Sample records for adjacent ocean basins

  1. The Canada Basin compared to the southwest South China Sea: Two marginal ocean basins with hyper-extended continent-ocean transitions

    NASA Astrophysics Data System (ADS)

    Li, Lu; Stephenson, Randell; Clift, Peter D.

    2016-11-01

    Both the Canada Basin (a sub-basin within the Amerasia Basin) and southwest (SW) South China Sea preserve oceanic spreading centres and adjacent passive continental margins characterized by broad COT zones with hyper-extended continental crust. We have investigated strain accommodation in the regions immediately adjacent to the oceanic spreading centres in these two basins using 2-D backstripping subsidence reconstructions, coupled with forward modelling constrained by estimates of upper crustal extensional faulting. Modelling is better constrained in the SW South China Sea but our results for the Canada Basin are analogous. Depth-dependent extension is required to explain the great depth of both basins because only modest upper crustal faulting is observed. A weak lower crust in the presence of high heat flow and, accordingly, a lower crust that extends far more the upper crust are suggested for both basins. Extension in the COT may have continued even after seafloor spreading has ceased. The analogous results for the two basins considered are discussed in terms of (1) constraining the timing and distribution of crustal thinning along the respective continental margins, (2) defining the processes leading to hyper-extension of continental crust in the respective tectonic settings and (3) illuminating the processes that control hyper-extension in these basins and more generally.

  2. Mapping of the air-sea CO2 flux in the Arctic Ocean and its adjacent seas: Basin-wide distribution and seasonal to interannual variability

    NASA Astrophysics Data System (ADS)

    Yasunaka, Sayaka; Murata, Akihiko; Watanabe, Eiji; Chierici, Melissa; Fransson, Agneta; van Heuven, Steven; Hoppema, Mario; Ishii, Masao; Johannessen, Truls; Kosugi, Naohiro; Lauvset, Siv K.; Mathis, Jeremy T.; Nishino, Shigeto; Omar, Abdirahman M.; Olsen, Are; Sasano, Daisuke; Takahashi, Taro; Wanninkhof, Rik

    2016-09-01

    We produced 204 monthly maps of the air-sea CO2 flux in the Arctic north of 60°N, including the Arctic Ocean and its adjacent seas, from January 1997 to December 2013 by using a self-organizing map technique. The partial pressure of CO2 (pCO2) in surface water data were obtained by shipboard underway measurements or calculated from alkalinity and total inorganic carbon of surface water samples. Subsequently, we investigated the basin-wide distribution and seasonal to interannual variability of the CO2 fluxes. The 17-year annual mean CO2 flux shows that all areas of the Arctic Ocean and its adjacent seas were net CO2 sinks. The estimated annual CO2 uptake by the Arctic Ocean was 180 TgC yr-1. The CO2 influx was strongest in winter in the Greenland/Norwegian Seas (>15 mmol m-2 day-1) and the Barents Sea (>12 mmol m-2 day-1) because of strong winds, and strongest in summer in the Chukchi Sea (∼10 mmol m-2 day-1) because of the sea-ice retreat. In recent years, the CO2 uptake has increased in the Greenland/Norwegian Sea and decreased in the southern Barents Sea, owing to increased and decreased air-sea pCO2 differences, respectively.

  3. Origin of the earth's ocean basins

    NASA Technical Reports Server (NTRS)

    Frex, H.

    1977-01-01

    The earth's original ocean basins were mare-type basins produced 4 billion years ago by the flux of asteroid-sized objects responsible for the lunar mare basins. Scaling upwards from the observed number of lunar basins for the greater capture cross-section and impact velocity of the Earth indicates that at least 50 percent of an original global crust would have been converted to basin topography. These basins were flooded by basaltic liquids in times short compared to the isostatic adjustment time for the basin. The modern crustal dichotomy (60 percent oceanic, 40 percent continental crust) was established early in the history of the earth, making possible the later onset of plate tectonic processes. These later processes have subsequently reworked, in several cycles, principally the oceanic parts of the earth's crust, changing the configuration of the continents in the process. Ocean basins (and oceans themselves) may be rare occurrences on planets in other star systems.

  4. A comparison of the South China Sea and Canada Basin: two small marginal ocean basins with hyper-extended margins and central zones of sea-floor spreading.

    NASA Astrophysics Data System (ADS)

    Li, L.

    2015-12-01

    Both the South China Sea and Canada Basin preserve oceanic spreading centres and adjacent passive continental margins characterized by broad COT zones with hyper-extended continental crust. We have investigated the nature of strain accommodation in the regions immediately adjacent to the oceanic spreading centres in these two basins using 2-D backstripping subsidence reconstructions, coupled with forward modelling constrained by estimates of upper crustal extensional faulting. Modelling is better constrained in the South China Sea but our results for the Beaufort Sea are analogous. Depth-dependent extension is required to explain the great depth of both basins because only modest upper crustal faulting is observed. A weak lower crust in the presence of high heat flow is suggested for both basins. Extension in the COT may continue even after sea-floor spreading has ceased. The analogous results for the two basins considered are discussed in terms of (1) constraining the timing and distribution of crustal thinning along the respective continental margins, (2) defining the processes leading to hyper-extension of continental crust in the respective tectonic settings and (3) illuminating the processes that control hyper-extension in these basins and more generally.

  5. Water resources of the Waccasassa River Basin and adjacent areas, Florida

    USGS Publications Warehouse

    Taylor, G.F.; Snell, L.J.

    1978-01-01

    This map report was prepared in cooperation with the Southwest Florida Water Management District which, with the Waccasassa River Basin Board, had jurisdiction over waters within the Waccasassa River basin, the coastal areas adjacent to the basin, and other adjacent areas outside the basin. New water management district boundaries, effective January 1977, place most of the Waccasassa River basin in the Suwannee River Water Management District. The purpose of the report is to provide water information for consideration in land-use and water development which is accelerating, especially in the northeastern part of the study area. It is based largely on existing data in the relatively undeveloped area. Of the total area included in the topographic drainage basin for the Waccasassa River about 72 percent is in Levy County, 18 percent in Alachua County, 9 percent in Gilchrist County, and 1 percent in Marion County. The elongated north-south drainage basin is approximately 50 mi in length, averages 13 mi in width, and lies between the Suwannee River, the St. Johns River, and the Withlacoochee River basins. (Woodard-USGS)

  6. Sea-floor drainage features of Cascadia Basin and the adjacent continental slope, northeast Pacific Ocean

    USGS Publications Warehouse

    Hampton, M.A.; Karl, Herman A.; Kenyon, Neil H.

    1989-01-01

    Sea-floor drainage features of Cascadia Basin and the adjacent continental slope include canyons, primary fan valleys, deep-sea valleys, and remnant valley segments. Long-range sidescan sonographs and associated seismic-reflection profiles indicate that the canyons may originate along a mid-slope escarpment and grow upslope by mass wasting and downslope by valley erosion or aggradation. Most canyons are partly filled with sediment, and Quillayute Canyon is almost completely filled. Under normal growth conditions, the larger canyons connect with primary fan valleys or deep-sea valleys in Cascadia Basin, but development of accretionary ridges blocks or re-routes most canyons, forcing abandonment of the associated valleys in the basin. Astoria Fan has a primary fan valley that connects with Astoria Canyon at the fan apex. The fan valley is bordered by parallel levees on the upper fan but becomes obscure on the lower fan, where a few valley segments appear on the sonographs. Apparently, Nitinat Fan does not presently have a primary fan valley; none of the numerous valleys on the fan connect with a canyon. The Willapa-Cascadia-Vancouver-Juan de Fuca deep-sea valley system bypasses the submarine fans and includes deeply incised valleys to broad shallow swales, as well as within-valley terraces and hanging-valley confluences. ?? 1989.

  7. Phanerozoic stratigraphy of Northwind Ridge, magnetic anomalies in the Canada Basin, and the geometry and timing of rifting in the Amerasia Basin, Arctic Ocean

    USGS Publications Warehouse

    Grantz, A.; Clark, D.L.; Phillips, R.L.; Srivastava, S.P.; Blome, C.D.; Gray, L.-B.; Haga, H.; Mamet, B.L.; McIntyre, D.J.; McNeil, D.H.; Mickey, M.B.; Mullen, M.W.; Murchey, B.I.; Ross, C.A.; Stevens, C.H.; Silberling, Norman J.; Wall, J.H.; Willard, D.A.

    1998-01-01

    Cores from Northwind Ridge, a high-standing continental fragment in the Chukchi borderland of the oceanic Amerasia basin, Arctic Ocean, contain representatives of every Phanerozoic system except the Silurian and Devonian systems. Cambrian and Ordovician shallow-water marine carbonates in Northwind Ridge are similar to basement rocks beneath the Sverdrup basin of the Canadian Arctic Archipelago. Upper Mississippian(?) to Permian shelf carbonate and spicularite and Triassic turbidite and shelf lutite resemble coeval strata in the Sverdrup basin and the western Arctic Alaska basin (Hanna trough). These resemblances indicate that Triassic and older strata in southern Northwind Ridge were attached to both Arctic Canada and Arctic Alaska prior to the rifting that created the Amerasia basin. Late Jurassic marine lutite in Northwind Ridge was structurally isolated from coeval strata in the Sverdrup and Arctic Alaska basins by rift shoulder and grabens, and is interpreted to be a riftogenic deposit. This lutite may be the oldest deposit in the Canada basin. A cape of late Cenomanian or Turonian rhyodacite air-fall ash that lacks terrigenous material shows that Northwind Ridge was structurally isolated from the adjacent continental margins by earliest Late Cretaceous time. Closing Amerasia basin by conjoining seafloor magnetic anomalies beneath the Canada basin or by uniting the pre-Jurassic strata of Northwind Ridge with kindred sections in the Sverdrup basin and Hanna trough yield simular tectonic reconstructions. Together with the orientation and age of rift-marine structures, these data suggest that: 1) prior to opening of the Amerasia basin, both northern Alaska and continental ridges of the Chukchi borderland were part of North America, 2) the extension that created the Amerasia basin formed rift-margin graben beginning in Early Jurassic time and new oceanic crust probably beginning in Late Jurassic or early Neocomian time. Reconstruction of the Amerasia basin on the

  8. Consensuses and discrepancies of basin-scale ocean heat content changes in different ocean analyses

    NASA Astrophysics Data System (ADS)

    Wang, Gongjie; Cheng, Lijing; Abraham, John; Li, Chongyin

    2018-04-01

    Inconsistent global/basin ocean heat content (OHC) changes were found in different ocean subsurface temperature analyses, especially in recent studies related to the slowdown in global surface temperature rise. This finding challenges the reliability of the ocean subsurface temperature analyses and motivates a more comprehensive inter-comparison between the analyses. Here we compare the OHC changes in three ocean analyses (Ishii, EN4 and IAP) to investigate the uncertainty in OHC in four major ocean basins from decadal to multi-decadal scales. First, all products show an increase of OHC since 1970 in each ocean basin revealing a robust warming, although the warming rates are not identical. The geographical patterns, the key modes and the vertical structure of OHC changes are consistent among the three datasets, implying that the main OHC variabilities can be robustly represented. However, large discrepancies are found in the percentage of basinal ocean heating related to the global ocean, with the largest differences in the Pacific and Southern Ocean. Meanwhile, we find a large discrepancy of ocean heat storage in different layers, especially within 300-700 m in the Pacific and Southern Oceans. Furthermore, the near surface analysis of Ishii and IAP are consistent with sea surface temperature (SST) products, but EN4 is found to underestimate the long-term trend. Compared with ocean heat storage derived from the atmospheric budget equation, all products show consistent seasonal cycles of OHC in the upper 1500 m especially during 2008 to 2012. Overall, our analyses further the understanding of the observed OHC variations, and we recommend a careful quantification of errors in the ocean analyses.

  9. Slope and basinal deposits adjacent to isolated carbonate platforms in the Indian Ocean: Sedimentology, geomorphology, and a new 1.2 Ma record of highstand shedding

    NASA Astrophysics Data System (ADS)

    Counts, J. W.; Jorry, S.; Jouet, G.

    2017-12-01

    Newly analyzed bathymetric, seismic, and core data from carbonate-topped seamounts in the Mozambique Channel reveals a variety of depositional processes and products operating on platform slopes and adjacent basins. Mass transport complexes (including turbidites and debrites), leveed channel systems with basin-floor fans, and contourites are imaged in high resolution in both seafloor maps and cross-section, and show both differences and similarities compared with platform slopes in the Bahamas and elsewhere. In some, though not all, platforms, increased sedimentation can be observed on the leeward margins, and slope rugosity may be asymmetric with respect to prevailing wind direction. Deposition is also controlled by glacial-interglacial cycles; cores taken from the lower slopes (3000+ m water depth) of carbonate platforms reveal a causative relationship between sea level and aragonite export to the deep ocean. δ18O isotopes from planktonic and benthic foraminifera of two 27-meter cores, reveal a high-resolution, continuous depositional record of carbonate sediment dating back to 1.2 Ma. Sea level rise, as determined by correlation with the LR04 benthic stack, is coincident with increased aragonite flux from platform tops. Gravity flow deposits are also affected by platform flooding—the frequency of turbidite/debrite deposits on pinnacle slopes increases during highstand, although such deposits are also present during glacial episodes. The results reported here are the first record of highstand shedding in the southern Indian Ocean, and provide the longest Quaternary sediment record to date in the region, including the Mid-Brunhes transition (MIS 11) that serves as an analog for the current climate conditions. In addition, this is the first study to describe sedimentation on the slopes of these platforms, providing an important point of comparison that has the potential to influence source-to-sink carbonate facies models.

  10. Paleogeographic evolution of foldbelts adjacent to petroleum basins of Venezuela and Trinidad

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

    Goodman, E.D.; Koch, P.S.; Summa, L.L.

    1996-08-01

    The foldbelts of Venezuela and Trinidad have shaped the history of adjacent sedimentary basins. A set of paleogeographic maps on reconstructed bases depict the role of foldbelts in the development of the sedimentary basins of Venezuela. Some of the foldbelts are inverted, pre-Tertiary graben/passive margin systems. Other foldbelts are allochthonous nappes or parautochthons that override the Mesozoic passive margin hinge without inversion. The emergence of these foldbelts changed the course of existing river systems and provided a new source for sediments and maturation in adjacent deeps. The Merida Andes area was remobilized beginning in the Early Miocene as a zonemore » of lateral shear, along which the Bonaire Block has moved over 200 km to the northeast, dismembering the Maracaibo and Barinas basins. Late Miocene to Recent transpression and fault reactivation have driven rapid Andean uplift with thrust-related subsidence and maturation (e.g., SE Maracaibo foredeep). To the east, uplift and erosion of the Serrania del Interior (1) curtailed mid-Tertiary fluvial systems flowing northward from the igneous and sedimentary rocks of the Guyana Shield, deflecting them eastward, and (2) removed the thick early Miocene foredeep fill into a younger foredeep. Thus, the fold-thrust belts and sedimentary basins in this region are linked in their evolutionary histories.« less

  11. New view on tectonic structure of Siberian Sector of the Amerasian Basin (Arctic Ocean)

    NASA Astrophysics Data System (ADS)

    Vinokurov, Yu. I.

    2014-05-01

    In 2012, JSC Sevmorgeo with assistance of several research institutions of Federal Agency of Mineral Resources (Rosnedra) and Ministry of Defense carried out a unique set of offshore seismic and geological studies in the Mendeleev Rise area and adjacent areas of the Amerasia Basin. Two specially re-equipped icebreakers ("Kapitan Dranitsin" and "Dixon") were used in this campaign. The main results of the expedition were 5315 km of multichannel seismic profiles both with long and short streamers (4500 m and 600 m, respectively), 480 km long refraction profile crossing Mendeleev Rise. Seismic acquisition with short streamers was accompanied by deployment of sonobuoys. Geological studies included deep-water drilling and sea-bottom sampling by dredge, gravity corer, grab and by specially equipped research submarine. The newly acquired geological and geophysical data allowed for the following conclusions: 1. The Mendeleev Rise, the adjacent Lomonosov Ridge and Chukchi Plateau are the direct continuations of the East Siberian Sea tectonic structures. It is confirmed by direct tracking of some morphostructures, faults, gravity and magnetic anomalies from the shelf to deep-water highs. 2. The East Arctic Shelf and the adjacent Arctic Ocean represent offshore extent of the Verkhoyansk-Kolyma crustal domain constituted by a mosaic of separate blocks of the Pre-Cambrian basement (Okhotsk, Omulevka, Omolon, Wrangel-Gerald and Central Arctic) and Late Mesozoic orogens. This area differs significantly from the Ellesmerian crustal domain located to the east (including the Northwind Ridge, which coincides with inferred eastern boundary of the Mesozoides). The Central Arctic domain includes structures of the Mendeleev Ridge and the Chukchi Plateau. Western boundary of this block is inferred along the Spur of Geophysicists, which separates the Podvodnikov Basin into two unequal parts with different basement structure. From the south, southwest and west, the Central Arctic domain is

  12. Thin and layered subcontinental crust of the great Basin western north America inherited from Paleozoic marginal ocean basins?

    USGS Publications Warehouse

    Churkin, M.; McKee, E.H.

    1974-01-01

    The seismic profile of the crust of the northern part of the Basin and Range province by its thinness and layering is intermediate between typical continental and oceanic crust and resembles that of marginal ocean basins, especially those with thick sedimentary fill. The geologic history of the Great Basin indicates that it was the site of a succession of marginal ocean basins opening and closing behind volcanic arcs during much of Paleozoic time. A long process of sedimentation and deformation followed throughout the Mesozoic modifying, but possibly not completely transforming the originally oceanic crust to continental crust. In the Cenozoic, after at least 40 m.y. of quiescence and stable conditions, substantial crustal and upper-mantle changes are recorded by elevation of the entire region in isostatic equilibrium, crustal extension resulting in Basin and Range faulting, extensive volcanism, high heat flow and a low-velocity mantle. These phenomena, apparently the result of plate tectonics, are superimposed on the inherited subcontinental crust that developed from an oceanic origin in Paleozoic time and possibly retained some of its thin and layered characteristics. The present anomalous crust in the Great Basin represents an accretion of oceanic geosynclinal material to a Precambrian continental nucleus apparently as an intermediate step in the process of conversion of oceanic crust into a stable continental landmass or craton. ?? 1974.

  13. Petroleum prospectivity of the Canada Basin, Arctic Ocean

    USGS Publications Warehouse

    Grantz, A.; Hart, P.E.

    2011-01-01

    Reconnaissance seismic reflection data indicate that Canada Basin is a remnant of the Amerasia Basin of the Arctic Ocean that lies south of the Alpha-Mendeleev Large Igneous Province, which was constructed on the northern part of the Amerasia Basin between about 127 and 89-75 Ma. Canada Basin is filled with Early Jurassic to Holocene detritus from the Mackenzie River system, which drains the northern third of interior North America, with sizable contributions from Alaska and Northwest Canada. Except for the absence of a salt- and shale-bearing mobile substrate Canada Basin is analogous to the Mississippi Delta and the western Gulf of Mexico. Canada Basin contains about 7 to >14 km of sediment beneath the Mackenzie Prodelta on the southeast, 6 to 7 km of sediment beneath the abyssal plain on the west, and roughly 5 or 6 million cubic km of sediment. About three fourths of the basin fill generates low amplitude seismic reflections, interpreted to represent hemiplegic deposits, and a fourth of the fill generates interbedded lenses to extensive layers of moderate to high amplitude reflections interpreted to represent unconfined turbidite and amalgamated channel deposits. Extrapolation from Arctic Alaska and Northwest Canada suggests that three fourths of the section in Canada Basin may contain intervals of hydrocarbon source rocks and the apparent age of the basin suggests that it contains three of the six stratigraphic intervals that together provided >90?? of the World's discovered reserves of oil and gas.. Worldwide heat flow averages suggest that about two thirds of Canada Basin lies in the oil or gas window. At least five types of structural or stratigraphic features of local to regional occurrence offer exploration targets in Canada Basin. These consist of 1) a belt of late Eocene to Miocene shale-cored detachment folds containing with at least two anticlines that are capped by beds with bright spots, 2) numerous moderate to high amplitude reflection packets

  14. Lithospheric structure of the South China Sea and adjacent regions: Results from potential field modelling

    NASA Astrophysics Data System (ADS)

    Chen, Ming; Fang, Jian; Cui, Ronghua

    2018-02-01

    This work aims to investigate the crustal and lithospheric mantle thickness of the South China Sea (SCS) and adjacent regions. The crust-mantle interface, average crustal density, and lithospheric mantle base are calculated from free-air gravity anomaly and topographic data using an iterative inversion method. We construct a three-dimensional lithospheric model with different hierarchical layers. The satellite-derived gravity is used to invert the average crustal density and Moho (crust-mantle interface) undulations. The average crustal density and LAB (lithosphere-asthenosphere boundary) depths are further adjusted by topographic data under the assumption of local isostasy. The average difference in Moho depths between this study and the seismic measurement results is <1.5 km. The results show that in oceanic regions, the Moho depths are 7.5-30 km and the LAB depths are 65-120 km. The lithospheric thickness of the SCS basin and the adjacent regions increases from the sea basin to the continental margin with a large gradient in the ocean-continent transition zones. The Moho depths of conjugate plots during the opening of SCS, Zhongsha Islands and Reed Bank, reveal the asymmetric spreading pattern of SCS seafloor spreading. The lithospheric thinning pattern indicate two different spreading directions during seafloor spreading, which changed from N-S to NW-SE after the southward transition of the spreading axis. The lithosphere of the SCS basin and adjacent regions indicate that the SCS basin is a young basin with a stable interior lithosphere.

  15. Aleutian basin oceanic crust

    USGS Publications Warehouse

    Christeson, Gail L.; Barth, Ginger A.

    2015-01-01

    We present two-dimensional P-wave velocity structure along two wide-angle ocean bottom seismometer profiles from the Aleutian basin in the Bering Sea. The basement here is commonly considered to be trapped oceanic crust, yet there is a change in orientation of magnetic lineations and gravity features within the basin that might reflect later processes. Line 1 extends ∼225 km from southwest to northeast, while Line 2 extends ∼225 km from northwest to southeast and crosses the observed change in magnetic lineation orientation. Velocities of the sediment layer increase from 2.0 km/s at the seafloor to 3.0–3.4 km/s just above basement, crustal velocities increase from 5.1–5.6 km/s at the top of basement to 7.0–7.1 km/s at the base of the crust, and upper mantle velocities are 8.1–8.2 km/s. Average sediment thickness is 3.8–3.9 km for both profiles. Crustal thickness varies from 6.2 to 9.6 km, with average thickness of 7.2 km on Line 1 and 8.8 km on Line 2. There is no clear change in crustal structure associated with a change in orientation of magnetic lineations and gravity features. The velocity structure is consistent with that of normal or thickened oceanic crust. The observed increase in crustal thickness from west to east is interpreted as reflecting an increase in melt supply during crustal formation.

  16. Melting barriers to faunal exchange across ocean basins.

    PubMed

    McKeon, C Seabird; Weber, Michele X; Alter, S Elizabeth; Seavy, Nathaniel E; Crandall, Eric D; Barshis, Daniel J; Fechter-Leggett, Ethan D; Oleson, Kirsten L L

    2016-02-01

    Accelerated loss of sea ice in the Arctic is opening routes connecting the Atlantic and Pacific Oceans for longer periods each year. These changes may increase the ease and frequency with which marine birds and mammals move between the Pacific and Atlantic Ocean basins. Indeed, recent observations of birds and mammals suggest these movements have intensified in recent decades. Reconnection of the Pacific and Atlantic Ocean basins will present both challenges to marine ecosystem conservation and an unprecedented opportunity to examine the ecological and evolutionary consequences of interoceanic faunal exchange in real time. To understand these changes and implement effective conservation of marine ecosystems, we need to further develop modeling efforts to predict the rate of dispersal and consequences of faunal exchange. These predictions can be tested by closely monitoring wildlife dispersal through the Arctic Ocean and using modern methods to explore the ecological and evolutionary consequences of these movements. © 2015 John Wiley & Sons Ltd.

  17. Modern benthic foraminifer distribution in the Amerasian Basin, Arctic Ocean

    USGS Publications Warehouse

    Ishman, S.E.; Foley, K.M.

    1996-01-01

    A total of 38 box cores were collected from the Amerasian Basin, Arctic Ocean during the U.S. Geological Survey 1992 (PI92-AR) and 1993 (PI93-AR) Arctic Cruises aboard the U.S. Coast Guard Icebreaker Polar Star. In addition, the cruises collected geophysical data, piston cores and hydrographic data to address the geologic and oceanographic history of the western Arctic Ocean. This paper reports the results of the quantitative analyses of benthic foraminifer distribution data of the total (live + dead) assemblages derived from 22 box core-top samples. The results show that a distinct depth distribution of three dominant benthic foraminifer assemblages, the Textularia spp. - Spiroplectammina biformis, Cassidulina teretis and Oridorsalis tener - Eponides tumidulus Biofacies are strongly controlled by the dominant water masses within the Canada Basin: the Arctic Surface Water, Arctic Intermediate Water and Canada Basin Deep Water. The faunal distributions and their oceanographic associations in the Canada Basin are consistent with observations of benthic foraminifer distributions from other regions within the Arctic Ocean.

  18. Acquiring Marine Data in the Canada Basin, Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Hutchinson, Deborah R.; Jackson, H. Ruth; Shimeld, John W.; Chapman, C. Borden; Childs, Jonathan R.; Funck, Thomas; Rowland, Robert W.

    2009-06-01

    Despite the record minimum ice extent in the Arctic Ocean for the past 2 years, collecting geophysical data with towed sensors in ice-covered regions continues to pose enormous challenges. Significant parts of the Canada Basin in the western Arctic Ocean have remained largely unmapped because thick multiyear ice has limited access even by research vessels strengthened against ice [Jackson et al., 1990]. Because of the resulting paucity of data, the western Arctic Ocean is one of the few areas of ocean in the world where major controversies still exist with respect to its origin and tectonic evolution [Grantz et al., 1990; Lawver and Scotese, 1990; Lane, 1997; Miller et al., 2006]. This article describes the logistical challenges and initial data sets from geophysical seismic reflection, seismic refraction, and hydrographic surveys in the Canada Basin conducted by scientists with U.S. and Canadian government agencies (Figure 1a) to fulfill the requirements of the United Nations Convention on the Law of the Sea to determine sediment thickness, geological origin, and basin evolution in this unexplored part of the world. Some of these data were collected using a single ship, but the heaviest ice conditions necessitated using two icebreakers, similar to other recent Arctic surveys [e.g., Jokat, 2003].

  19. Carboniferous Proto-type Basin Evolution of Junggar Basin in Northwest China: Implications for the Growth Models of Central Asia Orogenic Belt

    NASA Astrophysics Data System (ADS)

    He, D.

    2016-12-01

    The Junggar Basin locates in the central part of Paleo-Asian Ocean tectonic domain, and records the dynamic processes of the Central Asian Orogenic Belt from subduction-accretion-collision to later intracontinental deformations. Carboniferous is the key period from subduction to closure in the tectonic evolution of Paleo-Asian Ocean. Based on the borehole, outcrop, seismic and gravity and magnetic anomaly data, the paper made analysis of the Carboniferous basin evolution.Geo-chronological results for the borehole volcanic rocks suggest that the Junggar Basin and adjacent area had five periods of volcanic activities, including two periods in the Early Carboniferous (359-347Ma 347-331Ma and 331-324Ma) and three periods in the Late Carboniferous (323-307Ma and 307-300Ma). Regional unconformities divided the Carboniferous into two tectono-stratigraphic sequences: Lower Carboniferous and Upper Carboniferous. The former is characterized by compressional structures and involves massive calc-alkaline basalts, andesites, dacites and rhyolites, whereas the later is mainly controlled by extensional faults and dominated by intermediate-mafic volcanic rocks, with bimodal volcanic rocks in parts. The paper determined four Carboniferous arc-basin belts in the Junggar Basin and adjacent area from north to south: the Saur-Fuhai-Dulate, Heshituoluogai-Wulungu-Yemaquan, Darbut-Luliang-Karamaili, and Zhongguai-Mosuowan-Baijiahai-Qitai, and identified multi-type basins, such as fore-arc basin, retro-arc basin, intra-arc rift basin, foreland basin and passive continental margin basin,etc.. The Carboniferous proto-type basin evolution of the Junggar Basin can be divided into three phases such as, the early to middle Early Carboniferous subduction-related compressional phase, the late Early Carboniferous to middle Late Carboniferous subduction-related extensional phase and the late Late Carboniferous intra-continental fault-sag phase. The study discloses that the Junggar Basin is likely

  20. Observed Recent Trends in Tropical Cyclone Rainfall Over Major Ocean Basins

    NASA Technical Reports Server (NTRS)

    Lau, K. M.; Zhou, Y. P.

    2011-01-01

    In this study, we use Tropical Rainfall Measuring Mission (TRMM) and Global Precipitation Climatology Project (GPCP) rainfall data together with historical storm track records to examine the trend of tropical cyclone (TC) rainfall in major ocean basins during recent decades (1980-2007). We find that accumulated total rainfall along storm tracks for all tropical cyclones shows a weak positive trend over the whole tropics. However, total rainfall associated with weak storms, and intense storms (Category 4-5) both show significant positive trends, while total rainfall associated with intermediate storms (Category1-3) show a significant negative trend. Storm intensity defined as total rain produced per unit storm also shows increasing trend for all storm types. Basin-wide, from the first half (1980-1993) to the second half (1994-2007) of the data period, the North Atlantic shows the pronounced increase in TC number and TC rainfall while the Northeast Pacific shows a significant decrease in all storm types. Except for the Northeast Pacific, all other major basins (North Atlantic, Northwest Pacific, Southern Oceans, and Northern Indian Ocean) show a significant increase in total number and rainfall amount in Category 4-5 storms. Overall, trends in TC rainfall in different ocean basins are consistent with long-term changes in the ambient large-scale environment, including SST, vertical wind shear, sea level pressure, mid-tropospheric humidity, and Maximum Potential Intensity (MPI). Notably the pronounced positive (negative) trend of TC rainfall in the North Atlantic (Northeast Pacific) appears to be related to the most (least) rapid increase in SST and MPI, and the largest decrease (increase) in vertical wind shear in the region, relative to other ocean basins.

  1. Seismic structure of the crust and uppermost mantle of north America and adjacent oceanic basins: A synthesis

    USGS Publications Warehouse

    Chulick, G.S.; Mooney, W.D.

    2002-01-01

    We present a new set of contour maps of the seismic structure of North America and the surrounding ocean basins. These maps include the crustal thickness, whole-crustal average P-wave and S-wave velocity, and seismic velocity of the uppermost mantle, that is, Pn and Sn. We found the following: (1) The average thickness of the crust under North America is 36.7 km (standard deviation [s.d.] ??8.4 km), which is 2.5 km thinner than the world average of 39.2 km (s.d. ?? 8.5) for continental crust; (2) Histograms of whole-crustal P- and S-wave velocities for the North American crust are bimodal, with the lower peak occurring for crust without a high-velocity (6.9-7.3 km/sec) lower crustal layer; (3) Regions with anomalously high average crustal P-wave velocities correlate with Precambrian and Paleozoic orogens; low average crustal velocities are correlated with modern extensional regimes; (4) The average Pn velocity beneath North America is 8.03 km/sec (s.d. ?? 0.19 km/sec); (5) the well-known thin crust beneath the western United States extends into northwest Canada; (6) the average P-wave velocity of layer 3 of oceanic crust is 6.61 km/ sec (s.d. ?? 0.47 km/sec). However, the average crustal P-wave velocity under the eastern Pacific seafloor is higher than the western Atlantic seafloor due to the thicker sediment layer on the older Atlantic seafloor.

  2. Resonance properties of tidal channels with multiple retention basins: role of adjacent sea

    NASA Astrophysics Data System (ADS)

    Roos, Pieter C.; Schuttelaars, Henk M.

    2015-03-01

    We present an idealised model of the tidal response in a main channel with multiple secondary basins, co-oscillating with an adjacent sea. The sea is represented as a semi-infinite strip of finite width, anywhere between the limits of a channel extension (narrow) and a half-plane (wide). The sea geometry controls the extent to which radiative damping takes place and hence the type of conditions that effectively apply at the channel mouth. These conditions range between the two extremes of prescribing elevation (deep sea limit) and prescribing the incoming wave (sea as channel extension of the same depth, as done in an earlier study). The closer to this first extreme, the stronger the oscillations in the secondary basins may feed back onto the channel mouth and thus produce an amplified or weakened response in the system as a whole. The possibly resonant response is explained by analysing the additional waves that emerge on either side of the entrance of the secondary basin. Finally, we show that the simultaneous presence of two secondary basins may amplify or weaken the accumulated responses to these basins individually.

  3. Numerical Simulation of Salinity and Dissolved Oxygen at Perdido Bay and Adjacent Coastal Ocean

    EPA Science Inventory

    Environmental Fluid Dynamic Code (EFDC), a numerical estuarine and coastal ocean circulation hydrodynamic model, was used to simulate the distribution of the salinity, temperature, nutrients and dissolved oxygen (DO) in Perdido Bay and adjacent Gulf of Mexico. External forcing fa...

  4. Latitudinal and Longitudinal Basin-scale Surface Salinity Contrasts and Freshwater Transport by Ocean Thermohaline Circulation

    NASA Astrophysics Data System (ADS)

    Seidov, D.; Haupt, B. J.

    2003-12-01

    The role of sea surface salinity (SSS) contrasts in maintaining vigorous global ocean thermohaline circulation (THC) is revisited. Relative importance of different generalizations of sea surface conditions in climate studies is explored. In numerical experiments using an ocean general circulation model, we have aggregated the observed sea surface temperature (SST) and SSS in several different ways: we used observed unchanged SST with SSS taken as constant (34.25 psu) everywhere; SST unchanged, and SSS zonally averaged globally, i.e., in the whole World Ocean; SST averaged globally, and SSS unchanged; SST zonally averaged globally and SSS zonally averaged basin-wide in individual basins, i.e., in the Atlantic, Indian, Pacific, and Southern Oceans separately; and, finally, both SST and SSS zonally averaged in individual basins. Global zonal averaging removes all longitudinal differences in sea surface climatology among ocean basins. However, latitudinal profiles of zonally averaged parameters preserve the main character of large-scale equator-to-pole sea surface variability. Basin-wide zonal averaging does an even better job of preserving latitudinal distributions within each basin. The results of the experiments could hardly be anticipated a priory. Surprisingly, SST could be used as a 2-D field, or as a zonally-averaged field without much difference in the THC dynamics. Moreover, SST could be averaged either globally, or basin-wide, and it also did not change the overall character of THC. At the same time, THC responded vigorously to how the SSS has been changed. It appeared that the THC structure with the globally averaged SST and basin-wide averaged SSS was very close to the one obtained in the control run (control run operates with 2-D observed SST and SSS). Our main conclusion is that ocean-wide inter-basin sea surface salinity contrasts serve as the major controlling element in global thermohaline circulation. Thermal inter-basin contrasts, as well as

  5. The thermal environment of Cascadia Basin

    NASA Astrophysics Data System (ADS)

    Johnson, H. Paul; Hautala, Susan L.; Bjorklund, Tor A.

    2012-07-01

    Located adjacent to the NE Pacific convergent boundary, Cascadia Basin has a global impact well beyond its small geographic size. Composed of young oceanic crust formed at the Juan de Fuca Ridge, igneous rocks underlying the basin are partially insulated from cooling of their initial heat of formation by a thick layer of pelagic and turbidite sediments derived from the adjacent North American margin. The igneous seafloor is eventually consumed at the Cascadia subduction zone, where interactions between the approaching oceanic crust and the North American continental margin are partially controlled by the thermal environment. Within Cascadia Basin, basement topographic relief varies dramatically, and sediments have a wide range of thickness and physical properties. This variation produces regional differences in heat flow and basement temperatures for seafloor even of similar age. Previous studies proposed a north-south thermal gradient within Cascadia Basin, with high geothermal flux and crustal temperatures measured in the heavily sedimented northern portion near Vancouver Island and lower than average heat flux and basement temperatures predicted for the central and southern portions of the basin. If confirmed, this prediction has implications for processes associated with the Cascadia subduction zone, including the location of the "locked zone" of the megathrust fault. Although existing archival geophysical data in the central and southern basin are sparse, nonuniformly distributed, and derived from a wide range of historical sources, a substantial N-S geothermal gradient appears to be confirmed by our present compilation of combined water column and heat flow measurements.

  6. Chapter 50: Geology and tectonic development of the Amerasia and Canada Basins, Arctic Ocean

    USGS Publications Warehouse

    Grantz, A.; Hart, P.E.; Childers, V.A.

    2011-01-01

    Amerasia Basin is the product of two phases of counterclockwise rotational opening about a pole in the lower Mackenzie Valley of NW Canada. Phase 1 opening brought ocean-continent transition crust (serpentinized peridotite?) to near the seafloor of the proto-Amerasia Basin, created detachment on the Eskimo Lakes Fault Zone of the Canadian Arctic margin and thinned the continental crust between the fault zone and the proto-Amerasia Basin to the west, beginning about 195 Ma and ending prior to perhaps about 160 Ma. The symmetry of the proto-Amerasia Basin was disrupted by clockwise rotation of the Chukchi Microcontinent into the basin from an original position along the Eurasia margin about a pole near 72??N, 165 Wabout 145.5-140 Ma. Phase 2 opening enlarged the proto-Amerasia Basin by intrusion of mid-ocean ridge basalt along its axis between about 131 and 127.5 Ma. Following intrusion of the Phase 2 crust an oceanic volcanic plateau, the Alpha-Mendeleev Ridge LIP (large igneous province), was extruded over the northern Amerasia Basin from about 127 to 89-75 Ma. Emplacement of the LIP halved the area of the Amerasia Basin, and the area lying south of the LIP became the Canada Basin. ?? 2011 The Geological Society of London.

  7. Climate-driven basin-scale decadal oscillations of oceanic phytoplankton.

    PubMed

    Martinez, Elodie; Antoine, David; D'Ortenzio, Fabrizio; Gentili, Bernard

    2009-11-27

    Phytoplankton--the microalgae that populate the upper lit layers of the ocean--fuel the oceanic food web and affect oceanic and atmospheric carbon dioxide levels through photosynthetic carbon fixation. Here, we show that multidecadal changes in global phytoplankton abundances are related to basin-scale oscillations of the physical ocean, specifically the Pacific Decadal Oscillation and the Atlantic Multidecadal Oscillation. This relationship is revealed in approximately 20 years of satellite observations of chlorophyll and sea surface temperature. Interaction between the main pycnocline and the upper ocean seasonal mixed layer is one mechanism behind this correlation. Our findings provide a context for the interpretation of contemporary changes in global phytoplankton and should improve predictions of their future evolution with climate change.

  8. Environmental forcing on life history strategies: Evidence for multi-trophic level responses at ocean basin scales

    USGS Publications Warehouse

    Suryan, Robert M.; Saba, Vincent S.; Wallace, Bryan P.; Hatch, Scott A.; Frederiksen, Morten; Wanless, Sarah

    2009-01-01

    Variation in life history traits of organisms is thought to reflect adaptations to environmental forcing occurring from bottom-up and top-down processes. Such variation occurs not only among, but also within species, indicating demographic plasticity in response to environmental conditions. From a broad literature review, we present evidence for ocean basin- and large marine ecosystem-scale variation in intra-specific life history traits, with similar responses occurring among trophic levels from relatively short-lived secondary producers to very long-lived apex predators. Between North Atlantic and North Pacific Ocean basins, for example, species in the Eastern Pacific exhibited either later maturation, lower fecundity, and/or greater annual survival than conspecifics in the Western Atlantic. Parallel variations in life histories among trophic levels also occur in adjacent seas and between eastern vs. western ocean boundaries. For example, zooplankton and seabird species in cooler Barents Sea waters exhibit lower fecundity or greater annual survival than conspecifics in the Northeast Atlantic. Sea turtles exhibit a larger size and a greater reproductive output in the Western Pacific vs. Eastern Pacific. These examples provide evidence for food-web-wide modifications in life history strategies in response to environmental forcing. We hypothesize that such dichotomies result from frequency and amplitude shifts in resource availability over varying temporal and spatial scales. We review data that supports three primary mechanisms by which environmental forcing affects life history strategies: (1) food-web structure; (2) climate variability affecting the quantity and seasonality of primary productivity; (3) bottom-up vs. top-down forcing. These proposed mechanisms provide a framework for comparisons of ecosystem function among oceanic regions (or regimes) and are essential in modeling ecosystem response to climate change, as well as for creating dynamic ecosystem

  9. On the role of inter-basin surface salinity contrasts in global ocean circulation

    NASA Astrophysics Data System (ADS)

    Seidov, D.; Haupt, B. J.

    2002-08-01

    The role of sea surface salinity (SSS) contrasts in maintaining vigorous global ocean thermohaline circulation (TOC) is revisited. Relative importance of different generalizations of sea surface conditions in climate studies is explored. Ocean-wide inter-basin SSS contrasts serve as the major controlling element in global TOC. These contrasts are shown to be at least as important as high-latitudinal freshwater impacts. It is also shown that intra-basin longitudinal distribution of sea surface salinity, as well as intra- and inter-basin longitudinal distribution of sea surface temperature, is not crucial to conveyor functionality if only inter-basin contrasts in sea surface salinity are retained. This is especially important for paleoclimate and future climate simulations.

  10. Permian plate margin volcanism and tuffs in adjacent basins of west Gondwana: Age constraints and common characteristics

    NASA Astrophysics Data System (ADS)

    López-Gamundí, Oscar

    2006-12-01

    Increasing evidence of Permian volcanic activity along the South American portion of the Gondwana proto-Pacific margin has directed attention to its potential presence in the stratigraphic record of adjacent basins. In recent years, tuffaceous horizons have been identified in late Early Permian-through Middle Permian (280-260 Ma) sections of the Paraná Basin (Brazil, Paraguay, and Uruguay). Farther south and closer to the magmatic tract developed along the continental margin, in the San Rafael and Sauce Grande basins of Argentina, tuffs are present in the Early to Middle Permian section. This tuff-rich interval can be correlated with the appearance of widespread tuffs in the Karoo Basin. Although magmatic activity along the proto-Pacific plate margin was continuous during the Late Paleozoic, Choiyoi silicic volcanism along the Andean Cordillera and its equivalent in Patagonia peaked between the late Early Permian and Middle Permian, when extensive rhyolitic ignimbrites and consanguineous airborne tuffaceous material erupted in the northern Patagonian region. The San Rafael orogenic phase (SROP) interrupted sedimentation along the southwestern segment of the Gondwana margin (i.e., Frontal Cordillera, San Rafael Basin), induced cratonward thrusting (i.e., Ventana and Cape foldbelts), and triggered accelerated subsidence in the adjacent basins (Sauce Grande and Karoo) located inboard of the deformation front. This accelerated subsidence favored the preservation of tuffaceous horizons in the syntectonic successions. The age constraints and similarities in composition between the volcanics along the continental margin and the tuffaceous horizons in the San Rafael, Sauce Grande, Paraná, and Karoo basins strongly suggest a genetic linkage between the two episodes. Radiometric ages from tuffs in the San Rafael, Paraná, and Karoo basins indicate an intensely tuffaceous interval between 280 and 260 Ma.

  11. Geologic interpretation of gravity data from the Date Creek basin and adjacent areas, west-central Arizona

    USGS Publications Warehouse

    Otton, James K.; Wynn, Jeffrey C.

    1978-01-01

    A gravity survey of the Date Creek Basin and adjacent areas was conducted in June 1977 to provide information for the interpretation of basin geology. A comparison of facies relations in the locally uraniferous Chapin Wash Formation and the position of the Anderson mine gravity anomaly in the Date Creek Basin suggested that a relationship between gravity lows and the development of thick lacustrine sections in the region might exist. A second-order residual gravity map derived from the complete Bouguer gravity map for the survey area (derived from survey data and pre-existing U.S. Department of Defense data) shows an excellent correspondence between gravity lows and sediment-filled basins and suggests considerable variation in basin-fill thickness. Using the Anderson mine anomaly as a model, gravity data and facies relations suggest that the southeastern flank of the Aguila Valley gravity low and the gravity low at the western end of the Hassayampa Plain are likely areas for finding thick sections of tuffaceous lacustrine rocks.

  12. Nature and tectonic implications of uneven sedimentary filling of the South China Sea oceanic basin

    NASA Astrophysics Data System (ADS)

    Yin, Shaoru; Li, Jiabiao; Ding, Weiwei; Fang, Yinxia

    2017-04-01

    The IODP Expedition 349 in 2014, for the first time, illustrated significant differences of sediment rate and lithology in the central South China Sea (SCS) oceanic basin. Based on seismic reflection profiles tied to IODP349 drilling data, we investigated characteristics of sedimentary filling of the whole SCS oceanic basin, and examined their implications for tectonics. Results show that sediments fill the SCS oceanic basin mainly in three depositional patterns. Firstly, during the Oligocene to middle Miocene, sediments amassed almost solely and then connected like a band parallel to the continent in a low average sediment rate (<10 m/Myr) in the northern oceanic basin. These sediments were deposited mainly in the form of submarine fans and mass transport deposits. Sediments were predominately supplied by the Red and Pearl Rivers and the Dongsha Islands. The sedimentary characteristics likely reflect the latest early Miocene end of seafloor spreading of the SCS and the first-phase rapid uplift of the Tibetan Plateau. Secondly, during the late Miocene, deposition mainly occurred in the Northwest Sub-basin and extended southeastward with a middle average sediment rate ( 30 m/Myr). Sediments were mostly transported by the Red River and Xisha Trough and deposited in the form of submarine fans. The abnormal increase of sediment rate in the Northwest Sub-basin reflects late Miocene slip reversal of the Red River Fault. Finally, since the Pliocene, sediments gradually propagated northeastward in the Southwestern Sub-basin, and accumulated rapidly in the southeastern and northeastern basin, especially in the northern Manila Trench during the Quaternary, in an average sediment rate about 60-80 m/Myr. These sediments were transported mainly by submarine canyons and settled in the form of submarine fans and canyon-overbank deposition. Sediments came from four major sources, including Taiwan, Dongsha Islands, Mekong River, and northern Palawan. The Pliocene to Quaternary

  13. A Basin-Wide Examination of the Arctic Ocean's Double-Diffusive Staircase

    NASA Astrophysics Data System (ADS)

    Shibley, N.; Timmermans, M. L.; Carpenter, J. R.; Toole, J. M.

    2016-02-01

    The Arctic Ocean thermohaline stratification frequently exhibits a staircase structure above the Atlantic Water Layer consisting of multiple mixed layers of order 1-m in height separated by sharp interfaces. This double-diffusive staircase structure is characterized across the entire Arctic Ocean through a detailed analysis of Ice-Tethered Profiler measurements acquired between 2004 and 2013. Staircase properties (mixed layer thicknesses and temperature-salinity jumps across interfaces) are examined in relation to a bulk vertical density ratio for 50-m spanning the staircase stratification. It is shown that the Lomonosov Ridge serves as an approximate boundary between regions of low density ratio (on the Eurasian side) and higher density ratio (on the Canadian side). We find that the diffusive staircase in the Eurasian Basin is characterized by fewer, thinner mixed layers than that in the Canadian Basin, although the margins of all basins are characterized by relatively thin staircase mixed layers. Using a double-diffusive 4/3 flux law parameterization, the distribution of vertical heat fluxes through the staircase is estimated across the Arctic; it is found that heat fluxes in the Eurasian Basin [O(1) W/m^2] are generally an order of magnitude larger than those in the Canadian Basin [O(0.1) W/m^2].

  14. Cretaceous evolution of the Indian Plate and consequences for the formation, deformation and obduction of adjacent oceanic crust

    NASA Astrophysics Data System (ADS)

    Gaina, C.; Van Hinsbergen, D. J.; Spakman, W.

    2012-12-01

    As part of the gradual Gondwana dispersion that started in the Jurassic, the Indian tectonic block was rifted away from the Antarctica-Australian margins, probably in the Early-Mid Cretaceous and started its long journey to the north until it collided with Eurasia in the Tertiary. In this contribution first we will revise geophysical and geological evidences for the formation of oceanic crust between India and Antarctica, India and Madagascar, and India and Somali/Arabian margins. This information and possible oceanic basin age interpretation are placed into regional kinematic models. Three important compressional events NW and W of the Indian plate are the result of the opening of the Enderby Basin from 132 to 124 Ma, the first phase of seafloor spreading in the Mascarene basin approximately from 84 to 80 Ma, and the incipient opening of the Arabian Sea and the Seychelles microplate formation around 65 to 60 Ma. Based on retrodeformation of the Afghan-Pakistan part of the India-Asia collision zone and the eastern Oman margin, the ages of regional ophiolite emplacement and crystallization of its oceanic crust, as well as the plate tectonic setting of these ophiolites inferred from its geochemistry, we evaluate possible scenarios for the formation of intra-oceanic subduction zones and their evolution until ophiolite emplacement time. Our kinematic scenarios are constructed for several regional models and are discussed in the light of global tomographic models that may image some of the subducted Cretaceous oceanic lithosphere.

  15. Summary of the geology and resources of uranium in the San Juan Basin and adjacent region, New Mexico, Arizona, Utah, and Colorado

    USGS Publications Warehouse

    Ridgley, Jennie L.; Green, M.W.; Pierson, C.T.; Finch, W.I.; Lupe, R.D.

    1978-01-01

    The San Juan Basin and adjacent region lie predominantly in the southeastern part of the uranium-rich Colorado Plateau of New Mexico, Arizona, Utah, and Colorado. Underlying the province are rocks of the Precambrian basement complex composed mainly of igneous and metamorphic rocks; a thickness of about 3,600 meters of generally horizontal Paleozoic, Mesozoic, and Cenozoic sedimentary rocks; and a variety of Upper Cretaceous and Cenozoic igneous rocks. Sedimentary rocks of the sequence are commonly eroded and well exposed near the present basin margins where Tertiary tectonic activity has uplifted, folded, and faulted the sequence into its present geologic configuration of basins, platforms, monoclines, and other related structural features. Sedimentary rocks of Jurassic age in the southern part of the San Juan Basin contain the largest uranium deposits in the United States, and offer the promise of additional uranium deposits. Elsewhere in the basin and the adjacent Colorado Plateau, reserves and resources of uranium are known primarily in Triassic, Jurassic, and Cretaceous strata. Only scattered occurrences of uranium are known in Paleozoic

  16. Formation of the Sputnik Planum basin and the thickness of Pluto's subsurface ocean

    NASA Astrophysics Data System (ADS)

    Johnson, Brandon C.; Bowling, Timothy J.; Trowbridge, Alexander J.; Freed, Andrew M.

    2016-10-01

    We simulate the formation of the large elliptical impact basin associated with Pluto's Sputnik Planum (SP; informal name). The location of SP suggests that it represents a large positive mass anomaly. To find the conditions necessary for SP to have a positive mass anomaly, we consider impacts into targets with a range of thermal states and ocean thicknesses. Assuming the basin evolves to its current-day configuration, we calculate the mass and gravity anomalies associated with SP. We find that SP can only achieve a large positive mass anomaly if Pluto has a more than 100 km thick salty ocean. This conclusion may help us better understand the composition and thermal evolution of Pluto. Furthermore, our work supports the hypothesis that SP basin has an impact origin.

  17. Laramide structure of the central Sangre de Cristo Mountains and adjacent Raton Basin, southern Colorado

    USGS Publications Warehouse

    Lindsey, D.A.

    1998-01-01

    Laramide structure of the central Sangre de Cristo Mountains (Culebra Range) is interpreted as a system of west-dipping, basement-involved thrusts and reverse faults. The Culebra thrust is the dominant structure in the central part of the range; it dips 30 -55?? west and brings Precambrian metamorphic base-ment rocks over unmetamorphosed Paleozoic rocks. East of the Culebra thrust, thrusts and reverse faults break the basement and overlying cover rocks into north-trending fault blocks; these boundary faults probably dip 40-60?? westward. The orientation of fault slickensides indicates oblique (northeast) slip on the Culebra thrust and dip-slip (ranging from eastward to northward) movement on adjacent faults. In sedimentary cover rocks, east-vergent anticlines overlie and merge with thrusts and reverse faults; these anticlines are interpreted as fault-propagation folds. Minor east-dipping thrusts and reverse faults (backthrusts) occur in both the hanging walls and footwalls of thrusts. The easternmost faults and folds of the Culebra Range form a continuous structural boundary between the Laramide Sangre de Cristo highland and the Raton Basin. Boundary structures consist of west-dipping frontal thrusts flanked on the basinward side by poorly exposed, east-dipping backthrusts. The backthrusts are interpreted to overlie structural wedges that have been emplaced above blind thrusts in the basin margin. West-dipping frontal thrusts and blind thrusts are interpreted to involve basement, but backthrusts are rooted in basin-margin cover rocks. At shallow structural levels where erosion has not exposed a frontal thrust, the structural boundary of the basin is represented by an anticline or monocline. Based on both regional and local stratigraphic evidence, Laramide deformation in the Culebra Range and accompanying synorogenic sedimentation in the western Raton Basin probably took place from latest Cretaceous through early Eocene time. The earliest evidence of uplift and

  18. Petroleum prospectivity of the Canada Basin, Arctic Ocean

    USGS Publications Warehouse

    Grantz, Arthur; Hart, Patrick E.

    2012-01-01

    Reconnaissance seismic reflection data indicate that Canada Basin is a >700,000 sq. km. remnant of the Amerasia Basin of the Arctic Ocean that lies south of the Alpha-Mendeleev Large Igneous Province, which was constructed across the northern part of the Amerasia Basin between about 127 and 89-83.5 Ma. Canada Basin was filled by Early Jurassic to Holocene detritus from the Beaufort-Mackenzie Deltaic System, which drains the northern third of interior North America, with sizable contributions from Alaska and Northwest Canada. The basin contains roughly 5 or 6 million cubic km of sediment. Three fourths or more of this volume generates low amplitude seismic reflections, interpreted to represent hemipelagic deposits, which contain lenses to extensive interbeds of moderate amplitude reflections interpreted to represent unconfined turbidite and amalgamated channel deposits.Extrapolation from Arctic Alaska and Northwest Canada suggests that three fourths of the section in Canada Basin is correlative with stratigraphic sequences in these areas that contain intervals of hydrocarbon source rocks. In addition, worldwide heat flow averages suggest that about two thirds of Canada Basin lies in the oil or gas windows. Structural, stratigraphic and combined structural and stratigraphic features of local to regional occurrence offer exploration targets in Canada Basin, and at least one of these contains bright spots. However, deep water (to almost 4000 m), remoteness from harbors and markets, and thick accumulations of seasonal to permanent sea ice (until its possible removal by global warming later this century) will require the discovery of very large deposits for commercial success in most parts of Canada Basin. ?? 2011 Elsevier Ltd.

  19. Chapter 50 Geology and tectonic development of the Amerasia and Canada Basins, Arctic Ocean

    USGS Publications Warehouse

    Grantz, Arthur; Hart, Patrick E.; Childers, Vicki A

    2011-01-01

    Amerasia Basin is the product of two phases of counterclockwise rotational opening about a pole in the lower Mackenzie Valley of NW Canada. Phase 1 opening brought ocean–continent transition crust (serpentinized peridotite?) to near the seafloor of the proto-Amerasia Basin, created detachment on the Eskimo Lakes Fault Zone of the Canadian Arctic margin and thinned the continental crust between the fault zone and the proto-Amerasia Basin to the west, beginning about 195 Ma and ending prior to perhaps about 160 Ma. The symmetry of the proto-Amerasia Basin was disrupted by clockwise rotation of the Chukchi Microcontinent into the basin from an original position along the Eurasia margin about a pole near 72°N, 165 W about 145.5–140 Ma. Phase 2 opening enlarged the proto-Amerasia Basin by intrusion of mid-ocean ridge basalt along its axis between about 131 and 127.5 Ma. Following intrusion of the Phase 2 crust an oceanic volcanic plateau, the Alpha–Mendeleev Ridge LIP (large igneous province), was extruded over the northern Amerasia Basin from about 127 to 89–75 Ma. Emplacement of the LIP halved the area of the Amerasia Basin, and the area lying south of the LIP became the Canada Basin.

  20. Decorrelation scales for Arctic Ocean hydrography - Part I: Amerasian Basin

    NASA Astrophysics Data System (ADS)

    Sumata, Hiroshi; Kauker, Frank; Karcher, Michael; Rabe, Benjamin; Timmermans, Mary-Louise; Behrendt, Axel; Gerdes, Rüdiger; Schauer, Ursula; Shimada, Koji; Cho, Kyoung-Ho; Kikuchi, Takashi

    2018-03-01

    Any use of observational data for data assimilation requires adequate information of their representativeness in space and time. This is particularly important for sparse, non-synoptic data, which comprise the bulk of oceanic in situ observations in the Arctic. To quantify spatial and temporal scales of temperature and salinity variations, we estimate the autocorrelation function and associated decorrelation scales for the Amerasian Basin of the Arctic Ocean. For this purpose, we compile historical measurements from 1980 to 2015. Assuming spatial and temporal homogeneity of the decorrelation scale in the basin interior (abyssal plain area), we calculate autocorrelations as a function of spatial distance and temporal lag. The examination of the functional form of autocorrelation in each depth range reveals that the autocorrelation is well described by a Gaussian function in space and time. We derive decorrelation scales of 150-200 km in space and 100-300 days in time. These scales are directly applicable to quantify the representation error, which is essential for use of ocean in situ measurements in data assimilation. We also describe how the estimated autocorrelation function and decorrelation scale should be applied for cost function calculation in a data assimilation system.

  1. Correlation of sea level falls interpreted from atoll stratigraphy with turbidites in adjacent basins

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

    Lincoln, J.M.

    Past sea levels can be derived from any atoll subsurface sediments deposited at or near sea level by determining the ages of deposition and correcting the present depths to the sediments for subsidence of the underlying edifice since the times of deposition. A sea level curve constructed by this method consists of discontinuous segments, each corresponding to a period of rising relative sea level and deposition of a discrete sedimentary package. Discontinuities in the sea level curve derived by this method correspond to relative sea level falls and stratigraphic hiatuses in the atoll subsurface. During intervals of relative sea levelmore » fall an atoll emerges to become a high limestone island. Sea level may fluctuate several times during a period of atoll emergence to become a high limestone island. Sea level may fluctuate several times during a period of atoll emergence without depositing sediments on top of the atoll. Furthermore, subaerial erosion may remove a substantial part of the depositional record of previous sea level fluctuations. For these reasons the authors must look to the adjacent basins to complement the incomplete record of sea level change recorded beneath atolls. During lowstands of sea level, faunas originally deposited near sea level on an atoll may be eroded and redeposited as turbidites in deep adjacent basins. Three such turbidites penetrated during deep-sea drilling at Sites 462 and 315 in the central Pacific correlate well with a late Tertiary sea level curve based on biostratigraphic ages and {sup 87}Sr/{sup 86}Sr chronostratigraphy for core from Enewetak Atoll in the northern Marshall Islands. Further drilling of the archipelagic aprons adjacent to atolls will improve the sea level history that may be inferred from atoll stratigraphy.« less

  2. Generations of spreading basins and stages of breakdown of Wegener's Pangea in the geodynamic evolution of the Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Shipilov, E. V.

    2008-03-01

    Chronological succession in the formation of spreading basins is considered in the context of reconstruction of breakdown of Wegener’s Pangea and the development of the geodynamic system of the Arctic Ocean. This study made it possible to indentify three temporally and spatially isolated generations of spreading basins: Late Jurassic-Early Cretaceous, Late Cretaceous-Early Cenozoic, and Cenozoic. The first generation is determined by the formation, evolution, and extinction of the spreading center in the Canada Basin as a tectonic element of the Amerasia Basin. The second generation is connected to the development of the Labrador-Baffin-Makarov spreading branch that ceased to function in the Eocene. The third generation pertains to the formation of the spreading system of interrelated ultraslow Mohna, Knipovich, and Gakkel mid-ocean ridges that has functioned until now in the Norwegian-Greenland and Eurasia basins. The interpretation of the available geological and geophysical data shows that after the formation of the Canada Basin, the Arctic region escaped the geodynamic influence of the Paleopacific, characterized by spreading, subduction, formation of backarc basins, collision-related processes, etc. The origination of the Makarov Basin marks the onset of the oceanic regime characteristic of the North Atlantic (intercontinental rifting, slow and ultraslow spreading, separation of continental blocks (microcontinents), extinction of spreading centers of primary basins, spreading jumps, formation of young spreading ridges and centers, etc., are typical) along with retention of northward propagation of spreading systems both from the Pacific and Atlantic sides. The aforesaid indicates that the Arctic Ocean is in fact a hybrid basin or, in other words, a composite heterogeneous ocean in respect to its architectonics. The Arctic Ocean was formed as a result of spatial juxtaposition of two geodynamic systems different in age and geodynamic style: the Paleopacific

  3. Downscaling ocean conditions with application to the Gulf of Maine, Scotian Shelf and adjacent deep ocean

    NASA Astrophysics Data System (ADS)

    Katavouta, Anna; Thompson, Keith

    2017-04-01

    A high resolution regional model (1/36 degree) of the Gulf of Maine, Scotian Shelf and adjacent deep ocean (GoMSS) is developed to downscale ocean conditions from an existing global operational system. First, predictions from the regional GoMSS model in a one-way nesting set up are evaluated using observations from multiple sources including satellite-borne sensors of surface temperature and sea level, CTDs, Argo floats and moored current meters. It is shown that on the shelf, the regional model predicts more realistic fields than the global system because it has higher resolution and includes tides that are absent from the global system. However, in deep water the regional model misplaces deep ocean eddies and meanders associated with the Gulf Stream. This is because of unrealistic internally generated variability (associated with the one-way nesting set up) that leads to decoupling of the regional model from the global system in the deep water. To overcome this problem, the large scales (length scales > 90 km) of the regional model are spectrally nudged towards the global system fields. This leads to more realistic predictions off the shelf. Wavenumber spectra show that even though spectral nudging constrains the large scales, it does not suppress the variability on small scales; on the contrary, it favours the formation of eddies with length scales below the cut-off wavelength of the spectral nudging.

  4. Ancient Continental Lithosphere Dislocated Beneath Ocean Basins Along the Mid-Lithosphere Discontinuity: A Hypothesis

    NASA Astrophysics Data System (ADS)

    Wang, Zhensheng; Kusky, Timothy M.; Capitanio, Fabio A.

    2017-09-01

    The documented occurrence of ancient continental cratonic roots beneath several oceanic basins remains poorly explained by the plate tectonic paradigm. These roots are found beneath some ocean-continent boundaries, on the trailing sides of some continents, extending for hundreds of kilometers or farther into oceanic basins. We postulate that these cratonic roots were left behind during plate motion, by differential shearing along the seismically imaged mid-lithosphere discontinuity (MLD), and then emplaced beneath the ocean-continent boundary. Here we use numerical models of cratons with realistic crustal rheologies drifting at observed plate velocities to support the idea that the mid-lithosphere weak layer fostered the decoupling and offset of the African continent's buoyant cratonic root, which was left behind during Meso-Cenozoic continental drift and emplaced beneath the Atlantic Ocean. We show that in some cratonic areas, the MLD plays a similar role as the lithosphere-asthenosphere boundary for accommodating lateral plate tectonic displacements.

  5. Volcanism and Tectonics of the Central Deep Basin, Sea of Japan

    NASA Astrophysics Data System (ADS)

    Lelikov, E. P.; Emelyanova, T. A.; Pugachev, A. A.

    2018-01-01

    The paper presents the results of a study on the geomorphic structure, tectonic setting, and volcanism of the volcanoes and volcanic ridges in the deep Central Basin of the Sea of Japan. The ridges rise 500-600 m above the acoustic basement of the basin. These ridges were formed on fragments of thinned continental crust along deep faults submeridionally crossing the Central Basin and the adjacent continental part of the Primorye. The morphostructures of the basin began to submerge below sea level in the Middle Miocene and reached their contemporary positions in the Pliocene. Volcanism in the Central Basin occurred mostly in the Middle Miocene-Pliocene and formed marginal-sea basaltoids with OIB (ocean island basalt) geochemical signatures indicating the lower-mantle plume origin of these rocks. The OIB signatures of basaltoids tend to be expressed better in the eastern part of the Central Basin, where juvenile oceanic crust has developed. The genesis of this crust is probably related to rising and melting of the Pacific superplume apophyse.

  6. Assessment of Plio-Pleistocene Sea Surface Temperature Evolution Across Ocean Basins, Hemispheres, and Latitudes

    NASA Astrophysics Data System (ADS)

    Peterson, L.; Lawrence, K. T.; Mauriello, H.; Wilson, J.; Holte, L.

    2015-12-01

    New sea surface temperature (SST) records from the southern Pacific and southern Atlantic Oceans allow assessment of similarities and differences in climate evolution across ocean basins, hemispheres, and latitudes over the last 5 million years. Our high-resolution, alkenone-derived SST records from ODP Sites 1088 (South Atlantic, 41°S) and 1125 (South Pacific, 42°S) share strong structural similarities. When compared with SST records from the mid-latitudes of the northern hemisphere, these records provide compelling evidence for broadly hemispherically symmetrical open-ocean temperature evolution in both ocean basins as tropical warm pools contracted over the Plio-Pleistocene. This symmetry in temperature evolution occurs despite strong asymmetries in the development of the cryosphere over this interval, which was marked by extensive northern hemisphere ice sheet growth. Parallel SST evolution across ocean basins and hemispheres suggests that on longterm (>105 yr) timescales, many regions of the world ocean are more sensitive to the global energy budget than to local or regional climate dynamics, although important exceptions include coastal upwelling zone SSTs, high latitude SSTs, and benthic δ18O. Our analysis further reveals that throughout the last 5 Ma, temperature evolution in the extra-tropical Pacific of both hemispheres is very similar to the evolution of SST in the eastern equatorial Pacific upwelling zone, revealing tight coupling between the growth of meridional and equatorial Pacific zonal temperature gradients over this interval as both the extra-tropics and the eastern equatorial Pacific cold tongue underwent cooling. Finally, while long term temperature evolution is broadly consistent across latitudes and ocean basins throughout the entire Plio-Pleistocene, we see evidence that climate coupling on orbital timescales strengthened significantly at 2.7 Ma, at which point obliquity-band coherence emerges among diverse SST records. We attribute this

  7. 33 CFR 334.1050 - Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of...

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. 334..., DEPARTMENT OF DEFENSE DANGER ZONE AND RESTRICTED AREA REGULATIONS § 334.1050 Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. (a...

  8. 33 CFR 334.1050 - Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of...

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. 334..., DEPARTMENT OF DEFENSE DANGER ZONE AND RESTRICTED AREA REGULATIONS § 334.1050 Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. (a...

  9. 33 CFR 334.1050 - Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of...

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. 334..., DEPARTMENT OF DEFENSE DANGER ZONE AND RESTRICTED AREA REGULATIONS § 334.1050 Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. (a...

  10. 33 CFR 334.1050 - Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of...

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. 334..., DEPARTMENT OF DEFENSE DANGER ZONE AND RESTRICTED AREA REGULATIONS § 334.1050 Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. (a...

  11. 33 CFR 334.1050 - Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of...

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. 334..., DEPARTMENT OF DEFENSE DANGER ZONE AND RESTRICTED AREA REGULATIONS § 334.1050 Oakland Outer Harbor adjacent to the Military Ocean Terminal, Bay Area, Pier No. 8 (Port of Oakland Berth No. 10); restricted area. (a...

  12. Formation of the Sputnik Planum basin and the thickness of Pluto's subsurface ocean

    NASA Astrophysics Data System (ADS)

    Johnson, B. C.; Bowling, T.; Trowbridge, A.; Freed, A. M.

    2016-12-01

    Since the New Horizons flyby, evidence has been mounting that Pluto's Sputnik Planum (SP; informal name) (1,2) is associated with a 800-1000 km diameter elliptical impact basin (3,4). Global tectonics and the location of SP suggests that Pluto reoriented to align the basin with its tidal axis (4,5). This indicates there is a large positive mass anomaly associated with SP (4,5). However, even with loading of 3-10 km of dense convecting N2 ice (6,7), a positive mass anomaly associated with the deep basin requires that Pluto has a liquid ocean and the ice shell under the basin is substantially thinned (4). Although the possibility of a slowly freezing current day subsurface ocean is supported by thermal modeling (8,9) and the ubiquity of young extensional tectonic features (1), the thickness of the putative ocean is unconstrained. Here, we simulate the SP basin-forming impact into targets with a range of thermal states and ocean thicknesses. We find that SP can only achieve a large positive mass anomaly if Pluto has a more than 100 km thick salty ocean (i.e. ocean density exceeding 1100 kg/m3). This conclusion may help us better understand the composition and thermal evolution of Pluto. 1. Moore, J. M. et al. Science 351,1284-1293 (2016). 2. Stern, S. A. et al. Science 350,aad1815-aad1815 (2015). 3. Schenk, P. M. et al. A Large Impact Origin for Sputnik Planum and Surrounding Terrains, Pluto? AAS/Division for Planetary Sciences Meeting Abstracts 47,(2015). 4. Nimmo, F. et al. Loading, Relaxation, and Tidal Wander at Sputnik Planum, Pluto. 47th Lunar and Planetary Science Conference 47,2207 (2016). 5. Keane, J. T. & Matsuyama, I. Pluto Followed Its Heart: True Polar Wander of Pluto Due to the Formation and Evolution of Sputnik Planum. 47th Lunar and Planetary Science Conference 47,2348 (2016). 6. Trowbridge, A. J., Melosh, H. J., Steckloff, J. K. & Freed, A. M. Nature 534,79-81 (2016). 7. McKinnon, W. B. et al. Nature 534,82-85 (2016). 8. Robuchon, G. & Nimmo, F

  13. Near-island biological hotspots in barren ocean basins

    PubMed Central

    Gove, Jamison M.; McManus, Margaret A.; Neuheimer, Anna B.; Polovina, Jeffrey J.; Drazen, Jeffrey C.; Smith, Craig R.; Merrifield, Mark A.; Friedlander, Alan M.; Ehses, Julia S.; Young, Charles W.; Dillon, Amanda K.; Williams, Gareth J.

    2016-01-01

    Phytoplankton production drives marine ecosystem trophic-structure and global fisheries yields. Phytoplankton biomass is particularly influential near coral reef islands and atolls that span the oligotrophic tropical oceans. The paradoxical enhancement in phytoplankton near an island-reef ecosystem—Island Mass Effect (IME)—was first documented 60 years ago, yet much remains unknown about the prevalence and drivers of this ecologically important phenomenon. Here we provide the first basin-scale investigation of IME. We show that IME is a near-ubiquitous feature among a majority (91%) of coral reef ecosystems surveyed, creating near-island ‘hotspots' of phytoplankton biomass throughout the upper water column. Variations in IME strength are governed by geomorphic type (atoll vs island), bathymetric slope, reef area and local human impacts (for example, human-derived nutrient input). These ocean oases increase nearshore phytoplankton biomass by up to 86% over oceanic conditions, providing basal energetic resources to higher trophic levels that support subsistence-based human populations. PMID:26881874

  14. Near-island biological hotspots in barren ocean basins.

    PubMed

    Gove, Jamison M; McManus, Margaret A; Neuheimer, Anna B; Polovina, Jeffrey J; Drazen, Jeffrey C; Smith, Craig R; Merrifield, Mark A; Friedlander, Alan M; Ehses, Julia S; Young, Charles W; Dillon, Amanda K; Williams, Gareth J

    2016-02-16

    Phytoplankton production drives marine ecosystem trophic-structure and global fisheries yields. Phytoplankton biomass is particularly influential near coral reef islands and atolls that span the oligotrophic tropical oceans. The paradoxical enhancement in phytoplankton near an island-reef ecosystem--Island Mass Effect (IME)--was first documented 60 years ago, yet much remains unknown about the prevalence and drivers of this ecologically important phenomenon. Here we provide the first basin-scale investigation of IME. We show that IME is a near-ubiquitous feature among a majority (91%) of coral reef ecosystems surveyed, creating near-island 'hotspots' of phytoplankton biomass throughout the upper water column. Variations in IME strength are governed by geomorphic type (atoll vs island), bathymetric slope, reef area and local human impacts (for example, human-derived nutrient input). These ocean oases increase nearshore phytoplankton biomass by up to 86% over oceanic conditions, providing basal energetic resources to higher trophic levels that support subsistence-based human populations.

  15. Origin, transport and deposition of leaf-wax biomarkers in the Amazon Basin and the adjacent Atlantic

    NASA Astrophysics Data System (ADS)

    Häggi, Christoph; Sawakuchi, André O.; Chiessi, Cristiano M.; Mulitza, Stefan; Mollenhauer, Gesine; Sawakuchi, Henrique O.; Baker, Paul A.; Zabel, Matthias; Schefuß, Enno

    2016-11-01

    -chain n-alkanes from the Amazon estuary and plume represent an integrated signal of different regions of the onshore basin. Our results also imply that n-alkanes are not extensively remineralized during transport and that the signal at the Amazon estuary and plume includes refractory compounds derived from the western sector of the Basin. These findings will aid in the interpretation of plant wax-based records of marine sediment cores collected from the adjacent ocean.

  16. Deformation Rates in the Snake River Plain and Adjacent Basin and Range Regions Based on GPS Measurements

    NASA Astrophysics Data System (ADS)

    Payne, S. J.; McCaffrey, R.; King, R. W.; Kattenhorn, S. A.

    2012-12-01

    We estimate horizontal velocities for 405 sites using Global Positioning System (GPS) phase data collected from 1994 to 2010 within the Northern Basin and Range Province, U.S.A. The velocities reveal a slowly-deforming region within the Snake River Plain in Idaho and Owyhee-Oregon Plateau in Oregon separated from the actively extending adjacent Basin and Range regions by shear. Our results show a NE-oriented extensional strain rate of 5.6 ± 0.7 nanostrain/yr in the Centennial Tectonic Belt and an ~E-oriented extensional strain rate of 3.5 ± 0.2 nanostrain/yr in the Great Basin. These extensional rates contrast with the very low strain rate within the 125 km x 650 km region of the Snake River Plain and Owyhee-Oregon Plateau which is not distinguishable from zero (-0.1 ± 0.4 x nanostrain/yr). Inversions of Snake River Plain velocities with dike-opening models indicate that rapid extension by dike intrusion in volcanic rift zones, as previously hypothesized, is not currently occurring. GPS data also disclose that rapid extension in the surrounding regions adjacent to the slowly-deforming region of the Snake River Plain drives shear between them. We estimate right-lateral shear with slip rates of 0.3-1.5 mm/yr along the northwestern boundary adjacent to the Centennial Tectonic Belt and left-lateral oblique extension with slip rates of 0.5-1.5 mm/yr along the southeastern boundary adjacent to the Intermountain Seismic Belt. The fastest lateral shearing evident in the GPS occurs near the Yellowstone Plateau where earthquakes with right-lateral strike-slip focal mechanisms are within a NE-trending zone of seismicity. The regional velocity gradients are best fit by nearby poles of rotation for the Centennial Tectonic Belt, Snake River Plain, Owyhee-Oregon Plateau, and eastern Oregon, indicating that clockwise rotation is not locally driven by Yellowstone hotspot volcanism, but instead by extension to the south across the Wasatch fault possibly due to gravitational

  17. Google Earth-Based Grand Tours of the World's Ocean Basins and Marine Sediments

    NASA Astrophysics Data System (ADS)

    St John, K. K.; De Paor, D. G.; Suranovic, B.; Robinson, C.; Firth, J. V.; Rand, C.

    2016-12-01

    The GEODE project has produced a collection of Google Earth-based marine geology teaching resources that offer grand tours of the world's ocean basins and marine sediments. We use a map of oceanic crustal ages from Müller et al (2008; doi:10.1029/2007GC001743), and a set of emergent COLLADA models of IODP drill core data as a basis for a Google Earth tour introducing students to the world's ocean basins. Most students are familiar with basic seafloor spreading patterns but teaching experience suggests that few students have an appreciation of the number of abandoned ocean basins on Earth. Students also lack a valid visualization of the west Pacific where the oldest crust forms an isolated triangular patch and the ocean floor becomes younger towards the subduction zones. Our tour links geographic locations to mechanical models of rifting, seafloor spreading, subduction, and transform faulting. Google Earth's built-in earthquake and volcano data are related to ocean floor patterns. Marine sediments are explored in a Google Earth tour that draws on exemplary IODP core samples of a range of sediment types (e.g., turbidites, diatom ooze). Information and links are used to connect location to sediment type. This tour compliments a physical core kit of core catcher sections that can be employed for classroom instruction (geode.net/marine-core-kit/). At a larger scale, we use data from IMLGS to explore the distribution of the marine sediments types in the modern global ocean. More than 2,500 sites are plotted with access to original data. Students are guided to compare modern "type sections" of primary marine sediment lithologies, as well as examine site transects to address questions of bathymetric setting, ocean circulation, chemistry (e.g., CCD), and bioproductivity as influences on modern seafloor sedimentation. KMZ files, student exercises, and tips for instructors are available at geode.net/exploring-marine-sediments-using-google-earth.

  18. Selected ground-water information for the Pasco basin and adjacent areas, Washington, 1986-1989

    USGS Publications Warehouse

    Drost, B.W.; Schurr, K.M.; Lum, W. E.

    1989-01-01

    The U.S. Geological Survey, in cooperation with the United States Department of Energy, conducted a study of the Pasco basin and adjacent areas, Washington, in support of the Basalt Waste Isolation Project at the Hanford site, Washington. The purpose of the study was to develop a data set that would help define the groundwater-flow system of the Pasco Basin. This report contains the basic data, without interpretation, that were collected from the start of the project in February 1986 through January 1989. Information presented is from the U.S. Bureau of Reclamation, State of Washington Department of Ecology , US Army Corps of Engineers, Kennewick Irrigation District, and the Survey, and consists of well location and construction data, records of water levels in the wells, and aquifer designations for each well. The aquifer designation represents the geohydrologic unit to which the well is reported to be open. (USGS)

  19. Downscaling ocean conditions with application to the Gulf of Maine, Scotian Shelf and adjacent deep ocean

    NASA Astrophysics Data System (ADS)

    Katavouta, Anna; Thompson, Keith R.

    2016-08-01

    The overall goal is to downscale ocean conditions predicted by an existing global prediction system and evaluate the results using observations from the Gulf of Maine, Scotian Shelf and adjacent deep ocean. The first step is to develop a one-way nested regional model and evaluate its predictions using observations from multiple sources including satellite-borne sensors of surface temperature and sea level, CTDs, Argo floats and moored current meters. It is shown that the regional model predicts more realistic fields than the global system on the shelf because it has higher resolution and includes tides that are absent from the global system. However, in deep water the regional model misplaces deep ocean eddies and meanders associated with the Gulf Stream. This is not because the regional model's dynamics are flawed but rather is the result of internally generated variability in deep water that leads to decoupling of the regional model from the global system. To overcome this problem, the next step is to spectrally nudge the regional model to the large scales (length scales > 90 km) of the global system. It is shown this leads to more realistic predictions off the shelf. Wavenumber spectra show that even though spectral nudging constrains the large scales, it does not suppress the variability on small scales; on the contrary, it favours the formation of eddies with length scales below the cutoff wavelength of the spectral nudging.

  20. Lunar Magma Ocean Bedrock Anorthosites Detected at Orientale Basin by M3

    NASA Astrophysics Data System (ADS)

    Pieters, C. M.; Boardman, J. W.; Burratti, B.; Cheek, L.; Clark, R. N.; Combe, J.; Green, R. O.; Head, J. W.; Hicks, M.; Isaacson, P.; Klima, R.; Kramer, G. Y.; Lundeen, S.; Malaret, E.; McCord, T. B.; Mustard, J. F.; Nettles, J. W.; Petro, N. E.; Runyon, C. J.; Staid, M.; Sunshine, J. M.; Taylor, L. A.; Tompkins, S.; Varanasi, P.

    2009-12-01

    The lunar crust is thought to have formed as a result of global melting of the outer parts of the Moon in its earliest history, a lunar magma ocean (LMO). Crystallization of this magma ocean set the stage for the ensuing history of the planet. Models for the formation of the lunar crust and the evolution of the LMO were derived from individual Apollo samples that could not be placed directly in the context of crustal bedrock with remote sensing data that was available. Data from modern sensors, such as the Moon Mineralogy Mapper (M3) on Chandrayaan-1, now allow such bedrock issues to be addressed. The ~930 km diameter Orientale multi-ringed impact basin in the western highlands provides an opportunity to evaluate the mineralogy of the in situ crust of the Moon in the search for LMO mineralogy and structure. Orientale is the youngest large basin on the Moon, and the basin deposits and ring structures expose progressively deeper bedrock layering that can be used to determine lunar crustal structure and test the LMO model. With its high spatial and spectral resolution, M3 data show that the ejecta of the basin is composed of mixed assemblages of processed feldspathic breccias with small amounts of low-Ca pyroxene comprising the upper kilometers-thick mega-regolith layer of the crust. Exposures in the outermost (Cordillera) ring reveal less processed examples of this material. The M3 data show that the next interior ring (Outer Rook), representing deeper material, is characterized by distinctly more crystalline blocks of impact-shocked anorthosite and noritic anorthosite. Most importantly, M3 data reveal that the mountains of the closest ring toward the basin interior (Inner Rook) consist of pure anorthosite, including outcrops of the unshocked crystalline form. This massive exposure of anorthosite across the entire mountain range provides validation for the LMO hypothesis. These mountains are believed to have originated in the upper crust below the impact fragmented

  1. A tale of two basins: An integrated physical and biological perspective of the deep Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Bluhm, B. A.; Kosobokova, K. N.; Carmack, E. C.

    2015-12-01

    domains have vertical stratification that constrains the transfer of nutrients to the surface layer (euphotic zone), thus leading to their oligotrophic state, particularly in the more strongly stratified Pacific Arctic where, despite high nutrient values in the inflow, convective reset of surface layer nutrients by haline convection in winter is virtually absent. First and multi-year sea ice drastically alters albedo and insulates the underlying water column from extreme winter heat loss while its mechanical properties (thickness, concentration, roughness, etc.) greatly affect the efficiency of momentum transfer from the wind to the underlying water. Biologically, sea ice algal growth in the basins is proportionally almost equal to or exceeding phytoplankton production, and is a habitat and transport platform for sympagic (ice-associated) fauna. Owing to nutrient limitation due to strong stratification and light limitation due to snow and ice cover and extreme sun angle, primary production in the two basin domains is very low compared to the adjacent shelves. Severe nutrient limitation and complete euphotic zone drawdown in the AB favors small phytoplankton, a ubiquitous deep chlorophyll maximum layer, a low f-ratio of new to recycled carbon fixation, and a low energy food web. In contrast, nutrients persist -albeit in low levels- in the western EB, even in summer, suggesting light limitation, heavy grazing or both. The higher stocks of nutrients in the EB are more conducive to marginal ice blooms than in the AB. The large-scale ocean currents (NHTC and ACBC) import substantial expatriate, not locally reproducing zooplankton biomass especially from the adjoining subarctic Atlantic (primarily Calanus finmarchicus), but also from the Pacific (e.g., Pseudocalanus spp., Neocalanus spp. and Metridia pacifica). These advective inputs serve both as source of food to resident pelagic and benthic biota within the basins, and as potential grazers exerting top down control on

  2. Upper-Ocean Variability in the Arctic’s Amundsen and Nansen Basins

    DTIC Science & Technology

    2017-05-01

    collect vertical profiles of ocean temperature, salinity and horizontal velocity at few- hour interval as well as sample for specified time periods...deployed for the MIZ program - specifically, vertical temperature, salinity and velocity profiles were collected every 3 hours in the upper 250m of the...the system), this ITP-V returned 5+ months of upper ocean temperature, salinity , velocity and turbulence data from the Makarov Basin, a region of

  3. Low frequency baleen whale calls detected on ocean-bottom seismometers in the Lau basin, southwest Pacific Ocean.

    PubMed

    Brodie, Dana C; Dunn, Robert A

    2015-01-01

    Ten months of broadband seismic data, recorded on six ocean-bottom seismographs located in the Lau Basin, were examined to identify baleen whale species. As the first systematic survey of baleen whales in this part of the southwest Pacific Ocean, this study reveals the variety of species present and their temporal occurrence in and near the basin. Baleen whales produce species-specific low frequency calls that can be identified by distinct patterns in data spectrograms. By matching spectrograms with published accounts, fin, Bryde's, Antarctic blue, and New Zealand blue whale calls were identified. Probable whale sounds that could not be matched to published spectrograms, as well as non-biologic sounds that are likely of volcanogenic origin, were also recorded. Detections of fin whale calls (mid-June to mid-October) and blue whale calls (June through September) suggest that these species migrate through the region seasonally. Detections of Bryde's whale calls (primarily February to June, but also other times of the year) suggest this species resides around the basin nearly year round. The discovery of previously unpublished call types emphasizes the limited knowledge of the full call repertoires of baleen whales and the utility of using seismic survey data to enhance understanding in understudied regions.

  4. Cyclonic eddies identified in the Cape Basin of the South Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Hall, C.; Lutjeharms, J. R. E.

    2011-03-01

    Inter-ocean exchange south of Africa takes place largely through the movement of Agulhas Rings into the Cape Basin. Recent observations have shown that the highly energetic flow field in this basin consists of anti-cyclonic rings as well as cyclonic eddies. Very little is known of the characteristics of the cyclonic eddies. Using altimetric data, this study determines the location, frequency and seasonality of these cyclonic eddies their size, trajectories, life spans and their association with Agulhas Rings. Cyclonic eddies were seen to split, merge and link with other cyclonic eddies, where splitting events created child cyclonic eddies. The 105 parent and 157 child cyclonic eddies identified over a decade show that on average 11 parent and 17 child cyclonic eddies appear annually in AVISO merged absolute dynamic topography data along the continental slope. Thirty-two percent follow an overall west south-westward direction, with 27% going west north-westward. Average translocation speeds are 2.2 ± 0.1 km/day for parent and 3.0 ± 0.2 km/day for child cyclonic eddies. Parent cyclonic eddy lifespan averaged 250 ± 18 days; whereas child cyclonic eddies survived for only 118 ± 11 days. A significant difference in lifespan for parent and child cyclonic eddies identified in the north and south region of the study area was detected. Seventy-seven percent of the northern and 93% of the southern cyclonic eddies were first detected directly adjacent to passing Agulhas Rings, suggesting a vital interaction between these mesoscale eddies within the region. Topographical features appeared to affect the behaviour and lifespan of these deep cyclonic eddies.

  5. Differential heating in the Indian Ocean differentially modulates precipitation in the Ganges and Brahmaputra basins

    USGS Publications Warehouse

    Pervez, Md Shahriar; Henebry, Geoffrey M.

    2016-01-01

    Indo-Pacific sea surface temperature dynamics play a prominent role in Asian summer monsoon variability. Two interactive climate modes of the Indo-Pacific—the El Niño/Southern Oscillation (ENSO) and the Indian Ocean dipole mode—modulate the amount of precipitation over India, in addition to precipitation over Africa, Indonesia, and Australia. However, this modulation is not spatially uniform. The precipitation in southern India is strongly forced by the Indian Ocean dipole mode and ENSO. In contrast, across northern India, encompassing the Ganges and Brahmaputra basins, the climate mode influence on precipitation is much less. Understanding the forcing of precipitation in these river basins is vital for food security and ecosystem services for over half a billion people. Using 28 years of remote sensing observations, we demonstrate that (i) the tropical west-east differential heating in the Indian Ocean influences the Ganges precipitation and (ii) the north-south differential heating in the Indian Ocean influences the Brahmaputra precipitation. The El Niño phase induces warming in the warm pool of the Indian Ocean and exerts more influence on Ganges precipitation than Brahmaputra precipitation. The analyses indicate that both the magnitude and position of the sea surface temperature anomalies in the Indian Ocean are important drivers for precipitation dynamics that can be effectively summarized using two new indices, one tuned for each basin. These new indices have the potential to aid forecasting of drought and flooding, to contextualize land cover and land use change, and to assess the regional impacts of climate change.

  6. Leveraging Somali Basin Magnetic Anomalies to Constrain Gondwana Breakup and Early Indian Ocean Formation

    NASA Astrophysics Data System (ADS)

    Davis, J. K.; Lawver, L. A.; Norton, I. O.; Gahagan, L.

    2015-12-01

    The Somali Basin, found between the Horn of Africa and Madagascar was formed during the rifting of East and West Gondwana. Understanding the evolution of the basin has historically been hindered by enigmatic seafloor fabric and an apparent paucity of magnetic anomaly data. Recent iterations of satellite gravity data have revealed nearly complete fracture zones as well as a distinct extinct spreading ridge within the basin. Through a thorough compilation of available Somali Basin shiptrack profiles, we have been able to successfully model and interpret magnetic anomalies with exceptional detail. This complication is unrivaled in completeness and provides unprecedented insight into basin formation. Using this high quality data, we have interpreted magnetic anomalies M0r (120.8 Ma) to M24Bn (152.43 Ma) about the extinct ridge. The interpreted Somali Basin spreading rate and spreading direction, through anomaly M15n (135.76 Ma), are similar to those observed in the neighboring coeval Mozambique Basin. This similarity suggests that East Gondwana separated from West Gondwana as a cohesive unit, and that the internal rifting of East Gondwana began later around 135 Ma. Our magnetic anomaly interpretations have been combined with additional magnetic interpretations from around the Indian Ocean to build a regionally consistent plate model of Gondwana breakup and early Indian Ocean formation. This plate model will be crucial for future efforts unraveling a precise history of East Gondwana fragmentation and constraining the formation of the Enderby Basin offshore East Antarctica and Bay of Bengal offshore East India.

  7. Weekly Cycle of Lightning and Associated Patterns of Rainfall, Cloud, and Aerosols over Korea and Adjacent Oceans during Boreal Summer

    NASA Technical Reports Server (NTRS)

    Kim, Ji-In; Kim, Kyu-Myong

    2011-01-01

    In this study, we analyze the weekly cycle of lightning over Korea and adjacent oceans and associated variations of aerosols, clouds, precipitation, and atmospheric circulations, using aerosol optical depth (AOD) from the NASA Moderate resolution Imaging Spectroradiometer (MODIS) and Multi-angle Imaging SpectroRadiometer (MISR), cloud properties from MODIS, precipitation and storm height from Tropical Rainfall Measuring Mission (TRMM) satellite, and lightning data from the Korean Lightning Detection Network (KLDN) during 9-year from 2002 to 2010. Lightning data was divided into three approximately equal areas, land area of Korea, and two adjacent oceans, Yellow Sea and South Sea. Preliminary results show that the number of lightning increases during the middle of the week over Yellow Sea. AOD data also shows moderately significant midweek increase at about the same time as lightning peaks. These results are consistent with the recent studies showing the invigoration of storms with more ice hydrometeors by aerosols, and subsequently wash out of aerosols by rainfall. Frequency of lightning strokes tend to peak at weekend in land area and over South Sea, indicating local weekly anomalous circulation between land and adjacent ocean. On the other hand, lightning frequency over Yellow Sea appears to have very strong weekly cycle with midweek peak on around Wednesday. It is speculated that the midweek peak of lightning over Yellow Sea was related with aerosol transport from adjacent land area. AOD data also suggests midweek peak over Yellow Sea, however, the weekly cycle of AOD was not statistically significant. Changes in weekly cycle of lightning from pre-monsoon to monsoon season, as well as associated clouds and circulation patterns are also discussed.

  8. Greater role for Atlantic inflows on sea-ice loss in the Eurasian Basin of the Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Polyakov, Igor V.; Pnyushkov, Andrey V.; Alkire, Matthew B.; Ashik, Igor M.; Baumann, Till M.; Carmack, Eddy C.; Goszczko, Ilona; Guthrie, John; Ivanov, Vladimir V.; Kanzow, Torsten; Krishfield, Richard; Kwok, Ronald; Sundfjord, Arild; Morison, James; Rember, Robert; Yulin, Alexander

    2017-04-01

    Arctic sea-ice loss is a leading indicator of climate change and can be attributed, in large part, to atmospheric forcing. Here, we show that recent ice reductions, weakening of the halocline, and shoaling of the intermediate-depth Atlantic Water layer in the eastern Eurasian Basin have increased winter ventilation in the ocean interior, making this region structurally similar to that of the western Eurasian Basin. The associated enhanced release of oceanic heat has reduced winter sea-ice formation at a rate now comparable to losses from atmospheric thermodynamic forcing, thus explaining the recent reduction in sea-ice cover in the eastern Eurasian Basin. This encroaching “atlantification” of the Eurasian Basin represents an essential step toward a new Arctic climate state, with a substantially greater role for Atlantic inflows.

  9. Glimpses of Arctic Ocean shelf-basin interaction from submarine-borne radium sampling

    NASA Astrophysics Data System (ADS)

    Kadko, David; Aagaard, Knut

    2009-01-01

    Evidence of shelf-water transfer from temperature, salinity, and 228Ra/ 226Ra sampling from the nuclear submarine USS L. Mendel Rivers SCICEX cruise in October, 2000 demonstrates the heterogeneity of the Arctic Ocean with respect to halocline ventilation. This likely reflects both time-dependent events on the shelves and the variety of dispersal mechanisms within the ocean, including boundary currents and eddies, at least one of which was sampled in this work. Halocline waters at the 132 m sampling depth in the interior Eurasian Basin are generally not well connected to the shelves, consonant with their ventilation within the deep basins, rather than on the shelves. In the western Arctic, steep gradients in 228Ra/ 226Ra ratio and age since shelf contact are consistent with very slow exchange between the Chukchi shelf and the interior Beaufort Gyre. These are the first radium measurements from a nuclear submarine.

  10. Non-basin Mare Provinces on the Moon: The Roles of Primordial Rifting and Adjacent Basin Loading at Mare Frigoris and Mare Tranquillitatis.

    NASA Astrophysics Data System (ADS)

    McGovern, P. J., Jr.; Kramer, G. Y.; Neumann, G. A.

    2017-12-01

    In the last decade, new missions to the Moon have returned a flood of new high-resolution imaging, spectroscopy, topography, and gravity data that have triggered major advances in our knowledge of that body's origin, structure, and evolution. One major development is the identification of several large mare provinces (basalt-covered plains) that lack a clear association with the interiors of large impact basins. These include the broad but narrow Mare Frigoris (MF) north of the Imbrium and Serentiatis basins, and Mare Tranquillitatis (MT), which occupies the center of a triangular region delineated by the Crisium, Serenitatis, and Nectaris basins ("CSN Triangle"). MF and the western margin of MT coincide with the proposed volcano-tectonic (rift) boundary structures of the Procellarum region detected in the GRAIL gravity data, but a search for gravitational signals of basins revealed evidence for only one small basin in western MT and none in the remainder of MT or MF. These observations clearly show that the standard paradigm for creating maria, with basaltic melt ascending from an anomalously warm (and presumably impact-heated) mantle region beneath an impact basin to fill the basin, is insufficient to explain the Frigoris and Tranquillitatis mare units (and corresponding intrusives below). Alternative scenarios for mare unit emplacement include 1) volcanism generated from ancient Procellarum-bounding rift (PBR) structures, and 2) stress-enhanced magma ascent potential from central mare unit lithospheric loading in adjacent basins. The PBR scenario can in principle explain the emplacement of MF, but the concentric nature of the geometry of western and central MF with respect to Imbrium and eastern MF with respect to Serenitatis is then rendered coincidental. Some element of outer ring structure inheritance from these basins is suggested by the geometric relationships. The PBR scenario is also relevant to the western margin of Mare Tranquillitatis, where a strong

  11. A model of ocean basin crustal magnetization appropriate for satellite elevation anomalies

    NASA Technical Reports Server (NTRS)

    Thomas, Herman H.

    1987-01-01

    A model of ocean basin crustal magnetization measured at satellite altitudes is developed which will serve both as background to which anomalous magnetizations can be contrasted and as a beginning point for studies of tectonic modification of normal ocean crust. The model is based on published data concerned with the petrology and magnetization of the ocean crust and consists of viscous magnetization and induced magnetization estimated for individual crustal layers. Thermal remanent magnetization and chemical remanent magnetization are excluded from the model because seafloor spreading anomalies are too short in wavelength to be resolved at satellite altitudes. The exception to this generalization is found at the oceanic magnetic quiet zones where thermal remanent magnetization and chemical remanent magnetization must be considered along with viscous magnetization and induced magnetization.

  12. Distribution of oil and natural-gas wells in relation to ground-water flow systems in the Great Basin region of Nevada and Utah, and adjacent states

    USGS Publications Warehouse

    Schaefer, Donald H.

    1996-01-01

    This map publication is one of several in a series concerning various aspects of the ground-water hydrology of the Great Basin in Nevada, Utah, and adjacent States.  One report in the series describes the hydrogeologic framework of the Great Basin (Plume and Carlton, 1988).  Another shows the ground-water levels for the aquifer systems of the Great Basin (Thomas and others, 1986).  A third report in the series describes the regional ground-water flow patterns in the Great Basin (Harrill and others, 1988).

  13. Detection of baleen whales on an ocean-bottom seismometer array in the Lau Basin

    NASA Astrophysics Data System (ADS)

    Brodie, D.; Dunn, R.

    2011-12-01

    Long-term deployment of ocean-bottom seismometer arrays provides a unique opportunity for identifying and tracking whales in a manner not usually possible in biological studies. Large baleen whales emit low frequency (>5Hz) sounds called 'calls' or 'songs' that can be detected on either the hydrophone or vertical channel of the instrument at distances in excess of 50 km. The calls are distinct to individual species and even geographical groups among species, and are thought to serve a variety of purposes. Distinct repeating calls can be automatically identified using matched-filter processing, and whales can be located in a manner similar to that of earthquakes. Many baleen whale species are endangered, and little is known about their geographic distribution, population dynamics, and basic behaviors. The Lau back-arc basin, a tectonically active, elongated basin bounded by volcanic shallows, lies in the southwestern Pacific Ocean between Fiji and Tonga. Although whales are known to exist around Fiji and Tonga, little is understood about the population dynamics and migration patterns throughout the basin. Twenty-nine broadband ocean-bottom seismometers deployed in the basin recorded data for approximately ten months during the years 2009-2010. To date, four species of whales have been identified in the data: Blue (one call type), Humpback (two call types, including long-lasting 'songs'), Bryde's (one call type), and Fin whales (three call types). Three as-yet-unknown call types have also been identified. After the calls were identified, idealized spectrograms of the known calls were matched against the entire data set using an auto-detection algorithm. The auto-detection output provides the number of calls and times of year when each call type was recorded. Based on the results, whales migrate seasonally through the basin with some overlapping of species. Initial results also indicate that different species of whales are more common in some parts of the basin than

  14. Seismic structure of western Mediterranean back-arc basins and rifted margins - constraints from the Algerian-Balearic and Tyrrhenian Basins

    NASA Astrophysics Data System (ADS)

    Grevemeyer, Ingo; Ranero, Cesar; Sallares, Valenti; Prada, Manel; Booth-Rea, Guillermo; Gallart, Josep; Zitellini, Nevio

    2017-04-01

    The Western Mediterranean Sea is a natural laboratory to study the processes of continental extension, rifting and back-arc spreading in a convergent setting caused by rollback of fragmented subducting oceanic slabs during the latest phase of consumption of the Tethys ocean, leading to rapid extension in areas characterized by a constant convergence of the African and European Plates since Cretaceous time. Opening of the Algerian-Balearic Basin was governed by a southward and westward retreating slab 21 to 18 Myr and 18 to15 Myr ago, respectively. Opening of the Tyrrhenian Basin was controlled by the retreating Calabrian slab 6 to 2 Myr ago. Yet, little is known about the structure of the rifted margins, back-arc extension and spreading. Here we present results from three onshore/offshore seismic refraction and wide-angle lines and two offshore lines sampling passive continental margins of southeastern Spain and to the south of the Balearic promontory and the structure of the Tyrrhenian Basin to the north of Sicily. Seismic refraction and wide-angle data were acquired in the Algerian-Balearc Basin during a cruise of the German research vessel Meteor in September of 2006 and in the Tyrrhenian Sea aboard the Spanish research vessel Sarmiento de Gamboa in July of 2015. All profiles sampled both continental crust of the margins surrounding the basins and extend roughly 100 km into the Algerian-Balearic and the Tyrrhenian Basins, yielding constraints on the nature of the crust covering the seafloor in the basins and adjacent margins. Crust in the Algerian-Balearic basin is roughly 5-6 km thick and the seismic velocity structure mimics normal oceanic crust with the exception that lower crustal velocity is <6.8 km/s, clearly slower than lower crust sampled in the Pacific Basin. The seismic Moho in the Algerian-Balearic Basin occurs at 11 km below sea level, reaching >24 km under SE Spain and the Balearic Islands, displaying typical features and structure of continental

  15. Hydrogeochemical studies of historical mining areas in the Humboldt River basin and adjacent areas, northern Nevada

    USGS Publications Warehouse

    Nash, J. Thomas

    2005-01-01

    The study area comprises the Humboldt River Basin and adjacent areas, with emphasis on mining areas relatively close to the Humboldt River. The basin comprises about 16,840 mi2 or 10,800,000 acres. The mineral resources of the Humboldt Basin have been investigated by many scientists over the past 100 years, but only recently has our knowledge of regional geology and mine geology been applied to the understanding and evaluation of mining effects on water and environmental quality. The investigations reported here apply some of the techniques and perspectives developed in the Abandoned Mine Lands Initiative (AMLI) of the U.S. Geological Survey (USGS), a program of integrated geological-hydrological-biological-chemical studies underway in the Upper Animas River watershed in Colorado and the Boulder River watershed in, Montana. The goal of my studies of sites and districts is to determine the character of mining-related contamination that is actively or potentially a threat to water quality and to estimate the potential for natural attenuation of that contamination. These geology-based studies and recommendations differ in matters of emphasis and data collection from the biology-based assessments that are the cornerstone of environmental regulations.

  16. Neogene-quaternary Ostracoda and paleoenvironments, of the Limón basin, Costa Rica, and Bocas del Toro basin, Panama

    USGS Publications Warehouse

    Borne, P.F.; Cronin, T. M.; Hazel, J.E.

    1999-01-01

    Tropical marine ostracodes from Neogene and Quaternary sediments of the Central American Caribbean region have been the subject of biostratigraphic, ecological, taxonomic, and evolutionary studies. As part of the Panama Paleontology Project (PPP), Neogene and Quaternary ostracodes are being studied from the Central American region. The overall goal of this research is to evaluate the impact of the emergence of the Central American Isthmus as a land barrier between the Caribbean/tropical Atlantic and the Pacific oceans on marine ostracode biodiversity and the oceanic environments in which extant ostracodes evolved. Due to the ecological specificity of many living tropical ostracode species, they are ideally suited for reconstructing paleoenvironments on the basis of their occurrence in fossil assemblages, which in turn can lead to a better understanding of the tropical climatic and tectonic history of Central America. The principal aims of this chapter are: (a) to document the composition of the ostracode assemblages from the Limón Basin of Costa Rica and the Bocas del Toro Basin of Panama, two areas yielding extensive ma rine ostracode assemblages; (b) to describe the environments of deposition within these basins; and (c) to document the stratigraphic distribution of potentially agediagnostic ostracode species in the Limón and Bocas del Toro basins in order to enhance their use in Central American biostratigraphy. A secondary, but none-the-less important goal is to assemble a database on the distribution of modem ostracode species in the Caribbean and adjacent areas as a basis for comparison with fossil assemblages. Although the ecological, biostratigraphic and paleoenvironmental conclusions presented here will improve as additional material is studied, these fossil and modem ostracode databases constitute the foundation for future evolutionary and geochernical studies of tropical Caribbean and eastern Pacific Ocean ostracodes. Moreover, we present here evidence

  17. Structures within the oceanic crust of the central South China Sea basin and their implications for oceanic accretionary processes

    NASA Astrophysics Data System (ADS)

    Ding, Weiwei; Sun, Zhen; Dadd, Kelsie; Fang, Yinxia; Li, Jiabiao

    2018-04-01

    Internal structures in mature oceanic crust can elucidate understanding of the processes and mechanism of crustal accretion. In this study, we present two multi-channel seismic (MCS) transects across the northern flank of the South China Sea basin to reveal the internal structures related to Cenozoic tectono-magmatic processes during seafloor spreading. Bright reflectors within the oceanic crust, including the Moho, upper crustal reflectors, and lower crustal reflectors, are clearly imaged in these two transects. The Moho reflection displays varied character in continuity, shape and amplitude from the continental slope area to the abyssal basin, and becomes absent in the central part of the basin where abundant seamounts and seamount chains formed after the cessation of seafloor spreading. Dipping reflectors are distinct in most parts of the MCS data but generally confined to the lower crust above the Moho reflection. These lower crustal reflectors merge downward into the Moho without offsetting it, probably arising from shear zones between the crust and mantle characterized by interstitial melt, although we cannot exclude other possibilities such as brittle faulting or magmatic layering in the local area. A notable feature of these lower crustal reflector events is their opposite inclinations. We suggest the two groups of conjugate lower crustal reflector events observed between magnetic anomalies C11 and C8 were associated with two unusual accretionary processes arising from plate reorganizations with southward ridge jumps.

  18. Glacial lake drainage in Patagonia (13-8 kyr) and response of the adjacent Pacific Ocean

    PubMed Central

    Glasser, Neil F.; Jansson, Krister N.; Duller, Geoffrey A. T.; Singarayer, Joy; Holloway, Max; Harrison, Stephan

    2016-01-01

    Large freshwater lakes formed in North America and Europe during deglaciation following the Last Glacial Maximum. Rapid drainage of these lakes into the Oceans resulted in abrupt perturbations in climate, including the Younger Dryas and 8.2 kyr cooling events. In the mid-latitudes of the Southern Hemisphere major glacial lakes also formed and drained during deglaciation but little is known about the magnitude, organization and timing of these drainage events and their effect on regional climate. We use 16 new single-grain optically stimulated luminescence (OSL) dates to define three stages of rapid glacial lake drainage in the Lago General Carrera/Lago Buenos Aires and Lago Cohrane/Pueyrredón basins of Patagonia and provide the first assessment of the effects of lake drainage on the Pacific Ocean. Lake drainage occurred between 13 and 8 kyr ago and was initially gradual eastward into the Atlantic, then subsequently reorganized westward into the Pacific as new drainage routes opened up during Patagonian Ice Sheet deglaciation. Coupled ocean-atmosphere model experiments using HadCM3 with an imposed freshwater surface “hosing” to simulate glacial lake drainage suggest that a negative salinity anomaly was advected south around Cape Horn, resulting in brief but significant impacts on coastal ocean vertical mixing and regional climate. PMID:26869235

  19. A new interpretation of deformation rates in the Snake River Plain and adjacent basin and range regions based on GPS measurements

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

    S.J. Payne; R. McCaffrey; R.W. King

    2012-04-01

    We evaluate horizontal Global Positioning System (GPS) velocities together with geologic, volcanic, and seismic data to interpret extension, shear, and contraction within the Snake River Plain and the Northern Basin and Range Province, U.S.A. We estimate horizontal surface velocities using GPS data collected at 385 sites from 1994 to 2009 and present an updated velocity field within the Stable North American Reference Frame (SNARF). Our results show an ENE-oriented extensional strain rate of 5.9 {+-} 0.7 x 10{sup -9} yr{sup -1} in the Centennial Tectonic belt and an E-oriented extensional strain rate of 6.2 {+-} 0.3 x 10{sup -9} yr{supmore » -1} in the Intermountain Seismic belt combined with the northern Great Basin. These extensional strain rates contrast with the regional north-south contraction of -2.6 {+-} 1.1 x 10{sup -9} yr{sup -1} calculated in the Snake River Plain and Owyhee-Oregon Plateau over a 125 x 650 km region. Tests that include dike-opening reveal that rapid extension by dike intrusion in volcanic rift zones does not occur in the Snake River Plain at present. This slow internal deformation in the Snake River Plain is in contrast to the rapidly-extending adjacent Basin and Range provinces and implies shear along boundaries of the Snake River Plain. We estimate right-lateral shear with slip rates of 0.5-1.5 mm/yr along the northwestern boundary adjacent to the Centennial Tectonic belt and left-lateral oblique extension with slip rates of <0.5 to 1.7 mm/yr along the southeastern boundary adjacent to the Intermountain Seismic belt. The fastest lateral shearing occurs near the Yellowstone Plateau where strike-slip focal mechanisms and faults with observed strike-slip components of motion are documented. The regional GPS velocity gradients are best fit by nearby poles of rotation for the Centennial Tectonic belt, Idaho batholith, Snake River Plain, Owyhee-Oregon Plateau, and central Oregon, indicating that clockwise rotation is driven by extension to

  20. A deliberate tracer experiment in Santa Monica Basin. [for ocean density strata diffusion

    NASA Technical Reports Server (NTRS)

    Ledwell, J. R.; Broecker, W. S.; Watson, A. J.

    1986-01-01

    A tracer technique was developed for measurements of diffusion across oceanic density strata using SF6 and perfluorodecalin (PFD) tracers in the Santa Monica Basin. Fifty days after injection, the tracers were found to have mixed along the isopycnal surface to nearly every part of the basin. The diapycnal spreading of the tracer distributions yielded an apparent eddy diffusivity of 0.33 + or - 0.08 sq cm/s at the ambient density gradient of 4.0 + or - 0.5 x 10 to the -9th g/cm to the 4th.

  1. Fate of copper complexes in hydrothermally altered deep-sea sediments from the Central Indian Ocean Basin.

    PubMed

    Chakraborty, Parthasarathi; Sander, Sylvia G; Jayachandran, Saranya; Nath, B Nagender; Nagaraju, G; Chennuri, Kartheek; Vudamala, Krushna; Lathika, N; Mascarenhas-Pereira, Maria Brenda L

    2014-11-01

    The current study aims to understand the speciation and fate of Cu complexes in hydrothermally altered sediments from the Central Indian Ocean Basin and assess the probable impacts of deep-sea mining on speciation of Cu complexes and assess the Cu flux from this sediment to the water column in this area. This study suggests that most of the Cu was strongly associated with different binding sites in Fe-oxide phases of the hydrothermally altered sediments with stabilities higher than that of Cu-EDTA complexes. The speciation of Cu indicates that hydrothermally influenced deep-sea sediments from Central Indian Ocean Basin may not significantly contribute to the global Cu flux. However, increasing lability of Cu-sediment complexes with increasing depth of sediment may increase bioavailability and Cu flux to the global ocean during deep-sea mining. Copyright © 2014 Elsevier Ltd. All rights reserved.

  2. Three types of Indian Ocean Basin modes

    NASA Astrophysics Data System (ADS)

    Guo, Feiyan; Liu, Qinyu; Yang, Jianling; Fan, Lei

    2017-04-01

    The persistence of the Indian Ocean Basin Mode (IOBM) from March to August is important for the prediction of Asian summer monsoon. Based on the observational data and the pre-industrial control run outputs of the Community Climate System Model, version 4 (CCSM4), the IOBM is categorized into three types: the first type can persist until August; the second type transforms from the positive (negative) IOBM into the negative (positive) Indian Ocean Dipole Mode (IODM), accompanied by the El Niño-to-La Niña (La Niña-to-El Niño) transition in the boreal summer; the third type transforms from the positive (negative) IOBM into the positive (negative) IODM in early summer. It is discovered that aside from the influence of anomalous Walker Circulation resulted from the phase transition of ENSO, the persistence of Australia high anomaly (AHA) over the southeastern tropical Indian Ocean (TIO) and the west of Australia from March to May is favorable for the positive (negative) IOBM transformation into the positive (negative) IODM in the boreal summer. The stronger equatorially asymmetric sea surface temperature anomalies (SSTAs) in the boreal spring are the main mechanism for the persistence of IOBM, because the asymmetric atmospheric responses to the stronger equatorially asymmetric SSTAs in the TIO confine the AHA to the east of Australia from May to August. This result indicates a possibility of predicting summer atmospheric circulation based on the equatorial symmetry of SSTAs in the TIO in spring.

  3. Early Carboniferous adakite-like and I-type granites in central Qiangtang, northern Tibet: Implications for intra-oceanic subduction and back-arc basin formation within the Paleo-Tethys Ocean

    NASA Astrophysics Data System (ADS)

    Liu, Jin-Heng; Xie, Chao-Ming; Li, Cai; Wang, Ming; Wu, Hao; Li, Xing-Kui; Liu, Yi-Ming; Zhang, Tian-Yu

    2018-01-01

    Recent studies have proposed that the Late Devonian ophiolites in the central Qiangtang region of northern Tibet were formed in an oceanic back-arc basin setting, which has led to controversy over the subduction setting of the Longmucuo-Shuanghu-Lancangjiang Suture Zone (LSLSZ) during the Late Devonian to Early Carboniferous. In this paper we present new data about a suite of granite plutons that intrude into ophiolite in central Qiangtang. Our aim was to identify the type of subduction and to clarify the existence of an intra-oceanic back-arc basin in the LSLSZ during the Late Devonian to Early Carboniferous. The suite of granites consists of monzogranites, syenogranites, and granodiorites. Our laser ablation-inductively coupled plasma-mass spectrometry zircon U-Pb data yielded Early Carboniferous crystallization ages of 357.2 Ma, 357.4 Ma and 351.1 Ma. We subsequently investigated the petrogenesis and tectonic setting of these granites based on their geochemical and Hf isotopic characteristics. First, we divided the granites into high Sr/Y (HSG) and low Sr/Y granites (LSG). The HSG group contains monzogranites and granodiorites that have similar geochemical characteristics to adakites (i.e., high Sr/Y and La/Yb ratios, low MgO, Y, and Yb contents, and no pronounced negative Eu anomaly), although they have slightly lower Sr and Al2O3 contents, caused by crystal fractionation during late magmatic evolution. Therefore, we define the HSG group as adakite-like granites. The study of the HSG shows that they are adakite-like granites formed by partial melting of oceanic crust and experience fractional crystallization process during late evolution. However, some differences between the monzogranites and granodiorites indicate that there are varying degree contributions of subducted sediments during diagenesis. The LSG group contains syenogranites that have distinct negative correlations between their P2O5 and SiO2 contents, and Y and Th contents have significant positive

  4. Groundwater quality in the shallow aquifers of the Tulare, Kaweah, and Tule Groundwater Basins and adjacent highlands areas, Southern San Joaquin Valley, California

    USGS Publications Warehouse

    Fram, Miranda S.

    2017-01-18

    Groundwater provides more than 40 percent of California’s drinking water. To protect this vital resource, the State of California created the Groundwater Ambient Monitoring and Assessment (GAMA) Program. The Priority Basin Project of the GAMA Program provides a comprehensive assessment of the State’s groundwater quality and increases public access to groundwater-quality information. The shallow aquifers of the Tulare, Kaweah, and Tule groundwater basins and adjacent highlands areas of the southern San Joaquin Valley constitute one of the study units being evaluated.

  5. Ancient drainage basin of the Tharsis region, Mars: Potential source for outflow channel systems and putative oceans or paleolakes

    USGS Publications Warehouse

    Dohm, J.M.; Ferris, J.C.; Baker, V.R.; Anderson, R.C.; Hare, T.M.; Strom, R.G.; Barlow, N.G.; Tanaka, K.L.; Klemaszewski, J.E.; Scott, D.H.

    2001-01-01

    Paleotopographic reconstructions based on a synthesis of published geologic information and high-resolution topography, including topographic profiles, reveal the potential existence of an enormous drainage basin/aquifer system in the eastern part of the Tharsis region during the Noachian Period. Large topographic highs formed the margin of the gigantic drainage basin. Subsequently, lavas, sediments, and volatiles partly infilled the basin, resulting in an enormous and productive regional aquifer. The stacked sequences of water-bearing strata were then deformed locally and, in places, exposed by magmatic-driven uplifts, tectonic deformation, and erosion. This basin model provides a potential source of water necessary to carve the large outflow channel systems of the Tharsis and surrounding regions and to contribute to the formation of putative northern-plains ocean(s) and/or paleolakes. Copyright 2001 by the American Geophysical Union.

  6. Chukchi Borderland | Crustal Complex of the Amerasia Basin, Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Ilhan, I.; Coakley, B.; Houseknecht, D. W.

    2017-12-01

    In the Arctic Ocean, Chukchi Borderland separates the North Chukchi shelf and Toll deep basins to the west and Canada deep basin to the east. Existing plate reconstructions have attempted to restore this north-striking, fragments of the continental crust to all margins of the Amerasia Basin based on sparse geologic and geophysical measurements. Regional multi-channel seismic reflection and potential field geophysics, and geologic data indicate it is a high standing continental block, requiring special accommodation to create a restorable model of the formation of the Amerasia Basin. The Borderland is composed of the Chukchi Plateau, Northwind Basin, and Northwind Ridge divided by mostly north striking normal faults. These offset the basement and bound a sequence of syn-tectonic sediments. Equivalent strata are, locally, uplifted, deformed and eroded. Seaward dipping reflectors (SDRs) are observed in the juncture between the North Chukchi, Toll basins, and southern Chukchi Plateau underlying a regional angular unconformity. This reveals that this rifted margin was associated with volcanism. An inferred condensed section, which is believed to be Hauterivian-Aptian in age, synchronous with the composite pebble shale and gamma-ray zone of the Alaska North Slope forms the basal sediments in the North Chukchi Basin. Approximately 15 km of post-rift strata onlap the condensed section, SDRs and, in part, the wedge sequence on the Chukchi Plateau from west to east, thinning to the north. These post-Aptian sediments imply that the rifted margin subsided no later than the earliest Cretaceous, providing a plausible time constraint for the inferred pre-Cretaceous rifting in this region. The recognition of SDRs and Hauterivian—Aptian condensed section, and continuity of the Early—Late Cretaceous post-rift strata along the margins of the Borderland, strike variations of the normal faults, absence of observable deformation along the Northwind Escarpment substantially constrain

  7. Analyzing coastal turbidity under complex terrestrial loads characterized by a 'stress connectivity matrix' with an atmosphere-watershed-coastal ocean coupled model

    NASA Astrophysics Data System (ADS)

    Yamamoto, Takahiro; Nadaoka, Kazuo

    2018-04-01

    Atmospheric, watershed and coastal ocean models were integrated to provide a holistic analysis approach for coastal ocean simulation. The coupled model was applied to coastal ocean in the Philippines where terrestrial sediment loads provided from several adjacent watersheds play a major role in influencing coastal turbidity and are partly responsible for the coastal ecosystem degradation. The coupled model was validated using weather and hydrologic measurement to examine its potential applicability. The results revealed that the coastal water quality may be governed by the loads not only from the adjacent watershed but also from the distant watershed via coastal currents. This important feature of the multiple linkages can be quantitatively characterized by a "stress connectivity matrix", which indicates the complex underlying structure of environmental stresses in coastal ocean. The multiple stress connectivity concept shows the potential advantage of the integrated modelling approach for coastal ocean assessment, which may also serve for compensating the lack of measured data especially in tropical basins.

  8. Sulu-Celebes-Banda basins: a trapped piece of Cretaceous to Eocene oceanic crust

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

    McCabe, R.J.; Hilde, T.W.; Cole, J.T.

    1986-07-01

    The Sulu-Celebes-Banda basin is composed of three poorly understood marginal basins located between northwest Australia and southeast Asia. Recent studies have proposed that these three basins are remnants of once-continuous ocean basin. The on-land geology of this region is complicated. However, numerous stratigraphic and paleomagnetic studies on pre-Oligocene rocks are consistent with the interpretation that older landmasses presently dissecting the basin were translated into their present position during the middle to late Tertiary. Paleomagnetic data from the Philippines suggest that the Philippine arc is a composite of Early Cretaceous to Holocene arcs that were translated clockwise and from the southeast.more » Paleomagnetic and stratigraphic data from Kalimantan and Sulawesi suggest that these landmasses share a common origin and that Sulawesi was rifted eastward off of Borneo during the late Tertiary. Stratigraphic studies from the Sula microcontinent, Buru, Ceram, and Timor show close correlation to the stratigraphy of northwest Australia or New Guinea. In addition, paleomagnetic studies from Timor suggest that a portion of the island was part of Australia since the early Mesozoic.« less

  9. Arctic Ocean Sedimentary Cover Structure, Based on 2D MCS Seismic Data.

    NASA Astrophysics Data System (ADS)

    Kireev, A.; Kaminsky, V.; Poselov, V.; Poselova, L.; Kaminsky, D.

    2016-12-01

    In 2016 the Russian Federation has submitted its partial revised Submission for establishment of the OLCS (outer limit of the continental shelf) in the Arctic Ocean. In order to prepare the Submission, in 2005 - 2014 the Russian organizations carried out a wide range of geological and geophysical studies, so that today over 23000 km of MCS lines and 4000 km of deep seismic sounding are accomplished. For correct time/depth conversion of seismic sections obtained with a short streamer in difficult ice conditions wide-angle reflection/refraction seismic sonobuoy soundings were used. All of these seismic data were used to refine the stratigraphy model, to identify sedimentary complexes and to estimate the total thickness of the sedimentary cover. Seismic stratigraphy model was successively determined for the Cenozoic and pre-Cenozoic parts of the sedimentary section and was based on correlation of the Russian MCS data and seismic data documented by boreholes. Cenozoic part of the sedimentary cover is based on correlation of the Russian MCS data and AWI91090 section calibrated by ACEX-2004 boreholes on the Lomonosov Ridge for Amerasia basin and by correlation of onlap contacts onto oceanic crust with defined magnetic anomalies for Eurasia basin. Pre-Cenozoic part of the sedimentary cover is based on tracing major unconformities from boreholes on the Chukchi shelf (Crackerjack, Klondike, Popcorn) to the North-Chuckchi Trough and further to the Mendeleev Rise as well as to the Vilkitsky Trough and the adjacent Podvodnikov Basin. Six main unconformities were traced: regional unconformity (RU), Eocene unconformity (EoU) (for Eurasia basin only), post-Campanian unconformity (pCU), Brookian (BU - base of the Lower Brookian unit), Lower Cretaceous (LCU) and Jurassic (JU - top of the Upper Ellesmerian unit). The final step in our research was to generalize all seismic surveys (top of acoustic basement correlation data) and bathymetry data in the sedimentary cover thickness map

  10. 33 CFR 334.910 - Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif...

    Code of Federal Regulations, 2010 CFR

    2010-07-01

    ... Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. 334.910 Section 334.910... AND RESTRICTED AREA REGULATIONS § 334.910 Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. (a) The area. All of the waters of Camp Pendleton Boat...

  11. 33 CFR 334.910 - Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif...

    Code of Federal Regulations, 2012 CFR

    2012-07-01

    ... Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. 334.910 Section 334.910... AND RESTRICTED AREA REGULATIONS § 334.910 Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. (a) The area. All of the waters of Camp Pendleton Boat...

  12. 33 CFR 334.910 - Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif...

    Code of Federal Regulations, 2013 CFR

    2013-07-01

    ... Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. 334.910 Section 334.910... AND RESTRICTED AREA REGULATIONS § 334.910 Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. (a) The area. All of the waters of Camp Pendleton Boat...

  13. 33 CFR 334.910 - Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif...

    Code of Federal Regulations, 2011 CFR

    2011-07-01

    ... Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. 334.910 Section 334.910... AND RESTRICTED AREA REGULATIONS § 334.910 Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. (a) The area. All of the waters of Camp Pendleton Boat...

  14. 33 CFR 334.910 - Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif...

    Code of Federal Regulations, 2014 CFR

    2014-07-01

    ... Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. 334.910 Section 334.910... AND RESTRICTED AREA REGULATIONS § 334.910 Pacific Ocean, Camp Pendleton Boat Basin, U.S. Marine Corps Base, Camp Pendleton, Calif.; restricted area. (a) The area. All of the waters of Camp Pendleton Boat...

  15. Under-ice turbulent microstructure and upper ocean vertical fluxes in the Makarov and Eurasian basins, Arctic Ocean, during late spring and late summer / autumn in 2015

    NASA Astrophysics Data System (ADS)

    Rabe, Benjamin; Janout, Markus; Graupner, Rainer; Hoelemann, Jens; Hampe, Hendrik; Hoppmann, Mario; Horn, Myriel; Juhls, Bennet; Korhonen, Meri; Nikolopoulos, Anna; Pisarev, Sergey; Randelhoff, Achim; Savy, Jean-Philippe; Villacieros Robineau, Nicolas

    2017-04-01

    The Arctic Ocean is generally assumed to be fairly quiescent when compared to many other oceans. The sea-ice cover, a strong halocline and a shallow, cold mixed-layer prevents much of the ocean to be affected by atmospheric conditions and properties of the ocean mixed-layer. In turn, the mixed-layer and the sea-ice is largely isolated from the warm layer of Atlantic origin below by the lower halocline. Yet, the content of heat, freshwater and biologically important nutrients differs strongly between these different layers. Hence, it is crucial to be able to estimate vertical fluxes of salt, heat and nutrients to understand variability in the upper Arctic Ocean and the sea-ice, including the ecosystem. Yet, it is difficult to obtain direct flux measurements, and estimates are sparse. We present several sets of under-ice turbulent microstructure profiles in the Eurasian and Makarov Basin of the Arctic Ocean from two expeditions, in 2015. These cover melt during late spring north of Svalbard and freeze-up during late summer / autumn across the Eurasian and Makarov basins. Our results are presented against a background of the anomalously warm atmospheric conditions during summer 2015 followed by unusually low temperatures in September. 4 - 24 h averages of the measurements generally show elevated dissipation rates at the base of the mixed-layer. We found highest levels of dissipation near the Eurasian continental slope and smaller peaks in the profiles where Bering Sea Summer Water (sBSW) lead to additional stratification within the upper halocline in the Makarov Basin. The elevated levels of dissipation associated with sBSW and the base of the mixed-layer were associated with the relatively low levels of vertical eddy diffusivity. We discuss these findings in the light of the anomalous conditions in the upper ocean, sea-ice and the atmosphere during 2015 and present estimates of vertical fluxes of heat, salt and other dissolved substances measured in water samples.

  16. The North Slope of Alaska and Adjacent Arctic Ocean (NSA/AAO) cart site begins operation: Collaboration with SHEBA and FIRE

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

    Zak, D. B.; Church, H.; Ivey, M.

    2000-04-04

    Since the 1997 Atmospheric Radiation Measurement (ARM) Science Team Meeting, the North Slope of Alaska and Adjacent Arctic Ocean (NSA/AAO) Cloud and Radiation Testbed (CART) site has come into being. Much has happened even since the 1998 Science Team Meeting at which this paper was presented. To maximize its usefulness, this paper has been updated to include developments through July 1998.

  17. A zonally averaged, three-basin ocean circulation model for climate studies

    NASA Astrophysics Data System (ADS)

    Hovine, S.; Fichefet, T.

    1994-09-01

    A two-dimensional, three-basin ocean model suitable for long-term climate studies is developed. The model is based on the zonally averaged form of the primitive equations written in spherical coordinates. The east-west density difference which arises upon averaging the momentum equations is taken to be proportional to the meridional density gradient. Lateral exchanges of heat and salt between the basins are explicitly resolved. Moreover, the model includes bottom topography and has representations of the Arctic Ocean and of the Weddell and Ross seas. Under realistic restoring boundary conditions, the model reproduces the global conveyor belt: deep water is formed in the Atlantic between 60 and 70°N at a rate of about 17 Sv (1 Sv=106 m3 s-1) and in the vicinity of the Antarctic continent, while the Indian and Pacific basins show broad upwelling. Superimposed on this thermohaline circulation are vigorous wind-driven cells in the upper thermocline. The simulated temperature and salinity fields and the computed meridional heat transport compare reasonably well with the observational estimates. When mixed boundary conditions (i.e., a restoring condition on sea-surface temperature and flux condition on sea-surface salinity) are applied, the model exhibits an irregular behavior before reaching a steady state characterized by self-sustained oscillations of 8.5-y period. The conveyor-belt circulation always results at this stage. A series of perturbation experiments illustrates the ability of the model to reproduce different steady-state circulations under mixed boundary conditions. Finally, the model sensitivity to various factors is examined. This sensitivity study reveals that the bottom topography and the presence of a submarine meridional ridge in the zone of the Drake Passage play a crucial role in determining the properties of the model bottom-water masses. The importance of the seasonality of the surface forcing is also stressed.

  18. Insights into mantle heterogeneities: mid-ocean ridge basalt tapping an ocean island magma source in the North Fiji Basin

    NASA Astrophysics Data System (ADS)

    Brens, R., Jr.; Jenner, F. E.; Bullock, E. S.; Hauri, E. H.; Turner, S.; Rushmer, T. A.

    2015-12-01

    The North Fiji Basin (NFB), and connected Lau Basin, is located in a complex area of volcanism. The NFB is a back-arc basin (BAB) that is a result of an extinct subduction zone, incorporating the complicated geodynamics of two rotating landmasses: Fiji and the Vanuatu island arc. Collectively this makes the spreading centers of the NFB the highest producing spreading centers recorded. Here we present volatile concentrations, major, and trace element data for a previously undiscovered triple junction spreading center in the NFB. We show our enrichment samples contain some of the highest water contents yet reported from (MORB). The samples from the NFB exhibit a combination of MORB-like major chemical signatures along with high water content similar to ocean island basalts (OIB). This peculiarity in geochemistry is unlike other studied MORB or back-arc basin (to our knowledge) that is not attributed to subduction related signatures. Our results employ the use of volatiles (carbon dioxide and water) and their constraints (Nb and Ce) combined with trace element ratios to indicate a potential source for the enrichment in the North Fiji Basin. The North Fiji Basin lavas are tholeiitic with similar major element composition as averaged primitive normal MORB; with the exception of averaged K2O and P2O5, which are still within range for observed normal MORB. For a mid-ocean ridge basalt, the lavas in the NFB exhibit a large range in volatiles: H2O (0.16-0.9 wt%) and CO2 (80-359 ppm). The NFB lavas have volatile levels that exceed the range of MORB and trend toward a more enriched source. In addition, when compared to MORB, the NFB lavas are all enriched in H2O/Ce. La/Sm values in the NFB lavas range from 0.9 to 3.8 while, Gd/Yb values range from 1.2 to 2.5. The NFB lavas overlap the MORB range for both La/Sm (~1.1) and Gd/Yb (~1.3). However, they span a larger range outside of the MORB array. High La/Sm and Gd/Yb ratios (>1) are indications of deeper melting within the

  19. The deep structure of the Sichuan basin and adjacent orogenic zones revealed by the aggregated deep seismic profiling datum

    NASA Astrophysics Data System (ADS)

    Xiong, X.; Gao, R.; Li, Q.; Wang, H.

    2012-12-01

    The sedimentary basin and the orogenic belt are the basic two tectonic units of the continental lithosphere, and form the basin-mountain coupling system, The research of which is the key element to the oil and gas exploration, the global tectonic theory and models and the development of the geological theory. The Sichuan basin and adjacent orogenic belts is one of the most ideal sites to research the issues above, in particular by the recent deep seismic profiling datum. From the 1980s to now, there are 11 deep seismic sounding profiles and 6 deep seismic reflection profiles and massive seismic broadband observation stations deployed around and crossed the Sichuan basin, which provide us a big opportunity to research the deep structure and other forward issues in this region. Supported by the National Natural Science Foundation of China (Grant No. 41104056) and the Fundamental Research Funds of the Institute of Geological Sciences, CAGS (No. J1119), we sampled the Moho depth and low-velocity zone depth and the Pn velocity of these datum, then formed the contour map of the Moho depth and Pn velocity by the interpolation of the sampled datum. The result shows the Moho depth beneath Sichuan basin ranges from 40 to 44 km, the sharp Moho offset appears in the western margin of the Sichuan basin, and there is a subtle Moho depression in the central southern part of the Sichuan basin; the P wave velocity can be 6.0 km/s at ca. 10 km deep, and increases gradually deeper, the average P wave velocity in this region is ca. 6.3 km/s; the Pn velocity is ca. 8.0-8.02 km/s in Sichuan basin, and 7.70-7.76 km/s in Chuan-Dian region; the low velocity zone appears in the western margin of the Sichuan basin, which maybe cause the cause of the earthquake.

  20. Marine magnetic anomalies in the NE Indian Ocean: the Wharton and Central Indian basins revisited

    NASA Astrophysics Data System (ADS)

    Jacob, J.; Dyment, J.; Yatheesh, V.; Bhattacharya, G. C.

    2009-04-01

    The North-eastern Indian Ocean has recently received a renewed interest. The disastrous earthquakes and tsunamis of Dec. 2004 off Sumatra have triggered a large international effort including several oceanographic cruises. The Ninetyeast Ridge, a long submarine ridge which extends NS on more than 4000 km, has been the focus of a recent cruise aiming to study the interaction of a hotspot with the oceanic lithosphere and spreading centres. Both the study of the seismogenic zone under Sumatra and the Ninetyeast Ridge formation require accurate determination of the age and structure of the oceanic lithosphere in the Wharton and Central Indian Basins. First we delineate tectonic elements such as the Sunda Trench, the Ninetyeast Ridge, and the fracture zones of the Wharton and Central Indian basins from a recent version of the free-air gravity anomaly deduced from satellite altimetry and available multibeam bathymetric data. We use all available magnetic data to identify magnetic anomalies and depict seafloor spreading isochrons in order to build a tectonic map of the Wharton Basin. To do so, we apply the analytic signal method to unambiguously determine the location of the magnetic picks. The new tectonic map shows more refinements than previous ones, as expected from a larger data set. The fossil ridge in the Wharton Basin is clearly defined; spreading ceased at anomaly 18 young (38.5 Ma), and, perhaps, as late as anomaly 15 (35 Ma). Symmetric anomalies are observed on both flanks of the fossil ridge up to anomaly 24 (54 Ma), preceded by a slight reorganization of the spreading compartments between anomalies 28 and 25 (64 - 56 Ma) and a more stable phase of spreading between anomalies 34 and 29 (83 - 64 Ma). Earlier, a major change of spreading direction is clearly seen in the bending fracture zones; interpolating in the Cretaceous Quiet Zone between anomaly 34 in the Wharton Basin and anomaly M0 off Australia leads to an age of ~100 Ma for this reorganization

  1. Geological Structure and History of the Arctic Ocean

    NASA Astrophysics Data System (ADS)

    Petrov, Oleg; Morozov, Andrey; Shokalsky, Sergey; Sobolev, Nikolay; Kashubin, Sergey; Pospelov, Igor; Tolmacheva, Tatiana; Petrov, Eugeny

    2016-04-01

    New data on geological structure of the deep-water part of the Arctic Basin have been integrated in the joint project of Arctic states - the Atlas of maps of the Circumpolar Arctic. Geological (CGS, 2009) and potential field (NGS, 2009) maps were published as part of the Atlas; tectonic (Russia) and mineral resources (Norway) maps are being completed. The Arctic basement map is one of supplements to the tectonic map. It shows the Eurasian basin with oceanic crust and submerged margins of adjacent continents: the Barents-Kara, Amerasian ("Amerasian basin") and the Canada-Greenland. These margins are characterized by strained and thinned crust with the upper crust layer, almost extinct in places (South Barents and Makarov basins). In the Central Arctic elevations, seismic studies and investigation of seabed rock samples resulted in the identification of a craton with the Early Precambrian crust (near-polar part of the Lomonosov Ridge - Alpha-Mendeleev Rise). Its basement presumably consists of gneiss granite (2.6-2.2 Ga), and the cover is composed of Proterozoic quartzite sandstone and dolomite overlain with unconformity and break in sedimentation by Devonian-Triassic limestone with fauna and terrigenous rocks. The old crust is surrounded by accretion belts of Timanides and Grenvillides. Folded belts with the Late Precambrian crust are reworked by Caledonian-Ellesmerian and the Late Mesozoic movements. Structures of the South Anuy - Angayucham ophiolite suture reworked in the Early Cretaceous are separated from Mesozoides proper of the Pacific - Verkhoyansk-Kolyma and Koryak-Kamchatka belts. The complicated modern ensemble of structures of the basement and the continental frame of the Arctic Ocean was formed as a result of the conjugate evolution and interaction of the three major oceans of the Earth: Paleoasian, Paleoatlantic and Paleopacific.

  2. Availability of free oxygen in deep bottom water of some Archean-Early Paleoproterozoic ocean basins as derived from iron formation facies analyses

    NASA Astrophysics Data System (ADS)

    Beukes, N. J.; Smith, A.

    2013-12-01

    Archean to Early Paleoproterozoic ocean basins are commonly, although not exclusively, depicted as rather static systems; either permanently stratified with shallow mixed oxygenated water overlying anoxic deep water or with a totally anoxic water column. The anoxic water columns are considered enriched in dissolved ferrous iron derived from hydrothermal plume activity. These sourced deposition of iron formations through precipitation of mainly ferrihydrite via reaction with free oxygen in the stratified model or anaerobic iron oxidizing photoautotrophs in the anoxic model. However, both these models face a simple basic problem if detailed facies reconstructions of deepwater microbanded iron formations (MIFs) are considered. In such MIFs it is common that the deepest water and most distal facies is hematite rich followed shoreward by magnetite, iron silicate and siderite facies iron formation. Examples of such facies relations are known from jaspilitic iron formation of the ~3,2 Ga Fig Tree Group (Barberton Mountainland), ~ 2,95 Ga iron formations of the Witwatersrand-Mozaan basin and the ~2,5 Ga Kuruman Iron Formation, Transvaal Supergroup, South Africa. Facies relations of these MIFs with associated siliciclastics or carbonates also indicate that the upper water columns of the basins, down to below wave base, were depleted in iron favoring anoxic-oxic stratification rather than total anoxia. In the MIFs it can be shown that hematite in the distal facies represents the earliest formed diagenetic mineral; most likely crystallized from primary ferrihydrite. The problem is one of how ferrihydrite could have been preserved on the ocean floor if it was in direct contact with reducing ferrous deep bottom water. Rather dissolved ferrous iron would have reacted with ferrihydrite to form diagenetic magnetite. This dilemma is resolved if in the area of deepwater hematite MIF deposition, the anoxic ferrous iron enriched plume was detached from the basin floor due to buoyancy

  3. Geophysical observations on northern part of Georges Bank and adjacent basins of Gulf of Maine

    USGS Publications Warehouse

    Oldale, R.N.; Hathaway, J.C.; Dillon, William P.; Hendricks, J.D.; Robb, James M.

    1974-01-01

    Continuous-seismic-reflection and magnetic-intensity profiles provide data for inferences about the geology of the northern part of Georges Bank and the basins of the Gulf of Maine adjacent to the bank.Basement is inferred to be mostly sedimentary and volcanic rocks of Paleozoic age that were metamorphosed and intruded locally by felsic and mafic plutons near the end of the Paleozoic Era. During Late Triassic time, large fault basins formed within the Gulf of Maine and probably beneath Georges Bank. The fault basins and a possible major northeast-trending fault zone beneath the northern part of the bank probably formed as a result of the opening Atlantic during the Mesozoic. Nonmarine sediments, associated with mafic flows and intrusive rocks, were deposited in the fault basins as they formed. The upper surface of the Triassic and pre-Triassic rocks that comprise basement is an unconformity that makes up much of the bottom of the Gulf of Maine. Depth to the basement surface beneath the gulf differ greatly because of fluvial erosion in Tertiary time and glacial erosion in Pleistocene time. Beneath the northern part of Georges Bank the basement surface is smoother and slopes southward. Prominent valleys, cut before Late Cretaceous time, are present beneath this part of the bank.Cretaceous, Tertiary, and possibly Jurassic times were characterized by episodes of coastal-plain deposition and fluvial erosion. During this time a very thick wedge of sediment, mostly of Jurassic(?) and Cretaceous ages, was deposited on the shelf. Major periods of erosion took place at the close of the Cretaceous and during the Pliocene. Fluvial erosion during the Pliocene removed much of the coastal-plain sedimentary wedge and formed the Gulf of Maine.Pleistocene glaciers eroded all but a few remnants of the coastal-plain sediments within the gulf and deposited a thick section of drift against the north slope of Georges Bank and a thin veneer of outwash on the bank. Marine sediments were

  4. Ocean Basin Impact of Ambient Noise on Marine Mammal Detectability, Distribution, and Acoustic Communication - YIP

    DTIC Science & Technology

    2011-09-30

    when applying the 4 passive sonar equation. The integration of acoustic time series from different ocean basins will provide a synoptic...Penn State ARL Hydrophone Analog signal (V) Preamplifiers & 24-bit AiD 1-100 HzBP filter Signal Flow for a Single Hydrophone Digital signal

  5. Tiger sharks can connect equatorial habitats and fisheries across the Atlantic Ocean basin.

    PubMed

    Afonso, André S; Garla, Ricardo; Hazin, Fábio H V

    2017-01-01

    Increasing our knowledge about the spatial ecology of apex predators and their interactions with diverse habitats and fisheries is necessary for understanding the trophic mechanisms that underlie several aspects of marine ecosystem dynamics and for guiding informed management policies. A preliminary assessment of tiger shark (Galeocerdo cuvier) population structure off the oceanic insular system of Fernando de Noronha (FEN) and the large-scale movements performed by this species in the equatorial Atlantic Ocean was conducted using longline and handline fishing gear and satellite telemetry. A total of 25 sharks measuring 175-372 cm in total length (TL) were sampled. Most sharks were likely immature females ranging between 200 and 260 cm TL, with few individuals < 200 cm TL being caught. This contrasts greatly with the tiger shark size-distribution previously reported for coastal waters off the Brazilian mainland, where most individuals measured < 200 cm TL. Also, the movements of 8 individuals measuring 202-310 cm TL were assessed with satellite transmitters for a combined total of 757 days (mean = 94.6 days∙shark-1; SD = 65.6). These sharks exhibited a considerable variability in their horizontal movements, with three sharks showing a mostly resident behavior around FEN during the extent of the respective tracks, two sharks traveling west to the South American continent, and two sharks moving mostly along the middle of the oceanic basin, one of which ending up in the northern hemisphere. Moreover, one shark traveled east to the African continent, where it was eventually caught by fishers from Ivory Coast in less than 474 days at liberty. The present results suggest that young tiger sharks measuring < 200 cm TL make little use of insular oceanic habitats from the western South Atlantic Ocean, which agrees with a previously-hypothesized ontogenetic habitat shift from coastal to oceanic habitats experienced by juveniles of this species in this region. In addition

  6. Tiger sharks can connect equatorial habitats and fisheries across the Atlantic Ocean basin

    PubMed Central

    Garla, Ricardo; Hazin, Fábio H. V.

    2017-01-01

    Increasing our knowledge about the spatial ecology of apex predators and their interactions with diverse habitats and fisheries is necessary for understanding the trophic mechanisms that underlie several aspects of marine ecosystem dynamics and for guiding informed management policies. A preliminary assessment of tiger shark (Galeocerdo cuvier) population structure off the oceanic insular system of Fernando de Noronha (FEN) and the large-scale movements performed by this species in the equatorial Atlantic Ocean was conducted using longline and handline fishing gear and satellite telemetry. A total of 25 sharks measuring 175–372 cm in total length (TL) were sampled. Most sharks were likely immature females ranging between 200 and 260 cm TL, with few individuals < 200 cm TL being caught. This contrasts greatly with the tiger shark size-distribution previously reported for coastal waters off the Brazilian mainland, where most individuals measured < 200 cm TL. Also, the movements of 8 individuals measuring 202–310 cm TL were assessed with satellite transmitters for a combined total of 757 days (mean = 94.6 days∙shark-1; SD = 65.6). These sharks exhibited a considerable variability in their horizontal movements, with three sharks showing a mostly resident behavior around FEN during the extent of the respective tracks, two sharks traveling west to the South American continent, and two sharks moving mostly along the middle of the oceanic basin, one of which ending up in the northern hemisphere. Moreover, one shark traveled east to the African continent, where it was eventually caught by fishers from Ivory Coast in less than 474 days at liberty. The present results suggest that young tiger sharks measuring < 200 cm TL make little use of insular oceanic habitats from the western South Atlantic Ocean, which agrees with a previously-hypothesized ontogenetic habitat shift from coastal to oceanic habitats experienced by juveniles of this species in this region. In

  7. The newfoundland basin - Ocean-continent boundary and Mesozoic seafloor spreading history

    NASA Technical Reports Server (NTRS)

    Sullivan, K. D.

    1983-01-01

    It is pointed out that over the past 15 years there has been considerable progress in the refinement of predrift fits and seafloor spreading models of the North Atlantic. With the widespread acceptance of these basic models has come increasing interest in resolution of specific paleogeographic and kinematic problems. Two such problems are the initial position of Iberia with respect to North America and the geometry and chronology of early (pre-80 m.y.) relative motions between these two plates. The present investigation is concerned with geophysical data from numerous Bedford Institute/Dalhousie University cruises to the Newfoundland Basin which were undrtaken to determine the location of the ocean-continent boundary (OCB) and the Mesozoic spreading history on the western side. From the examination of magnetic data in the Newfoundland Basin, the OCB east of the Grand Banks is defined as the seaward limit of the 'smooth' magnetic domain which characterizes the surrounding continental shelves. A substantial improvement in Iberia-North America paleographic reconstructions is achieved.

  8. Variations in freshwater pathways from the Arctic Ocean into the North Atlantic Ocean

    NASA Astrophysics Data System (ADS)

    Wang, Zeliang; Hamilton, James; Su, Jie

    2017-06-01

    Understanding the mechanisms that drive exchanges between the Arctic Ocean and adjacent oceans is critical to building our knowledge of how the Arctic is reacting to a warming climate, and how potential changes in Arctic Ocean freshwater export may impact the AMOC (Atlantic Meridional Overturning Circulation). Here, freshwater pathways from the Arctic Ocean to the North Atlantic are investigated using a 1 degree global model. An EOF analysis of modeled sea surface height (SSH) demonstrates that while the second mode accounts for only 15% of the variability, the associated geostrophic currents are strongly correlated with freshwater exports through CAA (Canadian Arctic Archipelago; r = 0.75), Nares Strait (r = 0.77) and Fram Strait (r = -0.60). Separation of sea level into contributing parts allows us to show that the EOF1 is primarily a barotropic mode reflecting variability in bottom pressure equivalent sea level, while the EOF2 mode reflects changes in steric height in the Arctic Basin. This second mode is linked to momentum wind driven surface current, and dominates the Arctic Ocean freshwater exports. Both the Arctic Oscillation and Arctic Dipole atmospheric indices are shown to be linked to Arctic Ocean freshwater exports, with the forcing associated with the Arctic Dipole reflecting the out-of-phase relationship between transports through the CAA and those through Fram Strait. Finally, observed freshwater transport variation through the CAA is found to be strongly correlated with tide gauge data from the Beaufort Sea coast (r = 0.81), and with the EOF2 mode of GRACE bottom pressure data (r = 0.85) on inter-annual timescales.

  9. Kinematics of a former oceanic plate of the Neotethys revealed by deformation in the Ulukışla basin (Turkey)

    NASA Astrophysics Data System (ADS)

    Gürer, Derya; van Hinsbergen, Douwe J. J.; Matenco, Liviu; Corfu, Fernando; Cascella, Antonio

    2016-10-01

    Kinematic reconstruction of modern ocean basins shows that since Pangea breakup a vast area in the Neotethyan realm was lost to subduction. Here we develop a first-order methodology to reconstruct the kinematic history of the lost plates of the Neotethys, using records of subducted plates accreted to (former) overriding plates, combined with the kinematic analysis of overriding plate extension and shortening. In Cretaceous-Paleogene times, most of Anatolia formed a separate tectonic plate—here termed "Anadolu Plate"—that floored part of the Neotethyan oceanic realm, separated from Eurasia and Africa by subduction zones. We study the sedimentary and structural history of the Ulukışla basin (Turkey); overlying relics of this plate to reconstruct the tectonic history of the oceanic plate and its surrounding trenches, relative to Africa and Eurasia. Our results show that Upper Cretaceous-Oligocene sediments were deposited on the newly dated suprasubduction zone ophiolites ( 92 Ma), which are underlain by mélanges, metamorphosed and nonmetamorphosed oceanic and continental rocks derived from the African Plate. The Ulukışla basin underwent latest Cretaceous-Paleocene N-S and E-W extension until 56 Ma. Following a short period of tectonic quiescence, Eo-Oligocene N-S contraction formed the folded structure of the Bolkar Mountains, as well as subordinate contractional structures within the basin. We conceptually explain the transition from extension, to quiescence, to shortening as slowdown of the Anadolu Plate relative to the northward advancing Africa-Anadolu trench resulting from collision of continental rocks accreted to Anadolu with Eurasia, until the gradual demise of the Anadolu-Eurasia subduction zone.

  10. Evidence of a modern deep water magmatic hydrothermal system in the Canary Basin (eastern central Atlantic Ocean)

    NASA Astrophysics Data System (ADS)

    Medialdea, T.; Somoza, L.; González, F. J.; Vázquez, J. T.; de Ignacio, C.; Sumino, H.; Sánchez-Guillamón, O.; Orihashi, Y.; León, R.; Palomino, D.

    2017-08-01

    New seismic profiles, bathymetric data, and sediment-rock sampling document for the first time the discovery of hydrothermal vent complexes and volcanic cones at 4800-5200 m depth related to recent volcanic and intrusive activity in an unexplored area of the Canary Basin (Eastern Atlantic Ocean, 500 km west of the Canary Islands). A complex of sill intrusions is imaged on seismic profiles showing saucer-shaped, parallel, or inclined geometries. Three main types of structures are related to these intrusions. Type I consists of cone-shaped depressions developed above inclined sills interpreted as hydrothermal vents. Type II is the most abundant and is represented by isolated or clustered hydrothermal domes bounded by faults rooted at the tips of saucer-shaped sills. Domes are interpreted as seabed expressions of reservoirs of CH4 and CO2-rich fluids formed by degassing and contact metamorphism of organic-rich sediments around sill intrusions. Type III are hydrothermal-volcanic complexes originated above stratified or branched inclined sills connected by a chimney to the seabed volcanic edifice. Parallel sills sourced from the magmatic chimney formed also domes surrounding the volcanic cones. Core and dredges revealed that these volcanoes, which must be among the deepest in the world, are constituted by OIB-type, basanites with an outer ring of blue-green hydrothermal Al-rich smectite muds. Magmatic activity is dated, based on lava samples, at 0.78 ± 0.05 and 1.61 ± 0.09 Ma (K/Ar methods) and on tephra layers within cores at 25-237 ky. The Subvent hydrothermal-volcanic complex constitutes the first modern system reported in deep water oceanic basins related to intraplate hotspot activity.Plain Language SummarySubmarine volcanism and associated hydrothermal systems are relevant processes for the evolution of the <span class="hlt">ocean</span> <span class="hlt">basins</span>, due their impact on the geochemistry of the <span class="hlt">oceans</span>, their potential to form significant ore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.2548M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.2548M"><span>The distribution and tectonic framework of Late Paleozoic volcanoes in the Junggar <span class="hlt">basin</span> and its <span class="hlt">adjacent</span> area, NW China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mao, X.; Li, J. H.</p> <p>2012-04-01</p> <p>We analyse the distribution and characteristics of 145 late Paleozoic volcanoes in north Xinjiang, NW China, including 32 volcanoes on the edge of the Junggar <span class="hlt">basin</span>. These volcanoes are clustered and can be divided into calderas, volcanic domes, and volcanic necks. There are also 85 volcanoes inside the Junggar <span class="hlt">basin</span>, which are dominantly distributed in the Ke-Bai fractured zone of the northwestern margin of Junggar <span class="hlt">Basin</span>, 4 depressions (Dongdaohaizi Depression, Dishuiquan Depression, Sannan Depression and Wucaiwan Depression) and 7 uplifts (Baijiahai uplift, Beisantai uplift, Dibei uplift, Dinan uplift, Sangequan uplift, Shixi uplift and Xiayan uplift). The volcanoes inside the <span class="hlt">basin</span> are principally controlled by Hercynian Fault Systems, along NE and nearly EW trending faults and most developed in the interjunctions of the faults. The long modification by late-stage weathering and leaching made the volcanoes difficult to identify. Remaining volcanic landforms, changing trends of the volcanic lithofacies and the typical volcanic rock, such as the crypto- explosive breccia, are the typical marks of the late Paleozoic volcanoes in the field; and the concealed volcanic edifices are identified by the techniques of seismic identification, such as seismic slicing, analysis of the attribute and tectonic trend plane. The ages of the volcanic rocks are focused on from 340 Ma to 320Ma and from 300 Ma to 295 Ma, corresponding to the subducting periods of West Junggar and East Junggar. From early Carboniferous to late Carboniferous, the volcanic activities in Junggar <span class="hlt">Basin</span> and its <span class="hlt">adjacent</span> areas show a variation trend from undersea to continental, from deep water to shallow water and from continental margin to intracontinental.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45..277G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45..277G"><span>Decadal Comparisons of Particulate Matter in Repeat Transects in the Atlantic, Pacific, and Indian <span class="hlt">Ocean</span> <span class="hlt">Basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gardner, W. D.; Mishonov, A. V.; Richardson, M. J.</p> <p>2018-01-01</p> <p><span class="hlt">Basin</span>-wide sections of beam cp (proxy for particle concentration) in <span class="hlt">ocean</span> <span class="hlt">basins</span> collected during numerous oceanographic programs over the last four decades record variable concentrations in euphotic surface waters, very low concentrations through most of the water column, and very low to very high concentrations near the seafloor. Sections resampled at decadal intervals show that intense benthic nepheloid layers (BNLs) recur in the same general locations in these repeat sections, most often where eddy kinetic energy (EKE: cm2 s-2) is high in overlying waters. Areas beneath regions of low surface EKE consistently have weak to no BNLs. The decadal persistence of the close connection between surface and benthic EKE and presence or absence of BNLs is clear. Understanding the location and causes of intense versus weak BNLs helps in assessing scavenging of adsorption-prone elements in the deep sea and quantifying the impact of deep <span class="hlt">ocean</span> sediment dynamics on sediment redistribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JESS..119..531P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JESS..119..531P"><span>Correlation of the oldest Toba Tuff to sediments in the central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattan, J. N.; Shyam Prasad, M.; Babu, E. V. S. S. K.</p> <p>2010-08-01</p> <p>We have identified an ash layer in association with Australasian microtektites of ˜0.77 Ma old in two sediment cores which are ˜450 km apart in the central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB). Morphology and chemical composition of glass shards and associated microtektites have been used to trace their provenance. In ODP site 758 from Ninetyeast Ridge, ash layer-D (13 cm thick, 0.73-0.75 Ma) and layer-E (5 cm thick, 0.77-0.78 Ma) were previously correlated to the oldest Toba Tuff (OTT) eruptions of the Toba caldera, Sumatra. In this investigation, we found tephra ˜3100 km to the southwest of Toba caldera that is chemically identical to layer D of ODP site 758 and ash in the South China Sea correlated to the OTT. Layer E is not present in the CIOB or other <span class="hlt">ocean</span> <span class="hlt">basins</span>. The occurrence of tephra correlating to layer D suggests a widespread distribution of OTT tephra (˜3.6 × 107 km2), an ash volume of at least ˜1800 km3, a total OTT volume of 2300 km3, and classification of the OTT eruption as a super-eruption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011E%26PSL.309...33S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011E%26PSL.309...33S"><span>Sediment focusing in the Panama <span class="hlt">Basin</span>, Eastern Equatorial Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Singh, Ajay K.; Marcantonio, Franco; Lyle, Mitchell</p> <p>2011-09-01</p> <p>Age-model derived sediment mass accumulation rates (MARs) are consistently higher than 230Th-normalized MARs in the Equatorial Pacific <span class="hlt">Ocean</span> during the past 25 ka. The offset, being highest in the Panama <span class="hlt">Basin</span>, suggests a significant role for deep-sea sediment redistribution (i.e., sediment focusing) in this region. Here, we test the hypothesis that downslope transport of sediments from topographically high regions that surround the Panama <span class="hlt">Basin</span> is the cause of higher-than-expected xs 230Th inventories over the past 25 ka in the deeper parts of the <span class="hlt">basin</span>. We find little difference in xs 230Th inventories between the highest and lowest reaches of the <span class="hlt">basin</span>. Furthermore, there is no correlation between xs 230Th-derived sediment focusing factors and water depth which suggests that the topographic highs do not serve as a source of xs 230Th. A spatial analysis suggests that there may be an enhanced scavenging effect on xs 230Th concentrations in sediment closest to the equator where productivity is the highest, although further data is necessary to corroborate this. At the equator xs 230Th-derived focusing factors are high and range from about 1 to 5 during the Holocene and about 1 to 11 during the last glacial. In contrast, non-equatorial cores show a smaller range in variability from about 0.7 to 2.8 during the Holocene and from 0.7 to 3.6 during the last glacial. Based on 232Th flux measurements, we hypothesize that the location at which eolian detrital fluxes surpass the riverine detrital fluxes is approximately 300 km from the margin. While riverine fluxes from coastal margins were higher during the Holocene, eolian fluxes were higher during the last glacial.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015971','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015971"><span>Hydrogeochemistry and stable isotopes of ground and surface waters from two <span class="hlt">adjacent</span> closed <span class="hlt">basins</span>, Atacama Desert, northern Chile</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Alpers, Charles N.; Whittemore, Donald O.</p> <p>1990-01-01</p> <p>The geochemistry and stable isotopes of groundwaters, surface waters, and precipitation indicate different sources of some dissolved constituents, but a common source of recharge and other constituents in two <span class="hlt">adjacent</span> closed <span class="hlt">basins</span> in the Atacama Desert region of northern Chile (24??15???-24??45???S). Waters from artesian wells, trenches, and ephemeral streams in the Punta Negra <span class="hlt">Basin</span> are characterized by concentrations of Na>Ca>Mg and Cl ???SO4, with TDS Mg ??? Ca and SO4 > Cl, with TDS also Mg ??? Ca and SO4 > Cl, but with TDS up to 40 g/l. The deep mine waters have pH between 3.2 and 3.9, and are high in dissolved CO2 (??13 C = -4.8%PDB), indicating probable interaction with oxidizing sulfides. The deep mine waters have ??18O values of ???-1.8%.compared with values < -3.5??? for other Hamburgo <span class="hlt">Basin</span> waters; thus the mine waters may represent a mixture of meteoric waters with deeper "metamorphic" waters, which had interacted with rocks and exchanged oxygen isotopes at elevated temperatures. Alternatively, the deep mine waters may represent fossil meteoric waters which evolved isotopically along an evaporative trend starting from values quite depleted in ??18O and ??Dd relative to either precipitation or shallow groundwaters. High I/Br ratios in the Hamburgo <span class="hlt">Basin</span> waters and La Escondida mine waters are consistent with regionally high I in surficial deposits in the Atacama Desert region and may represent dissolution of a wind-blown evaporite component. Rain and snow collected during June 1984, indicate systematic ??18O and ??D fractionation with increasing elevation between 3150 and 4180 m a.s.l. (-0.21??.??18O and -1.7??.??D per 100 m). Excluding the deep mine waters from La Escondida, the waters from the Hamburgo and Punta Negra <span class="hlt">Basins</span> have similar ??D and ??18O values and together show a distinct evaporative trend (??D = 5.0 ??18O - 20.2). Snowmelt from the central Andes Cordillera to the east is the most likely source of recharge to both <span class="hlt">basins</span>. Some of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015E%26PSL.429..197K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015E%26PSL.429..197K"><span>Is the Ordos <span class="hlt">Basin</span> floored by a trapped <span class="hlt">oceanic</span> plateau?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusky, Tim; Mooney, Walter</p> <p>2015-11-01</p> <p>The Ordos <span class="hlt">Basin</span> in China has about 10 km of Neoarchean to Quaternary sediments covering an enigmatic basement of uncertain origin. The basement is tectonically stable, has a thick mantle root, low heat flow, few earthquakes, and has been slowly subsiding for billions of years. The basement has geophysical signatures that indicate it is dominantly intermediate to mafic in composition, and is similar to some other cratons world-wide, and also to several major <span class="hlt">oceanic</span> plateaus. It was accreted to the amalgamated Eastern Block and Central Orogenic belt of the North China Craton (NCC) in the Paleoproterozoic, then involved in several Proterozoic tectonic events including being over-thrust by an accretionary orogen, and intruded by Andean arc-related magmas, and then involved in a continent-continent collision during amalgamation with the Columbia Supercontinent. Thus, the basement rocks are deformed, metamorphosed to granulite facies, and determining their initial origin is difficult. We suggest that the data is consistent with an origin as an <span class="hlt">oceanic</span> plateau that accreted to the NCC and, later experienced different episodes of differentiation associated with later subduction and collisions. Formation of cratonic lithosphere by accretion of <span class="hlt">oceanic</span> plateaus may be one mechanism to create stable cratons. Other cratons that apparently formed by partial melting of underplated and imbricated <span class="hlt">oceanic</span> slabs are stable in some cases, but also re-activated and ;de-cratonized; in some cases in Asia, where they have been affected by younger subduction, hydration, slab roll-back, and melt-peridotite reactions. This suggests that the initial mode of craton formation may be a factor in the preservation of stable cratons, and de-cratonization is not only influenced by younger tectonic activity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PApGe.tmp.1330S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PApGe.tmp.1330S"><span>Identification of Individual Efficiency for Barometric Pressure and <span class="hlt">Ocean</span> Tide Load Simultaneously Acted on Deep Aquifers <span class="hlt">Adjacent</span> to the West Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shih, David Ching-Fang</p> <p>2018-06-01</p> <p>Groundwater fluctuation usually reflects the property of aquifer in nature. Actually, water level change can be caused not only by barometric pressure changes resulted from atmospheric motion, but also by the tidal effect from nearby marine system or water body. In confined aquifer, an increase in barometric pressure usually will cause a decrease in water level in well to an amount described by the barometric efficiency. The barometric efficiency can be also used as a correction factor to remove barometric effects on water levels in wells during an aquifer test. With the rise of the tidal sea on the coastal aquifer, it indicates that there will be compensating increases of water pressure and stress in the skeleton of aquifer. External forcing on groundwater level in the coastal aquifer, such as barometric effect and tidal sea, usually affect the water level to fluctuate with different phases to some extent. An adaptive adjustment to remove the combination of barometric and <span class="hlt">oceanic</span> tidal efficiency is presented in this study. This research suggests that the presented formula can simultaneously identify the individual efficiency for barometric effect and load of tidal sea considering their combined observation of groundwater level in aquifer system. An innovative application has been demonstrated for the deep aquifers <span class="hlt">adjacent</span> to the West Pacific <span class="hlt">Ocean</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA504037','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA504037"><span>U.S. GODAE: Global <span class="hlt">Ocean</span> Prediction With the HYbrid Coordinate <span class="hlt">Ocean</span> Model (HYCOM)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2009-06-01</p> <p>REPORT DATE (DD-MM- YYYY) 12-08-2009 2. REPORT TYPE Journal Article 3. DATES COVERED (From - To) 4. TITLE AND SUBTITLE U.S. GODAE: Global ...the lerformance and application of eddy-resolving, real-time global - and <span class="hlt">basin</span>-scale <span class="hlt">ocean</span> prediction systems using the HYbrid Coordinate <span class="hlt">Ocean</span>...prediction system outputs. In addnion to providing real-time, eddy-resolving global - and <span class="hlt">basin</span>-scale <span class="hlt">ocean</span> prediction systems for the US Navy and NOAA, this</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/29306','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/29306"><span>Great <span class="hlt">Basin</span> aspen ecosystems</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Dale L. Bartos</p> <p>2008-01-01</p> <p>The health of quaking aspen (Populus tremuloides) in the Great <span class="hlt">Basin</span> is of growing concern. The following provides an overview of aspen decline and die-off in areas within and <span class="hlt">adjacent</span> to the Great <span class="hlt">Basin</span> and suggests possible directions for research and management.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1532S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1532S"><span>Integrating surface and mantle constraints for palaeo-<span class="hlt">ocean</span> evolution: a tour of the Arctic and <span class="hlt">adjacent</span> regions (Arne Richter Award for Outstanding Young Scientists Lecture)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shephard, Grace E.</p> <p>2016-04-01</p> <p>Plate tectonic reconstructions heavily rely on absolute motions derived from hotspot trails or palaeomagnetic data and <span class="hlt">ocean</span>-floor magnetic anomaies and fracture-zone geometries to constrain the detailed history of <span class="hlt">ocean</span> <span class="hlt">basins</span>. However, as <span class="hlt">oceanic</span> lithosphere is progressively recycled into the mantle, kinematic data regarding the history of these now extinct-<span class="hlt">oceans</span> is lost. In order to better understand their evolution, novel workflows, which integrate a wide range of complementary yet independent geological and geophysical datasets from both the surface and deep mantle, must be utilised. In particular, the emergence of time-dependent, semi or self-consistent geodynamic models of ever-increasing temporal and spatial resolution are revealing some critical constraints on the evolution and fate of <span class="hlt">oceanic</span> slabs. The tectonic evolution of the circum-Arctic is no exception; since the breakup of Pangea, this enigmatic region has seen major plate reorganizations and the opening and closure of several <span class="hlt">ocean</span> <span class="hlt">basins</span>. At the surface, a myriad of potential kinematic scenarios including polarity, timing, geometry and location of subduction have emerged, including for systems along continental margins and intra-<span class="hlt">oceanic</span> settings. Furthermore, recent work has reignited a debate about the origins of 'anchor' slabs, such as the Farallon and Mongol-Okhotsk slabs, which have been used to refine absolute plate motions. Moving to the mantle, seismic tomography models reveal a region peppered with inferred slabs, however assumptions about their affinities and subduction location, timing, geometry and polarity are often made in isolation. Here, by integrating regional plate reconstructions with insights from seismic tomography, satellite derived gravity gradients, slab sinking rates and geochemistry, I explore some Mesozoic examples from the palaeo-Arctic, northern Panthalassa and western margin of North America, including evidence for a discrete and previously undescribed slab under</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('http://adsabs.harvard.edu/abs/2017OcMod.114...45P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OcMod.114...45P"><span>Impact of data assimilation on <span class="hlt">ocean</span> current forecasts in the Angola <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phillipson, Luke; Toumi, Ralf</p> <p>2017-06-01</p> <p>The <span class="hlt">ocean</span> current predictability in the data limited Angola <span class="hlt">Basin</span> was investigated using the Regional <span class="hlt">Ocean</span> Modelling System (ROMS) with four-dimensional variational data assimilation. Six experiments were undertaken comprising a baseline case of the assimilation of salinity/temperature profiles and satellite sea surface temperature, with the subsequent addition of altimetry, OSCAR (satellite-derived sea surface currents), drifters, altimetry and drifters combined, and OSCAR and drifters combined. The addition of drifters significantly improves Lagrangian predictability in comparison to the baseline case as well as the addition of either altimetry or OSCAR. OSCAR assimilation only improves Lagrangian predictability as much as altimetry assimilation. On average the assimilation of either altimetry or OSCAR with drifter velocities does not significantly improve Lagrangian predictability compared to the drifter assimilation alone, even degrading predictability in some cases. When the forecast current speed is large, it is more likely that the combination improves trajectory forecasts. Conversely, when the currents are weaker, it is more likely that the combination degrades the trajectory forecast.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS32A..02X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS32A..02X"><span>A numerical study of the plume in Cape Fear River Estuary and <span class="hlt">adjacent</span> coastal <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xia, M.; Xia, L.; Pietrafesa, L. J.</p> <p>2006-12-01</p> <p>Cape Fear River Estuary (CFRE), located in southeast North Carolina, is the only river estuary system in the state which is directly connected to the Atlantic <span class="hlt">Ocean</span>. It is also an important nursery for economically and ecologically important juvenile fish, crabs, shrimp, and other species because of the tidal influence and saline waters. In this study, Environmental Fluid Dynamic Code (EFDC) is used to simulate the salinity plume and trajectory distribution at the mouth of the CFRE and <span class="hlt">adjacent</span> coastal <span class="hlt">ocean</span>. Prescribed with the climatological freshwater discharge rates in the rivers, the modeling system was used to simulate the salinity plume and trajectory distribution distribution in the mouth of the CFRE under the influence of climatological wind conditions and tidal effect. We analyzed the plume formation processes and the strong relationship between the various plume distributions with respect to the wind and river discharge in the region. The simulations also indicate that strong winds tend to reduce the surface CFRE plume size and distorting the bulge region near the estuary mouth due to enhanced wind induced surface mixing. Even moderate wind speeds could fully reverse the buoyancy-driven plume structure in CFRE under normal river discharge conditions. Tide and the river discharge also are important factors to influence the plume structure. The comparions between the distribution of salinity plume and trajectory also are discussed in the study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70048870','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70048870"><span>Active transtensional intracontinental <span class="hlt">basins</span>: Walker Lane in the western Great <span class="hlt">Basin</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>Jayko, Angela S.; Bursik, Marcus</p> <p>2012-01-01</p> <p>The geometry and dimensions of sedimentary <span class="hlt">basins</span> within the Walker Lane are a result of Plio-Pleistocene transtensive deformation and partial detachment of the Sierra Nevada crustal block from the North American plate. Distinct morpho-tectonic domains lie within this active transtensive zone. The northeast end of the Walker Lane is partly buried by active volcanism of the southern Cascades, and <span class="hlt">adjacent</span> <span class="hlt">basins</span> are filled or poorly developed. To the south, the <span class="hlt">basin</span> sizes are moderate, 25–45km × 15–10 km, with narrow 8-12km wide mountain ranges mainly oriented N-S to NNE. These <span class="hlt">basins</span> form subparallel arrays in discrete zones trending about 300° and have documented clockwise rotation. This is succeeded to the south by a releasing stepover domain ∼85-100km wide, where the <span class="hlt">basins</span> are elongated E-W to ENE, small (∼15-30km long, 5-15km wide), and locally occupied by active volcanic centers. The southernmost part of the Walker Lane is structurally integrated, with high to extreme relief. <span class="hlt">Adjacent</span> <span class="hlt">basins</span> are elongate, 50-200km long and ∼5 -20km wide. Variations in transtensive <span class="hlt">basin</span> orientations in the Walker Lane are largely attributable to variations in strain partitioning. Large <span class="hlt">basins</span> in the Walker Lane have 2-6km displacement across <span class="hlt">basin</span> bounding faults with up to 3 km of clastic accumulation based on gravity and drill hole data. The sedimentary deposits of the <span class="hlt">basins</span> may include interbedded volcanic deposits with bimodal basaltic and rhyolitic associations. The <span class="hlt">basins</span> may include lacustrine deposits that record a wide range of water chemistry from cold fresh water conditions to saline-evaporative</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28794274','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28794274"><span>Stable isotope analyses of feather amino acids identify penguin migration strategies at <span class="hlt">ocean</span> <span class="hlt">basin</span> scales.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Polito, Michael J; Hinke, Jefferson T; Hart, Tom; Santos, Mercedes; Houghton, Leah A; Thorrold, Simon R</p> <p>2017-08-01</p> <p>Identifying the at-sea distribution of wide-ranging marine predators is critical to understanding their ecology. Advances in electronic tracking devices and intrinsic biogeochemical markers have greatly improved our ability to track animal movements on <span class="hlt">ocean</span>-wide scales. Here, we show that, in combination with direct tracking, stable carbon isotope analysis of essential amino acids in tail feathers provides the ability to track the movement patterns of two, wide-ranging penguin species over <span class="hlt">ocean</span> <span class="hlt">basin</span> scales. In addition, we use this isotopic approach across multiple breeding colonies in the Scotia Arc to evaluate migration trends at a regional scale that would be logistically challenging using direct tracking alone. © 2017 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PrOce.132....1Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PrOce.132....1Y"><span>A new collective view of oceanography of the Arctic and North Atlantic <span class="hlt">basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yashayaev, Igor; Seidov, Dan; Demirov, Entcho</p> <p>2015-03-01</p> <p>We review some historical aspects of the major observational programs in the North Atlantic and <span class="hlt">adjacent</span> regions that contributed to establishing and maintaining the global <span class="hlt">ocean</span> climate monitoring network. The paper also presents the <span class="hlt">oceanic</span> perspectives of climate change and touches the important issues of <span class="hlt">ocean</span> climate variability on time scales from years to decades. Some elements of the improved understanding of the causes and mechanisms of variability in the subpolar North Atlantic and <span class="hlt">adjacent</span> seas are discussed in detail. The sophistication of current oceanographic analysis, especially in connection with the most recent technological breakthroughs - notably the launch of the global array of profiling Argo floats - allows us to approach new challenges in <span class="hlt">ocean</span> research. We demonstrate how the <span class="hlt">ocean</span>-climate changes in the subpolar <span class="hlt">basins</span> and polar seas correlate with variations in the major climate indices such as the North Atlantic Oscillation and Atlantic Multidecadal Oscillation, and discuss possible connections between the unprecedented changes in the Arctic and Greenland ice-melt rates observed over the past decade and variability of hydrographic conditions in the Labrador Sea. Furthermore, a synthesis of shipboard and Argo measurements in the Labrador Sea reveals the effects of the regional climate trends such as freshening of the upper layer - possible causes of which are also discussed - on the winter convection in the Labrador Sea including its strength, duration and spatial extent. These changes could have a profound impact on the regional and planetary climates. A section with the highlights of all papers comprising the Special Issue concludes the Preface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1715707P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1715707P"><span>Arctic-HYCOS: a Large Sample observing system for estimating freshwater fluxes in the drainage <span class="hlt">basin</span> of the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pietroniro, Al; Korhonen, Johanna; Looser, Ulrich; Hardardóttir, Jórunn; Johnsrud, Morten; Vuglinsky, Valery; Gustafsson, David; Lins, Harry F.; Conaway, Jeffrey S.; Lammers, Richard; Stewart, Bruce; Abrate, Tommaso; Pilon, Paul; Sighomnou, Daniel; Arheimer, Berit</p> <p>2015-04-01</p> <p>The Arctic region is an important regulating component of the global climate system, and is also experiencing a considerable change during recent decades. More than 10% of world's river-runoff flows to the Arctic <span class="hlt">Ocean</span> and there is evidence of changes in its fresh-water balance. However, about 30% of the Arctic <span class="hlt">basin</span> is still ungauged, with differing monitoring practices and data availability from the countries in the region. A consistent system for monitoring and sharing of hydrological information throughout the Arctic region is thus of highest interest for further studies and monitoring of the freshwater flux to the Arctic <span class="hlt">Ocean</span>. The purpose of the Arctic-HYCOS project is to allow for collection and sharing of hydrological data. Preliminary 616 stations were identified with long-term daily discharge data available, and around 250 of these already provide online available data in near real time. This large sample will be used in the following scientific analysis: 1) to evaluate freshwater flux to the Arctic <span class="hlt">Ocean</span> and Seas, 2) to monitor changes and enhance understanding of the hydrological regime and 3) to estimate flows in ungauged regions and develop models for enhanced hydrological prediction in the Arctic region. The project is intended as a component of the WMO (World Meteorological Organization) WHYCOS (World Hydrological Cycle Observing System) initiative, covering the area of the expansive transnational Arctic <span class="hlt">basin</span> with participation from Canada, Denmark, Finland, Iceland, Norway, Russian Federation, Sweden and United States of America. The overall objective is to regularly collect, manage and share high quality data from a defined basic network of hydrological stations in the Arctic <span class="hlt">basin</span>. The project focus on collecting data on discharge and possibly sediment transport and temperature. Data should be provisional in near-real time if available, whereas time-series of historical data should be provided once quality assurance has been completed. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/323733-review-science-issues-deployment-strategy-status-arm-north-slope-alaska-adjacent-arctic-ocean-climate-research-site','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/323733-review-science-issues-deployment-strategy-status-arm-north-slope-alaska-adjacent-arctic-ocean-climate-research-site"><span>Review of science issues, deployment strategy, and status for the ARM north slope of Alaska-<span class="hlt">Adjacent</span> Arctic <span class="hlt">Ocean</span> climate research 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>Stamnes, K.; Ellingson, R.G.; Curry, J.A.</p> <p>1999-01-01</p> <p>Recent climate modeling results point to the Arctic as a region that is particularly sensitive to global climate change. The Arctic warming predicted by the models to result from the expected doubling of atmospheric carbon dioxide is two to three times the predicted mean global warming, and considerably greater than the warming predicted for the Antarctic. The North Slope of Alaska-<span class="hlt">Adjacent</span> Arctic <span class="hlt">Ocean</span> (NSA-AAO) Cloud and Radiation Testbed (CART) site of the Atmospheric Radiation Measurement (ARM) Program is designed to collect data on temperature-ice-albedo and water vapor-cloud-radiation feedbacks, which are believed to be important to the predicted enhanced warming inmore » the Arctic. The most important scientific issues of Arctic, as well as global, significance to be addressed at the NSA-AAO CART site are discussed, and a brief overview of the current approach toward, and status of, site development is provided. ARM radiometric and remote sensing instrumentation is already deployed and taking data in the perennial Arctic ice pack as part of the SHEBA (Surface Heat Budget of the Arctic <span class="hlt">ocean</span>) experiment. In parallel with ARM`s participation in SHEBA, the NSA-AAO facility near Barrow was formally dedicated on 1 July 1997 and began routine data collection early in 1998. This schedule permits the US Department of Energy`s ARM Program, NASA`s Arctic Cloud program, and the SHEBA program (funded primarily by the National Science Foundation and the Office of Naval Research) to be mutually supportive. In addition, location of the NSA-AAO Barrow facility on National <span class="hlt">Oceanic</span> and Atmospheric Administration land immediately <span class="hlt">adjacent</span> to its Climate Monitoring and Diagnostic Laboratory Barrow Observatory includes NOAA in this major interagency Arctic collaboration.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29550607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29550607"><span>Plastic pollution in islands of the Atlantic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Monteiro, Raqueline C P; Ivar do Sul, Juliana A; Costa, Monica F</p> <p>2018-07-01</p> <p>Marine plastic pollution is present in all <span class="hlt">oceans</span>, including remote <span class="hlt">oceanic</span> islands. Despite the increasing number of articles on plastic pollution in the last years, there is still a lack of studies in islands, that are biodiversity hotspots when compared to the surrounding <span class="hlt">ocean</span>, and even other recognized highly biodiverse marine environments. Articles published in the peer reviewed literature (N = 20) were analysed according to the presence of macro (>5 mm) and microplastics (<5 mm) on beaches and the marine habitats immediately <span class="hlt">adjacent</span> to 31 islands of the Atlantic <span class="hlt">Ocean</span> and Caribbean Sea. The first articles date from the 1980s, but most were published in the 2000s. Articles on macroplastics were predominant in this review (N = 12). Beaches were the most studied environment, possibly due to easy access. The main focus of most articles was the spatial distribution of plastics associated with variables such as position of the beach in relation to wind and currents. Very few studies have analysed plastics colonization by organisms or the identification of persistent organic pollutants (POPs). Islands of the North/South Atlantic and Caribbean Sea were influenced by different sources of macroplastics, being marine-based sources (i.e., fishing activities) predominant in the Atlantic <span class="hlt">Ocean</span> <span class="hlt">basin</span>. On the other hand, in the Caribbean Sea, land-based sources were more common. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.6882D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.6882D"><span>Congo <span class="hlt">Basin</span> precipitation: Assessing seasonality, regional interactions, and sources of moisture</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dyer, Ellen L. E.; Jones, Dylan B. A.; Nusbaumer, Jesse; Li, Harry; Collins, Owen; Vettoretti, Guido; Noone, David</p> <p>2017-07-01</p> <p>Precipitation in the Congo <span class="hlt">Basin</span> was examined using a version of the National Center for Atmospheric Research Community Earth System Model (CESM) with water tagging capability. Using regionally defined water tracers, or tags, the moisture contribution from different source regions to Congo <span class="hlt">Basin</span> precipitation was investigated. We found that the Indian <span class="hlt">Ocean</span> and evaporation from the Congo <span class="hlt">Basin</span> were the dominant moisture sources and that the Atlantic <span class="hlt">Ocean</span> was a comparatively small source of moisture. In both rainy seasons the southwestern Indian <span class="hlt">Ocean</span> contributed about 21% of the moisture, while the recycling ratio for moisture from the Congo <span class="hlt">Basin</span> was about 25%. Near the surface, a great deal of moisture is transported from the Atlantic into the Congo <span class="hlt">Basin</span>, but much of this moisture is recirculated back over the Atlantic in the lower troposphere. Although the southwestern Indian <span class="hlt">Ocean</span> is a major source of Indian <span class="hlt">Ocean</span> moisture, it is not associated with the bulk of the variability in precipitation over the Congo <span class="hlt">Basin</span>. In wet years, more of the precipitation in the Congo <span class="hlt">Basin</span> is derived from Indian <span class="hlt">Ocean</span> moisture, but the spatial distribution of the dominant sources is shifted, reflecting changes in the midtropospheric circulation over the Indian <span class="hlt">Ocean</span>. During wet years there is increased transport of moisture from the equatorial and eastern Indian <span class="hlt">Ocean</span>. Our results suggest that reliably capturing the linkages between the large-scale circulation patterns over the Indian <span class="hlt">Ocean</span> and the local circulation over the Congo <span class="hlt">Basin</span> is critical for future projections of Congo <span class="hlt">Basin</span> precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016HydJ...24..757R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016HydJ...24..757R"><span>Quantity and location of groundwater recharge in the Sacramento Mountains, south-central New Mexico (USA), and their relation to the <span class="hlt">adjacent</span> Roswell Artesian <span class="hlt">Basin</span></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.; Newton, B. Talon</p> <p>2016-06-01</p> <p>The Sacramento Mountains and the <span class="hlt">adjacent</span> Roswell Artesian <span class="hlt">Basin</span>, in south-central New Mexico (USA), comprise a regional hydrologic system, wherein recharge in the mountains ultimately supplies water to the confined <span class="hlt">basin</span> aquifer. Geologic, hydrologic, geochemical, and climatologic data were used to delineate the area of recharge in the southern Sacramento Mountains. The water-table fluctuation and chloride mass-balance methods were used to quantify recharge over a range of spatial and temporal scales. Extrapolation of the quantitative recharge estimates to the entire Sacramento Mountains region allowed comparison with previous recharge estimates for the northern Sacramento Mountains and the Roswell Artesian <span class="hlt">Basin</span>. Recharge in the Sacramento Mountains is estimated to range from 159.86 × 106 to 209.42 × 106 m3/year. Both the location of recharge and range in estimates is consistent with previous work that suggests that ~75 % of the recharge to the confined aquifer in the Roswell Artesian <span class="hlt">Basin</span> has moved downgradient through the Yeso Formation from distal recharge areas in the Sacramento Mountains. A smaller recharge component is derived from infiltration of streamflow beneath the major drainages that cross the Pecos Slope, but in the southern Sacramento Mountains much of this water is ultimately derived from spring discharge. Direct recharge across the Pecos Slope between the mountains and the confined <span class="hlt">basin</span> aquifer is much smaller than either of the other two components.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP42B..08G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP42B..08G"><span>Terrestrial paleoclimatic changes in northeast Asia during OAE 3 in the Late Cretaceous: Organic geochemical evidences from the Songliao paleo-lake <span class="hlt">Basin</span>, northeast China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gao, Y.; Wang, C.; Huang, H.</p> <p>2016-12-01</p> <p><span class="hlt">Oceanic</span> anoxic events (OAEs) in the Cretaceous greenhouse world record significant paleoclimatic changes and represent major disturbances in the global carbon cycle. The Coniacian-Santonian <span class="hlt">oceanic</span> anoxic event (OAE 3), the last of the Cretaceous OAEs, is characterized by restricted black shale deposits in equatorial to mid-latitude Atlantic and <span class="hlt">adjacent</span> <span class="hlt">basins</span>. Continental hydroclimate on tropical Africa and South America was proved have a strong effect on carbon burial in <span class="hlt">ocean</span> <span class="hlt">basins</span> during OAE 3, although terrestrial paleoclimatic changes on the other continents were not well understood. The Continental Scientific Drilling Project of the Songliao paleo-lake <span class="hlt">Basin</span> (northeast China) recovered 500m thick, continuous, dark-colored, deep lacustrine mudstone of the Qingshankou Formation, with the age of 92.0-86.2Ma tightly constrained by radiometric dating on volcanic ashes, magnetostratigraphy and cyclostratigraphy. These sediments thus provide an opportunity to study terrestrial paleoclimate changes in northeast Asia during OAE 3. Our high-resolution ( 1m interval) TOC and δ13Corg data of the Qingshankou Formation in the Songliao <span class="hlt">Basin</span> show several positive δ13Corg excursions over the OAE 3 time period. Spectrum analysis shows remarkable Milankovich cycles including eccentricity cycles ( 400kyr) and precession cycles ( 20 kyr). These data suggest that dark-colored mudstone deposition in the Songliao paleo-lake was probably controlled by regional hydroclimatic changes which were influenced by orbital forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70027395','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70027395"><span>Mississippian carbonate buildups and development of cool-waterlike carbonate platforms in the Illinois <span class="hlt">Basin</span>, Midcontinent U.S.A.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lasemi, Z.; Norby, R.D.; Utgaard, J.E.; Ferry, W.R.; Cuffey, R.J.; Dever, G.R.</p> <p>2005-01-01</p> <p>Numerous biohermal buildups occur in Mississippian (Lower Carboniferous) strata in the Illinois <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> regions. They developed as mud mounds, biodetrital calcisiltite mounds, and bryozoan frame thickets (fenestrate-frame coquina or rudstone) during the Kinderhookian and early Meramecian (Tournaisian and early Visean), and as microbial mud mounds, microbial- serpulidbryozoanboundstones, and solenoporoid (red algal) boundstones during the Chesterian (late Visean and Serpukhovian). True Waulsortian mounds did not develop in the Illinois <span class="hlt">Basin</span>, but echinoderm (primarily crinoids)-bryozoan carbonate banks and bryozoan frame thickets generally occupied the same niche during the Kinderhookian-early Meramecian. Nutrient availability and the resulting increase in the productivity of echinoderms and bryozoans were apparently detrimental to Waulsortian mound development. Deposition of crinoidal-bryozoan carbonates during the Kinderhookian-Osagean initially occurred on a ramp setting that later evolved into a platform with a relatively steep margin through sediment aggradation and progradation. By mid-Osagean-early Meramecian, two such platforms, namely the Burlington Shelf and the Ullin Platform, developed <span class="hlt">adjacent</span> to a deep, initially starved <span class="hlt">basin</span>. Sedimentologic and petrographic characteristics of the Kinderhookian-earliest Meramecian carbonates resemble the modern cool-water Heterozoan Association. This is in contrast with post-earliest Meramecian carbonates, which are typically oolitic and peloidal with common peri tidal facies. The post-earliest Meramecian carbonates, therefore, resemble those of the warm-water Photozoan Association. The prevalence of Heterozoan carbonates in the Illinois <span class="hlt">Basin</span> correlates with a rapid increase in the rate of subsidence and a major second-order eustatic sea-level rise that resulted in deep-water starved <span class="hlt">basins</span> at this time. In the starved Illinois <span class="hlt">Basin</span>, deposition was initially limited to a thin phosphatic shale that was</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFM.V23E0681G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.V23E0681G"><span>Evidence for Thin <span class="hlt">Oceanic</span> Crust on the Extinct Aegir Ridge, Norwegian <span class="hlt">Basin</span>, N.E. Atlantic Derived from Satellite Gravity Inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Greenhalgh, E. E.; Kusznir, N. J.</p> <p>2006-12-01</p> <p>Satellite gravity inversion incorporating a lithosphere thermal gravity correction has been used to map crustal thickness and lithosphere thinning factor for the N.E. Atlantic. The inversion of gravity data to determine crustal thickness incorporates a lithosphere thermal gravity anomaly correction for both <span class="hlt">oceanic</span> and continental margin lithosphere. Predicted crustal thicknesses in the Norwegian <span class="hlt">Basin</span> are between 7 and 4 km on the extinct Aegir <span class="hlt">oceanic</span> ridge which ceased sea-floor spreading in the Oligocene. Crustal thickness estimates do not include a correction for sediment thickness and are upper bounds. Crustal thicknesses determined by gravity inversion for the Aegir Ridge are consistent with recent estimates derived using refraction seismology by Breivik et al. (2006). Failure to incorporate a lithosphere thermal gravity anomaly correction produces an over-estimate of crustal thickness. <span class="hlt">Oceanic</span> crustal thicknesses within the Norwegian <span class="hlt">Basin</span> are predicted by the gravity inversion to increase to 9-10 km eastwards towards the Norwegian (Moere) and westwards towards the Jan Mayen micro-continent, consistent with volcanic margin continental breakup at the end of the Palaeocene. The observation (from gravity inversion and seismic refraction studies) of thin <span class="hlt">oceanic</span> crust produced by the Aegir <span class="hlt">ocean</span> ridge in the Oligocene has implications for the temporal evolution of asthenosphere temperature under the N.E. Atlantic during the Tertiary. Thin Oligocene <span class="hlt">oceanic</span> crust may imply cool (normal) asthenosphere temperatures during the Oligocene in contrast to elevated asthenosphere temperatures in the Palaeocene and Miocene-Recent as indicated by volcanic margin formation and the formation of Iceland respectively. Gravity inversion also predicts a region of thin <span class="hlt">oceanic</span> crust to the west of the northern part of the Jan Mayen micro-continent and to the east of the thicker <span class="hlt">oceanic</span> crust currently being formed at the Kolbeinsey Ridge. Thicker crust (c.f. <span class="hlt">ocean</span> <span class="hlt">basins</span>) is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2010/5072/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2010/5072/"><span>Geohydrology of the Aucilla-Suwannee-Ochlockonee River <span class="hlt">Basin</span>, south-central Georgia and <span class="hlt">adjacent</span> parts of 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>Torak, Lynn J.; Painter, Jaime A.; Peck, Michael F.</p> <p>2010-01-01</p> <p>Major streams and tributaries located in the Aucilla-Suwannee-Ochlockonee (ASO) River <span class="hlt">Basin</span> of south-central Georgia and <span class="hlt">adjacent</span> parts of Florida drain about 8,000 square miles of a layered sequence of clastic and carbonate sediments and carbonate Coastal Plain sediments consisting of the surficial aquifer system, upper semiconfining unit, Upper Floridan aquifer, and lower confining unit. Streams either flow directly on late-middle Eocene to Oligocene karst limestone or carve a dendritic drainage pattern into overlying Miocene to Holocene sand, silt, and clay, facilitating water exchange and hydraulic connection with geohydrologic units. Geologic structures operating in the ASO River <span class="hlt">Basin</span> through time control sedimentation and influence geohydrology and water exchange between geohydrologic units and surface water. More than 300 feet (ft) of clastic sediments overlie the Upper Floridan aquifer in the Gulf Trough-Apalachicola Embayment, a broad area extending from the southwest to the northeast through the center of the <span class="hlt">basin</span>. These clastic sediments limit hydraulic connection and water exchange between the Upper Floridan aquifer, the surficial aquifer system, and surface water. Accumulation of more than 350 ft of low-permeability sediments in the Southeast Georgia Embayment and Suwannee Strait hydraulically isolates the Upper Floridan aquifer from land-surface hydrologic processes in the Okefenokee <span class="hlt">Basin</span> physiographic district. Burial of limestone beneath thick clastic overburden in these areas virtually eliminates karst processes, resulting in low aquifer hydraulic conductivity and storage coefficient despite an aquifer thickness of more than 900 ft. Conversely, uplift and faulting associated with regional tectonics and the northern extension of the Peninsular Arch caused thinning and erosion of clastic sediments overlying the Upper Floridan aquifer southeast of the Gulf Trough-Apalachicola Embayment near the Florida-Georgia State line. Limestone dissolution in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JAESc.131....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JAESc.131....1S"><span>Pseudofaults and associated seamounts in the conjugate Arabian and Eastern Somali <span class="hlt">basins</span>, NW Indian <span class="hlt">Ocean</span> - New constraints from high-resolution satellite-derived gravity data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sreejith, K. M.; Chaubey, A. K.; Mishra, Akhil; Kumar, Shravan; Rajawat, A. S.</p> <p>2016-12-01</p> <p>Marine gravity data derived from satellite altimeters are effective tools in mapping fine-scale tectonic features of the <span class="hlt">ocean</span> <span class="hlt">basins</span> such as pseudofaults, fracture zones and seamounts, particularly when the <span class="hlt">ocean</span> <span class="hlt">basins</span> are carpeted with thick sediments. We use high-resolution satellite-generated gravity and seismic reflection data to map boundaries of pseudofaults and transferred crust related to the Paleocene spreading ridge propagation in the Arabian and its conjugate Eastern Somali <span class="hlt">basins</span>. The study has provided refinement in the position of previously reported pseudofaults and their spatial extensions in the conjugate <span class="hlt">basins</span>. It is observed that the transferred crustal block bounded by inner pseudofault and failed spreading ridge is characterized by a gravity low and rugged basement. The refined satellite gravity image of the Arabian <span class="hlt">Basin</span> also revealed three seamounts in close proximity to the pseudofaults, which were not reported earlier. In the Eastern Somali <span class="hlt">Basin</span>, seamounts are aligned along NE-SW direction forming ∼300 km long seamount chain. Admittance analysis and Flexural model studies indicated that the seamount chain is isostatically compensated locally with Effective Elastic Thickness (Te) of 3-4 km. Based on the present results and published plate tectonic models, we interpret that the seamounts in the Arabian <span class="hlt">Basin</span> are formed by spreading ridge propagation and are associated with pseudofaults, whereas the seamount chain in the Eastern Somali <span class="hlt">Basin</span> might have probably originated due to melting and upwelling of upper mantle heterogeneities in advance of migrating/propagating paleo Carlsberg Ridge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025545','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025545"><span>Role of colloidal material in the removal of 234Th in the Canada <span class="hlt">basin</span> of the Arctic <span class="hlt">Ocean</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>Baskaran, M.; Swarzenski, P.W.; Porcelli, D.</p> <p>2003-01-01</p> <p>The phase partitioning of 234Th between dissolved ( 200m, general equilibrium existed between total 234Th and 238U. The inventory of SPM and the specific activity of particulate 234Th in the Canada <span class="hlt">Basin</span> was about an order of magnitude higher than the profile reported for the Alpha Ridge ice camp station. This higher concentration of SPM in the southwestern Canada <span class="hlt">Basin</span> is likely derived from ice-rafted sedimentary particles. Inventories of nutrients, and dissolved organic carbon and nitrogen in the upper 100 m of the Canada <span class="hlt">Basin</span> are comparable to the other estimates for the central Arctic <span class="hlt">Ocean</span>. Comparison of the mass concentrations of colloidal and filter-retained particulate matter as well as the activity of 234Th in these phases indicates that only a very small component of the colloidal material is actively involved in Th scavenging. Lower values of the conditional partition coefficient between the colloidal and dissolved phase indicate that the Arctic colloids are less reactive than colloidal material from other regions. The conditional partition coefficient between the filter-retained and dissolved phases (Kf) is generally higher than that for other regions, which is attributed to the higher complexation capacity of glacio-marine sedimentary particles in these waters. The 234Th-derived export of POC for the shelf and deep Canada <span class="hlt">Basin</span> ranges between 5.6 and 6.5 mmol m-2 d-1, and is in agreement with other estimates reported for the central Arctic <span class="hlt">Ocean</span> and Beaufort Sea. ?? 2003 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/1406c/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/1406c/report.pdf"><span>Geochemistry of ground water in alluvial <span class="hlt">basins</span> of Arizona and <span class="hlt">adjacent</span> parts of Nevada, New Mexico, and 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>Robertson, Frederick N.</p> <p>1991-01-01</p> <p>Chemical and isotope analyses of ground water from 28 <span class="hlt">basins</span> in the <span class="hlt">Basin</span> and Range physiographic province of Arizona and parts of <span class="hlt">adjacent</span> States were used to evaluate ground-water quality, determine processes that control ground-water chemistry, provide independent insight into the hydrologic flow system, and develop information transfer. The area is characterized by north- to northwest-trending mountains separated by alluvial <span class="hlt">basins</span> that form a regional topography of alternating mountains and valleys. On the basis of ground-water divides or zones of minimal <span class="hlt">basin</span> interconnection, the area was divided into 72 <span class="hlt">basins</span>, each representing an individual aquifer system. These systems are joined in a dendritic pattern and collectively constitute the major water resource in the region. Geochemical models were developed to identify reactions and mass transfer responsible for the chemical evolution of the ground water. On the basis of mineralogy and chemistry of the two major rock associations of the area, a felsic model and a mafic model were developed to illustrate geologic, climatic, and physiographic effects on ground-water chemistry. Two distinct hydrochemical processes were identified: (1) reactions of meteoric water with minerals and gases in recharge areas and (2) reactions of ground water as it moves down the hydraulic gradient. Reactions occurring in recharge and downgradient areas can be described by a 13-component system. Major reactions are the dissolution and precipitation of calcite and dolomite, the weathering of feldspars and ferromagnesian minerals, the formation of montmorillonite, iron oxyhydroxides, and probably silica, and, in some <span class="hlt">basins</span>, ion exchange. The geochemical modeling demonstrated that relatively few phases are required to derive the ground-water chemistry; 14 phases-12 mineral and 2 gas-consistently account for the chemical evolution in each <span class="hlt">basin</span>. The final phases were selected through analysis of X-ray diffraction and fluorescence data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6935608-tectonic-history-illinois-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6935608-tectonic-history-illinois-basin"><span>Tectonic history of the Illinois <span class="hlt">basin</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>Kolata, D.R.; Nelson, J.W.</p> <p>1990-05-01</p> <p>The Illinois <span class="hlt">basin</span> began as a failed rift that developed during breakup of a supercontinent approximately 550 Ma. A rift <span class="hlt">basin</span> in the southernmost part of the present Illinois <span class="hlt">basin</span> subsided rapidly and filled with about 3,000 m of probable Early and Middle Cambrian sediments. By the Late Cambrian, the rift-bounding faults became inactive and a broad relatively slowly subsiding embayment, extending well beyond the rift and open to the Iapetus <span class="hlt">Ocean</span>, persisted through most of the Paleozoic Era. Widespread deformation swept through the proto-Illinois <span class="hlt">basin</span> beginning in the latest Mississippian, continuing to the end of the Paleozoic Era. Upliftmore » of basement fault blocks resulted in the formation of many major folds and faults. The timing of deformation and location of these structures in the forelands of the Ouachita and Alleghanian orogenic belts suggest that much of the deformation resulted from continental collision between North America and Gondwana. The associated compressional stress reactivated the ancient rift-bounding faults, upthrusting the northern edge of a crustal block approximately 1,000 m within the rift. Concurrently, dikes (radiometrically dated as Early Permian), sills, and explosion breccias formed in or <span class="hlt">adjacent</span> to the reactivated rift. Subsequent extensional stress, probably associated with breakup of Pangea, caused the crustal block within the rift to sink back to near its original position. High-angle, northeast- to east-west-trending normal faults, with as much as 1,000 m of displacement, formed in the southern part of the <span class="hlt">basin</span>. These faults displace some of the northwest trending Early Permian dikes. Structural closure of the southern end of the Illinois <span class="hlt">basin</span> was caused by uplift of the Pascola arch sometime between the Late Pennsylvanian and Late Cretaceous.« less</p> </li> <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 recovered from the Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span></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 <span class="hlt">Ocean</span> between Canada and Alaska. As part of this on-going study, a joint US-Canadian ice breaker expedition operated in parts of the Canada <span class="hlt">Basin</span> 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 <span class="hlt">basin</span>. 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 recovered 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 recovered 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, recovered 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 <span class="hlt">Basin</span> recovered 4.94 m of sediment. 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/2007JAESc..30..696P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JAESc..30..696P"><span>Do manganese nodules grow or dissolve after burial? Results from the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattan, J. N.; Parthiban, G.</p> <p>2007-07-01</p> <p>Fifty buried manganese nodules at different depth intervals were recovered in 12 sediment cores from the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB). A maximum of 15 buried nodules were encountered in one sediment core (AAS-22/GC-07) and the deepest nodule was recovered at 5.50 m below seafloor in core AAS-04/GC-5A. Approximately 80% of the buried nodules are small in size (˜2 cm diameter) in contrast to the Atlantic <span class="hlt">Ocean</span> and Peru <span class="hlt">Basin</span> (Pacific <span class="hlt">Ocean</span>) where the majority of the buried nodules are large, ˜8 cm and >6 cm, respectively. Buried nodule size decreases with core depth and this distribution appears to be similar to the phenomenon of "Brazil Nut Effect". Buried nodules exhibit both smooth and rough surface textures and are ellipsoidal, elongated, rounded, sub rounded, irregular and polynucleated. Buried nodules from siliceous ooze are enriched in Mn, Cu, Ni, Zn, Mo, Ga, V and Rb whereas those from red clay are enriched in Fe, Co, Ti, U, Th, Y, Cr, Nb and Rare Earth Elements (REE). Buried nodules from siliceous ooze suggest their formation under hydrogenetic, early digenetic and diagenetic processes whereas those from red clay are of hydrogenetic origin. REE are enriched more than 1.5 times in buried nodules from red clay compared to siliceous ooze. However, the mode of incorporation of REE into buried nodules from both sedimentary environments is by a single authigenic phase consisting of Fe-Ti-P. Shale-normalized REE patterns and Ce anomalies suggest that nodules from siliceous ooze formed under more oxidizing conditions than those from red clay. Nodules buried at depths between 1.5 and 2.5 m are diagenetic (Mn/Fe ratio 10-15), formed in highly oxic environments (large positive Ce anomalies) and record aeolian dust (high Eu anomalies). Chemical composition, surface texture and morphology of buried nodules are similar to those of surface nodules from the same <span class="hlt">basin</span>. Furthermore, buried nodule compositions do not exhibit any distinct patterns within the core depth</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('https://www.ncbi.nlm.nih.gov/pubmed/25368148','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25368148"><span><span class="hlt">Basin</span>-scale estimates of pelagic and coral reef calcification in the Red Sea and Western Indian <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Steiner, Zvi; Erez, Jonathan; Shemesh, Aldo; Yam, Ruth; Katz, Amitai; Lazar, Boaz</p> <p>2014-11-18</p> <p><span class="hlt">Basin</span>-scale calcification rates are highly important in assessments of the global <span class="hlt">oceanic</span> carbon cycle. Traditionally, such estimates were based on rates of sedimentation measured with sediment traps or in deep sea cores. Here we estimated CaCO3 precipitation rates in the surface water of the Red Sea from total alkalinity depletion along their axial flow using the water flux in the straits of Bab el Mandeb. The relative contribution of coral reefs and open sea plankton were calculated by fitting a Rayleigh distillation model to the increase in the strontium to calcium ratio. We estimate the net amount of CaCO3 precipitated in the Red Sea to be 7.3 ± 0.4·10(10) kg·y(-1) of which 80 ± 5% is by pelagic calcareous plankton and 20 ± 5% is by the flourishing coastal coral reefs. This estimate for pelagic calcification rate is up to 40% higher than published sedimentary CaCO3 accumulation rates for the region. The calcification rate of the Gulf of Aden was estimated by the Rayleigh model to be ∼1/2 of the Red Sea, and in the northwestern Indian <span class="hlt">Ocean</span>, it was smaller than our detection limit. The results of this study suggest that variations of major ions on a <span class="hlt">basin</span> scale may potentially help in assessing long-term effects of <span class="hlt">ocean</span> acidification on carbonate deposition by marine organisms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4246267','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4246267"><span><span class="hlt">Basin</span>-scale estimates of pelagic and coral reef calcification in the Red Sea and Western Indian <span class="hlt">Ocean</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>Steiner, Zvi; Erez, Jonathan; Shemesh, Aldo; Yam, Ruth; Katz, Amitai; Lazar, Boaz</p> <p>2014-01-01</p> <p><span class="hlt">Basin</span>-scale calcification rates are highly important in assessments of the global <span class="hlt">oceanic</span> carbon cycle. Traditionally, such estimates were based on rates of sedimentation measured with sediment traps or in deep sea cores. Here we estimated CaCO3 precipitation rates in the surface water of the Red Sea from total alkalinity depletion along their axial flow using the water flux in the straits of Bab el Mandeb. The relative contribution of coral reefs and open sea plankton were calculated by fitting a Rayleigh distillation model to the increase in the strontium to calcium ratio. We estimate the net amount of CaCO3 precipitated in the Red Sea to be 7.3 ± 0.4·1010 kg·y−1 of which 80 ± 5% is by pelagic calcareous plankton and 20 ± 5% is by the flourishing coastal coral reefs. This estimate for pelagic calcification rate is up to 40% higher than published sedimentary CaCO3 accumulation rates for the region. The calcification rate of the Gulf of Aden was estimated by the Rayleigh model to be ∼1/2 of the Red Sea, and in the northwestern Indian <span class="hlt">Ocean</span>, it was smaller than our detection limit. The results of this study suggest that variations of major ions on a <span class="hlt">basin</span> scale may potentially help in assessing long-term effects of <span class="hlt">ocean</span> acidification on carbonate deposition by marine organisms. PMID:25368148</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5617298-caribbean-basin-framework-southern-central-america-colombian-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5617298-caribbean-basin-framework-southern-central-america-colombian-basin"><span>Caribbean <span class="hlt">basin</span> framework, 3: Southern Central America and Colombian <span class="hlt">basin</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>Kolarsky, R.A.; Mann, P.</p> <p>1991-03-01</p> <p>The authors recognize three <span class="hlt">basin</span>-forming periods in southern Central America (Panama, Costa Rica, southern Nicaragua) that they attempt to correlate with events in the Colombian <span class="hlt">basin</span> (Bowland, 1984): (1) Early-Late Cretaceous island arc formation and growth of the Central American island arc and Late Cretaceous formation of the Colombian <span class="hlt">basin</span> <span class="hlt">oceanic</span> plateau. During latest Cretaceous time, pelagic carbonate sediments blanketed the Central American island arc in Panama and Costa Rica and elevated blocks on the Colombian <span class="hlt">basin</span> <span class="hlt">oceanic</span> plateau; (2) middle Eocene-middle Miocene island arc uplift and erosion. During this interval, influx of distal terrigenous turbidites in most areas ofmore » Panama, Costa Rica, and the Colombian <span class="hlt">basin</span> marks the uplift and erosion of the Central American island arc. In the Colombian <span class="hlt">basin</span>, turbidites fill in basement relief and accumulate to thicknesses up to 2 km in the deepest part of the <span class="hlt">basin</span>. In Costa Rica, sedimentation was concentrated in fore-arc (Terraba) and back-arc (El Limon) <span class="hlt">basins</span>; (3) late Miocene-Recent accelerated uplift and erosion of segments of the Central American arc. Influx of proximal terrigenous turbidites and alluvial fans in most areas of Panama, Costa Rica, and the Colombian <span class="hlt">basin</span> marks collision of the Panama arc with the South American continent (late Miocene early Pliocene) and collision of the Cocos Ridge with the Costa Rican arc (late Pleistocene). The Cocos Ridge collision inverted the Terraba and El Limon <span class="hlt">basins</span>. The Panama arc collision produced northeast-striking left-lateral strike-slip faults and fault-related <span class="hlt">basins</span> throughout Panama as Panama moved northwest over the Colombian <span class="hlt">basin</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5200086-geohistory-analysis-santa-maria-basin-california-its-relationship-tectonic-evolution-continental-margin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5200086-geohistory-analysis-santa-maria-basin-california-its-relationship-tectonic-evolution-continental-margin"><span>Geohistory analysis of the Santa Maria <span class="hlt">basin</span>, California, and its relationship to tectonic evolution of the continental margin</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>McCrory, P.A.; Arends, R.G.; Ingle, J.C. Jr.</p> <p>1991-02-01</p> <p>The Santa Maria <span class="hlt">basin</span> of central California is a geologically complex area located along the tectonically active California continental margin. The record of Cenozoic tectonism preserved in Santa Maria strata provides an opportunity to compare the evolution of the region with plate tectonic models for Cenozoic interactions along the margin. Geohistory analysis of Neogene Santa Maria <span class="hlt">basin</span> strata provides important constraints for hypotheses of the tectonic evolution of the central California margin during its transition from a convergent to a transform plate boundary. Preliminary analyses suggest that the tectonic evolution of the Santa Maria area was dominated by coupling betweenmore » <span class="hlt">adjacent</span> <span class="hlt">oceanic</span> plates and the continental margin. This coupling is reflected in the timing of major hiatuses within the <span class="hlt">basin</span> sedimentary sequence and margin subsidence and uplift which occurred during periods of tectonic plate adjustment. Stratigraphic evidence indicates that the Santa Maria <span class="hlt">basin</span> originated on the continental shelf in early Miocene time. A component of margin subsidence is postulated to have been caused by cessation of spreading on <span class="hlt">adjacent</span> offshore microplates approximately 19-18 ma. A sharp reduction in rate of tectonic subsidence in middle Miocene time, observed in the Santa Maria <span class="hlt">basin</span> both onshore and offshore, was coeval with rotation of crustal blocks as major shearing shifts shoreward. Tectonic uplift of two eastern sites, offshore Point Arguello and near Point Sal, in the late Miocene may have been related to a change to transpressional motion between the Pacific and North American plates, as well as to rotation of the western Transverse Ranges in a restraining geometry.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRB..118..808G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRB..118..808G"><span>The breakup of East Gondwana: Assimilating constraints from Cretaceous <span class="hlt">ocean</span> <span class="hlt">basins</span> around India into a best-fit tectonic model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gibbons, Ana D.; Whittaker, Joanne M.; Müller, R. Dietmar</p> <p>2013-03-01</p> <p>models for the Cretaceous seafloor-spreading history of East Gondwana result in unlikely tectonic scenarios for at least one of the plate boundaries involved and/or violate particular constraints from at least one of the associated <span class="hlt">ocean</span> <span class="hlt">basins</span>. We link East Gondwana spreading corridors by integrating magnetic and gravity anomaly data from the Enderby <span class="hlt">Basin</span> off East Antarctica within a regional plate kinematic framework to identify a conjugate series of east-west-trending magnetic anomalies, M4 to M0 ( 126.7-120.4 Ma). The mid-<span class="hlt">ocean</span> ridge that separated Greater India from Australia-Antarctica propagated from north to south, starting at 136 Ma northwest of Australia, and reached the southern tip of India at 126 Ma. Seafloor spreading in the Enderby <span class="hlt">Basin</span> was abandoned at 115 Ma, when a ridge jump transferred the Elan Bank and South Kerguelen Plateau to the Antarctic plate. Our revised plate kinematic model helps resolve the problem of successive two-way strike-slip motion between Madagascar and India seen in many previously published reconstructions and also suggests that seafloor spreading between them progressed from south to north from 94 to 84 Ma. This timing is essential for tectonic flow lines to match the curved fracture zones of the Wharton and Enderby <span class="hlt">basins</span>, as Greater India gradually began to unzip from Madagascar from 100 Ma. In our model, the 85-East Ridge and Kerguelen Fracture Zone formed as conjugate flanks of a "leaky" transform fault following the 100 Ma spreading reorganization. Our model also identifies the Afanasy Nikitin Seamounts as products of the Conrad Rise hotspot.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS53A1165S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS53A1165S"><span>Sedimentary structure and tectonic setting of the abyssal <span class="hlt">basins</span> adjoining the southeast part of the Ontong Java Plateau, western Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shimizu, S.; Masato, N.; Miura, S.; Suetsugu, D.</p> <p>2017-12-01</p> <p>Ontong Java Plateau(OJP) in the western Pacific <span class="hlt">Ocean</span> is one of the largest <span class="hlt">oceanic</span> plateau in the world. Radioactive ages of drilling samples indicate that the most part of the OJP was emplaced about 122 Ma (Mahoney et al., 1993). Taylor (2006) proposed that the OJP formed as a single large volcanic province together with the Manihiki and Hikurangi plateaus. OJP is surrounding by East Mariana, Pigafetta, Nauru, Ellice, Stewart, and Lyra <span class="hlt">basins</span>. The East Mariana and Pigafetta <span class="hlt">basins</span> were formed at the Pacific-Izanagi ridge and the Nauru <span class="hlt">basin</span> was formed at Pacific-Phoenix ridges (Nakanishi et al., 1992). The tectonic history of the Ellice, Stewart, and Lyra <span class="hlt">basins</span> is still unknown because of lack of magnetic anomaly lineations. Tectonic setting during the OJP formation is thus a matter of controversy. To expose the tectonic setting of the Ellice, Stewart, and Lyra <span class="hlt">basins</span>, we conducted the Multi-Channel Seismic (MCS) survey in the <span class="hlt">basins</span> during the research cruise by R/V Mirai of JAMSTEC in 2014. We present our preliminary results of the MCS survey in the Stewart <span class="hlt">basin</span>(SB) and Ellice <span class="hlt">Basin</span>(EB). After the regular data processing, we compared the seismic facies of MCS profile with DSDP Site 288 and ODP Site 1184 to assign ages to seismic reflectors. Our processing exposed several remarkable structures in the <span class="hlt">basins</span>. The graben structures deformed only the igneous basement in the northwestern and northeastern and southwestern margins of the SB. This suggests the graben structures were formed before sedimentary layer deposited. Taylor (2006) proposed that the <span class="hlt">basin</span> was formed by the NW-SE rifting during the separation of OJP and Manihiki Plateau around 120 Ma. Neal (1997) proposed that the NE-SW rifting formed the <span class="hlt">basin</span> around 80 Ma. Our study supports the rifting model proposed by Neal et al. (1997) because the displacement of graben in northeastern and southwestern margins of the SB is larger than that in northwestern of the SB. We found several igneous diapirs in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23117411','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23117411"><span>Optimum interpolation analysis of <span class="hlt">basin</span>-scale ¹³⁷Cs transport in surface seawater in the North Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Inomata, Y; Aoyama, M; Tsumune, D; Motoi, T; Nakano, H</p> <p>2012-12-01</p> <p>¹³⁷Cs is one of the conservative tracers applied to the study of <span class="hlt">oceanic</span> circulation processes on decadal time scales. To investigate the spatial distribution and the temporal variation of ¹³⁷Cs concentrations in surface seawater in the North Pacific <span class="hlt">Ocean</span> after 1957, a technique for optimum interpolation (OI) was applied to understand the behaviour of ¹³⁷Cs that revealed the <span class="hlt">basin</span>-scale circulation of Cs ¹³⁷Cs in surface seawater in the North Pacific <span class="hlt">Ocean</span>: ¹³⁷Cs deposited in the western North Pacific <span class="hlt">Ocean</span> from global fallout (late 1950s and early 1960s) and from local fallout (transported from the Bikini and Enewetak Atolls during the late 1950s) was further transported eastward with the Kuroshio and North Pacific Currents within several years of deposition and was accumulated in the eastern North Pacific <span class="hlt">Ocean</span> until 1967. Subsequently, ¹³⁷Cs concentrations in the eastern North Pacific <span class="hlt">Ocean</span> decreased due to southward transport. Less radioactively contaminated seawater was also transported northward, upstream of the North Equatorial Current in the western North Pacific <span class="hlt">Ocean</span> in the 1970s, indicating seawater re-circulation in the North Pacific Gyre.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040171263','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040171263"><span>Contrasting Indian <span class="hlt">Ocean</span> SST Variability With and Without ENSO Influence: A Coupled Atmosphere-<span class="hlt">Ocean</span> GCM Study</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yu, Jin-Yi; Lau, K. M.</p> <p>2004-01-01</p> <p>In this study, we perform experiments with a coupled atmosphere-<span class="hlt">ocean</span> general circulation model (CGCM) to examine ENSO's influence on the interannual sea surface temperature (SST) variability of the tropical Indian <span class="hlt">Ocean</span>. The control experiment includes both the Indian and Pacific <span class="hlt">Oceans</span> in the <span class="hlt">ocean</span> model component of the CGCM (the Indo-Pacific Run). The anomaly experiment excludes ENSOs influence by including only the Indian <span class="hlt">Ocean</span> while prescribing monthly-varying climatological SSTs for the Pacific <span class="hlt">Ocean</span> (the Indian-<span class="hlt">Ocean</span> Run). In the Indo-Pacific Run, an oscillatory mode of the Indian <span class="hlt">Ocean</span> SST variability is identified by a multi-channel singular spectral analysis (MSSA). The oscillatory mode comprises two patterns that can be identified with the Indian <span class="hlt">Ocean</span> Zonal Mode (IOZM) and a <span class="hlt">basin</span>-wide warming/cooling mode respectively. In the model, the IOZM peaks about 3-5 months after ENSO reaches its maximum intensity. The <span class="hlt">basin</span> mode peaks 8 months after the IOZM. The timing and associated SST patterns suggests that the IOZM is related to ENSO, and the <span class="hlt">basin</span>- wide warming/cooling develops as a result of the decay of the IOZM spreading SST anomalies from western Indian <span class="hlt">Ocean</span> to the eastern Indian <span class="hlt">Ocean</span>. In contrast, in the Indian-<span class="hlt">Ocean</span> Run, no oscillatory modes can be identified by the MSSA, even though the Indian <span class="hlt">Ocean</span> SST variability is characterized by east-west SST contrast patterns similar to the IOZM. In both control and anomaly runs, IOZM-like SST variability appears to be associated with forcings from fluctuations of the Indian monsoon. Our modeling results suggest that the oscillatory feature of the IOZM is primarily forced by ENSO.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013QSRv...76...39Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013QSRv...76...39Y"><span>Responses of the deep <span class="hlt">ocean</span> carbonate system to carbon reorganization during the Last Glacial-interglacial cycle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Jimin; Anderson, Robert F.; Jin, Zhangdong; Rae, James W. B.; Opdyke, Bradley N.; Eggins, Stephen M.</p> <p>2013-09-01</p> <p>We present new deep water carbonate ion concentration ([CO32-]) records, reconstructed using Cibicidoides wuellerstorfi B/Ca, for one core from Caribbean <span class="hlt">Basin</span> (water depth = 3623 m, sill depth = 1.8 km) and three cores located at 2.3-4.3 km water depth from the equatorial Pacific <span class="hlt">Ocean</span> during the Last Glacial-interglacial cycle. The pattern of deep water [CO32-] in the Caribbean <span class="hlt">Basin</span> roughly mirrors that of atmospheric CO2, reflecting a dominant influence from preformed [CO32-] in the North Atlantic <span class="hlt">Ocean</span>. Compared to the amplitude of ˜65 μmol/kg in the deep Caribbean <span class="hlt">Basin</span>, deep water [CO32-] in the equatorial Pacific <span class="hlt">Ocean</span> has varied by no more than ˜15 μmol/kg due to effective buffering of CaCO3 on deep-sea pH in the Pacific <span class="hlt">Ocean</span>. Our results suggest little change in the global mean deep <span class="hlt">ocean</span> [CO32-] between the Last Glacial Maximum (LGM) and the Late Holocene. The three records from the Pacific <span class="hlt">Ocean</span> show long-term increases in [CO32-] by ˜7 μmol/kg from Marine Isotope Stage (MIS) 5c to mid MIS 3, consistent with the response of the deep <span class="hlt">ocean</span> carbonate system to a decline in neritic carbonate production associated with ˜60 m drop in sea-level (the “coral-reef” hypothesis). Superimposed upon the long-term trend, deep water [CO32-] in the Pacific <span class="hlt">Ocean</span> displays transient changes, which decouple with δ13C in the same cores, at the start and end of MIS 4. These changes in [CO32-] and δ13C are consistent with what would be expected from vertical nutrient fractionation and carbonate compensation. The observed ˜4 μmol/kg [CO32-] decline in the two Pacific cores at >3.4 km water depth from MIS 3 to the LGM indicate further strengthening of deep <span class="hlt">ocean</span> stratification, which contributed to the final step of atmospheric CO2 drawdown during the last glaciation. The striking similarity between deep water [CO32-] and 230Th-normalized CaCO3 flux at two <span class="hlt">adjacent</span> sites from the central equatorial Pacific <span class="hlt">Ocean</span> provides convincing evidence that deep</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED365555.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED365555.pdf"><span><span class="hlt">Ocean</span> Drilling Simulation Activity.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Telese, James A.; Jordan, Kathy</p> <p></p> <p>The <span class="hlt">Ocean</span> Drilling Project brings together scientists and governments from 20 countries to explore the earth's structure and history as it is revealed beneath the <span class="hlt">oceans</span>' <span class="hlt">basins</span>. Scientific expeditions examine rock and sediment cores obtained from the <span class="hlt">ocean</span> floor to learn about the earth's basic processes. The series of activities in this…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3755984','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3755984"><span>Large-Scale Distribution and Activity of Prokaryotes in Deep-Sea Surface Sediments of the Mediterranean Sea and the <span class="hlt">Adjacent</span> Atlantic <span class="hlt">Ocean</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>Giovannelli, Donato; Molari, Massimiliano; d’Errico, Giuseppe; Baldrighi, Elisa; Pala, Claudia; Manini, Elena</p> <p>2013-01-01</p> <p>The deep-sea represents a substantial portion of the biosphere and has a major influence on carbon cycling and global biogeochemistry. Benthic deep-sea prokaryotes have crucial roles in this ecosystem, with their recycling of organic matter from the photic zone. Despite this, little is known about the large-scale distribution of prokaryotes in the surface deep-sea sediments. To assess the influence of environmental and trophic variables on the large-scale distribution of prokaryotes, we investigated the prokaryotic assemblage composition (Bacteria to Archaea and Euryarchaeota to Crenarchaeota ratio) and activity in the surface deep-sea sediments of the Mediterranean Sea and the <span class="hlt">adjacent</span> North Atlantic <span class="hlt">Ocean</span>. Prokaryotic abundance and biomass did not vary significantly across the Mediterranean Sea; however, there were depth-related trends in all areas. The abundance of prokaryotes was positively correlated with the sedimentary concentration of protein, an indicator of the quality and bioavailability of organic matter. Moving eastwards, the Bacteria contribution to the total prokaryotes decreased, which appears to be linked to the more oligotrophic conditions of the Eastern Mediterranean <span class="hlt">basins</span>. Despite the increased importance of Archaea, the contributions of Crenarchaeota Marine Group I to the total pool was relatively constant across the investigated stations, with the exception of Matapan-Vavilov Deep, in which Euryarchaeota Marine Group II dominated. Overall, our data suggest that deeper areas of the Mediterranean Sea share more similar communities with each other than with shallower sites. Freshness and quality of sedimentary organic matter were identified through Generalized Additive Model analysis as the major factors for describing the variation in the prokaryotic community structure and activity in the surface deep-sea sediments. Longitude was also important in explaining the observed variability, which suggests that the overlying water masses might have a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029429','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029429"><span>Pliocene transpressional modification of depositional <span class="hlt">basins</span> by convergent thrusting <span class="hlt">adjacent</span> to the "Big Bend" of the San Andreas fault: An example from Lockwood Valley, southern 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>Kellogg, K.S.; Minor, S.A.</p> <p>2005-01-01</p> <p>The "Big Bend" of the San Andreas fault in the western Transverse Ranges of southern California is a left stepping flexure in the dextral fault system and has long been recognized as a zone of relatively high transpression compared to <span class="hlt">adjacent</span> regions. The Lockwood Valley region, just south of the Big Bend, underwent a profound change in early Pliocene time (???5 Ma) from <span class="hlt">basin</span> deposition to contraction, accompanied by widespread folding and thrusting. This change followed the recently determined initiation of opening of the northern Gulf of California and movement along the southern San Andreas fault at about 6.1 Ma, with the concomitant formation of the Big Bend. Lockwood Valley occupies a 6-km-wide, fault-bounded structural <span class="hlt">basin</span> in which converging blocks of Paleoproterozoic and Cretaceous crystalline basement and upper Oligocene and lower Miocene sedimentary rocks (Plush Ranch Formation) were thrust over Miocene and Pliocene <span class="hlt">basin</span>-fill sedimentary rocks (in ascending order, Caliente Formation, Lockwood Clay, and Quatal Formation). All the pre-Quatal sedimentary rocks and most of the Pliocene Quatal Formation were deposited during a mid-Tertiary period of regional transtension in a crustal block that underwent little clockwise vertical-axis rotation as compared to crustal blocks to the south. Ensuing Pliocene and Quaternary transpression in the Big Bend region began during deposition of the poorly dated Quatal Formation and was marked by four converging thrust systems, which decreased the areal extent of the sedimentary <span class="hlt">basin</span> and formed the present Lockwood Valley structural <span class="hlt">basin</span>. None of the thrusts appears presently active. Estimated shortening across the center of the <span class="hlt">basin</span> was about 30 percent. The fortnerly defined eastern Big Pine fault, now interpreted to be two separate, oppositely directed, contractional reverse or thrust faults, marks the northwestern structural boundary of Lockwood Valley. The complex geometry of the Lockwood Valley <span class="hlt">basin</span> is similar</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7005299-southern-rim-pacific-ocean-basin-southern-andes-southern-alps','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7005299-southern-rim-pacific-ocean-basin-southern-andes-southern-alps"><span>Southern rim of Pacific <span class="hlt">Ocean</span> <span class="hlt">basin</span>: southern Andes to southern Alps</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>Dalziel, I.W.D.; Garrett, S.W.; Grunow, A.M.</p> <p>1986-07-01</p> <p>Between the southern Andes of Tierra del Fuego and the southern Alps of New Zealand lies the least accessible and geologically least explored part of the Pacific <span class="hlt">Ocean</span> <span class="hlt">basin</span>. A joint United Kingdom-United States project was initiated in 1983 to elucidate the geologic history and structure of the Pacific margin of Antarctica from the Antarctic Peninsula to Pine Island Bay at approximately lone. 105/sup 0/W. The first season (1983-1984) of this West Antarctic Tectonics Project was spent in the Ellsworth-Whitmore crustal block, and the second (1984-1985) in the Thurston Island crustal block. The project involves structural and general field geology,more » petrology, geochemistry, paleomagnetism, and airborne geophysics (magnetics and radar ice echo sounding). A final geologic season will be spent in the Pensacola Mountains of the Transantarctic Range in 1987-1988.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T41C2607J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T41C2607J"><span>Three Plate Reconstruction in the Eastern Indian <span class="hlt">Ocean</span>: New Constraints on Wharton and Australian-Antarctic <span class="hlt">basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jacob, J.; Dyment, J.</p> <p>2012-12-01</p> <p>Understanding the continuous seismicity and repeated occurrence of major earthquakes in Sumatra and the neighboring area requires detailed constrains on the subducting plate. In this study we analyze the past plate kinematics evolution of the Wharton <span class="hlt">basin</span>, eastern Indian <span class="hlt">Ocean</span> through a three plate reconstruction involving Australia (AUS), Antarctica (ANT), and India (IND). We compile marine magnetic identifications in the Australian-Antarctic <span class="hlt">Basin</span> [1,2], the Crozet and Central Indian <span class="hlt">basins</span> (Yatheesh et al, in prep.) and the Wharton <span class="hlt">Basin</span> [3]. The Wharton <span class="hlt">Basin</span> is characterized by an extinct spreading center dated by anomaly 18 (38 Ma). The southern flank of the <span class="hlt">basin</span> exhibits a continuous sequence of anomalies 20n (42 Ma) to 34n (84 Ma), whereas the northern flank lacks some of the older anomalies because a significant part has been subducted in the Sunda Trench. The three-plate reconstructions have provided set of rotation parameters describing the evolution of IND-AUS. Using these parameters, we have reconstructed the missing isochrons of the northern flank and the detailed geometry of the subducted part of the Wharton <span class="hlt">basin</span>. Such an exercise provides useful constraints on the age and structure of the plate in subduction under Indonesia. As a byproduct, the three plate reconstruction provided set of rotation parameters for AUS-ANT as well, which constrains the conjugate fit between the <span class="hlt">basins</span>. Previous studies [1,2,4,5] have achieved such a fit on the base of ill-defined fracture zones. We consider the well-defined fracture zones from the Crozet, Central Indian, and Wharton <span class="hlt">basins</span>, but avoid using the poor fracture zone imprints from the Australian-Antarctic <span class="hlt">Basin</span>. As a result from this approach, we conclude that the relative motion of AUS with respect to ANT initially followed a north-south direction, then changed to northwest-southeast at anomaly 32ny, and reverted to northeast southwest at anomaly 24no prior to the establishment of the Southeast Indian</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51J..08F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51J..08F"><span>High pollution events in the Great Salt Lake <span class="hlt">Basin</span> and its <span class="hlt">adjacent</span> valleys. Insights on mechanisms and spatial distribution of the formation of secondary aerosol.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Franchin, A.; Middlebrook, A. M.; Baasandorj, M.; Brown, S. S.; Fibiger, D. L.; Goldberger, L.; McDuffie, E. E.; Moravek, A.; Murphy, J. G.; Thornton, J. A.; Womack, C.</p> <p>2017-12-01</p> <p>High pollution events are common in many locations in the U.S.A. and around the world. They can last several days or up to weeks and they negatively affect human health, deteriorate visibility, and increase premature mortality. The main causes for high pollution events are related to meteorology and sources. They often happen in the winter, when high emissions, stagnation and reduced mixing, due to a shallow boundary layer, cause high concentrations of pollutants to accumulate. In the last decades, the air quality in the U.S. has seen an overall improvement, due to the reductions in particulate and gaseous pollutants. However, some areas remain critical. The Great Salt Lake <span class="hlt">Basin</span> and its <span class="hlt">adjacent</span> valleys are currently areas where high pollution events are a serious environmental problem involving more than 2.4 million people. We will present the results of the Utah Wintertime Fine Particulate Study (UWFPS) that took place in winter 2017. During UWFPS, we carried out airborne measurements of aerosol chemical composition and precursor vapor concentrations over the Great Salt Lake <span class="hlt">Basin</span> and its <span class="hlt">adjacent</span> valleys. We will give insights into how and under which conditions conversion of precursor vapors into aerosol particles takes place in the area. We will also present a comparison of our measurements with models that will provide an insight of the mechanisms that lead to the formation of secondary aerosol particles. With the results of our work, we aim to inform strategies for pollution control in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28283355','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28283355"><span>Radiocesium in the western subarctic area of the North Pacific <span class="hlt">Ocean</span>, Bering Sea, and Arctic <span class="hlt">Ocean</span> in 2013 and 2014.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kumamoto, Yuichiro; Aoyama, Michio; Hamajima, Yasunori; Nishino, Shigeto; Murata, Akihiko; Kikuchi, Takashi</p> <p>2017-08-01</p> <p>We measured radiocesium ( 134 Cs and 137 Cs) in seawater from the western subarctic area of the North Pacific <span class="hlt">Ocean</span>, Bering Sea, and Arctic <span class="hlt">Ocean</span> in 2013 and 2014. Fukushima-derived 134 Cs in surface seawater was observed in the western subarctic area and Bering Sea but not in the Arctic <span class="hlt">Ocean</span>. Vertical profile of 134 Cs in the Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span> implies that Fukushima-derived 134 Cs intruded into the <span class="hlt">basin</span> from the Bering Sea through subsurface (150m depth) in 2014. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1411644M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1411644M"><span>Late tectonic uplift of an inverted <span class="hlt">oceanic</span> <span class="hlt">basin</span> in South East Asia: the case of Palawan Island (western Philippines)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meresse, F.; Savva, D.; Pubellier, M.; Steuer, S.; Franke, D.; Cordey, F.; Muller, C.; Sapin, F.; Mouly, B.; Auxiètre, J.-L.</p> <p>2012-04-01</p> <p>The elongated island of Palawan, bounded by two marginal <span class="hlt">basins</span>, the South China Sea to the North and the Sulu Sea to the South is composed of remnants of an inverted <span class="hlt">basin</span> (Proto-South China Sea) thrusted onto the margin of a continental terrane which rifted away from the Chinese-Vietnamese margin. Based on field observations coupled with seismic and drill-holes data, our study focuses on the structural architecture of the island in order to decipher the geodynamic evolution of the southern margin of the South China Sea. Structurally, the Palawan Island consists of: (i) the Palawan wedge, which extends towards the South China Sea is composed of deformed slope to deep <span class="hlt">ocean</span> deposits of Cretaceous (north Palawan) to Tertiary (central and south Palawan) ages. This accretionnary wedge is characterized by small wavelength folds of mainly NE-SW trend. Offshore, the unconformable Middle-Late Miocene Tabon limestones unit postdates the last stages of the Palawan wedge growth/setting; (ii) On top of this wedge lie thrust slices of ophiolite bodies comprising ribbon cherts of Albian age as indicated by radiolarians.; these bodies are likely to be relicts of the now-subducted Proto South China Sea; (iii) The central and southern parts of the Palawan island are characterized by a large wavelength antiform of NE-SW trend. This structure is sealed by the slightly tilted Early Pliocene marls unit; (iv) The island also presents necking zones bordered by N-S trending transform faults. This area witnessed the geodynamic evolution of the South East Asia which consists of a succession of opening/closure of <span class="hlt">oceanic</span> <span class="hlt">basins</span> and block accretions. The Palawan Island therefore results of the closing of the Proto-South China Sea which once formed both the Palawan accretionary wedge and the overlying ophiolite tectonic slices. During a later compressive event, the rifted continental margin which composes the basement of the Island was inverted, inducing the uplift and the large scale folding</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS33E..07M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS33E..07M"><span>Morphologic Variability of two <span class="hlt">Adjacent</span> Mass-Transport Deposits: Twin Slides, Gela <span class="hlt">Basin</span> (Sicily Channel).</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Minisini, D.; Trincardi, F.; Asioli, A.; Canu, M.; Foglini, F.</p> <p>2006-12-01</p> <p>Integrating geophysical, sedimentological, structural and paleontological data, we reconstruct the age, size and internal geometry of two <span class="hlt">adjacent</span> and recent mass-transport deposits (Twin Slides) exposed on the seafloor of Gela <span class="hlt">Basin</span> (Sicily Channel). Twin Slides are coeval (late-Holocene), and were likely triggered by an earthquake. Twin Slides originated from the mobilization of Pleistocene slope units, are only 6 km apart from each other, have their headscarps in similar water depth (230 m), and have a comparable run out distance (ca. 10 km). Both slides suggest a multistage evolution, but differ in internal organization and morphological expression. The northern slide shows a deposit characterised by pressure ridges in the toe region suggesting a component of plastic deformation, while the southern slide is characterised by large blocks and a reduced thickness of displaced masses. We ascribe the difference in deformation style and resulting morphology to the stratigraphic architecture of the Pleistocene progradational units involved in failure. In the case of the blocky southern slide the units affected by failure are slightly older (Eemian or pre-Emian) and more consolidated; furthermore, in the area where the headscarp is located these units appear affected by shallow faulting likely resulting in the definition of large blocks. The northern slide, instead, affects progradational units of the Last Glacial Maximum in an area where these units are more than 100 m thick and, possibly, underconsolidated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.C12B..08T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.C12B..08T"><span>The Southern <span class="hlt">Ocean</span>'s role in <span class="hlt">ocean</span> circulation and climate transients</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thompson, A. F.; Stewart, A.; Hines, S.; Adkins, J. F.</p> <p>2017-12-01</p> <p>The ventilation of deep and intermediate density classes at the surface of the Southern <span class="hlt">Ocean</span> impacts water mass modification and the air-sea exchange of heat and trace gases, which in turn influences the global overturning circulation and Earth's climate. Zonal variability occurs along the Antarctic Circumpolar Current and the Antarctic margins related to flow-topography interactions, variations in surface boundary conditions, and exchange with northern <span class="hlt">basins</span>. Information about these zonal variations, and their impact on mass and tracer transport, are suppressed when the overturning is depicted as a two-dimensional (depth-latitude) streamfunction. Here we present an idealized, multi-<span class="hlt">basin</span>, time-dependent circulation model that applies residual circulation theory in the Southern <span class="hlt">Ocean</span> and allows for zonal water mass transfer between different <span class="hlt">ocean</span> <span class="hlt">basins</span>. This model efficiently determines the temporal evolution of the <span class="hlt">ocean</span>'s stratification, ventilation and overturning strength in response to perturbations in the external forcing. With this model we explore the dynamics that lead to transitions in the circulation structure between multiple, isolated cells and a three-dimensional, "figure-of-eight," circulation in which traditional upper and lower cells are interleaved. The transient model is also used to support a mechanistic explanation of the hemispheric asymmetry and phase lag associated with Dansgaard-Oeschger (DO) events during the last glacial period. In particular, the 200 year lag in southern hemisphere temperatures, following a perturbation in North Atlantic deep water formation, depends critically on the migration of Southern <span class="hlt">Ocean</span> isopycnal outcropping in response to low-latitude stratification changes. Our results provide a self-consistent dynamical framework to explain various <span class="hlt">ocean</span> overturning transitions that have occurred over the Earth's last 100,000 years, and motivate an exploration of these mechanisms in more sophisticated climate models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/bul/1995/cc/pdf/bul1995cc.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/bul/1995/cc/pdf/bul1995cc.pdf"><span>Characterization of the Hosgri Fault Zone and <span class="hlt">adjacent</span> structures in the offshore Santa Maria <span class="hlt">Basin</span>, south-central California: Chapter CC of Evolution of sedimentary <span class="hlt">basins</span>/onshore oil and gas investigations - Santa Maria province</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Willingham, C. Richard; Rietman, Jan D.; Heck, Ronald G.; Lettis, William R.</p> <p>2013-01-01</p> <p>The Hosgri Fault Zone trends subparallel to the south-central California coast for 110 km from north of Point Estero to south of Purisima Point and forms the eastern margin of the present offshore Santa Maria <span class="hlt">Basin</span>. Knowledge of the attributes of the Hosgri Fault Zone is important for petroleum development, seismic engineering, and environmental planning in the region. Because it lies offshore along its entire reach, our characterizations of the Hosgri Fault Zone and <span class="hlt">adjacent</span> structures are primarily based on the analysis of over 10,000 km of common-depth-point marine seismic reflection data collected from a 5,000-km2 area of the central and eastern parts of the offshore Santa Maria <span class="hlt">Basin</span>. We describe and illustrate the along-strike and downdip geometry of the Hosgri Fault Zone over its entire length and provide examples of interpreted seismic reflection records and a map of the structural trends of the fault zone and <span class="hlt">adjacent</span> structures in the eastern offshore Santa Maria <span class="hlt">Basin</span>. The seismic data are integrated with offshore well and seafloor geologic data to describe the age and seismic appearance of offshore geologic units and marker horizons. We develop a <span class="hlt">basin</span>-wide seismic velocity model for depth conversions and map three major unconformities along the eastern offshore Santa Maria <span class="hlt">Basin</span>. Accompanying plates include maps that are also presented as figures in the report. Appendix A provides microfossil data from selected wells and appendix B includes uninterpreted copies of the annotated seismic record sections illustrated in the chapter. Features of the Hosgri Fault Zone documented in this investigation are suggestive of both lateral and reverse slip. Characteristics indicative of lateral slip include (1) the linear to curvilinear character of the mapped trace of the fault zone, (2) changes in structural trend along and across the fault zone that diminish in magnitude toward the ends of the fault zone, (3) localized compressional and extensional structures</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/2014AGUFMPP41C1406G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP41C1406G"><span>Global <span class="hlt">Ocean</span> Sedimentation Patterns: Plate Tectonic History Versus Climate Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Goswami, A.; Reynolds, E.; Olson, P.; Hinnov, L. A.; Gnanadesikan, A.</p> <p>2014-12-01</p> <p>Global sediment data (Whittaker et al., 2013) and carbonate content data (Archer, 1996) allows examination of <span class="hlt">ocean</span> sedimentation evolution with respect to age of the underlying <span class="hlt">ocean</span> crust (Müller et al., 2008). From these data, we construct time series of <span class="hlt">ocean</span> sediment thickness and carbonate deposition rate for the Atlantic, Pacific, and Indian <span class="hlt">ocean</span> <span class="hlt">basins</span> for the past 120 Ma. These time series are unique to each <span class="hlt">basin</span> and reflect an integrated response to plate tectonics and climate change. The goal is to parameterize <span class="hlt">ocean</span> sedimentation tied to crustal age for paleoclimate studies. For each <span class="hlt">basin</span>, total sediment thickness and carbonate deposition rate from 0.1 x 0.1 degree cells are binned according to basement crustal age; area-corrected moments (mean, variance, etc.) are calculated for each bin. Segmented linear fits identify trends in present-day carbonate deposition rates and changes in <span class="hlt">ocean</span> sedimentation from 0 to 120 Ma. In the North and South Atlantic and Indian <span class="hlt">oceans</span>, mean sediment thickness versus crustal age is well represented by three linear segments, with the slope of each segment increasing with increasing crustal age. However, the transition age between linear segments varies among the three <span class="hlt">basins</span>. In contrast, mean sediment thickness in the North and South Pacific <span class="hlt">oceans</span> are numerically smaller and well represented by two linear segments with slopes that decrease with increasing crustal age. These opposing trends are more consistent with the plate tectonic history of each <span class="hlt">basin</span> being the controlling factor in sedimentation rates, rather than climate change. Unlike total sediment thickness, carbonate deposition rates decrease smoothly with crustal age in all <span class="hlt">basins</span>, with the primary controls being <span class="hlt">ocean</span> chemistry and water column depth.References: Archer, D., 1996, Global Biogeochem. Cycles 10, 159-174.Müller, R.D., et al., 2008, Science, 319, 1357-1362.Whittaker, J., et al., 2013, Geochem., Geophys., Geosyst. DOI: 10.1002/ggge.20181</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMEP53A0995D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMEP53A0995D"><span>Equilibrium and Disequilibrium of River <span class="hlt">Basins</span>: Effects on Stream Captures in Serra do Mar and Serra da Mantiqueira, Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DA Silva, L. M.</p> <p>2015-12-01</p> <p>Landscapes are mainly driven by river processes that control the dynamic reorganization of networks. Discovering and identifying whether river <span class="hlt">basins</span> are in geometric equilibrium or disequilibrium requires an analysis of water divides, channels that shift laterally or expand upstream and river captures. Issues specifically discussed include the variation of drainage area change and erosion rates of the <span class="hlt">basins</span>. In southeastern Brazil there are two main escarpments with extensive geomorphic surfaces: Serra do Mar and Serra da Mantiqueira Mountains. These landscapes are constituted of Neoproterozoic and early Paleozoic rocks, presenting steep escarpments with low-elevation coastal plains and higher elevation interior plateaus. To identify whether river <span class="hlt">basins</span> and river profiles are in equilibrium or disequilibrium in Serra do Mar and Serra da Mantiqueira Mountains, we used the proxy (χ), evaluating the effect of drainage area change and erosion rates. We selected <span class="hlt">basins</span> that drain both sides of these two main escarpments (<span class="hlt">oceanic</span> and continental sides) and have denudation rates derived from pre-existing cosmogenic isotopes data (Rio de Janeiro, Paraná and Minas Gerais). Despite being an ancient and tectonically stable landscape, part of the coastal plain of Serra do Mar Mountain in Rio de Janeiro and Paraná is in geometric disequilibrium, with water divides moving in the direction of higher χ values. To achieve equilibrium, some <span class="hlt">basins</span> located in the continental side are retracting and disappearing, losing area to the coastal <span class="hlt">basins</span>. On the contrary, there are some <span class="hlt">adjacent</span> sub-<span class="hlt">basins</span> that are close to equilibrium, without strong contrasts in χ values. The same pattern was observed in Serra da Mantiqueira (Minas Gerais state), with stream captures and river network reorganization in its main rivers. The initial results suggest a strong contrast between erosion rates in the continental and the <span class="hlt">oceanic</span> portions of the escarpments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Tectp.726....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Tectp.726....1S"><span>Crustal characteristic variation in the central Yamato <span class="hlt">Basin</span>, Japan Sea back-arc <span class="hlt">basin</span>, deduced from seismic survey results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sato, Takeshi; No, Tetsuo; Miura, Seiichi; Kodaira, Shuichi</p> <p>2018-02-01</p> <p>The crustal structure of the Yamato Bank, the central Yamato <span class="hlt">Basin</span>, and the continental shelf in the southern Japan Sea back-arc <span class="hlt">basin</span> is obtained based on a seismic survey using <span class="hlt">ocean</span> bottom seismographs and seismic shot to elucidate the back-arc <span class="hlt">basin</span> formation processes. The central Yamato <span class="hlt">Basin</span> can be divided into three domains based on the crustal structure: the deep <span class="hlt">basin</span>, the seamount, and the transition domains. In the deep <span class="hlt">basin</span> domain, the crust without the sedimentary layer is about 12-13 km thick. Very few units have P-wave velocity of 5.4-6.0 km/s, which corresponds to the continental upper crust. In the seamount and transition domains, the crust without the sedimentary layer is about 12-16 km thick. The P-wave velocities of the upper and lower crusts differs among the deep <span class="hlt">basin</span>, the seamount, and the transition domains. These results indicate that the central Yamato <span class="hlt">Basin</span> displays crustal variability in different domains. The crust of the deep <span class="hlt">basin</span> domain is <span class="hlt">oceanic</span> in nature and suggests advanced back-arc <span class="hlt">basin</span> development. The seamount domain might have been affected by volcanic activity after <span class="hlt">basin</span> opening. In the transition domain, the crust comprises mixed characters of continental and <span class="hlt">oceanic</span> crust. This crustal variation might represent the influence of different processes in the central Yamato <span class="hlt">Basin</span>, suggesting that crustal development was influenced not only by back-arc opening processes but also by later volcanic activity. In the Yamato Bank and continental shelf, the upper crust has thickness of about 17-18 km and P-wave velocities of 3.3-4.1 to 6.6 km/s. The Yamato Bank and the continental shelf suggest a continental crustal character.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP24A..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP24A..01H"><span>Depositional History of the Western Amundsen <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span>, and Implications for Neogene Climate and Oceanographic Conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hopper, J. R.; Castro, C. F.; Knutz, P. C.; Funck, T.</p> <p>2017-12-01</p> <p>Seismic reflection data collected in the western Amundsen <span class="hlt">Basin</span> as part of the Law of the Sea program for the Kingdom of Denmark show a uniform and continuous cover of sediments over <span class="hlt">oceanic</span> basement. An interpretation of seismic facies units shows that the depositional history of the <span class="hlt">basin</span> reflects changing tectonic, climatic, and oceanographic conditions throughout the Cenozoic. In this contribution, the Miocene to present history is summarized. Two distinct changes in the depositional environment are proposed, first in response to the development of a deep water connection between the Arctic and North Atlantic, and the second in response to the onset of perennial sea ice cover in the Arctic. In the early to mid-Miocene, a buildup of contourite deposits indicates a distinct change in sedimentation that is particularly well developed near the flank of the Lomonosov Ridge. It is suggested that this is a response to the opening of the Fram Strait and the establishment of geostrophic bottom currents that flowed from the Laptev Sea towards Greenland. These deposits are overlain by a seismic facies unit characterized by buried channels and erosional features. These include prominent basinward levee systems that suggest a channel morphology maintained by overbank deposition of muddy sediments carried by suspension currents periodically spilling over the channel pathway. These deposits indicate a change to a much higher energy environment that is proposed to be a response to brine formation associated with the onset of perennial sea ice cover in the Arctic <span class="hlt">Ocean</span>. This interpretation implies that the development of extensive sea ice cover results in a significant change in the energy environment of the <span class="hlt">ocean</span> that is reflected in the depositional and erosional patterns observed. The lack of similar high energy erosional features and the presence of contourite deposits throughout most of the Miocene may indicate the Arctic <span class="hlt">Ocean</span> was relatively ice-free until the very latest</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4443878','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4443878"><span>A database for the monitoring of thermal anomalies over the Amazon forest and <span class="hlt">adjacent</span> intertropical <span class="hlt">oceans</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>Jiménez-Muñoz, Juan C.; Mattar, Cristian; Sobrino, José A.; Malhi, Yadvinder</p> <p>2015-01-01</p> <p>Advances in information technologies and accessibility to climate and satellite data in recent years have favored the development of web-based tools with user-friendly interfaces in order to facilitate the dissemination of geo/biophysical products. These products are useful for the analysis of the impact of global warming over different biomes. In particular, the study of the Amazon forest responses to drought have recently received attention by the scientific community due to the occurrence of two extreme droughts and sustained warming over the last decade. Thermal Amazoni@ is a web-based platform for the visualization and download of surface thermal anomalies products over the Amazon forest and <span class="hlt">adjacent</span> intertropical <span class="hlt">oceans</span> using Google Earth as a baseline graphical interface (http://ipl.uv.es/thamazon/web). This platform is currently operational at the servers of the University of Valencia (Spain), and it includes both satellite (MODIS) and climatic (ERA-Interim) datasets. Thermal Amazoni@ is composed of the viewer system and the web and ftp sites with ancillary information and access to product download. PMID:26029379</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26029379','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26029379"><span>A database for the monitoring of thermal anomalies over the Amazon forest and <span class="hlt">adjacent</span> intertropical <span class="hlt">oceans</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jiménez-Muñoz, Juan C; Mattar, Cristian; Sobrino, José A; Malhi, Yadvinder</p> <p>2015-01-01</p> <p>Advances in information technologies and accessibility to climate and satellite data in recent years have favored the development of web-based tools with user-friendly interfaces in order to facilitate the dissemination of geo/biophysical products. These products are useful for the analysis of the impact of global warming over different biomes. In particular, the study of the Amazon forest responses to drought have recently received attention by the scientific community due to the occurrence of two extreme droughts and sustained warming over the last decade. Thermal Amazoni@ is a web-based platform for the visualization and download of surface thermal anomalies products over the Amazon forest and <span class="hlt">adjacent</span> intertropical <span class="hlt">oceans</span> using Google Earth as a baseline graphical interface (http://ipl.uv.es/thamazon/web). This platform is currently operational at the servers of the University of Valencia (Spain), and it includes both satellite (MODIS) and climatic (ERA-Interim) datasets. Thermal Amazoni@ is composed of the viewer system and the web and ftp sites with ancillary information and access to product download.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.B33A..01W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.B33A..01W"><span>Dinitrogen Fixation Within and <span class="hlt">Adjacent</span> to Oxygen Deficient Waters of the Eastern Tropical South Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Widner, B.; Mulholland, M. R.; Bernhardt, P. W.; Chang, B. X.; Jayakumar, A.</p> <p>2016-02-01</p> <p>Recent work suggests that planktonic diazotrophs are geographically more widely distributed than previously thought including relatively warm (14-23oC) aphotic oxygenated pelagic waters and in aphotic waters within oxygen deficient zones. Because the volume of aphotic water in the <span class="hlt">ocean</span> is large and may increase in the future, if dinitrogen (N2) fixation is widely occurring at sub-euphotic depths, this could result in a dramatic upward revision of global nitrogen (N) inputs via this process. N2 fixation rates were measured during a cruise in the Eastern Tropical South Pacific using stable isotope tracer techniques that account for slow gas dissolution. Results are compared with light, nutrient, and oxygen gradients (and necessarily temperature gradients). In addition, rates of N2 fixation made in vertical profiles within and above oxygen deficient waters are compared with those measured in vertical profiles <span class="hlt">adjacent</span> to oxygen deficient waters. Results suggest that while rates of N2 fixation were measurable in deeper anoxic waters, volumetric N2 fixation rates were higher in surface waters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5537012-hydrocarbon-provinces-productive-trends-libya-adjacent-areas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5537012-hydrocarbon-provinces-productive-trends-libya-adjacent-areas"><span>Hydrocarbon provinces and productive trends in Libya and <span class="hlt">adjacent</span> areas</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>Missallati, A.A.</p> <p>1988-08-01</p> <p>According to the age of major reservoirs, hydrocarbon occurrences in Libya and <span class="hlt">adjacent</span> areas can be grouped into six major systems which, according to their geographic locations, can be classified into two major hydrocarbon provinces: (1) Sirte-Pelagian <span class="hlt">basins</span> province, with major reservoirs ranging from middle-late Mesozoic to early Tertiary, and (2) Murzog-Ghadames <span class="hlt">basins</span> province, with major reservoirs ranging from early Paleozoic to early Mesozoic. In the Sirte-Pelagian <span class="hlt">basins</span> province, hydrocarbons have been trapped in structural highs or in stratigraphic wedge-out against structural highs and in carbonate buildups. Here, hydrocarbon generation is characterized by the combined effect of abundant structural reliefmore » and reservoir development in the same hydrocarbon systems of the same age, providing an excellent example of hydrocarbon traps in sedimentary <span class="hlt">basins</span> that have undergone extensive tensional fracturing in a shallow marine environment. In the Murzog-Ghadames <span class="hlt">basins</span> province, hydrocarbons have been trapped mainly in structural highs controlled by paleostructural trends as basement arches which acted as focal points for oil migration and accumulation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040171141&hterms=tropospheric+ozone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dtropospheric%2Bozone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040171141&hterms=tropospheric+ozone&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dtropospheric%2Bozone"><span>New Perspectives from Satellite and Profile Observations on Tropospheric Ozone over Africa and the <span class="hlt">Adjacent</span> <span class="hlt">Oceans</span>: An Indian-Atlantic <span class="hlt">Ocean</span> Link to tbe "Ozone Paradox"</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thompson, Anne M.; Witte, Jacquelyn C.; Diab, Roseanne D.; Thouret, Valerie; Sauvage, Bastien; Chatfield, B.; Guan, Hong</p> <p>2004-01-01</p> <p>In the past few years, tropospheric ozone observations of Africa and its <span class="hlt">adjacent</span> ocenas have been greatly enhanced by high resolution (spatial and temporal) satellite measurements and profile data from aircraft (MOZAIC) and balloon-borne (SHADOZ) soundings. These views have demonstrated for the first time the complexity of chemical-dynamical interactions over the African continent and the Indian and Atlantic <span class="hlt">Oceans</span>. The tropical Atlantic "ozone paradax" refers to the observation that during the season of maximum biomass burning in west Africa north of the Intertropical Convergence Zone (ITCZ), the highest tropospheric ozone total column occurs south of the ITCZ over the tropical Atlantic. The longitudinal view of tropospheric ozone in the southern tropics from SHADOZ (Southern Hemisphere Additional Ozonesondes) soundings shown the persistence of a "zonal-wave one" pattern that reinforces the "ozone paradox". These ozone features interact with dynamics over southern and northern Africa where anthropogenic sources include the industrial regions of the South African Highveld and Mideastern-Mediterranean influences, respectively. Our newest studies with satellites and soundings show that up to half the ozone pollution over the Atlantic in the January-March "paradox" period may originate from south Asian pollution. Individual patches of pollurion over the Indian <span class="hlt">Ocean</span> are transported upward by convective mixing and are enriched by pyrogenic, biogenic sources and lightning as they cross Africa and descend over the Atlantic. In summary, local sources, intercontinental import and export and unique regional transport patterns put Africa at a crossroads of troposheric ozone influences.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176625','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176625"><span>Submarine landslides in Arctic sedimentation: Canada <span class="hlt">Basin</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>Mosher, David C.; Shimeld, John; Hutchinson, Deborah R.; Lebedova-Ivanova, N; Chapman, C.</p> <p>2016-01-01</p> <p>Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span> is the least studied <span class="hlt">ocean</span> <span class="hlt">basin</span> in the World. Marine seismic field programs were conducted over the past 6 years using Canadian and American icebreakers. These expeditions acquired more than 14,000 line-km of multibeam bathymetric and multi-channel seismic reflection data over abyssal plain, continental rise and slope regions of Canada <span class="hlt">Basin</span>; areas where little or no seismic reflection data existed previously. Canada <span class="hlt">Basin</span> is a turbidite-filled <span class="hlt">basin</span> with flat-lying reflections correlateable over 100s of km. For the upper half of the sedimentary succession, evidence of sedimentary processes other than turbidity current deposition is rare. The Canadian Archipelago and Beaufort Sea margins host stacked mass transport deposits from which many of these turbidites appear to derive. The stratigraphic succession of the MacKenzie River fan is dominated by mass transport deposits; one such complex is in excess of 132,000 km2 in area and underlies much of the southern abyssal plain. The modern seafloor is also scarred with escarpments and mass failure deposits; evidence that submarine landsliding is an ongoing process. In its latest phase of development, Canada <span class="hlt">Basin</span> is geomorphologically confined with stable oceanographic structure, resulting in restricted depositional/reworking processes. The sedimentary record, therefore, underscores the significance of mass-transport processes in providing sediments to <span class="hlt">oceanic</span> abyssal plains as few other <span class="hlt">basins</span> are able to do.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/dds/dds-54/Report/Bull2142.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/dds/dds-54/Report/Bull2142.pdf"><span>Thermal evolution of sedimentary <span class="hlt">basins</span> in Alaska</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Johnsson, Mark J.; Howell, D.G.</p> <p>1996-01-01</p> <p>The complex tectonic collage of Alaska is reflected in the conjunction of rocks of widely varying thermal maturity. Indicators of the level of thermal maturity of rocks exposed at the surface, such as vitrinite reflectance and conodont color alteration index, can help constrain the tectonic evolution of such complex regions and, when combined with petrographic, modern heat flow, thermogeochronologic, and isotopic data, allow for the detailed evaluation of a region?s burial and uplift history. We have collected and assembled nearly 10,000 vitrinite-reflectance and conodont-color-alteration index values from the literature, previous U.S. Geological Survey investigations, and our own studies in Alaska. This database allows for the first synthesis of thermal maturity on a broadly regional scale. Post-accretionary sedimentary <span class="hlt">basins</span> in Alaska show wide variability in terms of thermal maturity. The Tertiary interior <span class="hlt">basins</span>, as well as some of the forearc and backarc <span class="hlt">basins</span> associated with the Aleutian Arc, are presently at their greatest depth of burial, with immature rocks exposed at the surface. Other <span class="hlt">basins</span>, such as some backarc <span class="hlt">basins</span> on the Alaska Peninsula, show higher thermal maturities, indicating modest uplift, perhaps in conjunction with higher geothermal gradients related to the arc itself. Cretaceous ?flysch? <span class="hlt">basins</span>, such as the Yukon-Koyukuk <span class="hlt">basin</span>, are at much higher thermal maturity, reflecting great amounts of uplift perhaps associated with compressional regimes generated through terrane accretion. Many sedimentary <span class="hlt">basins</span> in Alaska, such as the Yukon-Koyukuk and Colville <span class="hlt">basins</span>, show higher thermal maturity at <span class="hlt">basin</span> margins, perhaps reflecting greater uplift of the margins in response to isostatic unloading, owing to erosion of the hinterland <span class="hlt">adjacent</span> to the <span class="hlt">basin</span> or to compressional stresses <span class="hlt">adjacent</span> to <span class="hlt">basin</span> margins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMOS33F..04V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMOS33F..04V"><span>Mesoscale dynamics in the Lofoten <span class="hlt">Basin</span> - a sub-Arctic "hot spot" of <span class="hlt">oceanic</span> variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volkov, D. L.; Belonenko, T. V.; Foux, V. R.</p> <p>2012-12-01</p> <p>A sub-Arctic "hot spot" of intense mesoscale variability is observed in the Lofoten <span class="hlt">Basin</span> (LB) - a topographic depression with a maximum depth of about 3250 m, located in the Norwegian Sea. The standard deviation of sea surface height (SSH), measured with satellite altimetry, reaches nearly 15 cm in the center of the <span class="hlt">basin</span> (Figure 1a). Using a space-time lagged correlation analysis of altimetry data, we discover a cyclonic propagation of the mesoscale SSH anomalies around the center of the LB with time-averaged phase speeds of 2-4 km/day, strongly linked to bottom topography (Figure 1c). The fact that surface drifter trajectories do not exhibit cyclonic circulation in the LB (Figure 1b) suggests that, at least in the upper <span class="hlt">ocean</span>, satellite altimetry observes only the propagation of form without the corresponding transfer of mass. Linearly propagating wavelike disturbances that do not trap fluid inside are related to planetary or Rossby waves. Variations in topography may lead to the concentration of wave energy in certain regions or wave trapping. The dispersion analysis suggests that the observed wavelike cyclonic propagation of SSH anomalies in the LB is the manifestation of baroclinic topographic Rossby waves, that we term "the <span class="hlt">basin</span> waves" in order to distinguish them from the other types of topographic waves, such as shelf or trench waves. We identify two modes of <span class="hlt">basin</span> waves in the LB: a di-pole mode and a quadri-pole mode. The wavelength of each mode is about 500 km. The frequency of these modes is not constant and the phase speed varies from about 2 to 8 km/day. We show that the cyclonically rotating <span class="hlt">basin</span> waves are responsible for the observed amplification of SSH variability in the LB. Because the baroclinic <span class="hlt">basin</span> waves in the LB are probably associated with large vertical displacements of the thermocline and due to possible wave breaking events, they can play an important role in the mixing of the inflowing Atlantic Water with ambient water masses</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.2602M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.2602M"><span>Continental Margins of the Arctic <span class="hlt">Ocean</span>: Implications for Law of 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>Mosher, David</p> <p>2016-04-01</p> <p>A coastal State must define the outer edge of its continental margin in order to be entitled to extend the outer limits of its continental shelf beyond 200 M, according to article 76 of the UN Convention on the Law of the Sea. The article prescribes the methods with which to make this definition and includes such metrics as water depth, seafloor gradient and thickness of sediment. Note the distinction between the "outer edge of the continental margin", which is the extent of the margin after application of the formula of article 76, and the "outer limit of the continental shelf", which is the limit after constraint criteria of article 76 are applied. For a relatively small <span class="hlt">ocean</span> <span class="hlt">basin</span>, the Arctic <span class="hlt">Ocean</span> reveals a plethora of continental margin types reflecting both its complex tectonic origins and its diverse sedimentation history. These factors play important roles in determining the extended continental shelves of Arctic coastal States. This study highlights the critical factors that might determine the outer edge of continental margins in the Arctic <span class="hlt">Ocean</span> as prescribed by article 76. Norway is the only Arctic coastal State that has had recommendations rendered by the Commission on the Limits of the Continental Shelf (CLCS). Russia and Denmark (Greenland) have made submissions to the CLCS to support their extended continental shelves in the Arctic and are awaiting recommendations. Canada has yet to make its submission and the US has not yet ratified the Convention. The various criteria that each coastal State has utilized or potentially can utilize to determine the outer edge of the continental margin are considered. Important criteria in the Arctic include, 1) morphological continuity of undersea features, such as the various ridges and spurs, with the landmass, 2) the tectonic origins and geologic affinities with the <span class="hlt">adjacent</span> land masses of the margins and various ridges, 3) sedimentary processes, particularly along continental slopes, and 4) thickness and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27801968','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27801968"><span>Estuary-<span class="hlt">ocean</span> connectivity: fast physics, slow biology.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Raimonet, Mélanie; Cloern, James E</p> <p>2017-06-01</p> <p>Estuaries are connected to both land and <span class="hlt">ocean</span> so their physical, chemical, and biological dynamics are influenced by climate patterns over watersheds and <span class="hlt">ocean</span> <span class="hlt">basins</span>. We explored climate-driven <span class="hlt">oceanic</span> variability as a source of estuarine variability by comparing monthly time series of temperature and chlorophyll-a inside San Francisco Bay with those in <span class="hlt">adjacent</span> shelf waters of the California Current System (CCS) that are strongly responsive to wind-driven upwelling. Monthly temperature fluctuations inside and outside the Bay were synchronous, but their correlations weakened with distance from the <span class="hlt">ocean</span>. These results illustrate how variability of coastal water temperature (and associated properties such as nitrate and oxygen) propagates into estuaries through fast water exchanges that dissipate along the estuary. Unexpectedly, there was no correlation between monthly chlorophyll-a variability inside and outside the Bay. However, at the annual scale Bay chlorophyll-a was significantly correlated with the Spring Transition Index (STI) that sets biological production supporting fish recruitment in the CCS. Wind forcing of the CCS shifted in the late 1990s when the STI advanced 40 days. This shift was followed, with lags of 1-3 years, by 3- to 19-fold increased abundances of five <span class="hlt">ocean</span>-produced demersal fish and crustaceans and 2.5-fold increase of summer chlorophyll-a in the Bay. These changes reflect a slow biological process of estuary-<span class="hlt">ocean</span> connectivity operating through the immigration of fish and crustaceans that prey on bivalves, reduce their grazing pressure, and allow phytoplankton biomass to build. We identified clear signals of climate-mediated <span class="hlt">oceanic</span> variability in this estuary and discovered that the response patterns vary with the process of connectivity and the timescale of <span class="hlt">ocean</span> variability. This result has important implications for managing nutrient inputs to estuaries connected to upwelling systems, and for assessing their responses to changing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70178587','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70178587"><span>Estuary-<span class="hlt">ocean</span> connectivity: Fast physics, slow biology</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Raimonet, Mélanie; Cloern, James E.</p> <p>2017-01-01</p> <p>Estuaries are connected to both land and <span class="hlt">ocean</span> so their physical, chemical, and biological dynamics are influenced by climate patterns over watersheds and <span class="hlt">ocean</span> <span class="hlt">basins</span>. We explored climate-driven <span class="hlt">oceanic</span> variability as a source of estuarine variability by comparing monthly time series of temperature and chlorophyll-a inside San Francisco Bay with those in <span class="hlt">adjacent</span> shelf waters of the California Current System (CCS) that are strongly responsive to wind-driven upwelling. Monthly temperature fluctuations inside and outside the Bay were synchronous, but their correlations weakened with distance from the <span class="hlt">ocean</span>. These results illustrate how variability of coastal water temperature (and associated properties such as nitrate and oxygen) propagates into estuaries through fast water exchanges that dissipate along the estuary. Unexpectedly, there was no correlation between monthly chlorophyll-a variability inside and outside the Bay. However, at the annual scale Bay chlorophyll-a was significantly correlated with the Spring Transition Index (STI) that sets biological production supporting fish recruitment in the CCS. Wind forcing of the CCS shifted in the late 1990s when the STI advanced 40 days. This shift was followed, with lags of 1–3 years, by 3- to 19-fold increased abundances of five <span class="hlt">ocean</span>-produced demersal fish and crustaceans and 2.5-fold increase of summer chlorophyll-a in the Bay. These changes reflect a slow biological process of estuary–<span class="hlt">ocean</span> connectivity operating through the immigration of fish and crustaceans that prey on bivalves, reduce their grazing pressure, and allow phytoplankton biomass to build. We identified clear signals of climate-mediated <span class="hlt">oceanic</span> variability in this estuary and discovered that the response patterns vary with the process of connectivity and the timescale of <span class="hlt">ocean</span> variability. This result has important implications for managing nutrient inputs to estuaries connected to upwelling systems, and for assessing their responses to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.9062K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.9062K"><span>Mooring-based long-term observation of oceanographic condition in the Chukchi Ses and Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kikuchi, Takashi; Itoh, Motoyo; Nishino, Shigeto; Watanabe, Eiji</p> <p>2015-04-01</p> <p>Changes of the Arctic <span class="hlt">Ocean</span> environment are well known as one of the most remarkable evidences of global warming, attracting social and public attentions as well as scientists'. However, to illustrate on-going changes and predict future condition of the Arctic marine environment, we still do not have enough knowledge of Arctic sea ice and marine environment. In particular, lack of observation data in winter, e.g., under sea ice, still remains a key issue for precise understanding of seasonal cycle on oceanographic condition in the Arctic <span class="hlt">Ocean</span>. Mooring-based observation is one of the most useful methods to collect year-long data in the Arctic <span class="hlt">Ocean</span>. We have been conducting long-term monitoring using mooring system in the Pacific sector of the Arctic <span class="hlt">Ocean</span>. Volume, heat, and freshwater fluxes through Barrow Canyon where is a major conduit of Pacific-origin water-masses into the Canada <span class="hlt">Basin</span> have been observed since 2000. We show from an analysis of the mooring results that volume flux through Barrow Canyon was about 60 % of Bering Strait volume flux. Averaged heat flux ranges from 0.9 to 3.07 TW, which could melt 88,000 to 300,000 km2 of 1m thick ice in the Canada <span class="hlt">Basin</span>, which likely contributed to sea ice retreat in the Pacific sector of the Arctic <span class="hlt">Ocean</span>. In winter, we found inter-annual variability in salinity related to coastal polynya activity in the Chukchi Sea. In collaboration with Distributed Biological Observatory (DBO) project, which is one of the tasks of Sustaining Arctic Observing Network (SAON), we also initiated year-long mooring observation in the Hope Valley of the southern Chukchi Sea since 2012. Interestingly, winter oceanographic conditions in the Hope Valley are greatly different between in 2012-2013 and in 2013-2014. We speculate that differences of sea ice freeze-up and coastal polynya activity in the southern Chukchi Sea cause significant difference of winter oceanographic condition. It suggests that recent sea ice reduction in the Pacific</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17752757','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17752757"><span>Arctic <span class="hlt">Ocean</span> Gravity Field Derived From ERS-1 Satellite Altimetry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Laxon, S; McAdoo, D</p> <p>1994-07-29</p> <p>The derivation of a marine gravity field from satellite altimetry over permanently ice-covered regions of the Arctic <span class="hlt">Ocean</span> provides much new geophysical information about the structure and development of the Arctic sea floor. The Arctic <span class="hlt">Ocean</span>, because of its remote location and perpetual ice cover, remains from a tectonic point of view the most poorly understood <span class="hlt">ocean</span> <span class="hlt">basin</span> on Earth. A gravity field has been derived with data from the ERS-1 radar altimeter, including permanently ice-covered regions. The gravity field described here clearly delineates sections of the Arctic <span class="hlt">Basin</span> margin along with the tips of the Lomonosov and Arctic mid-<span class="hlt">ocean</span> ridges. Several important tectonic features of the Amerasia <span class="hlt">Basin</span> are clearly expressed in this gravity field. These include the Mendeleev Ridge; the Northwind Ridge; details of the Chukchi Borderland; and a north-south trending, linear feature in the middle of the Canada <span class="hlt">Basin</span> that apparently represents an extinct spreading center that "died" in the Mesozoic. Some tectonic models of the Canada <span class="hlt">Basin</span> have proposed such a failed spreading center, but its actual existence and location were heretofore unknown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.1739F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.1739F"><span>Miocene-Recent sediment flux in the south-central Alaskan fore-arc <span class="hlt">basin</span> governed by flat-slab subduction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Finzel, Emily S.; Enkelmann, Eva</p> <p>2017-04-01</p> <p>The Cook Inlet in south-central Alaska contains the early Oligocene to Recent stratigraphic record of a fore-arc <span class="hlt">basin</span> <span class="hlt">adjacent</span> to a shallowly subducting <span class="hlt">oceanic</span> plateau. Our new measured stratigraphic sections and detrital zircon U-Pb geochronology and Hf isotopes from Neogene strata and modern rivers illustrate the effects of flat-slab subduction on the depositional environments, provenance, and subsidence in fore-arc sedimentary systems. During the middle Miocene, fluvial systems emerged from the eastern, western, and northern margins of the <span class="hlt">basin</span>. The axis of maximum subsidence was near the center of the <span class="hlt">basin</span>, suggesting equal contributions from subsidence drivers on both margins. By the late Miocene, the axis of maximum subsidence had shifted westward and fluvial systems originating on the eastern margin of the <span class="hlt">basin</span> above the flat-slab traversed the entire width of the <span class="hlt">basin</span>. These mud-dominated systems reflect increased sediment flux from recycling of accretionary prism strata. Fluvial systems with headwaters above the flat-slab region continued to cross the <span class="hlt">basin</span> during Pliocene time, but a change to sandstone-dominated strata with abundant volcanogenic grains signals a reactivation of the volcanic arc. The axis of maximum <span class="hlt">basin</span> subsidence during late Miocene to Pliocene time is parallel to the strike of the subducting slab. Our data suggest that the character and strike-orientation of the down-going slab may provide a fundamental control on the nature of depositional systems, location of dominant provenance regions, and areas of maximum subsidence in fore-arc <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MarGR.tmp...26D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MarGR.tmp...26D"><span>The crustal structure of the Enderby <span class="hlt">Basin</span>, East Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davis, Joshua K.; Lawver, Lawrence A.; Norton, Ian O.; Dalziel, Ian W. D.; Gahagan, Lisa M.</p> <p>2018-05-01</p> <p>The passive margin and <span class="hlt">ocean</span> crust of the Enderby <span class="hlt">Basin</span>, East Antarctica preserves a record of the breakup of East Gondwana. Using a suite of public domain geophysical data, we have examined and described the crustal morphology of the <span class="hlt">basin</span>. Based on our geophysical observations, we divide the Enderby <span class="hlt">Basin</span> into three distinct morphologic domains. The Eastern Domain demonstrates the most volcanic morphology of the <span class="hlt">basin</span>, with abundant seaward dipping reflector packages and anomalously thick <span class="hlt">oceanic</span> crust. These features suggest an early influence by the Kerguelen Hotspot on continental breakup within the domain. The Central Domain is characterized by two regions of <span class="hlt">oceanic</span> crust of varying morphology segregated by a high amplitude magnetic anomaly. Geophysical observations suggest that the basement directly inboard of this magnetic anomaly is composed of thin, rugged, and poorly structured, proto-<span class="hlt">oceanic</span> crust, similar in morphology to <span class="hlt">oceanic</span> crust formed at ultraslow/slow mid-<span class="hlt">ocean</span> ridged. Outboard of this anomaly, <span class="hlt">oceanic</span> crust appears to be well-structured and of normal thickness. We offer three, non-exclusive, explanations for the observed change in <span class="hlt">ocean</span> crustal structure: (1) melt production was initially low at the time of continental breakup, and the progressive decompression of the mantle led to a gradual increase in melt production and <span class="hlt">ocean</span> crust thickness, (2) melt production was initially low to due lower extension rates and that melt production increased following a change in spreading rate, (3) a change in spreading ridge geometry led to more effective seafloor spreading rate and concurrent increase in melt production. The Western Domain of the Enderby <span class="hlt">Basin</span> is characterized by abundant fracture zones and anomalously thin <span class="hlt">oceanic</span> crust. We believe these features arose as a geometric consequence of the originally oblique orientation of continental rifting relative to the extension direction within the domain. Together these observations suggest that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA610738','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA610738"><span>Estimation of the Barrier Layer Thickness in the Indian <span class="hlt">Ocean</span> Using Aquarius Salinity</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-07-08</p> <p>number of temperature and salinity measurements in <span class="hlt">ocean</span> <span class="hlt">basins</span> . In 2005, buoy coverage in the Indian <span class="hlt">Ocean</span> began meeting Argo program sampling...distribution of salinity in the Indian <span class="hlt">Ocean</span> is unique when compared to the other <span class="hlt">basins</span> with higher salinity in the western contrasted Journal of...eastern regions of the <span class="hlt">basin</span> (Figure 2). In the Arabian Sea, evaporation (E) greatly exceeds precipitation (P) resulting in high salinity (>36 PSU</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/2006AGUFM.U53A0024N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFM.U53A0024N"><span>Project SUMATRA: The Fore-arc <span class="hlt">Basin</span> System of Sumatra</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Neben, S.; Franke, D.; Gaedicke, C.; Ladage, S.; Berglar, K.; Damm, V.; Ehrhardt, A.; Heyde, I.; Schnabel, M.; Schreckenberger, B.</p> <p>2006-12-01</p> <p>The main scientific objective of the project SUMATRA is to determine or estimate the geological setting and evolution of the Sumatra fore-arc region. RV SONNE cruise SO189 Leg 1 was designed to investigate the architecture, sedimentary thickness, sedimentary evolution and subsidence history of the fore-arc <span class="hlt">basins</span> Siberut, Nias and Simeulue off Sumatra. During the cruise a total of 4375km of multichannel seismic (MCS), magnetics (M) and gravity (G) data were acquired and additional 990km with M and G alone. Along two lines with a total length of 390km refraction/wide-angle seismic experiments were carried out. 41 MCS lines cover as close grids the three fore- arc <span class="hlt">basins</span>. Five lines extend nearly orthogonal to the subduction front covering the whole subduction system from the <span class="hlt">adjacent</span> <span class="hlt">oceanic</span> plate, the trench and accretionary prism over the Outer Arc High to the fore-arc <span class="hlt">basins</span>. In the Simeulue <span class="hlt">Basin</span> it was possible to connect the seismic lines to three industry wells and to correlate the seismic horizons to the results from the wells. The Simeulue <span class="hlt">Basin</span> is divided into a northern and southern sub- <span class="hlt">basin</span>. The maximum thickness was determined to be 6s TWT. In the southern sub-<span class="hlt">basin</span> carbonate build-ups (which were already identified during the SEACAUSE project), bright spots and Bottom Simulating Reflectors (BSRs) are wide spread. The narrowest <span class="hlt">basin</span> surveyed was the Nias <span class="hlt">Basin</span>. As the Simeulue <span class="hlt">Basin</span> the Nias <span class="hlt">Basin</span> is divided into two sub-<span class="hlt">basins</span> which are separated by a structural high. Although the <span class="hlt">basin</span> has a maximum width of only 55km the maximum sediment thickness exceeds 5s TWT. The largest investigated fore-arc <span class="hlt">basin</span> is the Siberut <span class="hlt">Basin</span>. It extends over 550km and has a maximum width of 140km between Siberut and Sumatra. The maximum sediment thickness in this <span class="hlt">basin</span> is 4.8s TWT. The <span class="hlt">basin</span> geometry is uniform along its axis. At the <span class="hlt">basins</span> termination on the western side to the Outer Arc High the Mentawai Fault Zone could be traced. In the Siberut <span class="hlt">Basin</span> BSRs are</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70032994','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70032994"><span>Great <span class="hlt">Basin</span> paleontological database</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zhang, N.; Blodgett, R.B.; Hofstra, A.H.</p> <p>2008-01-01</p> <p>The U.S. Geological Survey has constructed a paleontological database for the Great <span class="hlt">Basin</span> physiographic province that can be served over the World Wide Web for data entry, queries, displays, and retrievals. It is similar to the web-database solution that we constructed for Alaskan paleontological data (www.alaskafossil.org). The first phase of this effort was to compile a paleontological bibliography for Nevada and portions of <span class="hlt">adjacent</span> states in the Great <span class="hlt">Basin</span> that has recently been completed. In addition, we are also compiling paleontological reports (Known as E&R reports) of the U.S. Geological Survey, which are another extensive source of l,egacy data for this region. Initial population of the database benefited from a recently published conodont data set and is otherwise focused on Devonian and Mississippian localities because strata of this age host important sedimentary exhalative (sedex) Au, Zn, and barite resources and enormons Carlin-type An deposits. In addition, these strata are the most important petroleum source rocks in the region, and record the transition from extension to contraction associated with the Antler orogeny, the Alamo meteorite impact, and biotic crises associated with global <span class="hlt">oceanic</span> anoxic events. The finished product will provide an invaluable tool for future geologic mapping, paleontological research, and mineral resource investigations in the Great <span class="hlt">Basin</span>, making paleontological data acquired over nearly the past 150 yr readily available over the World Wide Web. A description of the structure of the database and the web interface developed for this effort are provided herein. This database is being used ws a model for a National Paleontological Database (which we am currently developing for the U.S. Geological Survey) as well as for other paleontological databases now being developed in other parts of the globe. ?? 2008 Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.1598D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.1598D"><span>Intraplate compressional deformation in West-Congo and the Congo <span class="hlt">basin</span>: related to ridge-puch from the South Atlantic spreading ridge?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Delvaux, Damien; Everaerts, Michel; Kongota Isasi, Elvis; Ganza Bamulezi, Gloire</p> <p>2016-04-01</p> <p>After the break-up and separation of South America from Africa and the initiation of the South-Atlantic mid-<span class="hlt">oceanic</span> ridge in the Albian, at about 120 Ma, ridge-push forces started to build-up in the <span class="hlt">oceanic</span> lithosphere and were transmitted to the <span class="hlt">adjacent</span> continental plates. This is particularly well expressed in the passive margin and continental interior of Central Africa. According to the relations of Wiens and Stein (1985) between ridge-push forces and basal drag in function of the lithospheric age of <span class="hlt">oceanic</span> plates, the deviatoric stress reaches a compressional maximum between 50 and 100, Ma after the initiation of the spreading ridge, so broadly corresponding to the Paleocene in this case (~70-20 Ma). Earthquake focal mechanism data show that the West-Congo margin and a large part of the Congo <span class="hlt">basin</span> are still currently under compressional stresses with an horizontal compression parallel to the direction of the active transform fracture zones. We studied the fracture network along the Congo River in Kinshasa and Brazzaville which affect Cambrian sandstones and probably also the late Cretaceous-Paleocene sediments. Their brittle tectonic evolution is compatible with the buildup of ridge-push forces related to the South-Atlantic opening. Further inland, low-angle reverse faults are found affecting Jurassic to Middle Cretaceous cores from the Samba borehole in the Congo <span class="hlt">basin</span> and strike-slip movements are recorded as a second brittle phase in the Permian cores of the Dekese well, at the southern margin of the Congo <span class="hlt">basin</span>. An analysis of the topography and river network of the Congo <span class="hlt">basin</span> show the development of low-amplitude (50-100 m) long wavelengths (100-300 km) undulations that can be interpreted as lithospheric buckling in response to the compressional intraplate stress field generated by the Mid-Atlantic ridge-push. Wiens, D.A., Stein, S., 1985. Implications of <span class="hlt">oceanic</span> intraplate seismicity for plate stresses, driving forces and theology. Tectonophysics</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2012/3075/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2012/3075/"><span>Assessment of undiscovered oil and gas resources of the East Coast Mesozoic <span class="hlt">basins</span> of the Piedmont, Blue Ridge Thrust Belt, Atlantic Coastal Plain, and New England Provinces, 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>Milici, Robert C.; Coleman, James L.; Rowan, Elisabeth L.; Cook, Troy A.; Charpentier, Ronald R.; Kirschbaum, Mark A.; Klett, Timothy R.; Pollastro, Richard M.; Schenk, Christopher J.</p> <p>2012-01-01</p> <p>During the early opening of the Atlantic <span class="hlt">Ocean</span> in the Mesozoic Era, numerous extensional <span class="hlt">basins</span> formed along the eastern margin of the North American continent from Florida northward to New England and parts of <span class="hlt">adjacent</span> Canada. The <span class="hlt">basins</span> extend generally from the offshore Atlantic continental margin westward beneath the Atlantic Coastal Plain to the Appalachian Mountains. Using a geology-based assessment method, the U.S. Geological Survey estimated a mean undiscovered natural gas resource of 3,860 billion cubic feet and a mean undiscovered natural gas liquids resource of 135 million barrels in continuous accumulations within five of the East Coast Mesozoic <span class="hlt">basins</span>: the Deep River, Dan River-Danville, and Richmond <span class="hlt">basins</span>, which are within the Piedmont Province of North Carolina and Virginia; the Taylorsville <span class="hlt">basin</span>, which is almost entirely within the Atlantic Coastal Plain Province of Virginia and Maryland; and the southern part of the Newark <span class="hlt">basin</span> (herein referred to as the South Newark <span class="hlt">basin</span>), which is within the Blue Ridge Thrust Belt Province of New Jersey. The provinces, which contain these extensional <span class="hlt">basins</span>, extend across parts of Georgia, South Carolina, North Carolina, Virginia, Maryland, Delaware, Pennsylvania, New Jersey, New York, Connecticut, and Massachusetts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25273206','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25273206"><span>How well-connected is the surface of the global <span class="hlt">ocean</span>?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Froyland, Gary; Stuart, Robyn M; van Sebille, Erik</p> <p>2014-09-01</p> <p>The Ekman dynamics of the <span class="hlt">ocean</span> surface circulation is known to contain attracting regions such as the great <span class="hlt">oceanic</span> gyres and the associated garbage patches. Less well-known are the extents of the <span class="hlt">basins</span> of attractions of these regions and how strongly attracting they are. Understanding the shape and extent of the <span class="hlt">basins</span> of attraction sheds light on the question of the strength of connectivity of different regions of the <span class="hlt">ocean</span>, which helps in understanding the flow of buoyant material like plastic litter. Using short flow time trajectory data from a global <span class="hlt">ocean</span> model, we create a Markov chain model of the surface <span class="hlt">ocean</span> dynamics. The surface <span class="hlt">ocean</span> is not a conservative dynamical system as water in the <span class="hlt">ocean</span> follows three-dimensional pathways, with upwelling and downwelling in certain regions. Using our Markov chain model, we easily compute net surface upwelling and downwelling, and verify that it matches observed patterns of upwelling and downwelling in the real <span class="hlt">ocean</span>. We analyze the Markov chain to determine multiple attracting regions. Finally, using an eigenvector approach, we (i) identify the five major <span class="hlt">ocean</span> garbage patches, (ii) partition the <span class="hlt">ocean</span> into <span class="hlt">basins</span> of attraction for each of the garbage patches, and (iii) partition the <span class="hlt">ocean</span> into regions that demonstrate transient dynamics modulo the attracting garbage patches.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1615810K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1615810K"><span>Arctic and N Atlantic Crustal Thickness and <span class="hlt">Oceanic</span> Lithosphere Distribution from Gravity Inversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusznir, Nick; Alvey, Andy</p> <p>2014-05-01</p> <p>The <span class="hlt">ocean</span> <span class="hlt">basins</span> of the Arctic and N. Atlantic formed during the Mesozoic and Cenozoic as a series of distinct <span class="hlt">ocean</span> <span class="hlt">basins</span>, both small and large, leading to a complex distribution of <span class="hlt">oceanic</span> crust, thinned continental crust and rifted continental margins. The plate tectonic framework of this region was demonstrated by the pioneering work of Peter Ziegler in AAPG Memoir 43 " Evolution of the Arctic-North Atlantic and the Western Tethys" published in 1988. The spatial evolution of Arctic <span class="hlt">Ocean</span> and N Atlantic <span class="hlt">ocean</span> <span class="hlt">basin</span> geometry and bathymetry are critical not only for hydrocarbon exploration but also for understanding regional palaeo-oceanography and <span class="hlt">ocean</span> gateway connectivity, and its influence on global climate. Mapping crustal thickness and <span class="hlt">oceanic</span> lithosphere distribution represents a substantial challenge for the Polar Regions. Using gravity anomaly inversion we have produced comprehensive maps of crustal thickness and <span class="hlt">oceanic</span> lithosphere distribution for the Arctic and N Atlantic region, We determine Moho depth, crustal basement thickness, continental lithosphere thinning and <span class="hlt">ocean</span>-continent transition location using a 3D spectral domain gravity inversion method, which incorporates a lithosphere thermal gravity anomaly correction (Chappell & Kusznir 2008). Gravity anomaly and bathymetry data used in the gravity inversion are from the NGA (U) Arctic Gravity Project and IBCAO respectively; sediment thickness is from a new regional compilation. The resulting maps of crustal thickness and continental lithosphere thinning factor are used to determine continent-<span class="hlt">ocean</span> boundary location and the distribution of <span class="hlt">oceanic</span> lithosphere. Crustal cross-sections using Moho depth from the gravity inversion allow continent-<span class="hlt">ocean</span> transition structure to be determined and magmatic type (magma poor, "normal" or magma rich). Our gravity inversion predicts thin crust and high continental lithosphere thinning factors in the Eurasia, Canada, Makarov, Podvodnikov and Baffin <span class="hlt">Basins</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSAES..83...96E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSAES..83...96E"><span>Geometry and structure of the pull-apart <span class="hlt">basins</span> developed along the western South American-Scotia plate boundary (SW Atlantic <span class="hlt">Ocean</span>)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Esteban, F. D.; Tassone, A.; Isola, J. I.; Lodolo, E.; Menichetti, M.</p> <p>2018-04-01</p> <p>The South American-Scotia plate boundary is a left-lateral fault system which runs roughly E-W for more than 3000 km across the SW Atlantic <span class="hlt">Ocean</span> and the Tierra del Fuego Island, reaching to the west the southern Chile Trench. Analyses of a large dataset of single- and multi-channel seismic reflection profiles acquired offshore has allowed to map the trace of the plate boundary from Tierra del Fuego to the Malvinas Trough, a tectonic depression located in the eastern part of the fault system, and to reconstruct the shape and geometry of the <span class="hlt">basins</span> formed along the principal displacement zone of the fault system. Three main Neogene pull-apart <span class="hlt">basins</span> that range from 70 to 100 km in length, and from 12 to 22 km in width, have been identified along this segment of the plate boundary. These <span class="hlt">basins</span> have elongated shapes with their major axes parallel to the ENE-WSW direction of the fault zone. The sedimentary architecture and the infill geometry of the <span class="hlt">basins</span> suggest that they represent mostly strike-slip dominated transtension <span class="hlt">basins</span> which propagated from E to W. The <span class="hlt">basins</span> imaged by seismic data show in some cases geometrical and structural features linked to the possible reactivation of previous wedge-top <span class="hlt">basins</span> and inherited structures pertaining to the external front of the Magallanes fold-and-thrust compression belt, along which the South American-Scotia fault system has been superimposed. It is suggested that the sequence of the elongated <span class="hlt">basins</span> occur symmetrically to a thorough going strike-slip fault, in a left-stepping geometrical arrangement, in a manner similar to those <span class="hlt">basins</span> seen in other transcurrent environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013NatGe...6..223T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013NatGe...6..223T"><span>A Precambrian microcontinent in the Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torsvik, Trond H.; Amundsen, Hans; Hartz, Ebbe H.; Corfu, Fernando; Kusznir, Nick; Gaina, Carmen; Doubrovine, Pavel V.; Steinberger, Bernhard; Ashwal, Lewis D.; Jamtveit, Bjørn</p> <p>2013-03-01</p> <p>The Laccadive-Chagos Ridge and Southern Mascarene Plateau in the north-central and western Indian <span class="hlt">Ocean</span>, respectively, are thought to be volcanic chains formed above the Réunion mantle plume over the past 65.5 million years. Here we use U-Pb dating to analyse the ages of zircon xenocrysts found within young lavas on the island of Mauritius, part of the Southern Mascarene Plateau. We find that the zircons are either Palaeoproterozoic (more than 1,971 million years old) or Neoproterozoic (between 660 and 840 million years old). We propose that the zircons were assimilated from ancient fragments of continental lithosphere beneath Mauritius, and were brought to the surface by plume-related lavas. We use gravity data inversion to map crustal thickness and find that Mauritius forms part of a contiguous block of anomalously thick crust that extends in an arc northwards to the Seychelles. Using plate tectonic reconstructions, we show that Mauritius and the <span class="hlt">adjacent</span> Mascarene Plateau may overlie a Precambrian microcontinent that we call Mauritia. On the basis of reinterpretation of marine geophysical data, we propose that Mauritia was separated from Madagascar and fragmented into a ribbon-like configuration by a series of mid-<span class="hlt">ocean</span> ridge jumps during the opening of the Mascarene <span class="hlt">ocean</span> <span class="hlt">basin</span> between 83.5 and 61 million years ago. We suggest that the plume-related magmatic deposits have since covered Mauritia and potentially other continental fragments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040047277','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040047277"><span>Fresh Water Content Variability in the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hakkinen, Sirpa; Proshutinsky, Andrey</p> <p>2003-01-01</p> <p>Arctic <span class="hlt">Ocean</span> model simulations have revealed that the Arctic <span class="hlt">Ocean</span> has a <span class="hlt">basin</span> wide oscillation with cyclonic and anticyclonic circulation anomalies (Arctic <span class="hlt">Ocean</span> Oscillation; AOO) which has a prominent decadal variability. This study explores how the simulated AOO affects the Arctic <span class="hlt">Ocean</span> stratification and its relationship to the sea ice cover variations. The simulation uses the Princeton <span class="hlt">Ocean</span> Model coupled to sea ice. The surface forcing is based on NCEP-NCAR Reanalysis and its climatology, of which the latter is used to force the model spin-up phase. Our focus is to investigate the competition between <span class="hlt">ocean</span> dynamics and ice formation/melt on the Arctic <span class="hlt">basin</span>-wide fresh water balance. We find that changes in the Atlantic water inflow can explain almost all of the simulated fresh water anomalies in the main Arctic <span class="hlt">basin</span>. The Atlantic water inflow anomalies are an essential part of AOO, which is the wind driven barotropic response to the Arctic Oscillation (AO). The baroclinic response to AO, such as Ekman pumping in the Beaufort Gyre, and ice meldfreeze anomalies in response to AO are less significant considering the whole Arctic fresh water balance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PrOce.161...19H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PrOce.161...19H"><span>A window on the deep <span class="hlt">ocean</span>: The special value of <span class="hlt">ocean</span> bottom pressure for monitoring the large-scale, deep-<span class="hlt">ocean</span> circulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hughes, Chris W.; Williams, Joanne; Blaker, Adam; Coward, Andrew; Stepanov, Vladimir</p> <p>2018-02-01</p> <p>We show how, by focusing on bottom pressure measurements particularly on the global continental slope, it is possible to avoid the "fog" of mesoscale variability which dominates most observables in the deep <span class="hlt">ocean</span>. This makes it possible to monitor those aspects of the <span class="hlt">ocean</span> circulation which are most important for global scale <span class="hlt">ocean</span> variability and climate. We therefore argue that such measurements should be considered an important future component of the Global <span class="hlt">Ocean</span> Observing System, to complement the present open-<span class="hlt">ocean</span> and coastal elements. Our conclusions are founded on both theoretical arguments, and diagnostics from a fine-resolution <span class="hlt">ocean</span> model that has realistic amplitudes and spectra of mesoscale variability. These show that boundary pressure variations are coherent over along-slope distances of tens of thousands of kilometres, for several vertical modes. We illustrate the value of this in the model Atlantic, by determining the time for boundary and equatorial waves to complete a circuit of the northern <span class="hlt">basin</span> (115 and 205 days for the first and second vertical modes), showing how the boundary features compare with <span class="hlt">basin</span>-scale theoretical models, and demonstrating the ability to monitor the meridional overturning circulation using these boundary measurements. Finally, we discuss applicability to the real <span class="hlt">ocean</span> and make recommendations on how to make such measurements without contamination from instrumental drift.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2015/5175/sir20155175.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2015/5175/sir20155175.pdf"><span>Delineation of the Pahute Mesa–Oasis Valley groundwater <span class="hlt">basin</span>, Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fenelon, Joseph M.; Halford, Keith J.; Moreo, Michael T.</p> <p>2016-01-22</p> <p>This report delineates the Pahute Mesa–Oasis Valley (PMOV) groundwater <span class="hlt">basin</span>, where recharge occurs, moves downgradient, and discharges to Oasis Valley, Nevada. About 5,900 acre-feet of water discharges annually from Oasis Valley, an area of springs and seeps near the town of Beatty in southern Nevada. Radionuclides in groundwater beneath Pahute Mesa, an area of historical underground nuclear testing at the Nevada National Security Site, are believed to be migrating toward Oasis Valley. Delineating the boundary of the PMOV groundwater <span class="hlt">basin</span> is necessary to adequately assess the potential for transport of radionuclides from Pahute Mesa to Oasis Valley.The PMOV contributing area is defined based on regional water-level contours, geologic controls, and knowledge of <span class="hlt">adjacent</span> flow systems. The viability of this area as the contributing area to Oasis Valley and the absence of significant interbasin flow between the PMOV groundwater <span class="hlt">basin</span> and <span class="hlt">adjacent</span> <span class="hlt">basins</span> are shown regionally and locally. Regional constraints on the location of the contributing area boundary and on the absence of interbasin groundwater flow are shown by balancing groundwater discharges in the PMOV groundwater <span class="hlt">basin</span> and <span class="hlt">adjacent</span> <span class="hlt">basins</span> against available water from precipitation. Internal consistency for the delineated contributing area is shown by matching measured water levels, groundwater discharges, and transmissivities with simulated results from a single-layer, steady-state, groundwater-flow model. An alternative <span class="hlt">basin</span> boundary extending farther north than the final boundary was rejected based on a poor chloride mass balance and a large imbalance in the northern area between preferred and simulated recharge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSAES..84..351L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSAES..84..351L"><span>Imaging exhumed lower continental crust in the distal Jequitinhonha <span class="hlt">basin</span>, Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Loureiro, A.; Schnürle, P.; Klingelhöfer, F.; Afilhado, A.; Pinheiro, J.; Evain, M.; Gallais, F.; Dias, N. A.; Rabineau, M.; Baltzer, A.; Benabdellouahed, M.; Soares, J.; Fuck, R.; Cupertino, J. A.; Viana, A.; Matias, L.; Moulin, M.; Aslanian, D.; Vinicius Aparecido Gomes de Lima, M.; Morvan, L.; Mazé, J. P.; Pierre, D.; Roudaut-Pitel, M.; Rio, I.; Alves, D.; Barros Junior, P.; Biari, Y.; Corela, C.; Crozon, J.; Duarte, J. L.; Ducatel, C.; Falcão, C.; Fernagu, P.; Le Piver, D.; Mokeddem, Z.; Pelleau, P.; Rigoti, C.; Roest, W.; Roudaut, M.; Salsa Team</p> <p>2018-07-01</p> <p>Twelve combined wide-angle refraction and coincident multi-channel seismic profiles were acquired in the Jequitinhonha-Camamu-Almada, Jacuípe, and Sergipe-Alagoas <span class="hlt">basins</span>, NE Brazil, during the SALSA experiment in 2014. Profiles SL11 and SL12 image the Jequitinhonha <span class="hlt">basin</span>, perpendicularly to the coast, with 15 and 11 four-channel <span class="hlt">ocean</span>-bottom seismometers, respectively. Profile SL10 runs parallel to the coast, crossing profiles SL11 and SL12, imaging the proximal Jequitinhonha and Almada <span class="hlt">basins</span> with 17 <span class="hlt">ocean</span>-bottom seismometers. Forward modelling, combined with pre-stack depth migration to increase the horizontal resolution of the velocity models, indicates that sediment thickness varies between 3.3 km and 6.2 km in the distal <span class="hlt">basin</span>. Crustal thickness at the western edge of the profiles is of around 20 km, with velocity gradients indicating a continental origin. It decreases to less than 5 km in the distal <span class="hlt">basin</span>, with high seismic velocities and gradients, not compatible with normal <span class="hlt">oceanic</span> crust nor exhumed upper mantle. Typical <span class="hlt">oceanic</span> crust is never imaged along these about 200 km-long profiles and we propose that the transitional crust in the Jequitinhonha <span class="hlt">basin</span> is a made of exhumed lower continental crust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19890009730','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19890009730"><span>Multi-property modeling of <span class="hlt">ocean</span> <span class="hlt">basin</span> carbon fluxes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Volk, Tyler</p> <p>1988-01-01</p> <p>The objectives of this project were to elucidate the causal mechanisms in some of the most important features of the global <span class="hlt">ocean</span>/atomsphere carbon system. These included the interaction of physical and biological processes in the seasonal cycle of surface water pCo2, and links between productivity, surface chlorophyll, and the carbon cycle that would aid global modeling efforts. In addition, several other areas of critical scientific interest involving links between the marine biosphere and the global carbon cycle were successfully pursued; specifically, a possible relation between phytoplankton emitted DMS and climate, and a relation between the location of calcium carbonate burial in the <span class="hlt">ocean</span> and metamorphic source fluxes of CO2 to the atmosphere. Six published papers covering the following topics are summarized: (1) Mass extinctions, atmospheric sulphur and climatic warming at the K/T boundary; (2) Sensitivity of climate and atmospheric CO2 to deep-<span class="hlt">ocean</span> and shallow-<span class="hlt">ocean</span> carbonate burial; (3) Controls on CO2 sources and sinks in the earthscale surface <span class="hlt">ocean</span>; (4) pre-anthropogenic, earthscale patterns of delta pCO2 between <span class="hlt">ocean</span> and atmosphere; (5) Effect on atmospheric CO2 from seasonal variations in the high latitude <span class="hlt">ocean</span>; and (6) Limitations or relating <span class="hlt">ocean</span> surface chlorophyll to productivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70116459','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70116459"><span>Event sedimentation in low-latitude deep-water carbonate <span class="hlt">basins</span>, Anegada passage, northeast Caribbean</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Chaytor, Jason D.; ten Brink, Uri S.</p> <p>2015-01-01</p> <p>The Virgin Islands and Whiting <span class="hlt">basins</span> in the Northeast Caribbean are deep, structurally controlled depocentres partially bound by shallow-water carbonate platforms. Closed <span class="hlt">basins</span> such as these are thought to document earthquake and hurricane events through the accumulation of event layers such as debris flow and turbidity current deposits and the internal deformation of deposited material. Event layers in the Virgin Islands and Whiting <span class="hlt">basins</span> are predominantly thin and discontinuous, containing varying amounts of reef- and slope-derived material. Three turbidites/sandy intervals in the upper 2 m of sediment in the eastern Virgin Islands <span class="hlt">Basin</span> were deposited between ca. 2000 and 13 600 years ago, but do not extend across the <span class="hlt">basin</span>. In the central and western Virgin Islands <span class="hlt">Basin</span>, a structureless clay-rich interval is interpreted to be a unifite. Within the Whiting <span class="hlt">Basin</span>, several discontinuous turbidites and other sand-rich intervals are primarily deposited in base of slope fans. The youngest of these turbidites is ca. 2600 years old. Sediment accumulation in these <span class="hlt">basins</span> is low (−1) for <span class="hlt">basin</span> <span class="hlt">adjacent</span> to carbonate platform, possibly due to limited sediment input during highstand sea-level conditions, sediment trapping and/or cohesive <span class="hlt">basin</span> walls. We find no evidence of recent sediment transport (turbidites or debris flows) or sediment deformation that can be attributed to the ca. M7.2 1867 Virgin Islands earthquake whose epicentre was located on the north wall of the Virgin Islands <span class="hlt">Basin</span> or to recent hurricanes that have impacted the region. The lack of significant appreciable pebble or greater size carbonate material in any of the available cores suggests that submarine landslide and <span class="hlt">basin</span>-wide blocky debris flows have not been a significant mechanism of <span class="hlt">basin</span> margin modification in the last several thousand years. Thus, <span class="hlt">basins</span> such as those described here may be poor recorders of past natural hazards, but may provide a long-term record of past oceanographic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.2491Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.2491Z"><span>Variability of interleaving structure of Atlantic Water during its propagation along the Eurasian <span class="hlt">basin</span> (Arctic <span class="hlt">Ocean</span>) continental margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhurbas, Nataliya; Kuzmina, Natalia; Lyzhkov, Dmitry; Ostapchuk, Alexey</p> <p>2017-04-01</p> <p>In order to give detailed description of the interleaving structure in the Eurasian <span class="hlt">basin</span> results of observations carried out during NABOS 2008 and Polarstern cruise in 1996 were analyzed. The study was focused on interleaving parameters (structure and vertical scale of intrusions) variability in the upper (150-300 meters) and intermediate (300-700 meters) layers of the <span class="hlt">ocean</span>. Based on θ,S/θ,σ-diagrams (θ, S and σ are the potential temperature, salinity and potential density, correspondingly) analysis two main results were obtained. First of all it was shown that intrusive layers carried by the mean current along the Eurasian <span class="hlt">Basin</span> continental margin become deeper relatively isopycnals and thus stimulate ventilation of pycnocline. Second, the area in Eurasian <span class="hlt">Basin</span> thermocline was found where intrusive layers of large and small scale were absent. This distinctive feature can be explained by intensive mixing between two branches of Atlantic Water, one of which propagates along Eurasian <span class="hlt">basin</span> continental margin and the other spreads across the <span class="hlt">basin</span> due to large scale interleaving processes. Among others, one of the possible methods of integral estimation of Atlantic water masses heat and salt contents variations during their expansion along <span class="hlt">basin</span> continental margin was proposed. Thus it is reasonable to assess variation of square under the θ(S)-diagrams, which illustrate the data obtained from two CTD-stations located on diametrically opposite sides of Eurasian <span class="hlt">Basin</span>, taking 0.5°C isotherm as a reference value. For verification of the introduced approach the estimates of heat and salt contents variations were made by different methods. Detailed discussion of the results is presented. Work was supported by the Russian Foundation for Basic Research (Grant No 15-05-01479-a).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5069527','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5069527"><span>Impact of hydrothermalism on the <span class="hlt">ocean</span> iron cycle</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Resing, Joseph</p> <p>2016-01-01</p> <p>As the iron supplied from hydrothermalism is ultimately ventilated in the iron-limited Southern <span class="hlt">Ocean</span>, it plays an important role in the <span class="hlt">ocean</span> biological carbon pump. We deploy a set of focused sensitivity experiments with a state of the art global model of the <span class="hlt">ocean</span> to examine the processes that regulate the lifetime of hydrothermal iron and the role of different ridge systems in governing the hydrothermal impact on the Southern <span class="hlt">Ocean</span> biological carbon pump. Using GEOTRACES section data, we find that stabilization of hydrothermal iron is important in some, but not all regions. The impact on the Southern <span class="hlt">Ocean</span> biological carbon pump is dominated by poorly explored southern ridge systems, highlighting the need for future exploration in this region. We find inter-<span class="hlt">basin</span> differences in the isopycnal layer onto which hydrothermal Fe is supplied between the Atlantic and Pacific <span class="hlt">basins</span>, which when combined with the inter-<span class="hlt">basin</span> contrasts in oxidation kinetics suggests a muted influence of Atlantic ridges on the Southern <span class="hlt">Ocean</span> biological carbon pump. Ultimately, we present a range of processes, operating at distinct scales, that must be better constrained to improve our understanding of how hydrothermalism affects the <span class="hlt">ocean</span> cycling of iron and carbon. This article is part of the themed issue ‘Biological and climatic impacts of <span class="hlt">ocean</span> trace element chemistry’. PMID:29035256</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29035256','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29035256"><span>Impact of hydrothermalism on the <span class="hlt">ocean</span> iron cycle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tagliabue, Alessandro; Resing, Joseph</p> <p>2016-11-28</p> <p>As the iron supplied from hydrothermalism is ultimately ventilated in the iron-limited Southern <span class="hlt">Ocean</span>, it plays an important role in the <span class="hlt">ocean</span> biological carbon pump. We deploy a set of focused sensitivity experiments with a state of the art global model of the <span class="hlt">ocean</span> to examine the processes that regulate the lifetime of hydrothermal iron and the role of different ridge systems in governing the hydrothermal impact on the Southern <span class="hlt">Ocean</span> biological carbon pump. Using GEOTRACES section data, we find that stabilization of hydrothermal iron is important in some, but not all regions. The impact on the Southern <span class="hlt">Ocean</span> biological carbon pump is dominated by poorly explored southern ridge systems, highlighting the need for future exploration in this region. We find inter-<span class="hlt">basin</span> differences in the isopycnal layer onto which hydrothermal Fe is supplied between the Atlantic and Pacific <span class="hlt">basins</span>, which when combined with the inter-<span class="hlt">basin</span> contrasts in oxidation kinetics suggests a muted influence of Atlantic ridges on the Southern <span class="hlt">Ocean</span> biological carbon pump. Ultimately, we present a range of processes, operating at distinct scales, that must be better constrained to improve our understanding of how hydrothermalism affects the <span class="hlt">ocean</span> cycling of iron and carbon.This article is part of the themed issue 'Biological and climatic impacts of <span class="hlt">ocean</span> trace element chemistry'. © 2016 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://fl.water.usgs.gov/Abstracts/wri01_4230_knochenmus.html','USGSPUBS'); return false;" href="http://fl.water.usgs.gov/Abstracts/wri01_4230_knochenmus.html"><span>Hydrology of the coastal springs ground-water <span class="hlt">basin</span> and <span class="hlt">adjacent</span> parts of Pasco, Hernando, and Citrus Counties, 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>Knochenmus, Lari A.; Yobbi, Dann K.</p> <p>2001-01-01</p> <p>The coastal springs in Pasco, Hernando, and Citrus Counties, Florida consist of three first-order magnitude springs and numerous smaller springs, which are points of substantial ground-water discharge from the Upper Floridan aquifer. Spring flow is proportional to the water-level altitude in the aquifer and is affected primarily by the magnitude and timing of rainfall. Ground-water levels in 206 Upper Floridan aquifer wells, and surface-water stage, flow, and specific conductance of water from springs at 10 gaging stations were measured to define the hydrologic variability (temporally and spatially) in the Coastal Springs Ground-Water <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> parts of Pasco, Hernando, and Citrus Counties. Rainfall at 46 stations and ground-water withdrawals for three counties, were used to calculate water budgets, to evaluate long-term changes in hydrologic conditions, and to evaluate relations among the hydrologic components. Predictive equations to estimate daily spring flow were developed for eight gaging stations using regression techniques. Regression techniques included ordinary least squares and multiple linear regression techniques. The predictive equations indicate that ground-water levels in the Upper Floridan aquifer are directly related to spring flow. At tidally affected gaging stations, spring flow is inversely related to spring-pool altitude. The springs have similar seasonal flow patterns throughout the area. Water-budget analysis provided insight into the relative importance of the hydrologic components expected to influence spring flow. Four water budgets were constructed for small ground-water <span class="hlt">basins</span> that form the Coastal Springs Ground-Water <span class="hlt">Basin</span>. Rainfall averaged 55 inches per year and was the only source of inflow to the <span class="hlt">Basin</span>. The pathways for outflow were evapotranspiration (34 inches per year), runoff by spring flow (8 inches per year), ground-water outflow from upward leakage (11 inches per year), and ground-water withdrawal (2 inches per year</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GBioC..31..515E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GBioC..31..515E"><span>A global <span class="hlt">ocean</span> climatology of preindustrial and modern <span class="hlt">ocean</span> δ13C</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eide, Marie; Olsen, Are; Ninnemann, Ulysses S.; Johannessen, Truls</p> <p>2017-03-01</p> <p>We present a global <span class="hlt">ocean</span> climatology of dissolved inorganic carbon δ13C (‰) corrected for the 13C-Suess effect, preindustrial δ13C. This was constructed by first using Olsen and Ninnemann's (2010) back-calculation method on data from 25 World <span class="hlt">Ocean</span> Circulation Experiment cruises to reconstruct the preindustrial δ13C on sections spanning all major <span class="hlt">oceans</span>. Next, we developed five multilinear regression equations, one for each major <span class="hlt">ocean</span> <span class="hlt">basin</span>, which were applied on the World <span class="hlt">Ocean</span> Atlas data to construct the climatology. This reveals the natural δ13C distribution in the global <span class="hlt">ocean</span>. Compared to the modern distribution, the preindustrial δ13C spans a larger range of values. The maxima, of up to 1.8‰, occurs in the subtropical gyres of all <span class="hlt">basins</span>, in the upper and intermediate waters of the North Atlantic, as well as in mode waters with a Southern <span class="hlt">Ocean</span> origin. Particularly strong gradients occur at intermediate depths, revealing a strong potential for using δ13C as a tracer for changes in water mass geometry at these levels. Further, we identify a much tighter relationship between δ13C and apparent oxygen utilization (AOU) than between δ13C and phosphate. This arises because, in contrast to phosphate, AOU and δ13C are both partly reset when waters are ventilated in the Southern <span class="hlt">Ocean</span> and underscore that δ13C is a highly robust proxy for past changes in <span class="hlt">ocean</span> oxygen content and <span class="hlt">ocean</span> ventilation. Our global preindustrial δ13C climatology is openly accessible and can be used, for example, for improved model evaluation and interpretation of sediment δ13C records.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70177924','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70177924"><span>Sources, distributions and dynamics of dissolved organic matter in the Canada and Makarov <span class="hlt">Basins</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>Shen, Yuan; Benner, Ronald; Robbins, Lisa L.; Wynn, Jonathan</p> <p>2016-01-01</p> <p>A comprehensive survey of dissolved organic carbon (DOC) and chromophoric dissolved organic matter (CDOM) was conducted in the Canada and Makarov <span class="hlt">Basins</span> and <span class="hlt">adjacent</span> seas during 2010–2012 to investigate the dynamics of dissolved organic matter (DOM) in the Arctic <span class="hlt">Ocean</span>. Sources and distributions of DOM in polar surface waters were very heterogeneous and closely linked to hydrological conditions. Canada <span class="hlt">Basin</span> surface waters had relatively low DOC concentrations (69 ± 6 μmol L−1), CDOM absorption (a325: 0.32 ± 0.07 m−1) and CDOM-derived lignin phenols (3 ± 0.4 nmol L−1), and high spectral slope values (S275–295: 31.7 ± 2.3 μm−1), indicating minor terrigenous inputs and evidence of photochemical alteration in the Beaufort Gyre. By contrast, surface waters of the Makarov <span class="hlt">Basin</span> had elevated DOC (108 ± 9 μmol L−1) and lignin phenol concentrations (15 ± 3 nmol L−1), high a325 values (1.36 ± 0.18 m−1), and low S275–295 values (22.8 ± 0.8 μm−1), indicating pronounced Siberian river inputs associated with the Transpolar Drift and minor photochemical alteration. Observations near the Mendeleev Plain suggested limited interactions of the Transpolar Drift with Canada <span class="hlt">Basin</span> waters, a scenario favoring export of Arctic DOM to the North Atlantic. The influence of sea-ice melt on DOM was region-dependent, resulting in an increase (Beaufort Sea), a decrease (Bering-Chukchi Seas), and negligible change (deep <span class="hlt">basins</span>) in surface DOC concentrations and a325 values. Halocline structures differed between <span class="hlt">basins</span>, but the Canada <span class="hlt">Basin</span> upper halocline and Makarov <span class="hlt">Basin</span> halocline were comparable in their average DOC (65–70 μmol L−1) and lignin phenol concentrations (3–4 nmol L−1) and S275–295 values (22.9–23.7 μm−1). Deep-water DOC concentrations decreased by 6–8 μmol L−1 with increasing depth, water mass age, nutrient concentrations, and apparent oxygen utilization. Maximal estimates of DOC degradation rates (0.036–0.039 μmol L−1</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/1983JGR....88.9341B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1983JGR....88.9341B"><span>Sediment sound velocities from Sonobuoys: Sunda Trench and forearc <span class="hlt">basins</span>, Nicobar and Central Bengal Fans, and Andaman Sea <span class="hlt">Basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bachman, Richard T.; Hamilton, Edwin L.; Curray, Joseph R.</p> <p>1983-11-01</p> <p>Supplement is available with entire article on microfiche. Order from American Geophysical Union, 2000 Florida Avenue, N.W., Washington, DC 20009. Document B83-007; $2.50. Payment must accompany order. Measurements of mean sound velocities in the first, largely unlithified layers in the seafloor were made using the sonobuoy technique in several areas in the northern Indian <span class="hlt">Ocean</span>. Older measurements were added to new measurements, and regressions for mean and instantaneous velocity versus one-way travel time of sound are presented for the central Bengal Fan, the central Andaman Sea <span class="hlt">Basin</span>, the Nicobar Fan, and the Sunda Trench. New data and regression equations are presented for the Mergui-north Sumatra <span class="hlt">Basin</span> and for four forearc <span class="hlt">basins</span> between Sumatra and Java and the Sunda Trench. Minimum velocity gradients were found in those areas where sedimentation rates were high, and sediments have accumulated in thick sections which have not had time to fully consolidate (porosity in the top of the sediment section has not been fully reduced under overburden pressure). These minimum velocity gradients (just under the seafloor) were found in the four forearc <span class="hlt">basins</span> where they ranged from 0.34 s-1 to 0.84 s-1 with an average of 0.58 s-1. The near-surface velocity gradient in the Sunda Trench was 1.33 s-1, but was higher in the <span class="hlt">adjacent</span>, fossil Nicobar Fan (1.62 s-1). In the surface of the Bengal Fan the velocity gradient was low in the upper fan (0.86 s-1), high in the central fan (1.94 s-1), and again lower in the southern fan (1.18 s-1), which may support sedimentation models calling for bypassing of the central fan and higher rates of accumulation on the southern fan.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.T11A2290C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.T11A2290C"><span>Seismic Imaging Reveals Deep-Penetrating Fault Planes in the Wharton <span class="hlt">Basin</span> <span class="hlt">Oceanic</span> Mantle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carton, H. D.; Singh, S. C.; Dyment, J.; Hananto, N. D.; Chauhan, A.</p> <p>2011-12-01</p> <p>We present images from a deep multi-channel seismic reflection survey acquired in 2006 over the <span class="hlt">oceanic</span> lithosphere of the Wharton <span class="hlt">Basin</span> offshore northern Sumatra, NW of Simeulue island. The main ~230-km long seismic profile is roughly parallel to the trench at ~32-66 km distance from the subduction front and crosses (at oblique angles to both flow line and isochron directions) an entire segment of 55-57 my-old fast-spread crust formed at the extinct Wharton spreading center, as well as two bounding ~N5°E trending fracture zones near its extremities; complementary data is provided by the <span class="hlt">oceanic</span> portions of two margin-crossing profiles on either side shot during the same survey. This high-quality, 12-km streamer dataset acquired for deep reflection imaging (10000 cu in tuned airgun array and 15-m source and streamer depths) reveals the presence of mostly SE-dipping (20 to 40 degrees dip) events cutting across and extending below the <span class="hlt">oceanic</span> Moho, down to a maximum depth below seafloor of ~37 km, at ~5 km spacing along the trench-parallel profile. Similar dipping mantle events are imaged on the <span class="hlt">oceanic</span> portion of another long-offset profile acquired in 2009 offshore central Sumatra south of Pagai island, which will also be presented. Such events are unlikely to be imaging artefacts of the 2D acquisition, such as out-of-plane energy originating from sharp, buried basement reliefs trending obliquely to the profile. Due to their geometry, they do not seem to be associated with plate bending at the trench outer-rise, which has a relatively modest expression at the seafloor and within the incoming sedimentary section north of the Simeulue elbow. We propose that these deep-penetrating dipping reflectors are fossil fault planes formed due to compressive stresses at the beginning of the continent-continent collision between India and Eurasia, the early stages of which were responsible for the cessation of seafloor spreading at the Wharton ridge at ca 40 Ma.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22222749','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22222749"><span>Changing Arctic <span class="hlt">Ocean</span> freshwater pathways.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Morison, James; Kwok, Ron; Peralta-Ferriz, Cecilia; Alkire, Matt; Rigor, Ignatius; Andersen, Roger; Steele, Mike</p> <p>2012-01-04</p> <p>Freshening in the Canada <span class="hlt">basin</span> of the Arctic <span class="hlt">Ocean</span> began in the 1990s and continued to at least the end of 2008. By then, the Arctic <span class="hlt">Ocean</span> might have gained four times as much fresh water as comprised the Great Salinity Anomaly of the 1970s, raising the spectre of slowing global <span class="hlt">ocean</span> circulation. Freshening has been attributed to increased sea ice melting and contributions from runoff, but a leading explanation has been a strengthening of the Beaufort High--a characteristic peak in sea level atmospheric pressure--which tends to accelerate an anticyclonic (clockwise) wind pattern causing convergence of fresh surface water. Limited observations have made this explanation difficult to verify, and observations of increasing freshwater content under a weakened Beaufort High suggest that other factors must be affecting freshwater content. Here we use observations to show that during a time of record reductions in ice extent from 2005 to 2008, the dominant freshwater content changes were an increase in the Canada <span class="hlt">basin</span> balanced by a decrease in the Eurasian <span class="hlt">basin</span>. Observations are drawn from satellite data (sea surface height and <span class="hlt">ocean</span>-bottom pressure) and in situ data. The freshwater changes were due to a cyclonic (anticlockwise) shift in the <span class="hlt">ocean</span> pathway of Eurasian runoff forced by strengthening of the west-to-east Northern Hemisphere atmospheric circulation characterized by an increased Arctic Oscillation index. Our results confirm that runoff is an important influence on the Arctic <span class="hlt">Ocean</span> and establish that the spatial and temporal manifestations of the runoff pathways are modulated by the Arctic Oscillation, rather than the strength of the wind-driven Beaufort Gyre circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018IJEaS.tmp...50I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018IJEaS.tmp...50I"><span>Genesis of Central Indian <span class="hlt">Ocean</span> <span class="hlt">basin</span> seamounts: morphological, petrological, and geochemical evidence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Iyer, Sridhar D.; Amonkar, Ankeeta Ashok; Das, Pranab</p> <p>2018-04-01</p> <p>We present the petrological investigation carried out of the seamounts located between water depths of 4300 and 5385 m in the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB). The seamounts have variable shapes (conical and elongated) and heights (625-1200 m). The basalts have a glassy veneer that forms the outer rind, while the holocrystalline interior shows variable textures. The basalts are plagioclase phyric and compositionally have low FeO* (8.0-10.5 wt%) and TiO2 (1.3-2.0 wt%), and variable K2O (0.1-1.0 wt%) contents and are slightly enriched in the light rare-earth elements. These characteristics are similar to the basalts from the CIOB seafloor and the Central Indian and Southeast Indian Ridges. These facts attest to the simultaneous formation of the CIOB seafloor and associated seamounts that shared a common source between 56 and 51 Ma when the spreading (half) rate was 95 mm/year. Similar to the East Pacific Rise (EPR), the source melt was perhaps ferrobasalts which over a period of time fractionated to N-MORB during the emplacement of the seamounts. The production of the seamounts may have involved a periodic tapping of a regularly replenished and shallow seated source melt. These basalts from the older seamounts of the CIOB are analogous to their present-day counterparts that form at the fast-spreading EPR and other locales in the world <span class="hlt">oceans</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880005970','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880005970"><span>On estimating the <span class="hlt">basin</span>-scale <span class="hlt">ocean</span> circulation from satellite altimetry. Part 1: Straightforward spherical harmonic expansion</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Tai, Chang-Kou</p> <p>1988-01-01</p> <p>Direct estimation of the absolute dynamic topography from satellite altimetry has been confined to the largest scales (basically the <span class="hlt">basin</span>-scale) owing to the fact that the signal-to-noise ratio is more unfavorable everywhere else. But even for the largest scales, the results are contaminated by the orbit error and geoid uncertainties. Recently a more accurate Earth gravity model (GEM-T1) became available, providing the opportunity to examine the whole question of direct estimation under a more critical limelight. It is found that our knowledge of the Earth's gravity field has indeed improved a great deal. However, it is not yet possible to claim definitively that our knowledge of the <span class="hlt">ocean</span> circulation has improved through direct estimation. Yet, the improvement in the gravity model has come to the point that it is no longer possible to attribute the discrepancy at the <span class="hlt">basin</span> scales between altimetric and hydrographic results as mostly due to geoid uncertainties. A substantial part of the difference must be due to other factors; i.e., the orbit error, or the uncertainty of the hydrographically derived dynamic topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T22B..02U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T22B..02U"><span>Breaching of strike-slip faults and flooding of pull-apart <span class="hlt">basins</span> to form the southern Gulf of California seaway from 8 to 6 Ma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Umhoefer, P. J.; Skinner, L. A.; Oskin, M. E.; Dorsey, R. J.; Bennett, S. E. K.; Darin, M. H.</p> <p>2017-12-01</p> <p>Studies from multiple disciplines delineate the development of the oblique-divergent Pacific - North America plate boundary in the southern Gulf of California. Integration of onshore data from the Loreto - Santa Rosalia margin with offshore data from the Pescadero, Farallon, and Guaymas <span class="hlt">basins</span> provides a detailed geologic history. Our GIS-based paleotectonic maps of the plate boundary from 9 to 6 Ma show that evolution of pull-apart <span class="hlt">basins</span> led to the episodic northwestward encroachment of the Gulf of California seaway. Because <span class="hlt">adjacent</span> pull-apart <span class="hlt">basins</span> commonly have highlands between them, juxtaposition of <span class="hlt">adjacent</span> <span class="hlt">basin</span> lows during translation and pull apart lengthening played a critical role in seaway flooding. Microfossils and volcanic units date the earliest marine deposits at 9(?) - 8 Ma at the mouth of the Gulf. By ca. 8 Ma, the seaway had flooded north to the Pescadero <span class="hlt">basin</span>, while the Loreto fault and the related fault-termination <span class="hlt">basin</span> was proposed to have formed along strike at the plate margin. East of Loreto <span class="hlt">basin</span>, a short topographic barrier between the Pescadero and Farallon pull-apart <span class="hlt">basins</span> suggests that the Farallon <span class="hlt">basin</span> was either a terrestrial <span class="hlt">basin</span>, or if breaching occurred, it may contain 8 Ma salt or marine deposits. This early southern seaway formed along a series of pull-apart <span class="hlt">basins</span> within a narrow belt of transtension structurally similar to the modern Walker Lane in NV and CA. At ca. 7 Ma, a series of marine incursions breached a 75-100 km long transtensional fault barrier between the Farallon and Guaymas <span class="hlt">basins</span> offshore Bahía Concepción. Repeated breaching events and the isolation of the Guaymas <span class="hlt">basin</span> in a subtropical setting formed a 2 km-thick salt deposit imaged in offshore seismic data, and thin evaporite deposits in the onshore Santa Rosalia <span class="hlt">basin</span>. Lengthening of the Guaymas, Yaqui, and Tiburon <span class="hlt">basins</span> caused breaches of the intervening Guaymas and Tiburón transforms by 6.5-6.3 Ma, forming a permanent 1500 km-long marine seaway</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006Geo....34..197C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006Geo....34..197C"><span>Feast to famine: Sediment supply control on Laramide <span class="hlt">basin</span> fill</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carroll, Alan R.; Chetel, Lauren M.; Elliot Smith, M.</p> <p>2006-03-01</p> <p>Erosion of Laramide-style uplifts in the western United States exerted an important first-order influence on Paleogene sedimentation by controlling sediment supply rates to <span class="hlt">adjacent</span> closed <span class="hlt">basins</span>. During the latest Cretaceous through Paleocene, these uplifts exposed thick intervals of mud-rich Upper Cretaceous foreland <span class="hlt">basin</span> fill, which was quickly eroded and redeposited. Cretaceous sedimentary lithologies dominate Paleocene conglomerate clast compositions, and the volume of eroded foreland <span class="hlt">basin</span> strata is approximately twice the volume of preserved Paleocene <span class="hlt">basin</span> fill. As a result of this sediment oversupply, clastic alluvial and paludal facies dominate Paleocene strata, and are associated with relatively shallow and ephemeral freshwater lake facies. In contrast, large, long-lived, carbonate-producing lakes occupied several of the <span class="hlt">basins</span> during the Eocene. Basement-derived clasts (granite, quartzite, and other metamorphic rocks) simultaneously became abundant in lower Eocene conglomerate. We propose that Eocene lakes developed primarily due to exposure of erosion-resistant lithologies within cores of Laramide uplifts. The resultant decrease in erosion rate starved <span class="hlt">adjacent</span> <span class="hlt">basins</span> of sediment, allowing the widespread and prolonged deposition of organic-rich lacustrine mudstone. These observations suggest that geomorphic evolution of the surrounding landscape should be considered as a potentially important influence on sedimentation in many other interior <span class="hlt">basins</span>, in addition to more conventionally interpreted tectonic and climatic controls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930005782&hterms=McDougall&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DMcDougall','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930005782&hterms=McDougall&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3DMcDougall"><span><span class="hlt">Ocean</span> transport and variability studies of the South Pacific, Southern, and Indian <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Church, John A.; Cresswell, G. R.; Nilsson, C. S.; Mcdougall, T. J.; Coleman, R.; Rizos, C.; Penrose, J.; Hunter, J. R.; Lynch, M. J.</p> <p>1991-01-01</p> <p>The objectives of this study are to analyze <span class="hlt">ocean</span> dynamics in the western South Pacific and the <span class="hlt">adjacent</span> Southern <span class="hlt">Ocean</span> and the eastern Indian <span class="hlt">Ocean</span>. Specifically, our objectives for these three regions are, for the South Pacific <span class="hlt">Ocean</span>: (1) To estimate the volume transport of the east Australian Current (EAC) along the Australian coast and in the Tasman Front, and to estimate the time variability (on seasonal and interannual time scales) of this transport. (2) To contribute to estimating the meridional heat and freshwater fluxes (and their variability) at about 30 deg S. Good estimates of the transport in the western boundary current are essential for accurate estimates of these fluxes. (3) To determine how the EAC transport (and its extension, the Tasman Front and the East Auckland Current) closes the subtropical gyre of the South Pacific and to better determine the structure at the confluence of this current and the Antarctic Circumpolar Current. (4) To examine the structure and time variability of the circulation in the western South Pacific and the <span class="hlt">adjacent</span> Southern <span class="hlt">Ocean</span>, particularly at the Tasman Front. For the Indian <span class="hlt">Ocean</span>: (5) To study the seasonal interannual variations in the strength of the Leeuwin Current. (6) To monitor the Pacific-Indian <span class="hlt">Ocean</span> throughflow and the South Equatorial and the South Java Currents between northwest Australia and Indonesia. (7) To study the processes that form the water of the permanent <span class="hlt">oceanic</span> thermocline and, in particular, the way in which new thermocline water enters the permanent thermocline in late winter and early spring as the mixed layer restratifies. For the Southern <span class="hlt">Ocean</span>: (8) To study the mesoscale and meridional structure of the Southern <span class="hlt">Ocean</span> between 150 deg E and 170 deg E; in particular, to describe the Antarctic frontal system south of Tasmania and determine its interannual variability; to estimate the exchanges of heat, salt, and other properties between the Indian and Pacific <span class="hlt">Oceans</span>; and to investigate the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005AGUFMOS43B..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005AGUFMOS43B..02H"><span>An <span class="hlt">Ocean</span> <span class="hlt">Basin</span> of Dirt? Using Molecular Biomarkers and Radiocarbon to Identify Organic Carbon Sources and their Preservation in the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harvey, H.; Belicka, L. L.</p> <p>2005-12-01</p> <p>In the modern Arctic <span class="hlt">Ocean</span>, primary production in waters over the broad continental shelves and under ice contributes an estimated 250 Mt/yr of POC to Arctic waters. The delivery of terrestrial material from large rivers, ice transport and through coastal erosion adds at least an additional 12 Mt/yr of POC. Although the marine organic carbon signal in Arctic <span class="hlt">Ocean</span> exceeds that of terrestrial carbon by an order or magnitude or more, recent evidence suggests that this balance is not maintained and significant fractions of terrestrial carbon is preserved in sediments. Using an integrated approach combining lipid biomarkers and radiocarbon dating in particles and sediments, the process of organic carbon recycling and historical changes in its sources and preservation has been examined. A suite of lipid biomarkers in particles and sediments of western Arctic shelves and <span class="hlt">basins</span> were measured and principle components analysis (PCA) used to allow a robust comparison among the 120+ individual compounds to assign organic sources and relative inputs. Offshore particles from the chlorophyll maximum contained abundant algal markers (e.g. 20:5 and 22:6 FAMEs), low concentrations of terrestrial markers (amyrins and 24-ethylcholest-5-en-3b-ol), and reflected modern 14C values. Particles present in deeper halocline waters also reflect marine production, but a portion of older, terrestrial carbon accompanies the sinking of the spring bloom. Surface and deeper sediments of <span class="hlt">basins</span> contain older organic carbon and low concentrations of algal biomarkers, suggesting that marine carbon produced in surface waters is rapidly recycled. Taken together, these observations suggest that marine derived organic matter produced in shallow waters fuels carbon cycling, but relatively small amounts are preserved in sediments. As a result, the organic carbon preserved in sediments contrasts sharply to that typically observed in lower latitudes, with an increasing terrestrial signature with distance</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H11E1224K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H11E1224K"><span>Optimization and Modeling of Extreme Freshwater Discharge from Japanese First-Class River <span class="hlt">Basins</span> to Coastal <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kuroki, R.; Yamashiki, Y. A.; Varlamov, S.; Miyazawa, Y.; Gupta, H. V.; Racault, M.; Troselj, J.</p> <p>2017-12-01</p> <p>We estimated the effects of extreme fluvial outflow events from river mouths on the salinity distribution in the Japanese coastal zones. Targeted extreme event was a typhoon from 06/09/2015 to 12/09/2015, and we generated a set of hourly simulated river outflow data of all Japanese first-class rivers from these <span class="hlt">basins</span> to the Pacific <span class="hlt">Ocean</span> and the Sea of Japan during the period by using our model "Cell Distributed Runoff Model Version 3.1.1 (CDRMV3.1.1)". The model simulated fresh water discharges for the case of the typhoon passage over Japan. We used these data with a coupled hydrological-oceanographic model JCOPE-T, developed by Japan Agency for Marine-earth Science and Technology (JAMSTEC), for estimation of the circulation and salinity distribution in Japanese coastal zones. By using the model, the coastal <span class="hlt">oceanic</span> circulation was reproduced adequately, which was verified by satellite remote sensing. In addition to this, we have successfully optimized 5 parameters, soil roughness coefficient, river roughness coefficient, effective porosity, saturated hydraulic conductivity, and effective rainfall by using Shuffled Complex Evolution method developed by University of Arizona (SCE-UA method), that is one of the optimization method for hydrological model. Increasing accuracy of peak discharge prediction of extreme typhoon events on river mouths is essential for continental-<span class="hlt">oceanic</span> mutual interaction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195945','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195945"><span>Influence of <span class="hlt">basin</span>- and local-scale environmental conditions on nearshore production in the northeast Pacific <span class="hlt">Ocean</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>von Biela, Vanessa R.; Zimmerman, Christian E.; Kruse, Gordon H.; Mueter, Franz J.; Black, Bryan A.; Douglas, David C.; Bodkin, James L.</p> <p>2016-01-01</p> <p>Nearshore marine habitats are productive and vulnerable owing to their connections to pelagic and terrestrial landscapes. To understand how <span class="hlt">ocean</span> <span class="hlt">basin</span>- and local-scale conditions may influence nearshore species, we developed an annual index of nearshore production (spanning the period 1972–2010) from growth increments recorded in otoliths of representative pelagic-feeding (Black Rockfish Sebastes melanops) and benthic-feeding (Kelp Greenling Hexagrammos decagrammus) nearshore-resident fishes at nine sites in the California Current and Alaska Coastal Current systems. We explored the influence of <span class="hlt">basin</span>- and local-scale conditions across all seasons at lags of up to 2 years to represent changes in prey quantity (1- or 2-year time lags) and quality (within-year relationships). Relationships linking fish growth to <span class="hlt">basin</span>-scale (Pacific Decadal Oscillation, North Pacific Gyre Oscillation, and multivariate El Niño–Southern Oscillation index) and local-scale (sea surface temperature, sea surface height anomalies, upwelling index, photosynthetically active radiation, and freshwater discharge) environmental conditions varied by species and current system. Growth of Black Rockfish increased with cool <span class="hlt">basin</span>-scale conditions in the California Current and warm local-scale conditions in the Alaska Coastal Current, consistent with existing hypotheses linking climate to pelagic production on continental shelves in the respective regions. Relationships for Kelp Greenlings in the California Current were complex, with faster growth related to within-year warm conditions and lagged-year cool conditions. These opposing, lag-dependent relationships may reflect differences in conditions that promote quantity versus quality of benthic invertebrate prey in the California Current. Thus, we hypothesize that benthic production is maximized by alternating cool and warm years, as benthic invertebrate recruitment is food limited during warm years while growth is temperature limited by cool</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27851735','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27851735"><span>Reorientation of Sputnik Planitia implies a subsurface <span class="hlt">ocean</span> on Pluto.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nimmo, F; Hamilton, D P; McKinnon, W B; Schenk, P M; Binzel, R P; Bierson, C J; Beyer, R A; Moore, J M; Stern, S A; Weaver, H A; Olkin, C B; Young, L A; Smith, K E</p> <p>2016-12-01</p> <p>The deep nitrogen-covered <span class="hlt">basin</span> on Pluto, informally named Sputnik Planitia, is located very close to the longitude of Pluto's tidal axis and may be an impact feature, by analogy with other large <span class="hlt">basins</span> in the Solar System. Reorientation of Sputnik Planitia arising from tidal and rotational torques can explain the <span class="hlt">basin</span>'s present-day location, but requires the feature to be a positive gravity anomaly, despite its negative topography. Here we argue that if Sputnik Planitia did indeed form as a result of an impact and if Pluto possesses a subsurface <span class="hlt">ocean</span>, the required positive gravity anomaly would naturally result because of shell thinning and <span class="hlt">ocean</span> uplift, followed by later modest nitrogen deposition. Without a subsurface <span class="hlt">ocean</span>, a positive gravity anomaly requires an implausibly thick nitrogen layer (exceeding 40 kilometres). To prolong the lifetime of such a subsurface <span class="hlt">ocean</span> to the present day and to maintain <span class="hlt">ocean</span> uplift, a rigid, conductive water-ice shell is required. Because nitrogen deposition is latitude-dependent, nitrogen loading and reorientation may have exhibited complex feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4410635','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4410635"><span>Skilful multi-year predictions of tropical trans-<span class="hlt">basin</span> climate variability</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Chikamoto, Yoshimitsu; Timmermann, Axel; Luo, Jing-Jia; Mochizuki, Takashi; Kimoto, Masahide; Watanabe, Masahiro; Ishii, Masayoshi; Xie, Shang-Ping; Jin, Fei-Fei</p> <p>2015-01-01</p> <p>Tropical Pacific sea surface temperature anomalies influence the atmospheric circulation, impacting climate far beyond the tropics. The predictability of the corresponding atmospheric signals is typically limited to less than 1 year lead time. Here we present observational and modelling evidence for multi-year predictability of coherent trans-<span class="hlt">basin</span> climate variations that are characterized by a zonal seesaw in tropical sea surface temperature and sea-level pressure between the Pacific and the other two <span class="hlt">ocean</span> <span class="hlt">basins</span>. State-of-the-art climate model forecasts initialized from a realistic <span class="hlt">ocean</span> state show that the low-frequency trans-<span class="hlt">basin</span> climate variability, which explains part of the El Niño Southern Oscillation flavours, can be predicted up to 3 years ahead, thus exceeding the predictive skill of current tropical climate forecasts for natural variability. This low-frequency variability emerges from the synchronization of <span class="hlt">ocean</span> anomalies in all <span class="hlt">basins</span> via global reorganizations of the atmospheric Walker Circulation. PMID:25897996</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25897996','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25897996"><span>Skilful multi-year predictions of tropical trans-<span class="hlt">basin</span> climate variability.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chikamoto, Yoshimitsu; Timmermann, Axel; Luo, Jing-Jia; Mochizuki, Takashi; Kimoto, Masahide; Watanabe, Masahiro; Ishii, Masayoshi; Xie, Shang-Ping; Jin, Fei-Fei</p> <p>2015-04-21</p> <p>Tropical Pacific sea surface temperature anomalies influence the atmospheric circulation, impacting climate far beyond the tropics. The predictability of the corresponding atmospheric signals is typically limited to less than 1 year lead time. Here we present observational and modelling evidence for multi-year predictability of coherent trans-<span class="hlt">basin</span> climate variations that are characterized by a zonal seesaw in tropical sea surface temperature and sea-level pressure between the Pacific and the other two <span class="hlt">ocean</span> <span class="hlt">basins</span>. State-of-the-art climate model forecasts initialized from a realistic <span class="hlt">ocean</span> state show that the low-frequency trans-<span class="hlt">basin</span> climate variability, which explains part of the El Niño Southern Oscillation flavours, can be predicted up to 3 years ahead, thus exceeding the predictive skill of current tropical climate forecasts for natural variability. This low-frequency variability emerges from the synchronization of <span class="hlt">ocean</span> anomalies in all <span class="hlt">basins</span> via global reorganizations of the atmospheric Walker Circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2010/1114/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2010/1114/"><span>Megascopic lithologic studies of coals in the Powder River <span class="hlt">basin</span> in Wyoming and in <span class="hlt">adjacent</span> <span class="hlt">basins</span> in Wyoming and North Dakota</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Trippi, Michael H.; Stricker, Gary D.; Flores, Romeo M.; Stanton, Ronald W.; Chiehowsky, Lora A.; Moore, Timothy A.</p> <p>2010-01-01</p> <p>Between 1999 and 2007, the U.S. Geological Survey (USGS) investigated coalbed methane (CBM) resources in the Wyoming portion of the Powder River <span class="hlt">Basin</span>. The study also included the CBM resources in the North Dakota portion of the Williston <span class="hlt">Basin</span> of North Dakota and the Wyoming portion of the Green River <span class="hlt">Basin</span> of Wyoming. This project involved the cooperation of the State Office, Reservoir Management Group (RMG) of the Bureau of Land Management (BLM) in Casper, Wyo., and 16 independent gas operators in the Powder River, Williston, and Green River <span class="hlt">Basins</span>. The USGS and BLM entered into agreements with these CBM operators to supply samples for the USGS to analyze and provide the RMG with rapid, timely results of total gas desorbed, coal quality, and high-pressure methane adsorption isotherm data. This program resulted in the collection of 963 cored coal samples from 37 core holes. This report presents megascopic lithologic descriptive data collected from canister samples extracted from the 37 wells cored for this project.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP33C2321O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP33C2321O"><span>A History of Warming Sea Surface Temperature and <span class="hlt">Ocean</span> Acidification Recorded by Planktonic Foraminifera Geochemistry from the Santa Barbara <span class="hlt">Basin</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>Osborne, E.; Thunell, R.; Bizimis, M.; Buckley, W. P., Jr.; benitez-Nelson, C. R.; Chartier, C. J.</p> <p>2015-12-01</p> <p>The geochemistry of foraminiferal shells has been widely used to reconstruct past conditions of the <span class="hlt">ocean</span> and climate. Since the onset of the Industrial Revolution, anthropogenically produced CO2 has resulted in an increase in global temperatures and a decline in the mean pH of the world's <span class="hlt">oceans</span>. The California Current System is a particularly susceptible region to <span class="hlt">ocean</span> acidification due to natural upwelling processes that also cause a reduction in seawater pH. The trace element concentration of magnesium and boron in planktonic foraminiferal shells are used here as proxies for temperature and carbonate ion concentration ([CO32-]), respectively. Newly developed calibrations relating Mg/Ca ratios to temperature (R2 0.91) and B/Ca ratios to [CO32-] (R2 0.84) for the surface-mixed layer species Globogerina bulloides were generated using material collected in the Santa Barbara <span class="hlt">Basin</span> sediment trap time-series. Using these empirical relationships, temperature and [CO32-] are reconstructed using a 0.5 meter long multi-core collected within the <span class="hlt">basin</span>. 210Pb activities were used to determine a sedimentation rate for the core to estimate ages for core samples (sedimentation rate: 0.341 cm/yr). A spike in 137Cs activity is used as a tie-point to the year 1965 coinciding with the peak of nuclear bomb testing. Our down-core record extends through the mid-19th century to create a history of rising sea surface temperatures and declining [CO32-] as a result of anthropogenic CO2 emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910063775&hterms=biomass+production&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbiomass%2Bproduction','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910063775&hterms=biomass+production&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbiomass%2Bproduction"><span><span class="hlt">Basin</span>-scale estimates of <span class="hlt">oceanic</span> primary production by remote sensing - The North Atlantic</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Platt, Trevor; Caverhill, Carla; Sathyendranath, Shubha</p> <p>1991-01-01</p> <p>The monthly averaged CZCS data for 1979 are used to estimate annual primary production at <span class="hlt">ocean</span> <span class="hlt">basin</span> scales in the North Atlantic. The principal supplementary data used were 873 vertical profiles of chlorophyll and 248 sets of parameters derived from photosynthesis-light experiments. Four different procedures were tested for calculation of primary production. The spectral model with nonuniform biomass was considered as the benchmark for comparison against the other three models. The less complete models gave results that differed by as much as 50 percent from the benchmark. Vertically uniform models tended to underestimate primary production by about 20 percent compared to the nonuniform models. At horizontal scale, the differences between spectral and nonspectral models were negligible. The linear correlation between biomass and estimated production was poor outside the tropics, suggesting caution against the indiscriminate use of biomass as a proxy variable for primary production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/40095','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/40095"><span>An analysis of the carbon balance of the Arctic <span class="hlt">Basin</span> from 1997 to 2006</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>A.D. McGuire; D.J. Hayes; D.W. Kicklighter; M. Manizza; Q. Zhuang; M. Chen; M.J. Follows; K.R. Gurney; J.W. McClelland; J.M. Melillo; B.J. Peterson; R.G. Prinn</p> <p>2010-01-01</p> <p>This study used several model-based tools to analyze the dynamics of the Arctic <span class="hlt">Basin</span> between 1997 and 2006 as a linked system of land-<span class="hlt">ocean</span>-atmosphere C exchange. The analysis estimates that terrestrial areas of the Arctic <span class="hlt">Basin</span> lost 62.9 Tg C yr-1 and that the Arctic <span class="hlt">Ocean</span> gained 94.1 Tg C yr-1. Arctic lands and <span class="hlt">oceans</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70023584','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70023584"><span>Regional variations in provenance and abundance of ice-rafted clasts in Arctic <span class="hlt">Ocean</span> sediments: Implications for the configuration of late Quaternary <span class="hlt">oceanic</span> and atmospheric circulation in the Arctic</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Phillips, R.L.; Grantz, A.</p> <p>2001-01-01</p> <p>The composition and distribution of ice-rafted glacial erratics in late Quaternary sediments define the major current systems of the Arctic <span class="hlt">Ocean</span> and identify two distinct continental sources for the erratics. In the southern Amerasia <span class="hlt">basin</span> up to 70% of the erratics are dolostones and limestones (the Amerasia suite) that originated in the carbonate-rich Paleozoic terranes of the Canadian Arctic Islands. These clasts reached the Arctic <span class="hlt">Ocean</span> in glaciers and were ice-rafted to the core sites in the clockwise Beaufort Gyre. The concentration of erratics decreases northward by 98% along the trend of the gyre from southeastern Canada <span class="hlt">basin</span> to Makarov <span class="hlt">basin</span>. The concentration of erratics then triples across the Makarov <span class="hlt">basin</span> flank of Lomonosov Ridge and siltstone, sandstone and siliceous clasts become dominant in cores from the ridge and the Eurasia <span class="hlt">basin</span> (the Eurasia suite). The bedrock source for the siltstone and sandstone clasts is uncertain, but bedrock distribution and the distribution of glaciation in northern Eurasia suggest the Taymyr Peninsula-Kara Sea regions. The pattern of clast distribution in the Arctic <span class="hlt">Ocean</span> sediments and the sharp northward decrease in concentration of clasts of Canadian Arctic Island provenance in the Amerasia <span class="hlt">basin</span> support the conclusion that the modem circulation pattern of the Arctic <span class="hlt">Ocean</span>, with the Beaufort Gyre dominant in the Amerasia <span class="hlt">basin</span> and the Transpolar drift dominant in the Eurasia <span class="hlt">basin</span>, has controlled both sea-ice and glacial iceberg drift in the Arctic <span class="hlt">Ocean</span> during interglacial intervals since at least the late Pleistocene. The abruptness of the change in both clast composition and concentration on the Makarov <span class="hlt">basin</span> flank of Lomonosov Ridge also suggests that the boundary between the Beaufort Gyre and the Transpolar Drift has been relatively stable during interglacials since that time. Because the Beaufort Gyre is wind-driven our data, in conjunction with the westerly directed orientation of sand dunes that formed during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP13A1860A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP13A1860A"><span>Extreme diagenesis displayed by Pliocene-Pleistocene Calcareous Nannofossils in IODP Hole 1396A, <span class="hlt">adjacent</span> to Montserrat Island in the Lesser Antilles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aljahdali, M. H.; Behzad, A.; Missimer, T. M.; Wise, S. W.; Scientists, E.</p> <p>2013-12-01</p> <p><span class="hlt">Adjacent</span> to Montserrat Island in the Lesser Antilles of the Caribbean Sea, Integrated <span class="hlt">Ocean</span> Drilling Program (IODP) Site 1396 recovered lower Pliocene to Pleistocene calcareous nannofossil assemblages (CN11 to CN15) that range between common to abundant and display a variety of preservations. High-resolution Scanning Electron Microscopy (SEM) observation of calcareous nannofossil assemblages in selected samples from Hole 1396A, shows severe diagenesis (overgrowth and/or dissolution) even near the top of the sequence. The nannofossil assemblages in this relatively shallow <span class="hlt">basin</span> (e.g., 800 m) reveal abnormal diagenesis for such young specimens that are quite similar to the heavy overgrowths and dissolution generally seen only in older deposits (e.g., Cretaceous). Our hypothesis is that volcanic activity in the region probably induced this extreme diagenesis. A more detailed examination of these samples should provide a better understanding of the progression of carbonate diagenesis in this <span class="hlt">basin</span>. The nannofossil biostratigraphy and magnetostratigraphy at Site 1396 also suggest lower sedimentation rates in the Pleistocene than in the Pliocene. A comparison site (ODP Leg 165 Site 1000) in the Caribbean Sea also shows a similar sedimentation-rate pattern. This we interpret as a regional event caused by the closure of the Central American Seaway.</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4801315','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4801315"><span>Quantifying dispersal from hydrothermal vent fields in the western Pacific <span class="hlt">Ocean</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>Mitarai, Satoshi; Watanabe, Hiromi; Nakajima, Yuichi; Shchepetkin, Alexander F.; McWilliams, James C.</p> <p>2016-01-01</p> <p>Hydrothermal vent fields in the western Pacific <span class="hlt">Ocean</span> are mostly distributed along spreading centers in submarine <span class="hlt">basins</span> behind convergent plate boundaries. Larval dispersal resulting from deep-<span class="hlt">ocean</span> circulations is one of the major factors influencing gene flow, diversity, and distributions of vent animals. By combining a biophysical model and deep-profiling float experiments, we quantify potential larval dispersal of vent species via <span class="hlt">ocean</span> circulation in the western Pacific <span class="hlt">Ocean</span>. We demonstrate that vent fields within back-arc <span class="hlt">basins</span> could be well connected without particular directionality, whereas <span class="hlt">basin-to-basin</span> dispersal is expected to occur infrequently, once in tens to hundreds of thousands of years, with clear dispersal barriers and directionality associated with <span class="hlt">ocean</span> currents. The southwest Pacific vent complex, spanning more than 4,000 km, may be connected by the South Equatorial Current for species with a longer-than-average larval development time. Depending on larval dispersal depth, a strong western boundary current, the Kuroshio Current, could bridge vent fields from the Okinawa Trough to the Izu-Bonin Arc, which are 1,200 km apart. Outcomes of this study should help marine ecologists estimate gene flow among vent populations and design optimal marine conservation plans to protect one of the most unusual ecosystems on Earth. PMID:26929376</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26929376','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26929376"><span>Quantifying dispersal from hydrothermal vent fields in the western Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mitarai, Satoshi; Watanabe, Hiromi; Nakajima, Yuichi; Shchepetkin, Alexander F; McWilliams, James C</p> <p>2016-03-15</p> <p>Hydrothermal vent fields in the western Pacific <span class="hlt">Ocean</span> are mostly distributed along spreading centers in submarine <span class="hlt">basins</span> behind convergent plate boundaries. Larval dispersal resulting from deep-<span class="hlt">ocean</span> circulations is one of the major factors influencing gene flow, diversity, and distributions of vent animals. By combining a biophysical model and deep-profiling float experiments, we quantify potential larval dispersal of vent species via <span class="hlt">ocean</span> circulation in the western Pacific <span class="hlt">Ocean</span>. We demonstrate that vent fields within back-arc <span class="hlt">basins</span> could be well connected without particular directionality, whereas <span class="hlt">basin-to-basin</span> dispersal is expected to occur infrequently, once in tens to hundreds of thousands of years, with clear dispersal barriers and directionality associated with <span class="hlt">ocean</span> currents. The southwest Pacific vent complex, spanning more than 4,000 km, may be connected by the South Equatorial Current for species with a longer-than-average larval development time. Depending on larval dispersal depth, a strong western boundary current, the Kuroshio Current, could bridge vent fields from the Okinawa Trough to the Izu-Bonin Arc, which are 1,200 km apart. Outcomes of this study should help marine ecologists estimate gene flow among vent populations and design optimal marine conservation plans to protect one of the most unusual ecosystems on Earth.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA633506','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA633506"><span>Dynamics of <span class="hlt">Oceanic</span> Motions</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1997-09-30</p> <p>research is multiscale , interdisciplinary and generic. The methods are applicable to an arbitrary region of the coastal and/or deep <span class="hlt">ocean</span> and across the...dynamics. OBJECTIVES General objectives are: (I) To determine for the coastal and/or coupled deep <span class="hlt">ocean</span> the multiscale processes which occur: i) in...Straits and the eastern <span class="hlt">basin</span>; iii) extension and application of our balance of terms scheme (EVA) to multiscale , interdisciplinary fields with data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...104.3075R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...104.3075R"><span>Deep inflow into the Mozambique <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Read, J. F.; Pollard, R. T.</p> <p>1999-02-01</p> <p>More than 200 conductivity-temperature-depth (CTD) stations were worked around the Southwest Indian Ridge and Del Caño Rise as part of the World <span class="hlt">Ocean</span> Circulation Experiment. A selection of these data provides information about the inflow of bottom water into the Mozambique <span class="hlt">Basin</span>. The <span class="hlt">basin</span> is closed below 3000 m, yet the inflow is significantly large, of order 1 Sv (1 Sv = 106 m3 s-1). Estimates of the <span class="hlt">basin</span>-scale upwelling at 4000 m suggest that the vertical velocity is also large, 10 × 10-5 cm s-1 or more, an order of magnitude greater than global <span class="hlt">ocean</span> estimates. Examination of the characteristics of the bottom water in the Mozambique and Agulhas <span class="hlt">Basins</span> and the Prince Edward Fracture Zone shows that bottom water enters the Mozambique <span class="hlt">Basin</span> from the Agulhas <span class="hlt">Basin</span> and also directly from the Enderby <span class="hlt">Basin</span>. Most of the transport enters the Mozambique <span class="hlt">Basin</span> via the Agulhas <span class="hlt">Basin</span>, where two regions of northward flow below 4000 m are found. The major flow, on the eastern flank of the Mozambique Ridge, is through and above the deep, extending (5900 m) trench that connects the Agulhas and Mozambique <span class="hlt">Basins</span>. The second, weaker flow enters the Transkei <span class="hlt">Basin</span> along the deep eastern flank of the Agulhas Plateau, then turning east into the Mozambique <span class="hlt">Basin</span>. The only source of bottom water to the Agulhas <span class="hlt">Basin</span> is the Enderby <span class="hlt">Basin</span>, but a more direct route between the Enderby and Mozambique <span class="hlt">Basins</span> exists via the Prince Edward fracture, which extends deeper than 4000 m throughout its length and links the two <span class="hlt">basins</span> directly across the Southwest Indian Ridge. Full depth CTD stations trace the changing characteristics of the deep and bottom water in the fracture, and moored current meter data show the strength and persistence of the throughflow. Strong mixing with the overlying deep water elevates the salt content of the bottom water by comparison with the other water in the Mozambique <span class="hlt">Basin</span>. Thus two distinct bottom waters of the Mozambique <span class="hlt">Basin</span> originate in the same place</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19965425','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19965425"><span>Aragonite undersaturation in the Arctic <span class="hlt">Ocean</span>: effects of <span class="hlt">ocean</span> acidification and sea ice melt.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yamamoto-Kawai, Michiyo; McLaughlin, Fiona A; Carmack, Eddy C; Nishino, Shigeto; Shimada, Koji</p> <p>2009-11-20</p> <p>The increase in anthropogenic carbon dioxide emissions and attendant increase in <span class="hlt">ocean</span> acidification and sea ice melt act together to decrease the saturation state of calcium carbonate in the Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span>. In 2008, surface waters were undersaturated with respect to aragonite, a relatively soluble form of calcium carbonate found in plankton and invertebrates. Undersaturation was found to be a direct consequence of the recent extensive melting of sea ice in the Canada <span class="hlt">Basin</span>. In addition, the retreat of the ice edge well past the shelf-break has produced conditions favorable to enhanced upwelling of subsurface, aragonite-undersaturated water onto the Arctic continental shelf. Undersaturation will affect both planktonic and benthic calcifying biota and therefore the composition of the Arctic ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AIPC.1953h0007G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AIPC.1953h0007G"><span>The oxidation state of iron and manganese in polymetallic nodules from the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ganwani, Girish; Meena, Samay Singh; Ram, Sahi; Bijlani, N.; Bhatia, Beena; Tripathi, R. P.</p> <p>2018-05-01</p> <p>The study of oxidation states of iron (Fe) and manganese (Mn) in polymetallic nodules were carried out by means of X-ray photoelectron spectroscopic techniques. The polymetallic nodules were collected from different locations of the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB). The Mn/Fe ratio allowed the differentiation of these nodules from their origin: "hydrogeneous" or "hydrothermal". The binding energies of Mn 2p3/2 (ranging from 641.5 to 642.4 ev), Fe 2p3/2 (ranging from 711.0 to 711.8 ev) and O 1s (ranging from 530.2 to 530.9 ev) from XPS reveal that most of manganese is in Mn4+ and iron is in Fe3+ state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70058771','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70058771"><span><span class="hlt">Basins</span> in ARC-continental collisions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Draut, Amy E.; Clift, Peter D.; Busby, Cathy; Azor, Antonio</p> <p>2012-01-01</p> <p>Arc-continent collisions occur commonly in the plate-tectonic cycle and result in rapidly formed and rapidly collapsing orogens, often spanning just 5-15 My. Growth of continental masses through arc-continent collision is widely thought to be a major process governing the structural and geochemical evolution of the continental crust over geologic time. Collisions of intra-<span class="hlt">oceanic</span> arcs with passive continental margins (a situation in which the arc, on the upper plate, faces the continent) involve a substantially different geometry than collisions of intra-<span class="hlt">oceanic</span> arcs with active continental margins (a situation requiring more than one convergence zone and in which the arc, on the lower plate, backs into the continent), with variable preservation potential for <span class="hlt">basins</span> in each case. Substantial differences also occur between trench and forearc evolution in tectonically erosive versus tectonically accreting margins, both before and after collision. We examine the evolution of trenches, trench-slope <span class="hlt">basins</span>, forearc <span class="hlt">basins</span>, intra-arc <span class="hlt">basins</span>, and backarc <span class="hlt">basins</span> during arc-continent collision. The preservation potential of trench-slope <span class="hlt">basins</span> is low; in collision they are rapidly uplifted and eroded, and at erosive margins they are progressively destroyed by subduction erosion. Post-collisional preservation of trench sediment and trench-slope <span class="hlt">basins</span> is biased toward margins that were tectonically accreting for a substantial length of time before collision. Forearc <span class="hlt">basins</span> in erosive margins are usually floored by strong lithosphere and may survive collision with a passive margin, sometimes continuing sedimentation throughout collision and orogeny. The low flexural rigidity of intra-arc <span class="hlt">basins</span> makes them deep and, if preserved, potentially long records of arc and collisional tectonism. Backarc <span class="hlt">basins</span>, in contrast, are typically subducted and their sediment either lost or preserved only as fragments in melange sequences. A substantial proportion of the sediment derived from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1198293-ocean-cooling-pattern-last-glacial-maximum','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1198293-ocean-cooling-pattern-last-glacial-maximum"><span><span class="hlt">Ocean</span> Cooling Pattern at the Last Glacial Maximum</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Zhuang, Kelin; Giardino, John R.</p> <p>2012-01-01</p> <p><span class="hlt">Ocean</span> temperature and <span class="hlt">ocean</span> heat content change are analyzed based on four PMIP3 model results at the Last Glacial Maximum relative to the prehistorical run. <span class="hlt">Ocean</span> cooling mostly occurs in the upper 1000 m depth and varies spatially in the tropical and temperate zones. The Atlantic <span class="hlt">Ocean</span> experiences greater cooling than the rest of the <span class="hlt">ocean</span> <span class="hlt">basins</span>. <span class="hlt">Ocean</span> cooling is closely related to the weakening of meridional overturning circulation and enhanced intrusion of Antarctic Bottom Water into the North Atlantic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1978/0783/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1978/0783/report.pdf"><span>Subsurface geology and porosity distribution, Madison Limestone and underlying formations, Powder River <span class="hlt">basin</span>, northeastern Wyoming and southeastern Montana and <span class="hlt">adjacent</span> areas</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Peterson, James A.</p> <p>1978-01-01</p> <p>To evaluate the Madison Limestone and associated rocks as potential sources for water supplies in the Powder River <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, an understanding of the geologic framework of these units, their lithologic facies patterns, the distribution of porosity zones, and the relation between porosity development and stratigraphic facies is necessary. Regionally the Madison is mainly a fossiliferous limestone. However, in broad areas of the eastern Rocky Mountains and western Great Plains, dolomite is a dominant constituent and in places the Madison is almost entirely dolomite. Within these areas maximum porosity development is found and it seems to be related to the coarser crystalline dolomite facies. The porosity development is associated with tabular and fairly continuous crystalline dolomite beds separated by non-porous limestones. The maximum porosity development in the Bighorn Dolomite, as in the Madison, is directly associated with the occurrence of a more coarsely crystalline sucrosic dolomite facies. Well data indicate, however, that where the Bighorn is present in the deeper parts of the Powder River <span class="hlt">Basin</span>, it may be dominated by a finer crystalline dolomite facies of low porosity. The 'Winnipeg Sandstone' is a clean, generally well-sorted, medium-grained sandstone. It shows good porosity development in parts of the northern Powder River <span class="hlt">Basin</span> and northwestern South Dakota. Because the sandstone is silica-cemented and quartzitic in areas of deep burial, good porosity is expected only where it is no deeper than a few thousand feet. The Flathead Sandstone is a predominantly quartzose, slightly feldspathic sandstone, commonly cemented with iron oxide. Like the 'Winnipeg Sandstone,' it too is silica-cemented and quartzitic in many places so that its porosity is poor in areas of deep burial. Illustrations in this report show the thickness, percent dolomite, and porosity-feet for the Bighorn Dolomite and the Madison Limestone and its subdivisions. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS41F..02H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS41F..02H"><span>The quiet revolution: continuous glider monitoring at <span class="hlt">ocean</span> 'choke' points as a key component of new cross-platform <span class="hlt">ocean</span> observation systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heslop, E. E.; Tintore, J.; Ruiz, S.; Allen, J.; López-Jurado, J. L.</p> <p>2014-12-01</p> <p>A quiet revolution is taking place in <span class="hlt">ocean</span> observations; in the last decade new multi-platform, integrated <span class="hlt">ocean</span> observatories have been progressively implemented by forward looking countries with <span class="hlt">ocean</span> borders of economic and strategic importance. These systems are designed to fill significant gaps in our knowledge of the <span class="hlt">ocean</span> state and <span class="hlt">ocean</span> variability, through long-term, science and society-led, <span class="hlt">ocean</span> monitoring. These <span class="hlt">ocean</span> observatories are now delivering results, not the headline results of a single issue experiment, but carefully and systematically improving our knowledge of <span class="hlt">ocean</span> variability, and thereby, increasing model forecast skill and our ability to link physical processes to ecosystem response. Here we present the results from a 3-year quasi-continuous glider monitoring of a key circulation 'choke' point in the Western Mediterranean, undertaken by SOCIB (Balearic Islands Coastal <span class="hlt">Ocean</span> Observing and Forecasting System). For the first time data from the high frequency glider sampling show variations in the transport volumes of water over timescales of days to weeks, as large as those previously only identifiable as seasonal or eddy driven. Although previous surveys noted high cruise-to-cruise variability, they were insufficient to show that in fact water volumes exchanged through this narrow 'choke' point fluctuate on 'weather' timescales. Using the glider data to leverage an 18-year record of ship missions, we define new seasonal cycles for the exchange of watermasses, challenging generally held assumptions. The pattern of the exchange is further simplified through the characterisation of 5 circulation modes and the defining of a new seasonal cycle for the interplay between mesoscale and <span class="hlt">basin</span> scale dynamics. Restricted 'choke points' between our <span class="hlt">ocean</span> <span class="hlt">basins</span> are critical locations to monitor water transport variability, as they constrain the inter-<span class="hlt">basin</span> exchange of heat, salt and nutrients. At the Ibiza Channel 'choke' point, the exchange of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195036','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195036"><span>Resource potential of the western North Atlantic <span class="hlt">Basin</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>Dillon, William P.; Manheim, Frank T.; Jansa, L.F.; Palmason, Gudmundur; Tucholke, Brian E.; Landrum, Richard S.</p> <p>1986-01-01</p> <p>We here consider the petroleum resources only of the off shelf portion of the western North Atlantic <span class="hlt">Ocean</span>. Very little information is available for this region; off the eastern United States, only four petroleum exploration holes have been drilled in one restricted area seaward of the shelf, off the Baltimore Canyon trough. However, by interpreting seismic reflection profiles and Stratigraphie data from the Deep Sea Drilling Project (DSDP) and other wells on the <span class="hlt">adjacent</span> slope and shelf, we can evaluate the geologic conditions that existed during development of the <span class="hlt">basin</span> and that might lead to petroleum accumulations.The wellknown factors that lead to oil and gas accumulations are availability of source beds, adequate maturation, and the presence of reservoir beds and seals configured to create a trap. The western boundary of the area considered in this paper, the present sloperise break, is one that has developed from the interplay of sedimentation and erosion at the continental margin; these processes are affected by variations in margin subsidence, sedi-ment input, <span class="hlt">oceanic</span> circulation, sea level, and other factors. Thus the sloperise break has migrated over time and is locally underlain by slope and shelf deposits, as well as deepbasin facies. These changes in depositional environments may well have caused juxtaposition of source and reservoir beds with effective seals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title15-vol3/pdf/CFR-2012-title15-vol3-part922-subpartM-appD.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title15-vol3/pdf/CFR-2012-title15-vol3-part922-subpartM-appD.pdf"><span>15 CFR Appendix D to Subpart M of... - Dredged Material Disposal Sites <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-01-01</p> <p>... <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary D Appendix D to Subpart M of Part 922 Commerce and Foreign Trade Regulations Relating to Commerce and Foreign Trade (Continued) NATIONAL <span class="hlt">OCEANIC</span> AND ATMOSPHERIC ADMINISTRATION, DEPARTMENT OF COMMERCE <span class="hlt">OCEAN</span> AND COASTAL RESOURCE MANAGEMENT NATIONAL MARINE...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title15-vol3/pdf/CFR-2014-title15-vol3-part922-subpartM-appD.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title15-vol3/pdf/CFR-2014-title15-vol3-part922-subpartM-appD.pdf"><span>15 CFR Appendix D to Subpart M of... - Dredged Material Disposal Sites <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-01-01</p> <p>... <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary D Appendix D to Subpart M of Part 922 Commerce and Foreign Trade Regulations Relating to Commerce and Foreign Trade (Continued) NATIONAL <span class="hlt">OCEANIC</span> AND ATMOSPHERIC ADMINISTRATION, DEPARTMENT OF COMMERCE <span class="hlt">OCEAN</span> AND COASTAL RESOURCE MANAGEMENT NATIONAL MARINE...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title15-vol3/pdf/CFR-2013-title15-vol3-part922-subpartM-appD.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title15-vol3/pdf/CFR-2013-title15-vol3-part922-subpartM-appD.pdf"><span>15 CFR Appendix D to Subpart M of... - Dredged Material Disposal Sites <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-01-01</p> <p>... <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary D Appendix D to Subpart M of Part 922 Commerce and Foreign Trade Regulations Relating to Commerce and Foreign Trade (Continued) NATIONAL <span class="hlt">OCEANIC</span> AND ATMOSPHERIC ADMINISTRATION, DEPARTMENT OF COMMERCE <span class="hlt">OCEAN</span> AND COASTAL RESOURCE MANAGEMENT NATIONAL MARINE...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2006/5099/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2006/5099/"><span>Characterization of surface-water resources in the Great <span class="hlt">Basin</span> National Park area and their susceptibility to ground-water withdrawals in <span class="hlt">adjacent</span> valleys, White Pine County, Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Elliott, Peggy E.; Beck, David A.; Prudic, David E.</p> <p>2006-01-01</p> <p>Eight drainage <span class="hlt">basins</span> and one spring within the Great <span class="hlt">Basin</span> National Park area were monitored continually from October 2002 to September 2004 to quantify stream discharge and assess the natural variability in flow. Mean annual discharge for the stream drainages ranged from 0 cubic feet per second at Decathon Canyon to 9.08 cubic feet per second at Baker Creek. Seasonal variability in streamflow generally was uniform throughout the network. Minimum and maximum mean monthly discharges occurred in February and June, respectively, at all but one of the perennial streamflow sites. Synoptic-discharge, specific-conductance, and water- and air-temperature measurements were collected during the spring, summer, and autumn of 2003 along selected reaches of Strawberry, Shingle, Lehman, Baker, and Snake Creeks, and Big Wash to determine areas where surface-water resources would be susceptible to ground-water withdrawals in <span class="hlt">adjacent</span> valleys. Comparison of streamflow and water-property data to the geology along each stream indicated areas where surface-water resources likely or potentially would be susceptible to ground-water withdrawals. These areas consist of reaches where streams (1) are in contact with permeable rocks or sediments, or (2) receive water from either spring discharge or ground-water inflow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA575530','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA575530"><span>The Influence of Atmosphere-<span class="hlt">Ocean</span> Interaction on MJO Development and Propagation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>atmosphere-<span class="hlt">ocean</span> feedbacks and their influence on MJO development, and for forecasting of air sea interaction in the Indian <span class="hlt">Ocean</span> <span class="hlt">basin</span> and its influence...black line indicating precipitation maximum over the DYNAMO area and the red line indicating the precipitation anomaly west of Sumatra . The... <span class="hlt">basin</span> in December. Similar EOF decomposition of the precipitation associated with Kelvin waves (not shown here) indicates strong Kelvin wave anomaly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2004/1243','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2004/1243"><span>Seismic reflection and refraction data acquired in Canada <span class="hlt">Basin</span>, Northwind Ridge and Northwind <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span> in 1988, 1992 and 1993</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Grantz, Arthur; Hart, Patrick E.; May, Steven D.</p> <p>2004-01-01</p> <p>Seismic reflection and refraction data were collected in generally ice-covered waters of the Canada <span class="hlt">Basin</span> and the eastern part of the Chukchi Continental Borderland of the Amerasia <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span>, during the late summers of 1988, 1992, and 1993. The data were acquired from a Polar class icebreaker, the U.S. Coast Guard Cutter Polar Star, using a seismic reflection system designed by the U.S. Geological Survey (USGS). The northernmost data extend to 78? 48' N latitude. In 1988, 155 km of reflection data were acquired with a prototype system consisting of a single 195 cubic inch air gun seismic source and a two-channel hydrophone streamer with a 150-m active section. In 1992 and 1993, 500 and 1,900 km, respectively, of seismic reflection profile data were acquired with an improved six air gun, 674 to 1303 cubic inch tuned seismic source array and the same two-channel streamer. In 1993, a 12-channel streamer with a 150-m active section was used to record five of the reflection lines and one line was acquired using a three air gun, 3,000 cubic inch source. All data were recorded with a DFS-V digital seismic recorder. Processed sections feature high quality vertical incidence images to more than 6 km of sub-bottom penetration in the Canada <span class="hlt">Basin</span>. Refraction data were acquired with U.S. Navy sonobuoys recorded simultaneously with the seismic reflection profiles. In 1988 eight refraction profiles were recorded with the single air gun, and in 1992 and 1993 a total of 47 refraction profiles were recorded with the six air gun array. The sonobuoy refraction records, with offsets up to 35 km, provide acoustic velocity information to complement the short-offset reflection data. The report includes trackline maps showing the location of the data, as well as both digital data files (SEG-Y) and images of all of the profiles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011GeoRL..38.3601Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011GeoRL..38.3601Y"><span>Effects of <span class="hlt">ocean</span> acidification, warming and melting of sea ice on aragonite saturation of the Canada <span class="hlt">Basin</span> surface water</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yamamoto-Kawai, M.; McLaughlin, F. A.; Carmack, E. C.</p> <p>2011-02-01</p> <p>In 2008, surface waters in the Canada <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span> were found to be undersaturated with respect to aragonite. This is associated with recent extensive melting of sea ice in this region, as well as elevated sea surface temperature and atmospheric CO2 concentrations. We have estimated the relative contribution of each of these controlling factors to the calcium carbonate saturation state (Ω) from observations of dissolved inorganic carbon, total alkalinity and oxygen isotope ratio. Results indicate that the increase in atmospheric CO2 has lowered surface Ω by ˜0.3 in the Canada <span class="hlt">Basin</span> since the preindustrial period. Recent melting of sea ice has further lowered mean Ω by 0.4, and of this, half was due to dilution of surface water and half was due to the change in air-sea disequilibrium state. Surface water warming has generally counteracted the mean decrease in Ω by 0.1.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911799N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911799N"><span>Sensitivity of the <span class="hlt">ocean</span> overturning circulation to wind and mixing: theoretical scalings and global <span class="hlt">ocean</span> models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nikurashin, Maxim; Gunn, Andrew</p> <p>2017-04-01</p> <p>The meridional overturning circulation (MOC) is a planetary-scale <span class="hlt">oceanic</span> flow which is of direct importance to the climate system: it transports heat meridionally and regulates the exchange of CO2 with the atmosphere. The MOC is forced by wind and heat and freshwater fluxes at the surface and turbulent mixing in the <span class="hlt">ocean</span> interior. A number of conceptual theories for the sensitivity of the MOC to changes in forcing have recently been developed and tested with idealized numerical models. However, the skill of the simple conceptual theories to describe the MOC simulated with higher complexity global models remains largely unknown. In this study, we present a systematic comparison of theoretical and modelled sensitivity of the MOC and associated deep <span class="hlt">ocean</span> stratification to vertical mixing and southern hemisphere westerlies. The results show that theories that simplify the <span class="hlt">ocean</span> into a single-<span class="hlt">basin</span>, zonally-symmetric box are generally in a good agreement with a realistic, global <span class="hlt">ocean</span> circulation model. Some disagreement occurs in the abyssal <span class="hlt">ocean</span>, where complex bottom topography is not taken into account by simple theories. Distinct regimes, where the MOC has a different sensitivity to wind or mixing, as predicted by simple theories, are also clearly shown by the global <span class="hlt">ocean</span> model. The sensitivity of the Indo-Pacific, Atlantic, and global <span class="hlt">basins</span> is analysed separately to validate the conceptual understanding of the upper and lower overturning cells in the theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015CRGeo.347..227S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015CRGeo.347..227S"><span>Late Eocene to present isotopic (Sr-Nd-Pb) and geochemical evolution of sediments from the Lomonosov Ridge, Arctic <span class="hlt">Ocean</span>: Implications for continental sources and linkage with the North Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stevenson, Ross; Poirier, André; Véron, Alain; Carignan, Jean; Hillaire-Marcel, Claude</p> <p>2015-09-01</p> <p>New geochemical and isotopic (Sr, Nd, Pb) data are presented for a composite sedimentary record encompassing the past 50 Ma of history of sedimentation on the Lomonosov Ridge in the Arctic <span class="hlt">Ocean</span>. The sampled sediments encompass the transition of the Arctic <span class="hlt">basin</span> from an enclosed anoxic <span class="hlt">basin</span> to an open and ventilated oxidized <span class="hlt">ocean</span> <span class="hlt">basin</span>. The transition from anoxic <span class="hlt">basin</span> to open ventilated <span class="hlt">ocean</span> is accompanied by at least three geochemical and isotopic shifts and an increase in elements (e.g., K/Al) controlled by detrital minerals highlighting significant changes in sediment types and sources. The isotopic compositions of the sediments prior to ventilation are more variable but indicate a predominance of older crustal contributions consistent with sources from the Canadian Shield. Following ventilation, the isotopic compositions are more stable and indicate an increased contribution from younger material consistent with Eurasian and Pan-African crustal sources. The waxing and waning of these sources in conjunction with the passage of water through Fram Strait underlines the importance of the exchange of water mass between the Arctic and North Atlantic <span class="hlt">Oceans</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('http://adsabs.harvard.edu/abs/2018AnGeo..36..167I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AnGeo..36..167I"><span>Depth of origin of <span class="hlt">ocean</span>-circulation-induced magnetic signals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Irrgang, Christopher; Saynisch-Wagner, Jan; Thomas, Maik</p> <p>2018-01-01</p> <p>As the world <span class="hlt">ocean</span> moves through the ambient geomagnetic core field, electric currents are generated in the entire <span class="hlt">ocean</span> <span class="hlt">basin</span>. These <span class="hlt">oceanic</span> electric currents induce weak magnetic signals that are principally observable outside of the <span class="hlt">ocean</span> and allow inferences about large-scale <span class="hlt">oceanic</span> transports of water, heat, and salinity. The <span class="hlt">ocean</span>-induced magnetic field is an integral quantity and, to first order, it is proportional to depth-integrated and conductivity-weighted <span class="hlt">ocean</span> currents. However, the specific contribution of <span class="hlt">oceanic</span> transports at different depths to the motional induction process remains unclear and is examined in this study. We show that large-scale motional induction due to the general <span class="hlt">ocean</span> circulation is dominantly generated by <span class="hlt">ocean</span> currents in the upper 2000 m of the <span class="hlt">ocean</span> <span class="hlt">basin</span>. In particular, our findings allow relating regional patterns of the <span class="hlt">oceanic</span> magnetic field to corresponding <span class="hlt">oceanic</span> transports at different depths. <span class="hlt">Ocean</span> currents below 3000 m, in contrast, only contribute a small fraction to the <span class="hlt">ocean</span>-induced magnetic signal strength with values up to 0.2 nT at sea surface and less than 0.1 nT at the Swarm satellite altitude. Thereby, potential satellite observations of <span class="hlt">ocean</span>-circulation-induced magnetic signals are found to be likely insensitive to deep <span class="hlt">ocean</span> currents. Furthermore, it is shown that annual temporal variations of the <span class="hlt">ocean</span>-induced magnetic field in the region of the Antarctic Circumpolar Current contain information about sub-surface <span class="hlt">ocean</span> currents below 1000 m with intra-annual periods. Specifically, <span class="hlt">ocean</span> currents with sub-monthly periods dominate the annual temporal variability of the <span class="hlt">ocean</span>-induced magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70019615','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70019615"><span>Quaternary history of sea ice and paleoclimate in the Amerasia <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span>, as recorded in the cyclical strata of Northwind 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>Phillips, R.L.; Grantz, A.</p> <p>1997-01-01</p> <p>The 19 middle-early Pleistocene to Holocene bipartite lithostratigraphic cycles observed in high-resolution piston cores from Northwind Ridge in the Amerasia <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span>, provide a detailed record of alternating glacial and interglacial climatic and oceanographic conditions and of correlative changes in the character and thickness of the sea-ice cover in the Amerasia <span class="hlt">Basin</span>. Glacial conditions in each cycle are represented by gray pelagic muds that are suboxic, laminated, and essentially lacking in microfossils, macrofossils, trace fossils, and generally in glacial erratics. Interglacial conditions are represented by ochre pelagic muds that are oxic and bioturbated and contain rare to abundant microfossils and abundant glacial erratics. The synglacial laminated gray muds were deposited when the central Amerasia <span class="hlt">Basin</span> was covered by a floating sheet of sea ice of sufficient thickness and continuity to reduce downwelling solar irradiance and oxygen to levels that precluded photosynthesis, maintenance of a biota, and strong oxidation of the pelagic sediment. Except during the early part of 3 of the 19 synglacial episodes, when it was periodically breached by erratic-bearing glacial icebergs, the floating Arctic <span class="hlt">Ocean</span> sea-ice sheet was sufficiently thick to block the circulation of icebergs over Northwind Ridge and presumably other areas of the central Arctic <span class="hlt">Ocean</span>. Interglacial conditions were initiated by abrupt thinning and breakup of the floating sea-ice sheet at the close of glacial time, which permitted surges of glacial erratic-laden ice-bergs to reach Northwind Ridge and the central Arctic <span class="hlt">Ocean</span>, where they circulated freely and deposited numerous, and relatively thick, erratic clast-rich beds. Breakup of the successive synglacial sea-ice sheets initiated deposition of the interglacial ochre mud units under conditions that allowed sunlight and increased amounts of oxygen to enter the water column, resulting in photosynthesis and biologic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004Tectp.379...61M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004Tectp.379...61M"><span>Gravity anomalies and associated tectonic features over the Indian Peninsular Shield and adjoining <span class="hlt">ocean</span> <span class="hlt">basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mishra, D. C.; Arora, K.; Tiwari, V. M.</p> <p>2004-02-01</p> <p>A combined gravity map over the Indian Peninsular Shield (IPS) and adjoining <span class="hlt">oceans</span> brings out well the inter-relationships between the older tectonic features of the continent and the adjoining younger <span class="hlt">oceanic</span> features. The NW-SE, NE-SW and N-S Precambrian trends of the IPS are reflected in the structural trends of the Arabian Sea and the Bay of Bengal suggesting their probable reactivation. The Simple Bouguer anomaly map shows consistent increase in gravity value from the continent to the deep <span class="hlt">ocean</span> <span class="hlt">basins</span>, which is attributed to isostatic compensation due to variations in the crustal thickness. A crustal density model computed along a profile across this region suggests a thick crust of 35-40 km under the continent, which reduces to 22/20-24 km under the Bay of Bengal with thick sediments of 8-10 km underlain by crustal layers of density 2720 and 2900/2840 kg/m 3. Large crustal thickness and trends of the gravity anomalies may suggest a transitional crust in the Bay of Bengal up to 150-200 km from the east coast. The crustal thickness under the Laxmi ridge and east of it in the Arabian Sea is 20 and 14 km, respectively, with 5-6 km thick Tertiary and Mesozoic sediments separated by a thin layer of Deccan Trap. Crustal layers of densities 2750 and 2950 kg/m 3 underlie sediments. The crustal density model in this part of the Arabian Sea (east of Laxmi ridge) and the structural trends similar to the Indian Peninsular Shield suggest a continent-<span class="hlt">ocean</span> transitional crust (COTC). The COTC may represent down dropped and submerged parts of the Indian crust evolved at the time of break-up along the west coast of India and passage of Reunion hotspot over India during late Cretaceous. The crustal model under this part also shows an underplated lower crust and a low density upper mantle, extending over the continent across the west coast of India, which appears to be related to the Deccan volcanism. The crustal thickness under the western Arabian Sea (west of the Laxmi ridge</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ESSD...10..677Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ESSD...10..677Z"><span>An inventory of Arctic <span class="hlt">Ocean</span> data in the World <span class="hlt">Ocean</span> Database</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zweng, Melissa M.; Boyer, Tim P.; Baranova, Olga K.; Reagan, James R.; Seidov, Dan; Smolyar, Igor V.</p> <p>2018-03-01</p> <p>The World <span class="hlt">Ocean</span> Database (WOD) contains over 1.3 million oceanographic casts (where <q>cast</q> refers to an oceanographic profile or set of profiles collected concurrently at more than one depth between the <span class="hlt">ocean</span> surface and <span class="hlt">ocean</span> bottom) collected in the Arctic <span class="hlt">Ocean</span> <span class="hlt">basin</span> and its surrounding marginal seas. The data, collected from 1849 to the present, come from many submitters and countries, and were collected using a variety of instruments and platforms. These data, along with the derived products World <span class="hlt">Ocean</span> Atlas (WOA) and the Arctic Regional Climatologies, are exceptionally useful - the data are presented in a standardized, easy to use format and include metadata and quality control information. Collecting data in the Arctic <span class="hlt">Ocean</span> is challenging, and coverage in space and time ranges from excellent to nearly non-existent. WOD continues to compile a comprehensive collection of Arctic <span class="hlt">Ocean</span> profile data, ideal for oceanographic, environmental and climatic analyses (<a href="https://doi.org/10.7289/V54Q7S16" target="_blank">https://doi.org/10.7289/V54Q7S16</a>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3022W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3022W"><span>Triple seismic source, double research ship, single ambitious goal: integrated imaging of young <span class="hlt">oceanic</span> crust in the Panama <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Dean; Peirce, Christine; Hobbs, Richard; Gregory, Emma</p> <p>2016-04-01</p> <p>Understanding geothermal heat and mass fluxes through the seafloor is fundamental to the study of the Earth's energy budget. Using geophysical, geological and physical oceanography data we are exploring the interaction between the young <span class="hlt">oceanic</span> crust and the <span class="hlt">ocean</span> in the Panama <span class="hlt">Basin</span>. We acquired a unique geophysical dataset that will allow us to build a comprehensive model of young <span class="hlt">oceanic</span> crust from the Costa Rica Ridge axis to ODP borehole 504B. Data were collected over two 35 x 35 km2 3D grid areas, one each at the ridge axis and the borehole, and along three 330 km long 2D profiles orientated in the spreading direction, connecting the two grids. In addition to the 4.5 km long multichannel streamer and 75 <span class="hlt">ocean</span>-bottom seismographs (OBS), we also deployed 12 magnetotelluric (MT) stations and collected underway swath bathymetry, gravity and magnetic data. For the long 2D profiles we used two research vessels operating synchronously. The RRS James Cook towed a high frequency GI-gun array (120 Hz) to image the sediments, and a medium frequency Bolt-gun array (50 Hz) for shallow-to-mid-crustal imaging. The R/V Sonne followed the Cook, 9 km astern and towed a third seismic source; a low frequency, large volume G-gun array (30 Hz) for whole crustal and upper mantle imaging at large offsets. Two bespoke vertical hydrophone arrays recorded real far field signatures that have enabled us to develop inverse source filters and match filters. Here we present the seismic reflection image, forward and inverse velocity-depth models and a density model along the primary 330 km north-south profile, from ridge axis to 6 Ma crust. By incorporating wide-angle streamer data from our two-ship, synthetic aperture acquisition together with traditional wide-angle OBS data we are able to constrain the structure of the upper <span class="hlt">oceanic</span> crust. The results show a long-wavelength trend of increasing seismic velocity and density with age, and a correlation between velocity structure and basement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008DSRI...55..369P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008DSRI...55..369P"><span>Drift pumice in the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span>: Geochemical evidence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattan, J. N.; Mudholkar, A. V.; Jai Sankar, S.; Ilangovan, D.</p> <p>2008-03-01</p> <p>Abundant white to light grey-coloured pumice without ferromanganese oxide coating occurs within the Quaternary sediments of the Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB). Two distinct groups of pumice are identified from their geochemical composition, which allow one to define two different origins linked to two separate eruptions. One group of pumice is a dacitic type characterized by high Fe, Ti, Mg, Al and Ca with comparatively low contents of Si, rare-earth elements (∑REE, 69 ppm), Rb, Sr, U, Th, Ba, V, Nb, Sc, Mo and Co, which strongly suggest an origin from the 1883 Krakatau eruption. The other group is rhyolitic and is characterized by low contents of Fe, Ti, Mg and Ca and high Si, ∑REE content (121 ppm), Rb, Sr, U, Th, Ba, V, Nb, Mo, Co, and Sc and correlates well with the composition of the Youngest Toba Tuff (YTT) eruption of ˜74 ka from Northern Sumatra and is being reported for the first time. Therefore, correlation of the pumice to the 1883 Krakatau and YTT eruptions indicates that the pumice drifted to the CIOB and eventually sank when it became waterlogged. However, physical properties such as density, specific gravity, porosity and degree of saturation required for sinking of pumice for both 1883 Krakatau and YTT are almost similar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195119','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195119"><span>Significance of northeast-trending features in Canada <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</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>Hutchinson, Deborah; Jackson, H.R.; Houseknecht, David W.; Li, Q.; Shimeld, J.W.; Mosher, D.C.; Chian, D.; Saltus, Richard; Oakey, G.N.</p> <p>2017-01-01</p> <p>Synthesis of seismic velocity, potential field, and geological data from Canada <span class="hlt">Basin</span> and its surrounding continental margins suggests that a northeast-trending structural fabric has influenced the origin, evolution, and current tectonics of the <span class="hlt">basin</span>. This structural fabric has a crustal origin, based on the persistence of these trends in upward continuation of total magnetic intensity data and vertical derivative analysis of free-air gravity data. Three subparallel northeast-trending features are described. Northwind Escarpment, bounding the east side of the Chukchi Borderland, extends ∼600 km and separates continental crust of Northwind Ridge from high-velocity transitional crust in Canada <span class="hlt">Basin</span>. A second, shorter northeast-trending zone extends ∼300 km in northern Canada <span class="hlt">Basin</span> and separates inferred continental crust of Sever Spur from magmatically intruded crust of the High Arctic Large Igneous Province. A third northeast-trending feature, here called the Alaska-Prince Patrick magnetic lineament (APPL) is inferred from magnetic data and its larger regional geologic setting. Analysis of these three features suggests strike slip or transtensional deformation played a role in the opening of Canada <span class="hlt">Basin</span>. These features can be explained by initial Jurassic-Early Cretaceous strike slip deformation (phase 1) followed in the Early Cretaceous (∼134 to ∼124 Ma) by rotation of Arctic Alaska with seafloor spreading orthogonal to the fossil spreading axis preserved in the central Canada <span class="hlt">Basin</span> (phase 2). In this model, the Chukchi Borderland is part of Arctic Alaska.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GGG....18.4156H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GGG....18.4156H"><span>Significance of Northeast-Trending Features in Canada <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hutchinson, D. R.; Jackson, H. R.; Houseknecht, D. W.; Li, Q.; Shimeld, J. W.; Mosher, D. C.; Chian, D.; Saltus, R. W.; Oakey, G. N.</p> <p>2017-11-01</p> <p>Synthesis of seismic velocity, potential field, and geological data from Canada <span class="hlt">Basin</span> and its surrounding continental margins suggests that a northeast-trending structural fabric has influenced the origin, evolution, and current tectonics of the <span class="hlt">basin</span>. This structural fabric has a crustal origin, based on the persistence of these trends in upward continuation of total magnetic intensity data and vertical derivative analysis of free-air gravity data. Three subparallel northeast-trending features are described. Northwind Escarpment, bounding the east side of the Chukchi Borderland, extends ˜600 km and separates continental crust of Northwind Ridge from high-velocity transitional crust in Canada <span class="hlt">Basin</span>. A second, shorter northeast-trending zone extends ˜300 km in northern Canada <span class="hlt">Basin</span> and separates inferred continental crust of Sever Spur from magmatically intruded crust of the High Arctic Large Igneous Province. A third northeast-trending feature, here called the Alaska-Prince Patrick magnetic lineament (APPL) is inferred from magnetic data and its larger regional geologic setting. Analysis of these three features suggests strike slip or transtensional deformation played a role in the opening of Canada <span class="hlt">Basin</span>. These features can be explained by initial Jurassic-Early Cretaceous strike slip deformation (phase 1) followed in the Early Cretaceous (˜134 to ˜124 Ma) by rotation of Arctic Alaska with seafloor spreading orthogonal to the fossil spreading axis preserved in the central Canada <span class="hlt">Basin</span> (phase 2). In this model, the Chukchi Borderland is part of Arctic Alaska.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017BGeo...14.5727K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017BGeo...14.5727K"><span>Low pCO2 under sea-ice melt in the Canada <span class="hlt">Basin</span> of the western Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kosugi, Naohiro; Sasano, Daisuke; Ishii, Masao; Nishino, Shigeto; Uchida, Hiroshi; Yoshikawa-Inoue, Hisayuki</p> <p>2017-12-01</p> <p>In September 2013, we observed an expanse of surface water with low CO2 partial pressure (pCO2sea) (< 200 µatm) in the Chukchi Sea of the western Arctic <span class="hlt">Ocean</span>. The large undersaturation of CO2 in this region was the result of massive primary production after the sea-ice retreat in June and July. In the surface of the Canada <span class="hlt">Basin</span>, salinity was low (< 27) and pCO2sea was closer to the air-sea CO2 equilibrium (˜ 360 µatm). From the relationships between salinity and total alkalinity, we confirmed that the low salinity in the Canada <span class="hlt">Basin</span> was due to the larger fraction of meltwater input (˜ 0.16) rather than the riverine discharge (˜ 0.1). Such an increase in pCO2sea was not so clear in the coastal region near Point Barrow, where the fraction of riverine discharge was larger than that of sea-ice melt. We also identified low pCO2sea (< 250 µatm) in the depth of 30-50 m under the halocline of the Canada <span class="hlt">Basin</span>. This subsurface low pCO2sea was attributed to the advection of Pacific-origin water, in which dissolved inorganic carbon is relatively low, through the Chukchi Sea where net primary production is high. Oxygen supersaturation (> 20 µmol kg-1) in the subsurface low pCO2sea layer in the Canada <span class="hlt">Basin</span> indicated significant net primary production undersea and/or in preformed condition. If these low pCO2sea layers surface by wind mixing, they will act as additional CO2 sinks; however, this is unlikely because intensification of stratification by sea-ice melt inhibits mixing across the halocline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/3033','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/3033"><span>Research information needs on terrestrial vertebrate species of the interior Columbia <span class="hlt">basin</span> and northern portions of the Klamath and Great <span class="hlt">Basins</span>: a research, development, and application database.</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Bruce G. Marcot</p> <p>1997-01-01</p> <p>Research information needs on selected invertebrates and all vertebrates of the interior Columbia River <span class="hlt">basin</span> and <span class="hlt">adjacent</span> areas in the United States were collected into a research, development, and application database as part of the Interior Columbia <span class="hlt">Basin</span> Ecosystem Management Project. The database includes 482 potential research study topics on 232 individual...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Geomo.313...27S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Geomo.313...27S"><span>Morphology and shallow structure of seafloor mounds in the Canary <span class="hlt">Basin</span> (Eastern Central Atlantic <span class="hlt">Ocean</span>)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sanchez-Guillamón, O.; Vázquez, J. T.; Palomino, D.; Medialdea, T.; Fernández-Salas, L. M.; León, R.; Somoza, L.</p> <p>2018-07-01</p> <p>The increasing volume of high-resolution multibeam bathymetry data collected along continental margins and <span class="hlt">adjacent</span> deep seafloor regions is providing further opportunities to study new morphological seafloor features in deep water environments. In this paper, seafloor mounds have been imaged in detail with multibeam echosounders and parametric sub-bottom profilers in the deep central area of the Canary <span class="hlt">Basin</span> ( 350-550 km west off El Hierro Island) between 4800 and 5200 mbsl. These features have circular to elongated shapes with heights of 10 to 250 m, diameters of 2-24 km and with flank slopes of 2-50°. Based on their morphological features and the subsurface structures these mounds have been classified into five different types of mounds that follow a linear correlation between height and slope but not between height and size. The first, second (Subgroup A), and third mound-types show heights lower than 80 m and maximum slopes of 35° with extension ranging from 2 to 400 km2 and correspond to domes formed at the surface created by intrusions located at depth that have not outcropped yet. The second (Subgroup B), fourth, and fifth mound-types show higher heights up to 250 m high, maximum slopes of 47° and sizes between 10 and 20 km2 and are related to the expulsion of hot and hydrothermal fluids and/or volcanics from extrusive deep-seated systems. Based on the constraints on their morphological and structural analyses, we suggest that morphostructural types of mounds are intimately linked to a specific origin that leaves its footprint in the morphology of the mounds. We propose a growth model for the five morphostructural types of mounds where different intrusive and extrusive phenomena represent the dominant mechanisms for mound growth evolution. These structures are also affected by tectonics (bulge-like structures clearly deformed by faulting) and mass movements (slide scars and mass transport deposits). In this work, we report how intrusive and extrusive</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 sediments in coastal, island arc and <span class="hlt">oceanic</span> <span class="hlt">basins</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>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 sediments accumulated beneath high productivity zones in coastal, island arc and <span class="hlt">oceanic</span> <span class="hlt">basins</span>. Most of these deposits now crop out in fault-bounded accreted terranes. Biogenic siliceous sediments 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 sediments beneath high productivity zones in many parts of the Pacific and concurrent deposition of phosphatic as well as siliceous sediments in <span class="hlt">basins</span> 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://pubs.usgs.gov/wsp/2316/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/2316/report.pdf"><span>Methods for delineating flood-prone areas in the Great <span class="hlt">Basin</span> of Nevada and <span class="hlt">adjacent</span> states</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Burkham, D.E.</p> <p>1988-01-01</p> <p>The Great <span class="hlt">Basin</span> is a region of about 210,000 square miles having no surface drainage to the <span class="hlt">ocean</span>; it includes most of Nevada and parts of Utah, California, Oregon, Idaho, and Wyoming. The area is characterized by many parallel mountain ranges and valleys trending north-south. Stream channels usually are well defined and steep within the mountains, but on reaching the alluvial fan at the canyon mouth, they may diverge into numerous distributary channels, be discontinuous near the apex of the fan, or be deeply entrenched in the alluvial deposits. Larger rivers normally have well-defined channels to or across the valley floors, but all terminate at lakes or playas. Major floods occur in most parts of the Great <span class="hlt">Basin</span> and result from snowmelt, frontal-storm rainfall, and localized convective rainfall. Snowmelt floods typically occur during April-June. Floods resulting from frontal rain and frontal rain on snow generally occur during November-March. Floods resulting from convective-type rainfall during localized thunderstorms occur most commonly during the summer months. Methods for delineating flood-prone areas are grouped into five general categories: Detailed, historical, analytical, physiographic, and reconnaissance. The detailed and historical methods are comprehensive methods; the analytical and physiographic are intermediate; and the reconnaissance method is only approximate. Other than the reconnaissance method, each method requires determination of a T-year discharge (the peak rate of flow during a flood with long-term average recurrence interval of T years) and T-year profile and the development of a flood-boundary map. The procedure is different, however, for each method. Appraisal of the applicability of each method included consideration of its technical soundness, limitations and uncertainties, ease of use, and costs in time and money. Of the five methods, the detailed method is probably the most accurate, though most expensive. It is applicable to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA574456','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA574456"><span>The Influence of Atmosphere-<span class="hlt">Ocean</span> Interaction on MJO Development and Propagation</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2012-09-30</p> <p>feedbacks and their influence on MJO development, and for forecasting of air sea interaction in the Indian <span class="hlt">Ocean</span> <span class="hlt">basin</span> and its influence on MJO. The...indicating precipitation maximum over the DYNAMO area and the red line indicating the precipitation anomaly west of Sumatra . The corresponding EOF...characterizing the November episode, relatively weaker October episode and convection situated in the eastern part of the Indian <span class="hlt">Ocean</span> <span class="hlt">basin</span> in December</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.6964L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.6964L"><span><span class="hlt">Ocean</span> bottom characterestics between Iles Rodrigues and Chagos-Maldives Archepelago in western Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Longhinos, Biju; Thanu Iyer, Radhakrishnan; Mohan, Karthika</p> <p>2014-05-01</p> <p>The geological and geophysical complexities in Indian <span class="hlt">ocean</span> <span class="hlt">basin</span>, pointed out by many earlier workers remained unresolved. Instead, taking aid from stop gap arguments, the data has been construed to follow plate tectonics format. The concept of large igneous complexes emplaced through crustal drifting ( between the India and Mozambique) during later Mesozoic to Recent fail to address geophysical characteristics exhibited here. The geophysical signatures of the sub crustal part of the <span class="hlt">ocean</span> here resemble to that of continental regions elsewhere. Granites, greenstones and mylonized gabbro, recovered from the western Indian <span class="hlt">ocean</span> <span class="hlt">basin</span>, rather give Late Pre- Cambrian and Paleozoic isotopic dates. Under this light, the present paper looks into the <span class="hlt">ocean</span> bottom characteristics of a region between iles Rodrigues and Chagos- Maldives archipelago. The region has first order curvilienar fractures, with along which the crust has displaced more than 1000m. The sea-bottom topography of the region has been modeled in Geographical Information System environment using Modified ETOPO5 provided by National Institute of Oceanography. The spatial relationship of topography with gravity and magnetic data area are analysed visually and mathematically. The detail bathymetry, gravity and magnetic data give morphology similar to that of half graben formed on a felsic crust, which later has undergone basification / eclogitization through first order fracture zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2018/3026/fs20183026_v1.1.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2018/3026/fs20183026_v1.1.pdf"><span>Groundwater quality in the shallow aquifers of the Monterey Bay, Salinas Valley, and <span class="hlt">adjacent</span> highland areas, 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>Burton, Carmen</p> <p>2018-05-30</p> <p>Groundwater provides more than 40 percent of California’s drinking water. To protect this vital resource, the State of California created the Groundwater Ambient Monitoring and Assessment (GAMA) Program. The Priority <span class="hlt">Basin</span> Project of the GAMA Program provides a comprehensive assessment of the State’s groundwater quality and increases public access to groundwater-quality information. The shallow aquifers of the groundwater <span class="hlt">basins</span> around Monterey Bay, the Salinas Valley, and the highlands <span class="hlt">adjacent</span> to the Salinas Valley constitute one of the study units.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1816170W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1816170W"><span>Indo-Pacific ENSO modes in a double-<span class="hlt">basin</span> Zebiak-Cane model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wieners, Claudia; de Ruijter, Will; Dijkstra, Henk</p> <p>2016-04-01</p> <p>We study Indo-Pacific interactions on ENSO timescales in a double-<span class="hlt">basin</span> version of the Zebiak-Cane ENSO model, employing both time integrations and bifurcation analysis (continuation methods). The model contains two <span class="hlt">oceans</span> (the Indian and Pacific <span class="hlt">Ocean</span>) separated by a meridional wall. Interaction between the <span class="hlt">basins</span> is possible via the atmosphere overlaying both <span class="hlt">basins</span>. We focus on the effect of the Indian <span class="hlt">Ocean</span> (both its mean state and its variability) on ENSO stability. In addition, inspired by analysis of observational data (Wieners et al, Coherent tropical Indo-Pacific interannual climate variability, in review), we investigate the effect of state-dependent atmospheric noise. Preliminary results include the following: 1) The background state of the Indian <span class="hlt">Ocean</span> stabilises the Pacific ENSO (i.e. the Hopf bifurcation is shifted to higher values of the SST-atmosphere coupling), 2) the West Pacific cooling (warming) co-occurring with El Niño (La Niña) is essential to simulate the phase relations between Pacific and Indian SST anomalies, 3) a non-linear atmosphere is needed to simulate the effect of the Indian <span class="hlt">Ocean</span> variability onto the Pacific ENSO that is suggested by observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1511412L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1511412L"><span>Possible Origin of High-Amplitude Reflection Packages (HARPs) in the Canada <span class="hlt">Basin</span>, Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lebedeva-Ivanova, Nina; Hutchinson, Deborah; Shimeld, John; Chian, Deping; Hart, Patrick; Jackson, Ruth; Saltus, Richard; Mosher, David</p> <p>2013-04-01</p> <p>The Canada <span class="hlt">Basin</span> (CB) of the Arctic <span class="hlt">Ocean</span> is a semi-enclosed <span class="hlt">ocean</span> <span class="hlt">basin</span> surrounded by the Alaskan and Canadian margins to the south and east, the Alpha-Mendeleev Large Igneous Province (AMLIP) to the north and the subsided continental Chukchi Borderland (ChB) to the west. During 2007-2011, US-Canada expeditions collected ~15,000 km multichannel seismic data and sonobuoy reflection and refraction seismic data with average spacing of ~80 km mostly over the CB and AMLIP. High-amplitude reflective packages (HARPs) underlie the mostly flat-lying sediments of CB. Although HARPs are discontinuous in the central CB, they become more continuous toward ChB and AMLIP. HARPs are often the most reflective events in the seismic section, exceeding even the seafloor reflection. Only rarely are reflections seen beneath HARPs. Where best developed, HARPs are ~100-300 ms TWTT, consisting of several high-amplitude wavelets with a pronounced narrow frequency band within the limits of ~10-30 Hz. This character of HARPs is consistent with patterns produced by constructive interference of thin beds (Widess, 1973). Forward modeling of sonobuoy data, synthetic tests, and frequency analysis of the tuning effect suggest that HARPs are composed of a series of alternating high- and low-velocity layers. The high-velocity layers are ~100-200 m thick with P-velocities of ~3.5-4.5 km/s. The low-velocity layers are about half as thick with velocities of ~2-3 km/s. A broad range of possible interpretations of rock composition exists from these velocities, e.g. sandstone and interbedded shale (Prince Patrick Island, Harrison and Brent, 2005); or tholeiitic basalts flows and sediments (Voring volcanic margin, Olanke and Eldholm, 1994); or sills and sediments (Newfoundland margin, Peron-Pinvidic et all, 2010). HARP can be associated with several origins. In the central and southern CB, where <span class="hlt">oceanic</span> spreading is interpreted, HARPs are discontinuous among high-relief, but otherwise low</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT.......206G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT.......206G"><span>Mechanisms of <span class="hlt">Ocean</span> Heat Uptake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garuba, Oluwayemi</p> <p></p> <p>An important parameter for the climate response to increased greenhouse gases or other radiative forcing is the speed at which heat anomalies propagate downward in the <span class="hlt">ocean</span>. <span class="hlt">Ocean</span> heat uptake occurs through passive advection/diffusion of surface heat anomalies and through the redistribution of existing temperature gradients due to circulation changes. Atlantic meridional overturning circulation (AMOC) weakens in a warming climate and this should slow the downward heat advection (compared to a case in which the circulation is unchanged). However, weakening AMOC also causes a deep warming through the redistributive effect, thus increasing the downward rate of heat propagation compared to unchanging circulation. Total heat uptake depends on the combined effect of these two mechanisms. Passive tracers in a perturbed CO2 quadrupling experiments are used to investigate the effect of passive advection and redistribution of temperature anomalies. A new passive tracer formulation is used to separate <span class="hlt">ocean</span> heat uptake into contributions due to redistribution and passive advection-diffusion of surface heating during an <span class="hlt">ocean</span> model experiment with abrupt increase in surface temperature. The spatial pattern and mechanisms of each component are examined. With further experiments, the effects of surface wind, salinity and temperature changes in changing circulation and the resulting effect on redistribution in the individual <span class="hlt">basins</span> are isolated. Analysis of the passive advection and propagation path of the tracer show that the Southern <span class="hlt">ocean</span> dominates heat uptake, largely through vertical and horizontal diffusion. Vertical diffusion transports the tracer across isopycnals down to about 1000m in 100 years in the Southern <span class="hlt">ocean</span>. Advection is more important in the subtropical cells and in the Atlantic high latitudes, both with a short time scale of about 20 years. The shallow subtropical cells transport the tracer down to about 500m along isopycnal surfaces, below this vertical</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740018792','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740018792"><span>An ecological study of the KSC Turning <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> waters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nevin, T. A.; Lasater, J. A.; Clark, K. B.; Kalajian, E. H.</p> <p>1974-01-01</p> <p>The conditions existing in the waters and bottoms of the Turning <span class="hlt">Basin</span>, the borrow pit near Pad 39A, and the Barge Canal connecting them were investigated to determine the ecological significance of the chemical, biological, and microbiological parameters. The water quality, biological, microbiological findings are discussed. It is recommended that future dredging activities be limited in depth, and that fill materials should not be removed down to the clay strata.</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/2008AGUFM.T51B1895B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.T51B1895B"><span>Impact of Vishnu Fracture Zone on Tectono-Stratigraphy of Kerala Deepwater <span class="hlt">Basin</span>, 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 zones in Indian <span class="hlt">Ocean</span>. Kerala deepwater <span class="hlt">basin</span>, situated in the south-western tip of India, is bounded by two prominent north-south oriented <span class="hlt">ocean</span> fracture zones viz., Vishnu (west) and Indrani (east) of the Indian <span class="hlt">Ocean</span>. Vishnu Fracture Zone (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 sedimentation as well as structural fabric of the <span class="hlt">basin</span>. 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 <span class="hlt">ocean</span> 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 <span class="hlt">ocean</span> 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 <span class="hlt">Basin</span>, unheard earlier. Multi-episodic rifting in western continental margin of India starting during Mid Jurassic Karoo rift along the western Madagascar, Kerala deepwater <span class="hlt">basin</span>, and western Antarctica and conjugate margins of Africa forms the main corridor for sedimentation. Subsequent Late Cretaceous dextral oblique extension of Madagascar rift reactivated pre-existing structural framework creating major accommodation zones along the southern tip of India. Followed by separation of Seychelles during KT boundary led to the formation of VFZ (an <span class="hlt">oceanic</span> fracture zone) forming a transform boundary between newly formed Tertiary <span class="hlt">oceanic</span> crust to the west and older <span class="hlt">basin</span> to the east. The pulses of right-lateral movement were associated</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19760022699','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19760022699"><span>Thermal and mechanical structure of the upper mantle: A comparison between continental and <span class="hlt">oceanic</span> models</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Froidevaux, C.; Schubert, G.; Yuen, D. A.</p> <p>1976-01-01</p> <p>Temperature, velocity, and viscosity profiles for coupled thermal and mechanical models of the upper mantle beneath continental shields and old <span class="hlt">ocean</span> <span class="hlt">basins</span> show that under the continents, both tectonic plates and the asthenosphere, are thicker than they are beneath the <span class="hlt">oceans</span>. The minimum value of viscosity in the continental asthenosphere is about an order of magnitude larger than in the shear zone beneath <span class="hlt">oceans</span>. The shear stress or drag underneath continental plates is also approximately an order of magnitude larger than the drag on <span class="hlt">oceanic</span> plates. Effects of shear heating may account for flattening of <span class="hlt">ocean</span> floor topography and heat flux in old <span class="hlt">ocean</span> <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1013930','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1013930"><span>Canada <span class="hlt">Basin</span> Acoustic Propagation Experiment (CANAPE)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-09-30</p> <p>1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. Canada <span class="hlt">Basin</span> Acoustic Propagation Experiment (CANAPE...<span class="hlt">ocean</span> structure. Changes in sea ice and the water column affect both acoustic propagation and ambient noise. This implies that what was learned...about Arctic acoustics during the Cold War is now obsolete. The goal of the Canada <span class="hlt">Basin</span> Acoustic Propagation Experiment (CANAPE) is to determine the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGP11A..06H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGP11A..06H"><span>A paleomagnetic and relative paleointensity record from the Argentine <span class="hlt">Basin</span> (western South Atlantic <span class="hlt">Ocean</span>) for the last ~125 kyrs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heil, C. W., Jr.; Stoner, J. S.; St-Onge, G.; King, J. W.</p> <p>2015-12-01</p> <p>The paucity of paleomagnetic records from the western South Atlantic <span class="hlt">Ocean</span> presents a significant gap in our understanding of the spatial variations in geomagnetic field dynamics as they relate to the occurrence of geomagnetic excursions and changes in field strength. As such, high quality records from this region can help build upon Holocene observations and extend the geographic and temporal data coverage for spherical harmonic models. To that end, we present paleomagnetic directional (inclination) and strength (relative paleointensity) records from two cores from the Argentine <span class="hlt">Basin</span> (RC11-49 and RC16-88). Although the cores were collected more than 40 years ago, the sediments appear to hold a stable remanence and reliable magnetic directions, as evidenced by their reproducibility between the two cores that are separated by ~25 km. The records show evidence of 4 excursional features in the uppermost 16-m of the sediments from the <span class="hlt">basin</span>. A comparison of the relative paleointensity records from these cores to the South Atlantic Paleointensity Stack (SAPIS) (Stoner et al., 2002) and the relative paleointensity record from ODP Site 1089 (Stoner et al., 2003) indicate that the sediments reliably record relative changes in geomagnetic field intensity and suggests that the longest record (RC11-49) spans the last ~125 kyrs. Our results indicate that the sediments of the Argentine <span class="hlt">Basin</span> are an important sedimentary archive of geomagnetic field behavior and strength at least through the Holocene and Late Pleistocene and highlight the need for further studies of cores within the <span class="hlt">basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2006/1174/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1174/"><span>Gas desorption and adsorption isotherm studies of coals in the Powder River <span class="hlt">basin</span>, Wyoming and <span class="hlt">adjacent</span> <span class="hlt">basins</span> in Wyoming and North Dakota</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Stricker, Gary D.; Flores, Romeo M.; McGarry, Dwain E.; Stillwell, Dean P.; Hoppe, Daniel J.; Stillwell, Cathy R.; Ochs, Alan M.; Ellis, Margaret S.; Osvald, Karl S.; Taylor, Sharon L.; Thorvaldson, Marjorie C.; Trippi, Michael H.; Grose, Sherry D.; Crockett, Fred J.; Shariff, Asghar J.</p> <p>2006-01-01</p> <p>The U.S. Geological Survey (USGS), in cooperation with the State Office, Reservoir Management Group (RMG), of the Bureau of Land Management (BLM) in Casper (Wyoming), investigated the coalbed methane resources (CBM) in the Powder River <span class="hlt">Basin</span>, Wyoming and Montana, from 1999 to the present. Beginning in late 1999, the study also included the Williston <span class="hlt">Basin</span> in Montana and North and South Dakota and Green River <span class="hlt">Basin</span> and Big Horn <span class="hlt">Basin</span> in Wyoming. The rapid development of CBM (referred to as coalbed natural gas by the BLM) during the early 1990s, and the lack of sufficient data for the BLM to fully assess and manage the resource in the Powder River <span class="hlt">Basin</span>, in particular, gave impetus to the cooperative program. An integral part of the joint USGS-BLM project was the participation of 25 gas operators that entered individually into confidential agreements with the USGS, and whose cooperation was essential to the study. The arrangements were for the gas operators to drill and core coal-bed reservoirs at their cost, and for the USGS and BLM personnel to then desorb, analyze, and interpret the coal data with joint funding by the two agencies. Upon completion of analyses by the USGS, the data were to be shared with both the BLM and the gas operator that supplied the core, and then to be released or published 1 yr after the report was submitted to the operator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3770696','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3770696"><span>Baseline Monitoring of the Western Arctic <span class="hlt">Ocean</span> Estimates 20% of Canadian <span class="hlt">Basin</span> Surface Waters Are Undersaturated with Respect to Aragonite</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Robbins, Lisa L.; Wynn, Jonathan G.; Lisle, John T.; Yates, Kimberly K.; Knorr, Paul O.; Byrne, Robert H.; Liu, Xuewu; Patsavas, Mark C.; Azetsu-Scott, Kumiko; Takahashi, Taro</p> <p>2013-01-01</p> <p>Marine surface waters are being acidified due to uptake of anthropogenic carbon dioxide, resulting in surface <span class="hlt">ocean</span> areas of undersaturation with respect to carbonate minerals, including aragonite. In the Arctic <span class="hlt">Ocean</span>, acidification is expected to occur at an accelerated rate with respect to the global <span class="hlt">oceans</span>, but a paucity of baseline data has limited our understanding of the extent of Arctic undersaturation and of regional variations in rates and causes. The lack of data has also hindered refinement of models aimed at projecting future trends of <span class="hlt">ocean</span> acidification. Here, based on more than 34,000 data records collected in 2010 and 2011, we establish a baseline of inorganic carbon data (pH, total alkalinity, dissolved inorganic carbon, partial pressure of carbon dioxide, and aragonite saturation index) for the western Arctic <span class="hlt">Ocean</span>. This data set documents aragonite undersaturation in ∼20% of the surface waters of the combined Canada and Makarov <span class="hlt">basins</span>, an area characterized by recent acceleration of sea ice loss. Conservative tracer studies using stable oxygen isotopic data from 307 sites show that while the entire surface of this area receives abundant freshwater from meteoric sources, freshwater from sea ice melt is most closely linked to the areas of carbonate mineral undersaturation. These data link the Arctic Ocean’s largest area of aragonite undersaturation to sea ice melt and atmospheric CO2 absorption in areas of low buffering capacity. Some relatively supersaturated areas can be linked to localized biological activity. Collectively, these observations can be used to project trends of <span class="hlt">ocean</span> acidification in higher latitude marine surface waters where inorganic carbon chemistry is largely influenced by sea ice meltwater. PMID:24040074</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850015231&hterms=multi+location&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmulti%2Blocation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850015231&hterms=multi+location&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dmulti%2Blocation"><span>Ring-diameter Ratios for Multi-ring <span class="hlt">Basins</span> Average 2.0(0.5)D</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Pike, R. J.; Spudis, P. D.</p> <p>1985-01-01</p> <p>The spacing of the concentric rings of planetary impact <span class="hlt">basins</span> was studied. It is shown that a radial increment of x (sup 0.5) D, where x is about 2.0 and D = ring diameter, separates both (1) <span class="hlt">adjacent</span> least-squares groups of rings and arcs of multi-ring <span class="hlt">basins</span> on Mars, Mercury, and the Moon; and (2) <span class="hlt">adjacent</span> rings of individual <span class="hlt">basins</span> on the three planets. Statistics for ratios of ring diameters are presented, the first and most-applied parameter of ring spacing. It is found that ratios excluding rings flanking the main ring also have a mean spacing increment of about 2.0. Ratios including such rings, as for the least-squares groups, and (1) above, have a larger increment, averaging 2.1. The F-test indicates, that these spacings of <span class="hlt">basin</span> ring locations, and mode of ring formation are controlled by the mechanics of the impact event itself, rather than by crustal properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.2424C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.2424C"><span>Abyssal Upwelling in Mid-<span class="hlt">Ocean</span> Ridge Fracture Zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clément, Louis; Thurnherr, Andreas M.</p> <p>2018-03-01</p> <p>Turbulence in the abyssal <span class="hlt">ocean</span> plays a fundamental role in the climate system by sustaining the deepest branch of the overturning circulation. Over the western flank of the Mid-Atlantic Ridge in the South Atlantic, previously observed bottom-intensified and tidally modulated mixing of abyssal waters appears to imply a counterintuitive densification of deep and bottom waters. Here we show that inside fracture zones, however, turbulence is elevated away from the seafloor because of intensified downward propagating near-inertial wave energy, which decays below a subinertial shear maximum. Ray-tracing simulations predict a decay of wave energy subsequent to wave-mean flow interactions. The hypothesized wave-mean flow interactions drive a deep flow toward lighter densities of up to 0.6 Sv over the mid-<span class="hlt">ocean</span> ridge flank in the Brazil <span class="hlt">Basin</span>, and the same process may also cause upwelling of abyssal waters in other <span class="hlt">ocean</span> <span class="hlt">basins</span> with mid-<span class="hlt">ocean</span> ridges with fracture zones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS41B1952W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS41B1952W"><span>Mooring Measurements of the Abyssal Circulations in the Western Pacific <span class="hlt">Ocean</span></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.; Wang, F.</p> <p>2016-12-01</p> <p>A scientific observing network in the western tropical Pacific has initially been established by the Institute of Oceanology, Chinese Academy of Sciences (IOCAS). Using fifteen moorings that gives unprecedented measurements in the intermediate and abyssal layers, we present multi-timescale variations of the deep <span class="hlt">ocean</span> circulations prior to and during 2015 El Niño event. The deep <span class="hlt">ocean</span> velocities increase equatorward with high standard deviation and nearly zero mean. The deep <span class="hlt">ocean</span> currents mainly flow in meridional direction in the central Philippine <span class="hlt">Basin</span>, and are dominated by a series of alternating westward and eastward zonal jets in the Caroline <span class="hlt">Basin</span>. The currents in the deep channel connecting the East and West Mariana <span class="hlt">Basins</span> mainly flow southeastward. Seasonal variation is only present in the deep jets in the Caroline <span class="hlt">Basin</span>, associating with vertical propagating annual Rossby wave. The high-frequency flow bands are dominated by diurnal, and semi-diurnal tidal currents, and near-inertial currents. The rough topography has a strong influence on the abyssal circulations, including the intensifications in velocity and internal tidal energy, and the formation of upwelling flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015347','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015347"><span>Geologic framework of the offshore region <span class="hlt">adjacent</span> to Delaware</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Benson, R.N.; Roberts, J.H.</p> <p>1989-01-01</p> <p> postrift sediments that cover the more deeply buried rift <span class="hlt">basins</span> are estimated to be of Middle Jurassic age (Bajocian-Bathonian), the probable time of opening of the Atlantic <span class="hlt">Ocean</span> <span class="hlt">basin</span> and onset of continental drift about 175-180 m.y. ago. By late Oxfordian-early Kimmeridgian time, the less deeply buried <span class="hlt">basins</span> nearshore Delaware had been covered. A time-temperature index of maturity plot of one of the <span class="hlt">basins</span> indicates that only dry gas would be present in reservoirs in synrift rocks buried by more than 6000 m of postrift sediments and in the oldest (Bathonian?-Callovian?) postrift rocks. Less deeply buried synrift rocks landward of the <span class="hlt">basin</span> modeled might still be within the oil generation window. ?? 1989.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15794819','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15794819"><span><span class="hlt">Ocean</span> climate and seal condition.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Le Boeuf, Burney J; Crocker, Daniel E</p> <p>2005-03-28</p> <p>The condition of many marine mammals varies with fluctuations in productivity and food supply in the <span class="hlt">ocean</span> <span class="hlt">basin</span> where they forage. Prey is impacted by physical environmental variables such as cyclic warming trends. The weaning weight of northern elephant seal pups, Mirounga angustirostris, being closely linked to maternal condition, indirectly reflects prey availability and foraging success of pregnant females in deep waters of the northeastern Pacific. The aim of this study was to examine the effect of <span class="hlt">ocean</span> climate on foraging success in this deep-diving marine mammal over the course of three decades, using cohort weaning weight as the principal metric of successful resource accrual. The mean annual weaning weight of pups declined from 1975 to the late 1990s, a period characterized by a large-scale, <span class="hlt">basin</span>-wide warm decadal regime that included multiple strong or long-duration El Niños; and increased with a return to a cool decadal regime from about 1999 to 2004. Increased foraging effort and decreased mass gain of adult females, indicative of reduced foraging success and nutritional stress, were associated with high <span class="hlt">ocean</span> temperatures. Despite ranging widely and foraging deeply in cold waters beyond coastal thermoclines in the northeastern Pacific, elephant seals are impacted significantly by <span class="hlt">ocean</span> thermal dynamics. <span class="hlt">Ocean</span> warming redistributes prey decreasing foraging success of females, which in turn leads to lower weaning mass of pups. Annual fluctuations in weaning mass, in turn, reflect the foraging success of females during the year prior to giving birth and signals changes in <span class="hlt">ocean</span> temperature cycles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035509','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035509"><span>Late Quaternary sediment-accumulation rates within the inner <span class="hlt">basins</span> of the California Continental Borderland in support of geologic hazard evaluation</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Normark, W.R.; McGann, M.; Sliter, R.W.</p> <p>2009-01-01</p> <p>An evaluation of the geologic hazards of the inner California Borderland requires determination of the timing for faulting and mass-movement episodes during the Holocene. Our effort focused on <span class="hlt">basin</span> slopes and turbidite systems on the <span class="hlt">basin</span> floors for the area between Santa Barbara and San Diego, California. Dating condensed sections on slopes <span class="hlt">adjacent</span> to fault zones provides better control on fault history where high-resolution, seismic-reflection data can be used to correlate sediment between the core site and the fault zones. This study reports and interprets 147 radiocarbon dates from 43 U.S. Geological Survey piston cores as well as 11 dates from <span class="hlt">Ocean</span> Drilling Program Site 1015 on the floor of Santa Monica <span class="hlt">Basin</span>. One hundred nineteen dates from 39 of the piston cores have not previously been published. Core locations were selected for hazard evaluation, but despite the nonuniform distribution of sample locations, the dates obtained for the late Quaternary deposits are useful for documenting changes in sediment-accumulation rates during the past 30 ka. Cores from <span class="hlt">basins</span> receiving substantial sediment from rivers, i.e., Santa Monica <span class="hlt">Basin</span> and the Gulf of Santa Catalina, show a decrease in sediment supply during the middle Holocene, but during the late Holocene after sea level had reached the current highstand condition, rates then increased partly in response to an increase in El Ni??o-Southern Oscillation events during the past 3.5 ka. ?? 2009 The Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.1048P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.1048P"><span>Arctic <span class="hlt">Ocean</span> Circulation Patterns Revealed by GRACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peralta-Ferriz, Cecilia; Morison, James H.; Wallace, John M.; Bonin, Jennifer A.; Zhang, Jinlun</p> <p>2013-04-01</p> <p>EOF analysis of non-seasonal, month-to-month variations in GRACE derived Arctic <span class="hlt">Ocean</span> bottom pressure (OBP) yield three dominant modes. The first mode is a wintertime <span class="hlt">basin</span> wide variation in mass associated with high atmospheric pressure (SLP) over Scandinavia. The second mode is a shift of mass from the central Arctic <span class="hlt">Ocean</span> to the Siberian shelves due to low pressure over the <span class="hlt">basins</span>, associated with the strength of the Arctic Oscillation. The third mode is a shift in mass between the Eastern and Western Siberian shelves, related to strength of the Beaufort High mainly in summer, and to eastward alongshore winds on the Barents Sea in winter. The PIOMAS and ECCO2 modeled OBP are consistent with the form of these modes and provide context in terms of variations in sea surface height. The models are used to investigate the <span class="hlt">ocean</span> dynamics associated with each mode of OBP variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51H2178C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51H2178C"><span>Using trajectories to explain the moisture budget asymmetry between the Atlantic and Pacific <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Craig, P.; Ferreira, D.; Methven, J.</p> <p>2017-12-01</p> <p>The net surface water flux (evaporation minus precipitation minus runoff, E-P-R) of the Atlantic <span class="hlt">Ocean</span> is approximately 0.4 - 0.6 Sv (1 Sv = 109 kg s-1) larger than that of the Pacific <span class="hlt">Ocean</span>, as shown in atmospheric and <span class="hlt">oceanic</span> reanalyses and by oceanographic estimates. This asymmetry is linked to the asymmetry in sea surface salinity and the existence of the Atlantic Meridional Overturning Circulation. It is shown that the reason for the asymmetry in E-P-R is greater precipitation per unit area over the Pacific south of 30N, while evaporation rates are similar over both <span class="hlt">basins</span>. It is further argued that the Pacific <span class="hlt">Ocean</span> is anomalous compared to the Atlantic and Indian <span class="hlt">Oceans</span> in terms of atmospheric moisture flux convergence and precipitation across the tropics and subtropics. To clarify the mechanism by which water vapour is exported out of the Atlantic <span class="hlt">basin</span> and imported into the Pacific, we use an air mass trajectory model driven by ERA-Interim reanalysis. Using 12-hourly releases of 14-day back trajectories on the boundaries of <span class="hlt">ocean</span> drainage <span class="hlt">basins</span> over the period 2010-2014, we are able to partition the atmospheric moisture fluxes between <span class="hlt">basins</span> according to their origins (i.e. last contact with the boundary layer). We show that at most a quarter of the E-P-R asymmetry is explained by higher moisture export to the Arctic and Southern <span class="hlt">basins</span> from the Atlantic than from the Pacific. The main contributions come from differences in the longitudinal atmospheric transport of moisture between the Atlantic, Indian and Pacific <span class="hlt">basins</span>. In particular, during the Asian summer monsoon the recurvature of the low level flow in the Somali Jet results in a much weaker westward moisture transport from the Indian into the Atlantic <span class="hlt">basin</span> than across Central America (where it is similar to the zonal average) while there is stronger eastward transport from the Indian to Pacific <span class="hlt">basins</span>. The net effect is stronger moisture convergence into the Pacific, but weaker into the Atlantic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20120008820','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20120008820"><span>Does <span class="hlt">Ocean</span> Color Data Assimilation Improve Estimates of Global <span class="hlt">Ocean</span> Inorganic Carbon?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson</p> <p>2012-01-01</p> <p><span class="hlt">Ocean</span> color data assimilation has been shown to dramatically improve chlorophyll abundances and distributions globally and regionally in the <span class="hlt">oceans</span>. Chlorophyll is a proxy for phytoplankton biomass (which is explicitly defined in a model), and is related to the inorganic carbon cycle through the interactions of the organic carbon (particulate and dissolved) and through primary production where inorganic carbon is directly taken out of the system. Does <span class="hlt">ocean</span> color data assimilation, whose effects on estimates of chlorophyll are demonstrable, trickle through the simulated <span class="hlt">ocean</span> carbon system to produce improved estimates of inorganic carbon? Our emphasis here is dissolved inorganic carbon, pC02, and the air-sea flux. We use a sequential data assimilation method that assimilates chlorophyll directly and indirectly changes nutrient concentrations in a multi-variate approach. The results are decidedly mixed. Dissolved organic carbon estimates from the assimilation model are not meaningfully different from free-run, or unassimilated results, and comparisons with in situ data are similar. pC02 estimates are generally worse after data assimilation, with global estimates diverging 6.4% from in situ data, while free-run estimates are only 4.7% higher. <span class="hlt">Basin</span> correlations are, however, slightly improved: r increase from 0.78 to 0.79, and slope closer to unity at 0.94 compared to 0.86. In contrast, air-sea flux of C02 is noticeably improved after data assimilation. Global differences decline from -0.635 mol/m2/y (stronger model sink from the atmosphere) to -0.202 mol/m2/y. <span class="hlt">Basin</span> correlations are slightly improved from r=O.77 to r=0.78, with slope closer to unity (from 0.93 to 0.99). The Equatorial Atlantic appears as a slight sink in the free-run, but is correctly represented as a moderate source in the assimilation model. However, the assimilation model shows the Antarctic to be a source, rather than a modest sink and the North Indian <span class="hlt">basin</span> is represented incorrectly as a sink</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011148','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011148"><span>Turbidity distribution in the Atlantic <span class="hlt">Ocean</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>Eittreim, S.; Thorndike, E.M.; Sullivan, L.</p> <p>1976-01-01</p> <p>The regional coverage of Lamont nephelometer data in the North and South Atlantic can be used to map seawater turbidity at all depths. At the level of the clearest water, in the mid-depth regions, the turbidity distribution primarily reflects the pattern of productivity in the surface waters. This suggests that the 'background' turbidity level in the <span class="hlt">oceans</span> is largely a function of biogenic fallout. The bottom waters of the western Atlantic generally exhibit large increases in turbidity. The most intense benthic nepheloid layers are in the southwestern Argentine <span class="hlt">basin</span> and northern North American <span class="hlt">basin</span>; the lowest bottom water turbidity in the western Atlantic is in the equatorial regions. Both the Argentine and North American <span class="hlt">basin</span> bottom waters appear to derive their high turbidity largely from local resuspension of terrigenous input in these <span class="hlt">basins</span>. In contrast to the west, the eastern Atlantic <span class="hlt">basins</span> show very low turbidities with the exception of three regions: the Mediterranean outflow area, the Cape <span class="hlt">basin</span>, and the West European <span class="hlt">basin</span>. ?? 1976.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25966973','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25966973"><span>Estuarine fish communities respond to climate variability over both river and <span class="hlt">ocean</span> <span class="hlt">basins</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Feyrer, Frederick; Cloern, James E; Brown, Larry R; Fish, Maxfield A; Hieb, Kathryn A; Baxter, Randall D</p> <p>2015-10-01</p> <p>Estuaries are dynamic environments at the land-sea interface that are strongly affected by interannual climate variability. <span class="hlt">Ocean</span>-atmosphere processes propagate into estuaries from the sea, and atmospheric processes over land propagate into estuaries from watersheds. We examined the effects of these two separate climate-driven processes on pelagic and demersal fish community structure along the salinity gradient in the San Francisco Estuary, California, USA. A 33-year data set (1980-2012) on pelagic and demersal fishes spanning the freshwater to marine regions of the estuary suggested the existence of five estuarine salinity fish guilds: limnetic (salinity = 0-1), oligohaline (salinity = 1-12), mesohaline (salinity = 6-19), polyhaline (salinity = 19-28), and euhaline (salinity = 29-32). Climatic effects propagating from the <span class="hlt">adjacent</span> Pacific <span class="hlt">Ocean</span>, indexed by the North Pacific Gyre Oscillation (NPGO), affected demersal and pelagic fish community structure in the euhaline and polyhaline guilds. Climatic effects propagating over land, indexed as freshwater outflow from the watershed (OUT), affected demersal and pelagic fish community structure in the oligohaline, mesohaline, polyhaline, and euhaline guilds. The effects of OUT propagated further down the estuary salinity gradient than the effects of NPGO that propagated up the estuary salinity gradient, exemplifying the role of variable freshwater outflow as an important driver of biotic communities in river-dominated estuaries. These results illustrate how unique sources of climate variability interact to drive biotic communities and, therefore, that climate change is likely to be an important driver in shaping the future trajectory of biotic communities in estuaries and other transitional habitats. Published 2015. This article is a U.S. Government work and is in the public domain in the USA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012ESRv..113..212S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012ESRv..113..212S"><span>Global continental and <span class="hlt">ocean</span> <span class="hlt">basin</span> reconstructions since 200 Ma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seton, M.; Müller, R. D.; Zahirovic, S.; Gaina, C.; Torsvik, T.; Shephard, G.; Talsma, A.; Gurnis, M.; Turner, M.; Maus, S.; Chandler, M.</p> <p>2012-07-01</p> <p>Global plate motion models provide a spatial and temporal framework for geological data and have been effective tools for exploring processes occurring at the earth's surface. However, published models either have insufficient temporal coverage or fail to treat tectonic plates in a self-consistent manner. They usually consider the motions of selected features attached to tectonic plates, such as continents, but generally do not explicitly account for the continuous evolution of plate boundaries through time. In order to explore the coupling between the surface and mantle, plate models are required that extend over at least a few hundred million years and treat plates as dynamic features with dynamically evolving plate boundaries. We have constructed a new type of global plate motion model consisting of a set of continuously-closing topological plate polygons with associated plate boundaries and plate velocities since the break-up of the supercontinent Pangea. Our model is underpinned by plate motions derived from reconstructing the seafloor-spreading history of the <span class="hlt">ocean</span> <span class="hlt">basins</span> and motions of the continents and utilizes a hybrid absolute reference frame, based on a moving hotspot model for the last 100 Ma, and a true-polar wander corrected paleomagnetic model for 200 to 100 Ma. Detailed regional geological and geophysical observations constrain plate boundary inception or cessation, and time-dependent geometry. Although our plate model is primarily designed as a reference model for a new generation of geodynamic studies by providing the surface boundary conditions for the deep earth, it is also useful for studies in disparate fields when a framework is needed for analyzing and interpreting spatio-temporal data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914696K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914696K"><span>Global Mapping of <span class="hlt">Oceanic</span> and Continental Shelf Crustal Thickness and <span class="hlt">Ocean</span>-Continent Transition Structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kusznir, Nick; Alvey, Andy; Roberts, Alan</p> <p>2017-04-01</p> <p>The 3D mapping of crustal thickness for continental shelves and <span class="hlt">oceanic</span> crust, and the determination of <span class="hlt">ocean</span>-continent transition (OCT) structure and continent-<span class="hlt">ocean</span> boundary (COB) location, represents a substantial challenge. Geophysical inversion of satellite derived free-air gravity anomaly data incorporating a lithosphere thermal anomaly correction (Chappell & Kusznir, 2008) now provides a useful and reliable methodology for mapping crustal thickness in the marine domain. Using this we have produced the first comprehensive maps of global crustal thickness for <span class="hlt">oceanic</span> and continental shelf regions. Maps of crustal thickness and continental lithosphere thinning factor from gravity inversion may be used to determine the distribution of <span class="hlt">oceanic</span> lithosphere, micro-continents and <span class="hlt">oceanic</span> plateaux including for the inaccessible polar regions (e.g. Arctic <span class="hlt">Ocean</span>, Alvey et al.,2008). The gravity inversion method provides a prediction of continent-<span class="hlt">ocean</span> boundary location which is independent of <span class="hlt">ocean</span> magnetic anomaly and isochron interpretation. Using crustal thickness and continental lithosphere thinning factor maps with superimposed shaded-relief free-air gravity anomaly, we can improve the determination of pre-breakup rifted margin conjugacy and sea-floor spreading trajectory during <span class="hlt">ocean</span> <span class="hlt">basin</span> formation. By restoring crustal thickness & continental lithosphere thinning to their initial post-breakup configuration we show the geometry and segmentation of the rifted continental margins at their time of breakup, together with the location of highly-stretched failed breakup <span class="hlt">basins</span> and rifted micro-continents. For detailed analysis to constrain OCT structure, margin type (i.e. magma poor, "normal" or magma rich) and COB location, a suite of quantitative analytical methods may be used which include: (i) Crustal cross-sections showing Moho depth and crustal basement thickness from gravity inversion. (ii) Residual depth anomaly (RDA) analysis which is used to investigate OCT</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016996','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016996"><span>East Mariana <span class="hlt">Basin</span> tholeiites: Cretaceous intraplate basalts or rift basalts related to the Ontong Java 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>Castillo, P.R.; Pringle, M.S.; Carlson, R.W.</p> <p>1994-01-01</p> <p>Studies of seafloor magnetic anomaly patterns suggest the presence of Jurassic <span class="hlt">oceanic</span> crust in a large area in the western Pacific that includes the East Mariana, Nauru and Pigafetta <span class="hlt">Basins</span>. Sampling of the igneous crust in this area by the Deep Sea Drilling Program (DSDP) and the <span class="hlt">Ocean</span> Drilling Program (ODP) allows direct evaluation of the age and petrogenesis of this crust. ODP Leg 129 drilled a 51 m sequence of basalt pillows and massive flows in the central East Mariana <span class="hlt">Basin</span>. 40Ar 39Ar ages determined in this study for two Leg 129 basalts average 114.6 ?? 3.2 Ma. This age is in agreement with the Albian-late Aptian paleontologic age of the overlying sediments, but is distinctively younger than the Jurassic age predicted by magnetic anomaly patterns in the <span class="hlt">basin</span>. Compositionally, the East Mariana <span class="hlt">Basin</span> basalts are uniformly low-K tholeiites that are depleted in highly incompatible elements compared to moderately incompatible ones, which is typical of mid-<span class="hlt">ocean</span> ridge basalts (MORB) erupted near hotspots. The Sr, Nd and Pb isotopic compositions of the tholeiites ( 87Sr 86Srinit = 0.70360-0.70374; 143Nd 144Ndinit = 0.512769-0.512790; 206Pb 204Pbmeas = 18.355-18.386) also overlap with some Indian <span class="hlt">Ocean</span> Ridge MORB, although they are distinct from the isotopic compositions of Jurassic basalts drilled in the Pigafetta <span class="hlt">Basin</span>, the oldest Pacific MORB. The isotopic compositions of the East Mariana <span class="hlt">Basin</span> tholeiites are also similar to those of intraplate basalts, and in particular, to the isotopic signature of basalts from the nearby Ontong Java and Manihiki Plateaus. The East Mariana <span class="hlt">Basin</span> tholeiites also share many petrologic and isotopic characteristics with the <span class="hlt">oceanic</span> basement drilled in the Nauru <span class="hlt">Basin</span> at DSDP Site 462. In addition, the new 110.8 ?? 1.0 Ma 40Ar 39Ar age for two flows from the bottom of Site 462 in the Nauru <span class="hlt">Basin</span> is indistinguishable from the age of the East Mariana <span class="hlt">Basin</span> flows. Thus, while magnetic anomaly patterns predict that the igneous</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('https://www.ncbi.nlm.nih.gov/pubmed/29308292','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29308292"><span>Global trends in <span class="hlt">ocean</span> phytoplankton: a new assessment using revised <span class="hlt">ocean</span> colour data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gregg, Watson W; Rousseaux, Cécile S; Franz, Bryan A</p> <p>2017-01-01</p> <p>A recent revision of the NASA global <span class="hlt">ocean</span> colour record shows changes in global <span class="hlt">ocean</span> chlorophyll trends. This new 18-year time series now includes three global satellite sensors, the Sea-viewing Wide Field of view Sensor (SeaWiFS), Moderate Resolution Imaging Spectroradiometer (MODIS-Aqua), and Visible Infrared Imaging Radiometer Suite (VIIRS). The major changes are radiometric drift correction, a new algorithm for chlorophyll, and a new sensor VIIRS. The new satellite data record shows no significant trend in global annual median chlorophyll from 1998 to 2015, in contrast to a statistically significant negative trend from 1998 to 2012 in the previous version. When revised satellite data are assimilated into a global <span class="hlt">ocean</span> biogeochemical model, no trend is observed in global annual median chlorophyll. This is consistent with previous findings for the 1998-2012 time period using the previous processing version and only two sensors (SeaWiFS and MODIS). Detecting trends in <span class="hlt">ocean</span> chlorophyll with satellites is sensitive to data processing options and radiometric drift correction. The assimilation of these data, however, reduces sensitivity to algorithms and radiometry, as well as the addition of a new sensor. This suggests the assimilation model has skill in detecting trends in global <span class="hlt">ocean</span> colour. Using the assimilation model, spatial distributions of significant trends for the 18-year record (1998-2015) show recent decadal changes. Most notable are the North and Equatorial Indian <span class="hlt">Oceans</span> <span class="hlt">basins</span>, which exhibit a striking decline in chlorophyll. It is exemplified by declines in diatoms and chlorophytes, which in the model are large and intermediate size phytoplankton. This decline is partially compensated by significant increases in cyanobacteria, which represent very small phytoplankton. This suggests the beginning of a shift in phytoplankton composition in these tropical and subtropical Indian <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123..358J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123..358J"><span>Effects of Model Resolution and <span class="hlt">Ocean</span> Mixing on Forced Ice-<span class="hlt">Ocean</span> Physical and Biogeochemical Simulations Using Global and Regional System Models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jin, Meibing; Deal, Clara; Maslowski, Wieslaw; Matrai, Patricia; Roberts, Andrew; Osinski, Robert; Lee, Younjoo J.; Frants, Marina; Elliott, Scott; Jeffery, Nicole; Hunke, Elizabeth; Wang, Shanlin</p> <p>2018-01-01</p> <p>The current coarse-resolution global Community Earth System Model (CESM) can reproduce major and large-scale patterns but is still missing some key biogeochemical features in the Arctic <span class="hlt">Ocean</span>, e.g., low surface nutrients in the Canada <span class="hlt">Basin</span>. We incorporated the CESM Version 1 <span class="hlt">ocean</span> biogeochemical code into the Regional Arctic System Model (RASM) and coupled it with a sea-ice algal module to investigate model limitations. Four ice-<span class="hlt">ocean</span> hindcast cases are compared with various observations: two in a global 1° (40˜60 km in the Arctic) grid: G1deg and G1deg-OLD with/without new sea-ice processes incorporated; two on RASM's 1/12° (˜9 km) grid R9km and R9km-NB with/without a subgrid scale brine rejection parameterization which improves <span class="hlt">ocean</span> vertical mixing under sea ice. Higher-resolution and new sea-ice processes contributed to lower model errors in sea-ice extent, ice thickness, and ice algae. In the Bering Sea shelf, only higher resolution contributed to lower model errors in salinity, nitrate (NO3), and chlorophyll-a (Chl-a). In the Arctic <span class="hlt">Basin</span>, model errors in mixed layer depth (MLD) were reduced 36% by brine rejection parameterization, 20% by new sea-ice processes, and 6% by higher resolution. The NO3 concentration biases were caused by both MLD bias and coarse resolution, because of excessive horizontal mixing of high NO3 from the Chukchi Sea into the Canada <span class="hlt">Basin</span> in coarse resolution models. R9km showed improvements over G1deg on NO3, but not on Chl-a, likely due to light limitation under snow and ice cover in the Arctic <span class="hlt">Basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2003/ofr-03-230/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2003/ofr-03-230/"><span>Digital depth horizon compilations of the Alaskan North Slope and <span class="hlt">adjacent</span> Arctic regions</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Saltus, Richard W.; Bird, Kenneth J.</p> <p>2003-01-01</p> <p>Data have been digitized and combined to create four detailed depth horizon grids spanning the Alaskan North Slope and <span class="hlt">adjacent</span> offshore areas. These map horizon compilations were created to aid in petroleum system modeling and related studies. Topography/bathymetry is extracted from a recent Arctic compilation of global onshore DEM and satellite altimetry and ship soundings offshore. The Lower Cretaceous Unconformity (LCU), the top of the Triassic Shublik Formation, and the pre-Carboniferous acoustic basement horizon grids are created from numerous seismic studies, drill hole information, and interpolation. These horizons were selected because they mark critical times in the geologic evolution of the region as it relates to petroleum. The various horizons clearly show the major tectonic elements of this region including the Brooks Range, Colville Trough, Barrow Arch, Hanna Trough, Chukchi Platform, Nuwuk <span class="hlt">Basin</span>, Kaktovik <span class="hlt">Basin</span>, and Canada <span class="hlt">Basin</span>. The gridded data are available in a variety of data formats for use in regional studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3031525','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3031525"><span>Megafaunal Community Structure of Andaman Seamounts Including the Back-Arc <span class="hlt">Basin</span> – A Quantitative Exploration from the Indian <span class="hlt">Ocean</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>Sautya, Sabyasachi; Ingole, Baban; Ray, Durbar; Stöhr, Sabine; Samudrala, Kiranmai; Raju, K. A. Kamesh; Mudholkar, Abhay</p> <p>2011-01-01</p> <p>Species rich benthic communities have been reported from some seamounts, predominantly from the Atlantic and Pacific <span class="hlt">Oceans</span>, but the fauna and habitats on Indian <span class="hlt">Ocean</span> seamounts are still poorly known. This study focuses on two seamounts, a submarine volcano (cratered seamount – CSM) and a non-volcano (SM2) in the Andaman Back–arc <span class="hlt">Basin</span> (ABB), and the <span class="hlt">basin</span> itself. The main purpose was to explore and generate regional biodiversity data from summit and flank (upper slope) of the Andaman seamounts for comparison with other seamounts worldwide. We also investigated how substratum types affect the megafaunal community structure along the ABB. Underwater video recordings from TeleVision guided Gripper (TVG) lowerings were used to describe the benthic community structure along the ABB and both seamounts. We found 13 varieties of substratum in the study area. The CSM has hard substratum, such as boulders and cobbles, whereas the SM2 was dominated by cobbles and fine sediment. The highest abundance of megabenthic communities was recorded on the flank of the CSM. Species richness and diversity were higher at the flank of the CSM than other are of ABB. Non-metric multi-dimensional scaling (nMDS) analysis of substratum types showed 50% similarity between the flanks of both seamounts, because both sites have a component of cobbles mixed with fine sediments in their substratum. Further, nMDS of faunal abundance revealed two groups, each restricted to one of the seamounts, suggesting faunal distinctness between them. The sessile fauna corals and poriferans showed a significant positive relation with cobbles and fine sediments substratum, while the mobile categories echinoderms and arthropods showed a significant positive relation with fine sediments only. PMID:21297959</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1233231-diagnosing-isopycnal-diffusivity-eddying-idealized-midlatitude-ocean-basin-via-lagrangian-situ-global-high-performance-particle-tracking-light','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1233231-diagnosing-isopycnal-diffusivity-eddying-idealized-midlatitude-ocean-basin-via-lagrangian-situ-global-high-performance-particle-tracking-light"><span>Diagnosing isopycnal diffusivity in an eddying, idealized midlatitude <span class="hlt">ocean</span> <span class="hlt">basin</span> via Lagrangian, in Situ, Global, High-Performance Particle Tracking (LIGHT)</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Wolfram, Phillip J.; Ringler, Todd D.; Maltrud, Mathew E.; ...</p> <p>2015-08-01</p> <p>Isopycnal diffusivity due to stirring by mesoscale eddies in an idealized, wind-forced, eddying, midlatitude <span class="hlt">ocean</span> <span class="hlt">basin</span> is computed using Lagrangian, in Situ, Global, High-Performance Particle Tracking (LIGHT). Simulation is performed via LIGHT within the Model for Prediction across Scales <span class="hlt">Ocean</span> (MPAS-O). Simulations are performed at 4-, 8-, 16-, and 32-km resolution, where the first Rossby radius of deformation (RRD) is approximately 30 km. Scalar and tensor diffusivities are estimated at each resolution based on 30 ensemble members using particle cluster statistics. Each ensemble member is composed of 303 665 particles distributed across five potential density surfaces. Diffusivity dependence upon modelmore » resolution, velocity spatial scale, and buoyancy surface is quantified and compared with mixing length theory. The spatial structure of diffusivity ranges over approximately two orders of magnitude with values of O(10 5) m 2 s –1 in the region of western boundary current separation to O(10 3) m 2 s –1 in the eastern region of the <span class="hlt">basin</span>. Dominant mixing occurs at scales twice the size of the first RRD. Model resolution at scales finer than the RRD is necessary to obtain sufficient model fidelity at scales between one and four RRD to accurately represent mixing. Mixing length scaling with eddy kinetic energy and the Lagrangian time scale yield mixing efficiencies that typically range between 0.4 and 0.8. In conclusion, a reduced mixing length in the eastern region of the domain relative to the west suggests there are different mixing regimes outside the baroclinic jet region.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70048355','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70048355"><span>Baseline monitoring of the western Arctic <span class="hlt">Ocean</span> estimates 20% of the Canadian <span class="hlt">Basin</span> surface waters are undersaturated with respect to aragonite</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Robbins, Lisa L.; Wynn, Jonathan G.; Lisle, John T.; Yates, Kimberly K.; Knorr, Paul O.; Byrne, Robert H.; Liu, Xuewu; Patsavas, Mark C.; Azetsu-Scott, Kumiko; Takahashi, Taro</p> <p>2013-01-01</p> <p>Marine surface waters are being acidified due to uptake of anthropogenic carbon dioxide, resulting in surface <span class="hlt">ocean</span> areas of undersaturation with respect to carbonate minerals, including aragonite. In the Arctic <span class="hlt">Ocean</span>, acidification is expected to occur at an accelerated rate with respect to the global <span class="hlt">oceans</span>, but a paucity of baseline data has limited our understanding of the extent of Arctic undersaturation and of regional variations in rates and causes. The lack of data has also hindered refinement of models aimed at projecting future trends of <span class="hlt">ocean</span> acidification. Here, based on more than 34,000 data records collected in 2010 and 2011, we establish a baseline of inorganic carbon data (pH, total alkalinity, dissolved inorganic carbon, partial pressure of carbon dioxide, and aragonite saturation index) for the western Arctic <span class="hlt">Ocean</span>. This data set documents aragonite undersaturation in ~20% of the surface waters of the combined Canada and Makarov <span class="hlt">basins</span>, an area characterized by recent acceleration of sea ice loss. Conservative tracer studies using stable oxygen isotopic data from 307 sites show that while the entire surface of this area receives abundant freshwater from meteoric sources, freshwater from sea ice melt is most closely linked to the areas of carbonate mineral undersaturation. These data link the Arctic Ocean’s largest area of aragonite undersaturation to sea ice melt and atmospheric CO2 absorption in areas of low buffering capacity. Some relatively supersaturated areas can be linked to localized biological activity. Collectively, these observations can be used to project trends of <span class="hlt">ocean</span> acidification in higher latitude marine surface waters where inorganic carbon chemistry is largely influenced by sea ice meltwater.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1055480','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1055480"><span>Modeling the Physical and Biochemical Influence of <span class="hlt">Ocean</span> Thermal Energy Conversion Plant Discharges into their <span class="hlt">Adjacent</span> Waters</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>PAT GRANDELLI, P.E.; GREG ROCHELEAU; JOHN HAMRICK, Ph.D.</p> <p></p> <p>This paper describes the modeling work by Makai <span class="hlt">Ocean</span> Engineering, Inc. to simulate the biochemical effects of of the nutrient-enhanced seawater plumes that are discharged by one or several 100 megawatt OTEC plants. The modeling is needed to properly design OTEC plants that can operate sustainably with acceptably low biological impact. In order to quantify the effect of discharge configuration and phytoplankton response, Makai <span class="hlt">Ocean</span> Engineering implemented a biological and physical model for the waters surrounding O`ahu, Hawai`i, using the EPA-approved Environmental Fluid Dynamics Code (EFDC). Each EFDC grid cell was approximately 1 square kilometer by 20 meters deep, andmore » used a time step of three hours. The biological model was set up to simulate the biochemical response for three classes of organisms: Picoplankton (< 2 um) such as prochlorococccus, nanoplankton (2-20 um), and microplankton (> 20 um) e.g., diatoms. The dynamic biological phytoplankton model was calibrated using chemical and biological data collected for the Hawaii <span class="hlt">Ocean</span> Time Series (HOTS) project. Peer review of the biological modeling was performed. The physical oceanography model uses boundary conditions from a surrounding Hawai'i Regional <span class="hlt">Ocean</span> Model, (ROM) operated by the University of Hawai`i and the National Atmospheric and <span class="hlt">Oceanic</span> Administration. The ROM provided tides, <span class="hlt">basin</span> scale circulation, mesoscale variability, and atmospheric forcing into the edges of the EFDC computational domain. This model is the most accurate and sophisticated Hawai'ian Regional <span class="hlt">Ocean</span> Model presently available, assimilating real-time oceanographic observations, as well as model calibration based upon temperature, current and salinity data collected during 2010 near the simulated OTEC site. The ROM program manager peer-reviewed Makai's implementation of the ROM output into our EFDC model. The supporting oceanographic data was collected for a Naval Facilities Engineering Command / Makai project. Results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS12B..03A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS12B..03A"><span>Control of Atmospheric CO2 by the <span class="hlt">Ocean</span>'s Biological Pump and Shelf-<span class="hlt">Basin</span> Fractionation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Anderson, R. F.; Fleisher, M. Q.; Mix, A. C.</p> <p>2006-12-01</p> <p>Identifying the cause of the dramatic correlation between atmospheric CO2 concentrations and past climate variability has been one of the principal goals of paleoclimate research over the past quarter century. Several plausible mechanisms have been proposed, and each has been rejected as being incapable by itself of accounting for the full range (80 to 100 ppm) of glacial to interglacial variability of atmospheric CO2 concentration. Consequently, recent studies have focused on scenarios by which a combination of mechanisms work synergistically to account for the full range of CO2 variability. We will present evidence from equatorial Pacific sediment cores that increased strength of the <span class="hlt">ocean</span>'s biological pump was primarily responsible for drawdown of atmospheric CO2 during the early stages of glaciation, and that increased <span class="hlt">ocean</span> alkalinity (or, more specifically, an increase in the <span class="hlt">ocean</span> carbonate ion concentration) led to a further reduction of atmospheric CO2 during maximum glaciation. Increased strength of the biological pump is manifest as increasing differences between the carbon isotope composition of planktonic and benthic foraminifera during early stages of glaciation, as predicted a quarter century ago in classic works by Broecker and by Shackleton. Increased carbonate ion concentration is manifest by increased preservation and burial of calcium carbonate in deep equatorial Pacific sediments. The carbon isotope record is noisy, but the pattern is repeated over each of the past three glacial cycles, lending confidence to its reliability. Increased preservation and burial of CaCO3 occurred each time the oxygen isotope composition of benthic foraminifera rose above a threshold value corresponding to a sea level lowering of roughly 70 m below present. This relationship is reproduced systematically throughout the past 450 kyr, again lending confidence to the finding and supporting the view that shelf-<span class="hlt">basin</span> fractionation, or the shift in CaCO3 deposition from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1986/4094/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1986/4094/report.pdf"><span>Ground-water geochemistry of the Albuquerque-Belen <span class="hlt">Basin</span>, central New 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>Anderholm, S.K.</p> <p>1988-01-01</p> <p>The purpose of this study was to define the areal distribution of different water types, use the distribution to help define the groundwater flow system, and identify processes resulting in differences in groundwater quality in the Albuquerque-Belen <span class="hlt">Basin</span> in central New Mexico. The chemistry of surface water inflow from <span class="hlt">adjacent</span> areas, which infiltrates and recharges the aquifer along the <span class="hlt">basin</span> margin, affects the groundwater quality in the eastern and southeastern areas of the <span class="hlt">basin</span>. Groundwater in the eastern area generally has a specific conductance less than 400 microsiemens, and calcium and bicarbonate are the dominant ions. Mixing of recharge, groundwater inflow, and surface inflow from <span class="hlt">adjacent</span> areas, which have different chemical compositions, is the major process affecting groundwater quality in the southwestern, western, and northern areas of the <span class="hlt">basin</span>. In these areas, there is a large range in specific conductance and distribution of dissolved ions. Groundwater quality in the Rio Grande valley is affected by the infiltration of excess irrigation water. The excess irrigation water generally has a larger specific conductance than other groundwater in the valley, so mixing of these waters results in shallow groundwater generally having larger specific conductance than the deeper groundwater. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994JGR....9924189E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994JGR....9924189E"><span>Transition from continental to <span class="hlt">oceanic</span> crust on the Wilkes-Adelie margin of Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eittreim, Stephen L.</p> <p>1994-12-01</p> <p>The Wilkes-Adelie margin of East Antarctica, a passive margin rifted in the Early Cretaceous, has an unusually reflective Moho which can be traced seismically across the continent-<span class="hlt">ocean</span> transition. Velocity models and depth sections were constructed from a combined set of U.S. and French multichannel seismic reflection lines to investigate the transition from continental to <span class="hlt">oceanic</span> crust. These data show that the boundary between oldest <span class="hlt">oceanic</span> crust and transitional continental crust is marked by a minimum in subsediment crustal thickness and, in places, by a shoaling of Moho. The Moho reflection is continuous across the edge of <span class="hlt">oceanic</span> crust, and gradually deepens landward under the continental edge. A marginal rift <span class="hlt">basin</span>, some tens of kilometers in width, lies in the transition between continental and <span class="hlt">oceanic</span> crust, contains an average of about 4 km of synrift sediment that is prograded in places, and has characteristics of a former rift valley, now subsided to about 10 km. Three types of reflections in the seismic data are interpreted as volcanic deposits: (1) high-amplitude reflections that floor the marginal rift <span class="hlt">basin</span>, (2) irregularly seaward dipping sequences that comprise an anomalously thick edge of <span class="hlt">oceanic</span> crust, and (3) highly irregular and diffractive reflections from <span class="hlt">oceanic</span> crustal <span class="hlt">basins</span> that cap a normal-thickness <span class="hlt">ocean</span> crust. The present depth to the prefit surface of continental crust is compatible with passive margin subsidence since 95 Ma, corrected for its load of synrift and postrift sediment and mechanically stretched by factors of beta = 1.8 or higher. Comparison of seismic crustal thickness measurements with inferred crustal thinning from subsidence analysis shows agreement for areas where beta less than 4. In areas where beta greater than 4, measured thickness is greater than that inferred from subsidence analysis, a result that could be explained by underplating the crust beneath the marginal rift <span class="hlt">basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AAS...22732501C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AAS...22732501C"><span><span class="hlt">Ocean</span> Observations of Climate Change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chambers, Don</p> <p>2016-01-01</p> <p>The <span class="hlt">ocean</span> influences climate by storing and transporting large amounts of heat, freshwater, and carbon, and exchanging these properties with the atmosphere. About 93% of the excess heat energy stored by the earth over the last 50 years is found in the <span class="hlt">ocean</span>. More than three quarters of the total exchange of water between the atmosphere and the earth's surface through evaporation and precipitation takes place over the <span class="hlt">oceans</span>. The <span class="hlt">ocean</span> contains 50 times more carbon than the atmosphere and is at present acting to slow the rate of climate change by absorbing one quarter of human emissions of carbon dioxide from fossil fuel burning, cement production, deforestation and other land use change.Here I summarize the observational evidence of change in the <span class="hlt">ocean</span>, with an emphasis on <span class="hlt">basin</span>- and global-scale changes relevant to climate. These include: changes in subsurface <span class="hlt">ocean</span> temperature and heat content, evidence for regional changes in <span class="hlt">ocean</span> salinity and their link to changes in evaporation and precipitation over the <span class="hlt">oceans</span>, evidence of variability and change of <span class="hlt">ocean</span> current patterns relevant to climate, observations of sea level change and predictions over the next century, and biogeochemical changes in the <span class="hlt">ocean</span>, including <span class="hlt">ocean</span> acidification.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/bul/b2210-e/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/bul/b2210-e/"><span>Overview of mine drainage geochemistry at historical mines, Humboldt River <span class="hlt">basin</span> and <span class="hlt">adjacent</span> mining areas, Nevada. Chapter E.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Nash, J. Thomas; Stillings, Lisa L.</p> <p>2004-01-01</p> <p>Reconnaissance hydrogeochemical studies of the Humboldt River <span class="hlt">basin</span> and <span class="hlt">adjacent</span> areas of northern Nevada have identified local sources of acidic waters generated by historical mine workings and mine waste. The mine-related acidic waters are rare and generally flow less than a kilometer before being neutralized by natural processes. Where waters have a pH of less than about 3, particularly in the presence of sulfide minerals, the waters take on high to extremely high concentrations of many potentially toxic metals. The processes that create these acidic, metal-rich waters in Nevada are the same as for other parts of the world, but the scale of transport and the fate of metals are much more localized because of the ubiquitous presence of caliche soils. Acid mine drainage is rare in historical mining districts of northern Nevada, and the volume of drainage rarely exceeds about 20 gpm. My findings are in close agreement with those of Price and others (1995) who estimated that less than 0.05 percent of inactive and abandoned mines in Nevada are likely to be a concern for acid mine drainage. Most historical mining districts have no draining mines. Only in two districts (Hilltop and National) does water affected by mining flow into streams of significant size and length (more than 8 km). Water quality in even the worst cases is naturally attenuated to meet water-quality standards within about 1 km of the source. Only a few historical mines release acidic water with elevated metal concentrations to small streams that reach the Humboldt River, and these contaminants and are not detectable in the Humboldt. These reconnaissance studies offer encouraging evidence that abandoned mines in Nevada create only minimal and local water-quality problems. Natural attenuation processes are sufficient to compensate for these relatively small sources of contamination. These results may provide useful analogs for future mining in the Humboldt River <span class="hlt">basin</span>, but attention must be given to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013GeCoA.107...12T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013GeCoA.107...12T"><span>Iron isotopic systematics of <span class="hlt">oceanic</span> basalts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teng, Fang-Zhen; Dauphas, Nicolas; Huang, Shichun; Marty, Bernard</p> <p>2013-04-01</p> <p>The iron isotopic compositions of 93 well-characterized basalts from geochemically and geologically diverse mid-<span class="hlt">ocean</span> ridge segments, <span class="hlt">oceanic</span> islands and back arc <span class="hlt">basins</span> were measured. Forty-three MORBs have homogeneous Fe isotopic composition, with δ56Fe ranging from +0.07‰ to +0.14‰ and an average of +0.105 ± 0.006‰ (2SD/√n, n = 43, MSWD = 1.9). Three back arc <span class="hlt">basin</span> basalts have similar δ56Fe to MORBs. By contrast, OIBs are slightly heterogeneous with δ56Fe ranging from +0.05‰ to +0.14‰ in samples from Koolau and Loihi, Hawaii, and from +0.09‰ to +0.18‰ in samples from the Society Islands and Cook-Austral chain, French Polynesia. Overall, <span class="hlt">oceanic</span> basalts are isotopically heavier than mantle peridotite and pyroxenite xenoliths, reflecting Fe isotope fractionation during partial melting of the mantle. Iron isotopic variations in OIBs mainly reflect Fe isotope fractionation during fractional crystallization of olivine and pyroxene, enhanced by source heterogeneity in Koolau samples.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20130001846','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20130001846"><span>Closing the Seasonal <span class="hlt">Ocean</span> Surface Temperature Balance in the Eastern Tropical <span class="hlt">Oceans</span> from Remote Sensing and Model Reanalyses</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Roberts, J. Brent; Clayson, Carol A.</p> <p>2012-01-01</p> <p>The Eastern tropical <span class="hlt">ocean</span> <span class="hlt">basins</span> are regions of significant atmosphere-<span class="hlt">ocean</span> interaction and are important to variability across subseasonal to decadal time scales. The numerous physical processes at play in these areas strain the abilities of coupled general circulation models to accurately reproduce observed upper <span class="hlt">ocean</span> variability. Furthermore, limitations in the observing system of important terms in the surface temperature balance (e.g., turbulent and radiative heat fluxes, advection) introduce uncertainty into the analyses of processes controlling sea surface temperature variability. This study presents recent efforts to close the surface temperature balance through estimation of the terms in the mixed layer temperature budget using state-of-the-art remotely sensed and model-reanalysis derived products. A set of twelve net heat flux estimates constructed using combinations of radiative and turbulent heat flux products - including GEWEX-SRB, ISCCP-SRF, OAFlux, SeaFlux, among several others - are used with estimates of <span class="hlt">oceanic</span> advection, entrainment, and mixed layer depth variability to investigate the seasonal variability of <span class="hlt">ocean</span> surface temperatures. Particular emphasis is placed on how well the upper <span class="hlt">ocean</span> temperature balance is, or is not, closed on these scales using the current generation of observational and model reanalysis products. That is, the magnitudes and spatial variability of residual imbalances are addressed. These residuals are placed into context within the current uncertainties of the surface net heat fluxes and the role of the mixed layer depth variability in scaling the impact of those uncertainties, particularly in the shallow mixed layers of the Eastern tropical <span class="hlt">ocean</span> <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017HESS...21.6379S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017HESS...21.6379S"><span>The atmospheric branch of the hydrological cycle over the Indus, Ganges, and Brahmaputra river <span class="hlt">basins</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sorí, Rogert; Nieto, Raquel; Drumond, Anita; Vicente-Serrano, Sergio M.; Gimeno, Luis</p> <p>2017-12-01</p> <p>The atmospheric branch of the hydrological cycle over the Indus, Ganges, and Brahmaputra river <span class="hlt">basins</span> (IRB, GRB, and BRB respectively) in the South Asian region was investigated. The 3-dimensional model FLEXPART v9.0 was utilized. An important advantage of this model is that it permits the computation of the freshwater budget on air parcel trajectories both backward and forward in time from 0.1 to 1000 hPa in the atmospheric vertical column. The analysis was conducted for the westerly precipitation regime (WPR) (November-April) and the monsoonal precipitation regime (MPR) (May-October) in the period from 1981 to 2015. The main terrestrial and <span class="hlt">oceanic</span> climatological moisture sources for the IRB, GRB, and BRB and their contribution to precipitation over the <span class="hlt">basins</span> were identified. For the three <span class="hlt">basins</span>, the most important moisture sources for precipitation are (i) in the continental regions, the land masses to the west of the <span class="hlt">basins</span> (in this case called western Asia), the Indian region (IR), and the <span class="hlt">basin</span> itself, and (ii) from the <span class="hlt">ocean</span>, the utmost sources being the Indian <span class="hlt">Ocean</span> (IO) and the Bay of Bengal (BB), and it is remarkable that despite the amount of moisture reaching the Indus and Ganges <span class="hlt">basins</span> from land sources, the moisture supply from the IO seems to be first associated with the rapid increase or decrease in precipitation over the sources in the MPR. The technique of the composites was used to analyse how the moisture uptake values spatially vary from the sources (the budget of evaporation minus precipitation (E - P) was computed in a backward experiment from the <span class="hlt">basins</span>) but during the pre-onset and pre-demise dates of the monsoonal rainfall over each <span class="hlt">basin</span>; this confirmed that over the last days of the monsoon at the <span class="hlt">basins</span>, the moisture uptake areas decrease in the IO. The Indian region, the Indian <span class="hlt">Ocean</span>, the Bay of Bengal, and the <span class="hlt">basins</span> themselves are the main sources of moisture responsible for negative (positive) anomalies of moisture contribution to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70156458','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70156458"><span>Canada <span class="hlt">Basin</span> revealed</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Mosher, David C.; Shimeld, John; Hutchinson, Deborah R.; Chian, D; Lebedeva-Ivanova, Nina; Jackson, Ruth</p> <p>2012-01-01</p> <p>More than 15,000 line-km of new regional seismic reflection and refraction data in the western Arctic <span class="hlt">Ocean</span> provide insights into the tectonic and sedimentologic history of Canada <span class="hlt">Basin</span>, permitting development of new geologic understanding in one of Earth's last frontiers. These new data support a rotational opening model for southern Canada <span class="hlt">Basin</span>. There is a central basement ridge possibly representing an extinct spreading center with <span class="hlt">oceanic</span> crustal velocities and blocky basement morphology characteristic of spreading centre crust surrounding this ridge. Basement elevation is lower in the south, mostly due to sediment loading subsidence. The sedimentary succession is thickest in the southern Beaufort Sea region, reaching more than 15 km, and generally thins to the north and west. In the north, grabens and half-grabens are indicative of extension. Alpha-Mendeleev Ridge is a large igneous province in northern Amerasia <span class="hlt">Basin</span>, presumably emplaced synchronously with <span class="hlt">basin</span> formation. It overprints most of northern Canada <span class="hlt">Basin</span> structure. The seafloor and sedimentary succession of Canada <span class="hlt">Basin</span> is remarkably flat-lying in its central region, with little bathymetric change over most of its extent. Reflections that correlate over 100s of kms comprise most of the succession and on-lap bathymetric and basement highs. They are interpreted as representing deposits from unconfined turbidity current flows. Sediment distribution patterns reflect changing source directions during the basin’s history. Initially, probably late Cretaceous to Paleocene synrift sediments sourced from the Alaska and Mackenzie-Beaufort margins. This unit shows a progressive series of onlap unconformities with a younging trend towards Alpha and Northwind ridges, likely a response to contemporaneous subsidence. Sediment source direction appeared to shift to the Canadian Arctic Archipelago margin for the Eocene and Oligocene, likely due to uplift of Arctic islands during the Eurekan Orogeny. The final</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006Natur.441..606B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006Natur.441..606B"><span>Episodic fresh surface waters in the Eocene Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brinkhuis, Henk; Schouten, Stefan; Collinson, Margaret E.; Sluijs, Appy; Damsté, Jaap S. Sinninghe; Dickens, Gerald R.; Huber, Matthew; Cronin, Thomas M.; Onodera, Jonaotaro; Takahashi, Kozo; Bujak, Jonathan P.; Stein, Ruediger; van der Burgh, Johan; Eldrett, James S.; Harding, Ian C.; Lotter, André F.; Sangiorgi, Francesca; Cittert, Han Van Konijnenburg-Van; de Leeuw, Jan W.; Matthiessen, Jens; Backman, Jan; Moran, Kathryn; Expedition 302 Scientists</p> <p>2006-06-01</p> <p>It has been suggested, on the basis of modern hydrology and fully coupled palaeoclimate simulations, that the warm greenhouse conditions that characterized the early Palaeogene period (55-45Myr ago) probably induced an intensified hydrological cycle with precipitation exceeding evaporation at high latitudes. Little field evidence, however, has been available to constrain <span class="hlt">oceanic</span> conditions in the Arctic during this period. Here we analyse Palaeogene sediments obtained during the Arctic Coring Expedition, showing that large quantities of the free-floating fern Azolla grew and reproduced in the Arctic <span class="hlt">Ocean</span> by the onset of the middle Eocene epoch (~50Myr ago). The Azolla and accompanying abundant freshwater organic and siliceous microfossils indicate an episodic freshening of Arctic surface waters during an ~800,000-year interval. The abundant remains of Azolla that characterize basal middle Eocene marine deposits of all Nordic seas probably represent transported assemblages resulting from freshwater spills from the Arctic <span class="hlt">Ocean</span> that reached as far south as the North Sea. The termination of the Azolla phase in the Arctic coincides with a local sea surface temperature rise from ~10°C to 13°C, pointing to simultaneous increases in salt and heat supply owing to the influx of waters from <span class="hlt">adjacent</span> <span class="hlt">oceans</span>. We suggest that onset and termination of the Azolla phase depended on the degree of <span class="hlt">oceanic</span> exchange between Arctic <span class="hlt">Ocean</span> and <span class="hlt">adjacent</span> seas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70030357','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70030357"><span>Episodic fresh surface waters in the Eocene Arctic <span class="hlt">Ocean</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>Brinkhuis, H.; Schouten, S.; Collinson, M.E.; Sluijs, A.; Damste, J.S.S.; Dickens, G.R.; Huber, M.; Cronin, T. M.; Onodera, J.; Takahashi, K.; Bujak, J.P.; Stein, R.; Van Der Burgh, J.; Eldrett, J.S.; Harding, I.C.; Lotter, A.F.; Sangiorgi, F.; Cittert, H.V.K.V.; De Leeuw, J. W.; Matthiessen, J.; Backman, J.; Moran, K.</p> <p>2006-01-01</p> <p>It has been suggested, on the basis of modern hydrology and fully coupled palaeoclimate simulations, that the warm greenhouse conditions that characterized the early Palaeogene period (55-45 Myr ago) probably induced an intensified hydrological cycle with precipitation exceeding evaporation at high latitudes. Little field evidence, however, has been available to constrain <span class="hlt">oceanic</span> conditions in the Arctic during this period. Here we analyse Palaeogene sediments obtained during the Arctic Coring Expedition, showing that large quantities of the free-floating fern Azolla grew and reproduced in the Arctic <span class="hlt">Ocean</span> by the onset of the middle Eocene epoch (???50 Myr ago). The Azolla and accompanying abundant freshwater organic and siliceous microfossils indicate an episodic freshening of Arctic surface waters during an ???800,000-year interval. The abundant remains of Azolla that characterize basal middle Eocene marine deposits of all Nordic seas probably represent transported assemblages resulting from freshwater spills from the Arctic <span class="hlt">Ocean</span> that reached as far south as the North Sea. The termination of the Azolla phase in the Arctic coincides with a local sea surface temperature rise from ???10??C to 13??C, pointing to simultaneous increases in salt and heat supply owing to the influx of waters from <span class="hlt">adjacent</span> <span class="hlt">oceans</span>. We suggest that onset and termination of the Azolla phase depended on the degree of <span class="hlt">oceanic</span> exchange between Arctic <span class="hlt">Ocean</span> and <span class="hlt">adjacent</span> seas. ?? 2006 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-12-04/pdf/2013-28995.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-12-04/pdf/2013-28995.pdf"><span>78 FR 72860 - White River National Forest; Summit County, CO; 2013 Arapahoe <span class="hlt">Basin</span> Improvements EIS</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>2013-12-04</p> <p>... experience that A-<span class="hlt">Basin</span> provides; improve access to Montezuma Bowl; upgrade or remove existing lifts, as... Gullies and one in Beaver Bowl. Currently, The Beavers can be accessed legally through backcountry access... exit the controlled/patrolled portions of A-<span class="hlt">Basin</span>'s operational boundary to access <span class="hlt">adjacent</span> backcountry...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMDI21B..02C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMDI21B..02C"><span>Predicting Global Rates and Distribution of Carbonate Melting Beneath the <span class="hlt">Ocean</span> <span class="hlt">Basins</span>: Implications for the Origin of the Gutenberg Discontinuity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clerc, F.; Behn, M. D.; Parmentier, E. M.</p> <p>2017-12-01</p> <p>The pooling of carbonate melts beneath old <span class="hlt">ocean</span> lithosphere is a proposed explanation for the seismic Gutenberg (G) discontinuity. However, while the G discontinuity is observed ubiquitously across the <span class="hlt">ocean</span> <span class="hlt">basins</span>, carbonate melting only occurs in regions of mantle upwelling. Here we examine the global distribution and extent of carbonate melting by coupling a mantle flow model with a thermodynamic parameterization for carbonate melting. We obtain global upwelling velocities from a convection model driven by plate motions and mantle density differences [1], and calculate melt fractions from the R_DMC carbonate solidus [2]. We find low-degree carbonate melts are produced pervasively throughout <span class="hlt">ocean</span> <span class="hlt">basins</span>, driven by passive upwelling in response to subduction. Assuming melt formed within 100 km of the ridge is focused to its axis, our model predicts a 6-km thick <span class="hlt">oceanic</span> crust and a global CO2 ridge flux of 7 x 1011 mol/yr (for a mantle source concentration of 100 ppm CO2). This flux is consistent with other estimates of CO2 ridge fluxes [e.g.,3] over the inferred range of MORB-source mantle carbon concentrations [e.g.,4]. In addition to the ridge flux, off-axis carbonate melting results in a global CO2 flux of 1.6 x 1012mol/yr. To test for correlations between regions of upwelling-induced carbonate melting and seismic evidence for the LAB, we compare our results with a compilation of seismic G discontinuity observations [5]. While most observations of the G discontinuity are found in regions of predicted carbonate melting, some lie in regions of downwelling (where no melting occurs), suggesting that melt pooling does not conclusively explain these seismic signals. Further, we estimate off-axis porosities to be < 0.1%, indicating that the melt remaining in the mantle does not contribute substantially to a discontinuity of the observed magnitude. Carbonate melts pooled at the base of the lithosphere may refreeze within the thermal boundary layer and refertilize the</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('http://adsabs.harvard.edu/abs/2016AGUOSPO21B..07H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO21B..07H"><span>Coupled <span class="hlt">ocean</span>-shelf ecosystem modelling of northern North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harle, J.; Holt, J. T.; Butenschön, M.; Allen, J. I.</p> <p>2016-02-01</p> <p>The biogeochemistry and ecosystems of the open-<span class="hlt">ocean</span> and shelf seas are intimately connected. For example Northwest European continental shelf receives a substantial fraction of its nutrients from the wider North Atlantic and exports carbon at depth, sequestering it from atmospheric exchange. In the EC FP7 Euro<span class="hlt">Basin</span> project (Holt et al 2014) we have developed a 1/12 degree <span class="hlt">basin</span>-scale NEMO-ERSEM model with specific features relevant to shelf seas (e.g. tides and advanced vertical mixing schemes). This model is eddy resolving in the open-<span class="hlt">ocean</span>, and resolves barotropic scales on-shelf. We use this model to explore the interaction between finely resolved physical processes and the ecosystem. Here we focus on shelf-sea processes and the connection between the shelf seas and open-<span class="hlt">ocean</span>, and compare results with a 1/4 degree (eddy permitting) model that does not include shelf sea processes. We find tidal mixing fronts and river plume are well represented in the 1/12 degree model. Using approaches developed for the NW Shelf (Holt et al 2012), we provide estimates of across-shelf break nutrient fluxes to the seas surrounding this <span class="hlt">basin</span>, and relate these fluxes and their interannual variability to the physical processes driving <span class="hlt">ocean</span>-shelf exchange. Holt, J., et al, 2012. <span class="hlt">Oceanic</span> controls on the primary production of the northwest European continental shelf: model experiments under recent past conditions and a potential future scenario. Biogeosciences 9, 97-117. Holt, J., et al, 2014. Challenges in integrative approaches to modelling the marine ecosystems of the North Atlantic: Physics to Fish and Coasts to <span class="hlt">Ocean</span>. Progress in Oceanography doi:10.1016/j.pocean.2014.04.024.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58.1569M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58.1569M"><span>Seasonal evolution of the upper-<span class="hlt">ocean</span> <span class="hlt">adjacent</span> to the South Orkney Islands, Southern <span class="hlt">Ocean</span>: Results from a “lazy biological mooring”</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Meredith, Michael P.; Nicholls, Keith W.; Renfrew, Ian A.; Boehme, Lars; Biuw, Martin; Fedak, Mike</p> <p>2011-07-01</p> <p>A serendipitous >8-month time series of hydrographic properties was obtained from the vicinity of the South Orkney Islands, Southern <span class="hlt">Ocean</span>, by tagging a southern elephant seal ( Mirounga leonina) on Signy Island with a Conductivity-Temperature-Depth/Satellite-Relay Data Logger (CTD-SRDL) in March 2007. Such a time series (including data from the austral autumn and winter) would have been extremely difficult to obtain via other means, and it illustrates with unprecedented temporal resolution the seasonal progression of upper-<span class="hlt">ocean</span> water mass properties and stratification at this location. Sea ice production values of around 0.15-0.4 m month -1 for April to July were inferred from the progression of salinity, with significant levels still in September (around 0.2 m month -1). However, these values presume that advective processes have negligible effect on the salinity changes observed locally; this presumption is seen to be inappropriate in this case, and it is argued that the ice production rates inferred are better considered as "smeared averages" for the region of the northwestern Weddell Sea upstream from the South Orkneys. The impact of such advective effects is illustrated by contrasting the observed hydrographic series with the output of a one-dimensional model of the upper-<span class="hlt">ocean</span> forced with local fluxes. It is found that the difference in magnitude between local (modelled) and regional (inferred) ice production is significant, with estimates differing by around a factor of two. A halo of markedly low sea ice concentration around the South Orkneys during the austral winter offers at least a partial explanation for this, since it enabled stronger atmosphere/<span class="hlt">ocean</span> fluxes to persist and hence stronger ice production to prevail locally compared with the upstream region. The year of data collection was an El Niño year, and it is well-established that this phenomenon can impact strongly on the surface <span class="hlt">ocean</span> and ice field in this sector of the Southern <span class="hlt">Ocean</span>, thus</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20030064112&hterms=impacts+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dimpacts%2Bocean','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20030064112&hterms=impacts+ocean&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dimpacts%2Bocean"><span>Ejecta from <span class="hlt">Ocean</span> Impacts</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kyte, Frank T.</p> <p>2003-01-01</p> <p>Numerical simulations of deep-<span class="hlt">ocean</span> impact provide some limits on the size of a projectile that will not mix with the <span class="hlt">ocean</span> floor during a deep-<span class="hlt">ocean</span> impact. For a vertical impact at asteroidal velocities (approx. 20 km/s), mixing is only likely when the projectile diameter is greater than 112 of the water depth. For oblique impacts, even larger projectiles will not mix with <span class="hlt">ocean</span> floor silicates. Given the typical water depths of 4 to 5 km in deep-<span class="hlt">ocean</span> <span class="hlt">basins</span>, asteroidal projectiles with diameters as large as 2 or 3 km may commonly produce silicate ejecta that is composed only of meteoritic materials and seawater salts. However, the compressed water column beneath the projectile can still disrupt and shock metamorphose the <span class="hlt">ocean</span> floor. Therefore, production of a separate, terrestrial ejecta component is not ruled out in the most extreme case. With increasing projectile size (or energy) relative to water depths, there must be a gradation between <span class="hlt">oceanic</span> impacts and more conventional continental impacts. Given that 60% of the Earth's surface is covered by <span class="hlt">oceanic</span> lithosphere and 500 m projectiles impact the Earth on 10(exp 5) y timescales, there must be hundreds of <span class="hlt">oceanic</span> impact deposits in the sediment record awaiting discovery.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EP%26S...54..883I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EP%26S...54..883I"><span>Magnetic properties of sediments from <span class="hlt">Ocean</span> Drilling Program sites 1109, 1115, and 1118 (Leg 180), Woodlark <span class="hlt">Basin</span> (Papua New Guinea)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ishikawa, N.; Frost, G. M.</p> <p>2002-09-01</p> <p>Latest Miocene-Pleistocene synrift sediments at <span class="hlt">Ocean</span> Drilling Program sites 1109, 1115, and 1118 (Leg 180), located on the hanging wall margin north of the Moresby fault in the Woodlark <span class="hlt">Basin</span>, showed variations in magnetic parameters carried by magnetite and maghemite related to sedimentation process in the <span class="hlt">basin</span>. At sites 1109 and 1115, an increase in the sedimentation rate at 3.8 Ma was accompanied by the deposition of sediments with low ferrimagnetic mineral concentrations. An increase in the ferrimagnetic mineral concentrations occurred between 3.4 Ma and 3.2 Ma at the three sites. The onset age of the change became younger with distance from the subsidence center of the <span class="hlt">basin</span> near the Moresby fault: 3.4 Ma at Site 1118, 3.3 Ma at Site 1109, and 3.2 Ma at Site 1115, which implies a northward onlapping of sediments with high ferrimagnetic mineral concentration. Sediments with finer-grained ferrimagnetic minerals were deposited between 2.3 and 2.0 Ma at sites 1118 and 1109 and later, 2.8 Ma at Site 1115 during a period of a low sedimentation rate. The upper parts of sites 1109 and 1115 had a diamagnetic contribution, which is attributed to relatively high concentrations of diamagnetic pelagic materials at a low sedimentation rate associated with the low frequency of turbidites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP51B1067P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP51B1067P"><span>Chronostratigraphy and paleoenvironmental change in the Makarov <span class="hlt">Basin</span> of the western Arctic <span class="hlt">Ocean</span> during the last 1 Ma</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, K.; Nam, S. I.; Khim, B. K.; Kong, G. S.; Schreck, M.; Mackensen, A.; Niessen, F.</p> <p>2017-12-01</p> <p>Establishing an accurate chronostratigraphy is essential in reconstructing paleoenvironmental changes in the Arctic <span class="hlt">Ocean</span>. This requisition, however, has been impeded by the lack of biogenic remnants such as calcareous and siliceous microfossils, as well as alteration of paleomagnetic properties by post-depositional processes. Consequently, foundation of chronostratigraphy in the Arctic <span class="hlt">Ocean</span> has been mostly relying on stratigraphic correlations. This study examines lithological features and physical properties of sediments of gravity core ARA03B-41GC02 collected in the Makarov <span class="hlt">Basin</span> and correlates with previously studied cores from the western Arctic <span class="hlt">Ocean</span>, in order to establish an age model that could eventually facilitate a precise reconstruction of paleoenvironmental changes in the western Arctic <span class="hlt">Ocean</span>. Age control in the uppermost part was determined by AMS 14C dating of planktonic foraminifera and inter-core correlation was conducted in the upper ca. 3.8 m of the core which corresponded to MIS 15. Age constraints older than MIS 15 were treated using cyclostratigraphic model based on Mn-δ18O stack comparison, assuming that brown and high Mn concentration layers represent generally interglacial or interstadial periods. Based on our result, the core bottom corresponds to MIS 28 with an average sedimentation rate of ca. 0.5 cm/ky. The first appearance of detrital carbonate, planktonic foraminifera, and benthic foraminifera occurred during MIS 16, 11, and 7, respectively. MIS 16 is known as the coldest glacial period when δ18O of the LR04 stack first becomes heavier than 5‰; the occurrence of detrital carbonate likely transported from the Canadian Arctic indicates the initial buildup of the large ice sheets in the North America during this time. Since MIS 11 which is known as the warmest interglacial period during the late Pleistocene in the Northern Hemisphere, the appearance of planktonic foraminifera represents the warmer condition during interglacial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014E%26PSL.387...34V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014E%26PSL.387...34V"><span>River fluxes to the sea from the <span class="hlt">ocean</span>ʼs 10Be/9Be ratio</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>von Blanckenburg, Friedhelm; Bouchez, Julien</p> <p>2014-02-01</p> <p>The ratio of the meteoric cosmogenic radionuclide 10Be to the stable isotope 9Be is proposed here to be a flux proxy of terrigenous input into the <span class="hlt">oceans</span>. The <span class="hlt">ocean</span>'s dissolved 10Be/9Be is set by (1) the flux of meteoric 10Be produced in the atmosphere; (2) the denudational flux of the rivers discharging into a given <span class="hlt">ocean</span> <span class="hlt">basin</span>; (3) the fraction of 9Be that is released from primary minerals during weathering (meaning the 9Be transported by rivers in either the dissolved form or adsorbed onto sedimentary particles and incorporated into secondary oxides); and (4) the fraction of riverine 10Be and 9Be actually released into seawater. Using published 10Be/9Be data of rivers for which independent denudation rate estimates exist we first find that the global average fraction of 9Be released during weathering into river waters and their particulate load is 20% and does not depend on denudation rate. We then evaluate this quantitative proxy for terrigenous inputs by using published dissolved seawater Be isotope data and a compilation of global river loads. We find that the measured global average <span class="hlt">oceanic</span> dissolved 10Be/9Be ratio of about 0.9×10-7 is satisfied by the mass balance if only about 6% of the dissolved and adsorbed riverine Be is eventually released to the open <span class="hlt">ocean</span> after escaping the coastal zone. When we establish this mass balance for individual <span class="hlt">ocean</span> <span class="hlt">basins</span> good agreement results between 10Be/9Be ratios predicted from known river <span class="hlt">basin</span> denudation rates and measured <span class="hlt">ocean</span> 10Be/9Be ratios. Only in the South Atlantic and the South Pacific the 10Be/9Be ratio is dominated by advected Be and in these <span class="hlt">basins</span> the ratio is a proxy for <span class="hlt">ocean</span> circulation. As the seawater 10Be/9Be ratio is faithfully recorded in marine chemical precipitates the 10Be/9Be ratio extracted from authigenic sediments can now serve to estimate relative changes in terrigenous input into the <span class="hlt">oceans</span> back through time on a global and on an <span class="hlt">ocean</span> <span class="hlt">basin</span> scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/48360','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/48360"><span>Status and distribution of chinook salmon and steelhead in the interior Columbia River <span class="hlt">basin</span> and portions of the Klamath River <span class="hlt">basin</span> [Chapter 12</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Russell F. Thurow; Danny C. Lee; Bruce E. Rieman</p> <p>2000-01-01</p> <p>This chapter summarizes information on presence, absence, current status, and probable historical distribution of steelhead Oncorhynchus mykiss and stream-type (age-1 migrant) and <span class="hlt">ocean</span> type (age-0 migrant) chinook salmon O. tshawytscha in the interior Columbia River <span class="hlt">basin</span> and portions of the Klamath River <span class="hlt">basin</span>. Data were compiled from existing sources and via surveys...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021827','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021827"><span>Paleohydrogeology of the San Joaquin <span class="hlt">basin</span>, 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>Wilson, A.M.; Garven, G.; Boles, J.R.</p> <p>1999-01-01</p> <p>Mass transport can have a significant effect on chemical diagenetic processes in sedimentary <span class="hlt">basins</span>. This paper presents results from the first part of a study that was designed to explore the role of an evolving hydrodynamic system in driving mass transport and chemical diagenesis, using the San Joaquin <span class="hlt">basin</span> of California as a field area. We use coupled hydrogeologic models to establish the paleohydrogeology, thermal history, and behavior of nonreactive solutes in the <span class="hlt">basin</span>. These models rely on extensive geological information and account for variable-density fluid flow, heat transport, solute transport, tectonic uplift, sediment compaction, and clay dehydration. In our numerical simulations, tectonic uplift and <span class="hlt">ocean</span> regression led to large-scale changes in fluid flow and composition by strengthening topography-driven fluid flow and allowing deep influx of fresh ground water in the San Joaquin <span class="hlt">basin</span>. Sediment compaction due to rapid deposition created moderate overpressures, leading to upward flow from depth. The unusual distribution of salinity in the <span class="hlt">basin</span> reflects influx of fresh ground water to depths of as much as 2 km and dilution of saline fluids by dehydration reactions at depths greater than ???2.5 km. Simulations projecting the future salinity of the <span class="hlt">basin</span> show marine salinities persisting for more than 10 m.y. after <span class="hlt">ocean</span> regression. Results also show a change from topography-to compaction-driven flow in the Stevens Sandstone at ca. 5 Ma that coincides with an observed change in the diagenetic sequence. Results of this investigation provide a framework for future hydrologic research exploring the link between fluid flow and diagenesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GGG....17.5036P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GGG....17.5036P"><span>Madagascar's escape from Africa: A high-resolution plate reconstruction for the Western Somali <span class="hlt">Basin</span> and implications for supercontinent dispersal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Phethean, Jordan J. J.; Kalnins, Lara M.; van Hunen, Jeroen; Biffi, Paolo G.; Davies, Richard J.; McCaffrey, Ken J. W.</p> <p>2016-12-01</p> <p>Accurate reconstructions of the dispersal of supercontinent blocks are essential for testing continental breakup models. Here, we provide a new plate tectonic reconstruction of the opening of the Western Somali <span class="hlt">Basin</span> during the breakup of East and West Gondwana. The model is constrained by a new comprehensive set of spreading lineaments, detected in this heavily sedimented <span class="hlt">basin</span> using a novel technique based on directional derivatives of free-air gravity anomalies. Vertical gravity gradient and free-air gravity anomaly maps also enable the detection of extinct mid-<span class="hlt">ocean</span> ridge segments, which can be directly compared to several previous <span class="hlt">ocean</span> magnetic anomaly interpretations of the Western Somali <span class="hlt">Basin</span>. The best matching interpretations have <span class="hlt">basin</span> symmetry around the M0 anomaly; these are then used to temporally constrain our plate tectonic reconstruction. The reconstruction supports a tight fit for Gondwana fragments prior to breakup, and predicts that the continent-<span class="hlt">ocean</span> transform margin lies along the Rovuma <span class="hlt">Basin</span>, not along the Davie Fracture Zone (DFZ) as commonly thought. According to our reconstruction, the DFZ represents a major <span class="hlt">ocean-ocean</span> fracture zone formed by the coalescence of several smaller fracture zones during evolving plate motions as Madagascar drifted southwards, and offshore Tanzania is an obliquely rifted, rather than transform, margin. New seismic reflection evidence for <span class="hlt">oceanic</span> crust inboard of the DFZ strongly supports these conclusions. Our results provide important new constraints on the still enigmatic driving mechanism of continental rifting, the nature of the lithosphere in the Western Somali <span class="hlt">Basin</span>, and its resource potential.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP43A2068S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP43A2068S"><span>Sea-level and climate forcing of the Sr isotope composition of marginal <span class="hlt">basins</span> in the late Miocene Mediterranean <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schildgen, T. F.; Cosentino, D.; Frijia, G.; Castorina, F.; Dudas, F. O.; Iadanza, A.; Cipollari, P.; Caruso, A.; Bowring, S. A.; Strecker, M. R.</p> <p>2013-12-01</p> <p>Sr isotope records from marginal marine <span class="hlt">basins</span> track the mixing between sea water and local continental runoff. Because changes in sea level determine the amount of mixing between global marine and continental water, and climate affects the amount of continental runoff, both sea-level and climate changes can potentially be recorded in marine fossil Sr isotope composition. Our 128 new 87Sr/86Sr analyses on 73 oyster, foraminifera, and coral samples from eight late Miocene stratigraphic sections in southern Turkey, Crete, and Sicily show that 87Sr/86Sr in Mediterranean marginal <span class="hlt">basins</span> started to depart from global <span class="hlt">ocean</span> values several million years before the Messinian Salinity Crisis (MSC), with sub-<span class="hlt">basin</span> 87Sr/86Sr commonly dropping 0.000100 below contemporaneous global <span class="hlt">ocean</span> values. The marked departure coincided with tectonic uplift and <span class="hlt">basin</span> shallowing along the margins of the Mediterranean <span class="hlt">Basin</span>. In contrast, centrally-located <span class="hlt">basins</span> within the Mediterranean (e.g., Cyprus, Sicily, Crete) only record departures during the MSC. Besides this general trend, our 57 new 87Sr/86Sr analyses from the astronomically tuned Lower Evaporite unit deposited during the MSC in the central Apennines (Italy) allow us to explore in detail the effect of sea-level and humidity changes on 87Sr/86Sr . Most of the variation in 87Sr/86Sr that we observe can be explained by changes in eustatic sea level, with greatest departures from global <span class="hlt">ocean</span> values (with differences up to 0.000150) occurring during sea-level lowstands, which were characterized by relatively arid conditions in the Mediterranean. However, in a few cases, the greatest 87Sr/86Sr departures (up to 0.000300) occur during sea-level highstands, which are marked by more humid conditions. Because the correlations between peaks in Sr departures and highstands (humid conditions) occur only after episodes of prolonged aridity, variations of residence time of continental water (particularly groundwater) could have affected its Sr</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016Natur.540...94N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016Natur.540...94N"><span>Reorientation of Sputnik Planitia implies a subsurface <span class="hlt">ocean</span> on Pluto</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nimmo, F.; Hamilton, D. P.; McKinnon, W. B.; Schenk, P. M.; Binzel, R. P.; Bierson, C. J.; Beyer, R. A.; Moore, J. M.; Stern, S. A.; Weaver, H. A.; Olkin, C. B.; Young, L. A.; Smith, K. E.; Moore, J. M.; McKinnon, W. B.; Spencer, J. R.; Beyer, R.; Binzel, R. P.; Buie, M.; Buratti, B.; Cheng, A.; Cruikshank, D.; Ore, C. Dalle; Earle, A.; Gladstone, R.; Grundy, W.; Howard, A. D.; Lauer, T.; Linscott, I.; Nimmo, F.; Parker, J.; Porter, S.; Reitsema, H.; Reuter, D.; Roberts, J. H.; Robbins, S.; Schenk, P. M.; Showalter, M.; Singer, K.; Strobel, D.; Summers, M.; Tyler, L.; White, O. L.; Umurhan, O. M.; Banks, M.; Barnouin, O.; Bray, V.; Carcich, B.; Chaikin, A.; Chavez, C.; Conrad, C.; Hamilton, D. P.; Howett, C.; Hofgartner, J.; Kammer, J.; Lisse, C.; Marcotte, A.; Parker, A.; Retherford, K.; Saina, M.; Runyon, K.; Schindhelm, E.; Stansberry, J.; Steffl, A.; Stryk, T.; Throop, H.; Tsang, C.; Verbiscer, A.; Winters, H.; Zangari, A.; Stern, S. A.; Weaver, H. A.; Olkin, C. B.; Young, L. A.; Smith, K. E.</p> <p>2016-12-01</p> <p>The deep nitrogen-covered <span class="hlt">basin</span> on Pluto, informally named Sputnik Planitia, is located very close to the longitude of Pluto’s tidal axis and may be an impact feature, by analogy with other large <span class="hlt">basins</span> in the Solar System. Reorientation of Sputnik Planitia arising from tidal and rotational torques can explain the basin’s present-day location, but requires the feature to be a positive gravity anomaly, despite its negative topography. Here we argue that if Sputnik Planitia did indeed form as a result of an impact and if Pluto possesses a subsurface <span class="hlt">ocean</span>, the required positive gravity anomaly would naturally result because of shell thinning and <span class="hlt">ocean</span> uplift, followed by later modest nitrogen deposition. Without a subsurface <span class="hlt">ocean</span>, a positive gravity anomaly requires an implausibly thick nitrogen layer (exceeding 40 kilometres). To prolong the lifetime of such a subsurface <span class="hlt">ocean</span> to the present day and to maintain <span class="hlt">ocean</span> uplift, a rigid, conductive water-ice shell is required. Because nitrogen deposition is latitude-dependent, nitrogen loading and reorientation may have exhibited complex feedbacks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70016593','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70016593"><span>Holocene depocenter migration and sediment accumulation in Delaware Bay: A submerging marginal marine sedimentary <span class="hlt">basin</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>Fletcher, C. H.; Knebel, H.J.; Kraft, J.C.</p> <p>1992-01-01</p> <p>The Holocene transgression of the Delaware Bay estuary and <span class="hlt">adjacent</span> Atlantic coast results from the combined effect of regional crustal subsidence and eustasy. Together, the estuary and <span class="hlt">ocean</span> coast constitute a small sedimentary <span class="hlt">basin</span> whose principal depocenter has migrated with the transgression. A millenial time series of isopach and paleogeographic reconstructions for the migrating depocenter outlines the <span class="hlt">basin</span>-wide pattern of sediment distribution and accumulation. Upland sediments entering the <span class="hlt">basin</span> through the estuarine turbidity maximum accumulate in tidal wetland or open water sedimentary environments. Wind-wave activity at the edge of the tidal wetlands erodes the aggraded Holocene section and builds migrating washover barriers. Along the Atlantic and estuary coasts of Delaware, the area of the upland environment decreases from 2.0 billion m2 to 730 million m2 during the transgression. The area of the tidal wetland environment increases from 140 million to 270 million m2, and due to the widening of the estuary the area of open water increases from 190 million to 1.21 billion m2. Gross uncorrected rates of sediment accumulation for the tidal wetlands decrease from 0.64 mm/yr at 6 ka to 0.48 mm/yr at 1 ka. In the open water environments uncorrected rates decrease from 0.50 mm/yr to 0.04 mm/yr over the same period. We also present data on total sediment volumes within the tidal wetland and open water environments at specific intervals during the Holocene. </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMOS21D..07V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMOS21D..07V"><span>The pathways of Marine Plastic into the <span class="hlt">Ocean</span> Garbage Patches</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Sebille, E.; England, M. H.; Froyland, G.</p> <p>2013-12-01</p> <p>Much of the plastic debris in the near-surface <span class="hlt">ocean</span> collects in so-called garbage patches where, due to convergence of the surface flow, the debris is trapped for decades to millennia. Here, we use observational data from the Global Drifter Program in a particle-trajectory tracer approach to study the fate of marine debris in the open <span class="hlt">ocean</span> from coastal regions around the world on interannual to centennial time scales. We find that garbage patches emerge in each of the five subtropical <span class="hlt">basins</span>. The evolution of each of the five patches is markedly different, however. With the exception of the North Pacific, all patches are much more dispersive than expected from linear <span class="hlt">ocean</span> circulation theory, suggesting that on centennial time scales the different <span class="hlt">basins</span> are much better connected than previously thought and that inter-<span class="hlt">ocean</span> exchanges play a large role in the spreading of marine debris. In order to increase public awareness on this issue of sustainability in the <span class="hlt">ocean</span>, we have used the methods and data of this study to create a public website at www.adrift.org.au where all interested can investigate the spread of tracer from any and all points on the <span class="hlt">ocean</span> surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=185305&keyword=background+AND+wind&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=185305&keyword=background+AND+wind&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>COUPLING BETWEEN THE COASTAL <span class="hlt">OCEAN</span> AND YAQUINA BAY, OREGON: THE IMPORTANCE OF <span class="hlt">OCEANIC</span> INPUTS RELATIVE TO OTHER NITROGEN SOURCES</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>Understanding of the role of <span class="hlt">oceanic</span> input in nutrient loadings is important for understanding nutrient and phytoplankton dynamics in estuaries <span class="hlt">adjacent</span> to coastal upwelling regions as well as determining the natural background conditions. We examined the nitrogen sources to Yaqu...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21497089','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21497089"><span>Dynamic horizontal cultural transmission of humpback whale song at the <span class="hlt">ocean</span> <span class="hlt">basin</span> scale.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Garland, Ellen C; Goldizen, Anne W; Rekdahl, Melinda L; Constantine, Rochelle; Garrigue, Claire; Hauser, Nan Daeschler; Poole, M Michael; Robbins, Jooke; Noad, Michael J</p> <p>2011-04-26</p> <p>Cultural transmission, the social learning of information or behaviors from conspecifics, is believed to occur in a number of groups of animals, including primates, cetaceans, and birds. Cultural traits can be passed vertically (from parents to offspring), obliquely (from the previous generation via a nonparent model to younger individuals), or horizontally (between unrelated individuals from similar age classes or within generations). Male humpback whales (Megaptera novaeangliae) have a highly stereotyped, repetitive, and progressively evolving vocal sexual display or "song" that functions in sexual selection (through mate attraction and/or male social sorting). All males within a population conform to the current version of the display (song type), and similarities may exist among the songs of populations within an <span class="hlt">ocean</span> <span class="hlt">basin</span>. Here we present a striking pattern of horizontal transmission: multiple song types spread rapidly and repeatedly in a unidirectional manner, like cultural ripples, eastward through the populations in the western and central South Pacific over an 11-year period. This is the first documentation of a repeated, dynamic cultural change occurring across multiple populations at such a large geographic scale. Copyright © 2011 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/fs/2018/3031/fs20183031.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/fs/2018/3031/fs20183031.pdf"><span>Klamath River <span class="hlt">Basin</span> water-quality data</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Smith, Cassandra D.; Rounds, Stewart A.; Orzol, Leonard L.; Sobieszczyk, Steven</p> <p>2018-05-29</p> <p>The Klamath River <span class="hlt">Basin</span> stretches from the mountains and inland <span class="hlt">basins</span> of south-central Oregon and northern California to the Pacific <span class="hlt">Ocean</span>, spanning multiple climatic regions and encompassing a variety of ecosystems. Water quantity and water quality are important topics in the <span class="hlt">basin</span>, because water is a critical resource for farming and municipal use, power generation, and for the support of wildlife, aquatic ecosystems, and endangered species. Upper Klamath Lake is the largest freshwater lake in Oregon (112 square miles) and is known for its seasonal algal blooms. The Klamath River has dams for hydropower and the upper <span class="hlt">basin</span> requires irrigation water to support agriculture and grazing. Multiple species of endangered fish inhabit the rivers and lakes, and the marshes are key stops on the Pacific flyway for migrating birds. For these and other reasons, the water resources in this <span class="hlt">basin</span> have been studied and monitored to support their management distribution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN33A0103B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN33A0103B"><span>Tools and Methods for Visualization of Mesoscale <span class="hlt">Ocean</span> Eddies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bemis, K. G.; Liu, L.; Silver, D.; Kang, D.; Curchitser, E.</p> <p>2017-12-01</p> <p>Mesoscale <span class="hlt">ocean</span> eddies form in the Gulf Stream and transport heat and nutrients across the <span class="hlt">ocean</span> <span class="hlt">basin</span>. The internal structure of these three-dimensional eddies and the kinematics with which they move are critical to a full understanding of their transport capacity. A series of visualization tools have been developed to extract, characterize, and track <span class="hlt">ocean</span> eddies from 3D modeling results, to visually show the <span class="hlt">ocean</span> eddy story by applying various illustrative visualization techniques, and to interactively view results stored on a server from a conventional browser. In this work, we apply a feature-based method to track instances of <span class="hlt">ocean</span> eddies through the time steps of a high-resolution multidecadal regional <span class="hlt">ocean</span> model and generate a series of eddy paths which reflect the life cycle of individual eddy instances. The basic method uses the Okubu-Weiss parameter to define eddy cores but could be adapted to alternative specifications of an eddy. Stored results include pixel-lists for each eddy instance, tracking metadata for eddy paths, and physical and geometric properties. In the simplest view, isosurfaces are used to display eddies along an eddy path. Individual eddies can then be selected and viewed independently or an eddy path can be viewed in the context of all eddy paths (longer than a specified duration) and the <span class="hlt">ocean</span> <span class="hlt">basin</span>. To tell the story of mesoscale <span class="hlt">ocean</span> eddies, we combined illustrative visualization techniques, including visual effectiveness enhancement, focus+context, and smart visibility, with the extracted volume features to explore eddy characteristics at multiple scales from <span class="hlt">ocean</span> <span class="hlt">basin</span> to individual eddy. An evaluation by domain experts indicates that combining our feature-based techniques with illustrative visualization techniques provides an insight into the role eddies play in <span class="hlt">ocean</span> circulation. A web-based GUI is under development to facilitate easy viewing of stored results. The GUI provides the user control to choose amongst available</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFM.T31B1303C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFM.T31B1303C"><span>Walled Sedimentary <span class="hlt">Basins</span> of China: Perpetrators or Victims of Plateau Growth?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carroll, A. R.; Graham, S. A.; Smith, M. E.</p> <p>2004-12-01</p> <p>Western China and <span class="hlt">adjacent</span> areas of central Asia are characterized by low relief, internally drained sedimentary <span class="hlt">basins</span> that are divided by actively uplifting mountain ranges. The margins of these <span class="hlt">basins</span> often show evidence for extensive contractional deformation, yet their interiors are surprisingly stable. <span class="hlt">Basins</span> such as the Tarim and Junggar also exhibit long and apparently continuous histories of closed drainage in the same approximate location (over 250 my in the case of Junggar). In contrast to traditional foreland <span class="hlt">basins</span>, these <span class="hlt">basins</span> are not uniquely associated with a specific thrust belt, nor do they show evidence for underlying decollements. We therefore propose the new term "walled <span class="hlt">basin</span>", in recognition of the essential role of peripheral orogenic walls in creating and maintaining closed drainage and impounding sediments. Walled <span class="hlt">basins</span> in Asia currently are restricted to areas that receive less than 40 cm/yr precipitation, suggesting that aridity plays a role in preventing fluvial breach of the <span class="hlt">basin</span> walls (cf., Sobel et al., 2003). Entrapment of sediment within the closed Qaidam <span class="hlt">basin</span> in the northeast Tibetan plateau has been implicated as a potential mechanism of plateau growth, based on the observations that the <span class="hlt">basin</span> retains mass within the orogen and creates level topography. However, we propose that the Qaidam instead represents a walled <span class="hlt">basin</span> that has been elevated due to underplating of the plateau, and is fated to eventual destruction as deformation continues. Several lines of reasoning support this conclusion. First, DEM analysis shows that modern drainage divides for the Qaidam and other walled <span class="hlt">basins</span> never rise more than 1-2 km above the <span class="hlt">basin</span> floors, limiting the amount of possible topgraphic infill. Second, the Tarim and Junggar <span class="hlt">basins</span> presently remain well below 2000 m and probably have never been higher, despite receiving large influxes of detritus from <span class="hlt">adjacent</span> ranges. Third, the Qaidam <span class="hlt">basin</span>, like the Tarim and Junggar <span class="hlt">basins</span>, has an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAESc.156..316K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAESc.156..316K"><span>Moho depth variations over the Maldive Ridge and adjoining Arabian and Central Indian <span class="hlt">Basins</span>, Western Indian <span class="hlt">Ocean</span>, from three dimensional inversion of gravity anomalies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kunnummal, Priyesh; Anand, S. P.; Haritha, C.; Rama Rao, P.</p> <p>2018-05-01</p> <p>Analysis of high resolution satellite derived free air gravity data has been undertaken in the Greater Maldive Ridge (GMR) (Maldive Ridge, Deep Sea Channel, northern limit of Chagos Bank) segment of the Chagos Laccadive Ridge and the adjoining Arabian and Central Indian <span class="hlt">Basins</span>. A Complete Bouguer Anomaly (CBA) map was generated from the Indian <span class="hlt">Ocean</span> Geoidal Low removed Free Air Gravity (hereinafter referred to as "FAG-IOGL") data by incorporating Bullard A, B and C corrections. Using the Parker method, Moho topography was initially computed by inverting the CBA data. From the CBA the Mantle Residual Gravity Anomalies (MRGA) were computed by incorporating gravity effects of sediments and lithospheric temperature and pressure induced anomalies. Further, the MRGA was inverted to get Moho undulations from which the crustal thickness was also estimated. It was found that incorporating the lithospheric thermal and pressure anomaly correction has provided substantial improvement in the computed Moho depths especially in the <span class="hlt">oceanic</span> areas. But along the GMR, there was not much variation in the Moho thickness computed with and without the thermal and pressure gravity correction implying that the crustal thickness of the ridge does not depend on the <span class="hlt">oceanic</span> isochrones used for the thermal corrections. The estimated Moho depths in the study area ranges from 7 km to 28 km and the crustal thickness from 2 km to 27 km. The Moho depths are shallower in regions closer to Central Indian Ridge in the Arabian <span class="hlt">Basin</span> i.e., the region to the west of the GMR is thinner compared to the region in the east (Central Indian <span class="hlt">Basin</span>). The thickest crust and the deepest Moho are found below the N-S trending GMR segment of the Chagos-Laccadive Ridge. Along the GMR the crustal thickness decreases from north to south with thickness of 27 km below the Maldives Ridge reducing to ∼9 km at 3°S and further increasing towards Chagos Bank. Even though there are similarities in crustal thickness between</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JAESc..40..569P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JAESc..40..569P"><span>Geochemistry of ferromanganese nodule-sediment pairs from Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pattan, J. N.; Parthiban, G.</p> <p>2011-01-01</p> <p>Fourteen ferromanganese nodule-sediment pairs from different sedimentary environments such as siliceous ooze (11), calcareous ooze (two) and red clay (one) from Central Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (CIOB) were analysed for major, trace and rare earth elements (REE) to understand the possible elemental relationship between them. Nodules from siliceous and calcareous ooze are diagenetic to early diagenetic whereas, nodule from red clay is of hydrogenetic origin. Si, Al and Ba are enriched in the sediments compared to associated nodules; K and Na are almost in the similar range in nodule-sediment pairs and Mn, Fe, Ti, Mg, P, Ni, Cu, Mo, Zn, Co, Pb, Sr, V, Y, Li and REEs are all enriched in nodules compared to associated sediments (siliceous and calcareous). Major portion of Si, Al and K in both nodules and sediments appear to be of terrigenous nature. The elements which are highly enriched in the nodules compared to associated sediments from both siliceous and calcareous ooze are Mo - (307, 273), Ni - (71, 125), Mn - (64, 87), Cu - (43, 80), Co - (23, 75), Pb - (15, 24), Zn - (9, 11) and V - (8, 19) respectively. These high enrichment ratios of elements could be due to effective diagenetic supply of metals from the underlying sediment to the nodule. Enrichment ratios of transition metals and REEs in the nodule to sediment are higher in CIOB compared to Pacific and Atlantic <span class="hlt">Ocean</span>. Nodule from red clay, exhibit very small enrichment ratio of four with Mn and Ce while, Al, Fe, Ti, Ca, Na, K, Mg, P, Zn, Co, V, Y and REE are all enriched in red clay compared to associated nodule. This is probably due to presence of abundant smectite, fish teeth, micronodules and phillipsite in the red clay. The strong positive correlation ( r ⩾ 0.8) of Mn with Ni, Cu, Zn and Mo and a convex pattern of shale-normalized REE pattern with positive Ce-anomaly of siliceous ooze could be due to presence of abundant manganese micronodules. None of the major trace and REE exhibits any type of inter</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/2014NHESD...2.1671P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014NHESD...2.1671P"><span>Spatial and seasonal responses of precipitation in the Ganges and Brahmaputra river <span class="hlt">basins</span> to ENSO and Indian <span class="hlt">Ocean</span> dipole modes: implications for flooding and drought</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pervez, M. S.; Henebry, G. M.</p> <p>2014-02-01</p> <p>We evaluated the spatial and temporal responses of precipitation in the <span class="hlt">basins</span> as modulated by the El Niño Southern Oscillation (ENSO) and Indian <span class="hlt">Ocean</span> (IO) dipole modes using observed precipitation records at 43 stations across the Ganges and Brahmaputra <span class="hlt">basins</span> from 1982 to 2010. Daily observed precipitation records were extracted from Global Surface Summary of the Day dataset and spatial and monthly anomalies were computed. The anomalies were averaged for the years influenced by climate modes combinations. Occurrences of El Niño alone significantly reduced (60% and 88% of baseline in the Ganges and Brahmaputra <span class="hlt">basins</span>, respectively) precipitation during the monsoon months in the northwestern and central Ganges <span class="hlt">basin</span> and across the Brahmaputra <span class="hlt">basin</span>. In contrast, co-occurrence of La Niña and a positive IO dipole mode significantly enhanced (135% and 160% of baseline, respectively) precipitation across both <span class="hlt">basins</span>. During the co-occurrence of neutral phases in both climate modes (occurring 13 out of 28 yr), precipitation remained below average to average in the agriculturally extensive areas of Haryana, Uttar Pradesh, Bihar, eastern Nepal, and the Rajshahi district in Bangladesh in the Ganges <span class="hlt">basin</span> and northern Bangladesh, Meghalaya, Assam, and Arunachal Pradesh in the Brahmaputra <span class="hlt">basin</span>. This pattern implies that a regular water deficit is likely in these areas with implications for the agriculture sector due to its reliance on consistent rainfall for successful production. Major flooding and drought occurred as a consequence of the interactive effects of the ENSO and IO dipole modes, with the sole exception of extreme precipitation and flooding during El Niño events. This observational analysis will facilitate well informed decision making in minimizing natural hazard risks and climate impacts on agriculture, and supports development of strategies ensuring optimized use of water resources in best management practice under changing climate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70014227','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70014227"><span><span class="hlt">Basin</span>-ring spacing on the Moon, Mercury, and 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>Pike, R.J.; Spudis, P.D.</p> <p>1987-01-01</p> <p>Radial spacing between concentric rings of impact <span class="hlt">basins</span> that lack central peaks is statistically similar and nonrandom on the Moon, Mercury, and Mars, both inside and outside the main ring. One spacing interval, (2.0 ?? 0.3)0.5D, or an integer multiple of it, dominates most <span class="hlt">basin</span> rings. Three analytical approaches yield similar results from 296 remapped or newly mapped rings of 67 multi-ringed <span class="hlt">basins</span>: least-squares of rank-grouped rings, least-squares of rank and ring diameter for each <span class="hlt">basin</span>, and averaged ratios of <span class="hlt">adjacent</span> rings. Analysis of 106 rings of 53 two-ring <span class="hlt">basins</span> by the first and third methods yields an integer multiple (2 ??) of 2.00.5D. There are two exceptions: (1) Rings <span class="hlt">adjacent</span> to the main ring of multi-ring <span class="hlt">basins</span> are consistently spaced at a slightly, but significantly, larger interval, (2.1 ?? 0.3)0.5D; (2) The 88 rings of 44 protobasins (large peak-plus-inner-ring craters) are spaced at an entirely different interval (3.3 ?? 0.6)0.5D. The statistically constant and target-invariant spacing of so many rings suggests that this characteristic may constrain formational models of impact <span class="hlt">basins</span> on the terrestrial planets. The key elements of such a constraint include: (1) ring positions may not have been located by the same process(es) that formed ring topography; (2) ring location and emplacement of ring topography need not be coeval; (3) ring location, but not necessarily the mode of ring emplacement, reflects one process that operated at the time of impact; and (4) the process yields similarly-disposed topographic features that are spatially discrete at 20.5D intervals, or some multiple, rather than continuous. These four elements suggest that some type of wave mechanism dominates the location, but not necessarily the formation, of <span class="hlt">basin</span> rings. The waves may be standing, rather than travelling. The ring topography itself may be emplaced at impact by this and/or other mechanisms and may reflect additional, including post-impact, influences. ?? 1987</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC41B1015W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC41B1015W"><span>Interannual to Decadal SST Variability in the Tropical Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, G.; Newman, M.; Han, W.</p> <p>2017-12-01</p> <p>The Indian <span class="hlt">Ocean</span> has received increasing attention in recent years for its large impacts on regional and global climate. However, due mainly to the close interdependence of the climate variation within the Tropical Pacific and the Indian <span class="hlt">Ocean</span>, the internal sea surface temperature (SST) variability within the Indian <span class="hlt">Ocean</span> has not been studied extensively on longer time scales. In this presentation we will show analysis of the interannual to decadal SST variability in the Tropical Indian <span class="hlt">Ocean</span> in observations and Linear Inverse Model (LIM) results. We also compare the decoupled Indian <span class="hlt">Ocean</span> SST variability from the Pacific against fully coupled one based on LIM integrations, to test the factors influence the features of the leading SST modes in the Indian <span class="hlt">Ocean</span>. The result shows the Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> (IOB) mode, which is strongly related to global averaged SST variability, passively responses to the Pacific variation. Without tropical Indo-Pacific coupling interaction, the intensity of IOB significantly decreases by 80%. The Indian <span class="hlt">Ocean</span> Dipole (IOD) mode demonstrates its independence from the Pacific SST variability since the IOD does not change its long-term characteristics at all without inter-<span class="hlt">basin</span> interactions. The overall SSTA variance decreases significantly in the Tropical Indian <span class="hlt">Ocean</span> in the coupling restricted LIM runs, especially when the one-way impact from the Pacific to the Indian <span class="hlt">Ocean</span> is turned off, suggesting that most of the variability in the Indian <span class="hlt">Ocean</span> comes from the Pacific influence. On the other hand, the Indian <span class="hlt">Ocean</span> could also transport anomalies to the Pacific, making the interaction a complete two-way process.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PrOce.129..285H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PrOce.129..285H"><span>Challenges in integrative approaches to modelling the marine ecosystems of the North Atlantic: Physics to fish and coasts to <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Holt, Jason; Icarus Allen, J.; Anderson, Thomas R.; Brewin, Robert; Butenschön, Momme; Harle, James; Huse, Geir; Lehodey, Patrick; Lindemann, Christian; Memery, Laurent; Salihoglu, Baris; Senina, Inna; Yool, Andrew</p> <p>2014-12-01</p> <p>It has long been recognised that there are strong interactions and feedbacks between climate, upper <span class="hlt">ocean</span> biogeochemistry and marine food webs, and also that food web structure and phytoplankton community distribution are important determinants of variability in carbon production and export from the euphotic zone. Numerical models provide a vital tool to explore these interactions, given their capability to investigate multiple connected components of the system and the sensitivity to multiple drivers, including potential future conditions. A major driver for ecosystem model development is the demand for quantitative tools to support ecosystem-based management initiatives. The purpose of this paper is to review approaches to the modelling of marine ecosystems with a focus on the North Atlantic <span class="hlt">Ocean</span> and its <span class="hlt">adjacent</span> shelf seas, and to highlight the challenges they face and suggest ways forward. We consider the state of the art in simulating <span class="hlt">oceans</span> and shelf sea physics, planktonic and higher trophic level ecosystems, and look towards building an integrative approach with these existing tools. We note how the different approaches have evolved historically and that many of the previous obstacles to harmonisation may no longer be present. We illustrate this with examples from the on-going and planned modelling effort in the Integrative Modelling Work Package of the EURO-<span class="hlt">BASIN</span> programme.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015Geote..49...27K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015Geote..49...27K"><span>Correlation of Late Precambrian and Paleozoic events in the East European platform and the <span class="hlt">adjacent</span> paleooceanic domains</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kheraskova, T. N.; Volozh, Yu. A.; Antipov, M. P.; Bykadorov, V. A.; Sapozhnikov, R. B.</p> <p>2015-01-01</p> <p>The correlation of geological events and structure-forming processes occurring contemporaneously in the inner parts of cratons and the <span class="hlt">adjacent</span> paleooceanic <span class="hlt">basins</span> is discussed in order to understand the effects of these processes on sedimentation and structural rearrangements. For this purpose, a series of paleodynamic reconstructions of the Riphean, Vendian, and Paleozoic epicontinental <span class="hlt">basins</span> of the East European Platform and zones of their transition to marginal <span class="hlt">basins</span> of the same age once situated in the Ural, Timan, Caucasus, Scandinavian fold regions and in the Scythian-Turan Plate have been performed on the basis of the available original and published data combined with interpretation of seismic profiles. As a result, a set of structural-facies maps of this territory have been compiled for several time intervals from the Late Riphean to Early Permian.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.1447H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.1447H"><span>Crustal structure of the Boreas <span class="hlt">Basin</span> formed at ultraslow spreading Knipovich Ridge - Northern North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hermann, T.; Jokat, W.</p> <p>2012-04-01</p> <p>The Boreas <span class="hlt">Basin</span> is located in Norwegian Greenland Sea bordered by the Greenland Fracture Zone in the south and the Hovgard Ridge in the north, respectively. In the east it adjoins the ultraslow mid-<span class="hlt">ocean</span> Knipovich Ridge. Previous seismic reflection studies in the Boreas <span class="hlt">Basin</span> have shown that the basement topography has a roughness, which is typical for ultraslow spreading ridges. This observation supports assumptions that the <span class="hlt">basin</span> was formed at ultraslow spreading rates during its entire geological history. However, the detailed crustal structure remained unresolved. In summer 2009 new seismic refraction data were acquired in the Boreas <span class="hlt">Basin</span> during the expedition ARK-XXIV/3 with the research vessel Polarstern. The deep seismic sounding line has a length of 340 km. Forward modelling of the data of 18 <span class="hlt">ocean</span> bottom seismometers deployed along the NW-SE trending profile reveal an unusual 3.2 km thin <span class="hlt">oceanic</span> crust. The crustal model is further constrained by S-wave and 2D gravity modelling. The P-wave velocity model shows a layered <span class="hlt">oceanic</span> crust without <span class="hlt">oceanic</span> layer 3 and with velocities less than 6.3 km/s except beneath a nearly 2000 m high seamount. Beneath the seamount velocities of up to 6.7 km/s were observed. The mantle velocities range between 7.5 km/s in the uppermost mantle and 8.0 km/s in almost 15 km depth. A serpentinisation of approximately 13% in the uppermost mantle decreasing downwards can explain the low mantle velocities. In summary, the transect confirms earlier models that the entire Boreas <span class="hlt">Basin</span> was formed at ultraslow spreading rates. Indications for this are the basement roughness and the overall thin <span class="hlt">oceanic</span> crust. Both observations are typical for ultraslow spreading systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=69342&keyword=indian&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=69342&keyword=indian&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>ON THE WIND-INDUCED EXCHANGE BETWEEN INDIAN RIVER BAY, DELAWARE AND THE <span class="hlt">ADJACENT</span> CONTINENTAL SHELF. (R826945)</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><p>The structure of the wind-induced exchange between Indian River Bay, Delaware and the <span class="hlt">adjacent</span> continental shelf is examined based on current measurements made at the Indian River Inlet which represents the only conduit of exchange between the bay and the coastal <span class="hlt">ocean</span>. Local ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1916685G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1916685G"><span>From rifting to spreading - seismic structure of the rifted western Mariana extinct arc and the ParceVela back-arc <span class="hlt">basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Grevemeyer, Ingo; Kodaira, Shuichi; Fujie, Gou; Takahashi, Narumi</p> <p>2017-04-01</p> <p> <span class="hlt">adjacent</span> <span class="hlt">basins</span> mimic the structure found in the Lau <span class="hlt">Basin</span> - Tonga Arc system, perhaps indicating entrainment of hydrous melts from the <span class="hlt">adjacent</span> arc governing early seafloor spreading when the spreading centre was at close distant to the volcanic arc. Upper mantle below the PVB shows typical mantle properties, supporting a P-wave velocity of >8 km/s. However, with respect to <span class="hlt">oceanic</span> crust sampled in the Pacific <span class="hlt">Basin</span>, PVB crust is with 5 km thinner and seismic velocities in the lower crust are with 6.7 km/s much lower.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122..980S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122..980S"><span>Spatial variability of the Arctic <span class="hlt">Ocean</span>'s double-diffusive staircase</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shibley, N. C.; Timmermans, M.-L.; Carpenter, J. R.; Toole, J. M.</p> <p>2017-02-01</p> <p>The Arctic <span class="hlt">Ocean</span> thermohaline stratification frequently exhibits a staircase structure overlying the Atlantic Water Layer that can be attributed to the diffusive form of double-diffusive convection. The staircase consists of multiple layers of O(1) m in thickness separated by sharp interfaces, across which temperature and salinity change abruptly. Through a detailed analysis of Ice-Tethered Profiler measurements from 2004 to 2013, the double-diffusive staircase structure is characterized across the entire Arctic <span class="hlt">Ocean</span>. We demonstrate how the large-scale Arctic <span class="hlt">Ocean</span> circulation influences the small-scale staircase properties. These staircase properties (layer thicknesses and temperature and salinity jumps across interfaces) are examined in relation to a bulk vertical density ratio spanning the staircase stratification. We show that the Lomonosov Ridge serves as an approximate boundary between regions of low density ratio (approximately 3-4) on the Eurasian side and higher density ratio (approximately 6-7) on the Canadian side. We find that the Eurasian <span class="hlt">Basin</span> staircase is characterized by fewer, thinner layers than that in the Canadian <span class="hlt">Basin</span>, although the margins of all <span class="hlt">basins</span> are characterized by relatively thin layers and the absence of a well-defined staircase. A double-diffusive 4/3 flux law parametrization is used to estimate vertical heat fluxes in the Canadian <span class="hlt">Basin</span> to be O(0.1) W m-2. It is shown that the 4/3 flux law may not be an appropriate representation of heat fluxes through the Eurasian <span class="hlt">Basin</span> staircase. Here molecular heat fluxes are estimated to be between O(0.01) and O(0.1) W m-2. However, many uncertainties remain about the exact nature of these fluxes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T31C0644B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T31C0644B"><span>Geothermal heating in the Panama <span class="hlt">Basin</span> and its impact on water mass transformation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Banyte, D.; Morales Maqueda, M. A.; Hobbs, R. W.; Megann, A.; Smeed, D.</p> <p>2017-12-01</p> <p>Geothermal heating is a driving force of abyssal water transformation. To quantify its impact at the <span class="hlt">basin</span> scale, a hydrographic survey of the Panama <span class="hlt">Basin</span> was carried out in 2014-2015 as part of the international project OSCAR (Oceanographic and Seismic Characterisation of heat dissipation and alteration by hydrothermal fluids at an Axial Ridge). The study shows that about half of the water entering the <span class="hlt">basin</span>, which is connected to the Pacific <span class="hlt">Ocean</span> only through the a narrow passage part of the Ecuador Trench, is converted to lighter water within just 200 km downstream of the passage. Of the resulting water, a staggering 90% is transformed by geothermal heating inside the <span class="hlt">basin</span>, welling up into the <span class="hlt">ocean</span> interior from a bottom boundary layer (BBL) that can be up to 1000 m thick. The geothermal forcing leaves an imprint in temperature-salinity properties hundreds of meters above the thick BBL. We present a conceptual model of the abyssal water transformation in the <span class="hlt">basin</span> that incorporates these processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRII.137..307L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRII.137..307L"><span>Gene flow between Atlantic and Pacific <span class="hlt">Ocean</span> <span class="hlt">basins</span> in three lineages of deep-sea clams (Bivalvia: Vesicomyidae: Pliocardiinae) and subsequent limited gene flow within the Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>LaBella, Abigail Leavitt; Van Dover, Cindy L.; Jollivet, Didier; Cunningham, Clifford W.</p> <p>2017-03-01</p> <p>Pliocardiin (vesicomyid) clams rely on microbial symbionts for nutrition and are obligate inhabitants of deep-sea chemosynthetic ecosystems. Unlike many other invertebrate hosts of chemosynthetic microbes, pliocardiin clams are found in every <span class="hlt">ocean</span> in a variety of reducing habitats, including hydrothermal vents, cold seeps, organic falls and deep-sea fans. The global distribution of pliocardiin clams suggests historical gene flow between <span class="hlt">ocean</span> <span class="hlt">basins</span>. We focus on 3 pliocardiin genera-'Pliocardia' I, Calyptogena and Abyssogena-each of which has a pair of sister clades in the Atlantic and Pacific. Our work tests the hypothesis that historical gene flow between the Atlantic and Pacific <span class="hlt">Oceans</span> within these genera was interrupted by the closure of the Panamanian seaway and tests whether isolation between the <span class="hlt">ocean</span> <span class="hlt">basins</span> is the result of vicariance or past colonization. These questions are investigated in the context of fossil evidence, biogeography and phylogenetics. This study revealed a set of substitution rates consistent with other invertebrate studies (μ=0.8%/My/lineage), and a set consistent with much lower rates often attributed to deep-sea organisms (μ=0.3%/My/lineage). Among the Pacific/Atlantic sister pairs, 'Pliocardia' I COI divergence per lineage is intermediate (2.5%), Calyptogena is the highest (6.1%) and Abyssogena the lowest (0.8%). The substitution rates suggest that 'Pliocardia' I and Calyptogena have histories of at least 2.8 My in the Atlantic, with Calyptogena likely older. The slower rate, however, is inconsistent with both the maximum age of the family and several well studied fossils: leaving the faster rate preferred. With the faster rate, the Abyssogena southwardae clade diverged from its Pacific sister clade around 1 Mya, which likely post-dates the closure of the Isthmus of Panama and the opening of the Bering Strait. In light of this recent divergence, we test the previously proposed hypothesis that there is a high level of ongoing gene</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=water+AND+politics&pg=5&id=ED235091','ERIC'); return false;" href="https://eric.ed.gov/?q=water+AND+politics&pg=5&id=ED235091"><span>The Future of the Pacific <span class="hlt">Basin</span>: A Keynote Address.</span></a></p> <p><a target="_blank" href="http://www.eric.ed.gov/ERICWebPortal/search/extended.jsp?_pageLabel=advanced">ERIC Educational Resources Information Center</a></p> <p>Cleveland, Harlan</p> <p></p> <p>People of the Pacific <span class="hlt">Basin</span> must decide how to manage the Pacific <span class="hlt">Ocean</span> commons, who does what in a changing industrial structure, and how to adapt to the new technological revolution. Although the United Nations' Law of the Sea moved into national jurisdiction many of the <span class="hlt">ocean</span> resources of the Pacific Region, there is one new major…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70021101','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70021101"><span>More than one way to stretch: A tectonic model for extension along the plume track of the Yellowstone hotspot and <span class="hlt">adjacent</span> <span class="hlt">Basin</span> and Range Province</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Parsons, T.; Thompson, G.A.; Smith, R.P.</p> <p>1998-01-01</p> <p>The eastern Snake River Plain of southern Idaho poses a paradoxical problem because it is nearly aseismic and unfaulted although it appears to be actively extending in a SW-NE direction continuously with the <span class="hlt">adjacent</span> block-faulted <span class="hlt">Basin</span> and Range Province. The plain represents the 100-km-wide track of the Yellowstone hotspot during the last ???16-17 m.y., and its crust has been heavily intruded by mafic magma, some of which has erupted to the surface as extensive basalt flows. Outside the plain's distinct topographic boundaries is a transition zone 30-100 km wide that has variable expression of normal faulting and magmatic activity as compared with the surrounding <span class="hlt">Basin</span> and Range Province. Many models for the evolution of the Snake River Plain have as an integral component the suggestion that the crust of the plain became strong enough through basaltic intrusion to resist extensional deformation. However, both the boundaries of the plain and its transition zone lack any evidence of zones of strike slip or other accommodation that would allow the plain to remain intact while the <span class="hlt">Basin</span> and Range Province extended around it; instead, the plain is coupled to its surroundings and extending with them. We estimate strain rates for the northern <span class="hlt">Basin</span> and Range Province from various lines of evidence and show that these strains would far exceed the elastic limit of any rocks coupled to the <span class="hlt">Basin</span> and Range; thus, if the plain is extending along with its surroundings, as the geologic evidence indicates, it must be doing so by a nearly aseismic process. Evidence of the process is provided by volcanic rift zones, indicators of subsurface dikes, which trend across the plain perpendicular to its axis. We suggest that variable magmatic strain accommodation, by emplacement and inflation of dikes perpendicular to the least principal stress in the elastic crust, allows the crust of the plain to extend nearly aseismically. Dike injection releases accumulated elastic strain but</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.6295V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.6295V"><span>Lagrangian pathways of upwelling in the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Viglione, Giuliana A.; Thompson, Andrew F.</p> <p>2016-08-01</p> <p>The spatial and temporal variability of upwelling into the mixed layer in the Southern <span class="hlt">Ocean</span> is studied using a 1/10<mrow></mrow>° <span class="hlt">ocean</span> general circulation model. Virtual drifters are released in a regularly spaced pattern across the Southern <span class="hlt">Ocean</span> at depths of 250, 500, and 1000 m during both summer and winter months. The drifters are advected along isopycnals for a period of 4 years, unless they outcrop into the mixed layer, where lateral advection and a parameterization of vertical mixing are applied. The focus of this study is on the discrete exchange between the model mixed layer and the interior. Localization of interior-mixed layer exchange occurs downstream of major topographic features across the Indian and Pacific <span class="hlt">basins</span>, creating "hotspots" of outcropping. Minimal outcropping occurs in the Atlantic <span class="hlt">basin</span>, while 59% of drifters outcrop in the Pacific sector and in Drake Passage (the region from 140<mrow></mrow>° W to 40<mrow></mrow>° W), a disproportionately large amount even when considering the relative <span class="hlt">basin</span> sizes. Due to spatial and temporal variations in mixed layer depth, the Lagrangian trajectories provide a statistical measure of mixed layer residence times. For each exchange into the mixed layer, the residence time has a Rayleigh distribution with a mean of 30 days; the cumulative residence time of the drifters is 261 ± 194 days, over a period of 4 years. These results suggest that certain <span class="hlt">oceanic</span> gas concentrations, such as CO2 and 14C, will likely not reach equilibrium with the atmosphere before being resubducted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..14.4977G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..14.4977G"><span>The African Plate: A history of <span class="hlt">oceanic</span> crust accretion and subduction since the Jurassic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gaina, C.; Torsvik, T. H.; Labails, C.; van Hinsbergen, D.; Werner, S.; Medvedev, S.</p> <p>2012-04-01</p> <p>Initially part of Gondwana and Pangea, and now surrounded almost entirely by spreading centres, the African plate moved relatively slowly for the last 200 million years. Yet both Africa's cratons and passive margins were affected by tectonic stresses developed at distant plate boundaries. Moreover, the African plate was partly underlain by hot mantle (at least for the last 300 Ma) - either a series of hotspots or a superswell, or both - that contributed to episodic volcanism, <span class="hlt">basin</span>-swell topography, and consequent sediment deposition, erosion, and structural deformation. A systematic study of the African plate boundaries since the opening of surrounding <span class="hlt">oceanic</span> <span class="hlt">basins</span> is presently lacking. This is mainly because geophysical data are sparse and there are still controversies regarding the ages of <span class="hlt">oceanic</span> crust. The publication of individual geophysical datasets and more recently, global Digital Map of Magnetic Anomalies (WDMAM, EMAG2) prompted us to systematically reconstruct the ages and extent of <span class="hlt">oceanic</span> crust around Africa for the last 200 Ma. Location of Continent <span class="hlt">Ocean</span> Boundary/Continent <span class="hlt">Ocean</span> Transition and older <span class="hlt">oceanic</span> crust (Jurassic and Cretaceous) are updates in the light of gravity, magnetic and seismic data and models of passive margin formation. Reconstructed NeoTethys <span class="hlt">oceanic</span> crust is based on a new model of microcontinent and intr-<span class="hlt">oceanic</span> subduction zone evolution in this area.The new set of <span class="hlt">oceanic</span> palaeo-age grid models constitutes the basis for estimating the dynamics of <span class="hlt">oceanic</span> crust through time and will be used as input for quantifying the paleo-ridge push and slab pull that contributed to the African plate palaeo-stresses and had the potential to influence the formation of sedimentary <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A23F0362C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A23F0362C"><span>Influence of SST from Pacific and Atlantic <span class="hlt">Ocean</span> and atmospheric circulation in the precipitation regime of <span class="hlt">basin</span> from Brazilian SIN</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Custodio, M. D.; Ramos, C. G.; Madeira, P.; de Macedo, A. L.</p> <p>2013-12-01</p> <p>The South American climate presents tropical, subtropical and extratropical features because of its territorial extension, being influenced by a variety of dynamical systems with different spatial and temporal scales which result in different climatic regimes in their subregions. Furthermore, the precipitation regime in South America is influenced by low-frequency phenomena as El Niño-Southern Oscillation (ENSO), the Atlantic dipole and the Madden Julian Oscilation (MJO), in other words, is directly influenced by variations of the Sea Surface Temperature (SST). Due to the importance of the precipitation for many sectors including the planning of productive activities, such as agriculture, livestock and hydropower energy, many studies about climate variations in Brazil have tried to determine and explain the mechanisms that affect the precipitation regime. However, because of complexity of the climate system, and consequently of their impacts on the global precipitation regime, its interactions are not totally understood and therefore misrepresented in numerical models used to forecast climate. The precipitation pattern over hydrographic <span class="hlt">basin</span> which form the Brasilian National Interconnected System (Sistema Interligado Nacional-SIN) are not yet known and therefore the climate forecast of these regions still presents considerable failure that need to be corrected due to its economic importance. In this context, the purpose here is to determine the precipitation patterns on the Brazilian SIN, based on SST and circulation observed data. In a second phase a forecast climate model for these regions will be produced. In this first moment 30 years (1983 to 2012) of SST over Pacific and Atlantic <span class="hlt">Ocean</span> were analyzed, along with wind in 850 and 200 hPa and precipitation observed data. The precipitation patterns were analyzed through statistical analyses for interannual (ENSO) and intraseasonal (MJO) anomalies for these variables over the SIN <span class="hlt">basin</span>. Subsequently, these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...10412909M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...10412909M"><span>Contrasting styles of seafloor spreading in the Woodlark <span class="hlt">Basin</span>: Indications of rift-induced secondary mantle convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>MartíNez, Fernando; Taylor, Brian; Goodliffe, Andrew M.</p> <p>1999-06-01</p> <p>The Woodlark <span class="hlt">Basin</span> in the southwest Pacific is a young <span class="hlt">ocean</span> <span class="hlt">basin</span> which began forming by ˜6 Ma following the rifting of continental and arc lithosphere. The N-S striking Moresby Transform divides the <span class="hlt">oceanic</span> <span class="hlt">basin</span> into eastern and western parts which have contrasting characteristics. Seafloor spreading west of Moresby Transform began after ˜2 Ma, and although spreading rates decrease to the west, the western <span class="hlt">basin</span> has faster spreading characteristics than the eastern <span class="hlt">basin</span>. These include (1) ˜500 m shallower seafloor; (2) Bouguer gravity anomalies that are >30 mGals lower; (3) magnetic anomaly and modeled seafloor magnetization amplitudes that are higher; (4) a spreading center with an axial high in contrast to the axial valleys of the eastern <span class="hlt">basin</span>; (5) smoother seafloor fabric; and (6) exclusively nontransform spreading center offsets in contrast to the eastern <span class="hlt">basin</span>, which has transform faults and fracture zones that extend across most of the <span class="hlt">basin</span>. Overall depth contrasts and Bouguer anomalies can be matched by end-member models of thicker crust (˜2 km) or thinner lithosphere (<1/3) in the western <span class="hlt">basin</span>. Correlated with these contrasts, the surrounding rifted margins abruptly thicken westward of the longitude of Moresby Transform. We examine alternative explanations for these contrasts and propose that rift-induced secondary mantle convection driven by thicker western margin lithosphere is most consistent with the observations. Although rift-induced convection has been cited as a cause for the voluminous excess magmatism at some rifted margins, the observations in the Woodlark <span class="hlt">Basin</span> suggest that this mechanism may significantly affect the morphology, structure, and geophysical characteristics of young <span class="hlt">ocean</span> <span class="hlt">basins</span> in alternate ways which resemble increased spreading rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA348887','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA348887"><span>Variability of the Arctic <span class="hlt">Basin</span> Oceanographic Fields</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1996-02-01</p> <p>the model a very sophisticated turbulence closure scheme. 9. Imitation of the CO2 doubling We parameterized the " greenhouse " effect by changing the...of the Arctic <span class="hlt">Ocean</span>. A more realistic model of the Arctic <span class="hlt">Ocean</span> circulation was obtained, and an estimation of the impact of the greenhouse effect on... greenhouse effect is in freshening of the upper Arctic <span class="hlt">Basin</span>. Although some shortcomings of the model still exist (an unrealistic high coefficient of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5740475-structural-evolution-petroleum-productivity-baltic-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5740475-structural-evolution-petroleum-productivity-baltic-basin"><span>Structural evolution and petroleum productivity of the Baltic <span class="hlt">basin</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>Ulmishek, G.F.</p> <p></p> <p>The Baltic <span class="hlt">basin</span> is an oval depression located in the western part of the Russian craton; it occupies the eastern Baltic Sea and <span class="hlt">adjacent</span> onshore areas. The <span class="hlt">basin</span> contains more than 5,000 m of sedimentary rocks ranging from latest Proterozoic to Tertiary in age. These rocks consist of four tectonostratigraphic sequences deposited during major tectonic episodes of <span class="hlt">basin</span> evolution. Principal unconformities separate the sequences. The <span class="hlt">basin</span> is underlain by a rift probably filled with Upper Proterozoic rocks. Vendian and Lower Cambrian rocks (Baikalian sequence) form two northeast-trending depressions. The principal stage of the <span class="hlt">basin</span> development was during deposition of amore » thick Middle Cambrian-Lower Devonian (Caledonian) sequence. This stage was terminated by the most intense deformations in the <span class="hlt">basin</span> history. The Middle Devonian-Carboniferous (Hercynian) and Permian-Tertiary (Kimmerian-Alpine) tectonic and depositional cycles only slightly modified the <span class="hlt">basin</span> geometry and left intact the main structural framework of underlying rocks. The petroleum productivity of the <span class="hlt">basin</span> is related to the Caledonian tectonostratigraphic sequence that contains both source rocks and reservoirs. However, maturation of source rocks, migration of oil, and formation of fields took place mostly during deposition of the Hercynian sequence.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T44B..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T44B..04W"><span>The role of Mesozoic sedimentary <span class="hlt">basin</span> tapers on the formation of Cenozoic crustal shortening structures and foredeep in the western Sichuan <span class="hlt">Basin</span>, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, M.</p> <p>2017-12-01</p> <p>The foreland <span class="hlt">basin</span> records important clues of tectonic and sedimentary process of mountain-building, thus to explore its dynamic mechanism on the formation is an important issue of the mountain-<span class="hlt">basin</span> interaction. The Longmen Shan fold-and-thrust belt and its <span class="hlt">adjacent</span> Sichuan <span class="hlt">basin</span> located in the eastern margin of Tibetan Plateau, are one of the most-concerned regions of studying modern mountain-building and seismic process, and are also a natural laboratory of studying the dynamics of the formation and development of foreland <span class="hlt">basin</span>. However, it still need further explore on the mechanics of the development of the Cenozoic foreland <span class="hlt">basin</span> and thrust-belts in the western Sichuan <span class="hlt">Basin</span>. The Longmen Shan thrust belt has experienced multi-stages of tectonics evolution, foreland <span class="hlt">basin</span> formation and topography growth since Late Triassic, and whether the early formed <span class="hlt">basin</span> architecture and large Mesozoic sedimentary <span class="hlt">basin</span> taper can influence the formation and development of the Cenozoic foreland <span class="hlt">basin</span> and thrust belts? To solve these issues, this project aim to focus on the Cenozoic foreland <span class="hlt">basin</span> and internal crustal shortening structures in the western Sichuan <span class="hlt">basin</span>, on the basis of growth critical wedge taper theory. We will reconstruct the shape of multi-phases of sedimentary <span class="hlt">basin</span> tapers, the temporal-spatial distribution of crustal shortening and thrusting sequences, and analyze the control mechanism of Mesozoic sedimentary <span class="hlt">basin</span> taper on the formation of Cenozoic foreland <span class="hlt">basins</span>, and final explore the interaction between the tectonics geomorphology, stress field and dynamic propagation of foreland <span class="hlt">basin</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_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('https://www.ncbi.nlm.nih.gov/pubmed/26989263','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26989263"><span>Calls reveal population structure of blue whales across the southeast Indian <span class="hlt">Ocean</span> and the southwest Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Balcazar, Naysa E; Tripovich, Joy S; Klinck, Holger; Nieukirk, Sharon L; Mellinger, David K; Dziak, Robert P; Rogers, Tracey L</p> <p>2015-11-24</p> <p>For effective species management, understanding population structure and distribution is critical. However, quantifying population structure is not always straightforward. Within the Southern Hemisphere, the blue whale ( Balaenoptera musculus ) complex is extremely diverse but difficult to study. Using automated detector methods, we identified "acoustic populations" of whales producing region-specific call types. We examined blue whale call types in passive acoustic data at sites spanning over 7,370 km across the southeast Indian <span class="hlt">Ocean</span> and southwest Pacific <span class="hlt">Ocean</span> (SWPO) from 2009 to 2012. In the absence of genetic resolution, these acoustic populations offer unique information about the blue whale population complex. We found that the Australian continent acts as a geographic boundary, separating Australia and New Zealand blue whale acoustic populations at the junction of the Indian and Pacific <span class="hlt">Ocean</span> <span class="hlt">basins</span>. We located blue whales in previously undocumented locations, including the far SWPO, in the Tasman Sea off the east coast of Australia, and along the Lau <span class="hlt">Basin</span> near Tonga. Our understanding of population dynamics across this broad scale has significant implications to recovery and conservation management for this endangered species, at a regional and global scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP43F..03T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP43F..03T"><span>Centennial-scale links between Atlantic <span class="hlt">Ocean</span> dynamics and hydroclimate over the last 4400 years: Insights from 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>Thirumalai, K.; Quinn, T. M.; Okumura, Y.; Richey, J. N.; Partin, J. W.; Poore, R. Z.</p> <p>2015-12-01</p> <p>Surface circulation in the Atlantic <span class="hlt">Ocean</span> is an important mediator of global climate and yet its variability is poorly constrained on centennial timescales. Changes in the Atlantic meridional overturning circulation (AMOC) have been implicated in late Holocene climate variability in the Western Hemisphere, although the relationship between AMOC variability and hydroclimate is uncertain due to the lack of sufficiently highly resolved proxy records. Here we present a replicated reconstruction of sea-surface temperature (SST) and salinity (SSS) from the Garrison <span class="hlt">Basin</span> in the northern Gulf of Mexico (NGOM) spanning the last 4,400 years to better constrain past sea-surface conditions. We generated time series of paired Mg/Ca (SST proxy) and δ18O (SST and SSS proxy) variations in planktic foraminifer Globigerinoides ruber (white variety) from three multi-cores collected in 2010. Using a Monte Carlo-based technique we produce a stacked record from the three multi-cores and constrain analytical, calibration, chronological, and sampling uncertainties. We apply this technique to existing paired Mg/Ca- δ18O studies in the Gulf of Mexico and Atlantic <span class="hlt">Ocean</span> to facilitate comparison between time-uncertain proxy reconstructions. The Garrison <span class="hlt">Basin</span> stack exhibits large centennial-scale variability (σSST~0.6°C; δ18Osw~0.17‰) and indicates a substantially cool (0.9±0.5°C) and fresh (0.26±0.1‰) Little Ice Age (LIA; 1450-1850 A.D.), corroborating extant records from the Gulf of Mexico. Focusing on the last millennium, we analyze a suite of <span class="hlt">oceanic</span> and terrestrial proxy records to demonstrate a centennial-scale link between salt advection in the Atlantic <span class="hlt">Ocean</span>, a diagnostic parameter of <span class="hlt">ocean</span> circulation, and hydroclimate in the <span class="hlt">adjacent</span> continents. The ensuing multiproxy relationships seem to be consistent with spatial field correlations of limited salinity and rainfall instrumental/reanalysis data, which suggest that NGOM salinity varies with large-scale Atlantic <span class="hlt">Ocean</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2006/1281/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1281/"><span>Water-Level Data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">Adjacent</span> Areas, Central New Mexico, Period of Record Through 2004</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>DeWees, R.K.</p> <p>2006-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25 to 40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompass the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the Albuquerque <span class="hlt">Basin</span> are obtained solely from ground-water resources. An increase of approximately 20 percent in the population from 1991 to present also resulted in an increased demand for water. From April 1982 through September 1983, a network of wells was established to monitor changes in ground-water levels throughout the Albuquerque <span class="hlt">Basin</span>. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly. Currently (2004), the network consists of 234 wells and piezometers. This report presents water-level data collected by U.S. Geological Survey personnel at 155 sites through 2004. Water-level and other data for 71 sites are collected by other agencies. Water-level data for 8 sites of the 155 sites measured by the U.S. Geological Survey were not available for this report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wsp/1652a/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/1652a/report.pdf"><span>Floods of January-February 1957 in southeastern Kentucky and <span class="hlt">adjacent</span> areas</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>1964-01-01</p> <p>Heavy rains over an extensive area on January 27-February 2, caused extreme flooding in southeastern Kentucky and <span class="hlt">adjacent</span> areas in West Virginia, Virginia, and Tennessee. Total rainfall for the storm period ranged from 6-9 inches over most of the report area and was 12? inches at the eastern end of the Virginia-Kentucky State line. The principal <span class="hlt">basins</span> affected by the storm were those of the Big Sandy, Kentucky, Cumberland, and Tennessee Rivers. Maximum discharge of record occurred in many streams. On Levisa Fork near Grundy, Va., the peak discharge of 33,200 cfs was 50 percent greater than the previous maximum in 17 years of record and was 3.3 times the mean annual flood. The peak discharges on-tributaries of the Kentucky River and on ,the Holston and Clinch Rivers were also the greatest of record and .those on the upper Cumberland River were nearly as great as .those during the historic floods of 1918 and 1946. Total flood damage was estimated at $61 million of which $39 million was in the Big Sandy River <span class="hlt">basin</span> (mostly in Kentucky) and $15 million was in the Kentucky River <span class="hlt">basin</span>--$52 million of the total damage was in Kentucky.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EOSTr..95...53A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EOSTr..95...53A"><span><span class="hlt">Basin</span>-Wide Oceanographic Array Bridges the South Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ansorge, I. J.; Baringer, M. O.; Campos, E. J. D.; Dong, S.; Fine, R. A.; Garzoli, S. L.; Goni, G.; Meinen, C. S.; Perez, R. C.; Piola, A. R.; Roberts, M. J.; Speich, S.; Sprintall, J.; Terre, T.; Van den Berg, M. A.</p> <p>2014-02-01</p> <p>The meridional overturning circulation (MOC) is a global system of surface, intermediate, and deep <span class="hlt">ocean</span> currents. The MOC connects the surface layer of the <span class="hlt">ocean</span> and the atmosphere with the huge reservoir of the deep sea and is the primary mechanism for transporting heat, freshwater, and carbon between <span class="hlt">ocean</span> <span class="hlt">basins</span>. Climate models show that past changes in the strength of the MOC were linked to historical climate variations. Further research suggests that the MOC will continue to modulate climate change scenarios on time scales ranging from decades to centuries [Latif et al., 2006].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70013452','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70013452"><span>Amino acid epimerization implies rapid sedimentation rates in Arctic <span class="hlt">Ocean</span> 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>Sejrup, H.P.; Miller, G.H.; Brigham-Grette, J.; Lovlie, R.; Hopkins, D.</p> <p>1984-01-01</p> <p>The palaeooceanography of the Arctic <span class="hlt">Ocean</span> is less well known than any other <span class="hlt">ocean</span> <span class="hlt">basin</span>, due to difficulties in obtaining cores and in providing a secure chronological framework for those cores that have been raised. Most recent investigators have suggested that low sedimentation rates (0.05-0.1 cm kyr-1) have characterized the deep <span class="hlt">basins</span> over the past 5 Myr (refs 1,2) despite the glacial-marine character of the sediment and proximity to major centres of shelf glaciation. These calculations have been primarily based on the down-core pattern in the inclination of magnetic minerals, supported by uranium-series, 14C and micropalaeontological evidence. Here we analyse amino acid diagnesis in foraminifera from two gravity cores raised from the floor of the Arctic <span class="hlt">Ocean</span>, our results suggest that these cores span <200 kyr., conflicting with the earlier estimate of 3 Myr based on palaeomagnetic data. The chronology of other Arctic <span class="hlt">Ocean</span> cores and previous palaeoenvironmental interpretations need re-evaluation. ?? 1984 Nature Publishing Group.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7201819-late-paleozoic-paleolatitude-paleogeography-midland-basin-texas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7201819-late-paleozoic-paleolatitude-paleogeography-midland-basin-texas"><span>Late Paleozoic paleolatitude and paleogeography of the Midland <span class="hlt">basin</span>, Texas</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>Walker, D.A.; Golonka, J.; Reid, A.M.</p> <p>1992-04-01</p> <p>During the Late Pennsylvanian through Early Permian, the Midland <span class="hlt">basin</span> was located in the low latitudes. In the Desmoinesian (Strawn), the <span class="hlt">basin</span> was astride the equator; during the Missourian (Canyon), the center of the <span class="hlt">basin</span> had migrated northward so it was located at 1-2N latitude. In the Virgilian (Cisco), the <span class="hlt">basin</span> center was located around 2-4N latitude, and by the Wolfcampian, it was positioned at around 4-6N latitude. From the Desmoinesian (312 Ma) through the Missourian (306 Ma), the relative motion of the <span class="hlt">basin</span> was 63NE. Later during the Virgilian (298 Ma) to Wolfcampian (280 Ma), the direction of motionmore » was 24NE. This change in motion reflects a major tectonic event, occurring between the Missourian and Virgilian, that greatly modifed the movement of the Laurentian (North American) plate. At that time, Laurentia had collided with Gondwana and become part of the supercontinent Pangea. Throughout the late Paleozoic, Laurentia was rotated so the Midland <span class="hlt">basin</span> was oriented 43{degree} northeast from its current setting. Late Paleozoic paleogeography and paleolatitude controlled the direction of prevailing winds and <span class="hlt">ocean</span> currents, thereby influencing the distribution of carbonate facies in the Midland <span class="hlt">basin</span>. Present prevailing winds and <span class="hlt">ocean</span> currents have been shown to have a major impact on modern carbonate sedimentation and facies distribution in Belize, the Bahamas and Turks, and Caicos. A clearer understanding of how late Paleozoic latitude and geography affected sedimentation helps explain and predict the distribution of carbonates throughout the Midland <span class="hlt">basin</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H43D1671W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H43D1671W"><span>Climate controls on streamflow variability in the Missouri River <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wise, E.; Woodhouse, C. A.; McCabe, G. J., Jr.; Pederson, G. T.; St-Jacques, J. M.</p> <p>2017-12-01</p> <p>The Missouri River's hydroclimatic variability presents a challenge for water managers, who must balance many competing demands on the system. Water resources in the Missouri River <span class="hlt">Basin</span> (MRB) have increasingly been challenged by the droughts and floods that have occurred over the past several decades and the potential future exacerbation of these extremes by climate change. Here, we use observed and modeled hydroclimatic data and estimated natural flow records to describe the climatic controls on streamflow in the upper and lower portions of the MRB, examine atmospheric and <span class="hlt">oceanic</span> patterns associated with high- and low-flow years, and investigate trends in climate and streamflow over the instrumental period. Results indicate that the two main source regions for total outflow, in the uppermost and lowermost parts of the <span class="hlt">basin</span>, are under the influence of very different sets of climatic controls. Winter precipitation, impacted by changes in zonal versus meridional flow from the Pacific <span class="hlt">Ocean</span>, as well as spring precipitation and temperature, play a key role in surface water supply variability in the upper <span class="hlt">basin</span>. Lower <span class="hlt">basin</span> flow is significantly correlated with precipitation in late spring and early summer, indicative of Atlantic-influenced circulation variability affecting the flow of moisture from the Gulf of Mexico. The upper <span class="hlt">basin</span>, with decreasing snowpack and streamflow and warming spring temperatures, will be less likely to provide important flow supplements to the lower <span class="hlt">basin</span> in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994DSRI...41.1091F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994DSRI...41.1091F"><span>Measurements within the Pacific-Indian <span class="hlt">oceans</span> throughflow region</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fieux, M.; Andrié, C.; Delecluse, P.; Ilahude, A. G.; Kartavtseff, A.; Mantisi, F.; Molcard, R.; Swallow, J. C.</p> <p>1994-07-01</p> <p>Two hydrographic (θ, S, O 2) and trichlorofluoromethane (F-11) sections were carried out between the Australian continental shelf and Indonesia, in August 1989, on board the R.V. Marion Dufresne. The sections lie in the easternmost part of the Indian <span class="hlt">Ocean</span> where the throughflow between the Pacific <span class="hlt">Ocean</span> and the Indian <span class="hlt">Ocean</span> emerges. They allow us to describe the features of the water-property and circulation fields of the throughflow at its entrance in the Indian <span class="hlt">Ocean</span>. Between the Australian continental shelf and Bali, the Subtropical and Central waters are separated from the waters of the Indonesian seas by a sharp hydrological front, located around 13°30 S, below the thermocline down to 700 m. Near the coast of Bali, upwelling occurs in the near-surface layer under the effect of the southeast monsoon; at depth, between 300 m to more than 800 m, a water mass of northern Indian <span class="hlt">Ocean</span> origin was present. From the characteristics of the bottom water found in the Lombok <span class="hlt">basin</span>, the maximum depth of the Java ridge which separates the Lombok <span class="hlt">basin</span> from the Northwest Australian <span class="hlt">basin</span> lies around 3650 m. Off Sumba, Savu, Roti and Timor channels a core of low salinity and high oxygen content near-surface water was found in the axis of each channel, which suggests strong currents from the interior Indonesian seas towards the Indian <span class="hlt">Ocean</span>. The entrance of the deep water flowing in the opposite direction, from the Indian <span class="hlt">Ocean</span> to the Timor <span class="hlt">basin</span>, was marked below 1400 m to the sill depth, through an increase of salinity and oxygen content. The flow reversal, observed briefly by a Pegasus direct current profiler in the Timor strait, was located at 1200 m depth. During the southeast monsoon, the net (geostrophic + Ekman) transport calculated on the section Australia-Bali give an estimate of the throughflow between 0 and 500 m of 22 ± 4 × 10 6 m 3 s -1 towards the Indian <span class="hlt">Ocean</span>, with a concentration of the transport in the upper layers (19 × 10 6 m 3 s -1 in 0-200 m) and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860017310','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860017310"><span>Objective analysis of tidal fields in the Atlantic and Indian <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sanchez, B. V.; Rao, D. B.; Steenrod, S. D.</p> <p>1986-01-01</p> <p>An objective analysis technique has been developed to extrapolate tidal amplitudes and phases over entire <span class="hlt">ocean</span> <span class="hlt">basins</span> using existing gauge data and the altimetric measurements which are now beginning to be provided by satellite oceanography. The technique was previously tested in the Lake Superior <span class="hlt">basin</span>. The method has now been developed and applied in the Atlantic-Indian <span class="hlt">ocean</span> <span class="hlt">basins</span> using a 6 deg x 6 deg grid to test its essential features. The functions used in the interpolation are the eigenfunctions of the velocity potential (Proudman functions) which are computed numerically from a knowledge of the <span class="hlt">basin</span>'s bottom topography, the horizontal plan form and the necessary boundary conditions. These functions are characteristic of the particular <span class="hlt">basin</span>. The gravitational normal modes of the <span class="hlt">basin</span> are computed as part of the investigation, they are used to obtain the theoretical forced solutions for the tidal constituents, the latter provide the simulated data for the testing of the method and serve as a guide in choosing the most energetic modes for the objective analysis. The results of the objective analysis of the M2 and K1 tidal constituents indicate the possibility of recovering the tidal signal with a degree of accuracy well within the error bounds of present day satellite techniques.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFMOS11B1188V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFMOS11B1188V"><span>Statistical mechanics explanation for the structure of <span class="hlt">ocean</span> eddies and currents</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Venaille, A.; Bouchet, F.</p> <p>2010-12-01</p> <p>The equilibrium statistical mechanics of two dimensional and geostrophic flows predicts the outcome for the large scales of the flow, resulting from the turbulent mixing. This theory has been successfully applied to describe detailed properties of Jupiter's Great Red Spot. We discuss the range of applicability of this theory to <span class="hlt">ocean</span> dynamics. It is able to reproduce mesoscale structures like <span class="hlt">ocean</span> rings. It explains, from statistical mechanics, the westward drift of rings at the speed of non dispersive baroclinic waves, and the recently observed (Chelton and col.) slower northward drift of cyclonic eddies and southward drift of anticyclonic eddies. We also uncover relations between strong eastward mid-<span class="hlt">basin</span> inertial jets, like the Kuroshio extension and the Gulf Stream, and statistical equilibria. We explain under which conditions such strong mid-<span class="hlt">basin</span> jets can be understood as statistical equilibria. We claim that these results are complementary to the classical Sverdrup-Munk theory: they explain the inertial part <span class="hlt">basin</span> dynamics, the jets structure and location, using very simple theoretical arguments. References: A. VENAILLE and F. BOUCHET, <span class="hlt">Ocean</span> rings and jets as statistical equilibrium states, submitted to JPO F. BOUCHET and A. VENAILLE, Statistical mechanics of two-dimensional and geophysical flows, arxiv ...., submitted to Physics Reports P. BERLOFF, A. M. HOGG, W. DEWAR, The Turbulent Oscillator: A Mechanism of Low- Frequency Variability of the Wind-Driven <span class="hlt">Ocean</span> Gyres, Journal of Physical Oceanography 37 (2007) 2363-+. D. B. CHELTON, M. G. SCHLAX, R. M. SAMELSON, R. A. de SZOEKE, Global observations of large <span class="hlt">oceanic</span> eddies, Geo. Res. Lett.34 (2007) 15606-+ b) and c) are snapshots of streamfunction and potential vorticity (red: positive values; blue: negative values) in the upper layer of a three layer quasi-geostrophic model of a mid-latitude <span class="hlt">ocean</span> <span class="hlt">basin</span> (from Berloff and co.). a) Streamfunction predicted by statistical mechanics. Even in an out</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/wri80-10/pdf/wrir80-10.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/wri80-10/pdf/wrir80-10.pdf"><span>Investigation of acidity and other water-quality characteristics of Upper Oyster Creek, <span class="hlt">Ocean</span> County, New Jersey</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Fusillo, Thomas V.; Schornick, J.C.; Koester, H.E.; Harriman, D.A.</p> <p>1980-01-01</p> <p>Water-quality data collected in the upper Oyster Creek drainage <span class="hlt">basin</span>, <span class="hlt">Ocean</span> County, N.J., indicate that the stream has excellent water quality except for a persistently low pH. The mean concentrations of the major inorganic ions were all less than 6.0 milligrams per liter. Mean concentrations of total nitrogen and total phosphorus were 0.15 mg/L and 0.01 mg/L, respectively. Dissolved oxygen averaged 8.7 mg/L and 81% saturation. Low pH levels are typical of streams draining cedar swamps. In Oyster Creek, the pH tended to decrease downstream due to chemical and biological processes. The pH levels in swamps were one-half unit or more lower than the pH levels in the <span class="hlt">adjacent</span> stream. Sharp declines in stream pH were noted during runoff periods as the result of the mixing of poorly-buffered stream water with more highly acidic water from surrounding swamp areas. The quality of ground water within the study area was similar to the quality of streamflow, except for higher iron and ammonia-nitrogen concentrations and a higher pH range of 4.9 to 6.5. Precipitation represented a major source of many chemical constituents in the ground- and surface-waters of the Oyster Creek <span class="hlt">basin</span>. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013OcDyn..63.1203D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013OcDyn..63.1203D"><span>SMOS reveals the signature of Indian <span class="hlt">Ocean</span> Dipole events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durand, Fabien; Alory, Gaël; Dussin, Raphaël; Reul, Nicolas</p> <p>2013-12-01</p> <p>The tropical Indian <span class="hlt">Ocean</span> experiences an interannual mode of climatic variability, known as the Indian <span class="hlt">Ocean</span> Dipole (IOD). The signature of this variability in <span class="hlt">ocean</span> salinity is hypothesized based on modeling and assimilation studies, on account of scanty observations. Soil Moisture and <span class="hlt">Ocean</span> Salinity (SMOS) satellite has been designed to take up the challenge of sea surface salinity remote sensing. We show that SMOS data can be used to infer the pattern of salinity variability linked with the IOD events. The core of maximum variability is located in the central tropical <span class="hlt">basin</span>, south of the equator. This region is anomalously salty during the 2010 negative IOD event, and anomalously fresh during the 2011 positive IOD event. The peak-to-peak anomaly exceeds one salinity unit, between late 2010 and late 2011. In conjunction with other observational datasets, SMOS data allow us to draw the salt budget of the area. It turns out that the horizontal advection is the main driver of salinity anomalies. This finding is confirmed by the analysis of the outputs of a numerical model. This study shows that the advent of SMOS makes it feasible the quantitative assessment of the mechanisms of <span class="hlt">ocean</span> surface salinity variability in the tropical <span class="hlt">basins</span>, at interannual timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/52487','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/52487"><span>Physical, chemical, and biological properties of soil under soybean cultivation and at an <span class="hlt">adjacent</span> rainforest in Amazonia</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>T.P. Beldini; R.C. Oliveira Junior; Michael Keller; P.B. de Camargo; P.M. Crill; A. Damasceno da Silva; D. Bentes dos Santos; D. Rocha de Oliveira</p> <p>2015-01-01</p> <p>Land-use change in the Amazon <span class="hlt">basin</span> has occurred at an accelerated pace during the last decade, and it is important that the effects induced by these changes on soil properties are better understood. This study investigated the chemical, physical, and biological properties of soil in a field under cultivation of soy and rice, and at an <span class="hlt">adjacent</span> primary rain forest....</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51L..06W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51L..06W"><span>The <span class="hlt">Oceanic</span> Contribution to Atlantic Multi-Decadal Variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wills, R. C.; Armour, K.; Battisti, D. S.; Hartmann, D. L.</p> <p>2017-12-01</p> <p>Atlantic multi-decadal variability (AMV) is typically associated with variability in <span class="hlt">ocean</span> heat transport (OHT) by the Atlantic Meridional Overturning Circulation (AMOC). However, recent work has cast doubt on this connection by showing that slab-<span class="hlt">ocean</span> climate models, in which OHT cannot vary, exhibit similar variability. Here, we apply low-frequency component analysis to isolate the variability of Atlantic sea-surface temperatures (SSTs) that occurs on decadal and longer time scales. In observations and in pre-industrial control simulations of comprehensive climate models, we find that AMV is confined to the extratropics, with the strongest temperature anomalies in the North Atlantic subpolar gyre. We show that warm subpolar temperatures are associated with a strengthened AMOC, increased poleward OHT, and local heat fluxes from the <span class="hlt">ocean</span> into the atmosphere. In contrast, the traditional index of AMV based on the <span class="hlt">basin</span>-averaged SST anomaly shows warm temperatures preceded by heat fluxes from the atmosphere into the <span class="hlt">ocean</span>, consistent with the atmosphere driving this variability, and shows a weak relationship with AMOC. The autocorrelation time of the <span class="hlt">basin</span>-averaged SST index is 1 year compared to an autocorrelation time of 5 years for the variability of subpolar temperatures. This shows that multi-decadal variability of Atlantic SSTs is sustained by OHT variability associated with AMOC, while atmosphere-driven SST variability, such as exists in slab-<span class="hlt">ocean</span> models, contributes primarily on interannual time scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007Ocgy...47..705V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007Ocgy...47..705V"><span>Plate tectonics of the northern part of the Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Verzhbitsky, E. V.; Kononov, M. V.; Kotelkin, V. D.</p> <p>2007-10-01</p> <p>Geophysical data on the northern part of the Pacific <span class="hlt">Ocean</span> were systematized to compile a map of geomagnetic and geothermal studies of the Bering Sea. The absence of reliable data about the formation time of the Bering Sea structures of <span class="hlt">oceanic</span> and continental origins is noted; this hampered the assessment of the geodynamical processes in the North Pacific. Based on the geophysical data, we estimated the age of the structures of the Bering Sea floor such as the Commander <span class="hlt">Basin</span> (21 My), the Shirshov Ridge (95 and 33 My in the northern and southern parts, respectively), the Aleutian <span class="hlt">Basin</span> (70 My), the Vitus Arch (44 My), the Bowers Ridge (30 My), and the Bowers <span class="hlt">Basin</span> (40 My). These values are confirmed by the geological, geophysical, and kinematic data. A numerical modeling of the formation of extensive regional structures (Emperor Fracture Zone, Chinook Trough, and others) in the Northern Pacific is carried out. A conclusion was made on the basis of the geological and geothermal analysis that the northern and southern parts of the Shirshov Ridge have different geological ages and different tectonic structures. The northern part of the ridge is characterized by an upthrust-nappe terrain origin, while the southern part has originated from a torn-away island arc similar to the origin of the Bowers Ridge. The sea floor of the Aleutian <span class="hlt">Basin</span> represents a detached part of the Upper Cretaceous Kula plate, on which spreading processes took place in the Vitus Arch area in the Eocene. The final activity phase in the Bering Sea began 21 My B.P. by spreading of the ancient <span class="hlt">oceanic</span> floor of the Commander <span class="hlt">Basin</span>. Based on the age estimations of the structures of the Bering Sea floor, the results of the modeling of the process of formation of regional fracture zones and of the geomagnetic, geothermal, tectonic, geological, and structural data, we calculated and compiled a kinematic model (with respect to a hot spot reference system) of the northern part of the Pacific <span class="hlt">Ocean</span> for 21</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PalOc..31..732G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PalOc..31..732G"><span>Onset and demise of Cretaceous <span class="hlt">oceanic</span> anoxic events: The coupling of surface and bottom <span class="hlt">oceanic</span> processes in two pelagic <span class="hlt">basins</span> of the western Tethys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gambacorta, G.; Bersezio, R.; Weissert, H.; Erba, E.</p> <p>2016-06-01</p> <p>The upper Albian-lower Turonian pelagic successions of the Tethys record processes acting during the onset, core, and recovery from perturbed conditions across <span class="hlt">oceanic</span> anoxic event (OAE) 1d, OAE 2, and the mid-Cenomanian event I (MCE I) relative to intervening intervals. Five sections from Umbria-Marche and Belluno <span class="hlt">Basins</span> (Italy) were analyzed at high resolution to assess processes in surface and deep waters. Recurrent facies stacking patterns (SP) and their associations record periods of bottom current activity coupled with surface changes in trophic level. Climate changes appear to have been influential on deep circulation dynamics. Under greenhouse conditions, vigorous bottom currents were arguably induced by warm and dense saline deep waters originated on tropical shelves in the Tethys and/or proto-Atlantic <span class="hlt">Ocean</span>. Tractive facies postdating intermittent anoxia during OAE 1d and in the interval bracketed by MCE I and OAE 2 are indicative of feeble bottom currents, though capable of disrupting stratification and replenish deep water with oxygen. The major warming at the onset of OAE 2 might have enhanced the formation of warm salty waters, possibly producing local hiatuses at the base of the Bonarelli Level and winnowing at the seafloor. Hiatuses detected at the top of the Bonarelli Level possibly resulted from most effective bottom currents during the early Turonian thermal maximum. Times of minimal sediment displacement correlate with cooler climatic conditions and testify a different mechanism of deep water formation, as further suggested by a color change to reddish lithologies of the post-OAE 1d and post-OAE 2 intervals.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5617801-basin-formation-neogene-sedimentation-backarc-setting-halmahera-eastern-indonesia','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5617801-basin-formation-neogene-sedimentation-backarc-setting-halmahera-eastern-indonesia"><span><span class="hlt">Basin</span> formation and Neogene sedimentation in a backarc setting, Halmahera, eastern Indonesia</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>Hall, R.; Nichols, G.J.</p> <p>1991-03-01</p> <p>It has been proposed that <span class="hlt">basins</span> in backarc setting form in association with subduction by thinning of continental crust, backarc spreading in <span class="hlt">oceanic</span> crust, compression, or trapping of pieces of <span class="hlt">oceanic</span> plate behind an arc. The Halmahera <span class="hlt">basin</span> in eastern Indonesia developed in a backarc setting but does not fall into these categories; it formed by subsidence of thickened crust made up of imbricated Mesozoic-Paleogene arc and ophiolite rocks. Halmahera lies at the western edge of the Philippine Sea Plate in a complex zone of convergence between the Eurasian margin, the <span class="hlt">oceanic</span> plates of the West Pacific, and the Australian/Indianmore » Plate to the south. The basement is an imbricated complex of Mesozoic to Paleogene ophiolite, arc, and arc-related rocks. During the Miocene this basement complex formed an area of thickened crust upon which carbonate reef and reef-associated sediments were deposited. The authors interpret this shallow marine region to be similar to many of the <span class="hlt">oceanic</span> plateaus and ridges found within the Philippine Sea Plate today. In the Late Miocene, convergence between the Philippine Sea Plate and the Eurasian margin resulted in the formation of the Halmahera Trench to the west of this region of thickened crust. Subduction of the Molucca Sea Plate caused the development of a volcanic island arc. Subsidence in the backarc area produced a broad sedimentary <span class="hlt">basin</span> filled by clastics eroded from the arc and from uplifted basement and cover rocks. The <span class="hlt">basin</span> was asymmetric with the thickest sedimentary fill on the western side, against the volcanic arc. The Halmahera <span class="hlt">basin</span> was modified in the Plio-Pleistocene by east-west compression as the Molucca Sea Plate was eliminated by subduction.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/3245','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/3245"><span>Macroecology, paleoecology, and ecological integrity of terrestrial species and communities of the interior Columbia <span class="hlt">basin</span> and northern portions of the Klamath and Great <span class="hlt">Basins</span>.</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Bruce G. Marcot; L.K. Croft; J.F. Lehmkuhl; R.H. Naney; C.G. Niwa; W.R. Owen; R.E. Sandquist</p> <p>1998-01-01</p> <p>This report present information on biogeography and broad-scale ecology (macroecology) of selected fungi, lichens, bryophytes, vascular plants, invertebrates, and vertebrates of the interior Columbia River <span class="hlt">basin</span> and <span class="hlt">adjacent</span> areas. Rareplants include many endemics associated with local conditions. Potential plant and invertebrate bioindicators are identified. Species...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012610','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012610"><span>Circum-arctic plate accretion - Isolating part of a pacific plate to form the nucleus of the Arctic <span class="hlt">Basin</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>Churkin, M.; Trexler, J.H.</p> <p>1980-01-01</p> <p>A mosaic of large lithospheric plates rims the Arctic <span class="hlt">Ocean</span> <span class="hlt">Basin</span>, and foldbelts between these plates contain numerous allochthonous microplates. A new model for continental drift and microplate accretion proposes that prior to the late Mesozoic the Kula plate extended from the Pacific into the Arctic. By a process of circumpolar drift and microplate accretion, fragments of the Pacific <span class="hlt">basin</span>, including parts of the Kula plate, were cut off and isolated in the Arctic <span class="hlt">Ocean</span>, the Yukon-Koyukuk <span class="hlt">basin</span> in Alaska, and the Bering Sea. ?? 1980.</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('https://www.osti.gov/biblio/6750226-some-cenozoic-hydrocarbon-basins-continental-shelf-vietnam','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6750226-some-cenozoic-hydrocarbon-basins-continental-shelf-vietnam"><span>Some Cenozoic hydrocarbon <span class="hlt">basins</span> on the continental shelf of Vietnam</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>Dien, P.T.</p> <p>1994-07-01</p> <p>The formation of the East Vietnam Sea <span class="hlt">basins</span> was related to different geodynamic processes. The pre-Oligocene basement consists of igneous, metamorphic, and metasediment complexes. The Cretaceous-Eocene basement formations are formed by convergence of continents after destruction of the Tethys <span class="hlt">Ocean</span>. Many Jurassic-Eocene fractured magmatic highs of the Cuulong <span class="hlt">basin</span> basement constitute important reservoirs that are producing good crude oil. The Paleocene-Eocene formations are characterized by intramountain metamolasses, sometimes interbedded volcanic rocks. Interior structures of the Tertiary <span class="hlt">basins</span> connect with rifted branches of the widened East Vietnam Sea. Bacbo (Song Hong) <span class="hlt">basin</span> is predominated by alluvial-rhythmic clastics in high-constructive deltas, whichmore » developed on the rifting and sagging structures of the continental branch. Petroleum plays are constituted from Type III source rocks, clastic reservoirs, and local caprocks. Cuulong <span class="hlt">basin</span> represents sagging structures and is predominated by fine clastics, with tidal-lagoonal fine sandstone and shalestone in high-destructive deltas that are rich in Type II source rocks. The association of the pre-Cenozoic fractured basement reservoirs and the Oligocene-Miocene clastic reservoir sequences with the Oligocene source rocks and the good caprocks is frequently met in petroleum plays of this <span class="hlt">basin</span>. Nan Conson <span class="hlt">basin</span> was formed from complicated structures that are related to spreading of the <span class="hlt">oceanic</span> branch. This <span class="hlt">basin</span> is characterized by Oligocene epicontinental fine clastics and Miocene marine carbonates that are rich in Types I, II, and III organic matter. There are both pre-Cenozoic fractured basement reservoirs, Miocene buildup carbonate reservoir rocks and Oligocene-Miocene clastic reservoir sequences, in this <span class="hlt">basin</span>. Pliocene-Quaternary sediments are sand and mud carbonates in the shelf facies of the East Vietnam Sea back-arc <span class="hlt">basin</span>. Their great thickness provides good conditions for maturation and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5537159-tectonic-evolution-black-sea-orogene-belt-history-opening-black-sea-basin','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5537159-tectonic-evolution-black-sea-orogene-belt-history-opening-black-sea-basin"><span>Tectonic evolution of the Black Sea orogene belt and the history of opening of the Black Sea <span class="hlt">basin</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>Uesuemezsoy, S.</p> <p>1988-08-01</p> <p>The Black Sea <span class="hlt">basin</span> is surrounded by successive orogenic belts of Hercynian, Cimmerian, and Alpine ages. The Rhodope, Thracian, western Pontian, and Transcaucasian (RTPT) blocks of Precambrian age were involved by the circum-Black Sea orogene belts. The Hercynian orogene was documented in the Balkanide, Great Caucasian, Kriastide, southern Pontian, and Transcaucasian belts. The Cimmerian orogene extended north and south of the Black Sea. The southern Cimmerian orogene was represented by the circum-Rhodope and East Thracian-Strandja-Kuere belts. The northern Cimmerian orogene belt extended along the Dobruca-Crimean and southern slope belts. Following the demise of the Black Sea Cimmerian <span class="hlt">basin</span>, the northernmostmore » <span class="hlt">oceanic</span> branch extending from Nish-Trajan through the present Black Sea to the intra-Transcaucasian <span class="hlt">basin</span>, was opened within the Hercynian and Cimmerian consolidated terrain in the Late Jurassic. The other <span class="hlt">oceanic</span> branch, extending from Izmir-Ankara through circum Kirsehir to various <span class="hlt">basins</span>, was opened within the Paleotethyan collision belt, considered to be eastern extension of the Pindus <span class="hlt">basin</span>. The Nish-Trajan sector of the northernmost <span class="hlt">basin</span> was closed in the middle Cretaceous, and the Moesian platform re-fused to the Getic-Serbo-Macedonian-Rhodope belt. The easternmost extension of the intra-Transcaucasian <span class="hlt">basin</span> disappeared in the Late Cretaceous. Consequently, the northernmost <span class="hlt">oceanic</span> branch was reduced to the present Black Sea <span class="hlt">basin</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70029983','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70029983"><span>Thermal structure of <span class="hlt">oceanic</span> transform 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>Behn, M.D.; Boettcher, M.S.; Hirth, G.</p> <p>2007-01-01</p> <p>We use three-dimensional finite element simulations to investigate the temperature structure beneath <span class="hlt">oceanic</span> transform faults. We show that using a rheology that incorporates brittle weakening of the lithosphere generates a region of enhanced mantle upwelling and elevated temperatures along the transform; the warmest temperatures and thinnest lithosphere are predicted to be near the center of the transform. Previous studies predicted that the mantle beneath <span class="hlt">oceanic</span> transform faults is anomalously cold relative to <span class="hlt">adjacent</span> intraplate regions, with the thickest lithosphere located at the center of the transform. These earlier studies used simplified rheologic laws to simulate the behavior of the lithosphere and underlying asthenosphere. We show that the warmer thermal structure predicted by our calculations is directly attributed to the inclusion of a more realistic brittle rheology. This temperature structure is consistent with a wide range of observations from ridge-transform environments, including the depth of seismicity, geochemical anomalies along <span class="hlt">adjacent</span> ridge segments, and the tendency for long transforms to break into small intratransform spreading centers during changes in plate motion. ?? 2007 Geological Society of America.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JGRC..118.4699D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGRC..118.4699D"><span>Hydrographic changes in the Lincoln Sea in the Arctic <span class="hlt">Ocean</span> with focus on an upper <span class="hlt">ocean</span> freshwater anomaly between 2007 and 2010</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de Steur, L.; Steele, M.; Hansen, E.; Morison, J.; Polyakov, I.; Olsen, S. M.; Melling, H.; McLaughlin, F. A.; Kwok, R.; Smethie, W. M.; Schlosser, P.</p> <p>2013-09-01</p> <p>Hydrographic data from the Arctic <span class="hlt">Ocean</span> show that freshwater content in the Lincoln Sea, north of Greenland, increased significantly from 2007 to 2010, slightly lagging changes in the eastern and central Arctic. The anomaly was primarily caused by a decrease in the upper <span class="hlt">ocean</span> salinity. In 2011 upper <span class="hlt">ocean</span> salinities in the Lincoln Sea returned to values similar to those prior to 2007. Throughout 2008-2010, the freshest surface waters in the western Lincoln Sea show water mass properties similar to fresh Canada <span class="hlt">Basin</span> waters north of the Canadian Arctic Archipelago. In the northeastern Lincoln Sea fresh surface waters showed a strong link with those observed in the Makarov <span class="hlt">Basin</span> near the North Pole. The freshening in the Lincoln Sea was associated with a return of a subsurface Pacific Water temperature signal although this was not as strong as observed in the early 1990s. Comparison of repeat stations from the 2000s with the data from the 1990s at 65°W showed an increase of the Atlantic temperature maximum which was associated with the arrival of warmer Atlantic water from the Eurasian <span class="hlt">Basin</span>. Satellite-derived dynamic <span class="hlt">ocean</span> topography of winter 2009 showed a ridge extending parallel to the Canadian Archipelago shelf as far as the Lincoln Sea, causing a strong flow toward Nares Strait and likely Fram Strait. The total volume of anomalous freshwater observed in the Lincoln Sea and exported by 2011 was close to 1100±250km3, approximately 13% of the total estimated FW increase in the Arctic in 2008.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.8706A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.8706A"><span>Colorado <span class="hlt">Basin</span> Structure and Rifting, Argentine passive margin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Autin, Julia; Scheck-Wenderoth, Magdalena; Loegering, Markus; Anka, Zahie; Vallejo, Eduardo; Rodriguez, Jorge; Marchal, Denis; Reichert, Christian; di Primio, Rolando</p> <p>2010-05-01</p> <p>The Argentine margin presents a strong segmentation with considerable strike-slip movements along the fracture zones. We focus on the volcanic segment (between the Salado and Colorado transfer zones), which is characterized by seaward dipping reflectors (SDR) all along the <span class="hlt">ocean</span>-continent transition [e.g. Franke et al., 2006; Gladczenko et al., 1997; Hinz et al., 1999]. The segment is structured by E-W trending <span class="hlt">basins</span>, which differs from the South African margin <span class="hlt">basins</span> and cannot be explained by classical models of rifting. Thus the study of the relationship between the <span class="hlt">basins</span> and the Argentine margin itself will allow the understanding of their contemporary development. Moreover the comparison of the conjugate margins suggests a particular evolution of rifting and break-up. We firstly focus on the Colorado <span class="hlt">Basin</span>, which is thought to be the conjugate of the well studied Orange <span class="hlt">Basin</span> [Hirsch et al., 2009] at the South African margin [e.g. Franke et al., 2006]. This work presents results of a combined approach using seismic interpretation and structural, isostatic and thermal modelling highlighting the structure of the crust. The seismic interpretation shows two rift-related discordances: one intra syn-rift and the break-up unconformity. The overlying sediments of the sag phase are less deformed (no sedimentary wedges) and accumulated before the generation of <span class="hlt">oceanic</span> crust. The axis of the Colorado <span class="hlt">Basin</span> trends E-W in the western part, where the deepest pre-rift series are preserved. In contrast, the <span class="hlt">basin</span> axis turns to a NW-SE direction in its eastern part, where mainly post-rift sediments accumulated. The most distal part reaches the margin slope and opens into the <span class="hlt">oceanic</span> <span class="hlt">basin</span>. The general <span class="hlt">basin</span> direction is almost orthogonal to the present-day margin trend. The most frequent hypothesis explaining this geometry is that the Colorado <span class="hlt">Basin</span> is an aborted rift resulting from a previous RRR triple junction [e.g. Franke et al., 2002]. The structural interpretation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26156374','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26156374"><span><span class="hlt">Basin</span>-scale transport of hydrothermal dissolved metals across the South Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Resing, Joseph A; Sedwick, Peter N; German, Christopher R; Jenkins, William J; Moffett, James W; Sohst, Bettina M; Tagliabue, Alessandro</p> <p>2015-07-09</p> <p>Hydrothermal venting along mid-<span class="hlt">ocean</span> ridges exerts an important control on the chemical composition of sea water by serving as a major source or sink for a number of trace elements in the <span class="hlt">ocean</span>. Of these, iron has received considerable attention because of its role as an essential and often limiting nutrient for primary production in regions of the <span class="hlt">ocean</span> that are of critical importance for the global carbon cycle. It has been thought that most of the dissolved iron discharged by hydrothermal vents is lost from solution close to ridge-axis sources and is thus of limited importance for <span class="hlt">ocean</span> biogeochemistry. This long-standing view is challenged by recent studies which suggest that stabilization of hydrothermal dissolved iron may facilitate its long-range <span class="hlt">oceanic</span> transport. Such transport has been subsequently inferred from spatially limited oceanographic observations. Here we report data from the US GEOTRACES Eastern Pacific Zonal Transect (EPZT) that demonstrate lateral transport of hydrothermal dissolved iron, manganese, and aluminium from the southern East Pacific Rise (SEPR) several thousand kilometres westward across the South Pacific <span class="hlt">Ocean</span>. Dissolved iron exhibits nearly conservative (that is, no loss from solution during transport and mixing) behaviour in this hydrothermal plume, implying a greater longevity in the deep <span class="hlt">ocean</span> than previously assumed. Based on our observations, we estimate a global hydrothermal dissolved iron input of three to four gigamoles per year to the <span class="hlt">ocean</span> interior, which is more than fourfold higher than previous estimates. Complementary simulations with a global-scale <span class="hlt">ocean</span> biogeochemical model suggest that the observed transport of hydrothermal dissolved iron requires some means of physicochemical stabilization and indicate that hydrothermally derived iron sustains a large fraction of Southern <span class="hlt">Ocean</span> export production.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008Tectp.451..290K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008Tectp.451..290K"><span>Detrital-zircon geochronology of Paleozoic sedimentary rocks in the Hangay Hentey <span class="hlt">basin</span>, north-central Mongolia: Implications for the tectonic evolution of the Mongol Okhotsk <span class="hlt">Ocean</span> in central Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelty, Thomas K.; Yin, An; Dash, Batulzii; Gehrels, George E.; Ribeiro, Angela E.</p> <p>2008-04-01</p> <p>Understanding the development of the Central Asian Orogenic System (CAOS), which is the largest Phanerozoic accretionary orogen in the world, is critical to the determination of continental growth mechanisms and geological history of central Asia. A key to unraveling its geological history is to ascertain the origin and tectonic setting of the large flysch complexes that dominate the CAOS. These complexes have been variably interpreted as deep-marine deposits that were accreted onto a long-evolving arc against large continents to form a mega-accretionary complex or sediments trapped in back-arc to fore-arc <span class="hlt">basins</span> within <span class="hlt">oceanic</span> island-arc systems far from continents. To differentiate the above models we conducted U-Pb geochronological analyses of detrital-zircon grains from turbidites in the composite Hangay-Hentey <span class="hlt">basin</span> of central Mongolia. This <span class="hlt">basin</span> was divided by a Cenozoic fault system into the western and eastern sub-<span class="hlt">basins</span>: the Hangay <span class="hlt">Basin</span> in the west and Hentey <span class="hlt">basin</span> in the east. This study focuses on the Hentey <span class="hlt">basin</span> and indicates two groups of samples within this <span class="hlt">basin</span>: (1) a southern group that were deposited after the earliest Carboniferous (˜ 339 Ma to 354 Ma) and a northern group that were deposited after the Cambrian to Neoproterozoic (˜ 504 Ma to 605 Ma). The samples from the northern part of the <span class="hlt">basin</span> consistently contain Paleoproterozoic and Archean zircon grains that may have been derived from the Tuva-Mongol massif and/or the Siberian craton. In contrast, samples from the southern part of the <span class="hlt">basin</span> contain only a minor component of early Paleozoic to Neoproterozoic zircon grains, which were derived from the crystalline basement bounding the Hangay-Hentey <span class="hlt">basin</span>. Integrating all the age results from this study, we suggest that the Hangay-Hentey <span class="hlt">basin</span> was developed between an island-arc system with a Neoproterozoic basement in the south and an Andean continental-margin arc in the north. The initiation of the southern arc occurred at or after the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.3723F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.3723F"><span>Numerical Simulation of The Mediterranean Sea Using Diecast: Interaction Between <span class="hlt">Basin</span>, Sub-<span class="hlt">basin</span> and Local Scale Features and Natural Variability.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernández, V.; Dietrich, D. E.; Haney, R. L.; Tintoré, J.</p> <p></p> <p>In situ and satellite data obtained during the last ten years have shown that the circula- tion in the Mediterranean Sea is extremely complex in space, with significant features ranging from mesoscale to sub-<span class="hlt">basin</span> and <span class="hlt">basin</span> scale, and highly variable in time, with mesoscale to seasonal and interannual signals. Also, the steep bottom topography and the variable atmospheric conditions from one sub-<span class="hlt">basin</span> to another, make the circula- tion to be composed of numerous energetic and narrow coastal currents, density fronts and mesoscale structures that interact at sub-<span class="hlt">basin</span> scale with the large scale circula- tion. To simulate numerically and better understand these features, besides high grid resolution, a low numerical dispersion and low physical dissipation <span class="hlt">ocean</span> model is required. We present the results from a 1/8z horizontal resolution numerical simula- tion of the Mediterranean Sea using DieCAST <span class="hlt">ocean</span> model, which meets the above requirements since it is stable with low general dissipation and uses accurate fourth- order-accurate approximations with low numerical dispersion. The simulations are carried out with climatological surface forcing using monthly mean winds and relax- ation towards climatological values of temperature and salinity. The model reproduces the main features of the large <span class="hlt">basin</span> scale circulation, as well as the seasonal variabil- ity of sub-<span class="hlt">basin</span> scale currents that are well documented by observations in straits and channels. In addition, DieCAST brings out natural fronts and eddies that usually do not appear in numerical simulations of the Mediterranean and that lead to a natural interannual variability. The role of this intrinsic variability in the general circulation will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918855A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918855A"><span>Arctic <span class="hlt">Ocean</span> Pathways in the 21st century</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aksenov, Yevgeny; van Gennip, Simon J.; Kelly, Stephen J.; Popova, Ekaterina E.; Yool, Andrew</p> <p>2017-04-01</p> <p>In the last three decades, changes in the Arctic environment have been occurring at an increasing rate. The opening up of large areas of previously sea ice-covered <span class="hlt">ocean</span> affects the marine environment with potential impacts on Arctic ecosystems, including through changes in Arctic access, industries and societies. Changes to sea ice and surface winds result in large-scale shifts in <span class="hlt">ocean</span> circulation and <span class="hlt">oceanic</span> pathways. This study presents a high-resolution analysis of the projected <span class="hlt">ocean</span> circulation and pathways of the Arctic water masses across the 21st century. The analysis is based on an eddy-permitting high-resolution global simulation of the <span class="hlt">ocean</span> general circulation model NEMO (Nucleus for European Modelling of the <span class="hlt">Ocean</span>) at the 1/4-degree horizontal resolution. The atmospheric forcing is from HadGEM2-ES model output from IPCC Assessment Report 5 (AR5) simulations performed for Coupled Model Intercomparison Project 5 (CMIP5), and follow the Representative Concentration Pathway 8.5 (RCP8.5) scenario. During the 21st century the AO experiences a significant warming, with sea surface temperature increased by in excess of 4 deg. C. Annual mean Arctic sea ice thickness drops to less than 0.5m, and the Arctic <span class="hlt">Ocean</span> is ice-free in summer from the mid-century. We use an off-line tracer technique to investigate Arctic pathways of the Atlantic and Pacific waters (AW and PW respectively) under this future climate. The AW tracers have been released in the eastern Fram Strait and in the western Barents Sea, whereas the PW tracer has been seeded in the Bering Strait. In the second half of the century the upper 1000 m <span class="hlt">ocean</span> circulation shows a reduction in the eastward AW flow along the continental slopes towards the Makarov and Canada <span class="hlt">basins</span> and a deviation of the PW flow away from the Beaufort Sea towards the Siberian coast. Strengthening of Arctic boundary current and intensification of the cyclonic gyre in the Nansen <span class="hlt">basin</span> of the Arctic <span class="hlt">Ocean</span> is accompanied by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611667P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611667P"><span>Role of tropical Indian and Atlantic <span class="hlt">Oceans</span> variability on ENSO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Prodhomme, Chloé; Terray, Pascal; Masson, Sebastien; Boschat, Ghyslaine</p> <p>2014-05-01</p> <p>There are strong evidences of an interaction between tropical Indian, Atlantic and Pacific <span class="hlt">Oceans</span>. Nevertheless, these interactions remain deeply controversial. While some authors claim the tropical Indian and Atlantic <span class="hlt">oceans</span> only play a passive role with respect to ENSO, others suggest a driving role for these two <span class="hlt">basins</span> on ENSO. The mecanisms underlying these relations are not fully understood and, in the Indian <span class="hlt">Ocean</span>, the possible role of both modes of tropical variability (the Indian <span class="hlt">Ocean</span> Dipole (IOD) and the Indian <span class="hlt">Ocean</span> <span class="hlt">Basin</span> mode (IOB)) remain unclear. To better quantify and understand how the variability of the tropical Indian and Atlantic <span class="hlt">Oceans</span> impact ENSO variability, we performed two sensitivity experiments using the SINTEX-F2 coupled model. For each experiment, we suppressed the variability of SST and the air-sea coupling in either the tropical Indian <span class="hlt">Ocean</span> or tropical Atlantic <span class="hlt">Ocean</span> by applying a strong nudging of the SST to the observed SST climatology. In both experiments, the ENSO periodicity increases. In the Atlantic experiment, our understanding of this increased periodicity is drastically limited by the strongly biased mean state in this region. Conversely, in the Indian <span class="hlt">Ocean</span> experiment, the increase of ENSO periodicity is related to the absence of the IOB following the El Niño peak, which leads to a decrease of westerly winds in the western Pacific during late winter and spring after the peak. These weaker westerlies hinders the transition to a La Niña phase and thus increase the duration and periodicity of the event.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...94a2132W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...94a2132W"><span>Water scarcity in Beijing and countermeasures to solve the problem at river <span class="hlt">basins</span> scale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Lixia; Gao, Jixi; Zou, Changxin; Wang, Yan; Lin, Naifeng</p> <p>2017-11-01</p> <p>Beijing has been subject to water scarcity in recent decades. Over-exploitation of water resources reduced water availability, and water-saving measures were not enough to mitigate the water scarcity. To address this problem, water transfer projects across river <span class="hlt">basins</span> are being built. This paper assessed water scarcity in Beijing and the feasibility of solving the problem at river <span class="hlt">basins</span> scale. The results indicate that there was an average annual water deficit of 13×108 m3 y-1 in Beijing, which totaled 208.9 ×108 m3 for 1998-2014, despite the adoption of various measures to alleviate water scarcity. Three of the <span class="hlt">adjacent</span> four sub-river <span class="hlt">basins</span> suffered a serious water deficit from 1998-2014. It was therefore impossible to transfer enough water from the <span class="hlt">adjacent</span> river <span class="hlt">basins</span> to mitigate the water scarcity in Beijing. However, the annual water deficit will be eliminated after the comprehensive operation of the world’s largest water transfer project (the South-to-North Water Transfer Project, SNWTP) in 2020, but it will take approximately 200 years before Beijing’s water resources are restored to the 1998 levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AtmEn.179..118R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AtmEn.179..118R"><span>Total dissolved atmospheric nitrogen deposition in the anoxic Cariaco <span class="hlt">basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rasse, R.; Pérez, T.; Giuliante, A.; Donoso, L.</p> <p>2018-04-01</p> <p>Atmospheric deposition of total dissolved nitrogen (TDN) is an important source of nitrogen for <span class="hlt">ocean</span> primary productivity that has increased since the industrial revolution. Thus, understanding its role in the <span class="hlt">ocean</span> nitrogen cycle will help assess recent changes in <span class="hlt">ocean</span> biogeochemistry. In the anoxic Cariaco <span class="hlt">basin</span>, the place of the CARIACO <span class="hlt">Ocean</span> Time-Series Program, the influence of atmospherically-deposited TDN on marine biogeochemistry is unknown. In this study, we measured atmospheric TDN concentrations as dissolved organic (DON) and inorganic (DIN) nitrogen (TDN = DIN + DON) in atmospheric suspended particles and wet deposition samples at the northeast of the <span class="hlt">basin</span> during periods of the wet (August-September 2008) and dry (March-April 2009) seasons. We evaluated the potential anthropogenic N influences by measuring wind velocity and direction, size-fractionated suspended particles, chemical traces and by performing back trajectories. We found DIN and DON concentration values that ranged between 0.11 and 0.58 μg-N m-3 and 0.11-0.56 μg-N m-3 in total suspended particles samples and between 0.08 and 0.54 mg-N l-1 and 0.02-1.3 mg-N l-1 in wet deposition samples, respectively. Continental air masses increased DON and DIN concentrations in atmospheric suspended particles during the wet season. We estimate an annual TDN atmospheric deposition (wet + particles) of 3.6 × 103 ton-N year-1 and concluded that: 1) Atmospheric supply of TDN plays a key role in the C and N budget of the <span class="hlt">basin</span> because replaces a fraction of the C (20% by induced primary production) and N (40%) removed by sediment burial, 2) present anthropogenic N could contribute to 30% of TDN atmospheric deposition in the <span class="hlt">basin</span>, and 3) reduced DON (gas + particles) should be a significant component of bulk N deposition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.6570B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.6570B"><span>The <span class="hlt">oceanic</span> variability of the Lofoten <span class="hlt">basin</span>: first results from the glider activity of the ProVoLo project</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bosse, Anthony; Fer, Ilker</p> <p>2017-04-01</p> <p>Located in the northern Norwegian Sea at high latitude between 68°N and 73°N, the Lofoten <span class="hlt">basin</span> is one of the world's most energetic areas regarding the <span class="hlt">ocean</span> dynamics. It hosts the largest and deepest pool of warm Atlantic Waters in the Nordic Seas, thus leading to very intense air-sea energy fluxes and deep convection in winter. Understanding the physical processes involved in the water mass transformations of this very productive area is thus of crucial interest in a climate perspective, as well as for the fishery economics. The ProVoLo project aims at quantifying the energy pathways from the large-scale circulation to the (sub-)mesoscale, and eventually to the dissipation scale. To this end, the project is largely devoted to in situ observations involving R/V cruises (CTD, LADCP, microstructure), mooring lines, gliders (CTD and microstructure) and RAFOS floats. Collecting data with gliders in such a dynamical environment is a challenge. We present results from two completed Seaglider missions of 8-months duration each, started in May 2016, as well as from three ongoing missions. The observations enable the description of two key features of the Lofoten <span class="hlt">basin</span> circulation: 1 - The Lofoten <span class="hlt">Basin</span> eddy, which is permanent anticyclonic vortex that has been regularly detected in the center of the <span class="hlt">basin</span> over the last decades. The vortex has very intense subsurface peak velocities exceeding 0.7 m/s and a small radius of about 15 km. The collected data also enable a description of the seasonal variability associated with the vortex, and give insight into its interaction with higher frequency flows. 2 - The frontal region situated along the Mohn ridge. The front is characterized by a narrow ( 15 km) and intense baroclinic jet separating the warm Atlantic waters from the cold waters coming from the Arctic. The observations from intensive sampling of this front, testify an important variability, at both seasonal time scale and from meso to submesoscale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016CliPa..12..837A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016CliPa..12..837A"><span>Constraints on <span class="hlt">ocean</span> circulation at the Paleocene-Eocene Thermal Maximum from neodymium isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abbott, April N.; Haley, Brian A.; Tripati, Aradhna K.; Frank, Martin</p> <p>2016-04-01</p> <p>Global warming during the Paleocene-Eocene Thermal Maximum (PETM) ˜ 55 million years ago (Ma) coincided with a massive release of carbon to the <span class="hlt">ocean</span>-atmosphere system, as indicated by carbon isotopic data. Previous studies have argued for a role of changing <span class="hlt">ocean</span> circulation, possibly as a trigger or response to climatic changes. We use neodymium (Nd) isotopic data to reconstruct short high-resolution records of deep-water circulation across the PETM. These records are derived by reductively leaching sediments from seven globally distributed sites to reconstruct past deep-<span class="hlt">ocean</span> circulation across the PETM. The Nd data for the leachates are interpreted to be consistent with previous studies that have used fish teeth Nd isotopes and benthic foraminiferal δ13C to constrain regions of convection. There is some evidence from combining Nd isotope and δ13C records that the three major <span class="hlt">ocean</span> <span class="hlt">basins</span> may not have had substantial exchanges of deep waters. If the isotopic data are interpreted within this framework, then the observed pattern may be explained if the strength of overturning in each <span class="hlt">basin</span> varied distinctly over the PETM, resulting in differences in deep-water aging gradients between <span class="hlt">basins</span>. Results are consistent with published interpretations from proxy data and model simulations that suggest modulation of overturning circulation had an important role for initiation and recovery of the <span class="hlt">ocean</span>-atmosphere system associated with the PETM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2006/1203/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1203/"><span>Reconnaissance Borehole Geophysical, Geological, and Hydrological Data from the Proposed Hydrodynamic Compartments of the Culpeper <span class="hlt">Basin</span> in Loudoun, Prince William, Culpeper, Orange, and Fairfax Counties, Virginia (Version 1.0)</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, Michael P.; Pierce, Herbert A.; Johnson, Carole D.; Sutphin, David M.; Daniels, David L.; Smoot, Joseph P.; Costain, John K.; Coruh, Cahit; Harlow, George E.</p> <p>2006-01-01</p> <p>The Culpeper <span class="hlt">basin</span> is part of a much larger system of ancient depressions or troughs, that lie inboard of the Atlantic Coastal Plain, and largely within the Applachian Piedmont Geologic Province of eastern North America, and the transition region with the neighboring Blue Ridge Geologic Province. This <span class="hlt">basin</span> system formed during an abortive attempt to make a great <span class="hlt">ocean</span> <span class="hlt">basin</span> during the Late Triassic and Early Jurassic, and the eroded remnants of the <span class="hlt">basins</span> record major episodes of sedimentation, igneous intrusion and eruption, and pervasive contact metamorphism. Altogether, some twenty nine <span class="hlt">basins</span> formed between what is now Nova Scotia and Georgia. Many of these <span class="hlt">basins</span> are discontinuous along their strike, and have therefore recorded isolated environments for fluvial and lacustrine sedimentation. Several <span class="hlt">basins</span> (including the Culpeper, Gettysburg, and Newark <span class="hlt">basins</span>) are fault-bounded on the west, and Mesozoic crustal stretching has produced assymetrical patterns of <span class="hlt">basin</span> subsidence resulting in a progressive <span class="hlt">basin</span> deepening to the west, and a virtual onlap relationship with the pre-<span class="hlt">basin</span> Proterozoic rocks to the east. A result of such a pattern of <span class="hlt">basin</span> deepening is the development of sequences of sandstones and siltstones that systemmatically increase in dip towards the accomodating western border faults. A second major structural theme in several of the major Mesozoic <span class="hlt">basins</span> (including the Culpeper) concerns the geometry of igneous intrusion, as discussed below. Froelich (1982, 1985) and Lee and Froelich (1989) discuss the general geology of the Culpeper <span class="hlt">basin</span>, and Smoot (1989) discusses the sedimentation environments and sedimentary facies of the Mesozoic with respect to fluvial and shallow lacustrine deposition in the Culpeper <span class="hlt">basin</span>. Ryan and others, 2007a, b, discuss the role of diabase-induced compartmentalization in the Culpeper <span class="hlt">basin</span> (and other Mesozoic <span class="hlt">basins</span>), and illustrate (using alteration mineral suites within the diabase and <span class="hlt">adjacent</span> hornfels, among</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/68210','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/68210"><span>Water resources of the Bighorn <span class="hlt">basin</span>, northwestern Wyoming</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Lowry, Marlin E.; Lowham, H.W.; Lines, Gregory C.</p> <p>1976-01-01</p> <p>This 2-sheet map report includes the part of the Bighorn <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> mountains in northwestern Wyoming. Water-bearing properties of the geologic units are summarized. The hydrogeologic map illustrates the distribution of wells in the different units and gives basic data on the yields of wells, depth of wells, depth to water, and dissolved solids and conductance of the water. Aquifers capable of yielding more than 1,000 gpm (gallons per minute) underlie the area everywhere, except in the mountains on the periphery of the <span class="hlt">basin</span>. In 1970, approximately 29,500 of the 40,475 people living in the Bighorn <span class="hlt">Basin</span> were served by municipal water supplies. The municipal supply for about 6,300 of these people was from ground water. The natural flows of streams in the Bighorn <span class="hlt">Basin</span> differ greatly due to a wide range in the meteorologic, topographic, and geologic conditions of the <span class="hlt">basin</span>. The station locations and the average discharge per square mile are shown on the map and give an indication of the geographic variation of <span class="hlt">basin</span> yields. The maximum instantaneous discharge that has occurred at each station during its period of record is shown. Most of the runoff in the <span class="hlt">basin</span> is from snowmelt in the mountains. (Woodard-USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..192....1M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..192....1M"><span>Quaternary dinoflagellate cysts in the Arctic <span class="hlt">Ocean</span>: Potential and limitations for stratigraphy and paleoenvironmental reconstructions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Matthiessen, Jens; Schreck, Michael; De Schepper, Stijn; Zorzi, Coralie; de Vernal, Anne</p> <p>2018-07-01</p> <p>The Arctic <span class="hlt">Ocean</span> is a siliciclastic depositional environment which lacks any rock-forming biogenic calcareous and siliceous components during large parts of its Quaternary history. These hemipelagic sediments are nevertheless suitable for the study of organic-walled microfossils of which the fossil remains of dinoflagellates - dinoflagellate cysts - are the most important group. Dinoflagellate cysts have become an important tool in paleoceanography of the high northern latitudes, but their potential for Quaternary biostratigraphy has remained largely unexplored. Dinoflagellate cysts are the dominant marine palynomorph group which is more continuously present in the marginal seas (e.g. Barents Sea, Bering Sea) than in the Arctic <span class="hlt">Ocean</span> itself throughout the Quaternary. Most species have long stratigraphic ranges, are temporary absent and show abundance variations on glacial-interglacial timescales. Of the more than 30 taxa recorded, only Habibacysta tectata and Filisphaera filifera became extinct in the Pleistocene. The highest persistent occurrence of H. tectata at ca. 2.0 Ma and the top of F. filifera acme at ca. 1.8 Ma can be used for supra-regional stratigraphic correlation between the Arctic <span class="hlt">Ocean</span> and <span class="hlt">adjacent</span> <span class="hlt">basins</span>. These events corroborate a slow sedimentation rate model for the Quaternary section on the central Lomonosov Ridge, but a combination of different methods will have to be applied to provide a detailed chronostratigraphy. The occurrence of cysts of phototrophic dinoflagellates in certain stratigraphic intervals on Lomonosov Ridge supports published evidence of episodic opening of the multiyear Arctic sea ice cover during the Quaternary probably related to a stronger inflow of Atlantic water. This contradicts the hypothesis of a permanently ice covered central Arctic <span class="hlt">Ocean</span> in the Quaternary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wri/1998/4031/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wri/1998/4031/report.pdf"><span>Ground Water in the Southern Lihue <span class="hlt">Basin</span>, Kauai, 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>Izuka, Scot K.; Gingerich, Stephen B.</p> <p>1998-01-01</p> <p>A multi-phased study of ground-water resources, including well drilling, aquifer tests, analysis of ground-water discharge, and numerical ground-water modeling, indicates that the rocks of the southern Lihue <span class="hlt">Basin</span>, Kauai, have permeabilities that are much lower than in most other areas of ground-water development in the Hawaiian islands. The regional hydraulic conductivity of the Koloa Volcanics, which dominates fresh ground-water flow in the <span class="hlt">basin</span>, is about 0.275 foot per day. The Waimea Canyon Basalt which surrounds the <span class="hlt">basin</span> and underlies the Koloa Volcanics within the <span class="hlt">basin</span> is intruded by dikes that reduce the bulk hydraulic conductivity of the rocks to about 1.11 feet per day. The low permeabilities result in steeper head gradients compared with other areas in the Hawaiian islands, and a higher proportion of ground-water discharging to streams than to the <span class="hlt">ocean</span>. Water levels rise from near sea level at the coast to several hundreds of feet above sea level at the center of the <span class="hlt">basin</span> a few miles inland. The high inland water levels are part of a completely saturated ground-water system. Because of the low regional hydraulic conductivity and high influx of water from recharge in the southern Lihue <span class="hlt">Basin</span>, the rocks become saturated nearly to the surface and a variably saturated/unsaturated (perched) condition is not likely to exist. Streams incising the upper part of the aquifer drain ground water and keep the water levels just below the surface in most places. Streams thus play an important role in shaping the water table in the southern Lihue <span class="hlt">Basin</span>. At least 62 percent of the ground water discharging from the aquifer in the southern Lihue <span class="hlt">Basin</span> seeps to streams; the remainder seeps directly to the <span class="hlt">ocean</span> or is withdrawn by wells.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614588C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614588C"><span>Long-term <span class="hlt">oceanic</span> changes prior the end-Triassic mass extinction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clémence, Marie-Emilie; Mette, Wolfgang; Thibault, Nicolas; Korte, Christoph</p> <p>2014-05-01</p> <p>A number of potential causes and kill mechanisms have been proposed for the end-Triassic mass extinction such as palaeoclimatic and sea-level variations, massive volcanism and <span class="hlt">ocean</span> acidification. Recent analysis of the stomatal index and density of fossil leaves and geochemical research on pedogenic carbonate nodules are suggestive of rising atmospheric CO2 concentration and fluctuating climate in the Rhaetian. It seems therefore probable that the end-Triassic event was preceded by large climatic fluctuations and environmental perturbations in the Rhaetian which might have partly affected the composition and diversity of the terrestrial and marine biota prior to the end-Triassic interval. The Northern Calcareous Alps (NCA) has long been favored for the study of the Rhaetian, since the GSSP of the Triassic/Jurassic (T/J) boundary and other important T/J sections are situated in this region. However, the most famous Rhaetian sections in the NCA are composed of carbonates from the Koessen Formation and were situated in a large isolated intraplatform <span class="hlt">Basin</span> (the Eiberg <span class="hlt">Basin</span>), bordered to the south-east by a well-developed coral reef in the NW of the Tethys border. Several Rhaetian sections composed of marls and shales of the Zlambach Formation were deposited at the same time on the other side of this reef, in the <span class="hlt">oceanic</span> Halstatt <span class="hlt">Basin</span>, which was in direct connection to the Tethys. Here, we present new results on sedimentology, stable isotope and trace element analysis of both intraplatform and <span class="hlt">oceanic</span> <span class="hlt">basin</span> deposits in the NCA. Intraplatform Rhaetian sections from the Koessen Formation bear a few minor intervals of shales with enrichments in organic matter, some of which are associated to carbon isotopic excursions. <span class="hlt">Oceanic</span> sections from the Hallstatt <span class="hlt">Basin</span> are characterized at the base by very cyclic marl-limestone alternations. Higher up in the section, sediments progressively turn into pure shale deposits and the top of the Formation is characterized by organic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol3/pdf/CFR-2013-title33-vol3-sec334-961.pdf','CFR2013'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2013-title33-vol3/pdf/CFR-2013-title33-vol3-sec334-961.pdf"><span>33 CFR 334.961 - Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2013&page.go=Go">Code of Federal Regulations, 2013 CFR</a></p> <p></p> <p>2013-07-01</p> <p>... 33 Navigation and Navigable Waters 3 2013-07-01 2013-07-01 false Pacific <span class="hlt">Ocean</span>, San Clemente... RESTRICTED AREA REGULATIONS § 334.961 Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore. (a) The danger zone: The waters of the Pacific <span class="hlt">Ocean</span> <span class="hlt">adjacent</span> to San Clemente...</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('https://www.gpo.gov/fdsys/pkg/CFR-2011-title33-vol3/pdf/CFR-2011-title33-vol3-sec334-961.pdf','CFR2011'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2011-title33-vol3/pdf/CFR-2011-title33-vol3-sec334-961.pdf"><span>33 CFR 334.961 - Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore.</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>... 33 Navigation and Navigable Waters 3 2011-07-01 2011-07-01 false Pacific <span class="hlt">Ocean</span>, San Clemente... RESTRICTED AREA REGULATIONS § 334.961 Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore. (a) The danger zone: The waters of the Pacific <span class="hlt">Ocean</span> <span class="hlt">adjacent</span> to San Clemente...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2012-title33-vol3/pdf/CFR-2012-title33-vol3-sec334-961.pdf','CFR2012'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2012-title33-vol3/pdf/CFR-2012-title33-vol3-sec334-961.pdf"><span>33 CFR 334.961 - Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2012&page.go=Go">Code of Federal Regulations, 2012 CFR</a></p> <p></p> <p>2012-07-01</p> <p>... 33 Navigation and Navigable Waters 3 2012-07-01 2012-07-01 false Pacific <span class="hlt">Ocean</span>, San Clemente... RESTRICTED AREA REGULATIONS § 334.961 Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore. (a) The danger zone: The waters of the Pacific <span class="hlt">Ocean</span> <span class="hlt">adjacent</span> to San Clemente...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol3/pdf/CFR-2014-title33-vol3-sec334-961.pdf','CFR2014'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2014-title33-vol3/pdf/CFR-2014-title33-vol3-sec334-961.pdf"><span>33 CFR 334.961 - Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore.</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2014&page.go=Go">Code of Federal Regulations, 2014 CFR</a></p> <p></p> <p>2014-07-01</p> <p>... 33 Navigation and Navigable Waters 3 2014-07-01 2014-07-01 false Pacific <span class="hlt">Ocean</span>, San Clemente... RESTRICTED AREA REGULATIONS § 334.961 Pacific <span class="hlt">Ocean</span>, San Clemente Island, California, naval danger zone off the northwest shore. (a) The danger zone: The waters of the Pacific <span class="hlt">Ocean</span> <span class="hlt">adjacent</span> to San Clemente...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70015537','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70015537"><span>Origin of the <span class="hlt">oceanic</span> basalt basement of the Solomon Islands arc and its relationship to the Ontong Java Plateau-insights from Cenozoic plate motion models</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Wells, R.E.</p> <p>1989-01-01</p> <p>Cenozoic global plate motion models based on a hotspot reference frame may provide a useful framework for analyzing the tectonic evolution of the Solomon Islands convergent margin. A postulated late Miocene collision of the Ontong Java Plateau (OJP) with a NE-facing arc is consistent with the predicted path of the OJP across the Pacific <span class="hlt">Basin</span> and its Miocene arrival at the trench. Late-stage igneous activity (65-30 Ma) predicted for the OJP as it rode over the Samoan hotspot occurred in correlative stratigraphic sections on Malaita, the supposed accreted flake of OJP in the Solomon Islands arc. Convergence similar to the present velocities between Australia and the Pacific plates was characteristic of the last 43 million years. Prior to 43 Ma Pacific-Australia plate motions were divergent, seemingly at odds with geologic evidence for early Tertiary convergence, particularly in Papua New Guinea. A postulated South Pacific plate may have existed between Australia and the Pacific plate and would have allowed implied northward subduction along the northeastern Australia plate boundary that lasted into the early Eocene. Subsequent reorganization of plate motions in the middle Eocene correlates with middle Eocene marginal <span class="hlt">basin</span> formation along ridges oblique to the main plate boundary. Cessation of spreading on the Pacific-South Pacific Ridge and its subsequent subduction beneath Asia followed the change in Pacific plate motion at 43 Ma. A trapped remnant of the extinct, NW-trending ridge may still lie beneath the western Philippine Sea. The terminal deformation, metamorphism and ophiolite obduction in the Eocene orogen of the southwest Pacific also correlates with the major change in Pacific plate motion at 43 Ma and the subsequent compression of the dying Eocene arc against outlying continental and <span class="hlt">oceanic</span> crustal blocks of the Australian plate. The Solomon Islands <span class="hlt">oceanic</span> basement may represent juxtaposition of <span class="hlt">oceanic</span> plateaus of the Australian plate beneath</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050217111','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050217111"><span>Remote Sensing of Particulate Organic Carbon Pools in the High-Latitude <span class="hlt">Oceans</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stramski, Dariusz; Stramska, Malgorzata</p> <p>2005-01-01</p> <p>The general goal of this project was to characterize spatial distributions at <span class="hlt">basin</span> scales and variability on monthly to interannual timescales of particulate organic carbon (POC) in the high-latitude <span class="hlt">oceans</span>. The primary objectives were: (1) To collect in situ data in the north polar waters of the Atlantic and in the Southern <span class="hlt">Ocean</span>, necessary for the derivation of POC <span class="hlt">ocean</span> color algorithms for these regions. (2) To derive regional POC algorithms and refine existing regional chlorophyll (Chl) algorithms, to develop understanding of processes that control bio-optical relationships underlying <span class="hlt">ocean</span> color algorithms for POC and Chl, and to explain bio-optical differentiation between the examined polar regions and within the regions. (3) To determine <span class="hlt">basin</span>-scale spatial patterns and temporal variability on monthly to interannual scales in satellite-derived estimates of POC and Chl pools in the investigated regions for the period of time covered by SeaWiFS and MODIS missions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4900D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4900D"><span>Indian <span class="hlt">Ocean</span> sources of Agulhas leakage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durgadoo, Jonathan; Rühs, Siren; Biastoch, Arne; Böning, Claus</p> <p>2017-04-01</p> <p>We examine the mean pathways, transit timescales, and transformation of waters flowing from the Pacific and the marginal seas through the Indian <span class="hlt">Ocean</span> (IO) on their way toward the South Atlantic within a high-resolution <span class="hlt">ocean</span>/sea-ice model. The model fields are analysed from a Lagrangian perspective where water volumes are tracked as they enter the IO. The IO contributes 12.6 Sv to Agulhas leakage, which within the model is 14.1 ± 2.2 Sv, the rest originates from the South Atlantic. The Indonesian Through-flow constitutes about half of the IO contribution, is surface bound, cools and salinificates as it leaves the <span class="hlt">basin</span> within 1-3 decades. Waters entering the IO south of Australia are at intermediate depths and maintain their temperature-salinity properties as they exit the <span class="hlt">basin</span> within 1.5-3.5 decades. Of these waters, the contribution from Tasman leakage is 1.4 Sv. The rest stem from recirculation of Subantarctic Mode Water formed within the IO. The marginal seas export 1.0 Sv into the Atlantic within 1.5-4 decades, and the waters cool and freshen on-route. However, the model's simulation of waters from the Gulfs of Aden and Oman are too light and hence overly susceptible to upper <span class="hlt">ocean</span> circulations. In the Cape <span class="hlt">Basin</span>, Agulhas leakage is well mixed. On-route, temperature-salinity transformations occur predominantly in the Arabian Sea and within the greater Agulhas Current region. Overall, the IO communicates at least 7.9 Sv from the Pacific to the Atlantic, thereby quantifying the strength of the upper cell of the global conveyor belt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050136630','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050136630"><span>Simulation of Water Sources and Precipitation Recycling for the MacKenzie, Mississippi and Amazon River <span class="hlt">Basins</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bosilovich, Michael G.; Chern, Jiun-Dar</p> <p>2005-01-01</p> <p>An atmospheric general circulation model simulation for 1948-1997 of the water budgets for the MacKenzie, Mississippi and Amazon River <span class="hlt">basins</span> is presented. In addition to the water budget, we include passive tracers to identify the geographic sources of water for the <span class="hlt">basins</span>, and the analysis focuses on the mechanisms contributing to precipitation recycling in each <span class="hlt">basin</span>. While each <span class="hlt">basin</span> s precipitation recycling has a strong dependency on evaporation during the mean annual cycle, the interannual variability of the recycling shows important relationships with the atmospheric circulation. The MacKenzie River <span class="hlt">basin</span> has only a weak interannual dependency on evaporation, where the variations in zonal moisture transport from the Pacific <span class="hlt">Ocean</span> can affect the <span class="hlt">basin</span> water cycle. On the other hand, the Mississippi River <span class="hlt">basin</span> has strong interannual dependencies on evaporation. While the precipitation recycling weakens with increased low level jet intensity, the evaporation variations exert stronger influence in providing water vapor for convective precipitation at the convective cloud base. High precipitation recycling is also found to be partly connected to warm SSTs in the tropical Pacific <span class="hlt">Ocean</span>. The Amazon River <span class="hlt">basin</span> evaporation exhibits small interannual variations, so that the interannual variations of precipitation recycling are related to atmospheric moisture transport from the tropical south Atlantic <span class="hlt">Ocean</span>. Increasing SSTs over the 50-year period are causing increased easterly transport across the <span class="hlt">basin</span>. As moisture transport increases, the Amazon precipitation recycling decreases (without real time varying vegetation changes). In addition, precipitation recycling from a bulk diagnostic method is compared to the passive tracer method used in the analysis. While the mean values are different, the interannual variations are comparable between each method. The methods also exhibit similar relationships to the terms of the <span class="hlt">basin</span> scale water budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PIAHS.379...31Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PIAHS.379...31Z"><span>Stability and tilting of regional water cycle over Tarim <span class="hlt">Basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Hongquan; Ma, Zhuguo</p> <p>2018-06-01</p> <p>The Tarim <span class="hlt">Basin</span> is located upwind of the Gobi Desert where individual deserts have expanded significantly during the last 50 years. In recent history, stable runoff in the Tarim <span class="hlt">Basin</span> has been observed despite the Lop Nur dry up and dramatic water consumption shift from east to west. This regional water cycle stability is conceptually explained based on the relationship between precipitation and evapotranspiration. The water consumption imbalance is caused by human activities near the river sources, which tilts the humidity profile over the <span class="hlt">basin</span>. As a result, more water vapour spills from the western part of the <span class="hlt">basin</span> and causes precipitation to increase in <span class="hlt">adjacent</span> areas. At the same time, the Westerlies carry the low humidity air mass out of the eastern part of the <span class="hlt">basin</span> to make the downwind Gobi Desert and surrounding areas drier. Therefore, the observed wetting on the west and drying on the east of northwest China are coupled.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150000330','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150000330"><span>Sensitivity of Simulated Global <span class="hlt">Ocean</span> Carbon Flux Estimates to Forcing by Reanalysis Products</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson W.; Casey, Nancy W.; Rousseaux, Cecile S.</p> <p>2015-01-01</p> <p>Reanalysis products from MERRA, NCEP2, NCEP1, and ECMWF were used to force an established <span class="hlt">ocean</span> biogeochemical model to estimate air-sea carbon fluxes (FCO2) and partial pressure of carbon dioxide (pCO2) in the global <span class="hlt">oceans</span>. Global air-sea carbon fluxes and pCO2 were relatively insensitive to the choice of forcing reanalysis. All global FCO2 estimates from the model forced by the four different reanalyses were within 20% of in situ estimates (MERRA and NCEP1 were within 7%), and all models exhibited statistically significant positive correlations with in situ estimates across the 12 major oceanographic <span class="hlt">basins</span>. Global pCO2 estimates were within 1% of in situ estimates with ECMWF being the outlier at 0.6%. <span class="hlt">Basin</span> correlations were similar to FCO2. There were, however, substantial departures among <span class="hlt">basin</span> estimates from the different reanalysis forcings. The high latitudes and tropics had the largest ranges in estimated fluxes among the reanalyses. Regional pCO2 differences among the reanalysis forcings were muted relative to the FCO2 results. No individual reanalysis was uniformly better or worse in the major oceanographic <span class="hlt">basins</span>. The results provide information on the characterization of uncertainty in <span class="hlt">ocean</span> carbon models due to choice of reanalysis forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25534631','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25534631"><span>Modelling the transport and accumulation of floating marine debris in the Mediterranean <span class="hlt">basin</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mansui, J; Molcard, A; Ourmières, Y</p> <p>2015-02-15</p> <p>In the era of plastic and global environmental issues, when large garbage patches have been observed in the main <span class="hlt">oceanic</span> <span class="hlt">basins</span>, this work is the first attempt to explore the possibility that similar permanent accumulation structures may exist in the Mediterranean Sea. The questions addressed in this work are: can the general circulation, with its sub-<span class="hlt">basins</span> scale gyres and mesoscale instabilities, foster the concentration of floating items in some regions? Where are the more likely coastal zones impacted from open <span class="hlt">ocean</span> sources? Multi-annual simulations of advected surface passive debris depict the Tyrrhenian Sea, the north-western Mediterranean sub-<span class="hlt">basin</span> and the Gulf of Sirte as possible retention areas. The western Mediterranean coasts present very low coastal impact, while the coastal strip from Tunisia to Syria appears as the favourite destination. No permanent structure able to retain floating items in the long-term were found, as the <span class="hlt">basin</span> circulation variability brings sufficient anomalies. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70131491','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70131491"><span>Spatial and seasonal responses of precipitation in the Ganges and Brahmaputra river <span class="hlt">basins</span> to ENSO and Indian <span class="hlt">Ocean</span> dipole modes: implications for flooding and drought</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pervez, Md Shahriar; Henebry, Geoffry M.</p> <p>2015-01-01</p> <p>We evaluated the spatial and seasonal responses of precipitation in the Ganges and Brahmaputra <span class="hlt">basins</span> as modulated by the El Niño Southern Oscillation (ENSO) and Indian <span class="hlt">Ocean</span> Dipole (IOD) modes using Global Precipitation Climatology Centre (GPCC) full data reanalysis of monthly global land-surface precipitation data from 1901 to 2010 with a spatial resolution of 0.5° × 0.5°. The GPCC monthly total precipitation climatology targeting the period 1951–2000 was used to compute gridded monthly anomalies for the entire time period. The gridded monthly anomalies were averaged for the years influenced by combinations of climate modes. Occurrences of El Niño alone significantly reduce (88% of the long-term average (LTA)) precipitation during the monsoon months in the western and southeastern Ganges <span class="hlt">Basin</span>. In contrast, occurrences of La Niña and co-occurrences of La Niña and negative IOD events significantly enhance (110 and 109% of LTA in the Ganges and Brahmaputra <span class="hlt">Basin</span>, respectively) precipitation across both <span class="hlt">basins</span>. When El Niño co-occurs with positive IOD events, the impacts of El Niño on the <span class="hlt">basins</span>' precipitation diminishes. When there is no active ENSO or IOD events (occurring in 41 out of 110 years), precipitation remains below average (95% of LTA) in the agriculturally intensive areas of Haryana, Uttar Pradesh, Rajasthan, Madhya Pradesh, and Western Nepal in the Ganges <span class="hlt">Basin</span>, whereas precipitation remains average to above average (104% of LTA) across the Brahmaputra <span class="hlt">Basin</span>. This pattern implies that a regular water deficit is likely, especially in the Ganges <span class="hlt">Basin</span>, with implications for the agriculture sector due to its reliance on consistent rainfall for successful production. Historically, major droughts occurred during El Niño and co-occurrences of El Niño and positive IOD events, while major flooding occurred during La Niña and co-occurrences of La Niña and negative IOD events in the <span class="hlt">basins</span>. This observational analysis will facilitate well</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27933047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27933047"><span>Diazotroph Diversity in the Sea Ice, Melt Ponds, and Surface Waters of the Eurasian <span class="hlt">Basin</span> of the Central Arctic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fernández-Méndez, Mar; Turk-Kubo, Kendra A; Buttigieg, Pier L; Rapp, Josephine Z; Krumpen, Thomas; Zehr, Jonathan P; Boetius, Antje</p> <p>2016-01-01</p> <p>The Eurasian <span class="hlt">basin</span> of the Central Arctic <span class="hlt">Ocean</span> is nitrogen limited, but little is known about the presence and role of nitrogen-fixing bacteria. Recent studies have indicated the occurrence of diazotrophs in Arctic coastal waters potentially of riverine origin. Here, we investigated the presence of diazotrophs in ice and surface waters of the Central Arctic <span class="hlt">Ocean</span> in the summer of 2012. We identified diverse communities of putative diazotrophs through targeted analysis of the nifH gene, which encodes the iron protein of the nitrogenase enzyme. We amplified 529 nifH sequences from 26 samples of Arctic melt ponds, sea ice and surface waters. These sequences resolved into 43 clusters at 92% amino acid sequence identity, most of which were non-cyanobacterial phylotypes from sea ice and water samples. One cyanobacterial phylotype related to Nodularia sp. was retrieved from sea ice, suggesting that this important functional group is rare in the Central Arctic <span class="hlt">Ocean</span>. The diazotrophic community in sea-ice environments appear distinct from other cold-adapted diazotrophic communities, such as those present in the coastal Canadian Arctic, the Arctic tundra and glacial Antarctic lakes. Molecular fingerprinting of nifH and the intergenic spacer region of the rRNA operon revealed differences between the communities from river-influenced Laptev Sea waters and those from ice-related environments pointing toward a marine origin for sea-ice diazotrophs. Our results provide the first record of diazotrophs in the Central Arctic and suggest that microbial nitrogen fixation may occur north of 77°N. To assess the significance of nitrogen fixation for the nitrogen budget of the Arctic <span class="hlt">Ocean</span> and to identify the active nitrogen fixers, further biogeochemical and molecular biological studies are needed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5120112','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5120112"><span>Diazotroph Diversity in the Sea Ice, Melt Ponds, and Surface Waters of the Eurasian <span class="hlt">Basin</span> of the Central Arctic <span class="hlt">Ocean</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>Fernández-Méndez, Mar; Turk-Kubo, Kendra A.; Buttigieg, Pier L.; Rapp, Josephine Z.; Krumpen, Thomas; Zehr, Jonathan P.; Boetius, Antje</p> <p>2016-01-01</p> <p>The Eurasian <span class="hlt">basin</span> of the Central Arctic <span class="hlt">Ocean</span> is nitrogen limited, but little is known about the presence and role of nitrogen-fixing bacteria. Recent studies have indicated the occurrence of diazotrophs in Arctic coastal waters potentially of riverine origin. Here, we investigated the presence of diazotrophs in ice and surface waters of the Central Arctic <span class="hlt">Ocean</span> in the summer of 2012. We identified diverse communities of putative diazotrophs through targeted analysis of the nifH gene, which encodes the iron protein of the nitrogenase enzyme. We amplified 529 nifH sequences from 26 samples of Arctic melt ponds, sea ice and surface waters. These sequences resolved into 43 clusters at 92% amino acid sequence identity, most of which were non-cyanobacterial phylotypes from sea ice and water samples. One cyanobacterial phylotype related to Nodularia sp. was retrieved from sea ice, suggesting that this important functional group is rare in the Central Arctic <span class="hlt">Ocean</span>. The diazotrophic community in sea-ice environments appear distinct from other cold-adapted diazotrophic communities, such as those present in the coastal Canadian Arctic, the Arctic tundra and glacial Antarctic lakes. Molecular fingerprinting of nifH and the intergenic spacer region of the rRNA operon revealed differences between the communities from river-influenced Laptev Sea waters and those from ice-related environments pointing toward a marine origin for sea-ice diazotrophs. Our results provide the first record of diazotrophs in the Central Arctic and suggest that microbial nitrogen fixation may occur north of 77°N. To assess the significance of nitrogen fixation for the nitrogen budget of the Arctic <span class="hlt">Ocean</span> and to identify the active nitrogen fixers, further biogeochemical and molecular biological studies are needed. PMID:27933047</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001DSRII..48.2241H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001DSRII..48.2241H"><span><span class="hlt">Basin</span>-scale variability in plankton biomass and community metabolism in the sub-tropical North Atlantic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harrison, W. G.; Arístegui, J.; Head, E. J. H.; Li, W. K. W.; Longhurst, A. R.; Sameoto, D. D.</p> <p></p> <p>Three trans-Atlantic oceanographic surveys (Nova Scotia to Canary Islands) were carried out during fall 1992 and spring 1993 to describe the large-scale variability in hydrographic, chemical and biological properties of the upper water column of the subtropical gyre and <span class="hlt">adjacent</span> waters. Significant spatial and temporal variability characterized a number of the biological pools and rate processes whereas others were relatively invariant. Systematic patterns were observed in the zonal distribution of some properties. Most notable were increases (eastward) in mixed-layer temperature and salinity, depths of the nitracline and chlorophyll- a maximum, regenerated production (NH 4 uptake) and bacterial production. Dissolved inorganic carbon (DIC) concentrations, phytoplankton biomass, mesozooplankton biomass and new production (NO 3 uptake) decreased (eastward). Bacterial biomass, primary production, and community respiration exhibited no discernible zonal distribution patterns. Seasonal variability was most evident in hydrography (cooler/fresher mixed-layer in spring), and chemistry (mixed-layer DIC concentration higher and nitracline shallower in spring) although primary production and bacterial production were significantly higher in spring than in fall. In general, seasonal variability was greater in the west than in the east; seasonality in most properties was absent west of Canary Islands (˜20°W). The distribution of autotrophs could be reasonably well explained by hydrography and nutrient structure, independent of location or season. Processes underlying the distribution of the microheterophs, however, were less clear. Heterotrophic biomass and metabolism was less variable than autotrophs and appeared to dominate the upper <span class="hlt">ocean</span> carbon balance of the subtropical North Atlantic in both fall and spring. Geographical patterns in distribution are considered in the light of recent efforts to partition the <span class="hlt">ocean</span> into distinct "biogeochemical provinces".</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29289084','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29289084"><span>The role of simulated small-scale <span class="hlt">ocean</span> variability in inverse computations for <span class="hlt">ocean</span> acoustic tomography.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dushaw, Brian D; Sagen, Hanne</p> <p>2017-12-01</p> <p><span class="hlt">Ocean</span> acoustic tomography depends on a suitable reference <span class="hlt">ocean</span> environment with which to set the basic parameters of the inverse problem. Some inverse problems may require a reference <span class="hlt">ocean</span> that includes the small-scale variations from internal waves, small mesoscale, or spice. Tomographic inversions that employ data of stable shadow zone arrivals, such as those that have been observed in the North Pacific and Canary <span class="hlt">Basin</span>, are an example. Estimating temperature from the unique acoustic data that have been obtained in Fram Strait is another example. The addition of small-scale variability to augment a smooth reference <span class="hlt">ocean</span> is essential to understanding the acoustic forward problem in these cases. Rather than a hindrance, the stochastic influences of the small scale can be exploited to obtain accurate inverse estimates. Inverse solutions are readily obtained, and they give computed arrival patterns that matched the observations. The approach is not ad hoc, but universal, and it has allowed inverse estimates for <span class="hlt">ocean</span> temperature variations in Fram Strait to be readily computed on several acoustic paths for which tomographic data were obtained.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMOS52B..06Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMOS52B..06Z"><span>Seismic investigation of an <span class="hlt">ocean</span>-continent transition zone in the northern 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>Zhu, J.; Qiu, X.; Xu, H.; Zhan, W.; Sun, Z.</p> <p>2011-12-01</p> <p>Rifted continental margins and <span class="hlt">basins</span> are mainly formed by the lithospheric extension. Thined lithosphere of passive continental margins results in decompression melt of magma and created <span class="hlt">oceanic</span> crust and thined <span class="hlt">ocean</span>-continent transition (OCT) zone. Two refraction profiles used <span class="hlt">ocean</span> bottom seismometers deployed in the broad continental shelf and three multi-channel seismic reflection lines in the northern South China Sea, acquired by the ship "Shiyan 2" of the South China Sea Institute of Oceanology, Chinese Academy of Sciences in 2010, are processed and interpreted in this study. Seismic reflection lines cut through the Dongsha rise, Zhu-1 and Zhu-2 depression within a Tertiary <span class="hlt">basin</span>, Pear River Mouth <span class="hlt">basin</span> (called as Zhujiangkou <span class="hlt">basin</span>). These tectonic features are clear imaged in the seismic reflection records. Numerous normal faults, cutted through the basement and related to the stretch of the northern South China Sea margin, are imaged and interpreted. Reflection characteristics of the <span class="hlt">ocean</span>-continent transition (OCT) zone are summaried and outlined. The COT zone is mainly divided into the northern syn-rift subsidence zone, central volcano or buried volcano uplift zone and tilt faulted block near the South Chia Sea <span class="hlt">basin</span>. Compared to the previous seismic reflection data and refraction velocity models, the segmentation range of the OCT zone is outlined, from width of about 225 km in the northeastern South China Sea , of 160 km in the central to of 110 km in the north-central South China Sea. Based on the epicenter distribution of sporadic and large than 6 magnitude earthquakes, it suggests the OCT zone in the northern South China Sea at present is still an active seismic zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1512902S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1512902S"><span>Partitioning of deformation along a reactivated rifted margin: example of the northern Ligurian margin.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sage, Françoise; Beslier, Marie-Odile; Gaullier, Virginie; Larroque, Christophe; Dessa, Jean-Xavier; Mercier de Lepinay, Bernard; Corradi, Nicola; Migeon, Sébastien; Katz, Hélène; Ruiz Constan, Ana</p> <p>2013-04-01</p> <p>The northern Ligurian margin, of Oligo-Miocene age, is currently undergoing compression related to microplate motions and/or to gravity spreading of the Alpine chain located immediately north of it. Active thrust faults and folds have previously been identified below the margin, together with a global uplift of the continental edge, since at least the Messinian. The seismicity that goes with the present-day margin contraction (e.g. Mw 6.9, 1887/02/23) extends to the axis of the <span class="hlt">adjacent</span> <span class="hlt">oceanic</span> <span class="hlt">basin</span> (e.g. ML 6.0, 1963/07/19; ML 5.4, 2011/07/07). However, we do not know of any recent or active crustal contractional structure within this <span class="hlt">oceanic</span> domain. In this study, we use new 12-channel high-resolution seismic data (FABLES seismic cruise, 2012, R/V Tethys II) in order to image the sedimentary cover of the Ligurian <span class="hlt">oceanic</span> <span class="hlt">basin</span>, up to ~3km below the seabed, including the Plio-Quaternary and the Messinian sediment down to the bottom of the Messinian salt layer. Because the Messinian event is well dated (5.96-5.32 Ma) and well identified in the seismic data, it forms a clear marker that we use to characterize the recent deformation related to both mobile salt motion and crustal tectonics. About 50 km south of the margin offshore of Italy, we identify huge and complex salt walls that elongate SW-NE. Such salt walls, which cannot be explained by salt tectonics only, are interpreted as evidence of deep-seated crustal deformation. They form en echelon structures that are well expressed in the seabed morphology, and do not correspond to any significant vertical throw at the base of the salt layer. This suggests that within the deep <span class="hlt">basin</span>, mainly strike-slip faulting accommodates long-term crustal deformation. It thus offers a contrast with the margin where deformation is mainly marked by shortening and reverse faulting, with vertical throws of several hundred meters. This discrepancy in the tectonic styles between the margin and the <span class="hlt">adjacent</span> <span class="hlt">oceanic</span> <span class="hlt">basin</span> suggests some</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS24B..02P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS24B..02P"><span>Decadal trends in deep <span class="hlt">ocean</span> salinity and regional effects on steric sea level</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Purkey, S. G.; Llovel, W.</p> <p>2017-12-01</p> <p>We present deep (below 2000 m) and abyssal (below 4000 m) global <span class="hlt">ocean</span> salinity trends from the 1990s through the 2010s and assess the role of deep salinity in local and global sea level budgets. Deep salinity trends are assessed using all deep <span class="hlt">basins</span> with available full-depth, high-quality hydrographic section data that have been occupied two or more times since the 1980s through either the World <span class="hlt">Ocean</span> Circulation Experiment (WOCE) Hydrographic Program or the Global Ship-Based Hydrographic Investigations Program (GO-SHIP). All salinity data is calibrated to standard seawater and any intercruise offsets applied. While the global mean deep halosteric contribution to sea level rise is close to zero (-0.017 +/- 0.023 mm/yr below 4000 m), there is a large regional variability with the southern deep <span class="hlt">basins</span> becoming fresher and northern deep <span class="hlt">basins</span> becoming more saline. This meridional gradient in the deep salinity trend reflects different mechanisms driving the deep salinity variability. The deep Southern <span class="hlt">Ocean</span> is freshening owing to a recent increased flux of freshwater to the deep <span class="hlt">ocean</span>. Outside of the Southern <span class="hlt">Ocean</span>, the deep salinity and temperature changes are tied to isopycnal heave associated with a falling of deep isopycnals in recent decades. Therefore, regions of the <span class="hlt">ocean</span> with a deep salinity minimum are experiencing both a halosteric contraction with a thermosteric expansion. While the thermosteric expansion is larger in most cases, in some regions the halosteric compensates for as much as 50% of the deep thermal expansion, making a significant contribution to local sea level rise budgets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70037529','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70037529"><span>An analysis of the carbon balance of the Arctic <span class="hlt">Basin</span> from 1997 to 2006</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>McGuire, A.D.; Hayes, D.J.; Kicklighter, D.W.; Manizza, M.; Zhuang, Q.; Chen, M.; Follows, M.J.; Gurney, K.R.; McClelland, J.W.; Melillo, J.M.; Peterson, B.J.; Prinn, R.G.</p> <p>2010-01-01</p> <p>This study used several model-based tools to analyse the dynamics of the Arctic <span class="hlt">Basin</span> between 1997 and 2006 as a linked system of land-<span class="hlt">ocean</span>-atmosphere C exchange. The analysis estimates that terrestrial areas of the Arctic <span class="hlt">Basin</span> lost 62.9 Tg C yr-1 and that the Arctic <span class="hlt">Ocean</span> gained 94.1 Tg C yr-1. Arctic lands and <span class="hlt">oceans</span> were a net CO2 sink of 108.9 Tg C yr-1, which is within the range of uncertainty in estimates from atmospheric inversions. Although both lands and <span class="hlt">oceans</span> of the Arctic were estimated to be CO2 sinks, the land sink diminished in strength because of increased fire disturbance compared to previous decades, while the <span class="hlt">ocean</span> sink increased in strength because of increased biological pump activity associated with reduced sea ice cover. Terrestrial areas of the Arctic were a net source of 41.5 Tg CH4 yr-1 that increased by 0.6 Tg CH4 yr-1 during the decade of analysis, a magnitude that is comparable with an atmospheric inversion of CH4. Because the radiative forcing of the estimated CH4 emissions is much greater than the CO2 sink, the analysis suggests that the Arctic <span class="hlt">Basin</span> is a substantial net source of green house gas forcing to the climate system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/wsp/1532e/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/wsp/1532e/report.pdf"><span>Hydrology and sedimentation of Corey Creek and Elk Run <span class="hlt">basins</span>, north-central Pennsylvania</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Reed, Lloyd A.</p> <p>1971-01-01</p> <p>Analysis of data collected from two small agricultural <span class="hlt">basins</span> in northcehtral Pennsylvania during the period May 1954 to September 1967 indicates that conservation measures reduced the quantity of suspended sediment leaving the Corey Creek <span class="hlt">basin</span> as a result of frequent storms during the growing season. Extensive soil conservation treatments were applied in the 12.2-squaremile Corey Creek <span class="hlt">basin</span>, but only minor treatments were applied in the <span class="hlt">adjacent</span> 10.2-square-mile Elk Run <span class="hlt">basin</span>. These treatments included the construction of ponds and diversion terraces and altering land use by such measures as establishing permanent hay land and changing marginal pasture land to wood lands. Elk Run <span class="hlt">basin</span>, which is topographically and hydrologically similar to the Corey Creek <span class="hlt">basin</span>, was used as an external control to assist in detecting and evaluating the hydrologic changes in Corey Creek. Trend analyses of data from both <span class="hlt">basins</span> indicate a 47-percent decrease in sediment discharge from Corey Creek during the frequent storms that occur in the May to October growing season. Six percent of the sediment discharged from Corey Creek during the period of this investigation (1954-67) was discharged during these frequent growing-season storms. The remaining 94 percent of the sediment was discharged during the November to April dormant season and during two major events during the growing season, one October 1955 and one May 1961. No decrease in sediment discharge was observed for these events or for this period. The <span class="hlt">adjacent</span> <span class="hlt">basin</span> of similar size, topography, and hydrologic characteristics, Elk Run, was not scheduled for extensive conservation treatment; it was selected as a control for this study "because of the assumption that any changes in precipitation and runoff patterns would affect both <span class="hlt">basins</span> in a similar manner. Rainfall, runoff, sediment, and stream-channel data are used in this report to estimate the probable hydrologic behavior of the Corey Creek <span class="hlt">basin</span> provided the intensive</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/2017EGUGA..1911248Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911248Y"><span><span class="hlt">Oceanic</span> Channel of the IOD-ENSO teleconnection over the Indo-Pacific <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yuan, Dongliang; Wang, Jing; Zhao, Xia; Zhou, Hui; Xu, Tengfei; Xu, Peng</p> <p>2017-04-01</p> <p>The lag correlations of observations and model simulated data that participate the Coupled Model Intercomparison Project phase-5 (CMIP5) are used to study the precursory teleconnection between the Indian <span class="hlt">Ocean</span> Dipole (IOD) and the Pacific ENSO one year later through the Indonesian seas. The results suggest that Indonesian Throughflow (ITF) play an important role in the IOD-ENSO teleconnection. Numerical simulations using a hierarchy of <span class="hlt">ocean</span> models and climate coupled models have shown that the interannual sea level depressions in the southeastern Indian <span class="hlt">Ocean</span> during IOD force enhanced ITF to transport warm water of the Pacific warm pool to the Indian <span class="hlt">Ocean</span>, producing cold subsurface temperature anomalies, which propagate to the eastern equatorial Pacific and induce significant coupled <span class="hlt">ocean</span>-atmosphere evolution. The teleconnection is found to have decadal variability. Similar decadal variability has also been identified in the historical simulations of the CMIP5 models. The dynamics of the inter-<span class="hlt">basin</span> teleconnection during the positive phases of the decadal variability are diagnosed to be the interannual variations of the ITF associated with the Indian <span class="hlt">Ocean</span> Dipole (IOD). During the negative phases, the thermocline in the eastern equatorial Pacific is anomalously deeper so that the sea surface temperature anomalies in the cold tongue are not sensitive to the thermocline depth changes. The IOD-ENSO teleconnection is found not affected significantly by the anthropogenic forcing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28202958','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28202958"><span>Decline in global <span class="hlt">oceanic</span> oxygen content during the past five decades.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schmidtko, Sunke; Stramma, Lothar; Visbeck, Martin</p> <p>2017-02-15</p> <p><span class="hlt">Ocean</span> models predict a decline in the dissolved oxygen inventory of the global <span class="hlt">ocean</span> of one to seven per cent by the year 2100, caused by a combination of a warming-induced decline in oxygen solubility and reduced ventilation of the deep <span class="hlt">ocean</span>. It is thought that such a decline in the <span class="hlt">oceanic</span> oxygen content could affect <span class="hlt">ocean</span> nutrient cycles and the marine habitat, with potentially detrimental consequences for fisheries and coastal economies. Regional observational data indicate a continuous decrease in <span class="hlt">oceanic</span> dissolved oxygen concentrations in most regions of the global <span class="hlt">ocean</span>, with an increase reported in a few limited areas, varying by study. Prior work attempting to resolve variations in dissolved oxygen concentrations at the global scale reported a global oxygen loss of 550 ± 130 teramoles (10 12  mol) per decade between 100 and 1,000 metres depth based on a comparison of data from the 1970s and 1990s. Here we provide a quantitative assessment of the entire <span class="hlt">ocean</span> oxygen inventory by analysing dissolved oxygen and supporting data for the complete <span class="hlt">oceanic</span> water column over the past 50 years. We find that the global <span class="hlt">oceanic</span> oxygen content of 227.4 ± 1.1 petamoles (10 15  mol) has decreased by more than two per cent (4.8 ± 2.1 petamoles) since 1960, with large variations in oxygen loss in different <span class="hlt">ocean</span> <span class="hlt">basins</span> and at different depths. We suggest that changes in the upper water column are mostly due to a warming-induced decrease in solubility and biological consumption. Changes in the deeper <span class="hlt">ocean</span> may have their origin in <span class="hlt">basin</span>-scale multi-decadal variability, <span class="hlt">oceanic</span> overturning slow-down and a potential increase in biological consumption.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.C21A0693M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.C21A0693M"><span><span class="hlt">Ocean</span> observations from below Petermann Gletscher</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muenchow, A.; Nicholls, K. W.; Heuzé, C.; Wahlin, A.; Mix, A. C.</p> <p>2015-12-01</p> <p>Petermann Gletscher drains 4% of the Greenland ice sheet via a floating ice shelf that has shrunk from 1,300 to 900 km^2 in area via two calving events in 2010 and 2012. The glacier is thinning by about 10 vertical meters per year when integrated over 45 km from the grounding zone to the terminus. Most of this mass loss is caused by <span class="hlt">ocean</span> melting, but only a single vertical <span class="hlt">ocean</span> profile taken in 2002 exists. The fjord was mostly free of sea ice in August when we visited in 2003, 2006, 2007, 2009, and 2012 and noticed a small warming trend of bottom waters. During a 2-day survey of Petermann Fjord and <span class="hlt">adjacent</span> Nares Strait in 2012 we documented a large intrusion of warmer Atlantic waters spilling over the 400 m deep sill and sinking to more than 800 m depth. These waters fill the deep <span class="hlt">basin</span> of the fjord and move towards the grounding zone of glacier at 550 m below the sea surface. In August 2015 the Swedish icebreaker I/B Oden is scheduled to enter Nares Strait and Petermann Fjord to support field work on land, on water, and on the floating glacier. We here report preliminary results from both <span class="hlt">ocean</span> surveys and ice shelf moorings. The moored observations from under the ice shelf extend synoptic survey data from Oden. The ice shelf moorings are designed to resolve tidal to interannual variations of water properties under the floating glacier. More specifically, we plan to install a total 13 discrete sensors to measure <span class="hlt">ocean</span> temperature, salinity, and pressure at five locations distributed both along and across the floating glacier. Hot water drilling provides the holes through the 200 to 500 m thick glacier ice to collect sediment cores, take a profile of temperature and salinity, and deploy two to five cabled sensors per mooring. If successful, data from these cabled instruments will be distributed via surface Iridium connections and posted on the web in near real time. We will discuss successes and failures of this ambitious and high risk program that was</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012NatGe...5..775N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012NatGe...5..775N"><span>Compositional evidence for an impact origin of the Moon's Procellarum <span class="hlt">basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nakamura, Ryosuke; Yamamoto, Satoru; Matsunaga, Tsuneo; Ishihara, Yoshiaki; Morota, Tomokatsu; Hiroi, Takahiro; Takeda, Hiroshi; Ogawa, Yoshiko; Yokota, Yasuhiro; Hirata, Naru; Ohtake, Makiko; Saiki, Kazuto</p> <p>2012-11-01</p> <p>The asymmetry between the nearside and farside of the Moon is evident in the distribution of mare basalt, crustal thickness and concentrations of radioactive elements, but its origin remains controversial. According to one attractive scenario, a gigantic impact early in the Moon's history produced the observed dichotomy; the putative 3,000-km-diameter Procellarum <span class="hlt">basin</span> has been suggested to be a relic of this ancient impact. Low-calcium pyroxene can be formed during an impact by melting a mixture of crust and mantle materials or by excavating differentiated cumulates from the lunar magma <span class="hlt">ocean</span>. Therefore, the association of low-calcium pyroxene with a lunar <span class="hlt">basin</span> could indicate an impact origin. Here we use spectral mapping data from KAGUYA/SELENE (ref. ) to show that low-calcium pyroxene is concentrated around two established impact structures, the South Pole-Aitken and Imbrium <span class="hlt">basins</span>. In addition, we detect a high concentration of low-calcium pyroxene at Procellarum, which supports an impact origin of the ancient <span class="hlt">basin</span>. We propose that, in forming the largest known <span class="hlt">basin</span> on the Moon, the impact excavated the nearside's primary feldspathic crust, which derived from the lunar magma <span class="hlt">ocean</span>. A secondary feldspathic crust would have later recrystallized from the sea of impact melt, leading to two distinct sides of the Moon.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/sir/2007/5099/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/sir/2007/5099/"><span>Application of the <span class="hlt">Basin</span> Characterization Model to Estimate In-Place Recharge and Runoff Potential in the <span class="hlt">Basin</span> and Range Carbonate-Rock Aquifer System, White Pine County, Nevada, and <span class="hlt">Adjacent</span> Areas in Nevada and Utah</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Flint, Alan L.; Flint, Lorraine E.</p> <p>2007-01-01</p> <p>A regional-scale water-balance model was used to estimate recharge and runoff potential and support U.S. Geological Survey efforts to develop a better understanding of water availability for the <span class="hlt">Basin</span> and Range carbonate-rock aquifer system (BARCAS) study in White Pine County, Nevada, and <span class="hlt">adjacent</span> areas in Nevada and Utah. The water-balance model, or <span class="hlt">Basin</span> Characterization Model (BCM), was used to estimate regional ground-water recharge for the 13 hydrographic areas in the study area. The BCM calculates recharge by using a distributed-parameter, water-balance method and monthly climatic boundary conditions. The BCM requires geographic information system coverages of soil, geology, and topographic information with monthly time-varying climatic conditions of air temperature and precipitation. Potential evapotranspiration, snow accumulation, and snowmelt are distributed spatially with process models. When combined with surface properties of soil-water storage and saturated hydraulic conductivity of bedrock and alluvium, the potential water available for in-place recharge and runoff is calculated using monthly time steps using a grid scale of 866 feet (270 meters). The BCM was used with monthly climatic inputs from 1970 to 2004, and results were averaged to provide an estimate of the average annual recharge for the BARCAS study area. The model estimates 526,000 acre-feet of potential in-place recharge and approximately 398,000 acre-feet of potential runoff. Assuming 15 percent of the runoff becomes recharge, the model estimates average annual ground-water recharge for the BARCAS area of about 586,000 acre-feet. When precipitation is extrapolated to the long-term climatic record (1895-2006), average annual recharge is estimated to be 530,000 acre-feet, or about 9 percent less than the recharge estimated for 1970-2004.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1047/srp/srp025/of2007-1047srp025.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1047/srp/srp025/of2007-1047srp025.pdf"><span>Basement and crustal structure of the Davis Sea region (East Antarctica): implications for tectonic setting and continent to <span class="hlt">oceanic</span> boundary definition</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Guseva, Y.B.; Leitchenkov, G.L.; Gandyukhin, V.V.; Ivanov, S.V.</p> <p>2007-01-01</p> <p>This study is based on about 8400 km of MCS, magnetic and gravity data as well as 20 sonobuoys collected by the Russian Antarctic Expedition during 2003 and 2004 in the Davis Sea and <span class="hlt">adjacent</span> areas between 80°E and 102°E. Major tectonic provinces and features are identified and mapped in the study region including: 1) A marginal rift with a the extended continental crust ranging 130 to more than 200 km in width; 2) The marginal volcanic plateau of the Bruce Bank consisting of the Early Cretaceous igneous rocks; 3) The Early Cretaceous and Late Cretaceous−Paleogene <span class="hlt">oceanic</span> <span class="hlt">basins</span>; and 4) The Early Cretaceous igneous province of the Kerguelen Plateau. Four major horizons identified in the sedimentary cover of the Davis Sea region are attributed to main tectonic events and/or paleoenvironmental changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://archives.datapages.com/data/specpubs/oversiz2/data/a189/a189/0001/0050/0081.htm','USGSPUBS'); return false;" href="http://archives.datapages.com/data/specpubs/oversiz2/data/a189/a189/0001/0050/0081.htm"><span>Passive margins: U.S. Geological Survey Line 19 across the Georges Bank <span class="hlt">basin</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>Klitgord, Kim D.; Schlee, John S.; Grow, John A.; Bally, A.W.</p> <p>1987-01-01</p> <p>Georges Bank is a shallow part of the Atlantic continental shelf southeast of New England (Emery and Uchupi, 1972, 1984). This bank, however, is merely the upper surface of several sedimentary <span class="hlt">basins</span> overlying a block-faulted basement of igneous and metamorphic crystalline rock. Sedimentary rock forms a seaward-thickening cover that has accumulated in one main depocenter and several ancillary depressions, <span class="hlt">adjacent</span> to shallow basement platforms of paleozoic and older crystalline rock. Georges Bank <span class="hlt">basin</span> contains a thickness of sedimentary rock greater than 10 km, whereas the basement platforms that flank the <span class="hlt">basin</span> are areas of thin sediment accumulation (less than 5 km).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981Tectp..72..229D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981Tectp..72..229D"><span>Variations in the degree of crustal extension during formation of a back-arc <span class="hlt">basin</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 Wit, Maarten J.; Stern, Charles R.</p> <p>1981-02-01</p> <p>Ophiolite complexes in southern Chile represent the remnants of the mafic portion of the floor of a Cretaceous back-arc <span class="hlt">basin</span> which widened markedly from north to south over a length of 600 km. Detailed field and geochemical studies of ophiolites in the northern (Sarmiento complex) and southern (Tortuga complex) extremities of the originally wedge-shaped back-arc <span class="hlt">basin</span> floor, indicate significant north—south differences in the mode of emplacement of basaltic magmas into the pre-existing continental crust, during the formation of the <span class="hlt">basin</span>. In the northern narrow extremity of the original <span class="hlt">basin</span>, mafic melts intruded into the continental crust over a diffuse zone causing extensive remobilization and reconstitution of the sialic continental crust. In the southern wider part of the original <span class="hlt">basin</span>, mafic magmas appear to have been emplaced at a localized <span class="hlt">oceanic</span>-type spreading centre. The observed north—south variations resulted in formation of back-arc floor with crustal characteristics ranging from intermediate between continental and <span class="hlt">oceanic</span> to typically <span class="hlt">oceanic</span>. These variations are interpreted as representing different stages of evolution of a back-arc <span class="hlt">basin</span> which formed due to a subtle interplay between subduction induced back-arc mantle convection and the release of stress across the convergent plate boundary, possibly related to ridge subduction. Prior to the release of stress, heat transferred from mantle diapirs to the base of crust caused widespread silicic volcanism in South America. With the release of stress, mantle derived melts erupted to the surface along structural pathways resulting in extensive basaltic volcanism in a linear belt behind the island arc and the cessation of silicic volcanism. Initially, basaltic magmas intruded the continental crust over a diffuse region causing reconstitution of sialic crustal rocks. Progressive localization of the zone of intrusion of mafic magmas from the mantle eventually resulted in the development of an</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ClDy...45..989M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ClDy...45..989M"><span>The <span class="hlt">ocean</span>-atmosphere response to wind-induced thermocline changes in the tropical South Western Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manola, Iris; Selten, F. M.; de Ruijter, W. P. M.; Hazeleger, W.</p> <p>2015-08-01</p> <p>In the Indian <span class="hlt">Ocean</span> <span class="hlt">basin</span> the sea surface temperatures (SSTs) are most sensitive to changes in the <span class="hlt">oceanic</span> depth of the thermocline in the region of the Seychelles Dome. Observational studies have suggested that the strong SST variations in this region influence the atmospheric evolution around the <span class="hlt">basin</span>, while its impact could extend far into the Pacific and the extra-tropics. Here we study the adjustments of the coupled atmosphere-<span class="hlt">ocean</span> system to a winter shallow doming event using dedicated ensemble simulations with the state-of-the-art EC-Earth climate model. The doming creates an equatorial Kelvin wave and a pair of westward moving Rossby waves, leading to higher SST 1-2 months later in the Western equatorial Indian <span class="hlt">Ocean</span>. Atmospheric convection is strengthened and the Walker circulation responds with reduced convection over Indonesia and cooling of the SST in that region. The Pacific warm pool convection shifts eastward and an <span class="hlt">oceanic</span> Kelvin wave is triggered at thermocline depth. The wave leads to an SST warming in the East Equatorial Pacific 5-6 months after the initiation of the Seychelles Dome event. The atmosphere responds to this warming with weak anomalous atmospheric convection. The changes in the upper tropospheric divergence in this sequence of events create large-scale Rossby waves that propagate away from the tropics along the atmospheric waveguides. We suggest to repeat these types of experiments with other models to test the robustness of the results. We also suggest to create the doming event in June so that the East-Pacific warming occurs in November when the atmosphere is most sensitive to SST anomalies and El Niño could possibly be triggered by the doming event under suitable conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Tectp.716...21J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Tectp.716...21J"><span>Crustal structure of the Agulhas Ridge (South Atlantic <span class="hlt">Ocean</span>): Formation above a hotspot?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jokat, Wilfried; Hagen, Claudia</p> <p>2017-10-01</p> <p>The southern South Atlantic <span class="hlt">Ocean</span> contains several features believed to document the traces of hotspot volcanism during the early formation of the <span class="hlt">ocean</span> <span class="hlt">basin</span>, namely the Agulhas Ridge and the Cape Rise seamounts located in the southeast Atlantic between 36°S and 50°S. The Agulhas Ridge parallels the Agulhas-Falkland Fracture Zone, one of the major transform zones of the world. The morphology of the ridge changes dramatically from two parallel segments in the southwest, to the broad plateau-like Agulhas Ridge in the northeast. Because the crustal fabric of the ridge is unknown relating its evolution to hotspots in the southeast Atlantic is an open question. During the RV Polarstern cruise ANT-XXIII-5 seismic reflection and refraction data were collected along a 370 km long profile with 8 <span class="hlt">Ocean</span> Bottom Stations to investigate its crustal fabric. The profile extends in NNE direction from the Agulhas <span class="hlt">Basin</span>, 60 km south of the Agulhas Ridge, and continues into the Cape <span class="hlt">Basin</span> crossing the southernmost of the Cape Rise seamounts. In the Cape <span class="hlt">Basin</span> we found a crustal thickness of 5.5-7.5 km, and a velocity distribution typical for <span class="hlt">oceanic</span> crust. The Cape Rise seamounts, however, show a higher velocity in comparison to the surrounding <span class="hlt">oceanic</span> crust and the Agulhas Ridge. Underplated material is evident below the southernmost of the Cape Rise seamounts. It also has a 5-8% higher density compared to the Agulhas Plateau. The seismic velocities of the Agulhas Ridge are lower, the crustal thickness is approximately 14 km, and age dating of dredge samples from its top provides clear evidence of rejuvenated volcanism at around 26 Ma. Seismic data indicate that although the Cape Rise seamounts formed above a mantle thermal anomaly it had a limited areal extent, whereas the hotspot material that formed the Agulhas Ridge likely erupted along a fracture zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.6106G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.6106G"><span><span class="hlt">Ocean</span> Hydrodynamics Numerical Model in Curvilinear Coordinates for Simulating Circulation of the Global <span class="hlt">Ocean</span> and its Separate <span class="hlt">Basins</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gusev, Anatoly; Diansky, Nikolay; Zalesny, Vladimir</p> <p>2010-05-01</p> <p>The original program complex is proposed for the <span class="hlt">ocean</span> circulation sigma-model, developed in the Institute of Numerical Mathematics (INM), Russian Academy of Sciences (RAS). The complex can be used in various curvilinear orthogonal coordinate systems. In addition to <span class="hlt">ocean</span> circulation model, the complex contains a sea ice dynamics and thermodynamics model, as well as the original system of the atmospheric forcing implementation on the basis of both prescribed meteodata and atmospheric model results. This complex can be used as the <span class="hlt">oceanic</span> block of Earth climate model as well as for solving the scientific and practical problems concerning the World <span class="hlt">ocean</span> and its separate <span class="hlt">oceans</span> and seas. The developed program complex can be effectively used on parallel shared memory computational systems and on contemporary personal computers. On the base of the complex proposed the <span class="hlt">ocean</span> general circulation model (OGCM) was developed. The model is realized in the curvilinear orthogonal coordinate system obtained by the conformal transformation of the standard geographical grid that allowed us to locate the system singularities outside the integration domain. The horizontal resolution of the OGCM is 1 degree on longitude, 0.5 degree on latitude, and it has 40 non-uniform sigma-levels in depth. The model was integrated for 100 years starting from the Levitus January climatology using the realistic atmospheric annual cycle calculated on the base of CORE datasets. The experimental results showed us that the model adequately reproduces the basic characteristics of large-scale World <span class="hlt">Ocean</span> dynamics, that is in good agreement with both observational data and results of the best climatic OGCMs. This OGCM is used as the <span class="hlt">oceanic</span> component of the new version of climatic system model (CSM) developed in INM RAS. The latter is now ready for carrying out the new numerical experiments on climate and its change modelling according to IPCC (Intergovernmental Panel on Climate Change) scenarios in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.C34B..01M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.C34B..01M"><span>North Greenland's Ice Shelves and <span class="hlt">Ocean</span> Warming</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Muenchow, A.; Schauer, U.; Padman, L.; Melling, H.; Fricker, H. A.</p> <p>2014-12-01</p> <p>Rapid disintegration of ice shelves (the floating extensions of marine-terminating glaciers) can lead to increasing ice discharge, thinning upstream ice sheets, rising sea level. Pine Island Glacier, Antarctica, and Jacobshavn Isbrae, Greenland, provide prominent examples of these processes which evolve at decadal time scales. We here focus on three glacier systems north of 78 N in Greenland, each of which discharges more than 10 Gt per year of ice and had an extensive ice shelf a decade ago; Petermann Gletscher (PG), Niogshalvfjerdsfjorden (79N), and Zachariae Isstrom (ZI). We summarize and discuss direct observations of <span class="hlt">ocean</span> and glacier properties for these systems as they have evolved in the northwest (PG) and northeast (79N and ZI) of Greenland over the last two decades. We use a combination of modern and historical snapshots of <span class="hlt">ocean</span> temperature and salinity (PG, 79N, ZI), moored observations in Nares Strait (PG), and snapshots of temperature and velocity fields on the broad continental shelf off northeast Greenland (79N, ZI) collected between 1993 and 2014. <span class="hlt">Ocean</span> warming <span class="hlt">adjacent</span> to PG has been small relative to the <span class="hlt">ocean</span> warming <span class="hlt">adjacent</span> to 79N and ZI; however, ZI lost its entire ice shelf during the last decade while 79N, less than 70 km to the north of ZI, remained stable. In contrast, PG has thinned by about 10 m/y just prior to shedding two ice islands representing almost half its ice shelf area or a fifth by volume. At PG advective ice flux divergence explains about half of the dominantly basal melting while response to non-steady external forcing explains the other half. The observations at PG,79N, and ZI suggest that remotely sensed ambient surface <span class="hlt">ocean</span> temperatures are poor proxies to explain ice shelf thinning and retreat. We posit that local dynamics of the subsurface <span class="hlt">ocean</span> heat flux matters most. <span class="hlt">Ocean</span> heat must first be delivered over the sill into the fjord and then within the ice shelf cavity to the base of the shelf near the grounding line</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040081066&hterms=chlorophyll&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchlorophyll','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040081066&hterms=chlorophyll&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dchlorophyll"><span>Recent Trends in Global <span class="hlt">Ocean</span> Chlorophyll</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gregg, Watson; Casey, Nancy</p> <p>2004-01-01</p> <p>Recent analyses of SeaWiFS data have shown that global <span class="hlt">ocean</span> chlorophyll has increased more than 5% since 1998. The North Pacific <span class="hlt">ocean</span> <span class="hlt">basin</span> has increased nearly 19%. To understand the causes of these trends we have applied the newly developed NASA <span class="hlt">Ocean</span> Biogeochemical Assimilation Model (OBAM), which is driven in mechanistic fashion by surface winds, sea surface temperature, atmospheric iron deposition, sea ice, and surface irradiance. The mode1 utilizes chlorophyll from SeaWiFS in a daily assimilation. The model has in place many of the climatic variables that can be expected to produce the changes observed in SeaWiFS data. Ths enables us to diagnose the model performance, the assimilation performance, and possible causes for the increase in chlorophyll.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMOS51C2081H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMOS51C2081H"><span>Formation of post-spreading volcanic ridges in the East sub-<span class="hlt">basin</span> of the 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>He, E.; Zhao, M.; Sibuet, J. C.; Tan, P.; Wang, J.; Qiu, X.</p> <p>2016-12-01</p> <p>In the South China Sea (SCS), the post-spreading magmatism ( 3-13 Ma) largely masks the initial seafloor spreading fabric. The resulting post-spreading seamounts are more numerous in the northern part than in the southern part of the East sub-<span class="hlt">basin</span>. In the eastern part of the East sub-<span class="hlt">basin</span>, the post-spreading volcanic ridge (PSVR) is approximately N055° oriented and follows the extinct spreading ridge (ESR). In the western part of the East sub-<span class="hlt">basin</span>, the PSVR, called the Zhenbei-Huangyan seamounts chain, is E-W oriented and hides the ESR (Sibuet et al., 2016). We conducted a seismic refraction survey covering both the Zhenbei-Huangyan seamount chain and the location of the <span class="hlt">adjacent</span> ESR. Three E-W oriented profiles and one N-S oriented profile are parallel and perpendicular to the Zhenbei-Huangyan seamounts chain, respectively. Our research is focused on the understanding of the relationship between the crustal thicknesses and crustal seismic velocities. The detailed velocity structure shows that the Zhenbei-Huangyan seamount chain was emplaced through a typical <span class="hlt">oceanic</span> crust. Crustal thicknesses and seismic velocities suggest an asymmetric generation of seamounts in the East sub-<span class="hlt">basin</span>, where active upwelling mantle (Holbrook et al., 2001) or buoyancy-driven decompression melting happened (Castillo et al., 2010). The Zhenbei and Huangyan seamounts were probably formed 3-5 Ma and 7-9 Ma, after seafloor spreading cessation; their thickened lower crusts were probably due to magmatic intrusions associated with a high-velocity layer (7.4-7.6 km/s),and their large thickness of upper crust were mainly due to volcanic extrusions. These two seamounts presents a different structural orientation and their crustal thicknesses are different, suggesting an independent origin for their magmatic feeding. This research was granted by the Natural Science Foundation of China (91428204, 91028002, 41176053).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996PalOc..11..579S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996PalOc..11..579S"><span>Can increased poleward <span class="hlt">oceanic</span> heat flux explain the warm Cretaceous climate?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmidt, Gavin A.; Mysak, Lawrence A.</p> <p>1996-10-01</p> <p>The poleward transport of heat in the mid-Cretaceous (100 Ma) is examined using an idealized coupled <span class="hlt">ocean</span>-atmosphere model. The <span class="hlt">oceanic</span> component consists of two zonally averaged <span class="hlt">basins</span> representing the proto-Pacific and proto-Indian <span class="hlt">oceans</span> and models the dynamics of the meridional thermohaline circulation. The atmospheric component is a simple energy and moisture balance model which includes the diffusive meridional transport of sensible heat and moisture. The <span class="hlt">ocean</span> model is spun up with a variety of plausible Cretaceous surface temperature and salinity profiles, and a consistent atmosphere is objectively derived based on the resultant sea surface temperature and the surface heat and freshwater fluxes. The coupled model does not exhibit climate drift. Multiple equilibria of the coupled model are found that break the initial symmetry of the <span class="hlt">ocean</span> circulation; several of these equilibria have one-cell (northern or southern sinking) thermohaline circulation patterns. Two main classes of circulation are found: circulations where the densest water is relatively cool and is formed at the polar latitudes and circulations where the densest water is warm, but quite saline, and the strongest sinking occurs at the tropics. In all cases, significant amounts of warm, saline bottom water are formed in the proto-Indian <span class="hlt">basin</span> which modify the deepwater characteristics in the larger (proto-Pacific) <span class="hlt">basin</span>. Temperatures in the deep <span class="hlt">ocean</span> are warm, 10°-17°C, in agreement with benthic foraminiferal oxygen isotope data. The poleward transport of heat in the modeled Cretaceous <span class="hlt">oceans</span> is larger than in some comparable models of the present day thermohaline circulation and significantly larger than estimates of similar processes in the present-day <span class="hlt">ocean</span>. It is consistently larger in the polar sinking cases when compared with that seen in the tropical sinking cases, but this represents an increase of only 10%. The largest increase over present-day model transports is in the atmospheric</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1113178S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1113178S"><span>300 million years of <span class="hlt">basin</span> evolution - the thermotectonic history of the Ukrainian Donbas Foldbelt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Spiegel, C.; Danisik, M.; Sachsenhofer, R.; Frisch, W.; Privalov, V.</p> <p>2009-04-01</p> <p>The Ukrainian-Russian Pripyat-Dniepr-Donets <span class="hlt">Basin</span> is a large intracratonic rift structure formed during the Late Devonian. It is situated at the southern margin of the Precambrian East European Craton, <span class="hlt">adjacent</span> to the Hercynian Tethyan belt in the Black Sea area and the Alpine Caucasus orogen. With a sediment thickness of more than 20 km, it is one of the deepest sedimentary <span class="hlt">basins</span> on earth. The eastern part of the Pripyat-Dniepr-Donets <span class="hlt">Basin</span> - called Donbas foldbelt - is strongly folded and inverted. Proposed models of <span class="hlt">basin</span> evolution are often controversial and numerous issues are still a matter of speculation, particularly the erosion history and the timing of <span class="hlt">basin</span> inversion. <span class="hlt">Basin</span> inversion may have taken place during the Permian related to the Uralian orogeny, or in response to Alpine tectonics during the Late Cretaceous to Early Tertiary. We investigated the low-temperature thermal history of the Donbas Foldbelt and the <span class="hlt">adjacent</span> Ukrainian shield by a combination of zircon fission track, apatite fission track and apatite (U-Th)/He thermochronology. Although apatite fission track ages of all sedimentary samples were reset shortly after deposition during the Carboniferous, we took advantage of the fact that samples contained kinetically variable apatites, which are sensitive to different temperatures. By using statistic-based component analysis incorporating physical properties of individual grains we identified several distinct age population, ranging from late Permian (~265 Ma) to the Late Cretaceous (70 Ma). We could thus constrain the thermal history of the Donbas Foldbelt and the <span class="hlt">adjacent</span> basement during a ~300 Myr long time period. The Precambrian crystalline basement of the Ukrainian shield was affected by a Permo-Triassic thermal event associated with magmatic activity, which also strongly heated the sediments of the Donbas Foldbelt. The basement rocks cooled to near-surface conditions during the Early to Middle Triassic and since then was thermally</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2007/1273/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2007/1273/"><span>Water-Level Data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">Adjacent</span> Areas, Central New Mexico, Period of Record Through September 30, 2006</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2007-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25 to 40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompass the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> are currently (2007) obtained solely from ground-water resources. An increase of about 20 percent in the population from 1990 to 2000 also resulted in an increased demand for water. From April 1982 through September 1983, a network of wells was established to monitor changes in ground-water levels throughout the <span class="hlt">basin</span>. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly. Currently (2007), the network consists of 133 wells and piezometers. This report presents water-level data collected by U.S. Geological Survey personnel at 133 sites through 2007.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/22339','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/22339"><span>Study plan for the regional aquifer-system analysis of alluvial <span class="hlt">basins</span> in south-central Arizona and <span class="hlt">adjacent</span> states</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Anderson, T.W.</p> <p>1980-01-01</p> <p>The U.S. Geological Survey has started a 4-year study of the alluvial <span class="hlt">basins</span> in south-central Arizona and parts of California , Nevada, and New Mexico to describe the hydrologic setting, available groundwater resources, and effects of historical development on the groundwater system. To aid in the study, mathematical models of selected <span class="hlt">basins</span> will be developed for appraising local and regional flow systems. Major components necessary to accomplish the study objectives include the accumulation of existing data on groundwater quantity and quality, entering the data into a computer file, identification of data deficiencies, and development of a program to remedy the deficiencies by collection of additional data. The approach to the study will be to develop and calibrate models of selected <span class="hlt">basins</span> for which sufficient data exist and to develop interpretation-transfer techniques whereby general predevelopment and postdevelopment conceptual models of the hydrologic system in other <span class="hlt">basins</span> may be synthesized. The end result of the project will be a better definition of the hydrologic parameters and a better understanding of the workings of the hydrologic system. The models can be used to study the effects of management alternatives and water-resources development on the system. (USGS)</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMEP51D..03V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMEP51D..03V"><span>River fluxes to the sea from the <span class="hlt">ocean</span>'s 10Be/9Be ratio</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>von Blanckenburg, F.; Bouchez, J.</p> <p>2013-12-01</p> <p>The ratio of the meteoric cosmogenic radionuclide 10Be to the stable isotope 9Be is proposed here to be a flux proxy of terrigenous input into the <span class="hlt">oceans</span>. The <span class="hlt">ocean</span>'s dissolved 10Be/9Be is set by (1) the flux of meteoric 10Be produced in the atmosphere; (2) the denudational flux of the rivers discharging into a given <span class="hlt">ocean</span> <span class="hlt">basin</span>; (3) the fraction of 9Be that is released from primary minerals during weathering (meaning the 9Be transported by rivers in either the dissolved form or adsorbed onto sedimentary particles and incorporated into secondary oxides); and (4) the fraction of riverine 10Be and 9Be actually released into seawater. Using published 10Be/9Be data of rivers for which independent denudation rate estimates exist we first find that the global average fraction of 9Be released during weathering into river waters and their particulate load is 20% and does not depend on denudation rate. We then evaluate this quantitative denudation rate proxy by using published dissolved seawater Be isotope data and a compilation of global river loads (15Gt/yr). We find that the measured global average <span class="hlt">oceanic</span> dissolved 10Be/9Be ratio of about 0.9E-7 is satisfied by the mass balance if only 6.5% of the dissolved and reactive riverine Be is eventually released to the open <span class="hlt">ocean</span> by boundary exchange. Except for the South Atlantic and the South Pacific, in which the 10Be/9Be ratio is dominated by Be advected through <span class="hlt">ocean</span> circulation, good agreement results between 10Be/9Be ratios predicted by denudation rates and measured <span class="hlt">ocean</span> 10Be/9Be ratios when we establish this mass balance for individual <span class="hlt">ocean</span> <span class="hlt">basins</span>. As the seawater 10Be/9Be ratio is faithfully recorded in marine chemical precipitates the 10Be/9Be ratio extracted from authigenic sediments can now serve to estimate relative changes in terrigenous input into the <span class="hlt">oceans</span> back through time on a global and on a <span class="hlt">basin</span> scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1911281R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1911281R"><span>Folding and fracturing of rock <span class="hlt">adjacent</span> to salt diapirs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rowan, Mark G.</p> <p>2017-04-01</p> <p>When John Ramsay wrote his groundbreaking book in 1967, deformation around salt diapirs was not something he covered. At the time, most geologists considered diapirs to form due to density inversion, rising through thick overlying strata due to buoyancy. In doing so, salt was thought to shove aside the younger rocks, shearing and fracturing them in drag folds and supposedly producing "salt gouge". Even after it was realized that the majority of diapirs spend most of their history growing at or just beneath the surface, the relative rise of salt and sinking of minibasins were (and are) still thought by many to be accommodated in part by shear and fracturing of rocks in a collar zone around the salt. There are two arguments against this model. The first is mechanical: whereas halite behaves as a viscous fluid, even young sediment deforms as a brittle material with layer anisotropy. Thus, the salt-sediment interface is the outer margin of an intrasalt shear zone caused by viscous drag against the diapir margin. The velocity of salt flow decreases dramatically toward the edge of the diapir, so that the outermost salt effectively doesn't move. Hence, no shear or fracturing is expected in surrounding strata. The second and more important argument is that empirical field data do not support the idea of drag folds and associated deformation. Certainly, strata are typically folded and thinned <span class="hlt">adjacent</span> to diapirs. However, stratal upturn is generated by monoclinal drape folding of the diapir roof over the edge of the rising salt, and thinning is caused by deposition onto the bathymetric highs formed by the diapirs, often supplemented by roof erosion and slumping. Halokinetic sequences observed in numerous salt <span class="hlt">basins</span> (e.g., Paradox <span class="hlt">Basin</span>, La Popa <span class="hlt">Basin</span>, Spanish Pyrenees, Sivas <span class="hlt">Basin</span>, Zagros Mountains, Kuqa <span class="hlt">Basin</span>) contain no diapir-parallel shear zones and minimal thinning and fracturing caused by diapir rise. Even megaflaps, in which strata extend for kilometers up the sides</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('http://adsabs.harvard.edu/abs/2012AGUFM.G33A0946P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.G33A0946P"><span>Modes of Arctic <span class="hlt">Ocean</span> Change from GRACE, ICESat and the PIOMAS and ECCO2 Models of the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peralta Ferriz, C.; Morison, J. H.; Bonin, J. A.; Chambers, D. P.; Kwok, R.; Zhang, J.</p> <p>2012-12-01</p> <p>EOF analysis of month-to-month variations in GRACE derived Arctic <span class="hlt">Ocean</span> bottom pressure (OBP) with trend and seasonal variation removed yield three dominant modes. The first mode is a <span class="hlt">basin</span> wide variation in mass associated with high atmospheric pressure (SLP) over Scandinavia mainly in winter. The second mode is a shift of mass from the central Arctic <span class="hlt">Ocean</span> to the Siberian shelves due to low pressure over the <span class="hlt">basins</span>, associated with the Arctic Oscillation. The third mode is a shift in mass between the Eastern and Western Siberian shelves, related to strength of the Beaufort High mainly in summer, and to eastward alongshore winds on the Barents Sea in winter. The PIOMAS and ECCO2 modeled OBP show fair agreement with the form of these modes and provide context in terms of variations in sea surface height SSH. Comparing GRACE OBP from 2007 to 2011 with GRACE OBP from 2002 to 2006 reveals a rising trend over most of the Arctic <span class="hlt">Ocean</span> but declines in the Kara Sea region and summer East Siberian Sea. ECCO2 bears a faint resemblance to the observed OBP change but appears to be biased negatively. In contrast, PIOMAS SSH and ECCO2 especially, show changes between the two periods that are muted but similar to ICESat dynamic <span class="hlt">ocean</span> topography and GRACE-ICESat freshwater trends from 2005 through 2008 [Morison et al., 2012] with a rising DOT and freshening in the Beaufort Sea and a trough with decreased freshwater on the Russian side of the Arctic <span class="hlt">Ocean</span>. Morison, J., R. Kwok, C. Peralta-Ferriz, M. Alkire, I. Rigor, R. Andersen, and M. Steele (2012), Changing Arctic <span class="hlt">Ocean</span> freshwater pathways, Nature, 481(7379), 66-70.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004GMS...149.....C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004GMS...149.....C"><span>Continent-<span class="hlt">Ocean</span> Interactions Within East Asian Marginal Seas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clift, Peter; Kuhnt, Wolfgang; Wang, Pinxian; Hayes, Dennis</p> <p></p> <p>The study of the complex interactions between continents and <span class="hlt">oceans</span> has become a leading area for 21st century earth cience. In this volume, continent—<span class="hlt">ocean</span> interactions in tectonics, arc-continent collision, sedimentology, and climatic volution within the East Asian Marginal Seas take precedence. Links between <span class="hlt">oceanic</span> and continental climate, the sedimentology of coastal and shelf areas, and the links between deformation of continental and <span class="hlt">oceanic</span> lithosphere are also discussed. As an introduction to the science presented throughout the volume, Wang discusses many of the possible interactions between the tectonic evolution of Asia and both regional and global climate. He speculates that uplift of central Asia in the Pliocene may have triggered the formation of many of the major rivers that drain north through Siberia into the Arctic <span class="hlt">Ocean</span>. He also argues that it is the delivery of this fresh water that allows the formation of sea ice in that area and triggered the start of Northern Hemispheric glaciation. This may be one of the most dramatic ways in which Asia has shaped the Earth's climate and represents an alternative to the other competing models that have previously emphasized the role of <span class="hlt">oceanic</span> gateway closure in Central America. Moreover, his proposal for major uplift of at least part of Tibet and Mongolia as late as the Pliocene, based on the history of drainage evolution in Siberia, supports recent data from the southern Tarim <span class="hlt">Basin</span> and from the Qilian Shan and Qaidam and Jiuxi <span class="hlt">Basins</span> in northeast Tibet that indicate surface uplift at that time. Constraining the timing and patterns of Tibetan surface uplift is crucial to testing competing models for strain accommodation in Asia following India—Asia collision.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...516770F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...516770F"><span>Trends of pH decrease in the Mediterranean Sea through high frequency observational data: indication of <span class="hlt">ocean</span> acidification in the <span class="hlt">basin</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flecha, Susana; Pérez, Fiz F.; García-Lafuente, Jesús; Sammartino, Simone; Ríos, Aida. F.; Huertas, I. Emma</p> <p>2015-11-01</p> <p>A significant fraction of anthropogenic carbon dioxide (CO2) released to the atmosphere is absorbed by the <span class="hlt">oceans</span>, leading to a range of chemical changes and causing <span class="hlt">ocean</span> acidification (OA). Assessing the impact of OA on marine ecosystems requires the accurate detection of the rate of seawater pH change. This work reports the results of nearly 3 years of continuous pH measurements in the Mediterranean Sea at the Strait of Gibraltar GIFT time series station. We document a remarkable decreasing annual trend of -0.0044 ± 0.00006 in the Mediterranean pH, which can be interpreted as an indicator of acidification in the <span class="hlt">basin</span> based on high frequency records. Modeling pH data of the Mediterranean outflow allowed to discriminate between the pH values of its two main constituent water masses, the Levantine Intermediate Water (LIW) and the Western Mediterranean Deep Water (WMDW). Both water masses also exhibited a decline in pH with time, particularly the WMDW, which can be related to their different biogeochemical nature and processes occurring during transit time from formation sites to the Strait of Gibraltar.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2006/1342/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2006/1342/"><span>Response to memorandum by Rowley and Dixon regarding U.S. Geological Survey report titled "Characterization of Surface-Water Resources in the Great <span class="hlt">Basin</span> National Park Area and Their Susceptibility to Ground-Water Withdrawals in <span class="hlt">Adjacent</span> Valleys, White Pine County, Nevada"</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Prudic, David E.</p> <p>2006-01-01</p> <p>Applications pending for permanent permits to pump large quantities of ground water in Spring and Snake Valleys <span class="hlt">adjacent</span> to Great <span class="hlt">Basin</span> National Park (the Park) prompted the National Park Service to request a study by the U.S. Geological Survey to evaluate the susceptibility of the Park's surface-water resources to pumping. The result of this study was published as U.S. Geological Survey Scientific Investigations Report 2006-5099 'Characterization of Surface-Water Resources in the Great <span class="hlt">Basin</span> National Park Area and Their Susceptibility to Ground-Water Withdrawals in <span class="hlt">Adjacent</span> Valleys, White Pine County, Nevada,' by P.E. Elliott, D.A. Beck, and D.E. Prudic. That report identified areas within the Park where surface-water resources are susceptible to ground-water pumping; results from the study showed that three streams and several springs near the eastern edge of the Park were susceptible. However, most of the Park's surface-water resources likely would not be affected by pumping because of either low-permeability rocks or because ground water is sufficiently deep as to not be directly in contact with the streambeds. A memorandum sent by Peter D. Rowley and Gary L. Dixon, Consulting Geologists, to the Southern Nevada Water Authority (SNWA) on June 29, 2006 was critical of the report. The memorandum by Rowley and Dixon was made available to the National Park Service, the U.S. Geological Survey, and the public during the Nevada State Engineer's 'Evidentiary Exchange' process for the recent hearing on applications for ground-water permits by SNWA in Spring Valley <span class="hlt">adjacent</span> to Great <span class="hlt">Basin</span> National Park. The U.S. Geological Survey was asked by the National Park Service to assess the validity of the concerns and comments contained in the Rowley and Dixon memorandum. An Administrative Letter Report responding to Rowley and Dixon's concerns and comments was released to the National Park Service on October 30, 2006. The National Park Service subsequently requested that the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.7172H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.7172H"><span>Bio- and chemostratigraphy of the Early Aptian <span class="hlt">Oceanic</span> Anoxic Event 1a within the mid-latitudes of northwest Europe (Germany, Lower Saxony <span class="hlt">Basin</span>)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heldt, Matthias; Mutterlose, Joerg; Berner, Uli; Erbacher, Jochen</p> <p>2013-04-01</p> <p>The Mid-Cretaceous period was characterised by a series of prominent anoxic events, one of these was the late Early Aptian <span class="hlt">Oceanic</span> Anoxic Event 1a (OAE 1a). The Fischschiefer horizon is the regional sedimentary expression of this event in a small epicontinental sea in northwest Europe (Germany, Lower Saxony <span class="hlt">Basin</span>). In the present study, two sediment cores of Lower to Upper Aptian age (Hoheneggelsen KB 9 and 40) from the Brunswick area, north Germany, have been investigated in detail with respect to their lithostratigraphy, geochemistry (CaCO3, TOC), biostratigraphy (coccoliths, nannoliths) and high-resolution chemostratigraphy (^13Ccarb and ^13Corg). Together with separately published new planktonic foraminifer data of the cores it was possible to establish a detailed time frame and to recognise the OAE 1a. The ^13C data enabled us to subdivide the deposits into isotope segments (C2-C7), which are commonly used as stratigraphic markers in coeval sediments around the world. The carbon isotope curves are compared to recently published Aptian curves from other parts of the Lower Saxony <span class="hlt">Basin</span>, all of which record the prominent carbon isotope anomaly of the OAE 1a. A high-resolution correlation of the typical isotope trends of OAE 1a (segments C3-6) across the Lower Saxony <span class="hlt">Basin</span> appears difficult due to an early diagenetic overprint of the primary isotope signal. These alterations can be explained by the temporary establishment of euxinic conditions the Lower Saxony <span class="hlt">Basin</span> during OAE 1a as consequence of an interplay of different factors, such as global warming, restricted palaeogeography, increased fluvial input and intensified stable water stratification, which is supported by several lines of regional evidence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914241S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914241S"><span>Contrasting <span class="hlt">basin</span> architecture and rifting style of the Vøring <span class="hlt">Basin</span>, offshore mid-Norway and the Faroe-Shetland <span class="hlt">Basin</span>, offshore United Kingdom</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schöpfer, Kateřina; Hinsch, Ralph</p> <p>2017-04-01</p> <p>The Vøring and the Faroe-Shetland <span class="hlt">basins</span> are offshore deep sedimentary <span class="hlt">basins</span> which are situated on the outer continental margin of the northeast Atlantic <span class="hlt">Ocean</span>. Both <span class="hlt">basins</span> are underlain by thinned continental crust whose structure is still debated. In particular the nature of the lower continental crust and the origin of high velocity bodies located at the base of the lower crust are a subject of discussion in recent literature. Regional interpretation of 2D and 3D seismic reflection data, combined with well data, suggest that both <span class="hlt">basins</span> share several common features: (i) Pre-Cretaceous faults that are distributed across the entire <span class="hlt">basin</span> width. (ii) Geometries of pre-Jurassic strata reflecting at least two extensional phases. (iii) Three common rift phases, Late Jurassic, Campanian-Maastrichtian and Palaeocene. (iv) Large pre-Cretaceous fault blocks that are buried by several kilometres of Cretaceous and Cenozoic strata. (iii). (v) Latest Cretaceous/Palaeocene inversion. (vi) Occurrence of partial mantle serpentinization during Early Cretaceous times, as proposed by other studies, seems improbable. The detailed analysis of the data, however, revealed significant differences between the two <span class="hlt">basins</span>: (i) The Faroe-Shetland <span class="hlt">Basin</span> was a fault-controlled <span class="hlt">basin</span> during the Late Jurassic but also the Late Cretaceous extensional phase. In contrast, the Vøring <span class="hlt">Basin</span> is dominated by the late Jurassic rifting and subsequent thermal subsidence. It exhibits only minor Late Cretaceous faults that are localised above intra-<span class="hlt">basinal</span> and marginal highs. In addition, the Cretaceous strata in the Vøring <span class="hlt">Basin</span> are folded. (ii) In the Vøring <span class="hlt">Basin</span>, the locus of Late Cretaceous rifting shifted westwards, affecting mainly the western <span class="hlt">basin</span> margin, whereas in the Faroe-Shetland <span class="hlt">Basin</span> Late Cretaceous rifting was localised in the same area as the Late Jurassic phase, hence masking the original Jurassic geometries. (iii) Devono-Carboniferous and Aptian/Albian to Cenomanian rift phases</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRG..121.1468V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRG..121.1468V"><span>Influences of riverine and upwelling waters on the coastal carbonate system off Central Chile and their <span class="hlt">ocean</span> acidification implications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vargas, Cristian A.; Contreras, Paulina Y.; Pérez, Claudia A.; Sobarzo, Marcus; Saldías, Gonzalo S.; Salisbury, Joe</p> <p>2016-06-01</p> <p>A combined data set, combining data from field campaigns and oceanographic cruises, was used to ascertain the influence of both river discharges and upwelling processes, covering spatial and temporal variation in dissolved inorganic carbon (DIC) and aragonite saturation state. This work was conducted in one of the most productive river-influenced upwelling areas in the South Pacific coasts (36°S). Additionally, further work was also conducted to ascertain the contribution of different DIC sources, influencing the dynamics of DIC along the land-<span class="hlt">ocean</span> range. Six sampling campaigns were conducted across seven stations at the Biobío River <span class="hlt">basin</span>, covering approximately 200 km. Three research cruises were undertaken simultaneously, covering the <span class="hlt">adjacent</span> continental shelf, including 12 sampling stations for hydrographic measurements. Additionally, six stations were also sampled for chemical analyses, covering summer, winter, and spring conditions over 2010 and 2011. Our results evidenced that seaward extent of the river plume was more evident during the winter field campaign, when highest riverine DIC fluxes were observed. The carbonate system along the river-<span class="hlt">ocean</span> continuum was very heterogeneous varying over spatial and temporal scales. High DIC and pCO2 were observed in river areas with larger anthropogenic effects. CO2 supersaturation at the river plume was observed during all campaigns due to the influence of low pH river waters in winter/spring and high-pCO2 upwelling waters in summer. δ13CDIC evidenced that main DIC sources along the river and river plume corresponded to the respiration of terrestrial organic matter. We have linked this natural process to the carbonate saturation on the <span class="hlt">adjacent</span> river-influenced coastal area, suggesting that Ωaragonite undersaturation in surface/subsurface waters is largely modulated by the influence of both river discharge and coastal upwelling events in this productive coastal area. Conditions of low Ωaragonite might impact</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.T43H..05D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.T43H..05D"><span>Early Opening of Seychelles and India: the Gop <span class="hlt">Basin</span> Revisited</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dyment, J.; Vadakkeyakath, Y.; Bhattacharya, G.</p> <p>2012-12-01</p> <p>The deep offshore region located between the India-Pakistan continental margin and the Laxmi Ridge continental sliver contains valuable imprints of the early <span class="hlt">oceanic</span> opening phase between India and the Seychelles. The acquisition of wide-angle deep seismic data by British scientists in 2003 provided new information about the deep structure and nature of the crust [1,2]. These data complement the large amount of seismic reflection profiles, altimetry-derived gravity and marine magnetic data which allow mapping the structure and determining the age of the <span class="hlt">oceanic</span> crust [3,4,5]. Although these authors all agree on the <span class="hlt">oceanic</span> nature of the Gop <span class="hlt">Basin</span>, they surprisingly differ on the extent of the <span class="hlt">oceanic</span> crust, the location of the extinct spreading center and the age of the <span class="hlt">basin</span>. Here we re-evaluate published interpretations of the Gop <span class="hlt">Basin</span> in light of all available data. The major discrepancy between [1,2,4] and [5] is the location of the extinct spreading center. [1,2,4] place it on an unnamed basement high located at 19°55'N, whereas [5] identify it with the Palitana Ridge at 19°25'N. Checking the location of the basement high of [1,2,4] on the basement isobath map of [3], based on many seismic reflection profiles, reveals that this basement high actually is an isolated feature of limited extent, which at best can be considered as part of a NE-SW trending basement high zone. This basement high locally coincides with a strong positive magnetic anomaly and a narrow gravity anomaly low but the trend of these anomalies is E-W, in contrast to the NE-SW trend of the basement in this area. For these reasons, this basement high probably is not the location of the Gop <span class="hlt">Basin</span> extinct spreading center. Conversely, on the basement isobath map of [3], the Palitana Ridge appears as a prominent E-W high, located in the middle of a broad E-W graben, the Gop <span class="hlt">Basin</span>. It extends over 200 km and is flanked on both sides by basement 2000 m deeper. On free air gravity anomaly maps, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27..229K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27..229K"><span>Earth: Physico-mathematical Meaning of "primary" and "secondary" <span class="hlt">Oceans</span> Conception</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kochemasov, G.</p> <p></p> <p>Geologists term the Pacific <span class="hlt">ocean</span> "primary" and Atlantic and Indian <span class="hlt">oceans</span> "sec- ondary" meaning that the first is larger, deeper, older (?) and plays more fundamental role in the Earth's tectonics. The wave planetology as hierarchically higher than geol- ogy (Earth is only one of planets and of many celestial bodies), states that all celestial bodies are dichotomic ( "Pacific" as a tectonic feature is found in any celestial body) and sectoral (i.g., the Arctic-Antarctic symptom is also in any body) (Theorems 1, 2 [1]). The tectonic dichotomy and sectoring are related to the first and second harmon- ica (wave1 and wave2) of warping standing waves appearing in any body just because they move in non-circular (elliptic, parabolic) orbits and hence inertia forces tend to distort original shapes. This disfiguring of a rotating body is not just a superficial fea- ture, it involves fundamental changes in the entire vertical section above and below surface rises and falls (Theorem 4 [1]). Here acts the law of angular momentum equi- libration. Thus, under the Pacific <span class="hlt">basin</span> hollow -the deepest hollow produced by wave1 - mantle is denser than under the Atlantic and Indian <span class="hlt">oceanic</span> <span class="hlt">basins</span> - <span class="hlt">basins</span> produced by wave2. We know it because squeezed out of mantle tholeiites in the mid-<span class="hlt">oceanic</span> ridges are Fe-richer in Pacific than in other <span class="hlt">oceans</span>. The "primary" <span class="hlt">ocean</span> is thus a fundamental or "wave1" or 2pR-structure. The "secondary" <span class="hlt">oceans</span> are "wave2" or pR-structures. pR-structures represented by continents, secondary <span class="hlt">oceans</span> and <span class="hlt">basins</span> and the "superswell" (Darwin rise) in the Pacific, i.e. by most important terrestrial lithospheric tectonic blocks, are distributed on the Earth's surface not randomly. As must be expected of the standing wave interference picture, the pR-structure pattern shows regular grouping around certain centres. There are 6 centres - vertices of an oc- tahedron occurring at equator (1, 2), tropics (3, 4) and polar circles (5, 6). They are: 1. New Guinea, 2</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981SeaF...27..300S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981SeaF...27..300S"><span>Turbines in the <span class="hlt">ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Smith, F. G. W.; Charlier, R. H.</p> <p>1981-10-01</p> <p>It is noted that the relatively high-speed <span class="hlt">ocean</span> currents flowing northward along the east coast of the U.S. may be able to supply a significant proportion of the future electric power requirements of urban areas. The Gulf Stream core lies only about 20 miles east of Miami; here its near-surface water reaches velocities of 4.3 miles per hour. Attention is called to the estimate that the energy available in the current of the Gulf Stream <span class="hlt">adjacent</span> to Florida is approximately equivalent to that generated by 25 1,000-megawatt power plants. It is also contended that this power could be produced at competitive prices during the 1980s using large turbines moored below the <span class="hlt">ocean</span> surface near the center of the Stream. Assuming an average <span class="hlt">ocean</span>-current speed between 4 and 5 knots at the current core, the power density of a hydroturbine could reach 410 watts per square foot, about 100 times that of a wind-driven device of similar scale operating in an airflow of approximately 11 knots.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70195226','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70195226"><span>Hydroclimatology of the Missouri River <span class="hlt">basin</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>Wise, Erika K.; Woodhouse, Connie A.; McCabe, Gregory; Pederson, Gregory T.; St. Jacques, Jeannine-Marie</p> <p>2018-01-01</p> <p>Despite the importance of the Missouri River for navigation, recreation, habitat, hydroelectric power, and agriculture, relatively little is known about the basic hydroclimatology of the Missouri River <span class="hlt">basin</span> (MRB). This is of particular concern given the droughts and floods that have occurred over the past several decades and the potential future exacerbation of these extremes by climate change. Here, observed and modeled hydroclimatic data and estimated natural flow records in the MRB are used to 1) assess the major source regions of MRB flow, 2) describe the climatic controls on streamflow in the upper and lower <span class="hlt">basins</span> , and 3) investigate trends over the instrumental period. Analyses indicate that 72% of MRB runoff is generated by the headwaters in the upper <span class="hlt">basin</span> and by the lowest portion of the <span class="hlt">basin</span> near the mouth. Spring precipitation and temperature and winter precipitation impacted by changes in zonal versus meridional flow from the Pacific <span class="hlt">Ocean</span> play key roles in surface water supply variability in the upper <span class="hlt">basin</span>. Lower <span class="hlt">basin</span> flow is significantly correlated with precipitation in late spring and early summer, indicative of Atlantic-influenced circulation variability affecting the flow of moisture from the Gulf of Mexico. Although increases in precipitation in the lower <span class="hlt">basin</span> are currently overriding the effects of warming temperatures on total MRB flow, the upper basin’s long-term trend toward decreasing flows, reduction in snow versus rain fraction, and warming spring temperatures suggest that the upper <span class="hlt">basin</span> may less often provide important flow supplements to the lower <span class="hlt">basin</span> in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SedG..261....1C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SedG..261....1C"><span>Identifying glacial influences on sedimentation in tectonically-active, mass flow dominated arc <span class="hlt">basins</span> with reference to the Neoproterozoic Gaskiers glaciation (c. 580 Ma) of the Avalonian-Cadomian Orogenic Belt</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carto, Shannon L.; Eyles, Nick</p> <p>2012-06-01</p> <p>Neoproterozoic 'Avalonian-Cadomian' volcanic arc <span class="hlt">basins</span> once lay peripheral to Gondwana and are now found around the North Atlantic <span class="hlt">Ocean</span> in New England, Atlantic Canada and northwestern Europe as 'peri-Gondwanan terranes.' Their thick (up to 9 km) marine fills are dominated by turbidites, debrites (diamictites and variably graded conglomerates), slumps and olistostromes recording the dominance of mass flow processes in arc <span class="hlt">basins</span> oversupplied with volcaniclastic sediment. Several diamictite horizons in these <span class="hlt">basins</span> were identified as glacial tillites more than one hundred years ago on the basis of poor textural sorting, and the lack of any understanding of mass flow processes. An association with thin-bedded turbidite facies, then interpreted as glaciolacustrine varvites, was seen as evidence for widespread glacial conditions which is still the basis today of a near global 'Gaskiers glaciation' at c. 580 Ma, despite classic sedimentological work which shows that the 'tillites' and 'varvites' of these <span class="hlt">basins</span> are deep marine sediment gravity flow deposits. Only in two <span class="hlt">basins</span> (Gaskiers Formation, Avalon Peninsula in Newfoundland, and the Konnarock Formation of Virginia) is a distal and regionally-restricted glacial influence on marine sedimentation identified from ice-rafted, striated dropstones in turbidites but terrestrial 'ice-contact' facies are absent. As revealed in this study, terrestrial glacial facies may not have survived frequent volcanic activity such as seen today on glaciated active plate margin volcanoes such as Mount Rainier in Washington USA, and Cotopaxi Volcano in Ecuador where primary glacial sediment is frequently reworked by lahars, pyroclastic flows, debris avalanches and outburst floods. The weight of evidence presented in this study indicates that ice covers during the Gaskiers glaciation were not widespread across the Avalonian-Cadomian back arc <span class="hlt">basins</span>; the deep marine Grenada <span class="hlt">Basin</span> (Caribbean Sea) filled with turbidites, debrites (lahars</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/dds/dds-069/dds-069-bb/+','USGSPUBS'); return false;" href="https://pubs.usgs.gov/dds/dds-069/dds-069-bb/+"><span>Oil shale resources of the Uinta <span class="hlt">Basin</span>, Utah and Colorado</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>2010-01-01</p> <p>The U.S. Geological Survey (USGS) recently completed a comprehensive assessment of in-place oil in oil shales of the Eocene Green River Formation of the Uinta <span class="hlt">Basin</span> of eastern Utah and western Colorado. The oil shale interval was subdivided into eighteen roughly time-stratigraphic intervals, and each interval was assessed for variations in gallons per ton, barrels per acre, and total barrels in each township. The Radial Basis Function extrapolation method was used to generate isopach and isoresource maps, and to calculate resources. The total inplace resource for the Uinta <span class="hlt">Basin</span> is estimated at 1.32 trillion barrels. This is only slightly lower than the estimated 1.53 trillion barrels for the <span class="hlt">adjacent</span> Piceance <span class="hlt">Basin</span>, Colorado, to the east, which is thought to be the richest oil shale deposit in the world. However, the area underlain by oil shale in the Uinta <span class="hlt">Basin</span> is much larger than that of the Piceance <span class="hlt">Basin</span>, and the average gallons per ton and barrels per acre values for each of the assessed oil shale zones are significantly lower in the depocenter in the Uinta <span class="hlt">Basin</span> when compared to the Piceance <span class="hlt">Basin</span>. These relations indicate that the oil shale resources in the Uinta <span class="hlt">Basin</span> are of lower grade and are more dispersed than the oil shale resources of the Piceance <span class="hlt">Basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.T52A..01V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.T52A..01V"><span>Diachronous demise of the Neotethys <span class="hlt">Ocean</span> as driver for non-cylindrical orogenesis in Anatolia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Van Hinsbergen, D. J. J.; Gurer, D.</p> <p>2017-12-01</p> <p>Continent-continent collision drives crustal deformation, topographic rise, and geodynamic change. Africa-Eurasia convergence accommodated in the Eastern Mediterranean involved subduction of the Neotethyan <span class="hlt">oceanic</span> lithosphere in Anatolia. Subduction was followed by collision of Greater Adria continental crust with Eurasia forming the Izmir-Ankara-Erzincan suture zone. Discerning the effects of this collision from pre-collisional ophiolite obduction-related orogeny of Greater Adria is notoriously difficult, and estimates from Central Anatolia based on a forearc-to-foreland <span class="hlt">basin</span> transition along the Eurasian margin suggest a 60 Ma initial collision. Here we assess whether this age is also representative for collision in eastern Anatolia across the Cenozoic Sivas <span class="hlt">basin</span> that straddles the Greater Adria-Europe suture by retro-deforming regional block rotations in the Pontides, Kırşehir and Taurides, building a first-order regional `block circuit' around the Sivas <span class="hlt">basin</span>. We show that up to 700 km of convergence must have been accommodated after central Anatolian Kırşehir-Pontide collision at 65-60 Ma across the Sivas <span class="hlt">Basin</span> - an order of magnitude more than estimated crustal shortening. We consequently infer that <span class="hlt">oceanic</span> subduction continued much longer in eastern Anatolia, perhaps into the Oligocene or beyond, demonstrating the a recently postulated greater paleogeographic width of the Neotethys in eastern Anatolia. Prolonged <span class="hlt">oceanic</span> subduction likely resulted from a paleogeography with a sharp kink in the former Kırşehir-Tauride passive margin. The strong non-cylindricity of the Anatolian collisional orogen is explained continued slab pull during ongoing <span class="hlt">oceanic</span> subduction in eastern Anatolia following central Anatolian collision.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/623/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/623/"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 2010</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2011-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25-40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompasses the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when surface water from the Rio Grande began being treated and integrated into the system. An increase of about 20 percent in the <span class="hlt">basin</span> human population from 1990 to 2000 and about a 22 percent increase from 2000 to 2010 also resulted in an increased demand for water. A network of wells was established by the U.S. Geological Survey in cooperation with the City of Albuquerque to monitor changes in groundwater levels throughout the <span class="hlt">basin</span> from April 1982 through September 1983. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2010), the network consists of 124 wells and piezometers (a piezometer is a small-diameter subwell usually nested within a larger well). To better help the Albuquerque Bernalillo County Water Utility Authority manage water use, this report presents water-level data collected by U.S. Geological Survey personnel at those 124 sites through water year 2010.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5070528','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5070528"><span>Arctic pathways of Pacific Water: Arctic <span class="hlt">Ocean</span> Model Intercomparison experiments</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Karcher, Michael; Proshutinsky, Andrey; Gerdes, Rüdiger; de Cuevas, Beverly; Golubeva, Elena; Kauker, Frank; Nguyen, An T.; Platov, Gennady A.; Wadley, Martin; Watanabe, Eiji; Coward, Andrew C.; Nurser, A. J. George</p> <p>2016-01-01</p> <p>Abstract Pacific Water (PW) enters the Arctic <span class="hlt">Ocean</span> through Bering Strait and brings in heat, fresh water, and nutrients from the northern Bering Sea. The circulation of PW in the central Arctic <span class="hlt">Ocean</span> is only partially understood due to the lack of observations. In this paper, pathways of PW are investigated using simulations with six state‐of‐the art regional and global <span class="hlt">Ocean</span> General Circulation Models (OGCMs). In the simulations, PW is tracked by a passive tracer, released in Bering Strait. Simulated PW spreads from the Bering Strait region in three major branches. One of them starts in the Barrow Canyon, bringing PW along the continental slope of Alaska into the Canadian Straits and then into Baffin Bay. The second begins in the vicinity of the Herald Canyon and transports PW along the continental slope of the East Siberian Sea into the Transpolar Drift, and then through Fram Strait and the Greenland Sea. The third branch begins near the Herald Shoal and the central Chukchi shelf and brings PW into the Beaufort Gyre. In the models, the wind, acting via Ekman pumping, drives the seasonal and interannual variability of PW in the Canadian <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span>. The wind affects the simulated PW pathways by changing the vertical shear of the relative vorticity of the <span class="hlt">ocean</span> flow in the Canada <span class="hlt">Basin</span>. PMID:27818853</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27818853','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27818853"><span>Arctic pathways of Pacific Water: Arctic <span class="hlt">Ocean</span> Model Intercomparison experiments.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aksenov, Yevgeny; Karcher, Michael; Proshutinsky, Andrey; Gerdes, Rüdiger; de Cuevas, Beverly; Golubeva, Elena; Kauker, Frank; Nguyen, An T; Platov, Gennady A; Wadley, Martin; Watanabe, Eiji; Coward, Andrew C; Nurser, A J George</p> <p>2016-01-01</p> <p>Pacific Water (PW) enters the Arctic <span class="hlt">Ocean</span> through Bering Strait and brings in heat, fresh water, and nutrients from the northern Bering Sea. The circulation of PW in the central Arctic <span class="hlt">Ocean</span> is only partially understood due to the lack of observations. In this paper, pathways of PW are investigated using simulations with six state-of-the art regional and global <span class="hlt">Ocean</span> General Circulation Models (OGCMs). In the simulations, PW is tracked by a passive tracer, released in Bering Strait. Simulated PW spreads from the Bering Strait region in three major branches. One of them starts in the Barrow Canyon, bringing PW along the continental slope of Alaska into the Canadian Straits and then into Baffin Bay. The second begins in the vicinity of the Herald Canyon and transports PW along the continental slope of the East Siberian Sea into the Transpolar Drift, and then through Fram Strait and the Greenland Sea. The third branch begins near the Herald Shoal and the central Chukchi shelf and brings PW into the Beaufort Gyre. In the models, the wind, acting via Ekman pumping, drives the seasonal and interannual variability of PW in the Canadian <span class="hlt">Basin</span> of the Arctic <span class="hlt">Ocean</span>. The wind affects the simulated PW pathways by changing the vertical shear of the relative vorticity of the <span class="hlt">ocean</span> flow in the Canada <span class="hlt">Basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070032962&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070032962&hterms=temperature+variability&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dtemperature%2Bvariability"><span>Intraseasonal Variability of the Equatorial Indian <span class="hlt">Ocean</span> Observed from Sea Surface Height, Wind, and Temperature Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Fu, Lee-Lueng</p> <p>2007-01-01</p> <p>The forcing of the equatorial Indian <span class="hlt">Ocean</span> by the highly periodic monsoon wind cycle creates many interesting intraseasonal variabilities. The frequency spectrum of the wind stress observations from the European Remote Sensing Satellite scatterometers reveals peaks at the seasonal cycle and its higher harmonics at 180, 120, 90, and 75 days. The observations of sea surface height (SSH) from the Jason and <span class="hlt">Ocean</span> Topography Experiment (TOPEX)/Poseidon radar altimeters are analyzed to study the <span class="hlt">ocean</span>'s response. The focus of the study is on the intraseasonal periods shorter than the annual period. The semiannual SSH variability is characterized by a <span class="hlt">basin</span> mode involving Rossby waves and Kelvin waves traveling back and forth in the equatorial Indian <span class="hlt">Ocean</span> between 10(deg)S and 10(deg)N. However, the interference of these waves with each other masks the appearance of individual Kelvin and Rossby waves, leading to a nodal point (amphidrome) of phase propagation on the equator at the center of the <span class="hlt">basin</span>. The characteristics of the mode correspond to a resonance of the <span class="hlt">basin</span> according to theoretical models. The theory also calls for similar modes at 90 and 60 days.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920060800&hterms=drilling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddrilling','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920060800&hterms=drilling&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddrilling"><span>Petrology of basaltic sills from <span class="hlt">ocean</span> drilling program sites 794 and 797 in the Yamato <span class="hlt">Basin</span> of the Japan Sea</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thy, P.</p> <p>1992-01-01</p> <p>The basaltic sills from <span class="hlt">ocean</span> drilling program sites 794 and 797 in the Yamato <span class="hlt">Basin</span> of the Japan Sea are characterized petrographically on the basis of a detailed study of the composition of relict phenocryst and groundmass phases. The systematic variation in the rock compositions is discussed. Results of 1-atm melting experiments on a relatively primitive basalt from site 797 are reported. The sills are found to constitute two distinct groups of suites: primitive, olivine-bearing suites with low potassium and primitive olivine-bearing to evolved, olivine-free suites with relatively high potassium. A pseudoinvariant reaction relationship between olivine and augite and magnetite is inferred. Complex magmatic and tectonic evolutions in the region, perhaps reflecting a transitional stage between subduction zone activity and back arc spreading, are suggested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SciDr..22...49F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SciDr..22...49F"><span>IODP workshop: developing scientific drilling proposals for the Argentina Passive Volcanic Continental Margin (APVCM) - <span class="hlt">basin</span> evolution, deep biosphere, hydrates, sediment dynamics and <span class="hlt">ocean</span> evolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flood, Roger D.; Violante, Roberto A.; Gorgas, Thomas; Schwarz, Ernesto; Grützner, Jens; Uenzelmann-Neben, Gabriele; Hernández-Molina, F. Javier; Biddle, Jennifer; St-Onge, Guillaume; Workshop Participants, Apvcm</p> <p>2017-05-01</p> <p>The Argentine margin contains important sedimentological, paleontological and chemical records of regional and local tectonic evolution, sea level, climate evolution and <span class="hlt">ocean</span> circulation since the opening of the South Atlantic in the Late Jurassic-Early Cretaceous as well as the present-day results of post-depositional chemical and biological alteration. Despite its important location, which underlies the exchange of southern- and northern-sourced water masses, the Argentine margin has not been investigated in detail using scientific drilling techniques, perhaps because the margin has the reputation of being erosional. However, a number of papers published since 2009 have reported new high-resolution and/or multichannel seismic surveys, often combined with multi-beam bathymetric data, which show the common occurrence of layered sediments and prominent sediment drifts on the Argentine and <span class="hlt">adjacent</span> Uruguayan margins. There has also been significant progress in studying the climatic records in surficial and near-surface sediments recovered in sediment cores from the Argentine margin. Encouraged by these recent results, our 3.5-day IODP (International <span class="hlt">Ocean</span> Discovery Program) workshop in Buenos Aires (8-11 September 2015) focused on opportunities for scientific drilling on the Atlantic margin of Argentina, which lies beneath a key portion of the global <span class="hlt">ocean</span> conveyor belt of thermohaline circulation. Significant opportunities exist to study the tectonic evolution, paleoceanography and stratigraphy, sedimentology, and biosphere and geochemistry of this margin.</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4134232','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4134232"><span>Promiscuous Speciation with Gene Flow in Silverside Fish Genus Odontesthes (Atheriniformes, Atherinopsidae) from South Western Atlantic <span class="hlt">Ocean</span> <span class="hlt">Basins</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>García, Graciela; Ríos, Néstor; Gutiérrez, Verónica; Varela, Jorge Guerra; Bouza Fernández, Carmen; Pardo, Belén Gómez; Portela, Paulino Martínez</p> <p>2014-01-01</p> <p>The present paper integrates phylogenetic and population genetics analyses based on mitochondrial and nuclear molecular markers in silversides, genus Odontesthes, from a non-sampled area in the SW Atlantic <span class="hlt">Ocean</span> to address species discrimination and to define Managements Units for sustainable conservation. All phylogenetic analyses based on the COI mitochondrial gene were consistent to support the monophyly of the genus Odontesthes and to include O. argentinensis, O. perugiae-humensis and some O. bonariensis haplotypes in a basal polytomy conforming a major derivative clade. Microsatellites data revealed somewhat higher genetic variability values in the O. argentinensis-perugia populations than in O. bonariensis and O. perugia-humensis taxa. Contrasting population genetics structuring emerged from mitochondrial and microsatellites analyses in these taxa. Whereas mitochondrial data supported two major groups (O. argentinensis-perugia-humensis vs. O. bonariensis-perugiae-humensis populations), microsatellite data detected three major genetic entities represented by O. bonariensis, O. perugiae-humensis and an admixture of populations belonging to O. argentinensis-perugiae respectively. Therefore, the star COI polytomy in the tree topology involving these taxa could be interpreted by several hypothetic scenarios such as the existence of shared ancestral polymorphisms, incomplete lineage sorting in a radiating speciation process and/or reticulation events. Present findings support that promiscuous and recent contact between incipient species sharing asymmetric gene flow exchanges, blurs taxa boundaries yielding complicated taxonomy and Management Units delimitation in silverside genus Odontesthes from SW Atlantic <span class="hlt">Ocean</span> <span class="hlt">basins</span>. PMID:25126842</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25126842','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25126842"><span>Promiscuous speciation with gene flow in silverside fish genus Odontesthes (Atheriniformes, Atherinopsidae) from south western Atlantic <span class="hlt">Ocean</span> <span class="hlt">basins</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>García, Graciela; Ríos, Néstor; Gutiérrez, Verónica; Varela, Jorge Guerra; Bouza Fernández, Carmen; Pardo, Belén Gómez; Portela, Paulino Martínez</p> <p>2014-01-01</p> <p>The present paper integrates phylogenetic and population genetics analyses based on mitochondrial and nuclear molecular markers in silversides, genus Odontesthes, from a non-sampled area in the SW Atlantic <span class="hlt">Ocean</span> to address species discrimination and to define Managements Units for sustainable conservation. All phylogenetic analyses based on the COI mitochondrial gene were consistent to support the monophyly of the genus Odontesthes and to include O. argentinensis, O. perugiae-humensis and some O. bonariensis haplotypes in a basal polytomy conforming a major derivative clade. Microsatellites data revealed somewhat higher genetic variability values in the O. argentinensis-perugia populations than in O. bonariensis and O. perugia-humensis taxa. Contrasting population genetics structuring emerged from mitochondrial and microsatellites analyses in these taxa. Whereas mitochondrial data supported two major groups (O. argentinensis-perugia-humensis vs. O. bonariensis-perugiae-humensis populations), microsatellite data detected three major genetic entities represented by O. bonariensis, O. perugiae-humensis and an admixture of populations belonging to O. argentinensis-perugiae respectively. Therefore, the star COI polytomy in the tree topology involving these taxa could be interpreted by several hypothetic scenarios such as the existence of shared ancestral polymorphisms, incomplete lineage sorting in a radiating speciation process and/or reticulation events. Present findings support that promiscuous and recent contact between incipient species sharing asymmetric gene flow exchanges, blurs taxa boundaries yielding complicated taxonomy and Management Units delimitation in silverside genus Odontesthes from SW Atlantic <span class="hlt">Ocean</span> <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870022774&hterms=oceans+behavior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Doceans%2Bbehavior','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870022774&hterms=oceans+behavior&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Doceans%2Bbehavior"><span>TOPEX/POSEIDON - Mapping the <span class="hlt">ocean</span> surface</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yamarone, C. A.; Rosell, S.; Farless, D. L.</p> <p>1986-01-01</p> <p>Global efforts are under way to model the earth as a complete planet so that weather patterns may be predicted on time scales of months and years. A major limitation in developing models of global weather is the inability to model the circulation of the <span class="hlt">oceans</span> including the geostrophic surface currents. NASA will soon be initiating a satellite program to correct this deficiency by directly measuring these currents using the science of radar altimetry. Measurement of the <span class="hlt">ocean</span> topography with broad, frequent coverage of all <span class="hlt">ocean</span> <span class="hlt">basins</span> for a long period of time will allow the derivation of the spatial and temporal behavior of surface <span class="hlt">ocean</span> currents. The TOPEX/POSEIDON mission is a cooperative effort between NASA and the French Centre National d'Etudes Spatiales. This paper describes the goals of this research mission, the data type to be acquired, the satellite and sensors to be used to acquire the data, and the methods by which the data are to be processed and utilized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.1573J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.1573J"><span>Coupled ice sheet-<span class="hlt">ocean</span> modelling to investigate <span class="hlt">ocean</span> driven melting of marine ice sheets in Antarctica</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jong, Lenneke; Gladstone, Rupert; Galton-Fenzi, Ben</p> <p>2017-04-01</p> <p><span class="hlt">Ocean</span> induced melting below the ice shelves of marine ice sheets is a major source of uncertainty for predictions of ice mass loss and Antarctica's resultant contribution to future sea level rise. The floating ice shelves provide a buttressing force against the flow of ice across the grounding line into the <span class="hlt">ocean</span>. Thinning of these ice shelves due to an increase in melting reduces this force and can lead to an increase in the discharge of grounded ice. Fully coupled modelling of ice sheet-<span class="hlt">ocean</span> interactions is key to improving understanding the influence of the Southern <span class="hlt">ocean</span> on the evolution of the Antarctic ice sheet, and to predicting its future behaviour under changing climate conditions. Coupling of <span class="hlt">ocean</span> and ice sheet models is needed to provide more realistic melt rates at the base of ice shelves and hence make better predictions of the behaviour of the grounding line and the shape of the ice-shelf cavity as the ice sheet evolves. The Framework for Ice Sheet - <span class="hlt">Ocean</span> Coupling (FISOC) has been developed to provide a flexible platform for performing coupled ice sheet - <span class="hlt">ocean</span> modelling experiments. We present preliminary results using FISOC to couple the Regional <span class="hlt">Ocean</span> Modelling System (ROMS) with Elmer/Ice in idealised experiments Marine Ice Sheet-<span class="hlt">Ocean</span> Model Intercomparison Project (MISOMIP). These experiments use an idealised geometry motivated by that of Pine Island glacier and the <span class="hlt">adjacent</span> Amundsen Sea in West Antarctica, a region which has shown shown signs of thinning ice and grounding line retreat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70190201','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70190201"><span>Use of modflow drain package for simulating inter-<span class="hlt">basin</span> transfer in abandoned coal mines</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kozar, Mark D.; McCoy, Kurt J.</p> <p>2017-01-01</p> <p>Simulation of groundwater flow in abandoned mines is difficult, especially where flux to and from mines is unknown or poorly quantified, and inter-<span class="hlt">basin</span> transfer of groundwater occurs. A 3-year study was conducted in the Elkhorn area, West Virginia to better understand groundwater-flow processes and inter-<span class="hlt">basin</span> transfer in above drainage abandoned coal mines. The study area was specifically selected, as all mines are located above the elevation of tributary receiving streams, to allow accurate measurements of discharge from mine portals and tributaries for groundwater model calibration. Abandoned mine workings were simulated in several ways, initially as a layer of high hydraulic conductivity bounded by lower permeability rock in <span class="hlt">adjacent</span> strata, and secondly as rows of higher hydraulic conductivity embedded within a lower hydraulic conductivity coal aquifer matrix. Regardless of the hydraulic conductivity assigned to mine workings, neither approach to simulate mine workings could accurately reproduce the inter-<span class="hlt">basin</span> transfer of groundwater from <span class="hlt">adjacent</span> watersheds. To resolve the problem, a third approach was developed. The MODFLOW DRAIN package was used to simulate seepage into and through mine workings discharging water under unconfined conditions to Elkhorn Creek, North Fork, and tributaries of the Bluestone River. Drain nodes were embedded in a matrix of uniform hydraulic conductivity cells that represented the coal mine aquifer. Drain heads were empirically defined from well observations, and elevations were based on structure contours for the Pocahontas No. 3 mine workings. Use of the DRAIN package to simulate mine workings as an internal boundary condition resolved the inter-<span class="hlt">basin</span> transfer problem, and effectively simulated a shift from a topographic- dominated to a dip-dominated flow system, by dewatering overlying unmined strata and shifting the groundwater drainage divide up dip within the Pocahontas No. 3 coal seam several kilometers into the <span class="hlt">adjacent</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5559419','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5559419"><span>High-latitude <span class="hlt">ocean</span> ventilation and its role in Earth's climate transitions</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>MacGilchrist, Graeme A. ; Brown, Peter J.; Evans, D. Gwyn; Meijers, Andrew J. S.; Zika, Jan D.</p> <p>2017-01-01</p> <p>The processes regulating <span class="hlt">ocean</span> ventilation at high latitudes are re-examined based on a range of observations spanning all scales of <span class="hlt">ocean</span> circulation, from the centimetre scales of turbulence to the <span class="hlt">basin</span> scales of gyres. It is argued that high-latitude <span class="hlt">ocean</span> ventilation is controlled by mechanisms that differ in fundamental ways from those that set the overturning circulation. This is contrary to the assumption of broad equivalence between the two that is commonly adopted in interpreting the role of the high-latitude <span class="hlt">oceans</span> in Earth's climate transitions. Illustrations of how recognizing this distinction may change our view of the <span class="hlt">ocean</span>'s role in the climate system are offered. This article is part of the themed issue ‘<span class="hlt">Ocean</span> ventilation and deoxygenation in a warming world’. PMID:28784714</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880020841&hterms=continental+drift&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dcontinental%2Bdrift','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880020841&hterms=continental+drift&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dcontinental%2Bdrift"><span>The tectonic setting of the Seychelles, Mascarene and Amirante Plateaus in the Western Equatorial Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mart, Y.</p> <p>1988-01-01</p> <p>A system of marine plateaus occurs in the western equatorial Indian <span class="hlt">Ocean</span>, forming an arcuate series of wide and shallow banks with small islands in places. The <span class="hlt">oceanic</span> <span class="hlt">basins</span> that surround the Seychelles - Amirante region are of various ages and reflect a complex seafloor spreading pattern. The structural analysis of the Seychelle - Amirante - Mascarene region reflects the tectonic evolution of the western equatorial Indian <span class="hlt">Ocean</span>. It is suggested that due to the seafloor spreading during a tectonic stage, the Seychelles continental block drifted southwestwards to collide with the <span class="hlt">oceanic</span> crust of the Mascarene <span class="hlt">Basin</span>, forming an elongated folded structure at first, and then a subduction zone. The morphological similarity, the lithological variability and the different origin of the Seychelles Bank, the Mascarene Plateau and the Amirante Arc emphasizes the significant convergent effects of various plate tectonic processes on the development of marine plateaus.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28494402','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28494402"><span>Polycyclic aromatic hydrocarbons in <span class="hlt">ocean</span> sediments from the North Pacific to the Arctic <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ma, Yuxin; Halsall, Crispin J; Xie, Zhiyong; Koetke, Danijela; Mi, Wenying; Ebinghaus, Ralf; Gao, Guoping</p> <p>2017-08-01</p> <p>Eighteen polycyclic aromatic hydrocarbons (PAHs) were measured in surficial sediments along a marine transect from the North Pacific into the Arctic <span class="hlt">Ocean</span>. The highest average Σ 18 PAHs concentrations were observed along the continental slope of the Canada <span class="hlt">Basin</span> in the Arctic (68.3 ± 8.5 ng g -1 dw), followed by sediments in the Chukchi Sea shelf (49.7 ± 21.2 ng g -1 dw) and Bering Sea (39.5 ± 11.3 ng g -1 dw), while the Bering Strait (16.8 ± 7.1 ng g -1 dw) and Central Arctic <span class="hlt">Ocean</span> sediments (13.1 ± 9.6 ng g -1 dw) had relatively lower average concentrations. The use of principal components analysis with multiple linear regression (PCA/MLR) indicated that on average oil related or petrogenic sources contributed ∼42% of the measured PAHs in the sediments and marked by higher concentrations of two methylnaphthalenes over the non-alkylated parent PAH, naphthalene. Wood and coal combustion contributed ∼32%, and high temperature pyrogenic sources contributing ∼26%. Petrogenic sources, such as oil seeps, allochthonous coal and coastally eroded material such as terrigenous sediments particularly affected the Chukchi Sea shelf and slope of the Canada <span class="hlt">Basin</span>, while biomass and coal combustion sources appeared to have greater influence in the central Arctic <span class="hlt">Ocean</span>, possibly due to the effects of episodic summertime forest fires. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T51E2957Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T51E2957Z"><span>Large Sanjiang <span class="hlt">basin</span> groups outside of the Songliao <span class="hlt">Basin</span> Meso-Senozoic Tectonic-sediment evolution and hydrocarbon accumulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, M.; Wu, X.</p> <p>2015-12-01</p> <p>The basis geological problem is still the bottleneck of the exploration work of the lager Sanjiang <span class="hlt">basin</span> groups. In general terms, the problems are including the prototype <span class="hlt">basins</span> and <span class="hlt">basin</span> forming mechanism of two aspects. In this paper, using the field geological survey and investigation, logging data analysis, seismic data interpretation technical means large Sanjiang <span class="hlt">basin</span> groups and <span class="hlt">basin</span> forming mechanism of the prototype are discussed. Main draw the following conclusions: 1. Sanjiang region group-level formation can be completely contrasted. 2. Tension faults, compressive faults, shear structure composition and structure combination of four kinds of compound fracture are mainly developed In the study area. The direction of their distribution can be divided into SN, EW, NNE, NEE, NNW, NWW to other groups of fracture. 3. Large Sanjiang <span class="hlt">basin</span> has the SN and the EW two main directions of tectonic evolution. Cenozoic <span class="hlt">basins</span> in Sanjiang region in group formation located the two tectonic domains of ancient Paleo-Asian <span class="hlt">Ocean</span> and the Pacific Interchange. 4. Large Sanjiang <span class="hlt">basin</span> has experienced in the late Mesozoic tectonic evolution of two-stage and nine times. The first stage, developmental stage basement, they are ① Since the Mesozoic era and before the Jurassic; ② Early Jurassic period; The second stage, cap stage of development, they are ③ Late Jurassic depression developmental stages of compression; ④ Early Cretaceous rifting stage; ⑤ depression in mid-Early Cretaceous period; ⑥ tensile Early Cretaceous rifting stage; ⑦ inversion of Late Cretaceous tectonic compression stage; ⑧ Paleogene - Neogene; ⑨ After recently Ji Baoquan Sedimentary Ridge. 5. Large Sanjiang <span class="hlt">basin</span> group is actually a residual <span class="hlt">basin</span> structure, and Can be divided into left - superimposed (Founder, Tangyuan depression, Hulin <span class="hlt">Basin</span>), residual - inherited type (Sanjiang <span class="hlt">basin</span>), residual - reformed (Jixi, Boli, Hegang <span class="hlt">basin</span>). there are two developed depression and the mechanism</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/CFR-2010-title15-vol3/pdf/CFR-2010-title15-vol3-part922-subpartM-appD.pdf','CFR'); return false;" href="https://www.gpo.gov/fdsys/pkg/CFR-2010-title15-vol3/pdf/CFR-2010-title15-vol3-part922-subpartM-appD.pdf"><span>15 CFR Appendix D to Subpart M of... - Dredged Material Disposal Sites <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collectionCfr.action?selectedYearFrom=2010&page.go=Go">Code of Federal Regulations, 2010 CFR</a></p> <p></p> <p>2010-01-01</p> <p>... 15 Commerce and Foreign Trade 3 2010-01-01 2010-01-01 false Dredged Material Disposal Sites <span class="hlt">Adjacent</span> to the Monterey Bay National Marine Sanctuary D Appendix D to Subpart M of Part 922 Commerce and Foreign Trade Regulations Relating to Commerce and Foreign Trade (Continued) NATIONAL <span class="hlt">OCEANIC</span> AND...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFM.H31G1263I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFM.H31G1263I"><span>Use of radon-222 to evaluate the influence of groundwater discharge on fecal indicator bacteria concentrations in the near-shore <span class="hlt">ocean</span>, Malibu, California</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Izbicki, J. A.; Burton, C.; Swarzenski, P. W.</p> <p>2011-12-01</p> <p>To protect beach-goers from waterborne disease, California requires water-quality monitoring for fecal indicator bacteria (FIB) at beaches having more than 50,000 visits annually. The source(s) of FIB in <span class="hlt">ocean</span> beaches in excess of marine recreational water standards is often not known, or may be incorrectly identified. Onsite wastewater treatment systems (OWTS) used to treat residential and commercial sewage have been implicated by regulatory agencies as a possible source of FIB to recreational <span class="hlt">ocean</span> beaches, near Malibu, California. For this to occur, treated wastewater must first move through groundwater prior to discharge at the <span class="hlt">ocean</span>. Groundwater discharge to the <span class="hlt">ocean</span> near Malibu Lagoon (the estuary of Malibu Creek) is complicated by seasonally changing water levels in the lagoon. The lagoon is isolated from the <span class="hlt">ocean</span> by a sand berm that develops across the mouth of the lagoon during the dry season. Higher water levels in the lagoon during the dry season, and lower water-levels during the wet season, cause seasonal changes in the direction of groundwater flow and the magnitude of discharge from the <span class="hlt">adjacent</span> small (3,400 hectare), alluvial aquifer. Radon-222, an indicator of groundwater discharge, was measured in Malibu Lagoon, in the near-shore <span class="hlt">ocean</span> <span class="hlt">adjacent</span> to the lagoon, and in the near-shore <span class="hlt">ocean</span> <span class="hlt">adjacent</span> to unsewered residential development to determine the timing and magnitude of groundwater discharge. During the dry season, when the berm of the lagoon was closed and the lagoon was isolated from the <span class="hlt">ocean</span>, radon-222 concentrations in the near-shore <span class="hlt">ocean</span> during low tide increased as water discharged from the lagoon through the berm. Enterococcus concentrations in the near-shore <span class="hlt">ocean</span> increased to almost 600 Most Probable Number (MPN) per 100 milliliter at this time. Radon-222 concentrations also increased at low tide as groundwater discharged to the <span class="hlt">ocean</span> from the <span class="hlt">adjacent</span> alluvial aquifer underlying the unsewered residential development, but there was</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.7095O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.7095O"><span>Flow and transport within a coastal aquifer <span class="hlt">adjacent</span> to a stratified water body</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oz, Imri; Yechieli, Yoseph; Eyal, Shalev; Gavrieli, Ittai; Gvirtzman, Haim</p> <p>2016-04-01</p> <p>The existence of a freshwater-saltwater interface and the circulation flow of saltwater beneath the interface is a well-known phenomenon found at coastal aquifers. This flow is a natural phenomenon that occurs due to density differences between fresh groundwater and the saltwater body. The goals of this research are to use analytical, numerical, and physical models in order to examine the configuration of the freshwater-saltwater interface and the density-driven flow patterns within a coastal aquifer <span class="hlt">adjacent</span> to long-term stratified saltwater bodies (e.g. meromictic lake). Such hydrological systems are unique, as they consist of three different water types: the regional fresh groundwater, and low and high salinity brines forming the upper and lower water layers of the stratified water body, respectively. This research also aims to examine the influence of such stratification on hydrogeological processes within the coastal aquifer. The coastal aquifer <span class="hlt">adjacent</span> to the Dead Sea, under its possible future meromictic conditions, serves as an ideal example to examine these processes. The results show that <span class="hlt">adjacent</span> to a stratified saltwater body three interfaces between three different water bodies are formed, and that a complex flow system, controlled by the density differences, is created, where three circulation cells are developed. These results are significantly different from the classic circulation cell that is found <span class="hlt">adjacent</span> to non-stratified water bodies (lakes or <span class="hlt">oceans</span>). In order to obtain a more generalized insight into the groundwater behavior <span class="hlt">adjacent</span> to a stratified water body, we used the numerical model to perform sensitivity analysis. The hydrological system was found be sensitive to three dimensionless parameters: dimensionless density (i.e. the relative density of the three water bodies'); dimensionless thickness (i.e. the ratio between the relative thickness of the upper layer and the whole thickness of the lake); and dimensionless flux. The results</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Icar..293....8W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Icar..293....8W"><span>Long-lived volcanism within Argyre <span class="hlt">basin</span>, Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Williams, Jean-Pierre; Dohm, James M.; Soare, Richard J.; Flahaut, Jessica; Lopes, Rosaly M. C.; Pathare, Asmin V.; Fairén, Alberto G.; Schulze-Makuch, Dirk; Buczkowski, Debra L.</p> <p>2017-09-01</p> <p>The Argyre <span class="hlt">basin</span>, one of the largest impact structures on Mars with a diameter >1200 km, formed in the Early Noachian ∼3.93 Ga. The <span class="hlt">basin</span> has collected volatiles and other material through time, and experienced partial infilling with water evident from stratigraphic sequences, crater statistics, topography, and geomorphology. Although volcanism has not been previously associated with the Argyre <span class="hlt">basin</span>, our study of the northwest portion of the <span class="hlt">basin</span> floor has revealed landforms suggesting volcanic and tectonic activity occurred including Argyre Mons, a ∼50 km wide volcanic-structure formed ∼3 Ga. Giant polygons with a similar surface age are also identified on terrain <span class="hlt">adjacent</span> to the base of Argyre Mons, indicating the structure may have formed in a water-rich environment. In addition to Argyre Mons, cones, vents, mounds, dikes, and cavi or hollows, many of which are associated with extensional tectonics, are observed in the region. Multiple features appear to disrupt icy (and largely uncratered) terrain indicating a relatively young, Late Amazonian, formation age for at least some of the volcanic and tectonic features. The discovery of Argyre Mons, along with additional endogenic modification of the <span class="hlt">basin</span> floor, suggests that the region has experienced episodes of volcanism over a protracted period of time. This has implications for habitability as the <span class="hlt">basin</span> floor has been a region of elevated heat flow coupled with liquid water, water ice, and accumulation of sediments of diverse provenance with ranging geochemistry, along with magma-water interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/873/pdf/ds873.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/873/pdf/ds873.pdf"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 2013</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2014-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25–40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompasses the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when treatment and distribution of surface water from the Rio Grande began. A population increase of about 20 percent in the <span class="hlt">basin</span> from 1990 to 2000 and a 22-percent increase from 2000 to 2010 resulted in an increased demand for water. An initial network of wells was established by the U.S. Geological Survey (USGS) in cooperation with the City of Albuquerque from April 1982 through September 1983 to monitor changes in groundwater levels throughout the <span class="hlt">basin</span>. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2013), the network consists of 123 wells and piezometers. (A piezometer is a specialized well open to a specific depth in the aquifer, often of small diameter and nested with other piezometers open to different depths.) The USGS, in cooperation with the Albuquerque Bernalillo County Water Utility Authority, currently (2013) measures and reports water levels from the 123 wells and piezometers in the network; this report presents water-level data collected by USGS personnel at those 123 sites through water year 2013.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/790/pdf/Data%20Series%20790.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/790/pdf/Data%20Series%20790.pdf"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 2012</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2013-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25-40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompasses the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when surface water from the Rio Grande began being treated and integrated into the system. A population increase of about 20 percent in the <span class="hlt">basin</span> from 1990 to 2000 and a 22 percent increase from 2000 to 2010 resulted in an increased demand for water. An initial network of wells was established by the U.S. Geological Survey (USGS) in cooperation with the City of Albuquerque from April 1982 through September 1983 to monitor changes in groundwater levels throughout the <span class="hlt">basin</span>. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2012), the network consists of 126 wells and piezometers. (A piezometer is a specialized well open to a specific depth in the aquifer, often of small diameter and nested with other piezometers open to different depths.) The USGS, in cooperation with the Albuquerque Bernalillo County Water Utility Authority (ABCWUA), currently (2012) measures and reports water levels from the 126 wells and piezometers in the network; this report presents water-level data collected by USGS personnel at those 126 sites through water year 2012.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/ds/714/ds714.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/ds/714/ds714.pdf"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 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>Beman, Joseph E.</p> <p>2012-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25–40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompasses the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when surface water from the Rio Grande began being treated and integrated into the system. An increase of about 20 percent in the <span class="hlt">basin</span> human population from 1990 to 2000 and of about 22 percent increase from 2000 to 2010 also resulted in an increased demand for water. A network of wells was established by the U.S. Geological Survey in cooperation with the City of Albuquerque from April 1982 through September 1983 to monitor changes in groundwater levels throughout the <span class="hlt">basin</span>. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2011), the network consists of 126 wells and piezometers (a piezometer is a specialized well open to a specific depth in the aquifer and is often of small diameter and nested with other piezometers open to different depths). This report presents water-level data collected by U.S. Geological Survey personnel at those 126 sites through water year 2011 to better help the Albuquerque Bernalillo County Water Utility Authority manage water use.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2009/1125/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2009/1125/"><span>Water-Level Data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">Adjacent</span> Areas, Central New Mexico, Period of Record Through September 30, 2008</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2009-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25 to 40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompass the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> are currently (2008) obtained soley from ground-water resources. An increase of about 20 percent in the population from 1990 to 2000 also resulted in an increased demand for water. A network of wells was established to monitor changes in ground-water levels throughout the <span class="hlt">basin</span> from April 1982 through September 1983. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2008), the network consists of 144 wells and piezometers. This report presents water-level data collected by U.S. Geological Survey personnel at 125 sites through water-year 2008. In addition, data from 19 wells (Sites 127-30, 132-134, 136, 138-142 and 144-149) owned, maintained, and measured by Sandia National Laboratories are presented in this report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70179638','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70179638"><span>Multi-decadal increases in dissolved organic carbon and alkalinity flux from the Mackenzie drainage <span class="hlt">basin</span> to the Arctic <span class="hlt">Ocean</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>Tank, Suzanne E.; Striegl, Robert G.; McClelland, James W.; Kokelj, Steven V.</p> <p>2016-01-01</p> <p>Riverine exports of organic and inorganic carbon (OC, IC) to <span class="hlt">oceans</span> are intricately linked to processes occurring on land. Across high latitudes, thawing permafrost, alteration of hydrologic flow paths, and changes in vegetation may all affect this flux, with subsequent implications for regional and global carbon (C) budgets. Using a unique, multi-decadal dataset of continuous discharge coupled with water chemistry measurements for the Mackenzie River, we show major increases in dissolved OC (DOC) and IC (as alkalinity) fluxes since the early 1970s, for a watershed that covers 1.8 M km2 of northwestern Canada, and provides substantial inputs of freshwater and biogeochemical constituents to the Arctic <span class="hlt">Ocean</span>. Over a 39-year period of record, DOC flux at the Mackenzie mouth increased by 39.3% (44.5 ± 22.6 Gmol), while alkalinity flux increased by 12.5% (61.5 ± 60.1 Gmol). Isotopic analyses and substantial increases in sulfate flux indicate that increases in alkalinity are driven by accelerating sulfide oxidation, a process that liberates IC from rock and soils in the absence of CO2 consumption. Seasonal and sub-catchment trends suggest that permafrost thaw plays an important role in the observed increases in DOC and alkalinity: sub-catchment increases for all constituents are confined to northern, permafrost-affected regions, while observed increases in autumn to winter are consistent with documented landscape-scale changes that have resulted from changing thaw dynamics. This increase in DOC and sulfide-derived alkalinity represents a substantial intensification of land-to-<span class="hlt">ocean</span> C mobilization, at a level that is significant within the regional C budget. The change we observe, for example, is similar to current and projected future rates of CO2 consumption by weathering in the Mackenzie <span class="hlt">basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....1463M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....1463M"><span>A boundary condition for layer to level <span class="hlt">ocean</span> model interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mask, A.; O'Brien, J.; Preller, R.</p> <p>2003-04-01</p> <p>A radiation boundary condition based on vertical normal modes is introduced to allow a physical transition between nested/coupled <span class="hlt">ocean</span> models that are of differing vertical structure and/or differing physics. In this particular study, a fine resolution regional/coastal sigma-coordinate Naval Coastal <span class="hlt">Ocean</span> Model (NCOM) has been successfully nested to a coarse resolution (in the horizontal and vertical) <span class="hlt">basin</span> scale NCOM and a coarse resolution <span class="hlt">basin</span> scale Navy Layered <span class="hlt">Ocean</span> Model (NLOM). Both of these models were developed at the Naval Research Laboratory (NRL) at Stennis Space Center, Mississippi, USA. This new method, which decomposes the vertical structure of the models into barotropic and baroclinic modes, gives improved results in the coastal domain over Orlanski radiation boundary conditions for the test cases. The principle reason for the improvement is that each mode has the radiation boundary condition applied individually; therefore, the packet of information passing through the boundary is allowed to have multiple phase speeds instead of a single-phase speed. Allowing multiple phase speeds reduces boundary reflections, thus improving results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035552','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035552"><span>Western Arctic <span class="hlt">Ocean</span> temperature variability during the last 8000 years</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Farmer, Jesse R.; Cronin, Thomas M.; De Vernal, Anne; Dwyer, Gary S.; Keigwin, Loyd D.; Thunell, Robert C.</p> <p>2011-01-01</p> <p>We reconstructed subsurface (∼200–400 m) <span class="hlt">ocean</span> temperature and sea-ice cover in the Canada <span class="hlt">Basin</span>, western Arctic <span class="hlt">Ocean</span> from foraminiferal δ18O, ostracode Mg/Ca ratios, and dinocyst assemblages from two sediment core records covering the last 8000 years. Results show mean temperature varied from −1 to 0.5°C and −0.5 to 1.5°C at 203 and 369 m water depths, respectively. Centennial-scale warm periods in subsurface temperature records correspond to reductions in summer sea-ice cover inferred from dinocyst assemblages around 6.5 ka, 3.5 ka, 1.8 ka and during the 15th century Common Era. These changes may reflect centennial changes in the temperature and/or strength of inflowing Atlantic Layer water originating in the eastern Arctic <span class="hlt">Ocean</span>. By comparison, the 0.5 to 0.7°C warm temperature anomaly identified in oceanographic records from the Atlantic Layer of the Canada <span class="hlt">Basin</span> exceeded reconstructed Atlantic Layer temperatures for the last 1200 years by about 0.5°C.</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://pubs.er.usgs.gov/publication/70017650','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70017650"><span>Quaternary paleoceanography of the deep Arctic <span class="hlt">Ocean</span> based on quantitative analysis of Ostracoda</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Cronin, T. M.; Holtz, T.R.; Whatley, R.C.</p> <p>1994-01-01</p> <p>Ostracodes were studied from deep Arctic <span class="hlt">Ocean</span> cores obtained during the Arctic 91 expedition of the Polarstern to the Nansen, Amundsen and Makarov <span class="hlt">Basins</span>, the Lomonosov Ridge, Morris Jesup Rise and Yermak Plateau, in order to investigate their distribution in Arctic <span class="hlt">Ocean</span> deep water (AODW) and apply these data to paleoceanographic reconstruction of bottom water masses during the Quaternary. Analyses of coretop assemblages from Arctic 91 boxcores indicate the following: ostracodes are common at all depths between 1000 and 4500 m, and species distribution is strongly influenced by water mass characteristics and bathymetry; quantitative analyses comparing Eurasian and Canada <span class="hlt">Basin</span> assemblages indicate that distinct assemblages inhabit regions east and west of the Lomonosov Ridge, a barrier especially important to species living in lower AODW; deep Eurasian <span class="hlt">Basin</span> assemblages are more similar to those living in Greenland Sea deep water (GSDW) than those in Canada <span class="hlt">Basin</span> deep water; two upper AODW assemblages were recognized throughout the Arctic <span class="hlt">Ocean</span>, one living between 1000 and 1500 m, and the other, having high species diversity, at 1500-3000 m. Downcore quantitative analyses of species' abundances and the squared chord distance coefficient of similarity reveals a distinct series of abundance peaks in key indicator taxa interpreted to signify the following late Quaternary deep water history of the Eurasian <span class="hlt">Basin</span>. During the Last Glacial Maximum (LGM), a GSDW/AODW assemblage, characteristic of cold, well oxygenated deep water > 3000 m today, inhabited the Lomonosov Ridge to depths as shallow as 1000 m, perhaps indicating the influence of GSDW at mid-depths in the central Arctic <span class="hlt">Ocean</span>. During Termination 1, a period of high organic productivity associated with a strong inflowing warm North Atlantic layer occurred. During the mid-Holocene, several key faunal events indicate a period of warming and/or enhanced flow between the Canada and Eurasian <span class="hlt">Basins</span>. A long</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007AGUSM.T23A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007AGUSM.T23A..06B"><span>Uplift of continental crustal blocks <span class="hlt">adjacent</span> to the Rancheria <span class="hlt">Basin</span>-Guasare area: the effects of Maastrichtian-Paleocene collision along the southern Caribbean plate boundary</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bayona, G.; Montes, C.; Jaramillo, C.; Ojeda, G.; Cardona, A.; Pardo, A.; Lamus, F.</p> <p>2007-05-01</p> <p>In the Rancheria <span class="hlt">basin</span> (RB) and Guasare area (GA), Maastrichtian-Paleocene synorogenic strata overlie the Aptian-Campanian carbonate platform. Nowadays, RB is bounded to the west by metamorphic-and-igneous cored Santa Marta massif, where Upper Cretaceous strata overlie unconformably pre-Cretaceous rocks. The eastern boundary of the RB is the Perija range that includes volcaniclastic and sedimentary rocks of Jurassic and Cretaceous age in the hanging-wall of a NW-verging, low-angle dipping thrust belt. The GA is on the eastern foothills of the Perija range and corresponds to the western boundary of the Maracaibo <span class="hlt">basin</span>. Strata architecture, seismic reflectors, gravity, provenance, and paleocurrent analyses carried out in those <span class="hlt">basins</span> constrain the timing and style of uplift of Santa Marta massif and Perija range, which are linked with tectonism along the southern Caribbean plate. Maastrichtian-Paleocene strata thicken eastward up to 2.2 km in the RB, and this succession includes (in stratigraphic order): foram-rich calcareous mudstone, oyster-pelecypod rich carbonate-siliciclastic strata, coal- bearing mudstones and feldspar-lithic-rich fluvial sandstones. Internal disconformities and truncations of seismic reflectors are identified to the west of the RB, but there are not major thrust faults at this part of the <span class="hlt">basin</span> to explain such unconformities and truncations. In Early Paleocene, carbonates developed better to the west of the RB, whereas mixed carbonate-siliciclastic deposition continued toward the east of the RB. In early Late Paleocene, influx of terrigenous material (key grains=metamorphic, microcline and garnet fragments) derived from the Santa Marta massif increased to the west, but to the east of the RB and GA carbonate-siliciclastic and carbonate deposition continued, respectively. In mid-Late Paleocene, diachronous eastward advance of paralic/deltaic environments, tropical humid climate, and high subsidence rates favored production and preservation of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70028874','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70028874"><span>Two alternative juvenile life history types for fall Chinook salmon in the Snake River <span class="hlt">basin</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>Connor, W.P.; Sneva, J.G.; Tiffan, K.F.; Steinhorst, R.K.; Ross, D.</p> <p>2005-01-01</p> <p>Fall Chinook salmon Oncorhynchus tshawytscha in the Snake River <span class="hlt">basin</span> were listed under the Endangered Species Act in 1992. At the time of listing, it was assumed that fall Chinook salmon juveniles in the Snake River <span class="hlt">basin</span> adhered strictly to an <span class="hlt">ocean</span>-type life history characterized by saltwater entry at age 0 and first-year wintering in the <span class="hlt">ocean</span>. Research showed, however, that some fall Chinook salmon juveniles in the Snake River <span class="hlt">basin</span> spent their first winter in a reservoir and resumed seaward movement the following spring at age 1 (hereafter, reservoir-type juveniles). We collected wild and hatchery <span class="hlt">ocean</span>-type fall Chinook salmon juveniles in 1997 and wild and hatchery reservoir-type juveniles in 1998 to assess the condition of the reservoir-type juveniles at the onset of seaward movement. The <span class="hlt">ocean</span>-type juveniles averaged 112-139 mm fork length, and the reservoir-type juveniles averaged 222-224 mm fork length. The large size of the reservoir-type juveniles suggested a high potential for survival to salt water and subsequent return to freshwater. Scale pattern analyses of the fall Chinook salmon spawners we collected during 1998-2003 supported this point. Of the spawners sampled, an overall average of 41% of the wild fish and 51% of the hatchery fish had been reservoir-type juveniles. Males that had been reservoir-type juveniles often returned as small "minijacks" (wild, 16% of total; hatchery, 40% of total), but 84% of the wild males, 60% of the hatchery males, and 100% of the wild and hatchery females that had been reservoir-type juveniles returned at ages and fork lengths commonly observed in populations of Chinook salmon. We conclude that fall Chinook salmon in the Snake River <span class="hlt">basin</span> exhibit two alternative juvenile life histories, namely <span class="hlt">ocean</span>-type and reservoir-type. ?? Copyright by the American Fisheries Society 2005.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://waterrights.utah.gov/docSys/v920/y920/y920000e.pdf','USGSPUBS'); return false;" href="http://waterrights.utah.gov/docSys/v920/y920/y920000e.pdf"><span>Hydrology of Cache Valley, Cache County, Utah, and <span class="hlt">adjacent</span> part of Idaho, with emphasis on simulation of ground-water flow</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Kariya, Kim A.; Roark, D. Michael; Hanson, Karen M.</p> <p>1994-01-01</p> <p>A hydrologic investigation of Cache Valley was done to better understand the ground-water system in unconsolidated <span class="hlt">basin</span>-fill deposits and the interaction between ground water and surface water. Ground-water recharge occurs by infiltration of precipitation and unconsumed irrigation water, seepage from canals and streams, and subsurface inflow from <span class="hlt">adjacent</span> consolidated rock and <span class="hlt">adjacent</span> unconsolidated <span class="hlt">basin</span>-fill deposit ground-water systems. Ground-water discharge occurs as seepage to streams and reservoirs, spring discharge, evapotranspiration, and withdrawal from wells.Water levels declined during 1984-90. Less-than-average precipitation during 1987-90 and increased pumping from irrigation and public-supply wells contributed to the declines.A ground-water-flow model was used to simulate flow in the unconsolidated <span class="hlt">basin</span>-fill deposits. Data primarily from 1969 were used to calibrate the model to steady-state conditions. Transient-state calibration was done by simulating ground-water conditions on a yearly basis for 1982-90.A hypothetical simulation in which the dry conditions of 1990 were continued for 5 years projected an average lO-foot water-level decline between Richmond and Hyrum. When increased pumpage was simulated by adding three well fields, each pumping 10 cubic feet per second, in the Logan, Smithfield, and College Ward areas, water-level declines greater than 10 feet were projected in most of the southeastern part of the valley and discharge from springs and seepage to streams and reservoirs decreased.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70176638','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70176638"><span>Seismic velocities within the sedimentary succession of the Canada <span class="hlt">Basin</span> and southern Alpha-Mendeleev Ridge, Arctic <span class="hlt">Ocean</span>: evidence for accelerated porosity reduction?</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Shimeld, John; Li, Qingmou; Chian, Deping; Lebedeva-Ivanova, Nina; Jackson, Ruth; Mosher, David; Hutchinson, Deborah R.</p> <p>2016-01-01</p> <p>The Canada <span class="hlt">Basin</span> and the southern Alpha-Mendeleev ridge complex underlie a significant proportion of the Arctic <span class="hlt">Ocean</span>, but the geology of this undrilled and mostly ice-covered frontier is poorly known. New information is encoded in seismic wide-angle reflections and refractions recorded with expendable sonobuoys between 2007 and 2011. Velocity–depth samples within the sedimentary succession are extracted from published analyses for 142 of these records obtained at irregularly spaced stations across an area of 1.9E + 06 km2. The samples are modelled at regional, subregional and station-specific scales using an exponential function of inverse velocity versus depth with regionally representative parameters determined through numerical regression. With this approach, smooth, non-oscillatory velocity–depth profiles can be generated for any desired location in the study area, even where the measurement density is low. Practical application is demonstrated with a map of sedimentary thickness, derived from seismic reflection horizons interpreted in the time domain and depth converted using the velocity–depth profiles for each seismic trace. A thickness of 12–13 km is present beneath both the upper Mackenzie fan and the middle slope off of Alaska, but the sedimentary prism thins more gradually outboard of the latter region. Mapping of the observed-to-predicted velocities reveals coherent geospatial trends associated with five subregions: the Mackenzie fan; the continental slopes beyond the Mackenzie fan; the abyssal plain; the southwestern Canada <span class="hlt">Basin</span>; and, the Alpha-Mendeleev magnetic domain. Comparison of the subregional velocity–depth models with published borehole data, and interpretation of the station-specific best-fitting model parameters, suggests that sandstone is not a predominant lithology in any of the five subregions. However, the bulk sand-to-shale ratio likely increases towards the Mackenzie fan, and the model for this subregion compares</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoJI.204....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoJI.204....1S"><span>Seismic velocities within the sedimentary succession of the Canada <span class="hlt">Basin</span> and southern Alpha-Mendeleev Ridge, Arctic <span class="hlt">Ocean</span>: evidence for accelerated porosity reduction?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shimeld, John; Li, Qingmou; Chian, Deping; Lebedeva-Ivanova, Nina; Jackson, Ruth; Mosher, David; Hutchinson, Deborah</p> <p>2016-01-01</p> <p>The Canada <span class="hlt">Basin</span> and the southern Alpha-Mendeleev ridge complex underlie a significant proportion of the Arctic <span class="hlt">Ocean</span>, but the geology of this undrilled and mostly ice-covered frontier is poorly known. New information is encoded in seismic wide-angle reflections and refractions recorded with expendable sonobuoys between 2007 and 2011. Velocity-depth samples within the sedimentary succession are extracted from published analyses for 142 of these records obtained at irregularly spaced stations across an area of 1.9E + 06 km2. The samples are modelled at regional, subregional and station-specific scales using an exponential function of inverse velocity versus depth with regionally representative parameters determined through numerical regression. With this approach, smooth, non-oscillatory velocity-depth profiles can be generated for any desired location in the study area, even where the measurement density is low. Practical application is demonstrated with a map of sedimentary thickness, derived from seismic reflection horizons interpreted in the time domain and depth converted using the velocity-depth profiles for each seismic trace. A thickness of 12-13 km is present beneath both the upper Mackenzie fan and the middle slope off of Alaska, but the sedimentary prism thins more gradually outboard of the latter region. Mapping of the observed-to-predicted velocities reveals coherent geospatial trends associated with five subregions: the Mackenzie fan; the continental slopes beyond the Mackenzie fan; the abyssal plain; the southwestern Canada <span class="hlt">Basin</span>; and, the Alpha-Mendeleev magnetic domain. Comparison of the subregional velocity-depth models with published borehole data, and interpretation of the station-specific best-fitting model parameters, suggests that sandstone is not a predominant lithology in any of the five subregions. However, the bulk sand-to-shale ratio likely increases towards the Mackenzie fan, and the model for this subregion compares favourably with</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..18.3471W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.3471W"><span><span class="hlt">Basin</span>-mountain structures and hydrocarbon exploration potential of west Junggar orogen in China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Xiaozhi; He, Dengfa; Qi, Xuefeng</p> <p>2016-04-01</p> <p>Situated in northern Xinjiang, China, in NE-SW trend, West Junggar Orogen is <span class="hlt">adjacent</span> to Altai fold belt on the north with the Ertix Fault as the boundary, North Tianshan fold belt on the south with the Ebinur Lake Strike-slip Fault as the boundary, and the Junggar <span class="hlt">Basin</span> on the southeast with Zaire-Genghis Khan-Hala'alat fold belt as the boundary. Covering an area of about 10×104 km2 in China, there are medium and small intermontane <span class="hlt">basins</span>, Burqin-Fuhai, Tacheng, Hefeng and Hoxtolgay, distributing inside the orogen. Tectonically West Junggar Orogen lies in the middle section of the Palaeo-Asian tectonic domain where the Siberia, Kazakhstan and Tarim Plates converge, and is the only orogen trending NE-SW in the Palaeo-Asian tectonic domain. Since the Paleozoic, the orogen experienced pre-Permian plate tectonic evolution and post-Permian intra-plate <span class="hlt">basin</span> evolution. Complex tectonic evolution and multi-stage structural superimposition not only give rise to long term controversial over the <span class="hlt">basin</span> basement property but also complex <span class="hlt">basin</span>-mountain coupling relations, structures and <span class="hlt">basin</span> superimposition modes. According to analysis of several kinds of geological and geophysical data, the orogen was dominated by compressive folding and thrust napping from the Siberia plate in the north since the Late Paleozoic. Compressive stress weakened from north to south, corresponding to subdued vertical movement and enhanced horizontal movement of crustal surface from north to south, and finally faded in the overthrust-nappe belt at the northwest margin of the Junggar <span class="hlt">Basin</span>. The variation in compressive stress is consistent with the surface relief of the orogen, which is high in the north and low in the south. There are two kinds of <span class="hlt">basin</span>-mountain coupling relationships, i.e. high angle thrusting and overthrusting and napping, and two kinds of <span class="hlt">basin</span> superimposition modes, i.e. inherited and progressive, and migrating and convulsionary modes. West Junggar orogen has rich oil and gas</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914729D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914729D"><span>Observing mass exchange with the Lofoten <span class="hlt">Basin</span> using surface drifters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dugstad, Johannes S.; LaCasce, Joe; Koszalka, Inga M.; Fer, Ilker</p> <p>2017-04-01</p> <p>The Lofoten <span class="hlt">Basin</span> in the Nordic Seas plays a central role in the global overturning circulation, acting as a reservoir for northward-flowing Atlantic water. Substantial heat loss occurs here, permitting the waters to become denser and eventually sink nearer the Arctic. Idealized modeling studies and theoretical arguments suggest the warm water enters the Lofoten <span class="hlt">Basin</span> via eddy transport from the boundary current over the <span class="hlt">adjacent</span> continental slope. But there is no observational evidence that this is the major contribution to mass exchange between the warm Atlantic Current and the <span class="hlt">Basin</span>. How the <span class="hlt">basin</span> waters exit also remains a mystery. Surface drifters offer an unique possibility to study the pathways of the boundary-<span class="hlt">basin</span> exchange of mass and heat. We thereby examine trajectories of surface drifters released in the Nordic Seas in the POLEWARD and PROVOLO experiments, and supplemented by historical data from the Global Drifter Array. Contrary to the idea that the boundary current eddies are the main source, the results suggest that fluid is entering the Lofoten <span class="hlt">Basin</span> from all sides. However, the drifters exit preferentially in the northeast corner of the <span class="hlt">basin</span>. This asymmetry likely contributes to the extended residence times of the warm Atlantic waters in the Lofoten <span class="hlt">Basin</span>. We consider various measures to quantify the effect, and test whether this is captured in a high resolution numerical model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28899339','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28899339"><span>Ciliate diversity and distribution patterns in the sediments of a seamount and <span class="hlt">adjacent</span> abyssal plains in the tropical Western Pacific <span class="hlt">Ocean</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhao, Feng; Filker, Sabine; Stoeck, Thorsten; Xu, Kuidong</p> <p>2017-09-12</p> <p>Benthic ciliates and the environmental factors shaping their distribution are far from being completely understood. Likewise, deep-sea systems are amongst the least understood ecosystems on Earth. In this study, using high-throughput DNA sequencing, we investigated the diversity and community composition of benthic ciliates in different sediment layers of a seamount and an <span class="hlt">adjacent</span> abyssal plain in the tropical Western Pacific <span class="hlt">Ocean</span> with water depths ranging between 813 m and 4566 m. Statistical analyses were used to assess shifts in ciliate communities across vertical sediment gradients and water depth. Nine out of 12 ciliate classes were detected in the different sediment samples, with Litostomatea accounting for the most diverse group, followed by Plagiopylea and Oligohymenophorea. The novelty of ciliate genetic diversity was extremely high, with a mean similarity of 93.25% to previously described sequences. On a sediment depth gradient, ciliate community structure was more similar within the upper sediment layers (0-1 and 9-10 cm) compared to the lower sediment layers (19-20 and 29-30 cm) at each site. Some unknown ciliate taxa which were absent from the surface sediments were found in deeper sediments layers. On a water depth gradient, the proportion of unique OTUs was between 42.2% and 54.3%, and that of OTUs shared by all sites around 14%. However, alpha diversity of the different ciliate communities was relatively stable in the surface layers along the water depth gradient, and about 78% of the ciliate OTUs retrieved from the surface layer of the shallowest site were shared with the surface layers of sites deeper than 3800 m. Correlation analyses did not reveal any significant effects of measured environmental factors on ciliate community composition and structure. We revealed an obvious variation in ciliate community along a sediment depth gradient in the seamount and the <span class="hlt">adjacent</span> abyssal plain and showed that water depth is a less important factor</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ClDy...42..203D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ClDy...42..203D"><span>Indian <span class="hlt">Ocean</span> warming during 1958-2004 simulated by a climate system model and its mechanism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dong, Lu; Zhou, Tianjun; Wu, Bo</p> <p>2014-01-01</p> <p>The mechanism responsible for Indian <span class="hlt">Ocean</span> Sea surface temperature (SST) <span class="hlt">basin</span>-wide warming trend during 1958-2004 is studied based on both observational data analysis and numerical experiments with a climate system model FGOALS-gl. To quantitatively estimate the relative contributions of external forcing (anthropogenic and natural forcing) and internal variability, three sets of numerical experiments are conducted, viz. an all forcing run forced by both anthropogenic forcing (greenhouse gases and sulfate aerosols) and natural forcing (solar constant and volcanic aerosols), a natural forcing run driven by only natural forcing, and a pre-industrial control run. The model results are compared to the observations. The results show that the observed warming trend during 1958-2004 (0.5 K (47-year)-1) is largely attributed to the external forcing (more than 90 % of the total trend), while the residual is attributed to the internal variability. Model results indicate that the anthropogenic forcing accounts for approximately 98.8 % contribution of the external forcing trend. Heat budget analysis shows that the surface latent heat flux due to atmosphere and surface longwave radiation, which are mainly associated with anthropogenic forcing, are in favor of the <span class="hlt">basin</span>-wide warming trend. The <span class="hlt">basin</span>-wide warming is not spatially uniform, but with an equatorial IOD-like pattern in climate model. The atmospheric processes, <span class="hlt">oceanic</span> processes and climatological latent heat flux together form an equatorial IOD-like warming pattern, and the <span class="hlt">oceanic</span> process is the most important in forming the zonal dipole pattern. Both the anthropogenic forcing and natural forcing result in easterly wind anomalies over the equator, which reduce the wind speed, thereby lead to less evaporation and warmer SST in the equatorial western <span class="hlt">basin</span>. Based on Bjerknes feedback, the easterly wind anomalies uplift the thermocline, which is unfavorable to SST warming in the eastern <span class="hlt">basin</span>, and contribute to SST</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.2556N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.2556N"><span>The record of India-Asia collision preserved in Tethyan <span class="hlt">ocean</span> <span class="hlt">basin</span> sediments.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Najman, Yani; Jenks, Dan; Godin, Laurent; Boudagher-Fadel, Marcelle; Bown, Paul; Horstwood, Matt; Garzanti, Eduardo; Bracialli, Laura; Millar, Ian</p> <p>2015-04-01</p> <p>The timing of India-Asia collision is critical to the understanding of crustal deformation processes, since, for example, it impacts on calculations regarding the amount of convergence that needs to be accommodated by various mechanisms. In this research we use sediments originally deposited in the Tethyan <span class="hlt">ocean</span> <span class="hlt">basin</span> and now preserved in the Himalayan orogeny to constrain the timing of collision. In the NW Himalaya, a number of workers have proposed a ca 55-50 Ma age for collision along the Indus suture zone which separates India from the Kohistan-Ladakh Intraoceanic Island arc (KLA) to the north. This is based on a number of factors including the age of youngest marine sediments in the Indus suture (e.g. Green et al. 2008), age of eclogites indicative of onset of Indian continental subduction (e.g. de Sigoyer et al. 2000), and first evidence of detritus from north of the suture zone deposited on the Indian plate (e.g. Clift et al. 2002). Such evidence can be interpreted as documenting the age of India-Asia collision if one takes the KLA to have collided with the Asian plate prior to its collision with India (e.g. Petterson 2010 and refs therein). However, an increasing number of workers propose that the KLA collided with Asia subsequent to its earlier collision with India, dated variously at 85 Ma (Chatterjee et al. 2013), 61 Ma (Khan et al. 2009) and 50 Ma (Bouilhol et al. 2013). This, plus the questioning of earlier provenance work (Clift et al. 2002) regarding the validity of their data for constraining timing of earliest arrival of material north of the suture deposited on the Indian plate (Henderson et al. 2011) suggests that the time is right for a reappraisal of this topic. We use a provenance-based approach here, using combined U-Pb and Hf on detrital zircons from Tethyan <span class="hlt">ocean</span> <span class="hlt">basin</span> sediments, along with petrography and biostratigraphy, to identify first arrival of material from north of the Indian plate to arrive on the Indian continent, to constrain</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70042009','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70042009"><span>Seismic structure of the crust and uppermost mantle of South America and surrounding <span class="hlt">oceanic</span> <span class="hlt">basins</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>Chulick, Gary S.; Detweiler, Shane; Mooney, Walter D.</p> <p>2013-01-01</p> <p>We present a new set of contour maps of the seismic structure of South America and the surrounding <span class="hlt">ocean</span> <span class="hlt">basins</span>. These maps include new data, helping to constrain crustal thickness, whole-crustal average P-wave and S-wave velocity, and the seismic velocity of the uppermost mantle (Pn and Sn). We find that: (1) The weighted average thickness of the crust under South America is 38.17 km (standard deviation, s.d. ±8.7 km), which is ∼1 km thinner than the global average of 39.2 km (s.d. ±8.5 km) for continental crust. (2) Histograms of whole-crustal P-wave velocities for the South American crust are bi-modal, with the lower peak occurring for crust that appears to be missing a high-velocity (6.9–7.3 km/s) lower crustal layer. (3) The average P-wave velocity of the crystalline crust (Pcc) is 6.47 km/s (s.d. ±0.25 km/s). This is essentially identical to the global average of 6.45 km/s. (4) The average Pn velocity beneath South America is 8.00 km/s (s.d. ±0.23 km/s), slightly lower than the global average of 8.07 km/s. (5) A region across northern Chile and northeast Argentina has anomalously low P- and S-wave velocities in the crust. Geographically, this corresponds to the shallowly-subducted portion of the Nazca plate (the Pampean flat slab first described by Isacks et al., 1968), which is also a region of crustal extension. (6) The thick crust of the Brazilian craton appears to extend into Venezuela and Colombia. (7) The crust in the Amazon <span class="hlt">basin</span> and along the western edge of the Brazilian craton may be thinned by extension. (8) The average crustal P-wave velocity under the eastern Pacific seafloor is higher than under the western Atlantic seafloor, most likely due to the thicker sediment layer on the older Atlantic seafloor.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.4694L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.4694L"><span>The Taili-Yiwulüshan metamorphic core complex corridor: Diachronous exhumation and relationships to the <span class="hlt">adjacent</span> <span class="hlt">basins</span> based on new 40Ar/39Ar and (U-Th-Sm)/He mineral ages</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liang, Chenyue; Neubauer, Franz; Liu, Yongjiang; Genser, Johann; Dunkl, István; Heberer, Bianca; Jin, Wei; Zeng, Zuoxun; Li, Weimin; Wen, Quanbo; Li, Jing</p> <p>2015-04-01</p> <p>The Xingcheng-Taili ductile shear zone (western Liaoning Province in China) formed during latest Jurassic to Early Cretaceous crustal extension of the eastern North China craton, and exhumed low to medium metamorphic grade Archean, Upper Triassic and Upper Jurassic granitic rocks. The Mesozoic Yiwulüshan metamorphic core complex (Yiwulüshan MCC) is dominated by a NNE-SSW elongated dome with a left-lateral shear zone, which is located in the northeastern part of Xingcheng-Taili ductile shear zone, and combine as Taili-Yiwulüshan metamorphic core complex corridor. To the east, it is bounded by the NNE-trending Cretaceous to Eocene Liaohe <span class="hlt">basin</span> (the northern extension of the Bohai Bay <span class="hlt">basin</span>), and to the west by the Cretaceous-aged Fuxin-Yixian <span class="hlt">basin</span>, which could potentially interpreted as supra-detachment <span class="hlt">basins</span>. Here, we present results from a multi-method thermochronological study and coupled with structural investigations and sections of <span class="hlt">adjacent</span> supra-detachment <span class="hlt">basins</span>, which constrain the timing of regional deformation as well as the cooling history and exhumation processes of the low- to middle-grade metamorphic complex in the Taili-Yiwulüshan MCC corridor, in order to understand the mode of lithospheric scale reactivation, extension and thinning of the North China craton. The new40Ar/39Ar muscovite, biotite, K-feldspar and (U-Th)/He apatite ages from granitic rocks help constrain the thermal evolution during its exhumation. The thermochronologic studies have shown at least three stages of exhumation and cooling from late Jurassic to Eocene in Xingcheng-Taili shear zone should be distinguished, e.g., ~ 150-130 Ma, 130-115 Ma and 115-52 Ma, respectively. Diachronous onset and subsequent parallel cooling and exhumation characterize the early thermal history. The Yiwulüshan MCC has a similar exhumation history from 135 to 97 Ma with a similar cooling history. The development of Taili-Yiwulüshan MCC corridor is associated with synkinematic emplacement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012BGD.....9.1667C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012BGD.....9.1667C"><span>Whole water column distribution and carbon isotopic composition of bulk particulate organic carbon, cholesterol and brassicasterol from the Cape <span class="hlt">Basin</span> to the northern Weddell Gyre in the Southern <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavagna, A.-J.; Dehairs, F.; Woule-Ebongué, V.; Bouillon, S.; Planchon, F.; Delille, B.; Bouloubassi, I.</p> <p>2012-02-01</p> <p>The combination of concentrations and δ13C signatures of Particulate Organic Carbon (POC) and sterols provides a powerful approach to study ecological and environmental changes both in the modern and ancient <span class="hlt">ocean</span>, but its application has so far been restricted to the surface area. We applied this tool to study the biogeochemical changes in the modern <span class="hlt">ocean</span> water column during the BONUS-GoodHope survey (Feb-Mar 2008) from Cape <span class="hlt">Basin</span> to the northern part of the Weddell Gyre. Cholesterol and brassicasterol were chosen as ideal biomarkers of the heterotrophic and autotrophic carbon pools, respectively, because of their ubiquitous and relatively refractory nature. We document depth distributions of concentrations (relative to bulk POC) and δ13C signatures of cholesterol and brassicasterol from the Cape <span class="hlt">Basin</span> to the northern Weddell Gyre combined with CO2 aq. surface concentration variation. While relationships between surface water CO2 aq. and δ13C of bulk POC and biomarkers have been previously established for surface waters, our data show that these remain valid in deeper waters, suggesting that δ13C signatures of certain biomarkers could be developed as proxies for surface water CO2 aq. Our data suggest a key role of zooplankton fecal aggregates in carbon export for this part of the Southern <span class="hlt">Ocean</span>. We observed a general increase in sterol δ13C signatures with depth, which is likely related to a combination of particle size effects, selective feeding on larger cells by zooplankton, and growth rate related effects Additionally, in the southern part of the transect south of the Polar Front (PF), the release of sea-ice algae is hypothesized to influence the isotopic signature of sterols in the open <span class="hlt">ocean</span>. Overall, combined use of δ13C and concentrations measurements of both bulk organic C and specific sterol markers throughout the water column shows the promising potential of analyzing δ13C signatures of individual marine sterols to explore the recent history of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915904J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915904J"><span>Structural development of the Dieppe-Hampshire <span class="hlt">Basin</span> (Eastern English Channel): Contribution of new 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>Jollivet-Castelot, Martin; Gaullier, Virginie; Paquet, Fabien; Chanier, Frank; Thinon, Isabelle; Lasseur, Eric; Averbuch, Olivier</p> <p>2017-04-01</p> <p>The Dieppe-Hampshire <span class="hlt">Basin</span> is a Cenozoic <span class="hlt">basin</span> crossing the eastern English Channel, between SE of England and the French coast. This <span class="hlt">basin</span> and its borders developed during the Cenozoic, a period of overall tectonic inversion, in response to the opening of the North Atlantic <span class="hlt">Ocean</span> and Pyrenean-alpine deformation episodes. Both extensional and subsequent compressional deformations within this area involve the reactivation of older major regional structures, inherited from the Variscan Orogeny. However, the detailed structural development of the Dieppe-Hampshire <span class="hlt">Basin</span> still remains poorly constrained, as well as the detailed stratigraphic framework of Cenozoic series, notably in terms of seismic stratigraphy and sequence stratigraphy. New very high resolution seismic data, acquired during the oceanographic cruise "TREMOR" (R/V "Côtes de la Manche", 2014, 1800 kilometers of Sparker profiles), and bathymetric data from SHOM and UKHO, have allowed to image the sedimentary filling and tectonic structures of the Dieppe-Hampshire <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas. The interpretation was first focused on a seismic facies analysis that led to evidence numerous unconformities and seismic units ranging from the Upper Cretaceous to the Bartonian (Late Eocene). The interpretation of the seismic profiles also allowed to map precisely many tectonic features, as faults, folds and monoclinal flexures. Thanks to the new data, we especially imaged the complexity of the deformation within the highest tectonized zones of the region, along the Nord-Baie de Seine <span class="hlt">Basin</span> and offshore the Boulonnais coast with an unprecedented resolution. The expression of the deformation appears to be very different between the Mesozoic and the Cenozoic series, with prevailing folding affecting the Cenozoic strata whereas the Mesozoic series are predominantly faulted. This deformation pattern illustrates two major structural trends, respectively E-W and NW-SE directed, both syn- to post-Bartonian in age. The first</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/hwcorrectiveactionsites/hazardous-waste-cleanup-military-ocean-terminal-bayonne-new-jersey','PESTICIDES'); return false;" href="https://www.epa.gov/hwcorrectiveactionsites/hazardous-waste-cleanup-military-ocean-terminal-bayonne-new-jersey"><span>Hazardous Waste Cleanup: Military <span class="hlt">Ocean</span> Terminal in Bayonne, New Jersey</span></a></p> <p><a target="_blank" href="http://www.epa.gov/pesticides/search.htm">EPA Pesticide Factsheets</a></p> <p></p> <p></p> <p>The Military <span class="hlt">Ocean</span> Terminal Bayonne (MOTBY) is a 652 acre, approximately 1/3-mile wide, 2-mile long, manmade peninsula that extends into the upper New York Harbor. It is located on Port Terminal Road <span class="hlt">adjacent</span> to (west of) the City of Bayonne. Site use as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2010/1228/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2010/1228/"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 2009</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.; Torres, Leeanna T.</p> <p>2010-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25 to 40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompass the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when surface water from the Rio Grande began being treated and integrated into the system. An increase of about 20 percent in the population from 1990 to 2000 also resulted in an increased demand for water. A network of wells was established to monitor changes in groundwater levels throughout the <span class="hlt">basin</span> from April 1982 through September 1983. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2009), the network consists of 131 wells and piezometers. This report presents water-level data collected by U.S. Geological Survey personnel at 123 sites through water year 2009. In addition, data from four wells (Sites 140, 147, 148, and 149) owned, maintained, and measured by Sandia National Laboratories and three from Kirtland Air Force Base (Sites 119, 125, and 126) are presented in this report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/2008/1255/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/2008/1255/"><span>Water-Level Data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">Adjacent</span> Areas, Central New Mexico, Period of Record Through September 30, 2007</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.</p> <p>2008-01-01</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25 to 40 miles wide. The <span class="hlt">basin</span> is defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompass the structural Rio Grande Rift within the <span class="hlt">basin</span>. Drinking-water supplies throughout the <span class="hlt">basin</span> are currently (2007) obtained solely from ground-water resources. An increase of about 20 percent in the population from 1990 to 2000 also resulted in an increased demand for water. A network of wells was established to monitor changes in ground-water levels throughout the <span class="hlt">basin</span> from April 1982 through September 1983. This network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly in 1983. Currently (2007), the network consists of 131 wells and piezometers. This report presents water-level data collected by U.S. Geological Survey personnel at 131 sites through water-year 2007. Data from five sites (Sites 9, 10, 31, 71 and 78) were not measured during the 2007 water-year, but are included in this report because recent data are useful for comparison and (or) data have been collected that will be included in the water-year 2008 report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70000341','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70000341"><span>Trace-element budgets in the Ohio/Sunbury shales of Kentucky: Constraints on <span class="hlt">ocean</span> circulation and primary productivity in the Devonian-Mississippian Appalachian <span class="hlt">Basin</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>Perkins, R.B.; Piper, D.Z.; Mason, C.E.</p> <p>2008-01-01</p> <p>The hydrography of the Appalachian <span class="hlt">Basin</span> in late Devonian-early Mississippian time is modeled based on the geochemistry of black shales and constrained by others' paleogeographic reconstructions. The model supports a robust exchange of <span class="hlt">basin</span> bottom water with the open <span class="hlt">ocean</span>, with residence times of less than forty years during deposition of the Cleveland Shale Member of the Ohio Shale. This is counter to previous interpretations of these carbon-rich units having accumulated under a stratified and stagnant water column, i.e., with a strongly restricted bottom bottom-water circulation. A robust circulation of bottom waters is further consistent with the palaeoclimatology, whereby eastern trade-winds drove upwelling and arid conditions limited terrestrial inputs of siliciclastic sediment, fresh waters, and riverine nutrients. The model suggests that primary productivity was high (~ 2??g C m- 2 d- 1), although no higher than in select locations in the <span class="hlt">ocean</span> today. The flux of organic carbon settling through the water column and its deposition on the sea floor was similar to fluxes found in modern marine environments. Calculations based on the average accumulation rate of the marine fraction of Ni suggest the flux of organic carbon settling out of the water column was approximately 9% of primary productivity, versus an accumulation rate (burial) of organic carbon of 0.5% of primary productivity. Trace-element ratios of V:Mo and Cr:Mo in the marine sediment fraction indicate that bottom waters shifted from predominantly anoxic (sulfate reducing) during deposition of the Huron Shale Member of the Ohio Shale to predominantly suboxic (nitrate reducing) during deposition of the Cleveland Shale Member and the Sunbury Shale, but with anoxic conditions occurring intermittently throughout this period. ?? 2008 Elsevier B.V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28784714','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28784714"><span>High-latitude <span class="hlt">ocean</span> ventilation and its role in Earth's climate transitions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Naveira Garabato, Alberto C; MacGilchrist, Graeme A; Brown, Peter J; Evans, D Gwyn; Meijers, Andrew J S; Zika, Jan D</p> <p>2017-09-13</p> <p>The processes regulating <span class="hlt">ocean</span> ventilation at high latitudes are re-examined based on a range of observations spanning all scales of <span class="hlt">ocean</span> circulation, from the centimetre scales of turbulence to the <span class="hlt">basin</span> scales of gyres. It is argued that high-latitude <span class="hlt">ocean</span> ventilation is controlled by mechanisms that differ in fundamental ways from those that set the overturning circulation. This is contrary to the assumption of broad equivalence between the two that is commonly adopted in interpreting the role of the high-latitude <span class="hlt">oceans</span> in Earth's climate transitions. Illustrations of how recognizing this distinction may change our view of the <span class="hlt">ocean</span>'s role in the climate system are offered.This article is part of the themed issue '<span class="hlt">Ocean</span> ventilation and deoxygenation in a warming world'. © 2017 The Authors.</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/2016SPIE.9688E..1EZ','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9688E..1EZ"><span>Visualization of <span class="hlt">ocean</span> forecast in BYTHOS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhuk, E.; Zodiatis, G.; Nikolaidis, A.; Stylianou, S.; Karaolia, A.</p> <p>2016-08-01</p> <p>The Cyprus Oceanography Center has been constantly searching for new ideas for developing and implementing innovative methods and new developments concerning the use of Information Systems in Oceanography, to suit both the Center's monitoring and forecasting products. Within the frame of this scope two major online managing and visualizing data systems have been developed and utilized, those of CYCOFOS and BYTHOS. The Cyprus Coastal <span class="hlt">Ocean</span> Forecasting and Observing System - CYCOFOS provides a variety of operational predictions such as ultra high, high and medium resolution <span class="hlt">ocean</span> forecasts in the Levantine <span class="hlt">Basin</span>, offshore and coastal sea state forecasts in the Mediterranean and Black Sea, tide forecasting in the Mediterranean, <span class="hlt">ocean</span> remote sensing in the Eastern Mediterranean and coastal and offshore monitoring. As a rich internet application, BYTHOS enables scientists to search, visualize and download oceanographic data online and in real time. The recent improving of BYTHOS system is the extension with access and visualization of CYCOFOS data and overlay forecast fields and observing data. The CYCOFOS data are stored at OPENDAP Server in netCDF format. To search, process and visualize it the php and python scripts were developed. Data visualization is achieved through Mapserver. The BYTHOS forecast access interface allows to search necessary forecasting field by recognizing type, parameter, region, level and time. Also it provides opportunity to overlay different forecast and observing data that can be used for complex analyze of sea <span class="hlt">basin</span> aspects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.U33A..04S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.U33A..04S"><span>Thermal Models of the <span class="hlt">Ocean</span> Floor: from Wegener to Cerro Prieto</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sclater, J. G.; Negrete-Aranda, R.</p> <p>2017-12-01</p> <p>Wegener (1925) argued that hot rock could explain the shallower depths of ridges in the center of the Atlantic <span class="hlt">Ocean</span>. Hess (1963) proposed that the intrusion of molten rock occurred at a world encircling mid-<span class="hlt">ocean</span> ridge system. However, he accounted for the elevation of the ridges by the formation of serpentinite and thermal convection. Langseth et al. (1966) provided the major advance by using a 100 km thick plate to argue such a concept could not explain the depth, heat flow versus distance relations. They had the correct model but misinterpreted the data. Reformulating theoretically, McKenzie (1967) created the generally accepted thermal model for the <span class="hlt">ocean</span> floor. Unfortunately, in attempting to match erroneously low heat flow data, he used a 50 km thick plate. Addition of the effect of water and the realization of the importance of advective flow, enabled various groups to create thermal plate models that accounted for the heat flow and depth age relations. From this came the understanding of hydrothermal circulation in the <span class="hlt">oceanic</span> crust, the thermal boundary layer concept of the <span class="hlt">oceanic</span> plate and the realization that all thermal models differed only in the way the different groups had chosen to analyze the data. During the past 40 years many have applied similar concepts to continental margins: (1) Measurement of subsidence of the Atlantic margin, continental stretching and a Time Temperature, Depth and Maturation analysis of continental <span class="hlt">basins</span> have created the field of <span class="hlt">Basin</span> Analysis; (2) Changes in heat flow at <span class="hlt">ocean</span> continent boundaries have determined the position of the transition and (3) In attempting to examine the <span class="hlt">ocean</span> continent transition process in the northernmost <span class="hlt">basin</span> of the Gulf of California, Neumann et al (in press) observed conductive heat flow values greater than 0.75 Watts, at a depth of < 150 m, along a 10 km section of a profile across the southern extension of the Cerro Prieto fault. The magnitude of these values overwhelms local</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918318H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918318H"><span>A distributed atmosphere-sea ice-<span class="hlt">ocean</span> observatory in the central Arctic <span class="hlt">Ocean</span>: concept and first results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoppmann, Mario; Nicolaus, Marcel; Rabe, Benjamin; Wenzhöfer, Frank; Katlein, Christian; Scholz, Daniel; Valcic, Lovro</p> <p>2017-04-01</p> <p>To understand the current evolution of the Arctic <span class="hlt">Ocean</span> towards a less extensive, thinner and younger sea ice cover is one of the biggest challenges in climate research. Especially the lack of simultaneous in-situ observations of sea ice, <span class="hlt">ocean</span> and atmospheric properties leads to significant knowledge gaps in their complex interactions, and how the associated processes impact the polar marine ecosystem. Here we present a concept for the implementation of a long-term strategy to monitor the most essential climate- and ecosystem parameters in the central Arctic <span class="hlt">Ocean</span>, year round and synchronously. The basis of this strategy is the development and enhancement of a number of innovative autonomous observational platforms, such as rugged weather stations, ice mass balance buoys, ice-tethered bio-optical buoys and upper <span class="hlt">ocean</span> profilers. The deployment of those complementing platforms in a distributed network enables the simultaneous collection of physical and biogeochemical in-situ data on <span class="hlt">basin</span> scales and year round, including the largely undersampled winter periods. A key advantage over other observatory systems is that the data is sent via satellite in near-real time, contributing to numerical weather predictions through the Global Telecommunication System (GTS) and to the International Arctic Buoy Programme (IABP). The first instruments were installed on ice floes in the Eurasian <span class="hlt">Basin</span> in spring 2015 and 2016, yielding exceptional records of essential climate- and ecosystem-relevant parameters in one of the most inaccessible regions of this planet. Over the next 4 years, and including the observational periods of the Year of Polar Prediction (YOPP, 2017-2019) and the Multidisciplinary drifting Observatory for the Study of the Arctic Climate (MOSAiC, 2020), the distributed observatory will be maintained by deployment of additional instruments in the central Arctic each year, benefitting from international logistical efforts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMEP23D3626M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMEP23D3626M"><span>Zinc and Its Isotopes in the Loire River <span class="hlt">Basin</span>, France</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Millot, R.; Desaulty, A. M.; Bourrain, X.</p> <p>2014-12-01</p> <p>The contribution of human activities such as industries, agriculture and domestic inputs, becomes more and more significant in the chemical composition of the dissolved load of rivers. Human factors act as a supplementary key process. Therefore the mass-balance for the budget of catchments and river <span class="hlt">basins</span> include anthropogenic disturbances. The Loire River in central France is approximately 1010 km long and drains an area of 117,800 km2. In the upper <span class="hlt">basin</span>, the bedrock is old plutonic rock overlain by much younger volcanic rocks. The intermediate <span class="hlt">basin</span> includes three major tributaries flowing into the Loire River from the left bank: the Cher, the Indre and the Vienne rivers; the main stream flows westward and its valley stretches toward the Atlantic <span class="hlt">Ocean</span>. Here, the Loire River drains the sedimentary series of the Paris <span class="hlt">Basin</span>, mainly carbonate deposits. The lower Loire <span class="hlt">basin</span> drains pre-Mesozoic basement of the Armorican Massif and its overlying Mesozoic to Cenozoic sedimentary deposits. The Loire River is one of the main European riverine inputs to the Atlantic <span class="hlt">ocean</span>. Here we are reporting concentration and isotope data for Zn in river waters and suspended sediments from the Loire River <span class="hlt">Basin</span>. In addition, we also report concentration and isotope data for the different industrial sources within the Loire <span class="hlt">Basin</span>, as well as data for biota samples such as mussels and oysters from the Bay of Biscay and North Brittany. These organisms are known to be natural accumulators of metal pollutants. Zinc isotopic compositions are rather homogeneous in river waters with δ66Zn values ranging from 0.21 to 0.39‰. This range of variation is very different from anthropogenic signature (industrial and/or agriculture release) that displays δ66Zn values between 0.02 to 0.14‰. This result is in agreement with a geogenic origin and the low Zn concentrations in the Loire River <span class="hlt">Basin</span> (from 0.8 to 6 µg/L).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A23O..06F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A23O..06F"><span>Madden-Julian Oscillation: Western Pacific and Indian <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fuchs, Z.; Raymond, D. J.</p> <p>2016-12-01</p> <p>The MJO has been and still remains a "holy grail" of today's atmospheric science research. Why does the MJO propagate eastward? What makes it unstable? What is the scaling for the MJO, i.e. why does it prefer long wavelengths or planetary wavenumbers 1-3? The MJO has the strongest signal in the Indian <span class="hlt">ocean</span> and in the West Pacific, but the average vertical structure is very different in each of those <span class="hlt">basins</span>. We look at the reanalysis/analysis FNL, ERAI vertical structure of temperature and moisture as well as the surface zonal winds for two <span class="hlt">ocean</span> <span class="hlt">basins</span>. We also look at data from DYNAMO and TOGA_COARE in great detail (saturation fraction, temperature, entropy, surface zonal winds, gross moist stability, etc). The findings from observations and field projects for the two <span class="hlt">ocean</span> <span class="hlt">basins</span> are then compared to a linear WISHE model on an equatorial beta plane. Though linear WISHE has long been discounted as a plausible model for the MJO, the version we have developed explains many of the observed features of this phenomenon, in particular, the preference for large zonal scale, the eastward propagation, the westward group velocity, and the thermodynamic structure. There is no need to postulate large-scale negative gross moist stability, as destabilization occurs via WISHE at long wavelengths only. This differs from early WISHE models because we take a moisture adjustment time scale of order one day in comparison to the much shorter time scales assumed in earlier models. Linear modeling cannot capture all of the features of the MJO, so we are in the process of adding nonlinearity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApWS....7.1161D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApWS....7.1161D"><span>Identifying the groundwater <span class="hlt">basin</span> boundaries, using environmental isotopes: a case study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Demiroğlu, Muhterem</p> <p>2017-06-01</p> <p>Groundwater, which is renewable under current climatic conditions separately from other natural sources, in fact is a finite resource in terms of quality and fossil groundwater. Researchers have long emphasized the necessity of exploiting, operating, conserving and managing groundwater in an efficient and sustainable manner with an integrated water management approach. The management of groundwater needs reliable information about changes on groundwater quantity and quality. Environmental isotopes are the most important tools to provide this support. No matter which method we use to calculate the groundwater budget and flow equations, we need to determine boundary conditions or the physical boundaries of the domain. The Groundwater divide line or <span class="hlt">basin</span> boundaries that separate the two <span class="hlt">adjacent</span> <span class="hlt">basin</span> recharge areas from each other must be drawn correctly to be successful in defining complex groundwater <span class="hlt">basin</span> boundary conditions. Environmental isotope data, as well as other methods provide support for determining recharge areas of the aquifers, especially for karst aquifers, residence time and interconnections between aquifer systems. This study demonstrates the use of environmental isotope data to interpret and correct groundwater <span class="hlt">basin</span> boundaries giving as an example the Yeniçıkrı <span class="hlt">basin</span> within the main Sakarya <span class="hlt">basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5506170-ocean-resources-economic-outlook','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5506170-ocean-resources-economic-outlook"><span><span class="hlt">Ocean</span> resources: an economic outlook</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>Covey, C.W.</p> <p>1985-10-01</p> <p>The scope and dimension of traditional marine activities in economic and marketing terms, e.g., offshore oil and gas, marine transportation, commercial fisheries, marine recreation, hard minerals recovery, and coastal zone activity, are reviewed. The economic outlook for <span class="hlt">ocean</span> resources is discussed under the following topics: (1) jurisdiction of <span class="hlt">adjacent</span> waters, (2) the coastal zone, (3) offshore oil and gas, (4) marine transport/shipbuilding, (5) national security, (6) commercial fisheries, (7) marine recreation, (8) hard minerals, and (9) future development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/of/1982/0445/report.pdf','USGSPUBS'); return false;" href="https://pubs.usgs.gov/of/1982/0445/report.pdf"><span>Aquifer systems in the Great <span class="hlt">Basin</span> region of Nevada, Utah, and <span class="hlt">adjacent</span> states: A study plan</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Harrill, James R.; Welch, Alan H.; Prudic, David E.; Thomas, James M.; Carman, Rita L.; Plume, Russell W.; Gates, Joseph S.; Mason, James L.</p> <p>1983-01-01</p> <p>The Great <span class="hlt">Basin</span> Regional Aquifer Study includes about 140,000 square miles in parts of Nevada, Utah, California, Idaho, Oregon, and Arizona. Within that area, 240 hydrographic areas occupy structural depressions formed primarily by <span class="hlt">basin</span>-and-range faulting. The principal aquifers are in <span class="hlt">basin</span>- fill deposits; however, permeable carbonate rocks underlie valleys in much of eastern Nevada and western Utah and are significant regional aquifers. Anticipated future water needs require a better understanding of the resource so that wise management will be possible. In October 1980, the U.S Geological Survey started a 4-year study to (1) describe the ground-water systems as they existed under natural conditions and as they exist today, (2) analyze the changes that have led to the systems' present condition, (3) tie the results of this and previous studies together in a regional analysis, and (4) provide means by which effects of future ground-water development can be estimated.A plan of work is presented that describes the general approach to be taken in this study. It defines (1) the major task necessary to meet objectives and (2) constraints on the scope of work. The approach has been strongly influenced by the diverse nature of ground-water flow systems and the large number of <span class="hlt">basins</span>. A detailed appraisal of 240 individual areas would require more resources than are available. Consequently, the general approach is to study selected "typical" areas and key hydrologic processes. Effort during the first 3 years will be directed toward describing the regional hydrology, conducting detailed studies of "type" areas, and studying selected hydrologic processes. Effort during the final year will be directed toward developing a regional analyses of results.Special studies that will address hydrologic processes, key components of the ground-water system, and improved use of technology include evaluations of regional geochemistry, regional hydrogeology, recharge, ground</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1213875S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1213875S"><span>Arctic <span class="hlt">Ocean</span> circulation during the anoxic Eocene Azolla event</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Speelman, Eveline; Sinninghe Damsté, Jaap; März, Christian; Brumsack, Hans; Reichart, Gert-Jan</p> <p>2010-05-01</p> <p>The Azolla interval, as encountered in Eocene sediments from the Arctic <span class="hlt">Ocean</span>, is characterized by organic rich sediments ( 4wt% Corg). In general, high levels of organic matter may be caused by increased productivity, i.e. extensive growth of Azolla, and/or enhanced preservation of organic matter, or a combination of both. Anoxic (bottom) water conditions, expanded oxygen minimum zones, or increased sedimentation rates all potentially increase organic matter preservation. According to plate tectonic, bathymetric, and paleogeographic reconstructions, the Arctic <span class="hlt">Ocean</span> was a virtually isolated shallow <span class="hlt">basin</span>, with one possible deeper connection to the Nordic Seas represented by a still shallow Fram Strait (Jakobsson et al., 2007), hampering ventilation of the Arctic <span class="hlt">Basin</span>. During the Azolla interval surface waters freshened, while at the same time bottom waters appear to have remained saline, indicating that the Arctic was highly stratified. The restricted ventilation and stratification in concert with ongoing export of organic matter most likely resulted in the development of anoxic conditions in the lower part of the water column. Whereas the excess precipitation over evaporation maintained the freshwater lid, sustained input of Nordic Sea water is needed to keep the deeper waters saline. To which degree the Arctic <span class="hlt">Ocean</span> exchanged with the Nordic Seas is, however, still largely unknown. Here we present a high-resolution trace metal record (ICP-MS and ICP-OES) for the expanded Early/Middle Eocene section capturing the Azolla interval from Integrated <span class="hlt">Ocean</span> Drilling Program (IODP) Expedition 302 (ACEX) drilled on the Lomonosov Ridge, central Arctic <span class="hlt">Ocean</span>. Euxinic conditions throughout the interval resulted in the efficient removal of redox sensitive trace metals from the water column. Using the sedimentary trace metal record we also constrained circulation in the Arctic <span class="hlt">Ocean</span> by assessing the relative importance of trace metal input sources (i.e. fluvial, eolian, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B24A..03B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B24A..03B"><span>Mercury genomics in the Arctic <span class="hlt">Ocean</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bowman, K.; Lamborg, C. H.; Collins, E.; Hammerschmidt, C. R.; Agather, A. M.</p> <p>2017-12-01</p> <p>Methyl-mercury production in the <span class="hlt">ocean</span> is likely dependent on microbial activity, however, methylation pathways remain elusive. In the Arctic, high concentrations of methyl-mercury are found in top predator marine mammals and seabirds. As a result of seafood consumption, pregnant women and women of child-bearing age in the Arctic often have blood Hg concentrations that exceed U.S. and Canadian safety guidelines. To understand the chemical cycling of mercury in the Arctic <span class="hlt">Ocean</span> we participated in the 2015 U.S. GEOTRACES Arctic expedition (GN01) to measure Hg speciation in the water column of the Bering Sea, Makarov <span class="hlt">basin</span>, and Canada <span class="hlt">basin</span> between Dutch Harbor, Alaska and the North Pole. At select stations, seawater was filtered through 0.22 µm Sterivex filters and genomic DNA was collected using a phenol-chloroform extraction. Broad-range degenerate PCR primers were used to detect the presence of hgcAB, and clade-specific degenerate quantitative PCR primers were used to determine the abundance of hgcA. Metagenomic sequencing was done at three stations to identify taxonomic and functional groups, and to search for hgcA-like genes that the PCR primers may have missed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://pubs.usgs.gov/ds/1025/ds1025.pdf','USGSPUBS'); return false;" href="http://pubs.usgs.gov/ds/1025/ds1025.pdf"><span>Water-level data for the Albuquerque <span class="hlt">Basin</span> and <span class="hlt">adjacent</span> areas, central New Mexico, period of record through September 30, 2015</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Beman, Joseph E.; Bryant, Christina F.</p> <p>2016-10-27</p> <p>The Albuquerque <span class="hlt">Basin</span>, located in central New Mexico, is about 100 miles long and 25–40 miles wide. The <span class="hlt">basin</span> is hydrologically defined as the extent of consolidated and unconsolidated deposits of Tertiary and Quaternary age that encompasses the structural Rio Grande Rift between San Acacia to the south and Cochiti Lake to the north. Drinking-water supplies throughout the <span class="hlt">basin</span> were obtained solely from groundwater resources until December 2008, when the Albuquerque Bernalillo County Water Utility Authority (ABCWUA) began treatment and distribution of surface water from the Rio Grande through the San Juan-Chama Drinking Water Project. A 20-percent population increase in the <span class="hlt">basin</span> from 1990 to 2000 and a 22-percent population increase from 2000 to 2010 may have resulted in an increased demand for water in areas within the <span class="hlt">basin</span>.An initial network of wells was established by the U.S. Geological Survey (USGS) in cooperation with the City of Albuquerque from April 1982 through September 1983 to monitor changes in groundwater levels throughout the Albuquerque <span class="hlt">Basin</span>. In 1983, this network consisted of 6 wells with analog-to-digital recorders and 27 wells where water levels were measured monthly. The network currently (2015) consists of 124 wells and piezometers. (A piezometer is a specialized well open to a specific depth in the aquifer, often of small diameter and nested with other piezometers open to different depths.) The USGS, in cooperation with the ABCWUA, currently (2015) measures and reports water levels from the 124 wells and piezometers in the network; this report presents water-level data collected by USGS personnel at those 124 sites through water year 2015 (October 1, 2014, through September 30, 2015).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017FrES...11..740A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017FrES...11..740A"><span>Major transgression during Late Cretaceous constrained by <span class="hlt">basin</span> sediments in northern Africa: implication for global rise in sea level</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>An, Kaixuan; Chen, Hanlin; Lin, Xiubin; Wang, Fang; Yang, Shufeng; Wen, Zhixin; Wang, Zhaoming; Zhang, Guangya; Tong, Xiaoguang</p> <p>2017-12-01</p> <p>The global rise in sea level during the Late Cretaceous has been an issue under discussion by the international geological community. Despite the significance, its impact on the deposition of continental <span class="hlt">basins</span> is not well known. This paper presents the systematic review on stratigraphy and sedimentary facies compiled from 22 continental <span class="hlt">basins</span> in northern Africa. The results indicate that the region was dominated by sediments of continental facies during Early Cretaceous, which were replaced by deposits of marine facies in Late Cretaceous. The spatio-temporal distribution of sedimentary facies suggests marine facies deposition reached as far south as Taoudeni-Iullemmeden-Chad-Al Kufra-Upper Egypt <span class="hlt">basins</span> during Turonian to Campanian. These results indicate that northern Africa underwent significant transgression during Late Cretaceous reaching its peak during Turonian to Coniacian. This significant transgression has been attributed to the global high sea-level during this time. Previous studies show that global rise in sea level in Late Cretaceous may have been driven by an increase in the volume of <span class="hlt">ocean</span> water (attributed to high CO2 concentration and subsequently warm climate) and a decrease in the volume of the <span class="hlt">ocean</span> <span class="hlt">basin</span> (attributed to rapid production of <span class="hlt">oceanic</span> crust and seamounts). Tectonic mechanism of rapid production of <span class="hlt">oceanic</span> crust and seamounts could play a fundamental role in driving the global rise in sea level and subsequent transgression in northern Africa during Late Cretaceous.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.C12B..01F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.C12B..01F"><span>Interactions of the Greenland Petermann Glacier with the <span class="hlt">ocean</span>: An initial perspective (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Falkner, K. K.; Johnson, H. L.; Melling, H.; Muenchow, A.; Samelson, R. M.; Friends Of Petermann</p> <p>2010-12-01</p> <p>Petermann Glacier is major outlet glacier that drains 6% of the area of the Greenland Ice Sheet in western North Greenland. It is one of four major outlet glaciers on Greenland with a grounding line substantially below sea level (about 500m) and one of two such glaciers to retain a substantial floating tongue. The floating ice tongue of Petermann glacier is thought to lose at least 80% of its mass through <span class="hlt">ocean</span> interaction. Based on three opportunistic <span class="hlt">ocean</span> surveys in Petermann Fjord, we present an overview of circulation at the fjord mouth, hydrographic structure beneath the ice tongue, <span class="hlt">oceanic</span> heat delivered to the under-ice cavity and the fate of the resulting melt water. We also present an historical perspective on the August 2010 major calving event. The 1100m-deep fjord is separated from neighboring Hall <span class="hlt">Basin</span> by a sill that is inferred to lie between 350m and 450m deep. Hall <span class="hlt">Basin</span> is a section of Nares Strait that connects the Arctic <span class="hlt">Ocean</span> (at the Lincoln Sea proceeding southward through Robeson Channel, Hall <span class="hlt">Basin</span>, Kennedy Channel, Kane <span class="hlt">Basin</span> and Smith Sound) to Baffin Bay. Sills in the Lincoln Sea (290m) and in Kane <span class="hlt">Basin</span> (220m) restrict communication with the Arctic <span class="hlt">Ocean</span> and Baffin Bay. The net flux of seawater through Nares Strait is southward and relatively fresh, conditioned by sources and processes within the Arctic <span class="hlt">Ocean</span> and locally. Within Petermann Fjord, glacial melt water appears on the northeast side at 200-600m. A cyclonic gyre occurs within the fjord mouth, with outflow on the northeast side. <span class="hlt">Oceanic</span> heat fluxes into the fjord are sufficient to account for the observed rate of basal melting. Cold, low salinity water intrudes far under the ice and likely limits basal melting to the inland half of the tongue. The recent major calving event resulted in a loss of 300 km2 or about 20% of the total area of the floating tongue, most of which remained intact as an ice island that garnered much media attention. Available observations show calving to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JAfES..58....1N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JAfES..58....1N"><span>Sedimentology and sequence stratigraphy from outcrops of the Kribi-Campo sub-<span class="hlt">basin</span>: Lower Mundeck Formation (Lower Cretaceous, southern Cameroon)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ntamak-Nida, Marie Joseph; Bourquin, Sylvie; Makong, Jean-Claude; Baudin, François; Mpesse, Jean Engelbert; Ngouem, Christophe Itjoko; Komguem, Paul Bertrand; Abolo, Guy Martin</p> <p>2010-08-01</p> <p>The Kribi-Campo sub-<span class="hlt">basin</span> is composed of an Early to Mid Cretaceous series from West Africa's Atlantic coast and is located in southern Cameroon in the Central African equatorial rain forest. It is the smallest coastal <span class="hlt">basin</span> in Cameroon and forms the southern part of the Douala/Kribi-Campo <span class="hlt">basin</span> known as Douala <span class="hlt">basin</span> ( s.l.). Until now, no detailed sedimentological studies have been carried out on the outcrops of this <span class="hlt">basin</span> located in the Campo area. The aim of this study was to characterise the depositional environments, vertical evolution and tectonic context of these Lower Cretaceous series in order to make a comparison with <span class="hlt">adjacent</span> <span class="hlt">basins</span> and replace them in the geodynamic context. Facies analysis of the Lower Mundeck Formation (Lower Cretaceous) indicates the presence of four major, interfigered facies associations, that are inferred to represent elements of an alluvial to lacustrine-fan delta system. The clast lithologies suggest proximity of relief supplying coarse-grained sediment during the deposition of the Lower Mundeck Formation at Campo. The general dip and direction of the bedding is approximately 10°-12°NW, which also corresponds to the orientation of the foliations in the underlying metamorphic basement. The main sedimentary succession is characterised by a major retrogradational/progradational cycle of Late Aptian age, evaluated at about 3 Ma, with a well-developed progradational trend characterised by fluctuations of the recognised depositional environments. Fluctuations in lake level and sediment supply were possibly controlled by active faults at the <span class="hlt">basin</span> margin, although climatic changes may have also played a role. The consistently W-WNW palaeoflow of sediments suggests that the palaeorelief was located to the east and could be oriented in a NNE-SSW direction, downthrown to the west. Local outcrops dated as Albian, both north and south of the main outcrop, display some marine influence. These deposits are cut by 040-060 faults parallel to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.T11D2923L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.T11D2923L"><span>Determining Crustal Structure beneath the New Madrid Seismic Zone and <span class="hlt">Adjacent</span> Areas: Application of a Reverberation-removal Filter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, L.; Gao, S. S.; Liu, K. H.</p> <p>2015-12-01</p> <p>The New Madrid Seismic Zone (NMSZ) and some of the <span class="hlt">adjacent</span> areas are covered by a low-velocity sedimentary sequence, giving rise to strong reverberations in the P-to-S receiver functions (RFs) and making it difficult to reliably determine crustal thickness and Poisson's ratio using the conventional H-k stacking technique. Here we apply a newly developed technique (Yu et al., 2015; doi: 10.1002/2014JB011610) to effectively remove or reduce the reverberations from the sedimentary layer to obtain more reliable results. Stacking of a total of 38528 radial RFs recorded by 343 stations in the study area shows systematic spatial variations in crustal thickness (H), Vp/Vs ratio and amplitude (R; relative to the direction P) of the converted Moho phases. Our results indicate that the upper Mississippi Embayment (ME), a broad southwest-plunging trough with the thickest sedimentary layer in the study area, is characterized by a thin crustal thickness (~32 km), while <span class="hlt">adjacent</span> areas have relatively thicker crust (>40 km). This area also possesses relatively large Vp/Vs (>1.85) values, suggesting possible intrusion of mantle-derived mafic rocks. Most part of the Ozark Uplift is characterized by relatively small Vp/Vs (<1.79) values which indicate an overall felsic crust. In contrast to the NMSZ which is part of the Reelfoot rift, the southern Illinois <span class="hlt">Basin</span>, which is an intracontinental sag <span class="hlt">basin</span>, is characterized by a crust of about 45 km which is a few km thicker than the surrounding areas, and a normal Vp/Vs, suggesting sharp differences in crustal structure between rift and sag <span class="hlt">basins</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AGUFMOS21A1571K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AGUFMOS21A1571K"><span>Are Salps A Silver Bullet Against Global Warming And <span class="hlt">Ocean</span> Acidification?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kithil, P. W.</p> <p>2006-12-01</p> <p> solar panel to power communications & provide remote control. <span class="hlt">Adjacent</span> pumps are connected at the bottom to maintain relative position. If required, periodic seafloor anchoring can maintain absolute position within an <span class="hlt">ocean</span> <span class="hlt">basin</span>. Deployment is low cost as the pumps self-deploy when dropped into the <span class="hlt">ocean</span> from barges. Pumps would not be deployed in <span class="hlt">ocean</span> shipping channels, regions used by recreational boaters, nor where excessive tides or currents exist. In a global application, 1,340 arrays each 100,000 km2 are needed to cover the 134 million km2 calculated above. Assuming one pump per square km costing 2,000, an investment of 268 billion is needed. Using a five year payback, this investment is recouped if the carbon credit price is 26.80 per ton applied to sequestering 1.96 billion tons per year of carbon. This is not dramatically different from today's carbon credit price of about 15 per ton. Assuming a governmental mandate of carbon sequestration, today's price could easily increase many-fold, making <span class="hlt">ocean</span> sequestration using forced upwelling economically attractive. Additional benefits of widespread forced upwelling include: 1 Buffering of <span class="hlt">ocean</span> pH by removing CO2 during photosynthesis; 2 Possible cooling the upper mixed layer upstream from coral reefs to reduce bleaching from <span class="hlt">ocean</span> hotspots; 3 Possible mitigation of rapid climate change by enhancing the mixing of arctic/Greenland meltwater; 4 Enhancement of wild fish populations; and, 5 Reduced hurricane intensity, achieved by cooling the upper mixed layer upon approach of a tropical storm in high risk regions such as the Gulf of Mexico.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70020995','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70020995"><span>Geochemistry of waters from springs, wells, and snowpack on and <span class="hlt">adjacent</span> to Medicine Lake volcano, 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>Mariner, R.H.; Lowenstern, Jacob B.</p> <p>1999-01-01</p> <p>Chemical analyses of waters from cold springs and wells of the Medicine Lake volcano and surrounding region indicate small chloride anomalies that may be due to water-rock interaction or limited mixing with high-temperature geothermal fluids. The Fall River Springs (FRS) with a combined discharge of approximately 37 m3/s, show a negative correlation between chloride (Cl) and temperature, implying that the Cl is not derived from a high-temperature geothermal fluid. The high discharge from the FRS indicates recharge over a large geographic region. Chemical and isotopic variations in the FRS show that they contain a mixture of three distinct waters. The isotopic composition of recharge on and <span class="hlt">adjacent</span> to the volcano are estimated from the isotopic composition of snow and precipitation amounts adjusted for evapotranspiration. Enough recharge of the required isotopic composition (-100 parts per thousand ??D) is available from a combination of the Medicine Lake caldera, the Fall River <span class="hlt">basin</span> and the Long Bell <span class="hlt">basin</span> to support the slightly warmer components of the FRS (32 m3/s). The cold-dilute part of the FRS (approximately 5 m3/s) may recharge in the Bear Creek <span class="hlt">basin</span> or at lower elevations in the Fall River <span class="hlt">basin</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6533797-carbonate-platform-slope-basinal-deposits-upper-oligocene-kalimantan-indonesia','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6533797-carbonate-platform-slope-basinal-deposits-upper-oligocene-kalimantan-indonesia"><span>Carbonate platform, slope, and <span class="hlt">basinal</span> deposits of Upper Oligocene, Kalimantan, Indonesia</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>Armin, R.A.; Cutler, W.G.; Mahadi, S.</p> <p>1987-05-01</p> <p>Upper Oligocene platform carbonates (Berai Formation) occur extensively on the Barito shelf in southeastern Kalimantan (Borneo) and are flanked northward by coeval slope and <span class="hlt">basinal</span> deposits (Bongan Formation) which accumulated in the southwestern part of the Kutei <span class="hlt">basin</span>. Isolated carbonate buildups equivalent to the Berai Formation also occur within the Kutei <span class="hlt">basin</span> and were probably deposited on basement highs. The distribution of these facies is fairly well constrained by the study of outcrops, wells, and seismic profiles. The Berai Formation consists of diverse limestone types with a wide range of textures and with dominant skeletal components of large foraminifera, redmore » algae, and corals. Deposition of the Berai Formation occurred in moderate- and high-energy shallow-marine conditions. Slope and <span class="hlt">basin</span> facies occur in extensional <span class="hlt">basins</span> <span class="hlt">adjacent</span> to the shelfal carbonates and peripheral to isolated carbonate buildups. Slope deposits consist of hemipelagic claystone, debris-flow conglomerate, calciturbidite, and volcaniclastic intervals. syndepositional downslope transport of slope deposits was an important process, as indicated by intervals containing redeposited debris flows, intraformational truncation surfaces, slide blocks, and associated shear planes. Recurrent movement on <span class="hlt">basin</span>-margin faults and local volcanism probably perpetuated instability of slope deposits. <span class="hlt">Basinal</span> deposits consist of calcareous claystone with intercalated thin, distal calciturbidite and volcaniclastic beds.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1614836P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1614836P"><span>Trends in Arctic <span class="hlt">Ocean</span> bottom pressure, sea surface height and freshwater content using GRACE and the ice-<span class="hlt">ocean</span> model PIOMAS from 2008-2012</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peralta-Ferriz, Cecilia; Morison, James; Zhang, Jinlun; Bonin, Jennifer</p> <p>2014-05-01</p> <p>The variability of <span class="hlt">ocean</span> bottom pressure (OBP) in the Arctic is dominated by the variations in sea surface height (SSH) from daily to monthly timescales. Conversely, OBP variability is dominated by the changes in the steric pressure (StP) at inter-annual timescales, particularly off the continental shelves. The combination of GRACE-derived <span class="hlt">ocean</span> bottom pressure and ICESat altimetry-derived sea surface height variations in the Arctic <span class="hlt">Ocean</span> have provided new means of identifying inter-annual trends in StP (StP = OBP-SSH) and associated freshwater content (FWC) of the Arctic region (Morison et al., 2012). Morison et al. (2012) showed that from 2004 to 2008, the FWC increased in the Beaufort Gyre and decreased in the Siberian and Central Arctic, resulting in a relatively small net <span class="hlt">basin</span>-averaged FWC change. In this work, we investigate the inter-annual trends from 2008 to 2012 in OBP from GRACE, SSH from the state-of-the-art pan-Arctic <span class="hlt">ocean</span> model PIOMAS -validated with tide and pressure gauges in the Arctic-, and compute the trends in StP and FWC from 2008-2012. We compare these results with the previous trends from 2005-2008 described in Morison et al. (2012). Our initial findings suggest increased salinity in the entire Arctic <span class="hlt">basin</span> (relative to the climatological seasonal variation) from 2008-2012, compared to the preceding four years (2005-2008). We also find that the trends in OBP, SSH and StP from 2008-2012 present a different behavior during the spring-summer and fall-winter, unlike 2005-2008, in which the trends were generally consistent through all months of the year. It seems since 2009, when the Beaufort Gyre relaxed and the export of freshwater from the Canada <span class="hlt">Basin</span> into the Canadian Archipelago and Fram Strait, via the Lincoln Sea, was anomalously large (de Steur et al., 2013), the Arctic <span class="hlt">Ocean</span> has entered a new circulation regime. The causes of such changes in the inter-annual trends of OBP, SSH and StP -hence FWC-, associated with the changes in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSAES..64..452F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSAES..64..452F"><span>Evolution of the Neogene Andean foreland <span class="hlt">basins</span> of the Southern Pampas and Northern Patagonia (34°-41°S), Argentina</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Folguera, Alicia; Zárate, Marcelo; Tedesco, Ana; Dávila, Federico; Ramos, Victor A.</p> <p>2015-12-01</p> <p>The Pampas plain (30°-41°S) has historically been considered as a sector that evolved independently from the <span class="hlt">adjacent</span> Andean ranges. Nevertheless, the study of the Pampas showed that it is reasonable to expect an important influence from the Andes into the extraandean area. The Pampas plain can be divided into two sectors: the northern portion, <span class="hlt">adjacent</span> to the Pampean Ranges, has been studied by Davila (2005, 2007, 2010). The southern sector (34°-41°S) is the objective of the present work. The study of this area allowed to characterize two separate foreland <span class="hlt">basins</span>: the Southern Pampa <span class="hlt">basin</span> and the Northern Patagonian <span class="hlt">basin</span>. The infill is composed of Late Miocene and Pliocene units, interpreted as distal synorogenic sequences associated with the late Cenozoic Andean uplift at this latitudinal range. These foreland <span class="hlt">basins</span> have been defined based on facies changes, distinct depositional styles, along with the analysis of sedimentary and isopach maps. The <span class="hlt">basins</span> geometries are proposed following De Celles and Gilles (1996) taking into account the infill geometry, distribution and grain size. In both cases, these depocenters are located remarkably far away from the Andean tectonics loads. Therefore they cannot be explained with short-wave subsidence patterns. Elastic models explain the tectonic subsidence in the proximal depocenters but fail to replicate the complete distal <span class="hlt">basins</span>. These characteristics show that dynamic subsidence is controlling the subsidence in the Southern Pampas and Northern Patagonian <span class="hlt">basins</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_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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