control sites in our high <span class="hlt">sedimentation</span> site. The effects of fertilizing with nitrogen (N) varied among sites and across the intertidal <span class="hlt">zone</span>, with enhancements in growth, photosynthetic carbon gain, N resorption prior to leaf senescence and the leaf area index of canopies being significantly greater at the high <span class="hlt">sedimentation</span> sites than at the low <span class="hlt">sedimentation</span> sites, and in landward dwarf trees compared to seaward fringing trees. <span class="hlt">Sediment</span> respiration (CO(2) efflux) was higher at the high <span class="hlt">sedimentation</span> site than at the low one <span class="hlt">sedimentation</span> site, but it was not significantly affected by fertilization, suggesting that the high <span class="hlt">sedimentation</span> site supported greater bacterial mineralization of <span class="hlt">sediment</span> carbon. Nutrient enrichment of the coastal <span class="hlt">zone</span> has a role in facilitating the expansion of mangroves in estuaries of the North Island of New Zealand, but this effect is secondary to that of <span class="hlt">sedimentation</span>, which increases habitat area and stimulates growth. In estuaries with high <span class="hlt">sediment</span> loads, enrichment with N will cause greater mangrove growth and further changes in ecosystem function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4134218','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4134218"><span>The Fate of Nitrate in Intertidal Permeable <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Marchant, Hannah K.; Lavik, Gaute; Holtappels, Moritz; Kuypers, Marcel M. M.</p> <p>2014-01-01</p> <p>Coastal <span class="hlt">zones</span> act as a sink for riverine and atmospheric nitrogen inputs and thereby buffer the open ocean from the effects of anthropogenic activity. Recently, microbial activity in sandy permeable <span class="hlt">sediments</span> has been identified as a dominant source of N-loss in coastal <span class="hlt">zones</span>, namely through denitrification. Some of the highest coastal denitrification rates measured so far occur within the intertidal permeable <span class="hlt">sediments</span> of the eutrophied Wadden Sea. Still, denitrification alone can often account for only half of the substantial nitrate (NO3 −) consumption. Therefore, to investigate alternative NO3 − sinks such as dissimilatory nitrate reduction to ammonium (DNRA), intracellular nitrate storage by eukaryotes and isotope equilibration effects we carried out 15NO3 − amendment experiments. By considering all of these sinks in combination, we could quantify the fate of the 15NO3 − added to the <span class="hlt">sediment</span>. Denitrification was the dominant nitrate sink (50–75%), while DNRA, which recycles N to the environment accounted for 10–20% of NO3 − consumption. Intriguingly, we also observed that between 20 and 40% of 15NO3 − added to the incubations entered an intracellular pool of NO3 − and was subsequently respired when nitrate became limiting. Eukaryotes were responsible for a large proportion of intracellular nitrate storage, and it could be shown through inhibition experiments that at least a third of the stored nitrate was subsequently also respired by eukaryotes. The environmental significance of the intracellular nitrate pool was confirmed by in situ measurements which revealed that intracellular storage can accumulate nitrate at concentrations six fold higher than the surrounding porewater. This intracellular pool is so far not considered when modeling N-loss from intertidal permeable <span class="hlt">sediments</span>; however it can act as a reservoir for nitrate during low tide. Consequently, nitrate respiration supported by intracellular nitrate storage can add an additional</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25127459','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25127459"><span>The fate of nitrate in intertidal permeable <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marchant, Hannah K; Lavik, Gaute; Holtappels, Moritz; Kuypers, Marcel M M</p> <p>2014-01-01</p> <p>Coastal <span class="hlt">zones</span> act as a sink for riverine and atmospheric nitrogen inputs and thereby buffer the open ocean from the effects of anthropogenic activity. Recently, microbial activity in sandy permeable <span class="hlt">sediments</span> has been identified as a dominant source of N-loss in coastal <span class="hlt">zones</span>, namely through denitrification. Some of the highest coastal denitrification rates measured so far occur within the intertidal permeable <span class="hlt">sediments</span> of the eutrophied Wadden Sea. Still, denitrification alone can often account for only half of the substantial nitrate (NO3-) consumption. Therefore, to investigate alternative NO3- sinks such as dissimilatory nitrate reduction to ammonium (DNRA), intracellular nitrate storage by eukaryotes and isotope equilibration effects we carried out 15NO3- amendment experiments. By considering all of these sinks in combination, we could quantify the fate of the 15NO3- added to the <span class="hlt">sediment</span>. Denitrification was the dominant nitrate sink (50-75%), while DNRA, which recycles N to the environment accounted for 10-20% of NO3- consumption. Intriguingly, we also observed that between 20 and 40% of 15NO3- added to the incubations entered an intracellular pool of NO3- and was subsequently respired when nitrate became limiting. Eukaryotes were responsible for a large proportion of intracellular nitrate storage, and it could be shown through inhibition experiments that at least a third of the stored nitrate was subsequently also respired by eukaryotes. The environmental significance of the intracellular nitrate pool was confirmed by in situ measurements which revealed that intracellular storage can accumulate nitrate at concentrations six fold higher than the surrounding porewater. This intracellular pool is so far not considered when modeling N-loss from intertidal permeable <span class="hlt">sediments</span>; however it can act as a reservoir for nitrate during low tide. Consequently, nitrate respiration supported by intracellular nitrate storage can add an additional 20% to previous nitrate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.728...92B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.728...92B"><span>Multivariate statistical analysis to investigate the subduction <span class="hlt">zone</span> parameters favoring the occurrence of giant megathrust earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brizzi, S.; Sandri, L.; Funiciello, F.; Corbi, F.; Piromallo, C.; Heuret, A.</p> <p>2018-03-01</p> <p>The observed maximum magnitude of subduction megathrust earthquakes is highly variable worldwide. One key question is which conditions, if any, favor the occurrence of giant earthquakes (Mw ≥ 8.5). Here we carry out a multivariate statistical study in order to investigate the factors affecting the maximum magnitude of subduction megathrust earthquakes. We find that the trench-parallel extent of subduction <span class="hlt">zones</span> and the thickness of trench <span class="hlt">sediments</span> provide the largest discriminating capability between subduction <span class="hlt">zones</span> that have experienced giant earthquakes and those having significantly lower maximum magnitude. Monte Carlo simulations show that the observed spatial distribution of giant earthquakes cannot be explained by pure chance to a statistically significant level. We suggest that the combination of a long subduction <span class="hlt">zone</span> with thick trench <span class="hlt">sediments</span> likely promotes a great lateral rupture propagation, characteristic of almost all giant earthquakes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21800629','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21800629"><span>[Microbial diversity of <span class="hlt">sediments</span> from the coasts of Dalian Changshan Islands].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Jialin; Wang, Zhonghua; Qin, Song; Wang, Guangyi</p> <p>2011-05-01</p> <p>To understand the impacts of anthropogenic activities on structure and composition of bacterial communities and to evaluate how bacterial communities respond to environmental gradients at coastal <span class="hlt">sediments</span>. The diversity of bacterial communities in <span class="hlt">sediments</span> from tourist and mariculture <span class="hlt">zones</span> at coastal area of Dalian Changshan Islands was assessed using terminal restriction fragment length polymorphism (t-RFLP) and denaturing gradient gel electrophoresis (DGGE) approaches. Meanwhile, 16S rRNA clone library was constructed to reveal the composition and structure of bacterial communities in the most seriously polluted site (D4). There were much higher values of richness, Shannon-wiener and evenness index at D4 site by the analysis of terminal restriction fragments (t-RFs). The clustering result on the t-RFs areas and DGGE patterns showed that the bacterial diversity of tourist <span class="hlt">zone</span> were more similar, while the distinction was increased with pollution levels among the tourist and mariculture <span class="hlt">zones</span>. The 16S rRNA clone of D4 revealed that the Proteobacteria were the dominant phylum, and gamma-proteobacteria was the main class within Proteobacteria. The study documented changes in bacterial community structure by human impacts of mariculture than geographical location.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...147...27M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...147...27M"><span>Implications of tidally-varying bed stress and intermittent estuarine stratification on fine-<span class="hlt">sediment</span> dynamics through the Mekong's tidal river to estuarine reach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McLachlan, R. L.; Ogston, A. S.; Allison, M. A.</p> <p>2017-09-01</p> <p>River gauging stations are often located upriver of tidal propagation where <span class="hlt">sediment</span> transport processes and storage are impacted by widely varying ratios of marine to freshwater influence. These impacts are not yet thoroughly understood. Therefore, <span class="hlt">sediment</span> fluxes measured at these stations may not be suitable for predicting changes to coastal morphology. To characterize <span class="hlt">sediment</span> transport dynamics in this understudied <span class="hlt">zone</span>, flow velocity, salinity, and suspended-<span class="hlt">sediment</span> properties (concentration, size, and settling velocity) were measured within the tidal Sông Hậu distributary of the lower Mekong River, Vietnam. Fine-<span class="hlt">sediment</span> aggregation, settling, and trapping rates were promoted by seasonal and tidal fluctuations in near-bed shear stress as well as the intermittent presence of a salt wedge and estuary turbidity maximum. Beginning in the tidal river, fine-grained particles were aggregated in freshwater. Then, in the interface <span class="hlt">zone</span> between the tidal river and estuary, impeded near-bed shear stress and particle flux convergence promoted settling and trapping. Finally, in the estuary, <span class="hlt">sediment</span> retention was further encouraged by stratification and estuarine circulation which protected the bed against particle resuspension and enhanced particle aggregation. These patterns promote mud export ( 1.7 t s-1) from the entire study area in the high-discharge season when fluvial processes dominate and mud import ( 0.25 t s-1) into the estuary and interface <span class="hlt">zone</span> in the low-discharge season when estuarine processes dominate. Within the lower region of the distributaries, morphological change in the form of channel abandonment was found to be promoted within minor distributaries by feedbacks between channel depth, vertical mixing, and aggregate trapping. In effect, this field study sheds light on the <span class="hlt">sediment</span> trapping capabilities of the tidal river - estuary interface <span class="hlt">zone</span>, a relatively understudied region upstream of where traditional concepts place sites of deposition</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5047066','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5047066"><span>The Interplay between Carbon Availability and Growth in Different <span class="hlt">Zones</span> of the Growing Maize Leaf1[OPEN</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Arrivault, Stéphanie; Lohse, Marc A.; Feil, Regina; Krohn, Nicole; Encke, Beatrice; Nunes-Nesi, Adriano; Fernie, Alisdair R.; Stitt, Mark</p> <p>2016-01-01</p> <p>Plants assimilate carbon in their photosynthetic tissues in the light. However, carbon is required during the night and in nonphotosynthetic organs. It is therefore essential that plants manage their carbon resources spatially and temporally and coordinate growth with carbon availability. In growing maize (Zea mays) leaf blades, a defined developmental gradient facilitates analyses in the cell division, elongation, and mature <span class="hlt">zones</span>. We investigated the responses of the metabolome and transcriptome and polysome loading, as a qualitative proxy for protein synthesis, at dusk, dawn, and 6, 14, and 24 h into an extended night, and tracked whole-leaf elongation over this time course. Starch and sugars are depleted by dawn in the mature <span class="hlt">zone</span>, but only after an extension of the night in the elongation and division <span class="hlt">zones</span>. Sucrose (Suc) <span class="hlt">recovers</span> partially between 14 and 24 h into the extended night in the growth <span class="hlt">zones</span>, but not the mature <span class="hlt">zone</span>. The global metabolome and transcriptome track these <span class="hlt">zone</span>-specific changes in Suc. Leaf elongation and polysome loading in the growth <span class="hlt">zones</span> also remain high at dawn, decrease between 6 and 14 h into the extended night, and then partially <span class="hlt">recover</span>, indicating that growth processes are determined by local carbon status. The level of Suc-signaling metabolite trehalose-6-phosphate, and the trehalose-6-phosphate:Suc ratio are much higher in growth than mature <span class="hlt">zones</span> at dusk and dawn but fall in the extended night. Candidate genes were identified by searching for transcripts that show characteristic temporal response patterns or contrasting responses to carbon starvation in growth and mature <span class="hlt">zones</span>. PMID:27582314</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFM.H51E0417W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFM.H51E0417W"><span>Source and Fate of <span class="hlt">Sediments</span> in the Bahia de Anasco, Puerto Rico</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Webb, R. M.</p> <p>2005-12-01</p> <p><span class="hlt">Sediments</span> and wastewater mix in the insular marine waters of the Bah'{i}a de Añasco near Mayag{u}ez, Puerto Rico. Trace metal concentrations in fine <span class="hlt">sediments</span> deposited in the bay were measured to assess potential impact of the ocean outfall on the biota and habitats that include coral reefs. A Q-mode factor analysis of elemental compositions identified three <span class="hlt">sediment</span> sources and their relative proportions in 51 core and surficial samples collected from the bay and within the coral reefs: (1) <span class="hlt">sediments</span> discharged by the R'{i}o Grande de Añasco; (2) calcareous skeletal remains; and (3) <span class="hlt">sediments</span> discharged by the R'{i}o Guanajibo. The nickel and chromium derived from laterite deposits provide a unique fingerprint for <span class="hlt">sediments</span> discharged from the R'{i}o Guanajibo. Naturally occurring concentrations of these elements exceed Probable Effect Limits (PEL's: 42 mg/kg for nickel and 160 mg/kg for chromium) in <span class="hlt">sediments</span> deposited near the river mouth. The detection of mercury at 1 mg/kg in one sample from a core <span class="hlt">recovered</span> near the wastewater outfall was the only indication of a possible outfall source in the data set. The temporal and spatial variations in source fractions proved useful in determining relative frequencies of historic floods and steady-state circulation patterns off the west coast of Puerto Rico.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1302596','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1302596"><span>Modeling the formation of methane hydrate-bearing intervals in fine-grained <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Malinverno, Alberto; Cook, Ann; Daigle, Hugh</p> <p></p> <p><span class="hlt">Sediment</span> grain size exerts a fundamental control on how methane hydrates are distributed within the pore space. Fine-grained muds are the predominant <span class="hlt">sediments</span> in continental margins, and hydrates in these <span class="hlt">sediments</span> have often been observed in semi-vertical veins and fractures. In several instances, these hydrate veins/fractures are found in discrete depth intervals a few tens meters thick within the gas hydrate stability <span class="hlt">zone</span> (GHSZ) surrounded by hydrate-free <span class="hlt">sediments</span> above and below. As they are not obviously connected with free gas occurring beneath the base of the GHSZ, these isolated hydrate-bearing intervals have been interpreted as formed by microbial methane generatedmore » in situ. To investigate further the formation of these hydrate deposits, we applied a time-dependent advection-diffusion-reaction model that includes the effects of <span class="hlt">sedimentation</span>, solute diffusion, and microbial methane generation. The microbial methane generation term depends on the amount of metabolizable organic carbon deposited at the seafloor, which is degraded at a prescribed rate resulting in methane formation beneath the sulfate reduction <span class="hlt">zone</span>. In the model, methane hydrate precipitates once the dissolved methane concentration is greater than solubility, or hydrate dissolves if concentration goes below solubility. If the deposition of organic carbon at the seafloor is kept constant in time, we found that the predicted amounts of hydrate formed in discrete intervals within the GHSZ are much less than those estimated from observations. We then investigated the effect of temporal variations in the deposition of organic carbon. If greater amounts of organic carbon are deposited during some time interval, methane generation is enhanced during burial in the corresponding <span class="hlt">sediment</span> interval. With variations in organic carbon deposition that are consistent with observations in continental margin <span class="hlt">sediments</span>, we were able to reproduce the methane hydrate contents estimated in discrete</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B11I0557C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B11I0557C"><span>Heterotrophic potential of Atribacteria from deep marine Antarctic <span class="hlt">sediment</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carr, S. A.; Orcutt, B.; Mandernack, K. W.; Spear, J. R.</p> <p>2015-12-01</p> <p>Bacteria belonging to the newly classified candidate phylum "Atribacteria" (formerly referred to as "OP9" and "JS1") are common in anoxic methane-rich <span class="hlt">sediments</span>. However, the metabolic functions and biogeochemical role of these microorganisms in the subsurface remains unrealized due to the lack of pure culture representatives. This study observed a steady increase of Atribacteria-related sequences with increasing <span class="hlt">sediment</span> depth throughout the methane-rich <span class="hlt">zone</span> of the Adélie Basin, Antarctica (according to a 16S rRNA gene survey). To explore the functional potential of Atribacteria in this basin, samples from various depths (14, 25 and 97 meters below seafloor), were subjected to metagenomic sequencing. Additionally, individual cells were separated from frozen, unpreserved <span class="hlt">sediment</span> for whole genome amplification. The successful isolation and sequencing of a single-amplified Atribacteria genome from these unpreserved <span class="hlt">sediments</span> demonstrates a future use of single cell techniques with previously collected and frozen <span class="hlt">sediments</span>. Our resulting single-cell amplified genome, combined with metagenomic interpretations, provides our first insights to the functional potential of Atribacteria in deep subsurface settings. As observed for non-marine Atribacteria, genomic analyses suggest a heterotrophic metabolism, with Atribacteria potentially producing fermentation products such as acetate, ethanol and CO2. These products may in turn support methanogens within the <span class="hlt">sediment</span> microbial community and explain the frequent occurrence of Atribacteria in anoxic methane-rich <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNS23A0022G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNS23A0022G"><span>Spectral Induced Polarization Response of Biofilm Formation in Hanford Vadose <span class="hlt">Zone</span> <span class="hlt">Sediment</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garcia, A.; Katsenovich, Y.; Lee, B.; Whitman, D.</p> <p>2017-12-01</p> <p>As a result of the U.S. Nuclear weapons program during the second world war and the cold war, there now exists a significant amount of uranium contamination at the U.S. Department of Energy Hanford site located in Washington state. In-situ immobilization of mobile uranium via injections of a soluble sodium tripolyphosphate amendment may prove effective in the formation of insoluble uranyl phosphate mineral, autunite. However, the injected polyphosphate undergoes hydrolysis in aqueous solutions to form orthophosphate, which serves as a readily available nutrient for the various microorganisms in the <span class="hlt">sediment</span>. <span class="hlt">Sediment</span>-filled column experiments conducted under saturated oxygen restricted conditions using geophysical Spectral Induced Polarization technique have shown the impact of microbes on the dissolution of autunite, a calcium uranyl phosphate mineral. Spectral Induced Polarization may be an effective way to track changes indicative of bacterial activities on the surrounding environment. This method can be a cost-effective alternative to the drilling of boreholes at a field scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26PSL.474...32M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26PSL.474...32M"><span>The onset of fabric development in deep marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maffione, Marco; Morris, Antony</p> <p>2017-09-01</p> <p>Post-depositional compaction is a key stage in the formation of sedimentary rocks that results in porosity reduction, grain realignment and the production of sedimentary fabrics. The progressive time-depth evolution of the onset of fabric development in deep marine <span class="hlt">sediments</span> is poorly constrained due to the limited quantity and resolution of existing data. Here we present high-resolution anisotropy of magnetic susceptibility (AMS) results from clay-rich deep marine <span class="hlt">sediments</span> <span class="hlt">recovered</span> at International Ocean Discovery Program Site U1438 (Philippine Sea). AMS is a petrofabric tool sensitive to the preferred orientation of grains in rocks. Down-section variations of AMS parameters, density, porosity and the inclination of magnetic remanences demonstrate that fabrics develop in response to compaction and dewatering but also that they do not develop progressively with depth below the mudline. Instead, a horizontal foliation first forms at 83 mbsf once the <span class="hlt">sediment</span> load reaches an effective stress threshold for the onset of compaction and is then continuously enhanced down to 113 mbsf, defining a 30 m-thick 'initial compaction window'. The magnetostratigraphic age model for IODP Site U1438 indicates a delay of 5.7 Ma in initial fabric formation following <span class="hlt">sediment</span> deposition, with strongly defined fabrics then taking an additional 6.5 Ma to develop.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP21D1876A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP21D1876A"><span>Numerical model of turbulence, <span class="hlt">sediment</span> transport, and morphodynamics tested in the Colorado River at Grand Canyon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alvarez, L. V.; Grams, P.</p> <p>2017-12-01</p> <p>We present a parallelized, three-dimensional, turbulence-resolving model using the Detached-Eddy Simulation (DES) technique, tested at the scale of the river-reach in the Colorado River. DES is a hybrid large eddy simulation (LES) and Reynolds-averaged Navier Stokes (RANS). RANS is applied to the near-bed grid cells, where grid resolution is not sufficient to fully resolve wall turbulence. LES is applied in the flow interior. We utilize the Spalart-Allmaras one equation turbulence closure with a rough wall extension. The model resolves large-scale turbulence using DES and simultaneously integrates the suspended <span class="hlt">sediment</span> advection-diffusion equation. The Smith and McLean suspended <span class="hlt">sediment</span> boundary condition is used to calculate the upward and downward settling of <span class="hlt">sediment</span> fluxes in the grid cells attached to the bed. Model results compare favorably with ADCP measurements of flow taken on the Colorado River in Grand Canyon during the High Flow Experiment (HFE) of 2008. The model accurately reproduces the size and position of the major recirculation currents, and the error in velocity magnitude was found to be less than 17% or 0.22 m/s absolute error. The mean deviation of the direction of velocity with respect to the measured velocity was found to be 20 degrees. Large-scale turbulence structures with vorticity predominantly in the vertical direction are produced at the shear layer between the main channel and the separation <span class="hlt">zone</span>. However, these structures rapidly become three-dimensional with no preferred orientation of vorticity. Cross-stream velocities, into the main recirculation <span class="hlt">zone</span> just upstream of the point of reattachment and out of the main recirculation region just downstream of the point of separation, are highest near the bed. Lateral separation eddies are more efficient at storing and exporting <span class="hlt">sediment</span> than previously modeled. The input of <span class="hlt">sediment</span> to the eddy recirculation <span class="hlt">zone</span> occurs in the interface of the eddy and main channel. Pulsation of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4997W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4997W"><span>What multi-beam bathymetric data can tell about morphodynamics and <span class="hlt">sediment</span> transport in an estuarine environment?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winterscheid, Axel; Reiß, Marcel</p> <p>2017-04-01</p> <p>The Elbe River Estuary is one of the most important waterways for commercial shipping in Europe. It connects the North Sea with the Port of Hamburg located about 100 km inlands. To secure navigation, the Federal Waterways and Shipping Administration (WSV) is operating a fleet of survey vessels all equipped with a multi-beam echo sounder controlling the required water depths. Beyond navigational purposes, this monitoring is creating a comprehensive and ever-growing data base, which can be used for a consistent morphodynamical description of the river bed. The history of multi-beam records in the Elbe River Estuary reaches back to 2008. At particular river sections where large amounts of fine grained <span class="hlt">sediments</span> accumulate surveys are taken biweekly; at other sections there are monthly surveys. Locally, <span class="hlt">sedimentation</span> rates of up to 12 cm per day have been observed within the fairway. The time series of multiple multi-beam records have been analyzed with a particular focus on morphodynamics and <span class="hlt">sedimentation</span> rates. Here we compare the morphodynamical characteristics of two river sections. The first section is located at the downstream end of the estuarine turbidity <span class="hlt">zone</span> near the city of Cuxhaven; the second section is located 50 km away at the upstream end of the turbidity <span class="hlt">zone</span> near the city of Hamburg. These two sections have been selected because in both the morphology of the river bed and the <span class="hlt">sedimentation</span> processes are strongly influenced by the presence of fine grained <span class="hlt">sediments</span>. The results show that changing <span class="hlt">sedimentation</span> rates in both sections are conditioned by different site specific factors, e.g. the dynamic shifting of the turbidity <span class="hlt">zone</span> along the estuary, which is resulting in a temporarily higher availability of suspended <span class="hlt">sediments</span> and more intense <span class="hlt">sedimentation</span> rates in the upper part of the estuary and the respective section. In contrast, in the downstream located river section more intense <span class="hlt">sedimentation</span> rates could be related to periods of strong north</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.T11A4537L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.T11A4537L"><span>Shallow velocity structure of the Alaska Peninsula subduction <span class="hlt">zone</span> and implications for controls on seismic behavior</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, J.; Shillington, D. J.; Becel, A.; Nedimovic, M. R.; Kuehn, H.; Webb, S. C.; Abers, G. A.; Keranen, K. M.; Saffer, D. M.</p> <p>2014-12-01</p> <p>Downdip and along-strike variations in the seismic behavior of subduction <span class="hlt">zone</span> megathrust faults are thought to be strongly controlled by changes in the material properties along the plate boundary. Roughness and hydration of the incoming plate, fluid pressure and lithology in the subducting <span class="hlt">sediment</span> channel are likely to control the distribution of shallower rupture. Here, we focus on the subduction <span class="hlt">zone</span> offshore of the Alaska Peninsula. In 2011, the ALEUT program acquired deep penetration multichannel seismic (MCS) reflection and ocean bottom seismometer (OBS) data across the apparently freely sliding Shumagin Gap, the locked Semidi segment that last ruptured in 1938 M8.2 earthquake, and the locked western Kodiak asperity, which ruptured in the 1964 M9.2 earthquake. Seismic reflection data from the ALEUT cruise reveal significant variability in the thickness of <span class="hlt">sediment</span> on the incoming plate and entering the trench, and the roughness and degree of hydration of the incoming plate. Oceanic crust entering the trench in the Shumagin gap is rugged with extensive faults and only a thin layer of <span class="hlt">sediment</span> (<0.5 km thick). Farther east in the Semidi segment, the subducting plate has a smoother surface with thicker <span class="hlt">sediments</span> (~1 km thick) and less faulting/hydration. To better constrain the properties of the accretionary prism and shallow part of the plate boundary, we are undertaking travel time tomography using reflection/refraction phases in OBS and MCS data, and constraints on the interface geometry from MCS images to estimate the detailed shallow velocity structure, with particular focus on properties within the shallow subduction channel. We observe refractions and reflections in OBS data from the shallow part of the subduction <span class="hlt">zone</span> in both the Shumagin Gap and Semidi segment, including reflections off the top and base of what appears to be a layer of subducting <span class="hlt">sediment</span>, which can be used for this work. We plan to present initial models of the shallow part of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGeo..117...75Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGeo..117...75Y"><span>Estimates of effective elastic thickness at subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, An; Fu, Yongtao</p> <p>2018-06-01</p> <p>The effective elastic thickness (Te) is an important parameter that characterizes the long-term strength of the lithosphere. Estimates of Te at subduction <span class="hlt">zones</span> have important tectonic and geodynamic implications, providing constraints for the strength of the oceanic lithosphere at a short-term scale. We estimated Te values in several subduction <span class="hlt">zones</span> worldwide by using models including both surface and subsurface loads from the analysis of free-air gravity anomaly and bathymetric data, together with a moving window admittance technique (MWAT). Tests with synthetic gravity and bathymetry data show that this method is a reliable way to <span class="hlt">recover</span> Te of oceanic lithosphere. Our results show that there is a noticeable reduction in the effective elastic thickness of the subducting plate from the outer rise to the trench axis for most studied subduction <span class="hlt">zones</span>, suggesting plate weakening at the trench-outer rise of the subduction <span class="hlt">zones</span>. These subduction <span class="hlt">zones</span> have Te range of 6-60 km, corresponding to a wide range of isotherms from 200 to 800 °C. Different trenches show distinct patterns. The Caribbean, Kuril-Japan, Mariana and Tonga subduction <span class="hlt">zones</span> show predominantly high Te. By contrast, the Middle America and Java subduction <span class="hlt">zones</span> have a much lower Te. The Peru-Chile, Aleutian and Philippine subduction <span class="hlt">zones</span> show considerable scatter. The large variation of the isotherm for different trenches does not show clear relationship with plate weakening at the outer rise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007SedG..201..286B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007SedG..201..286B"><span>Non-seagrass meadow sedimentary facies of the Pontinian Islands, Tyrrhenian Sea: A modern example of mixed carbonate siliciclastic <span class="hlt">sedimentation</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brandano, Marco; Civitelli, Giacomo</p> <p>2007-10-01</p> <p> epibathyal <span class="hlt">zones</span> that represent shelf-break and upper slope <span class="hlt">sedimentation</span>. The Maerl facies (F4a,b; mf4a,b) and the skeletal sands (F2a,b; mf2a1, mf2a2, mf2b) fall within the circalittoral <span class="hlt">zone</span>. The circalittoral <span class="hlt">zone</span> in the water depth interval between 82 m and 112 m display relict facies (F6, mf6). Finally facies F5 (Siliciclastic sands) includes subfacies F5b (mf5b), located in the circalittoral <span class="hlt">zone</span> at depths of 49 to 101 mwd and restricted to the western and eastern sectors of Ponza, and subfacies F5a in the upper infralittoral <span class="hlt">zone</span> (15 mwd/25 mwd) where erosional processes prevail. Carbonate content analyses indicate that maximum carbonate production on the Pontinian shelf took place in the 60-80 mwd interval. Facies F4 (Maerl) represents the environment characterized by the highest carbonate production rates. In the Pontian area siliciclastic-carbonate mixing took place in the infralittoral <span class="hlt">zone</span> and in the lower circalittoral <span class="hlt">zone</span>. In the infralittoral <span class="hlt">zone</span> erosional processes on the rocky shoreline produced lithoclasts and vulcanoclastic deposits that were reworked by wave-induced near-shore currents. In the lower circalittoral <span class="hlt">zone</span> the prolific production by photic biota (red algae) ends, while skeletal remains of the aphotic environment mixes with planktonic <span class="hlt">sediments</span> characterized by low carbonate values. Sand (63 μm-2 mm) is the dominant grain size class, however gravel-dominated facies (F4 Maerl) are present in water depths (50 to 112 mwd) which are significantly below the storm wave base. Glauconite mineralization appears on the Pontinian shelf from 50 mwd and increases in abundance along the deeper bathymetries. The compositional characteristics of relict facies F6 shows the concurrence of biota assemblages of the infralittoral and circalittoral <span class="hlt">zones</span>, likely representing the record of the last Holocene transgressive event (18 ky) and expressed by the overlapping of components of different environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28984430','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28984430"><span>Modeling <span class="hlt">sediment</span> transport in Qatar: Application for coastal development planning.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yousif, Ruqaiya; Warren, Christopher; Ben-Hamadou, Radhouan; Husrevoglu, Sinan</p> <p>2018-03-01</p> <p>Hydrodynamics and <span class="hlt">sediment</span> transport are key physical processes contributing to habitat structure within the marine environment. Coastal development that results in the alteration of these processes (e.g., changing water flushing and/or <span class="hlt">sedimentation</span> rates) can have detrimental impacts on sensitive systems. This is a current, relevant issue in Qatar as its coastal regions continue to be developed, not only around the capital of Doha, but in many areas around this Arabian Gulf peninsula. The northeastern Qatari coast is comprised of diverse and sensitive flora and fauna such as seagrass and macroalgae meadows, coral reefs and patches, turtles, and dugongs that tolerate harsh environmental conditions. In the near future, this area may see a rise in anthropogenic activity in the form of coastal development projects. These projects will add to existing natural stresses, such as high temperature, high salinity, and low rates of precipitation. Consequently, there is a need to characterize this area and assess the potential impacts that these anthropogenic activities may have on the region. In the present study, a novel <span class="hlt">sediment</span> transport model is described and used to demonstrate the potential impact of altering hydrodynamics and subsequent <span class="hlt">sediment</span> transport along the northeastern Qatar nearshore marine environment. The developed models will be tested using potential scenarios of future anthropogenic activities forecasted to take place in the area. The results will show the effects on water and <span class="hlt">sediment</span> behavior and provide a scientific approach for key stakeholders to make decisions with respect to the management of the considered coastal <span class="hlt">zone</span>. Furthermore, it provides a tool and framework that can be utilized in environmental impact assessment and associated hydrodynamic studies along other areas of the Qatari coastal <span class="hlt">zone</span>. Integr Environ Assess Manag 2018;14:240-251. © 2017 SETAC. © 2017 SETAC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMEP53D1009M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMEP53D1009M"><span>Modification of the Undertow and Turbulence by Submerged Vegetation in a Laboratory Surf <span class="hlt">Zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mandel, T.; Suckale, J.; Marras, S.; Maldonado, S.; Koseff, J. R.</p> <p>2016-12-01</p> <p>Breaking waves in the surf <span class="hlt">zone</span> are a dominant factor shaping the evolution of our coastlines. The turbulence generated by wave breaking causes <span class="hlt">sediment</span> resuspension, while wave runup, rundown, and the undertow transport this <span class="hlt">sediment</span> along and across the shore (Longo et al., 2002). Coastal hazard models must now address the added complications of climate change, including sea level rise, stronger storm events, and ecosystem degradation (Arkema et al., 2013). A robust theoretical understanding of surf <span class="hlt">zone</span> dynamics is therefore imperative to considering the magnitude and implications of these potential changes. However, little work has been done to extend our current theoretical understanding to realistic beach faces, with aquatic vegetation, reefs, and other roughness elements that might mitigate scour and <span class="hlt">sedimentation</span>. Clarifying these relationships will help scientists and policy-makers decide where to focus ecosystem restoration and preservation efforts, in order to maximize their protective benefits to infrastructure and economic activity on the coast. In order to evaluate the role of vegetation in coastal protection, we conducted a series of experiments in an idealized laboratory surf <span class="hlt">zone</span>. We examine the impact of submerged model vegetation on the undertow profile, wave orbital velocities, turbulent kinetic energy, and wave-induced stresses, and compare these results to theoretical formulations that model these quantities. We find that vegetation reduces the wave energy available to be converted to turbulent kinetic energy during breaking, indicating a mechanism to mitigate suspension of <span class="hlt">sediment</span>. Vegetation also reduces the magnitude of the undertow, likely reducing transport of <span class="hlt">sediment</span> offshore. These results suggest that vegetation provides significant protective benefits for coastal communities at risk from erosion beyond its well-characterized ability to attenuate wave height, and motivate further work to incorporate these effects into models of near</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14..683B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14..683B"><span>Long-distance electron transport occurs globally in marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Burdorf, Laurine D. W.; Tramper, Anton; Seitaj, Dorina; Meire, Lorenz; Hidalgo-Martinez, Silvia; Zetsche, Eva-Maria; Boschker, Henricus T. S.; Meysman, Filip J. R.</p> <p>2017-02-01</p> <p>Recently, long filamentous bacteria have been reported conducting electrons over centimetre distances in marine <span class="hlt">sediments</span>. These so-called cable bacteria perform an electrogenic form of sulfur oxidation, whereby long-distance electron transport links sulfide oxidation in deeper <span class="hlt">sediment</span> horizons to oxygen reduction in the upper millimetres of the <span class="hlt">sediment</span>. Electrogenic sulfur oxidation exerts a strong impact on the local <span class="hlt">sediment</span> biogeochemistry, but it is currently unknown how prevalent the process is within the seafloor. Here we provide a state-of-the-art assessment of its global distribution by combining new field observations with previous reports from the literature. This synthesis demonstrates that electrogenic sulfur oxidation, and hence microbial long-distance electron transport, is a widespread phenomenon in the present-day seafloor. The process is found in coastal <span class="hlt">sediments</span> within different climate <span class="hlt">zones</span> (off the Netherlands, Greenland, the USA, Australia) and thrives on a range of different coastal habitats (estuaries, salt marshes, mangroves, coastal hypoxic basins, intertidal flats). The combination of a widespread occurrence and a strong local geochemical imprint suggests that electrogenic sulfur oxidation could be an important, and hitherto overlooked, component of the marine cycle of carbon, sulfur and other elements.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.2741M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.2741M"><span>Planktonic foraminifera-derived environmental DNA extracted from abyssal <span class="hlt">sediments</span> preserves patterns of plankton macroecology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morard, Raphaël; Lejzerowicz, Franck; Darling, Kate F.; Lecroq-Bennet, Béatrice; Winther Pedersen, Mikkel; Orlando, Ludovic; Pawlowski, Jan; Mulitza, Stefan; de Vargas, Colomban; Kucera, Michal</p> <p>2017-06-01</p> <p>Deep-sea <span class="hlt">sediments</span> constitute a unique archive of ocean change, fueled by a permanent rain of mineral and organic remains from the surface ocean. Until now, paleo-ecological analyses of this archive have been mostly based on information from taxa leaving fossils. In theory, environmental DNA (eDNA) in the <span class="hlt">sediment</span> has the potential to provide information on non-fossilized taxa, allowing more comprehensive interpretations of the fossil record. Yet, the process controlling the transport and deposition of eDNA onto the <span class="hlt">sediment</span> and the extent to which it preserves the features of past oceanic biota remains unknown. Planktonic foraminifera are the ideal taxa to allow an assessment of the eDNA signal modification during deposition because their fossils are well preserved in the <span class="hlt">sediment</span> and their morphological taxonomy is documented by DNA barcodes. Specifically, we re-analyze foraminiferal-specific metabarcodes from 31 deep-sea <span class="hlt">sediment</span> samples, which were shown to contain a small fraction of sequences from planktonic foraminifera. We confirm that the largest portion of the metabarcode originates from benthic bottom-dwelling foraminifera, representing the in situ community, but a small portion (< 10 %) of the metabarcodes can be unambiguously assigned to planktonic taxa. These organisms live exclusively in the surface ocean and the <span class="hlt">recovered</span> barcodes thus represent an allochthonous component deposited with the rain of organic remains from the surface ocean. We take advantage of the planktonic foraminifera portion of the metabarcodes to establish to what extent the structure of the surface ocean biota is preserved in sedimentary eDNA. We show that planktonic foraminifera DNA is preserved in a range of marine <span class="hlt">sediment</span> types, the composition of the <span class="hlt">recovered</span> eDNA metabarcode is replicable and that both the similarity structure and the diversity pattern are preserved. Our results suggest that sedimentary eDNA could preserve the ecological structure of the entire pelagic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/5223369','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/5223369"><span>Toxicity of <span class="hlt">sediments</span> and pore water from Brunswick Estuary, Georgia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Winger, Parley V.; Lasier, Peter J.; Geitner, Harvey</p> <p>1993-01-01</p> <p>A chlor-alkali plant in Brunswick, Georgia, USA, discharged >2 kg mercury/d into a tributary of the Turtle River-Brunswick Estuary from 1966 to 1971. Mercury concentrations in <span class="hlt">sediments</span> collected in 1989 along the tributary near the chlor-alkali plant ranged from 1 to 27 μg/g (dry weight), with the highest concentrations found in surface (0–8 cm) <span class="hlt">sediments</span> of subtidal <span class="hlt">zones</span> in the vicinity of the discharge site. Toxicity screening in 1990 using Microtox® bioassays on pore water extracted on site from <span class="hlt">sediments</span> collected at six stations distributed along the tributary indicated that pore water was highly toxic near the plant discharge. Ten-day toxicity tests on pore water from subsequent <span class="hlt">sediment</span> samples collected near the plant discharge confirmed high toxicity to Hyalella azteca, and feeding activity was significantly reduced in whole-<span class="hlt">sediment</span> tests. In addition to mercury in the <span class="hlt">sediments</span>, other metals (chromium, lead, and zinc) exceeded 50 μg/g, and polychlorobiphenyl (PCB) concentrations ranged from 67 to 95 μg/g. On a molar basis, acid-volatile sulfide concentrations (20–45 μmol/g) in the <span class="hlt">sediments</span> exceeded the metal concentrations. Because acid-volatile sulfides bind with cationic metals and form metal sulfides, which are generally not bioavailable, toxicities shown by these <span class="hlt">sediments</span> were attributed to the high concentrations of PCBs and possibly methylmercury.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014CSR....82...72O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014CSR....82...72O"><span>Flocculation and <span class="hlt">sediment</span> deposition in a hypertidal creek</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Laughlin, C.; van Proosdij, D.; Milligan, T. G.</p> <p>2014-07-01</p> <p>In the hypertidal Bay of Fundy, environmental impacts in response to commercial-scale tidal power development remain to be fully understood. The extraction of tidal energy may impact <span class="hlt">sediment</span> dynamics in far-field environments, such as the intertidal <span class="hlt">zone</span>, through potential alterations to tidal amplitude in the Minas Basin. Tidal conditions (e.g. current velocity, turbulence, suspended <span class="hlt">sediment</span> concentration) were monitored in a sheltered salt marsh creek over 18 tidal cycles in various stages of the spring-neap cycle. Samples of deposited and suspended <span class="hlt">sediments</span> were collected and analyzed for grain size using a Beckman Coulter Multisizer III. Results suggest that the flocculated component of both deposited and suspended <span class="hlt">sediment</span> is consistently high over a wide range of tidal conditions. A routinely high incoming concentration of highly-flocculated material results in large amounts of <span class="hlt">sediment</span> deposition in tidal creeks in response to individual tidal cycles. Resuspension and removal of newly deposited material is shown to vary with over-marsh, bankfull and channel-restricted tides. Disruption of the tidal regime due to a reduction in Minas Basin tidal amplitude may lessen the cumulative export capacity of tidal channels over time, potentially leading to gradual infilling of tidal creeks. The long-term effects of tidal power development on intertidal areas are generally unknown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1041003','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1041003"><span>Methane Recovery from Hydrate-bearing <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>J. Carlos Santamarina; Costas Tsouris</p> <p>2011-04-30</p> <p> emphasis; (6) detailed study of CH4-CO2 exchange as a unique alternative to <span class="hlt">recover</span> CH4 gas while sequestering CO2; (7) the relevance of fines in otherwise clean sand <span class="hlt">sediments</span> on gas recovery and related phenomena such as fines migration and clogging, vuggy structure formation, and gas-driven fracture formation during gas production by depressurization.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033805','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033805"><span>Geologic columns for the ICDP-USGS Eyreville A and C cores, Chesapeake Bay impact structure: Postimpact <span class="hlt">sediments</span>, 444 to 0 m depth</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Edwards, L.E.; Powars, D.S.; Browning, J.V.; McLaughlin, P.P.; Miller, K.G.; ,; Kulpecz, A.A.; Elbra, T.</p> <p>2009-01-01</p> <p>A 443.9-m-thick, virtually undisturbed section of postimpact deposits in the Chesapeake Bay impact structure was <span class="hlt">recovered</span> in the Eyreville A and C cores, Northampton County, Virginia, within the "moat" of the structure's central crater. <span class="hlt">Recovered</span> <span class="hlt">sediments</span> are mainly fine-grained marine siliciclastics, with the exception of Pleistocene sand, clay, and gravel. The lowest postimpact unit is the upper Eocene Chickahominy Formation (443.9-350.1 m). At 93.8 m, this is the maximum thickness yet <span class="hlt">recovered</span> for deposits that represent the return to "normal marine" <span class="hlt">sedimentation</span>. The Drummonds Corner beds (informal) and the Old Church Formation are thin Oligocene units present between 350.1 and 344.7 m. Above the Oligocene, there is a more typical Virginia coastal plain succession. The Calvert Formation (344.7-225.4 m) includes a thin lower Miocene part overlain by a much thicker middle Miocene part. From 225.4 to 206.0 m, <span class="hlt">sediments</span> of the middle Miocene Choptank Formation, rarely reported in the Virginia coastal plain, are present. The thick upper Miocene St. Marys and Eastover Formations (206.0-57.8 m) appear to represent a more complete succession than in the type localities. Correlation with the nearby Kiptopeke core indicates that two Pliocene units are present: Yorktown (57.8-32.2 m) and Chowan River Formations (32.2-18.3 m). <span class="hlt">Sediments</span> at the top of the section represent an upper Pleistocene channel-fill and are assigned to the Butlers Bluff and Occohannock Members of the Nassawadox Formation (18.3-0.6 m). ?? 2009 The Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035615','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035615"><span>Microbial abundance in the deep subsurface of the Chesapeake Bay impact crater: Relationship to lithology and impact processes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cockell, Charles S.; Gronstal, Aaron L.; Voytek, Mary A.; Kirshtein, Julie D.; Finster, Kai; Sanford, Ward E.; Glamoclija, Mihaela; Gohn, Gregroy S.; Powars, David S.; Horton, J. Wright</p> <p>2009-01-01</p> <p>Asteroid and comet impact events are known to cause profound disruption to surface ecosystems. The aseptic collection of samples throughout a 1.76-km-deep set of cores <span class="hlt">recovered</span> from the deep subsurface of the Chesapeake Bay impact structure has allowed the study of the subsurface biosphere in a region disrupted by an impactor. Microbiological enumerations suggest the presence of three major microbiological <span class="hlt">zones</span>. The upper <span class="hlt">zone</span> (127–867 m) is characterized by a logarithmic decline in microbial abundance from the surface through the postimpact section of Miocene to Upper Eocene marine <span class="hlt">sediments</span> and across the transition into the upper layers of the impact tsunami resurge <span class="hlt">sediments</span> and <span class="hlt">sediment</span> megablocks. In the middle <span class="hlt">zone</span> (867–1397 m) microbial abundances are below detection. This <span class="hlt">zone</span> is predominantly quartz sand, primarily composed of boulders and blocks, and it may have been mostly sterilized by the thermal pulse delivered during impact. No samples were collected from the large granite block (1096–1371 m). The lowest <span class="hlt">zone</span> (below 1397 m) of increasing microbial abundance coincides with a region of heavily impact-fractured, hydraulically conductive suevite and fractured schist. These <span class="hlt">zones</span> correspond to lithologies influenced by impact processes. Our results yield insights into the influence of impacts on the deep subsurface biosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.B11I0562B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.B11I0562B"><span>Marine Subsurface Microbial Communities Across a Hydrothermal Gradient in Okinawa Trough <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brandt, L. D.; Hser Wah Saw, J.; Ettema, T.; House, C. H.</p> <p>2015-12-01</p> <p>IODP Expedition 331 to the Okinawa backarc basin provided an opportunity to study the microbial stratigraphy within the <span class="hlt">sediments</span> surrounding a hydrothermal vent. The Okinawa backarc basin is a <span class="hlt">sedimented</span> region of the seafloor located on a continental margin, and also hosts a hydrothermal network within the subsurface. Site C0014 within the Iheya North hydrothermal field is located 450 m east of the active vent and has a surface temperature of 5°C with no evidence of hydrothermal alteration within the top 10 meters below sea floor (mbsf). Temperature increases with depth at an estimated rate of 3°C/m and transitions from non-hydrothermal margin <span class="hlt">sediments</span> to a hydrothermally altered regime below 10 mbsf. In this study, we utilized deep 16S rRNA sequencing of DNA from IODP Expedition 331 Site C0014 <span class="hlt">sediment</span> horizons in order to assess diversity throughout the <span class="hlt">sediment</span> column as well as determine the potential limits of the biosphere. Analysis of the amplicon data shows a shift over 15 mbsf from a heterogeneous community of cosmopolitan marine subsurface taxa toward an archaeal-dominated community in the deepest horizons of the predicted biosphere. Notably, the phylum Chloroflexi represents a substantial taxon through most horizons, where it appears to be replaced below 10 mbsf by punctuations of thermophilic and methanotrophic Archaea and Miscellaneous Crenarchaeotic Group abundances. DNA from the aforementioned transition horizons was further analyzed using metagenomic sequencing. Preliminary taxonomic analysis of the metagenomic data agrees well with amplicon data in capturing the shift in relative abundance of Archaea increasing with depth. Additionally, reverse gyrase, a gene found exclusively in hyperthermophilic microorganisms, was <span class="hlt">recovered</span> only in the metagenome of the deepest horizon. A BLAST search of this protein sequence against the GenBank non-redudnant protein database produced top hits with reverse gyrase from Thermococcus and Pyrococcus, which are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeCoA.188..297F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeCoA.188..297F"><span>Controls on subsurface methane fluxes and shallow gas formation in Baltic Sea <span class="hlt">sediment</span> (Aarhus Bay, Denmark)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flury, Sabine; Røy, Hans; Dale, Andrew W.; Fossing, Henrik; Tóth, Zsuzsanna; Spiess, Volkhard; Jensen, Jørn Bo; Jørgensen, Bo Barker</p> <p>2016-09-01</p> <p>Shallow gas accumulates in coastal marine <span class="hlt">sediments</span> when the burial rate of reactive organic matter beneath the sulfate <span class="hlt">zone</span> is sufficiently high and the methanogenic <span class="hlt">zone</span> is sufficiently deep. We investigated the controls on methane production and free methane gas accumulation along a 400 m seismo-acoustic transect across a sharp transition from gas-free into gas-bearing <span class="hlt">sediment</span> in Aarhus Bay (Denmark). Twelve gravity cores were taken, in which the pore water was analyzed for inorganic solutes while rates of organic carbon mineralization were measured experimentally by 35SO42- radiotracer method. The thickness of organic-rich Holocene mud increased from 5 to 10 m along the transect concomitant with a shallowing of the depth of the sulfate-methane transition from >4 m to 2.5 m. In spite of drastic differences in the distribution of methane and sulfate in the <span class="hlt">sediment</span> along the transect, there were only small differences in total mineralization, and methanogenesis was only equivalent to about 1% of sulfate reduction. Shallow gas appeared where the mud thickness exceeded 8-9 m. Rates of methanogenesis increased along the transect as did the upward diffusive flux of methane. Interestingly, the increase in the <span class="hlt">sedimentation</span> rate and Holocene mud thickness had only a modest direct effect on methanogenesis rates in deep <span class="hlt">sediments</span>. This increase in methane flux, however, triggered a shallowing of the sulfate-methane transition which resulted in a large increase in methanogenesis at the top of the methanogenic <span class="hlt">zone</span>. Thus, our results demonstrate a positive feedback mechanism that causes a strong enhancement of methanogenesis and explains the apparently abrupt appearance of gas when a threshold thickness of organic-rich mud is exceeded.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..115M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..115M"><span>Soil conservation through <span class="hlt">sediment</span> trapping: A review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mekonnen, Mulatie; Keesstra, Saskia; Baartman, Jantiene; Maroulis, Jerry; Stroosnijder, Leo</p> <p>2014-05-01</p> <p>Preventing the off-site effects of soil erosion is an essential part of good catchment management. Most efforts are in the form of on-site soil and water conservation measures. However, <span class="hlt">sediment</span> trapping (ST) can be an alternative (or additional) measure to prevent the negative off-site effects of soil erosion. Therefore, not all efforts should focus solely on on-site soil conservation, but also on the safe routing of <span class="hlt">sediment</span>-laden flows and on creating sites and conditions where <span class="hlt">sediment</span> can be trapped, preferably in a cost effective or even profitable way. ST can be applied on-site (in-field) and off-site and involves both vegetative and structural measures. The main vegetative measures include grass strips, tree or bush buffers, grassed waterways and restoration of the waterways and their riparian <span class="hlt">zone</span>; while structural measures include terraces, ponds and check dams. This paper provides a review of studies that have assessed the <span class="hlt">sediment</span> trapping efficacy (STE) of such vegetative and structural measures. Vegetation type and integration of two or more measures (vegetative as well as structural) are important factors influencing STE. In this review, the STE of most measures was evaluated either individually or in such combinations. In real landscape situations, it is not only important to select the most efficient erosion control measures, but also to determine their optimum location in the catchment. Hence, there is a need for research that shows a more integrated determination of STE at the catchment scale. If integrated measures are implemented at the most appropriate spatial locations within a catchment where they can disconnect landscape units from each other, they will decrease runoff velocity and <span class="hlt">sediment</span> transport and, subsequently, reduce downstream flooding and <span class="hlt">sedimentation</span> problems. KEY WORDS: Integrated <span class="hlt">sediment</span> trapping, <span class="hlt">sediment</span> trapping efficacy, vegetative, structural, on-site and off-site measures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70018101','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70018101"><span>Microbial acetogenesis as a source of organic acids in ancient Atlantic Coastal Plain <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chapelle, F.H.; Bradley, P.M.</p> <p>1996-01-01</p> <p>Field and laboratory evidence shows that deeply buried (90-888 m) fine-grained <span class="hlt">sediments</span> of the Atlantic Coastal Plain contain viable acetogenic microorganisms, and that these microorganisms actively produce organic acids. Concentrations of formate, acetate, and propionate in pore waters extracted from fine-grained <span class="hlt">sediments</span> ranged from 50 ??M to 5 mM and were much higher than in adjacent pore waters associated with sandy <span class="hlt">sediments</span> (<2 ??M). Laboratory studies showed that asceptically cored fine-grained <span class="hlt">sediments</span> incubated under a H2 atmosphere produced formate and acetate, and that H14CO-3 was converted to 14C-acetate and 14C-formate over time. An enrichment culture of these acetogenic microorganisms was <span class="hlt">recovered</span> from one long-term incubation that showed the presence of several morphologically distinct gram-positive, rod-shaped bacteria. These microorganisms were capable of growth under autotrophic (H2 + CO2), heterotrophic (syringate), and mixotrophic (H2 + CO2 + syringate) conditions. These results suggest that microbial acetogenesis, rather than abiotic processes, is the most important organic acid-producing mechanism during low-temperature (???30 ??C) diagenesis of Atlantic Coastal Plain <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2015/5127/sir20155127.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2015/5127/sir20155127.pdf"><span>Characteristics of <span class="hlt">sediment</span> transport at selected sites along the Missouri River, 2011–12</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rus, David L.; Galloway, Joel M.; Alexander, Jason S.</p> <p>2015-10-22</p> <p>The Modified-Einstein Procedure tended to predict greater total-<span class="hlt">sediment</span> loads when compared to measured values. These differences may be the result of <span class="hlt">sediment</span> deficits in the Missouri River that lead to an overprediction by the Modified-Einstein Procedure, the unsampled <span class="hlt">zone</span> above the streambed that leads to an underprediction by the suspended sampler, or general uncertainty in the sampling approach. The differences between total-<span class="hlt">sediment</span> load obtained through measurements and that estimated from applied theoretical procedures such as the Modified-Einstein Procedure pose a challenge for reliably characterizing total-<span class="hlt">sediment</span> transport. Though it is not clear which of the two techniques is more accurate, the general tendency of the two to be within an order of magnitude of one another may be adequate for many <span class="hlt">sediment</span> studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.712..182G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.712..182G"><span>Rock strength measurements on Archaean basement granitoids <span class="hlt">recovered</span> from scientific drilling in the active Koyna seismogenic <span class="hlt">zone</span>, western India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goswami, Deepjyoti; Akkiraju, Vyasulu V.; Misra, Surajit; Roy, Sukanta; Singh, Santosh K.; Sinha, Amalendu; Gupta, Harsh; Bansal, B. K.; Nayak, Shailesh</p> <p>2017-08-01</p> <p>Reservoir triggered earthquakes have been occurring in the Koyna area, western India for the past five decades. Triaxial tests carried out on 181 core samples of Archaean granitoids underlying the Deccan Traps provide valuable constraints on rock strength properties in the Koyna seismogenic <span class="hlt">zone</span> for the first time. The data include measurements on granite gneiss, granite, migmatitic gneiss and mylonitised granite gneiss obtained from boreholes KBH-3, KBH-4A, KBH-5 and KBH-7 located in the western and eastern margins of the seismic <span class="hlt">zone</span>. Salient results are as follows. (i) Increase of rock strength with increasing confining pressure allow determination of the linearized failure envelopes from which the cohesive strength and angle of internal friction are calculated. (ii) Variable differential stresses at different depths are the manifestations of deformation partitioning in close association of fault <span class="hlt">zone(s</span>) or localized fracture <span class="hlt">zones</span>. (iii) Fractures controlled by naturally developed weak planes such as cleavage and fabric directly affect the rock strength properties, but the majority of failure planes developed during triaxial tests is not consistent with the orientations of pre-existing weak planes. The failure planes may, therefore, represent other planes of weakness induced by ongoing seismic activity. (iv) Stress-strain curves confirm that axial deformation is controlled by the varying intensity of pre-existing shear in the granitoids, viz., mylonite, granite gneiss and migmatitic gneiss. (v) Frequent occurrences of low magnitude earthquakes may be attributed to low and variable rock strength of the granitoids, which, in turn, is modified by successive seismic events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1862c0144P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1862c0144P"><span>Comparative study of original <span class="hlt">recover</span> and <span class="hlt">recover</span> KL in separable non-negative matrix factorization for topic detection in Twitter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prabandari, R. D.; Murfi, H.</p> <p>2017-07-01</p> <p>An increasing amount of information on social media such as Twitter requires an efficient way to find the topics so that the information can be well managed. One of an automated method for topic detection is separable non-negative matrix factorization (SNMF). SNMF assumes that each topic has at least one word that does not appear on other topics. This method uses the direct approach and gives polynomial-time complexity, while the previous methods are iterative approaches and have NP-hard complexity. There are three steps of SNMF algorithm, i.e. constructing word co-occurrences, finding anchor words, and <span class="hlt">recovering</span> topics. In this paper, we examine two topic <span class="hlt">recover</span> methods, namely original <span class="hlt">recover</span> that is using algebraic manipulation and <span class="hlt">recover</span> KL that using probability approach with Kullback-Leibler divergence. Our simulations show that <span class="hlt">recover</span> KL provides better accuracies in term of topic recall than original <span class="hlt">recover</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27090527','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27090527"><span>Spatial distribution and risk assessment of heavy metals and As pollution in the <span class="hlt">sediments</span> of a shallow lake.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Deng, Jiancai; Wang, Yuansheng; Liu, Xin; Hu, Weiping; Zhu, Jinge; Zhu, Lin</p> <p>2016-05-01</p> <p>The concentrations and spatial distributions of eight heavy metals in surface <span class="hlt">sediments</span> and <span class="hlt">sediment</span> core samples from a shallow lake in China were investigated to evaluate the extent of the contamination and potential ecological risks. The results showed that the heavy metal concentrations were higher in the northern and southwestern lake <span class="hlt">zones</span> than those in the other lake <span class="hlt">zones</span>, with lower levels of As, Hg, Zn, Cu, Pb, Cr, and Ni primarily observed in the central and eastern lake regions and Cd primarily confined to areas surrounding the lake. The concentrations of the eight heavy metals in the <span class="hlt">sediment</span> profiles tended to decrease with increasing <span class="hlt">sediment</span> depth. The contents of Ni, Cu, Zn, Pb, and Cd in the surface <span class="hlt">sediment</span> were approximately 1.23-18.41-fold higher than their background values (BVs), whereas the contents of Cr, As, and Hg were nearly identical to their BVs. The calculated pollution load index (PLI) suggested that the surface <span class="hlt">sediments</span> of this lake were heavily polluted by these heavy metals and indicated that Cd was a predominant contamination factor. The comprehensive potential ecological risk index (PERI) in the surface <span class="hlt">sediments</span> ranged from 99.2 to 2882.1, with an average of 606.1. Cd contributed 78.7 % to the PERI, and Hg contributed 8.4 %. Multivariate statistical analyses revealed that the surface <span class="hlt">sediment</span> pollution with heavy metals mainly originated from industrial wastewater discharged by rivers located in the western and northwestern portion of the lake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H51H..02D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H51H..02D"><span>Optimization of Remediation Conditions using Vadose <span class="hlt">Zone</span> Monitoring Technology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dahan, O.; Mandelbaum, R.; Ronen, Z.</p> <p>2010-12-01</p> <p> irrigation system to enrich the percolating water. The vadose <span class="hlt">zone</span> monitoring system that was installed at the site allowed accurate monitoring of the wetting cycles, including: (1) wetting front propagation velocities, (2) temporal variation of the <span class="hlt">sediment</span> water content, (2) chemical composition of the percolating water, (3) isotopic composition of BTEX compounds, (4) variations in nutrient concentration, and (5) variations in the vadose <span class="hlt">zone</span> redox potential. Preliminary results showed that the wetting front crossed the entire vadose <span class="hlt">zone</span> in four days reaching maximum water content values of 12 to 18 %. Temporal variation in the <span class="hlt">sediment</span> BTEX concentrations indicated significant reduction in highly soluble and mobile compounds such as MTBE. Yet the chemical composition of the water samples through the first sampling campaign indicated that the limiting factor for biodegradation at the first wetting cycle was insufficient nitrogen. Results from each wetting cycles were used to improve the following wetting cycles in order to optimize the vadose <span class="hlt">zone</span> conditions for microbial activity while minimizing leaching of contaminants to the groundwater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JSR....86...58H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JSR....86...58H"><span>The importance of benchmarking habitat structure and composition for understanding the extent of fishing impacts in soft <span class="hlt">sediment</span> ecosystems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Handley, Sean J.; Willis, Trevor J.; Cole, Russell G.; Bradley, Anna; Cairney, Daniel J.; Brown, Stephen N.; Carter, Megan E.</p> <p>2014-02-01</p> <p>Trawling and dredge fisheries remove vulnerable fauna, homogenise <span class="hlt">sediments</span> and assemblages, and break down biogenic habitats, but the full extent of these effects can be difficult to quantify in the absence of adequate control sites. Our study utilised rare control sites containing biogenic habitat, the Separation Point exclusion <span class="hlt">zone</span>, formally protected for 28 years, as the basis for assessing the degree of change experienced by adjacent areas subject to benthic fishing. Sidescan sonar surveys verified that intensive trawling and dredging occurred in areas adjacent to, but not inside, the exclusion area. We compared <span class="hlt">sediment</span> composition, biogenic cover, macrofaunal assemblages, biomass, and productivity of the benthos, inside and outside the exclusion <span class="hlt">zone</span>. Disturbed sites were dominated by fine mud, with little or no shell-gravel, reduced number of species, and loss of large bodied animals, with concomitant reductions in biomass and productivity. At protected sites, large, rarer molluscs were more abundant and contributed the most to size-based estimates of productivity and biomass. Functional changes in fished assemblages were consistent with previously reported relative increases in scavengers, predators and deposit feeders at the expense of filter feeders and a grazer. We propose that the colonisation of biogenic species in protected sites was contingent on the presence of shell-gravel atop these soft <span class="hlt">sediments</span>. The process of <span class="hlt">sediment</span> homogenisation by bottom fishing and elimination of shell-gravels from surficial <span class="hlt">sediments</span> appeared to have occurred over decades - a ‘shifting baseline’. Therefore, benchmarking historical <span class="hlt">sediment</span> structure at control site like the Separation Point exclusion <span class="hlt">zone</span> is necessary to determine the full extent of physical habitat change wrought by contact gears on sheltered soft <span class="hlt">sediment</span> habitats to better underpin appropriate conservation, restoration or fisheries management goals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.B23C0592R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.B23C0592R"><span>210Pb <span class="hlt">sediment</span> dating in coastal transition <span class="hlt">zones</span>: tropical saltmarshes.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ruiz-Fernandez, A. C.; Sanchez-Cabeza, J. A.; Carnero-Bravo, V.; Perez-Bernal, L. H.</p> <p>2016-12-01</p> <p>Sea level rise (SLR) is one of the climate change effects expected to have the largest impact on coastal environments. SLR rates are not uniform around the planet and, therefore, local and regional data and trends are needed for proper adaptation plans. As long term monitoring stations of SLR are very scarce in most of the world, SLR trends obtained from 210Pb-dated <span class="hlt">sediment</span> cores from tropical saltmarshes have become a practical alternative to obtain SLR trends within the past century, under the assumption that these ecosystems accrete at a similar rate to SLR. However, tropical saltmarshes are challenging environments for 210Pb dating: they are regularly dry, intermittently covered by seawater only during the highest tides, and sedimentary records often reflect the transition between terrestrial and marine environments (e.g. changes in grain size distribution, organic matter content and elemental composition) with all these factors contributing for atypical 210Pb depth profiles. In addition, 137Cs, the chronostratigraphic marker most commonly used to corroborate 210Pb dating, fails to be preserved in the sedimentary record in tropical areas, owing to its solubility in marine waters, if at all detectable. The present study describes the challenges and proposed solutions for 210Pb dating saltmarsh <span class="hlt">sediment</span> cores from two saltmarsh areas (southern Gulf of California and Yucatan Peninsula) including the use of plutonium isotopes for corroboration purposes. Acknowledgements: projects CONACYT CB2010/153492 and PDCPN201301/214349; UNAM PAPIIT-IN203313 and the PRODEP network "Aquatic contamination: levels and effects" (year 3).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995GeCoA..59.2435Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995GeCoA..59.2435Y"><span>Experimental study of boron geochemistry: implications for fluid processes in subduction <span class="hlt">zones</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>You, C. F.; Spivack, A. J.; Gieskes, J. M.; Rosenbauer, R.; Bischoff, J. L.</p> <p>1995-06-01</p> <p>A comprehensive experimental study, utilizing an autoclave hydrothermal apparatus with a 10B isotopic tracer, has been conducted to monitor the geochemical behavior of <span class="hlt">sediment</span> B during early subduction <span class="hlt">zone</span> processes. The partition coefficient of exchangeable B ( K D) was determined over a temperature range of 25-350°C, at 800 bars and a water/rock ratio of 3-1.5 w/w. These K D are shown to be a complex function of temperature, pH, and possibly mineralogy. At low temperatures, K D is significantly high at ˜4 in contrast to the value of essentially zero at temperatures higher than ˜100°C. A K D of zero represents no B adsorption, implying efficient mobilization of exchangeable B at shallow depths during <span class="hlt">sediment</span> subduction. Our experimental results demonstrate high mobilization of bulk B in <span class="hlt">sediments</span> (both exchangeable and lattice bound) at elevated temperatures (200-350°C), in good agreement with previous observations of B in metasediments indicating progressive depletion during metamorphism. In addition, this study emphasizes the importance of a possible water/rock ratio dependence of B mobilization. In other words, the degree of sedimentary B mobilization in subduction <span class="hlt">zones</span> strongly depends on the local thermal structure and porosity distribution. In low geothermal gradient areas, large amounts of porewater are expelled before significant B mobilization has occurred, so that some sedimentary B will survive and get into the deeper parts of the subduction <span class="hlt">zone</span>. Our results imply that efficient mobilization of B from the subducted slab must occur and that arc magmatism recycles most of the remaining subducted B back to surface reservoirs. A reconsideration of the B budget in subduction <span class="hlt">zones</span> provides critical information with respect to B sources and sinks in the ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRI...58..885M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRI...58..885M"><span>Deep-sea nematode assemblage has not <span class="hlt">recovered</span> 26 years after experimental mining of polymetallic nodules (Clarion-Clipperton Fracture <span class="hlt">Zone</span>, Tropical Eastern Pacific)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Miljutin, Dmitry M.; Miljutina, Maria A.; Arbizu, Pedro Martínez; Galéron, Joëlle</p> <p>2011-08-01</p> <p>We investigated nematode assemblages inhabiting the 26-year-old track created by experimental deep-sea mining of polymetallic nodules, and two adjacent, undisturbed sites, one with nodules and one without nodules. The aim was to compare density, assemblage structure, and diversity indices in order to assess the process of recovery of the nematode assemblage inhabiting the disturbed site. This experimental dredging was conducted in 1978 by the Ocean Minerals Company (USA) in the area of a French mining claim in the Clarion-Clipperton Fracture <span class="hlt">Zone</span> (Tropical Eastern Pacific) at a depth of about 5000 m. The nematode assemblage had not returned its initial state 26 years after the experimental dredging: the total nematode density and biomass within the dredging track were significantly lower than outside the track; the biodiversity indices showed significantly lower nematode diversity within the track; and the structure of the nematode assemblage within the track differed significantly from those in the two undisturbed sites outside the track. However, there were no significant differences in the mean body volumes of adult nematodes and adult-juvenile ratios between the track and reference sites. Parameters such as the rate of <span class="hlt">sediment</span> restoration (which depends on local hydrological conditions) and the degree and character of the disturbance appeared to be of considerable importance for the recovery rate of the deep-sea nematode assemblages and their ability to recolonize disturbed areas. The rates of recolonization and recovery may vary widely in different deep-sea regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2011-title40-vol31/pdf/CFR-2011-title40-vol31-sec721-4600.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title40-vol31/pdf/CFR-2011-title40-vol31-sec721-4600.pdf"><span>40 CFR 721.4600 - <span class="hlt">Recovered</span> metal hydroxide.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2011&page.go=Go">Code of Federal Regulations, 2011 CFR</a></p> <p></p> <p>2011-07-01</p> <p>... 40 Protection of Environment 31 2011-07-01 2011-07-01 false <span class="hlt">Recovered</span> metal hydroxide. 721.4600... Substances § 721.4600 <span class="hlt">Recovered</span> metal hydroxide. (a) Chemical substance and significant new uses subject to reporting. (1) The chemical substance identified generically as a <span class="hlt">recovered</span> metal hydroxide (PMN P-91-809...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_23 --> <div id="page_24" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="461"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26526906','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26526906"><span>Determination of refractive and volatile elements in <span class="hlt">sediment</span> using laser ablation inductively coupled plasma mass spectrometry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Duodu, Godfred Odame; Goonetilleke, Ashantha; Allen, Charlotte; Ayoko, Godwin A</p> <p>2015-10-22</p> <p>Wet-milling protocol was employed to produce pressed powder tablets with excellent cohesion and homogeneity suitable for laser ablation (LA) analysis of volatile and refractive elements in <span class="hlt">sediment</span>. The influence of sample preparation on analytical performance was also investigated, including sample homogeneity, accuracy and limit of detection. Milling in volatile solvent for 40 min ensured sample is well mixed and could reasonably <span class="hlt">recover</span> both volatile (Hg) and refractive (Zr) elements. With the exception of Cr (-52%) and Nb (+26%) major, minor and trace elements in STSD-1 and MESS-3 could be analysed within ±20% of the certified values. Comparison of the method with total digestion method using HF was tested by analysing 10 different <span class="hlt">sediment</span> samples. The laser method <span class="hlt">recovers</span> significantly higher amounts of analytes such as Ag, Cd, Sn and Sn than the total digestion method making it a more robust method for elements across the periodic table. LA-ICP-MS also eliminates the interferences from chemical reagents as well as the health and safety risks associated with digestion processes. Therefore, it can be considered as an enhanced method for the analysis of heterogeneous matrices such as river <span class="hlt">sediments</span>. Copyright © 2015 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wsp/2234e/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/2234e/report.pdf"><span>Shore erosion as a <span class="hlt">sediment</span> source to the tidal Potomac River, Maryland and Virginia</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Miller, Andrew J.</p> <p>1987-01-01</p> <p>The shoreline of the tidal Potomac River attained its present form as a result of the Holocene episode of sea-level rise; the drowned margins of the system are modified by wave activity in the shore <span class="hlt">zone</span> and by slope processes on banks steepened by basal-wave erosion. Shore erosion leaves residual sand and gravel in shallow water and transports silt and clay offshore to form a measurable component of the suspended-<span class="hlt">sediment</span> load of the tidal Potomac River. Erosion rates were measured by comparing digitized historical shoreline maps and modern maps, and by comparing stereopairs of aerial photographs taken at different points in time, with the aid of an interactive computer-graphics system and a digitizing stereoplotter. Cartographic comparisons encompassed 90 percent of the study reach and spanned periods of 38 to 109 years, with most measurements spanning at least 84 years. Photogrammetric comparisons encompassed 49 percent of the study reach and spanned 16 to 40 years. Field monitoring of erosion rates and processes at two sites, Swan Point Neck, Maryland, and Mason Neck, Virginia, spanned periods of 10 to 18 months. Estimated average recession rates of shoreline in the estuary, based on cartographic and photogrammetric measurements, were 0.42 to 0.52 meter per annum (Virginia shore) and 0.31 to 0.41 meter per annum (Maryland shore). Average recession rates of shoreline in the tidal river and transition <span class="hlt">zone</span> were close to 0.15 meter per annum. Estimated average volume-erosion rates along the estuary were 1.20 to 1.87 cubic meters per meter of shoreline per annum (Virginia shore) and 0.56 to 0.73 cubic meter per meter of shoreline per annum (Maryland shore); estimated average volume-erosion rates along the shores of the tidal river and transition <span class="hlt">zone</span> were 0.55 to 0.74 cubic meter per meter of shoreline per annum. Estimated total <span class="hlt">sediment</span> contributed to the tidal Potomac River by shore erosion was 0.375 x 10 6 to 0.565 x 10 6 metric tons per annum; of this, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29791448','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29791448"><span>Abundance and distribution of microplastics within surface <span class="hlt">sediments</span> of a key shellfish growing region of Canada.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kazmiruk, T N; Kazmiruk, V D; Bendell, L I</p> <p>2018-01-01</p> <p>The abundance and distribution of microplastics within 5 <span class="hlt">sediment</span> size classes (>5000 μm, 1000-5000 μm, 250-1000 μm, 250-0.63 μm and < 0.63 μm) were determined for 16 sites within Lambert Channel and Baynes Sound, British Columbia, Canada. This region is Canada's premier growing area for the Pacific oyster (Crassostrea gigas). Microplastics were found at all sampling locations indicating widespread contamination of this region with these particles. Three types of microplastics were <span class="hlt">recovered</span>: microbeads, which occurred in the greatest number (up to 25000/kg dry <span class="hlt">sediment</span>) and microfibers and microfragments, which were much less in number compared with microbeads and occurred in similar amounts (100-300/kg dry <span class="hlt">sediment</span>). Microbeads were <span class="hlt">recovered</span> primarily in the < 0.63 μm and 250-0.63 μm <span class="hlt">sediment</span> size class, whereas microfragments and microfibers were generally identified in all 5 <span class="hlt">sediment</span> size classes. Abundance and distribution of the three types of microplastics were spatially dependent with principal component analysis (PCA) indicating that 84 percent of the variation in abundance and distribution was due to the presence of high numbers of microbeads at three locations within the study region. At these sites, microbeads expressed as a percent component of the <span class="hlt">sediment</span> by weight was similar to key geochemical components that govern trace metal behavior and availability to benthic organisms. Microbeads have been shown to accumulate metals from the aquatic environment, hence in addition to the traditional geochemical components such as silt and organic matter, microplastics also need to be considered as a <span class="hlt">sediment</span> component that can influence trace metal geochemistry. Our findings have shown that BC's premier oyster growing region is highly contaminated with microplastics, notably microbeads. It would be prudent to assess the degree to which oysters from this region are ingesting microplastics. If so, it would have direct implications for Canada's oyster</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMEP13D0876G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMEP13D0876G"><span>The contribution of <span class="hlt">sediment</span> from forested areas of the Chesapeake Bay Watershed</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gellis, A.; Brakebill, J.</p> <p>2012-12-01</p> <p>Fine-grained <span class="hlt">sediment</span> is a major pollutant in the Chesapeake Bay and its receiving waters. <span class="hlt">Sediment</span> budget studies have been conducted in small basins draining to the Bay over the last decade to understand the important sources of fine-grained <span class="hlt">sediment</span>, quantify erosion rates, and determine <span class="hlt">sediment</span> yields. <span class="hlt">Sediment</span> budget approaches include modeling (SPARROW), <span class="hlt">sediment</span> fingerprinting, and quantifying upland rates of erosion (Cesium-137). SPARROW model results indicate that forests deliver between 2 to 8% of the total <span class="hlt">sediment</span> to the Bay. <span class="hlt">Sediment</span>-fingerprinting results from small watershed studies indicate that forests contribute between 13 to 29 % of the <span class="hlt">sediment</span>. The Cesium-137 technique was used to quantify soil redistribution (erosion and deposition) rates for forested areas in the Linganore Creek (146 km2) watershed which drains the Piedmont Physiographic Province. Average forest erosion rates measured in 2009 for Linganore Creek using Cesium-137 were 2.6 t/ha/yr. With 27% of the Linganore Creek watershed in forest, over 10,300 may be eroded off of forested lands which is more than the average annual suspended-<span class="hlt">sediment</span> load (8,050 Mg/yr) in Linganore Creek, indicating that much of the eroded forest <span class="hlt">sediment</span> goes in storage. Most of the forested areas in the Chesapeake Bay watershed were cut down for agriculture between the time of European colonization and the early 20th Century. In the late 20th century forested lands show an increase in areal extent. Although studies have not been conducted to understand why these secondary growth forests are eroding, it may involve that these forests have not fully <span class="hlt">recovered</span> from deforestation. Soil profiles are thin, and runoff and <span class="hlt">sediment</span> relations may have been altered, leading to high rates of erosion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/2765534','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/2765534"><span>Macro and micro rate zonal analytical centrifugation of polydisperse and slowly diffusing <span class="hlt">sedimenting</span> systems in isovolumetric density gradients. Application to cartilage proteoglycans.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Müller, F J; Pezon, C F; Pita, J C</p> <p>1989-06-13</p> <p>A method to study the polydispersity of zonally <span class="hlt">sedimenting</span> and slowly diffusing macromolecules or particles in isokinetic or isovolumetric density gradients is presented. First, a brief theory is given for predicting the zonal profile after a "triangular" (or "inverse") <span class="hlt">zone</span> is centrifuged. This type of <span class="hlt">zone</span> is essential to preserve hydrodynamic stability of the very slowly diffusing polydisperse solutes. It is proven, both by semitheoretical considerations and by computer calculations, that the resulting concentration profile of macrosolute is almost identical with that obtainable with a rectangular <span class="hlt">zone</span> coextensive with the triangular one and carrying the same total mass. Next, practical procedures are described for the convectionless layering of very small triangular <span class="hlt">zones</span> (50 microL or less). The linearity and stability of the <span class="hlt">zones</span> are experimentally tested and verified. Finally, the method is applied to cartilage proteoglycan preparations that included either the monomeric molecules only or both the monomeric and the aggregated ones. The zonal results are compared with those obtained by using conventional boundary <span class="hlt">sedimentation</span>. The two sets of results are seen to coincide fairly well, thus proving that the present technique can add to preparative zonal centrifugation the analytical precision of boundary <span class="hlt">sedimentation</span>. A multimodal polydisperse system is suggested to describe the aggregated proteoglycan macromolecules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993DSRI...40..425M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993DSRI...40..425M"><span>An automated leaching method for the determination of opal in <span class="hlt">sediments</span> and particulate matter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Müller, Peter J.; Schneider, Ralph</p> <p>1993-03-01</p> <p>An automated leaching method for the analysis of biogenic silica (opal) in <span class="hlt">sediments</span> and particulate matter is described. The opaline material is extracted with 1 M NaOH at 85°C in a stainless steel vessel under constant stirring, and the increase in dissolved silica is continuously monitored. For this purpose, a minor portion of the leaching solution is cycled to an autoanalyzer and analyzed for dissolved silicon by molybdate-blue spectrophotometry. The resulting absorbance versus time plot is then evaluated according to the extrapolation procedure of DEMASTER (1981). The method has been tested on sponge spicules, radiolarian tests. Recent and Pliocene diatomaceous ooze samples, clay minerals and quartz, artificial <span class="hlt">sediment</span> mixtures, and on various plankton, <span class="hlt">sediment</span> trap and <span class="hlt">sediment</span> samples. The results show that the relevant forms of biogenic opal in Quaternary <span class="hlt">sediments</span> are quantitatively <span class="hlt">recovered</span>. The time required for an analysis is dependent on the sample type, ranging from 10 to 20 min for plankton and <span class="hlt">sediment</span> trap material and up to 40-60 min for Quaternary <span class="hlt">sediments</span>. The silica co-extracted from silicate minerals is largely compensated for by the applied extrapolation technique. The remaining degree of uncertainty is on the order of 0.4 wt% SiO 2 or less, depending on the clay mineral composition and content.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMOS41A..08H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMOS41A..08H"><span>Hydrate Formation in Gas-Rich Marine <span class="hlt">Sediments</span>: A Grain-Scale Model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holtzman, R.; Juanes, R.</p> <p>2009-12-01</p> <p>We present a grain-scale model of marine <span class="hlt">sediment</span>, which couples solid- and multiphase fluid-mechanics together with hydrate kinetics. The model is applied to investigate the spatial distribution of the different methane phases - gas and hydrate - within the hydrate stability <span class="hlt">zone</span>. <span class="hlt">Sediment</span> samples are generated from three-dimensional packs of spherical grains, mapping the void space into a pore network by tessellation. Gas invasion into the water-saturated sample is simulated by invasion-percolation, coupled with a discrete element method that resolves the grain mechanics. The coupled model accounts for forces exerted by the fluids, including cohesion associated with gas-brine surface tension. Hydrate growth is represented by a hydrate film along the gas-brine interface, which increases <span class="hlt">sediment</span> cohesion by cementing the grain contacts. Our model of hydrate growth includes the possible rupture of the hydrate layer, which leads to the creation of new gas-water interface. In previous work, we have shown that fine-grained <span class="hlt">sediments</span> (FGS) exhibit greater tendency to fracture, whereas capillary invasion is the preferred mode of methane gas transport in coarse-grained <span class="hlt">sediments</span> (CGS). The gas invasion pattern has profound consequences on the hydrate distribution: a larger area-to-volume ratio of the gas cluster leads to a larger drop in gas pressure inside the growing hydrate shell, causing it to rupture. Repeated cycles of imbibition and hydrate growth accompanied by trapping of gas allow us to determine the distribution of hydrate and gas within the <span class="hlt">sediment</span> as a function of time. Our pore-scale model suggests that, even when film rupture takes place, the conversion of gas to hydrate is slow. This explains two common field observations: the coexistence of gas and hydrate within the hydrate stability <span class="hlt">zone</span> in CGS, and the high methane fluxes through fracture conduits in FGS. These results demonstrate the importance of accounting for the strong coupling among multiphase</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S21C0732R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S21C0732R"><span>Towards a Detailed Seismic Structure of the Valley of Mexico's Xochimilco Lake <span class="hlt">Zone</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rabade, S.; Sanchez-Sanchez, J.; Ayala Hernandez, M.; Macias, M. A.; Aguilar Calderon, L. A.; Alcántara, L.; Almora Mata, D.; Castro Parra, G.; Delgado, R.; Leonardo Suárez, M.; Molina Avila, I.; Mora, A.; Perez-Yanez, C.; Ruiz, A. L.; Sandoval, H.; Torres Noguez, M.; Vazquez Larquet, R.; Velasco Miranda, J. M.; Aguirre, J.; Ramirez-Guzmán, L.</p> <p>2017-12-01</p> <p>Six centuries of gradual, intentional <span class="hlt">sediment</span> filling in the Xochimilco Lake <span class="hlt">Zone</span> have drastically reduced the size of the lake. The basin structure and the lake's clay limits and thickness are poorly constrained, and yet, essential to explain the city's anomalous ground motion. Therefore, we conducted an experiment to define the 3D velocity model of Mexico's capital; the CDMX-E3D. The initial phase involved the deployment of a moving set of 18-broadband stations with an interstation distance of 500m over a period of 19 weeks. We collected the data and analyzed the results for the Xochimilco Lake <span class="hlt">Zone</span> using H/V Spectral Ratios (Nakamura, 1989), which provided an improved fundamental period map of the region. Results show that periods in the former lake <span class="hlt">zone</span> have larger variability than values previously estimated. In order to obtain group velocity maps at different periods, we estimated Green's functions from ambient noise cross-correlations following standard methodologies to invert Rayleigh wave travel times (Bensen et al., 2007). Preliminary result show very low-velocity <span class="hlt">zones</span> (100 m/s) and thick <span class="hlt">sediment</span> layers in most of the former Xochimilco Lake area. This Project was funded by the Secretaria de Ciencia, Tecnología e Innovación (SECITI) of Mexico City. Project SECITI/073/2016.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5954893-recent-carbonate-sedimentation-balearic-platform-model-temperate-climate-carbonate-shelves','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5954893-recent-carbonate-sedimentation-balearic-platform-model-temperate-climate-carbonate-shelves"><span>Recent carbonate <span class="hlt">sedimentation</span> on Balearic platform: model for temperate-climate carbonate shelves</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Fornos, J.; Rodriguez-Perea, A.; Massuti, C.</p> <p></p> <p>Existing models for carbonate <span class="hlt">sedimentation</span> on continental platforms are derived from the study of modern carbonate platforms in tropical climates. The Balearic platform in the western Mediterranean provides a new model for carbonate <span class="hlt">sedimentation</span> in a temperature, semiarid climate. On most of the continental shelf around the Balearic Islands, modern <span class="hlt">sediments</span> are exclusively bioclastic carbonates. Shoreline carbonate <span class="hlt">sediments</span> are bioclastic sands and muds accumulating in beach-dune systems without significant tidal influence (there are no astronomical tides in the western Mediterranean ). From the upper shoreface to 35 m deep, the sandy bottom is extensively colonized by sea grass (Posidonia oceanica),more » the rhizomes and roots of which form a rigid entrapment that retains the <span class="hlt">sediment</span> derived from calcareous organisms living within the sea grass and from calcareous epiphytes living on the stems and leaves. Archeological dating establishes a rate of vertical accretion in this <span class="hlt">zone</span> of 10/sup 3/ Bubnoff units (1 Bubnoff unit = 1 mm/1000 years). Between depths of 40 and 60 m, carbonate sands are composed predominantly or red-algal fragments. Intensely bioturbated wave ripples occur in environments dominated by laminar red algae (Lithothamnium and Phymatolithon). Below depths of 60 m, coarse <span class="hlt">sediment</span> produced by rhodolitic and ramose red algae is deposited in areas of tens to hundreds of meters in size. Biogenic buildups up to 2 m high occur in sandy areas as well as in deeper muddy areas. At the same depth in open-platform <span class="hlt">zones</span>, the bottom topography is characterized by large hummocks several hundred meters across. From the horizontal distribution of facies, it is possible to construct the probable vertical sequence of lithofacies which would characterize carbonates accumulating on a temperate-climate carbonate shelf. Many of these lithofacies are recognized in upper Miocene limestones on the Balearic Islands.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.5108T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.5108T"><span>Hydro- and <span class="hlt">sediment</span> dynamics in the estuary <span class="hlt">zone</span> of the Mekong Delta: case study Dinh An estuary.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tran, Anh Tuan; Thoss, Heiko; Gratiot, Nicolas; Dussouillez, Philippe; Brunier, Guillaume; Apel, Heiko</p> <p>2017-04-01</p> <p>The Mekong River is the tenth largest river in the world, covers an area of 795,000 km2, 4400km in length, the main river flows over the six countries including: China, Myanmar, Thailand, Laos, Cambodia and Vietnam. Its water discharge is 470 km3year-1 and the <span class="hlt">sediment</span> discharge is estimated about 160 million ton year-1. The <span class="hlt">sediment</span> transported by the Mekong River is the key factor in the formation and development of the delta. It is a vital factor for the stability of the coastline and river banks. Furthermore it compensates land subsidence by floodplain deposition, and is the major natural nutrient source for agriculture and aquaculture. However, only a few studies were conducted to characterize and quantify <span class="hlt">sediment</span> properties and process in the Delta. Also the morphodynamic processes were hardly studied systematically. Hence, this study targets to fill some important and open knowledge gaps with extensive field works that provide important information about the <span class="hlt">sediment</span> properties and hydrodynamic processes in different seasons Firstly three field survey campaigns are carried out along a 30 km section of the Bassac River from the beginning of Cu Lao Dung Island to Dinh An estuary in 2015 and 2016. During the field campaign, the movement of the salt wedge and the turbidity were monitored by vertical profiles along the river, as well as discharge measurements by ADCP were carried out at three cross sections continuously for 72 hours. The extension of the salt wedge in the river was determined, along with mixing processes. The movement and dynamics observed under different flow conditions indicate that <span class="hlt">sediment</span> was pumped during low flow upwards the river, while during high flow net transport towards the sea dominated. Also a distinct difference in the <span class="hlt">sediment</span> properties in the different seasons was observed, with a general tendency towards a higher proportion of coarser particles in the high flow season. These quantitative results give insights into the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017491','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017491"><span>The analysis of forms of sulfur in ancient <span class="hlt">sediments</span> and sedimentary rocks: comments and cautions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Rice, C.A.; Tuttle, M.L.; Reynolds, R.L.</p> <p>1993-01-01</p> <p>Assumptions commonly made during analysis of the amount of monosulfides [acid-volatile sulfides (AVS)] and disulfides in modern <span class="hlt">sediments</span>, may not be valid for ancient sedimentary rocks. It is known that ferric iron can oxidize H2S during AVS analysis unless a reducing agent such as stannous chloride is added to the treatment. In addition, some monosulfides such as greigite and pyrrhotite require heat during the AVS analysis in order to dissolve completely. However, the use of heat and/or stannous chloride in the AVS treatment may partially dissolve disulfides and it is generally recommended that stannous chloride not be used in the AVS treatment for modern <span class="hlt">sediments</span>. Most of the monosulfides are assumed to be <span class="hlt">recovered</span> as AVS without the addition of stannous chloride. This study investigates the recovery of monosulfides during sulfur speciation analysis with application to ancient sedimentary rocks. Sulfur in samples containing naturally occurring greigite and mackinawite or pyrite was measured using variations of a common sulfur-speciation scheme. The sulfur-speciation scheme analyzes for monosulfide sulfur, disulfide sulfur, elemental sulfur, inorganic sulfate and organically bound sulfur. The effects of heat, stannous chloride and ferric iron on the amounts of acid-volatile sulfide and disulfide <span class="hlt">recovered</span> during treatment for AVS were investigated. Isotopic compositions of the <span class="hlt">recovered</span> sulfur species along with yields from an extended sulfur-speciation scheme were used to quantify the effects. Hot 6 N HCl AVS treatment <span class="hlt">recovers</span> > 60% of the monosulfides as AVS in samples containing pure greigite and mackinawite. The remaining monosulfide sulfur is <span class="hlt">recovered</span> in a subsequent elemental sulfur extraction. Hot 6 N HCl plus stannous chloride <span class="hlt">recovers</span> 100% of the monosulfides as AVS. The addition of ferric iron to pure greigite and mackinawite samples during AVS treatment without stannous chloride decreased the amount of monosulfides <span class="hlt">recovered</span> as AVS and, if present</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.osti.gov/sciencecinema/biblio/987696','SCIGOVIMAGE-SCICINEMA'); return false;" href="http://www.osti.gov/sciencecinema/biblio/987696"><span><span class="hlt">Recovering</span> Radioactive Materials with OSRP team</span></a></p> <p><a target="_blank" href="http://www.osti.gov/sciencecinema/">ScienceCinema</a></p> <p>None</p> <p>2017-12-09</p> <p>The National Nuclear Security Administration sponsors a program, executed by Los Alamos National Laboratory, to <span class="hlt">recover</span> radioisotopes used by industry and academia and no longer needed. Called the "Offsite Source Recovery Program (OSRP), it has <span class="hlt">recovered</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005PhDT.......266L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhDT.......266L"><span>Tectono-stratigraphic evolution of normal fault <span class="hlt">zones</span>: Thal Fault <span class="hlt">Zone</span>, Suez Rift, Egypt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Leppard, Christopher William</p> <p></p> <p> propagation and early linkage of the precursor fault strands at depth before the fault segment broke surface, followed by the accumulation of displacement on the linked fault segment with minimal lateral propagation. This style of fault growth contrasts conventional fault growth models by which growth occurs through incremental increases in both displacement and length through time. The evolution of normal fault populations and fault <span class="hlt">zones</span> exerts a first- order control on basin physiography and <span class="hlt">sediment</span> supply, and therefore, the architecture and distribution of coeval syn-rift stratigraphy. The early syn-rift continental, Abu Zenima Formation, to shallow marine, Nukhul Formation show a pronounced westward increase in thickness controlled by the series of synthetic and antithetic faults up to 3 km west of present day Thai fault. The orientation of these faults controlled the location of fluvial conglomerates, sandstones and mudstones that shifted to the topographic lows created. The progressive localisation of displacement onto the Sarbut El Gamal fault segment during rift-climax resulted in an overall change in basin geometry. Accelerated subsidence rates led to <span class="hlt">sedimentation</span> rates being outpaced by subsidence resulting in the development of a marine, <span class="hlt">sediment</span>-starved, underfilled hangingwall depocentre characterised by slope-to-basinal depositional environments, with a laterally continuous slope apron in the immediate hangingwall, and point-sourced submarine fans. Controls on the spatial distribution, three dimensional architecture, and facies stacking patterns of coeval syn-rift deposits are identified as: I) structural style of the evolution and linkage of normal fault populations, ii) basin physiography, iii) evolution of drainage catchments, iv) bedrock lithology, and v) variations in sea/lake level.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51A2856P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51A2856P"><span>3D Porosity Estimation of the Nankai Trough <span class="hlt">Sediments</span> from Core-log-seismic Integration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, J. O.</p> <p>2015-12-01</p> <p>The Nankai Trough off southwest Japan is one of the best subduction-<span class="hlt">zone</span> to study megathrust earthquake fault. Historic, great megathrust earthquakes with a recurrence interval of 100-200 yr have generated strong motion and large tsunamis along the Nankai Trough subduction <span class="hlt">zone</span>. At the Nankai Trough margin, the Philippine Sea Plate (PSP) is being subducted beneath the Eurasian Plate to the northwest at a convergence rate ~4 cm/yr. The Shikoku Basin, the northern part of the PSP, is estimated to have opened between 25 and 15 Ma by backarc spreading of the Izu-Bonin arc. The >100-km-wide Nankai accretionary wedge, which has developed landward of the trench since the Miocene, mainly consists of offscraped and underplated materials from the trough-fill turbidites and the Shikoku Basin hemipelagic <span class="hlt">sediments</span>. Particularly, physical properties of the incoming hemipelagic <span class="hlt">sediments</span> may be critical for seismogenic behavior of the megathrust fault. We have carried out core-log-seismic integration (CLSI) to estimate 3D acoustic impedance and porosity for the incoming <span class="hlt">sediments</span> in the Nankai Trough. For the CLSI, we used 3D seismic reflection data, P-wave velocity and density data obtained during IODP (Integrated Ocean Drilling Program) Expeditions 322 and 333. We computed acoustic impedance depth profiles for the IODP drilling sites from P-wave velocity and density data. We constructed seismic convolution models with the acoustic impedance profiles and a source wavelet which is extracted from the seismic data, adjusting the seismic models to observed seismic traces with inversion method. As a result, we obtained 3D acoustic impedance volume and then converted it to 3D porosity volume. In general, the 3D porosities show decrease with depth. We found a porosity anomaly <span class="hlt">zone</span> with alteration of high and low porosities seaward of the trough axis. In this talk, we will show detailed 3D porosity of the incoming <span class="hlt">sediments</span>, and present implications of the porosity anomaly <span class="hlt">zone</span> for the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP41D..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP41D..04S"><span><span class="hlt">Sediment</span>-stabilizing and Destabilizing Ecoengineering Species from River to Estuary: the Case of the Scheldt System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Selakovic, S.; Cozzoli, F.; Leuven, J.; Van Braeckel, A.; Speybroeck, J.; Kleinhans, M. G.; Bouma, T.</p> <p>2017-12-01</p> <p>Interactions between organisms and landscape forming processes play an important role in evolution of coastal landscapes. In particular, biota has a strong potential to interact with important geomorphological processes such as <span class="hlt">sediment</span> dynamics. Although many studies worked towards quantifying the impact of different species groups on <span class="hlt">sediment</span> dynamics, information has been gathered on an ad hoc base. Depending on species' traits and distribution, functional groups of ecoengineering species may have differential effects on <span class="hlt">sediment</span> deposition and erosion. We hypothesize that the spatial distributions of <span class="hlt">sediment</span>-stabilizing and destabilizing species across the channel and along the whole salinity gradient of an estuary partly determine the planform shape and channel-shoal morphology of estuaries. To test this hypothesis, we analyze vegetation and macrobenthic data taking the Scheldt river-estuarine continuum as model ecosystem. We identify species traits with important effects on <span class="hlt">sediment</span> dynamics and use them to form functional groups. By using linearized mixed modelling, we are able to accurately describe the distributions of the different functional groups. We observe a clear distinction of dominant ecosystem engineering functional groups and their potential effects on the <span class="hlt">sediment</span> in the river-estuarine continuum. The first results of longitudinal cross section show the highest effects of stabilizing plant species in riverine and <span class="hlt">sediment</span> bioturbators in weak polyhaline part of continuum. The distribution of functional groups in transverse cross sections shows dominant stabilizing effect in supratidal <span class="hlt">zone</span> compared to dominant destabilizing effect in the lower intertidal <span class="hlt">zone</span>. This analysis offers a new and more general conceptualization of distributions of <span class="hlt">sediment</span> stabilizing and destabilizing functional groups and their potential impacts on <span class="hlt">sediment</span> dynamics, shoal patterns, and planform shapes in river-estuarine continuum. We intend to test this in future</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ECSS..207..203F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ECSS..207..203F"><span>Differential in surface elevation change across mangrove forests in the intertidal <span class="hlt">zone</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fu, Haifeng; Wang, Wenqing; Ma, Wei; Wang, Mao</p> <p>2018-07-01</p> <p>A better understanding of surface elevation changes in different mangrove forests would improve our predictions of sea-level rise impacts, not only upon mangrove species distributions in the intertidal <span class="hlt">zone</span>, but also on the functioning of these wetlands. Here, a two-year (2015-2017) dataset derived from 18 RSET-MH (rod surface elevation table-marker horizon) stations at Dongzhaigang Bay, Hainan, China, was analyzed to investigate how surface elevation changes differed across mangrove species <span class="hlt">zones</span>. The current SET data indicated a rather high rate (9.6 mm y-1, on average) of surface elevation gain that was mostly consistent with that (8.1 mm y-1, on average) inferred from either the 137Cs or 210Pb dating of <span class="hlt">sediment</span> cores. In addition, these surface elevation changes were sensitive to elevation in the intertidal <span class="hlt">zone</span> and differed significantly between the two study sites (Sanjiang and Houpai). Mangrove species inhabiting the lower intertidal <span class="hlt">zone</span> tended to experience greater surface elevation change at Sanjiang, which agrees with the general view that <span class="hlt">sedimentation</span> and elevation gains are driven by elevation in the intertidal <span class="hlt">zone</span> (i.e., greater when positioned lower in the intertidal profile). However, at Houpai, both surface elevation change and surface accretion showed the opposite trend (i.e., greater when positioned higher in the intertidal profile). This study's results indicate that the pattern of surface elevation changes across the intertidal profile maybe inconsistent due to intricate biophysical controls. Therefore, instead of using a constant rate, models should presume a topography that evolves at differing rates of surface elevation change in different species <span class="hlt">zones</span> across the intertidal profile when predicting the impacts of sea-level rise on mangrove distributions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009IJEaS..98..345L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009IJEaS..98..345L"><span>Detrital Cr-spinel in the Šambron-Kamenica <span class="hlt">Zone</span> (Slovakia): evidence for an ocean-spreading <span class="hlt">zone</span> in the Northern Vardar suture?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenaz, Davide; Mazzoli, Claudio; Spišiak, Jan; Princivalle, Francesco; Maritan, Lara</p> <p>2009-03-01</p> <p>The Šambron-Kamenica <span class="hlt">Zone</span> is situated on the northern margin of the Levočské vrchy mountains and Šarišskà vrchovina Highland, where the Central Carpathian Paleogene joins the Pieniny Klippen Belt. Sandstone outcrops in this area. From Cretaceous to Late Oligocene in age, these <span class="hlt">sediments</span> suggest transport directions from S and SE. The heavy mineral assemblages of this sandstone include Cr-spinel grains, mainly displaying types II and III alpine-peridotite affinities, and are representative of Ocean Island Basalt volcanism. A sample from Upper Eocene <span class="hlt">sediments</span> at Vit’az shows a clear change in Cr-spinel composition, which turns out to have types I and II peridotite affinities, and to derive from arc and Middle Ocean Ridge Basalt volcanism, with <span class="hlt">sediment</span> transport directions from SW and WSW. These data indicate major variations in the Upper Eocene tectonic setting, giving constraints to paleogeographic reconstruction of the Slovak Central Carpathians.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018NatGe..11..421E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018NatGe..11..421E"><span>Global diffusive fluxes of methane in marine <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Egger, Matthias; Riedinger, Natascha; Mogollón, José M.; Jørgensen, Bo Barker</p> <p>2018-06-01</p> <p>Anaerobic oxidation of methane provides a globally important, yet poorly constrained barrier for the vast amounts of methane produced in the subseafloor. Here we provide a global map and budget of the methane flux and degradation in diffusion-controlled marine <span class="hlt">sediments</span> in relation to the depth of the methane oxidation barrier. Our new budget suggests that 45-61 Tg of methane are oxidized with sulfate annually, with approximately 80% of this oxidation occurring in continental shelf <span class="hlt">sediments</span> (<200 m water depth). Using anaerobic oxidation as a nearly quantitative sink for methane in steady-state diffusive <span class="hlt">sediments</span>, we calculate that 3-4% of the global organic carbon flux to the seafloor is converted to methane. We further report a global imbalance of diffusive methane and sulfate fluxes into the sulfate-methane transition with no clear trend with respect to the corresponding depth of the methane oxidation barrier. The observed global mean net flux ratio between sulfate and methane of 1.4:1 indicates that, on average, the methane flux to the sulfate-methane transition accounts for only 70% of the sulfate consumption in the sulfate-methane transition <span class="hlt">zone</span> of marine <span class="hlt">sediments</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994JOM....46b..40J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994JOM....46b..40J"><span><span class="hlt">Recovering</span> recyclable materials from shredder residue</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jody, Bassam J.; Daniels, Edward J.; Bonsignore, Patrick V.; Brockmeier, Norman F.</p> <p>1994-02-01</p> <p>Each year, about 11 million tons of metals are <span class="hlt">recovered</span> in the United States from about 10 million discarded automobiles. The <span class="hlt">recovered</span> metals account for about 75 percent of the total weight of the discarded vehicles. The balance of the material, known as shredder residue, amounts to about three million tons annually and is currently landfilled. The residue contains a diversity of potentially recyclable materials, including polyurethane foams, iron oxides, and certain thermoplastics. This article discusses a process under development at Argonne National Laboratory to separate and <span class="hlt">recover</span> the recyclable materials from this waste stream. The process consists essentially of two stages. First, a physical separation is used to <span class="hlt">recover</span> the foams and the metal oxides, followed by a chemical process to extract certain thermoplastics. The status of the technology and the process economics are reviewed here.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.7840M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.7840M"><span>Evidence for iron-sulfate coupling in salt marsh <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mills, Jennifer; Antler, Gilad; Turchyn, Alexandra</p> <p>2014-05-01</p> <p>Organic carbon burial in shallow marine <span class="hlt">sediments</span> represents an important net sink in the global carbon cycle. Microbially mediated oxidation of organic matter in oxic, suboxic, and anoxic <span class="hlt">sediments</span> however, prevents the ultimate burial of organic carbon and its removal from the surface of the planet. Although the subsurface transformations of organic carbon have been studied extensively, an enigmatic question remains: when organic matter is deposited, what determines whether it will be buried, reoxidized, or undergo methanogenesis? One hypothesis is that the sulfur cycle, due to the abundance of sulfate in many surface environments, dominates the subsurface oxidation or other fate of organic carbon. However, it has also been suggested that iron may in turn play a key role in determining the behavior of the sulfur cycle. To better understand the controls on these processes, we are using stable isotope and geochemical techniques to explore the microbially mediated oxidation of organic carbon in salt marsh <span class="hlt">sediments</span> in North Norfolk, UK. In these <span class="hlt">sediments</span> there is a high supply of organic carbon, iron, and sulfate (from diurnal tidal cycles). Thus these environments may provide insight into the nature of interactions between the carbon, iron, and sulfur cycles. A series of sampling missions was undertaken in the autumn and winter of 2013-2014. In subsurface fluid samples we observe very high ferrous iron concentrations (>1mM), indicative of extended regions of iron reduction (to over 30cm depth). Within these <span class="hlt">zones</span> of iron reduction we would predict no sulfate reduction, and as expected δ34Ssulfate remains unchanged with depth. However, δ18Osulfate exhibits significant enrichments of up to 5 permil. This decoupling in the sulfur and oxygen isotopes of sulfate is suggestive of a sulfate recycling process in which sulfate is reduced to an intermediate sulfur species and subsequently reoxidized to sulfate. Taken together, these data suggest that microbial assemblages</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li class="active"><span>24</span></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_24 --> <div id="page_25" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="481"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.8919I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.8919I"><span>Maastrichtian <span class="hlt">sedimentation</span> and palaeoenvironments of the Saratov Volga region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iakovishina, Elena; Blinova, Irina; Kopaevich, Ludmila; Vishnevskaya, Valentina; Bordunov, Sergey</p> <p>2016-04-01</p> <p>The Saratov Volga region was a shallow-marine epicontinental basin North-Eastern shelf <span class="hlt">zone</span> of the Tethys Ocean in the Maastrichtian. The basis for the modeling conditions of <span class="hlt">sedimentation</span> was the detection mineral composition of rocks, as well as the contents of various chemical elements in rocks in three reference sections: Lower Bannovka, quarries "Bolshevik" and "Kommunar". Rocks of quarries "Bolshevik" and "Kommunar" characterized by quartz-calcite mineral association. The main rock-forming mineral is calcite, small amounts in rocks contain quartz. Other mineral composition characterized section Lower Bannovka. At the base of the section in the rock marked the presence of the opal. The source of silica are radiolarians. Favorable conditions for the existence of which is cold deep water enriched with SiO2. Above the section marked authigenic glauconite, which are confined to <span class="hlt">zones</span> of skip in <span class="hlt">sedimentation</span>.Further up begins to dominate the accumulation of calcite with rich bentic foraminifera. Clay minerals in rocks of the section Lower Bannovka presented montmorillonite and illite. The relationship of chemical elements and their alkali modules allow to detail the conditions of <span class="hlt">sedimentation</span>. The ratio of Fe/Mn in them varies from 44 to 5729. Higher values are characteristic of glauconite sandstones. Up the section marked decrease in the Ti/Zr, indicating that the increase in the distance from the source area to the place of deposition. The similarity values of the ratio Ti/Zr samples indicates a community source area. <span class="hlt">Sedimentation</span> Model revealed the impact of the PreUral strait connecting Tethys and Paleoarktic. Through the Strait of deep cold water saturated with SiO2, penetrated into the of the Saratov Volga region, were accumulated clay. The closing of the PreUral Strait changed the conditions of <span class="hlt">sedimentation</span>, the associated fall in sea levels due to global cooling reflected in the crisis of radiolarians, increase in the number of glauconite. Subsequent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=199718&keyword=Ford&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50','EPA-EIMS'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=199718&keyword=Ford&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>Assessing the Selectivity of Extractant Solutions for <span class="hlt">Recovering</span> Labile Arsenic Associated with Iron (Hydr)oxides and Sulfides in <span class="hlt">Sediments</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>Sequential extractions can provide analytical constraints on the identification of mineral phases that control arsenic speciation in <span class="hlt">sediments</span>. Model solids were used in this study to evaluate different solutions designed to extract arsenic from relatively labile solid phases. ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5326006-sedimentation-zoning-reservoir-rocks-siberian-basin-oil-fields','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5326006-sedimentation-zoning-reservoir-rocks-siberian-basin-oil-fields"><span><span class="hlt">Sedimentation</span>, <span class="hlt">zoning</span> of reservoir rocks in W. Siberian basin oil fields</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Kliger, J.A.</p> <p>1994-02-07</p> <p>A line pattern of well cluster spacing was chosen in western Siberia because of taiga, marshes, etc., on the surface. The <span class="hlt">zoning</span> of the oil pools within productive Upper Jurassic J[sub 3] intervals is complicated. This is why until the early 1990s almost each third well drilled in the Shaimsky region on the western edge of the West Siberian basin came up dry. The results of development drilling would be much better if one used some sedimentological relationships of <span class="hlt">zoning</span> of the reservoir rocks within the oil fields. These natural phenomena are: Paleobasin bathymetry; Distances from the sources of themore » clastic material; and Proximity of the area of deposition. Using the diagram in this article, one can avoid drilling toward areas where the sandstone pinch out, area of argillization of sand-stones, or where the probability of their absence is high.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25452749','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25452749"><span>Benthic protists and fungi of Mediterranean deep hypsersaline anoxic basin redoxcline <span class="hlt">sediments</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bernhard, Joan M; Kormas, Konstantinos; Pachiadaki, Maria G; Rocke, Emma; Beaudoin, David J; Morrison, Colin; Visscher, Pieter T; Cobban, Alec; Starczak, Victoria R; Edgcomb, Virginia P</p> <p>2014-01-01</p> <p>Some of the most extreme marine habitats known are the Mediterranean deep hypersaline anoxic basins (DHABs; water depth ∼3500 m). Brines of DHABs are nearly saturated with salt, leading many to suspect they are uninhabitable for eukaryotes. While diverse bacterial and protistan communities are reported from some DHAB water-column haloclines and brines, the existence and activity of benthic DHAB protists have rarely been explored. Here, we report findings regarding protists and fungi <span class="hlt">recovered</span> from <span class="hlt">sediments</span> of three DHAB (Discovery, Urania, L' Atalante) haloclines, and compare these to communities from <span class="hlt">sediments</span> underlying normoxic waters of typical Mediterranean salinity. Halocline <span class="hlt">sediments</span>, where the redoxcline impinges the seafloor, were studied from all three DHABs. Microscopic cell counts suggested that halocline <span class="hlt">sediments</span> supported denser protist populations than those in adjacent control <span class="hlt">sediments</span>. Pyrosequencing analysis based on ribosomal RNA detected eukaryotic ribotypes in the halocline <span class="hlt">sediments</span> from each of the three DHABs, most of which were fungi. Sequences affiliated with Ustilaginomycotina Basidiomycota were the most abundant eukaryotic signatures detected. Benthic communities in these DHABs appeared to differ, as expected, due to differing brine chemistries. Microscopy indicated that only a low proportion of protists appeared to bear associated putative symbionts. In a considerable number of cases, when prokaryotes were associated with a protist, DAPI staining did not reveal presence of any nuclei, suggesting that at least some protists were carcasses inhabited by prokaryotic scavengers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70017015','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017015"><span>A mid-Permian chert event: widespread deposition of biogenic siliceous <span class="hlt">sediments</span> in coastal, island arc and oceanic basins</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Murchey, B.L.; Jones, D.L.</p> <p>1992-01-01</p> <p>Radiolarian and conodont of Permian siliceous rocks from twenty-three areas in teh the circum-Pacific and Mediterranean regions reveal a widespread Permian Chert Event during the middle Leonardian to Wordian. Radiolarian- and (or) sponge spicule-rich siliceous <span class="hlt">sediments</span> accumulated beneath high productivity <span class="hlt">zones</span> in coastal, island arc and oceanic basins. Most of these deposits now crop out in fault-bounded accreted terranes. Biogenic siliceous <span class="hlt">sediments</span> did not accumulate in terranes lying beneath infertile waters including the marine sequences in terranes of northern and central Alaska. The Permian Chert Event is coeval with major phosphorite deposition along the western margin of Pangea (Phosphoria Formation and related deposits). A well-known analogue for this event is middle Miocene deposition of biogenic siliceous <span class="hlt">sediments</span> beneath high productivity <span class="hlt">zones</span> in many parts of the Pacific and concurrent deposition of phosphatic as well as siliceous <span class="hlt">sediments</span> in basins along the coast of California. Interrelated factors associated with both the Miocene and Permian depositional events include plate reorientations, small sea-level rises and cool polar waters. ?? 1992.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040089551&hterms=NH4&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DNH4','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040089551&hterms=NH4&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3DNH4"><span>Pathways of organic carbon oxidation in three continental margin <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Canfield, D. E.; Jorgensen, B. B.; Fossing, H.; Glud, R.; Gundersen, J.; Ramsing, N. B.; Thamdrup, B.; Hansen, J. W.; Nielsen, L. P.; Hall, P. O.</p> <p>1993-01-01</p> <p>We have combined several different methodologies to quantify rates of organic carbon mineralization by the various electron acceptors in <span class="hlt">sediments</span> from the coast of Denmark and Norway. Rates of NH4+ and Sigma CO2 liberation <span class="hlt">sediment</span> incubations were used with O2 penetration depths to conclude that O2 respiration accounted for only between 3.6-17.4% of the total organic carbon oxidation. Dentrification was limited to a narrow <span class="hlt">zone</span> just below the depth of O2 penetration, and was not a major carbon oxidation pathway. The processes of Fe reduction, Mn reduction and sulfate reduction dominated organic carbon mineralization, but their relative significance varied depending on the <span class="hlt">sediment</span>. Where high concentrations of Mn-oxide were found (3-4 wt% Mn), only Mn reduction occurred. With lower Mn oxide concentrations more typical of coastal <span class="hlt">sediments</span>, Fe reduction and sulfate reduction were most important and of a similar magnitude. Overall, most of the measured O2 flux into the <span class="hlt">sediment</span> was used to oxidized reduced inorganic species and not organic carbon. We suspect that the importance of O2 respiration in many coastal <span class="hlt">sediments</span> has been overestimated, whereas metal oxide reduction (both Fe and Mn reduction) has probably been well underestimated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3126381','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3126381"><span>Activity and Diversity of Methanotrophic Bacteria at Methane Seeps in Eastern Lake Constance <span class="hlt">Sediments</span> ▿</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Deutzmann, Jörg S.; Wörner, Susanne; Schink, Bernhard</p> <p>2011-01-01</p> <p>The activity and community structure of aerobic methanotrophic communities were investigated at methane seeps (pockmarks) in the littoral and profundal <span class="hlt">zones</span> of an oligotrophic freshwater lake (Lake Constance, Germany). Measurements of potential methane oxidation rates showed that <span class="hlt">sediments</span> inside littoral pockmarks are hot spots of methane oxidation. Potential methane oxidation rates at littoral pockmark sites exceeded the rates of the surrounding <span class="hlt">sediment</span> by 2 orders of magnitude. Terminal restriction fragment length polymorphism (T-RFLP) analysis of the pmoA gene revealed major differences in the methanotrophic community composition between littoral pockmarks and the surrounding <span class="hlt">sediments</span>. Clone library analysis confirmed that one distinct Methylobacter-related group dominates the community at littoral pockmarks. In profundal <span class="hlt">sediments</span>, the differences between pockmarks and surrounding <span class="hlt">sediments</span> were found to be less pronounced. PMID:21335392</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2006/5316/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2006/5316/"><span>Geostatistical Modeling of <span class="hlt">Sediment</span> Abundance in a Heterogeneous Basalt Aquifer at the Idaho National Laboratory, Idaho</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Welhan, John A.; Farabaugh, Renee L.; Merrick, Melissa J.; Anderson, Steven R.</p> <p>2007-01-01</p> <p>The spatial distribution of <span class="hlt">sediment</span> in the eastern Snake River Plain aquifer was evaluated and modeled to improve the parameterization of hydraulic conductivity (K) for a subregional-scale ground-water flow model being developed by the U.S. Geological Survey. The aquifer is hosted within a layered series of permeable basalts within which intercalated beds of fine-grained <span class="hlt">sediment</span> constitute local confining units. These <span class="hlt">sediments</span> have K values as much as six orders of magnitude lower than the most permeable basalt, and previous flow-model calibrations have shown that hydraulic conductivity is sensitive to the proportion of intercalated <span class="hlt">sediment</span>. Stratigraphic data in the form of <span class="hlt">sediment</span> thicknesses from 333 boreholes in and around the Idaho National Laboratory were evaluated as grouped subsets of lithologic units (composite units) corresponding to their relative time-stratigraphic position. The results indicate that median <span class="hlt">sediment</span> abundances of the stratigraphic units below the water table are statistically invariant (stationary) in a spatial sense and provide evidence of stationarity across geologic time, as well. Based on these results, the borehole data were kriged as two-dimensional spatial data sets representing the <span class="hlt">sediment</span> content of the layers that discretize the ground-water flow model in the uppermost 300 feet of the aquifer. Multiple indicator kriging (mIK) was used to model the geographic distribution of median <span class="hlt">sediment</span> abundance within each layer by defining the local cumulative frequency distribution (CFD) of <span class="hlt">sediment</span> via indicator variograms defined at multiple thresholds. The mIK approach is superior to ordinary kriging because it provides a statistically best estimate of <span class="hlt">sediment</span> abundance (the local median) drawn from the distribution of local borehole data, independent of any assumption of normality. A methodology is proposed for delineating and constraining the assignment of hydraulic conductivity <span class="hlt">zones</span> for parameter estimation, based on the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6776539-stratigraphic-architecture-depositional-history-lower-miocene-planulina-zone-southern-louisiana','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6776539-stratigraphic-architecture-depositional-history-lower-miocene-planulina-zone-southern-louisiana"><span>Stratigraphic architecture and depositional history of lower Miocene, Planulina <span class="hlt">Zone</span>, Southern Louisiana</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Gates, B.C.; Galloway, W.E.</p> <p>1988-01-01</p> <p>The Planulina <span class="hlt">zone</span> is a wedge of clastic <span class="hlt">sediment</span> positioned between the Anahuac shale below and the Oakville sandstone interval above. Planulna <span class="hlt">sediments</span> were deposited on an erosional surface, during a general rise in the sea level, and formed a retrogradational wedge. Within the study area, the Planulina <span class="hlt">zone</span> consists of two large depositional complexes: the Mud Lake complex in west Cameron Parish, Louisiana, and the East Cameron complex in east Cameron Parish. The lowermost depositional sequence in the East Cameron complex is preserved in a network of submarine canyons that were eroded into the upper slope. Framework sands weremore » deposited in channel systems confined to the axis of the canyons, and the sands are encased in marine shale containing benthonic foraminifera indicative of an upper to middle slope paleoenvironment. Two younger depositional sequences overlie the submarine canyon facies and were deposited by deltaic systems that prograded basinward. A <span class="hlt">zone</span> of expansion extends east to west through the Planulina interval and is named the ''Planulina flexure.'' The flexure is a large fault located at the relict shelf edge and soles out downdip inn the Anahuac shale. Several thousand feet of <span class="hlt">sediment</span> downthrown on the flexure is equivalent to several hundred feet upthrown, and the flexure represented the boundary dividing updip deltaic processes from downdip slope processes during the beginning of Planulina deposition. The Planulina depositional history and stratigraphic architecture are directly related to the displacement along the flexure and the structural deformation of the underlying Anahuac shale.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.T51B1895B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.T51B1895B"><span>Impact of Vishnu Fracture <span class="hlt">Zone</span> on Tectono-Stratigraphy of Kerala Deepwater Basin, India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bastia, R.; Krishna, K. S.; Nathaniel, D. M.; Tenepalli, S.</p> <p>2008-12-01</p> <p>Integration of regional seismic data extending from coast to deep water with the gravity-magnetics reveals the expression and evolution of ridge systems and fracture <span class="hlt">zones</span> in Indian Ocean. Kerala deepwater basin, situated in the south-western tip of India, is bounded by two prominent north-south oriented ocean fracture <span class="hlt">zones</span> viz., Vishnu (west) and Indrani (east) of the Indian Ocean. Vishnu Fracture <span class="hlt">Zone</span> (VFZ), which extends from the Kerala shelf southward to the Carlsberg-Ridge, over a length of more than 2500 km, has a strong bearing on the <span class="hlt">sedimentation</span> as well as structural fabric of the basin. VFZ is identified as the transform plate margin formed during Late-Cretaceous-Tertiary separation of Seychelles from India. Represented by a highly deformed structural fabric, VFZ forms an abrupt boundary between ocean floors of about 65 MY in the west and 140 MY in the east, implying a great scope for sedimentary pile on this very older ocean floor. Armed with this premise of an older sedimentary pile towards east of VFZ, congenial for petroleum hunt, the implemented modern long offset seismic program with an objective to enhance sub-basalt (Deccan) imagery, gravity-magnetic modelling and plate-tectonic reconstructions unraveled huge Mesozoic Basin, unheard earlier. Multi-episodic rifting in western continental margin of India starting during Mid Jurassic Karoo rift along the western Madagascar, Kerala deepwater basin, and western Antarctica and conjugate margins of Africa forms the main corridor for <span class="hlt">sedimentation</span>. Subsequent Late Cretaceous dextral oblique extension of Madagascar rift reactivated pre-existing structural framework creating major accommodation <span class="hlt">zones</span> along the southern tip of India. Followed by separation of Seychelles during KT boundary led to the formation of VFZ (an oceanic fracture <span class="hlt">zone</span>) forming a transform boundary between newly formed Tertiary oceanic crust to the west and older basin to the east. The pulses of right-lateral movement were associated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6265785-chitinozoan-zones-western-united-states-great-basin-comparison-those-canning-basin-western-australia','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6265785-chitinozoan-zones-western-united-states-great-basin-comparison-those-canning-basin-western-australia"><span>Chitinozoan <span class="hlt">zones</span> of the western United States (Great basin), and their comparison with those of the Canning basin, western Australia</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Hutter, T.J.</p> <p></p> <p>Within the Basin and Ranges of the Great basin of the western US, Ordovician chitinozoans have been <span class="hlt">recovered</span> in two major lithic facies; the western eugeosynclinal facies and the eastern miogeosynclinal facies. Chitinozoans <span class="hlt">recovered</span> from these facies range in age from Arenig to Ashgill. Extensive collections from this area make possible the establishment of chitinozoan faunal interval <span class="hlt">zones</span> from the Ordovician. These <span class="hlt">zones</span> are compared with those of other investigators for the Canning basin of Western Australia. Selected species of biostratigraphic value include, in chronostratigraphic order, Lagenochitina ovidea Benoit Taugourdeau 1961, Conochitina langei Combaz Peniguel 1972, Conochitina poumoti Combaz Peniguel,more » Desmochitina cf. nodosa Eisenack 1931 , Conochitina moclartii Combaz Peniguel 1972, Conochitina robusta Eisenack 1959, Angochitina capillata Eisenack 1937, Sphaerochitina lepta Jenkins 1970 and Ancyrochitina merga Jenkins 1970. In many cases these <span class="hlt">zones</span> can be divided into additional subzones using chitinozoans and acritarchs. In all cases, these chitinozoan faunal <span class="hlt">zones</span> are contrasted with established American graptolite <span class="hlt">zones</span>, as well as correlated with British standard graptolite <span class="hlt">zones</span>. The composition of these faunas of the Western US Great basin and Western Australia Canning basin is similar to that from the Marathon region of west Texas, and the Basin Ranges of Arizona and New Mexico.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027881','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027881"><span>Estimating <span class="hlt">sediment</span> budgets at the interface between rivers and estuaries with application to the Sacramento-San Joaquin River Delta</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wright, S.A.; Schoellhamer, D.H.</p> <p>2005-01-01</p> <p>[1] Where rivers encounter estuaries, a transition <span class="hlt">zone</span> develops where riverine and tidal processes both affect <span class="hlt">sediment</span> transport processes. One such transition <span class="hlt">zone</span> is the Sacramento-San Joaquin River Delta, a large, complex system where several rivers meet to form an estuary (San Francisco Bay). Herein we present the results of a detailed <span class="hlt">sediment</span> budget for this river/estuary transitional system. The primary regional goal of the study was to measure <span class="hlt">sediment</span> transport rates and pathways in the delta in support of ecosystem restoration efforts. In addition to achieving this regional goal, the study has produced general methods to collect, edit, and analyze (including error analysis) <span class="hlt">sediment</span> transport data at the interface of rivers and estuaries. Estimating <span class="hlt">sediment</span> budgets for these systems is difficult because of the mixed nature of riverine versus tidal transport processes, the different timescales of transport in fluvial and tidal environments, and the sheer complexity and size of systems such as the Sacramento-San Joaquin River Delta. <span class="hlt">Sediment</span> budgets also require error estimates in order to assess whether differences in inflows and outflows, which could be small compared to overall fluxes, are indeed distinguishable from zero. Over the 4 year period of this study, water years 1999-2002, 6.6 ?? 0.9 Mt of <span class="hlt">sediment</span> entered the delta and 2.2 ?? 0.7 Mt exited, resulting in 4.4 ?? 1.1 Mt (67 ?? 17%) of deposition. The estimated deposition rate corresponding to this mass of <span class="hlt">sediment</span> compares favorably with measured inorganic <span class="hlt">sediment</span> accumulation on vegetated wetlands in the delta.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H13C1379M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13C1379M"><span>Advancement in Watershed Modelling Using Dynamic Lateral and Longitudinal <span class="hlt">Sediment</span> (Dis)connectivity Prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mahoney, D. T.; al Aamery, N. M. H.; Fox, J.</p> <p>2017-12-01</p> <p>The authors find that <span class="hlt">sediment</span> (dis)connectivity has seldom taken precedence within watershed models, and the present study advances this modeling framework and applies the modeling within a bedrock-controlled system. <span class="hlt">Sediment</span> (dis)connectivity, defined as the detachment and transport of <span class="hlt">sediment</span> from source to sink between geomorphic <span class="hlt">zones</span>, is a major control on <span class="hlt">sediment</span> transport. Given the availability of high resolution geospatial data, coupling <span class="hlt">sediment</span> connectivity concepts within <span class="hlt">sediment</span> prediction models offers an approach to simulate <span class="hlt">sediment</span> sources and pathways within a watershed's <span class="hlt">sediment</span> cascade. Bedrock controlled catchments are potentially unique due to the presence of rock outcrops causing longitudinal impedance to <span class="hlt">sediment</span> transport pathways in turn impacting the longitudinal distribution of the energy gradient responsible for conveying <span class="hlt">sediment</span>. Therefore, the authors were motivated by the need to formulate a <span class="hlt">sediment</span> transport model that couples <span class="hlt">sediment</span> (dis)connectivity knowledge to predict <span class="hlt">sediment</span> flux for bedrock controlled catchments. A watershed-scale <span class="hlt">sediment</span> transport model was formulated that incorporates <span class="hlt">sediment</span> (dis)connectivity knowledge collected via field reconnaissance and predicts <span class="hlt">sediment</span> flux through coupling with the Partheniades equation and <span class="hlt">sediment</span> continuity model. <span class="hlt">Sediment</span> (dis)connectivity was formulated by coupling probabilistic upland lateral connectivity prediction with instream longitudinal connectivity assessments via discretization of fluid and <span class="hlt">sediment</span> pathways. Flux predictions from the upland lateral connectivity model served as an input to the instream longitudinal connectivity model. Disconnectivity in the instream model was simulated via the discretization of stream reaches due to barriers such as bedrock outcroppings and man-made check dams. The model was tested for a bedrock controlled catchment in Kentucky, USA for which extensive historic water and <span class="hlt">sediment</span> flux data was available. Predicted <span class="hlt">sediment</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMEP13C1633M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMEP13C1633M"><span>Benthic Foraminifers identify the source of displaced <span class="hlt">sediment</span> from a <span class="hlt">sediment</span> density flow at 1840 m near the Seafloor Instrument Node of the Monterey Coordinated Canyon Experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McGann, M.; Maier, K. L.; Gales, J. A.; Paull, C. K.; Gwiazda, R.; Barry, J.; Carvajal, C.; Clare, M. A.; Cartigny, M.; Chaffey, M. R.; Parsons, D. R.; O'Reilly, T. C.; Rosenberger, K. J.; Wolfson-Schwehr, M.; Simmons, S.; Sumner, E.; Talling, P.; Xu, J.</p> <p>2017-12-01</p> <p>Submarine canyons are found along the slopes of most continental margins and turbidity currents are thought to be the primary mechanism responsible for transporting <span class="hlt">sediment</span> through them to deep-sea fans. The initiation sites of these flows are difficult to locate with any degree of precision from lithology alone. Fortunately, the presence of allochthonous microscopic remains, such as benthic foraminifers, can aid in the identification of the source of the displaced <span class="hlt">sediments</span>. In Monterey Canyon, offshore California, a Seafloor Instrument Node (SIN) and adjacent mooring in the Coordinated Canyon Experiment indicate that a February 2017 turbidity current reached 1840 m water depth. In April 2017, one push core was obtained on each of four sides of the SIN just outside its frame and six others from 30-100 m away. Each was cut into 1 cm slices, stained with rose Bengal, washed, and analyzed for their microscopic constituents. Material <span class="hlt">recovered</span> included terrestrial debris (wood, leaves, seeds, highway safety spheres, and volcanic glass) as well as foraminiferal tests. Dead benthic foraminifers from the estuarine (0-10 m), inner shelf (0-50 m), outer shelf (50-150 m), slope break (150 m), upper bathyal (150-500 m), and middle bathyal (500-2000 m) biofacies were present, suggesting a staged progression of <span class="hlt">sediment</span> downslope from the continental shelf and slope. Living (rose Bengal stained) foraminifers <span class="hlt">recovered</span> represent estuarine (Ammonia tepida, Elphidium excavatum), inner shelf (Buccella frigida, B. tenerrima, Buliminella elegantissima, Cibicides fletcheri, Nonionella spp., Rotorbinella turbinata), and upper bathyal (Bolivina pacifica, B. spissa, Epistominella exigua, Uvigerina peregrina) species as well as an in-situ middle bathyal biofacies (Bolivina argentea, B. spissa, Buliminella tenuata, Epistominella pacifica, Globobulimina spp., Uvigerina peregrina, U. hispida). The presence of living allochthonous benthic foraminifers from these shallower biofacies suggests</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1510328G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1510328G"><span>Tracking <span class="hlt">sediment</span> through the Holocene: Determining anthropogenic contributions to a <span class="hlt">sediment</span>-rich agricultural system, north-central USA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gran, Karen; Belmont, Patrick; Finnegan, Noah</p> <p>2013-04-01</p> <p>Management and restoration of <span class="hlt">sediment</span>-impaired streams requires quantification of <span class="hlt">sediment</span> sources and pathways of transport. Addressing the role of humans in altering the magnitude and sources of <span class="hlt">sediment</span> supplied to a catchment is notoriously challenging. Here, we explore how humans have amplified erosion in geomorphically-sensitive portions of the predominantly-agricultural Minnesota River basin in north-central USA. In the Minnesota River basin, the primary sources of <span class="hlt">sediment</span> are classified generally as upland agricultural field vs. near-channel sources, with near-channel sources including stream banks, bluffs, and ravines. Using aerial lidar data, repeat terrestrial lidar scans of bluffs, ravine monitoring, historic air photo analyses, and <span class="hlt">sediment</span> fingerprinting, we have developed a <span class="hlt">sediment</span> budget to determine the relative importance of each source in a tributary to the Minnesota River, the Le Sueur River. We then investigate how these sources have changed through time, from changes evident over the past few decades to changes associated with valley evolution over the past 13,400 years. The Minnesota River valley was carved ~13,400 years ago through catastrophic drainage of glacial Lake Agassiz. As the Minnesota River valley incised, knickpoints have migrated upstream into tributaries, carving out deep valleys where the most actively eroding near-channel <span class="hlt">sediment</span> sources occur. The modern <span class="hlt">sediment</span> budget, closed for the time period 2000 to 2010, shows that the majority of the fine <span class="hlt">sediment</span> load in the Le Sueur River comes from bluffs and other near-channel sources in the deeply-incised knick <span class="hlt">zone</span>. Numerical modeling of valley evolution constrained by mapped and dated strath terraces cut into the glacial till presents an opportunity to compare the modern <span class="hlt">sediment</span> budget to that of the river prior to anthropogenic modification. This comparison reveals a natural background or "pre-agriculture" rate of erosion from near-channel sources to be 3-5 times lower</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMGC23B0914D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMGC23B0914D"><span>Summer temperatures inferred from varved lacustrine <span class="hlt">sediment</span> at Iceberg Lake in southcentral Alaska</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Diedrich, K.; Loso, M. G.</p> <p>2010-12-01</p> <p>Iceberg Lake, a glacier-dammed lake in southcentral Alaska, has been previously shown to record over 1,500 years of continuous laminated lacustrine <span class="hlt">sediment</span> deposition. Because previous work was based on examination of subaerial outcrops exposed by stream incision in the bed of the jökulhlaup-drained lake, the length of the record was limited by the extent of the outcrops. In August of 2010, we returned to core the remote lake; our goal was recovery of the complete sedimentary record in the lake, extending perhaps back to the onset of late Holocene glaciation—around 3-5 ka in this region. We used a Vibarcorer system to <span class="hlt">recover</span> <span class="hlt">sediment</span> cores from two locations, one near the site of previous work and another at the distal end of the lake. The longest cores <span class="hlt">recovered</span> were 5.2 meters and 6.2 meters at the proximal and distal sites, respectively. Based on the average lamination thickness established previously at the proximal site (4.7 mm), these cores should each represent over 1000 years of <span class="hlt">sediment</span> accumulation, and likely much longer at the distal site, where laminations are expected to be thinner. Having established previously that the lake’s laminations are annual varves and that they are positively correlated with summer (melt-season) temperatures, our analysis is focused on documenting a long time-series of annual <span class="hlt">sediment</span> accumulation and summer-layer particle size. Both measurements will be used to interpret the history of summer temperatures. The cores may also provide sedimentary evidence of the timing of advances/retreats of nearby glaciers, including the Tana Glacier and Bagley Icefield, helping to clarify the poorly-constrained timing of neoglaciation in Southern Alaska. The paleoclimate record produced at Iceberg Lake will be included in the Arctic System Science 8ka project</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008Ocgy...48..196P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008Ocgy...48..196P"><span>Geochemistry of polycyclic aromatic hydrocarbons in the bottom <span class="hlt">sediments</span> of the eastern Arctic shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Petrova, V. I.; Batova, G. I.; Kursheva, A. V.; Litvinenko, I. V.; Savinov, V. M.; Savinova, T. N.</p> <p>2008-04-01</p> <p>Sources and pathways of supply of polycyclic aromatic hydrocarbons (PAH) in the surface <span class="hlt">sediments</span> of the Laptev and East Siberian seas were identified based on an analysis of the lithological-geochemical characteristics and distribution of organic matter (OM). The distribution of organic carbon, humic acids, bitumoids, and hydrocarbons demonstrates the determining role of the riverine runoff in the formation of the recent <span class="hlt">sediments</span>. The total average content of PAH in the <span class="hlt">sediments</span> of this region approximates 37 ng/g, not exceeding 80 ng/g of dry <span class="hlt">sediment</span>. The biogenic components of the PAH (alkylphenanthrenes, alkylchrysenes, perylene) dominate in the estuarine-shelf and coastal-shelf <span class="hlt">sediments</span> enriched with plant detritus and significantly decrease in the pelagic <span class="hlt">zone</span>. The anthropogenic influence is observed in <span class="hlt">sediments</span> of the port of Tiksi, where the total content of PAH with dominant pyrogenic components is two orders of magnitude higher as compared with the background values in the study region.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20888603','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20888603"><span>Ecological evaluation of an experimental beneficial use scheme for dredged <span class="hlt">sediment</span> disposal in shallow tidal waters.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van der Wal, Daphne; Forster, Rodney M; Rossi, Francesca; Hummel, Herman; Ysebaert, Tom; Roose, Frederik; Herman, Peter M J</p> <p>2011-01-01</p> <p>An experiment was performed to test an alternative dredging strategy for the Westerschelde estuary. Clean sand dredged from the navigation channel was disposed seawards of an eroding intertidal flat in order to modify morphology and hydrodynamics, improving the multi-channel system with ecologically productive shallow water habitat. Five years of intensive monitoring revealed that part of the disposed <span class="hlt">sediment</span> moved slowly towards the flat, increasing the very shallow subtidal and intertidal area, as planned. The sand in the impact <span class="hlt">zone</span> became gradually finer after disposal, possibly due to reduced current velocities. Nevertheless, no changes in macrobenthic biomass, density, species richness and composition were detected in the subtidal <span class="hlt">zone</span>, also demonstrating rapid macrobenthic recovery. In the intertidal <span class="hlt">zone</span>, no ecological effects could be revealed superimposed on trends associated with long-term <span class="hlt">sediment</span> fining. Thus, despite morphological success and absence of detected negative ecological impacts of the experiment, new beneficial habitat was not created. Copyright © 2010 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70044029','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70044029"><span>Anaerobic methane oxidation in low-organic content methane seep <span class="hlt">sediments</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pohlman, John W.; Riedel, Michael; Bauer, James E.; Canuel, Elizabeth A.; Paull, Charles K.; Lapham, Laura; Grabowski, Kenneth S.; Coffin, Richard B.; Spence, George D.</p> <p>2013-01-01</p> <p>Sulfate-dependent anaerobic oxidation of methane (AOM) is the key sedimentary microbial process limiting methane emissions from marine <span class="hlt">sediments</span> and methane seeps. In this study, we investigate how the presence of low-organic content <span class="hlt">sediment</span> influences the capacity and efficiency of AOM at Bullseye vent, a gas hydrate-bearing cold seep offshore of Vancouver Island, Canada. The upper 8 m of <span class="hlt">sediment</span> contains 14C. A fossil origin for the DIC precludes remineralization of non-fossil OM present within the sulfate <span class="hlt">zone</span> as a significant contributor to pore water DIC, suggesting that nearly all sulfate is available for anaerobic oxidation of fossil seep methane. Methane flux from the SMT to the <span class="hlt">sediment</span> water interface in a diffusion-dominated flux region of Bullseye vent was, on average, 96% less than at an OM-rich seep in the Gulf of Mexico with a similar methane flux regime. Evidence for enhanced methane oxidation capacity within OM-poor <span class="hlt">sediments</span> has implications for assessing how climate-sensitive reservoirs of sedimentary methane (e.g., gas hydrate) will respond to ocean warming, particularly along glacially-influenced mid and high latitude continental margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15224927','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15224927"><span>Denitrification potential in relation to lithology in five headwater riparian <span class="hlt">zones</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hill, Alan R; Vidon, Philippe G F; Langat, Jackson</p> <p>2004-01-01</p> <p>The influence of riparian <span class="hlt">zone</span> lithology on nitrate dynamics is poorly understood. We investigated vertical variations in potential denitrification activity in relation to the lithology and stratigraphy of five headwater riparian <span class="hlt">zones</span> on glacial till and outwash landscapes in southern Ontario, Canada. Conductive coarse sand and gravel layers occurred in four of the five riparian areas. These layers were thin and did not extend to the field-riparian perimeter in some riparian <span class="hlt">zones</span>, which limited their role as conduits for ground water flow. We found widespread organic-rich layers at depths ranging from 40 to 300 cm that resulted from natural floodplain processes and the burial of surface soils by rapid valley-bottom <span class="hlt">sedimentation</span> after European settlement. The organic matter content of these layers varied considerably from 2 to 5% (relic channel deposit) to 5 to 21% (buried soils) and 30 to 62% (buried peat). Denitrification potential (DNP) was measured by the acetylene block method in <span class="hlt">sediment</span> slurries amended with nitrate. The highest DNP rates were usually found in the top 0- to 15-cm surface soil layer in all riparian <span class="hlt">zones</span>. However, a steep decline in DNP with depth was often absent and high DNP activity occurred in the deep organic-rich layers. Water table variations in 2000-2002 indicated that ground water only interacted frequently with riparian surface soils between late March and May, whereas subsurface organic layers that sustain considerable DNP were below the water table for most of the year. These results suggest that riparian <span class="hlt">zones</span> with organic deposits at depth may effectively remove nitrate from ground water even when the water table does not interact with organic-rich surface soil horizons.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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