Sample records for subantarctic mode water

  1. Comparison of Subantarctic Mode Water and Antarctic Intermediate Water formation rates in the South Pacific between NCAR-CCSM4 and observations

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

    Hartin, Corinne A.; Fine, Rana A.; Kamenkovich, Igor

    2014-01-28

    Average formation rates for Subantarctic Mode (SAMW) and Antarctic Intermediate Waters (AAIW) in the South Pacific are calculated from the National Center for Atmospheric Research Community Climate System Model version 4 (NCAR-CCSM4), using chlorofluorocarbon inventories. CFC-12 inventories and formation rates are compared to ocean observations. CCSM4 accurately simulates the southeast Pacific as the main formation region for SAMW and AAIW. CCSM4 formation rates for SAMW are 3.4 Sv, about half of the observational rate. Shallow mixed layers and a thinner SAMW in CCSM4 are responsible for lower formation rates. A formation rate of 8.1 Sv for AAIW in CCSM4 ismore » higher than observations. Higher inventories in CCSM4 in the southwest and central Pacific, and higher surface concentrations are the main reasons for higher formation rates of AAIW. This comparison of model and observations is useful for understanding the uptake and transport of other gases, e.g., CO2 by the model.« less

  2. Distribution, abundance and seasonal flux of pteropods in the Sub-Antarctic Zone

    NASA Astrophysics Data System (ADS)

    Howard, W. R.; Roberts, D.; Moy, A. D.; Lindsay, M. C. M.; Hopcroft, R. R.; Trull, T. W.; Bray, S. G.

    2011-11-01

    Pteropods were identified from epipelagic net and trawl samples in the Sub-Antarctic Zone during the 2007 mid-summer (January 17-February 20) Sub-Antarctic Zone Sensitivity to Environmental Change (SAZ-Sense) voyage, as well as in a moored sediment trap in the same region. Overall pteropod densities during SAZ-Sense were lower than those reported for higher-latitude Southern Ocean waters. The four major contributors to the Sub-Antarctic Zone pteropod community during the SAZ-Sense voyage, Clio pyramidata forma antarctica, Clio recurva, Limacina helicina antarctica and Limacina retroversa australis, accounted for 93% of all pteropods observed. The distribution of the two dominant pteropods collected in the Sub-Antarctic Zone, L. retroversa australis and C. pyramidata forma antarctica, is strongly related to latitude and depth. L. retroversa australis is typical of cold southern (50-54°S) polar waters and C. pyramidata forma antarctica is typical of shallow (top 20 m) Sub-Antarctic Zone waters. A moored sediment trap deployed to 2100 m at 47°S, 141°E in 2003/04 showed the pteropod flux in the Sub-Antarctic Zone had late-Spring and mid-summer peaks. The diversity, abundance and distribution of pteropods collected during SAZ-Sense provide a timely benchmark against which to monitor future changes in SAZ ocean pteropod communities, particularly in light of predictions of declining aragonite saturation in the Southern Ocean by the end of the century.

  3. Kelp genes reveal effects of subantarctic sea ice during the Last Glacial Maximum

    PubMed Central

    Fraser, Ceridwen I.; Nikula, Raisa; Spencer, Hamish G.; Waters, Jonathan M.

    2009-01-01

    The end of the Last Glacial Maximum (LGM) dramatically reshaped temperate ecosystems, with many species moving poleward as temperatures rose and ice receded. Whereas reinvading terrestrial taxa tracked melting glaciers, marine biota recolonized ocean habitats freed by retreating sea ice. The extent of sea ice in the Southern Hemisphere during the LGM has, however, yet to be fully resolved, with most palaeogeographic studies suggesting only minimal or patchy ice cover in subantarctic waters. Here, through population genetic analyses of the widespread Southern Bull Kelp (Durvillaea antarctica), we present evidence for persistent ice scour affecting subantarctic islands during the LGM. Using mitochondrial and chloroplast genetic markers (COI; rbcL) to genetically characterize some 300 kelp samples from 45 Southern Ocean localities, we reveal a remarkable pattern of recent recolonization in the subantarctic. Specifically, in contrast to the marked phylogeographic structure observed across coastal New Zealand and Chile (10- to 100-km scales), subantarctic samples show striking genetic homogeneity over vast distances (10,000-km scales), with a single widespread haplotype observed for each marker. From these results, we suggest that sea ice expanded further and ice scour during the LGM impacted shallow-water subantarctic marine ecosystems more extensively than previously suggested. PMID:19204277

  4. Controls and variability of solute and sedimentary fluxes in Antarctic and sub-Antarctic Environments

    NASA Astrophysics Data System (ADS)

    Zwolinski, Zbigniew

    2015-04-01

    . Solute and sediment transport in the streams of analyzed environments are constrained by the relatively short water runoff season that typically lasts from a few weeks to maximum of four months during the austral summer, for Antarctic and sub-Antarctic regions respectively. Because of high intensity of mechanical and chemical weathering processes solute and sediment transport are rather high within Antarctic environments. Weathering rates on slopes and magnitude of fluvial transport in relatively short streams control the intensity of denudational processes. Both mechanical and chemical denudation varies highly through sub-Antarctic and Antarctic environments. To generate accurate predictions of fluvial and denudational processes we must fully understand the actual geoecological processes, which in some places are under rapid change, e.g., the Antarctic Peninsula and sub-Antarctic islands.

  5. Impact of the Agulhas Return Current on the glacial Subantarctic region in the South Indian Ocean

    NASA Astrophysics Data System (ADS)

    Ikehara, M.; Crosta, X.; Manoj, M. C.

    2017-12-01

    The Southern Ocean has played an important role in the evolution of the global climate system. The Southern Ocean circulation is dominated by the Antarctic Circumpolar Current (ACC), the world's longest and largest current system. Sea ice coverage on sea surface strongly affects the climate of the Southern Hemisphere through its impacts on the energy and gas budget, on the atmospheric circulation, on the hydrological cycle, and on the biological productivity. The Agulhas Return Current (ARC) originates from the Agulhas Current, the major western boundary current in the Indian Ocean, and transports heat from subtropical to subantarctic region. It's thought that the Agulhas leakage from the Indian Ocean to the Atlantic was reduced for the last glacial due to a northward shift of the westerlies and ACC, however, there are still unknown yet how the ARC was responded to the reduced Agulhas leakage. A piston core DCR-1PC was collected from the Del Caño Rise (46°S, 44°E, 2632m), Indian sector of the Southern Ocean. Core site located in the Subantarctic region between the Subtropical Front (STF) and Subantarctic Front (SAF). Age model of the core was established by radiocarbon dating of planktic foraminifer Globorotalia bulloides and oxygen isotope stratigraphy of benthic foraminifers Cibicidoides wuellerstorfi and Melonis bareelanus. Sediment of DCR-1PC show the cyclic changes of diatom/carbonate ooze sedimentation corresponding to Southern Ocean fronts' migrations on glacial-interglacial timescales. Records of ice-rafted debris (IRD) and oxygen isotope in planktic foraminfer G. bulloides suggest that the melting of sea ice was significantly increased during the last glacial maximum (LGM) in the Subantarctic surface water. Diatom assemblage based summer SST also shows the relative warmer condition in the Subantarctic during the LGM. These results might be explained by the strong influence of the Agulhas Return Current during the LGM in the Subantarctic. The reduced

  6. Air-sea interaction regimes in the sub-Antarctic Southern Ocean and Antarctic marginal ice zone revealed by icebreaker measurements

    NASA Astrophysics Data System (ADS)

    Yu, Lisan; Jin, Xiangze; Schulz, Eric W.; Josey, Simon A.

    2017-08-01

    This study analyzed shipboard air-sea measurements acquired by the icebreaker Aurora Australis during its off-winter operation in December 2010 to May 2012. Mean conditions over 7 months (October-April) were compiled from a total of 22 ship tracks. The icebreaker traversed the water between Hobart, Tasmania, and the Antarctic continent, providing valuable in situ insight into two dynamically important, yet poorly sampled, regimes: the sub-Antarctic Southern Ocean and the Antarctic marginal ice zone (MIZ) in the Indian Ocean sector. The transition from the open water to the ice-covered surface creates sharp changes in albedo, surface roughness, and air temperature, leading to consequential effects on air-sea variables and fluxes. Major effort was made to estimate the air-sea fluxes in the MIZ using the bulk flux algorithms that are tuned specifically for the sea-ice effects, while computing the fluxes over the sub-Antarctic section using the COARE3.0 algorithm. The study evidenced strong sea-ice modulations on winds, with the southerly airflow showing deceleration (convergence) in the MIZ and acceleration (divergence) when moving away from the MIZ. Marked seasonal variations in heat exchanges between the atmosphere and the ice margin were noted. The monotonic increase in turbulent latent and sensible heat fluxes after summer turned the MIZ quickly into a heat loss regime, while at the same time the sub-Antarctic surface water continued to receive heat from the atmosphere. The drastic increase in turbulent heat loss in the MIZ contrasted sharply to the nonsignificant and seasonally invariant turbulent heat loss over the sub-Antarctic open water.Plain Language SummaryThe icebreaker Aurora Australis is a research and supply vessel that is regularly chartered by the Australian Antarctic Division during the southern summer to operate in <span class="hlt">waters</span> between Hobart, Tasmania, and Antarctica. The vessel serves as the main lifeline to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24687148','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24687148"><span>On Hokusai's Great wave off Kanagawa: localization, linearity and a rogue wave in <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dudley, J M; Sarano, V; Dias, F</p> <p>2013-06-20</p> <p>The Hokusai woodcut entitled The great wave off Kanagawa has been interpreted as an unusually large storm wave, likely to be classed as a rogue wave, and possibly generated from nonlinear wave dynamics (J. H. E. Cartwright and H. Nakamura, Notes Rec. R. Soc. 63 , 119-135 (2009)). In this paper, we present a complementary discussion of this hypothesis, discussing in particular how linear and nonlinear mechanisms can both contribute to the emergence of rogue wave events. By making reference to the Great wave 's simultaneous transverse and longitudinal localization, we show that the purely linear mechanism of directional focusing also predicts characteristics consistent with those of the Great wave . In addition, we discuss the properties of a particular rogue wave photographed on the open ocean in <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span>, which shows two-dimensional localization and breaking dynamics remarkably similar to Hokusai's depiction in the woodcut.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3645210','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3645210"><span>On Hokusai's Great wave off Kanagawa: localization, linearity and a rogue wave in <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</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>Dudley, J. M.; Sarano, V.; Dias, F.</p> <p>2013-01-01</p> <p>The Hokusai woodcut entitled The great wave off Kanagawa has been interpreted as an unusually large storm wave, likely to be classed as a rogue wave, and possibly generated from nonlinear wave dynamics (J. H. E. Cartwright and H. Nakamura, Notes Rec. R. Soc. 63, 119–135 (2009)). In this paper, we present a complementary discussion of this hypothesis, discussing in particular how linear and nonlinear mechanisms can both contribute to the emergence of rogue wave events. By making reference to the Great wave's simultaneous transverse and longitudinal localization, we show that the purely linear mechanism of directional focusing also predicts characteristics consistent with those of the Great wave. In addition, we discuss the properties of a particular rogue wave photographed on the open ocean in <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span>, which shows two-dimensional localization and breaking dynamics remarkably similar to Hokusai's depiction in the woodcut. PMID:24687148</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26267259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26267259"><span>The skin of Commerson's dolphins (Cephalorhynchus commersonii) as a biomonitor of mercury and selenium in <span class="hlt">Subantarctic</span> <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cáceres-Saez, Iris; Goodall, R Natalie P; Dellabianca, Natalia A; Cappozzo, H Luis; Ribeiro Guevara, Sergio</p> <p>2015-11-01</p> <p>The skin of bycaught Commerson's dolphins was tested for mercury (Hg) and selenium (Se) biomonitoring in <span class="hlt">Subantarctic</span> environments. The correlation of levels detected in the skin with those found in internal tissues - lung, liver, kidney and muscle - was assessed to evaluate how skin represents internal Hg and Se distribution for monitoring purposes. Mercury in skin had a concentration range of 0.68-3.11 μg g(-1) dry weight (DW), while Se had a higher concentration range of 74.3-124.5 μg g(-1) DW. There was no significant correlation between selenium levels in any of the analyzed tissues. Thus, the skin selenium concentration did not reflect the tissular Se levels and did not provide information for biomonitoring. The lack of correlation is explained by the biological role of Se, provided that each tissue regulates Se levels according to physiological needs. However, the skin Hg level had significant positive correlation with the levels in internal tissues (ANOVA p<0.05), particularly with that of muscle (R(2)=0.79; ANOVA p=0.0008). Thus, this correlation permits the estimation of Hg content in muscle based on the multiplication of skin biopsy levels by a factor of 1.85. Mercury bioindication using skin biopsies is a non-lethal approach that allows screening of a large number of specimens with little disturbance and makes possible an adequate sampling strategy that produces statistically valid results in populations and study areas. The correlation between Hg levels in the skin and internal tissues supports the use of the epidermis of Commerson's dolphins for Hg biomonitoring in the <span class="hlt">waters</span> of the <span class="hlt">Subantarctic</span>, which is a poorly studied region regarding Hg levels, sources and processes. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A21L..02M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A21L..02M"><span>Iron fertilization of the <span class="hlt">Subantarctic</span> Ocean during the last ice age</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martinez-Garcia, A.</p> <p>2015-12-01</p> <p>Dust has the potential to modify global climate by influencing the radiative balance of the atmosphere and by supplying iron and other essential limiting micronutrients to the ocean. The scarcity of iron limits marine productivity and carbon uptake in one-quarter of the world ocean where the concentration of major nutrients (phosphorus and nitrogen) is perennially high. The Southern Ocean is the region where variations in iron availability can have the largest effect on Earth's carbon cycle through its fertilizing effect on marine ecosystems. Paleoceanographic records from the <span class="hlt">Subantarctic</span> Atlantic have revealed a remarkable correlation between phytoplankton productivity and aeolian iron flux during glacial periods supporting the iron fertilization hypothesis. In addition, a recent study has shown that peak glacial times and millennial cold events were nearly universally associated not only with increases in dust flux and export production, but also with an increase in nutrient consumption (the last indicated by higher foraminifera-bound δ15N) (Martinez-Garcia et al. 2014). This combination of changes is uniquely consistent with ice age iron fertilization of the <span class="hlt">Subantarctic</span> Atlantic. The strengthening of the biological pump associated with the observed increase in <span class="hlt">Subantarctic</span> nutrient consumption during the high-dust intervals of the last two ice ages can explain up to ~40 ppm of the CO2 decrease that characterizes the transitions from mid-climate states to full ice age conditions. However, the impact of iron fertilization in other sectors of the Southern Ocean characterized by lower ice age dust fluxes than the Atlantic remains unclear. A series of recently published records from the <span class="hlt">Subantarctic</span> Pacific indicate that dust deposition and marine export production were three times higher during glacial periods than during interglacials (Lamy et al. 2014). Here we present new measurements of foraminifera-bound nitrogen isotopes in a sediment core located in the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26800986','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26800986"><span>Sensitivity of six <span class="hlt">subantarctic</span> marine invertebrates to common metal contaminants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Holan, Jessica R; King, Catherine K; Davis, Andrew R</p> <p>2016-09-01</p> <p>A long history of anthropogenic activities in the relatively pristine <span class="hlt">subantarctic</span> has resulted in areas of accumulated waste and contaminants. Sensitivities to metals of <span class="hlt">subantarctic</span> and Antarctic species may contrast with related species from temperate and tropical areas because of the unique characteristics of polar biota. In addition, response to contaminants may be delayed, and hence longer exposure periods may be required in toxicity tests with polar species. In the present study, the sensitivity of 6 common <span class="hlt">subantarctic</span> marine invertebrates to copper, zinc, and cadmium contaminants was determined. Large variations in sensitivities, both between species and between metals within species, were found. The bivalve Gaimardia trapesina and the copepod Harpacticus sp. were the most sensitive to copper, with 7-d median lethal concentration (LC50) values for both species ranging between 28 μg/L and 62 μg/L, whereas the copepod Tigriopus angulatus was the most tolerant of copper (7-d Cu LC50 1560 μg/L). Sensitivity to zinc varied by approximately 1 order of magnitude between species (7-d LC50: 329-3057 μg/L). Sensitivity to cadmium also varied considerably between species, with 7-d LC50 values ranging from 1612 μg/L to >4383 μg/L. The present study is the first to report the sensitivity of <span class="hlt">subantarctic</span> marine invertebrate to metals, and contributes significantly to the understanding of latitudinal gradients in the sensitivity of biota to metals. Although sensitivity is highly variable between species, in a global comparison of copepod data, it appears that species from higher latitudes may be more sensitive to copper. Environ Toxicol Chem 2016;35:2245-2251. © 2016 SETAC. © 2016 SETAC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CliPa..13.1301B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CliPa..13.1301B"><span>Late Holocene intensification of the westerly winds at the <span class="hlt">subantarctic</span> Auckland Islands (51° S), New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Browne, Imogen M.; Moy, Christopher M.; Riesselman, Christina R.; Neil, Helen L.; Curtin, Lorelei G.; Gorman, Andrew R.; Wilson, Gary S.</p> <p>2017-10-01</p> <p>The Southern Hemisphere westerly winds (SHWWs) play a major role in controlling wind-driven upwelling of Circumpolar Deep <span class="hlt">Water</span> (CDW) and outgassing of CO2 in the Southern Ocean, on interannual to glacial-interglacial timescales. Despite their significance in the global carbon cycle, our understanding of millennial- and centennial-scale changes in the strength and latitudinal position of the westerlies during the Holocene (especially since 5000 yr BP) is limited by a scarcity of palaeoclimate records from comparable latitudes. Here, we reconstruct middle to late Holocene SHWW variability using a fjord sediment core collected from the <span class="hlt">subantarctic</span> Auckland Islands (51° S, 166° E), located in the modern centre of the westerly wind belt. Changes in drainage basin response to variability in the strength of the SHWW at this latitude are interpreted from downcore variations in magnetic susceptibility (MS) and bulk organic δ13C and atomic C / N, which monitor influxes of lithogenous and terrestrial vs. marine organic matter, respectively. The fjord <span class="hlt">water</span> column response to SHWW variability is evaluated using benthic foraminifer δ18O and δ13C, both of which are influenced by the isotopic composition of shelf <span class="hlt">water</span> masses entering the fjord. Using these data, we provide marine and terrestrial-based evidence for increased wind strength from ˜ 1600 to 900 yr BP at <span class="hlt">subantarctic</span> latitudes that is broadly consistent with previous studies of climate-driven vegetation change at the Auckland Islands. Comparison with a SHWW reconstruction using similar proxies from Fiordland suggests a northward migration of the SHWW over New Zealand during the first half of the last millennium. Comparison with palaeoclimate and palaeoceanographic records from southern South America and West Antarctica indicates a late Holocene strengthening of the SHWW after ˜ 1600 yr BP that appears to be broadly symmetrical across the Pacific Basin. Contemporaneous increases in SHWW at localities on either</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.schweizerbart.de/publications/detail/isbn/9783443510657','USGSPUBS'); return false;" href="http://www.schweizerbart.de/publications/detail/isbn/9783443510657"><span>Diatom and silicoflagellate biostratigraphy for the late Eocene: ODP 1090 (<span class="hlt">sub-Antarctic</span> Atlantic)</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Barron, John A.; Bukry, David B.; Gersonde, Rainer</p> <p>2014-01-01</p> <p>Abundant and well-preserved diatoms and silicofl agellate assemblages are documented through a complete late Eocene sequence, ODP Hole 1090B, recovered from the southern Agulhas Ridge in the <span class="hlt">sub-Antarctic</span> South Atlantic. A sequence of Cestodiscus (diatom) species occurrence events involving C. pulchellus var. novazealandica, C. fennerae, C. antarcticus, C. convexus, C. trochus, and C. robustus is tied with paleomagnetic stratigraphy and provides the basis of proposing a new diatom zonation for the latest middle Eocene to early Oligocene (~37.6–33.4 Ma) of the <span class="hlt">sub-Antarctic</span> South Atlantic. Comparison with previously published diatom occurrence charts suggested this zonation should be applicable throughout the low latitude regions of the world’s oceans. Silicofl agellates belong to the Dictyocha hexacantha and the overlying Corbisema apiculata Zones. The late Eocene succession of silicofl agellate species is dominated by Naviculopsis (20–60%). Naviculopsis constricta and N. foliacea dominate the D. hexacantha Zone, followed by the N. constricta, then N. biapiculata in the C. apiculata Zone. Cold-<span class="hlt">water</span> Distephanus is most abundant in the latest Eocene along with N. biapiculata. The tops of zonal guide fossils Dictyocha hexacantha and Hannaites quadria (both 36.6 Ma) and Dictyocha spinosa (37.1 Ma) are tied with paleomagnetic stratigraphy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=107133&keyword=climate+AND+change+AND+evidence&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=107133&keyword=climate+AND+change+AND+evidence&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>INFLUENCE OF DIFFERENT <span class="hlt">WATER</span> MASSES AND BIOLOGICAL ACTIVITY ON DIMETHYLSULPHIDE AND DIMETHYLSULPHONIOPROPIONATE IN THE <span class="hlt">SUBANTARCTIC</span> ZONE OF THE SOUTHERN OCEAN DURING ACE-1</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>Measurements of salinity, temperature, phytoplankton biomass and speciation, dissolved nitrate, dimethylsulphide (DMS) in seawater and air, and dimethylsulphoniopropionate (DMSP), were made in the <span class="hlt">subantarctic</span> zone of the Southern Ocean from 40|-54|S, and 140|-153|E during the So...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29674908','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29674908"><span>Antarctic and <span class="hlt">Sub-Antarctic</span> Asteroidea database.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moreau, Camille; Mah, Christopher; Agüera, Antonio; Améziane, Nadia; David Barnes; Crokaert, Guillaume; Eléaume, Marc; Griffiths, Huw; Charlène Guillaumot; Hemery, Lenaïg G; Jażdżewska, Anna; Quentin Jossart; Vladimir Laptikhovsky; Linse, Katrin; Neill, Kate; Sands, Chester; Thomas Saucède; Schiaparelli, Stefano; Siciński, Jacek; Vasset, Noémie; Bruno Danis</p> <p>2018-01-01</p> <p>The present dataset is a compilation of georeferenced occurrences of asteroids (Echinodermata: Asteroidea) in the Southern Ocean. Occurrence data south of 45°S latitude were mined from various sources together with information regarding the taxonomy, the sampling source and sampling sites when available. Records from 1872 to 2016 were thoroughly checked to ensure the quality of a dataset that reaches a total of 13,840 occurrences from 4,580 unique sampling events. Information regarding the reproductive strategy (brooders vs. broadcasters) of 63 species is also made available. This dataset represents the most exhaustive occurrence database on Antarctic and <span class="hlt">Sub-Antarctic</span> asteroids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28187387','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28187387"><span>Permeable bio-reactive barriers to address petroleum hydrocarbon contamination at <span class="hlt">subantarctic</span> Macquarie Island.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Freidman, Benjamin L; Terry, Deborah; Wilkins, Dan; Spedding, Tim; Gras, Sally L; Snape, Ian; Stevens, Geoffrey W; Mumford, Kathryn A</p> <p>2017-05-01</p> <p>A reliance on diesel generated power and a history of imperfect fuel management have created a legacy of petroleum hydrocarbon contamination at <span class="hlt">subantarctic</span> Macquarie Island. Increasing environmental awareness and advances in contaminant characterisation and remediation technology have fostered an impetus to reduce the environmental risk associated with legacy sites. A funnel and gate permeable bio-reactive barrier (PRB) was installed in 2014 to address the migration of Special Antarctic Blend diesel from a spill that occurred in 2002, as well as older spills and residual contaminants in the soil at the Main Power House. The PRB gate comprised of granular activated carbon and natural clinoptilolite zeolite. Petroleum hydrocarbons migrating in the soil <span class="hlt">water</span> were successfully captured on the reactive materials, with concentrations at the outflow of the barrier recorded as being below reporting limits. The nutrient and iron concentrations delivered to the barrier demonstrated high temporal variability with significant iron precipitation observed across the bed. The surface of the granular activated carbon was largely free from cell attachment while natural zeolite demonstrated patchy biofilm formation after 15 months following PRB installation. This study illustrates the importance of informed material selection at field scale to ensure that adsorption and biodegradation processes are utilised to manage the environmental risk associated with petroleum hydrocarbon spills. This study reports the first installation of a permeable bio-reactive barrier in the <span class="hlt">subantarctic</span>. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58..839A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58..839A"><span>Grazing suppression of dimethylsulphoniopropionate (DMSP) accumulation in iron-fertilised, <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Archer, S. D.; Safi, K.; Hall, A.; Cummings, D. G.; Harvey, M.</p> <p>2011-03-01</p> <p>The impact of in situ iron fertilisation on the production of particulate dimethylsulphoniopropionate (DMSPp) and its breakdown product dimethyl sulphide (DMS) was monitored during the SOLAS air-sea gas exchange experiment (SAGE). The experiment was conducted in the high nitrate, low chlorophyll (HNLC) <span class="hlt">waters</span> of the <span class="hlt">sub-Antarctic</span> Southern Ocean (46.7°S 172.5°E) to the south-east of New Zealand, during March-April, 2004. In addition to monitoring net changes in the standing stocks of DMSPp and DMS, a series of dilution experiments were used to determine the DMSPp production and consumption rates in relation to increased iron availability. In contrast to previous experiments in the Southern Ocean, DMS concentrations decreased over the course of the 15-d iron-fertilisation experiment, from an integrated volume-specific concentration in the mixed layer on day 0 of 0.78 nM (measured values 0.65-0.91 nM) to 0.46 nM (measured values 0.42-0.47 nM) by day 15, in parallel with the surrounding <span class="hlt">waters</span>. DMSPp, chlorophyll a and the abundance of photosynthetic picoeukaryotes exhibited indiscernible or only moderate increases in response to the raised iron availability, despite an obvious physiological response by the phytoplankton. High specific growth rates of DMSPp, equivalent to 0.8-1.2 doublings d -1, occurred at the simulated 60% light level of the dilution experiments. Despite the high production rates, DMSPp accumulation was suppressed in part by microzooplankton grazers who consumed between 61% d -1 and 126% d -1 of the DMSPp production. Temporal trends in the rates of production and consumption illustrated a close coupling between the DMSP-producing phytoplankton and their microzooplankton grazers. Similar grazing and production rates were observed for the eukaryotic picophytoplankton that dominated the phytoplankton biomass, partial evidence that picoeukaryotes contributed a substantial proportion of the DMSP synthesis. These rates for DMSPp and picoeukaryotes were</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PrOce.129...50T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PrOce.129...50T"><span>Silicic acid enrichment of <span class="hlt">subantarctic</span> surface <span class="hlt">water</span> from continental inputs along the Patagonian archipelago interior sea (41-56°S)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torres, Rodrigo; Silva, Nelson; Reid, Brian; Frangopulos, Máximo</p> <p>2014-12-01</p> <p>We estimated Si∗, the surplus or deficit of orthosilicic acid (DSi) relative to nitrate available for diatom growth, in the Chilean Patagonian Archipelago Interior Sea (PAIS). Si∗ and salinity were negatively correlated in the PAIS because of the mixing of high nitrate, low DSi <span class="hlt">subantarctic</span> surface <span class="hlt">water</span> and high DSi, low nitrate continental freshwater runoff. Both the slope and the intercept of this relationship decreased from northern to southern Patagonia, which was likely a consequence of reduced DSi inputs from several overlapping hydrological, biological and geological drivers along this gradient. In general, lower freshwater DSi concentrations were expected below 46°S, and a lower total DSi load was expected from reduced runoff below 51°S. The north-south decreasing DSi concentration trend may be linked to dilutions from a higher proportion of runoff in latitudes with higher precipitation rates (45-53°S), the transition to more resistant granitic rocks and glacial melt-<span class="hlt">water</span> from the Northern and Southern Patagonia Ice Fields (46-51°S) and a reduced density of volcanoes active during the Holocene (48-56°S). The intensification of a southward DSi deficit may be a forcing factor involved in the reported southward reductions in plankton biomass and a more frequent occurrence of non-diatom blooms in southern PAIS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.2405N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.2405N"><span>Annual cycles of deep-ocean biogeochemical export fluxes in subtropical and <span class="hlt">subantarctic</span> <span class="hlt">waters</span>, southwest Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nodder, Scott D.; Chiswell, Stephen M.; Northcote, Lisa C.</p> <p>2016-04-01</p> <p>The annual cycles of particle fluxes derived from moored sediment trap data collected during 2000-2012 in subtropical (STW) and <span class="hlt">subantarctic</span> <span class="hlt">waters</span> (SAW) east of New Zealand are presented. These observations are the most comprehensive export flux time series from temperate Southern Hemisphere latitudes to date. With high levels of variability, fluxes in SAW were markedly lower than in STW, reflecting the picophytoplankton-dominated communities in the iron-limited, high nutrient-low chlorophyll SAW. Austral spring chlorophyll blooms in surface STW were near synchronous with elevated fluxes of bio-siliceous, carbonate, and organic carbon-rich materials to the deep ocean, probably facilitated by diatom and/or coccolithophorid sedimentation. Lithogenic fluxes were also high in STW, compared to SAW, reflecting proximity to the New Zealand landmass. In contrast, the highest biogenic fluxes in SAW occurred in spring when surface chlorophyll concentrations were low, while highest annual chlorophyll concentrations were in summer with no associated flux increase. We hypothesize that the high spring export in SAW results from subsurface chlorophyll accumulation that is not evident from remote-sensing satellites. This material was also rich in biogenic silica, perhaps related to the preferential export of diatoms and other silica-producing organisms, such as silicoflagellates and radiolarians. Organic carbon fluxes in STW are similar to that of other mesotrophic to oligotrophic <span class="hlt">waters</span> (˜6-7 mg C m-2 d-1), whereas export from SAW is below the global average (˜3 mg C m-2 d-1). Regional differences in flux across the SW Pacific and Tasman region reflect variations in physical processes and ecosystem structure and function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014Geomo.223...61E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014Geomo.223...61E"><span>Surface destabilisation by the invasive burrowing engineer Mus musculus on a <span class="hlt">sub-Antarctic</span> island</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eriksson, Bert; Eldridge, David J.</p> <p>2014-10-01</p> <p>Invasive species are known to have substantial trophic effects on ecosystems and ecosystem processes. The invasion of the house mouse (Mus musculus) onto <span class="hlt">sub-Antarctic</span> islands has had a devastating effect on plants, invertebrates, and birds with substantial changes in ecosystem functions. Less well understood, however, are the nontrophic, geomorphic effects of mice resulting from their burrowing activities. We examined the extent of burrow construction by M. musculus across an area of about 20 ha on Marion Island and the effects of burrows on <span class="hlt">water</span> flow and sediment movement. We recorded a density of 0.59 ± 0.48 (mean ± SD) burrows m- 2, with more burrows at lower altitudes and shallower slopes, and twice the density in the solifluction risers (0.86 ± 0.54 m- 2) than the intervening terraces or treads (0.40 ± 0.51 m- 2). Most burrows were dug horizontally into the slope and tended to extend about 20 cm deep before turning. A very conservative estimate of sediment removed from burrows from this depth is 2.4 t ha- 1. However, taking into account more detailed data on burrow morphology based on excavations, actual amounts may be closer to 8.4 t ha- 1. Average soil displacement rate for a single burrow, measured over 5 days, was 0.18 kg burrow- 1 day- 1. Burrows acted as conduits for <span class="hlt">water</span> and warmer air. Stones at burrow entrances were moved eight times farther by <span class="hlt">water</span> (10.4 cm) than those not associated with burrows. Similarly, temperatures adjacent to burrow entrances were 4.1 °C higher than sites 10 cm away. Together our data indicate that mice are having substantial deleterious and geomorphic effects on <span class="hlt">sub-Antarctic</span> ecosystems through their burrowing. With lower rates of mouse mortality resulting from warmer climates predicted under global climate models, we can expect an increase in damage resulting from mouse activity.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li class="active"><span>1</span></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_1 --> <div id="page_2" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="21"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990081083&hterms=coastal+zone&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcoastal%2Bzone','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990081083&hterms=coastal+zone&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dcoastal%2Bzone"><span>Near-Surface Phytoplankton Pigment from the Coastal Zone Color Scanner in the <span class="hlt">Subantarctic</span> Region Southeast of New Zealand</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Banse, Karl; English, David C.</p> <p>1997-01-01</p> <p>Primarily based on satellite images, the phytoplankton concentration southeast (down- stream) of New Zealand in the High Nitrate - Low Chlorophyll (HNLC) <span class="hlt">Subantarctic</span> <span class="hlt">water</span> between the Subtropical Convergence (STC) and the Polar Front (PF) is believed to be higher than in the remainder of the Pacific Sector. Iron enrichment is assumed to be the reason, To study the question, near-surface phytoplankton pigment estimates from the Coastal Zone Color Scanner for up to 7 yr were reprocessed with particular attention to interference by clouds. Monthly mean images were created for the U,S. JGOFS Box along 170 deg W and means for individual dates calculated for 7 large areas between 170 deg E and 160 deg W, 45 deg and 58 deg S, well offshore of New Zealand and principally between and away from the STC and PF. The areal means are about as low as in other HNLC regions (most values between 0.1 and 0.4 or 0.5 mg/ sq m, with very few winter images; median of seasonal means, 0.26 mg/sq m) except at times near the STC, The higher means tend to occur in late summer and autumn, However, contrary to expectations, neither the PF nor the environs of the <span class="hlt">Subantarctic</span> Front are distinguished by a zone of increased pigment. Also, of 24 spring-summer images of oceanic islands in mostly pigment-poor <span class="hlt">water</span>, 17 yielded no recognizable elevated pigment; islands were 5 times surrounded by approximately doubled concentrations (ca 100 km in diameter), and 2 cases may have been associated with an extensive bloom. Inspection of offshore images showed concentrations of 1 greater than or equal to(up to 5) mg/sq m in rare patches of 65 to 200 km size on approximately one-tenth of the dates; such patches were not seen in <span class="hlt">Sub-antarctic</span> <span class="hlt">waters</span> of the eastern Pacific Sector. A case is made for Australian airborne iron supply being the cause that, presumably, would enhance large-celled phytoplankton. Since, however, the putative iron supply from the seabed around the oceanic islands or the near</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26880785','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26880785"><span>Characterization of the faecal bacterial community of wild young South American (Arctocephalus australis) and <span class="hlt">Subantarctic</span> fur seals (Arctocephalus tropicalis).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Medeiros, Aline Weber; Giongo, Adriana; Valdez, Fernanda P; Blaese de Amorin, Derek; Tavares, Maurício; d'Azevedo, Pedro A; Franco, Ana Claudia; Frazzon, Jeverson; Frazzon, Ana P G</p> <p>2016-03-01</p> <p>The microbiota of wild marine mammals is poorly understood, perhaps due to the migratory habits of some species and the difficulty in obtaining samples. Using high-throughput sequencing, the present study examines the faecal bacterial community of wild young South American (Arctocephalus australis) and <span class="hlt">Subantarctic</span> fur seals (A. tropicalis). Faecal samples from South American (n = 6) and <span class="hlt">Subantarctic</span> fur seals (n = 4) found dead along the south coast of Brazil were collected. Sequences were assigned to taxa using the Ribosomal Database Project-Bayesian classifier. Diversity of the microbiota was assessed by categorization of sequence reads into operational taxonomic units. Results indicate that Firmicutes (88.556%-84.016%) was the predominant phylum in South American and <span class="hlt">Subantarctic</span> fur seals. The distribution of Actinobacteria and Proteobacteria varied according to the fur seal species. Fusobacteria and Bacteroidetes represented less than 1% of the sequences. The most abundant order in both fur seals was Clostridiales (88.64% and 87.49%). Individual variable incidences were observed in the composition of family among the fur seals, though the families Lachnospiraceae, Peptostreptococcaceae, Ruminococcaceae and Coriobacteriaceae were more prevalent. This study provides insight into the faecal bacterial community of wild young South American and <span class="hlt">Subantarctic</span> fur seals. © FEMS 2016. All rights reserved. For permissions, please e-mail: journals.permissions@oup.com.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1350G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1350G"><span>Late Glacial and Holocene Climate Change in the <span class="hlt">subantarctic</span> Auckland Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gilmer, G.; Moy, C. M.; Vandergoes, M.; Gadd, P.; Riesselman, C. R.; Jacobsen, G. E.; Wilson, G. S.; Visinand, C.</p> <p>2017-12-01</p> <p>Situated within the core of the Southern Hemisphere westerly winds, and between the subtropical and <span class="hlt">subantarctic</span> fronts, the New Zealand <span class="hlt">subantarctic</span> islands are uniquely positioned to evaluate past ocean and atmospheric change in the middle to high southern latitudes. We collected a series of sediment cores from Auckland Island fjords to produce a high-resolution record of climate change following the Last Glacial Maximum. Physical property and organic geochemical data, Itrax XRF, and visual core descriptions indicate the cores capture several phases of sedimentation. From these studies, we identify four primary sedimentary facies: 1) a deglacial facies exhibiting mm-scale laminae defined by magnetic susceptibility and density contrasts and high counts of elements associated with terrigenous sources; 2) a lacustrine facies defined by very low density, high organic carbon concentrations and low counts of lithophilic elements; 3) a marine transgression facies with moderate density, moderate bioturbation and alternating marine and lacustrine sedimentary components; 4) a marine facies that contains biogenic carbonate. Radiocarbon results indicate deglacial sedimentation was underway in the basin by approximately 19,000 cal yr BP. Lacustrine deposition in ice-free conditions began around 15,600 cal yr BP and continued until marine transgression at approximately 9,500 cal yr BP. During the early Holocene between 11 and 9.5 ka, we observe elevated n-alkane δD values and an overall increase in redox-sensitive elements that signal a combination of warmer atmospheric temperatures and reduced westerly wind strength that drives fjord stratification. Poleward-shifted westerlies south of the Auckland Islands could accommodate these results, but there are few records to corroborate this interpretation. We will discuss these results within the context of developing New Zealand and <span class="hlt">subantarctic</span> paleoclimate records in order to provide a more comprehensive record of past change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29207352','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29207352"><span>Ecosystem effects and the management of petroleum-contaminated soils on <span class="hlt">subantarctic</span> islands.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Errington, Ingrid; King, Catherine K; Wilkins, Daniel; Spedding, Tim; Hose, Grant C</p> <p>2018-03-01</p> <p>Human activity in the Polar Regions has resulted in petroleum contamination of soils. In this context, <span class="hlt">subantarctic</span> islands are a unique management challenge for climatic, biological and logistical reasons. In this review we identify the main abiotic factors affecting petroleum-contaminated soils in the <span class="hlt">subantarctic</span> environment, the primary effects of such contamination on biota, and lessons learned with regards to remediation techniques in this region. The sensitivity of biota to contamination depends on organism life stage, on soil properties, and on the degree of contaminant weathering. Initial studies using species endemic to <span class="hlt">subantarctic</span> islands suggest that for fresh diesel fuel, sensitivities may range between 103 and 20 000 mg total petroleum hydrocarbons (TPH) kg -1 soil. Diesel that has undergone a short period of weathering is generally more toxic, with sensitivities ranging between 52 and 13 000 mg TPH kg -1 soil for an earthworm and a grass respectively (based on EC 20 and IC 50 values). A sufficient body of data from which to develop remediation targets for existing spills in the region does not yet exist for the region, but there has been a recent increase in research attention to address this data gap. A range of remediation methods have also now been trialled, and techniques such as in-ground aeration and nutrient addition have achieved some success. Passive management techniques such as permeable reactive barriers and phytoremediation are in preliminary stages of investigation for the region and show promise, not least because they cause less collateral disturbance than other methods. Crown Copyright © 2017. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP51B2288M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP51B2288M"><span>Postglacial Records of Southern Hemisphere Westerly Wind Variability From the New Zealand <span class="hlt">Subantarctic</span> Auckland Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moy, C. M.; Vandergoes, M.; Gilmer, G. J.; Nichols, J. E.; Dagg, B. J.; Wilson, G. S.; Browne, I. M.; Curtin, L. G.; Aebig, C.; McGlone, M.</p> <p>2015-12-01</p> <p>The strength and latitudinal position of the Southern Hemisphere westerly winds (SHWW) play a fundamental role in influencing mid latitude climate and carbon dioxide exchange between the Southern Ocean and the atmosphere. Despite their importance, our understanding of past changes in the SHWW is limited by few paleoclimate records from the modern wind maximum that are often not in agreement. The New Zealand <span class="hlt">subantarctic</span> Auckland Islands are located within the core of the modern wind belt (50°S) where the ocean-atmospheric linkages between the Antarctic and middle latitudes are strong. In contrast to other <span class="hlt">subantarctic</span> islands on the Campbell Plateau, the Auckland Islands have protected fjord sub-basins, deep lakes, and peatlands that are advantageous for the development of high-resolution paleoclimate records. We will present ongoing work towards the establishment of multi-proxy and multi-site reconstructions of past SHWW variability from the Auckland Islands. Modern process and paleoclimate results from two research cruises in 2014 and 2015 suggest that in lacustrine and fjord settings, the degree of <span class="hlt">water</span> column mixing, the stable isotopic composition of n-alkanes and benthic foraminifera, the influx of terrestrial organic matter are good indicators of wind-induced mixing of the <span class="hlt">water</span> column or precipitation-driven erosion within catchments. In ombrotrophic peatlands, hydrogen isotope ratios of specific organic molecules allow reconstructions of the hydrogen isotope ratios of precipitation, which is related to precipitation source area and the latitudinal position of the SHWW. Using macrofossil counts paired with abundances of leaf wax biomarkers, we are able to estimate the moisture balance at peatland coring sites. Early results indicate an overall strengthening of the SHWW at the Auckland Islands through the Holocene. We will discuss these results within the context of complimentary records developed from New Zealand and southern South America to ultimately</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PalOc..31.1583G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PalOc..31.1583G"><span>Carbon isotope offsets between benthic foraminifer species of the genus Cibicides (Cibicidoides) in the glacial <span class="hlt">sub-Antarctic</span> Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gottschalk, Julia; Vázquez Riveiros, Natalia; Waelbroeck, Claire; Skinner, Luke C.; Michel, Elisabeth; Duplessy, Jean-Claude; Hodell, David; Mackensen, Andreas</p> <p>2016-12-01</p> <p>Epibenthic foraminifer δ13C measurements are valuable for reconstructing past bottom <span class="hlt">water</span> dissolved inorganic carbon δ13C (δ13CDIC), which are used to infer global ocean circulation patterns. Epibenthic δ13C, however, may also reflect the influence of 13C-depleted phytodetritus, microhabitat changes, and/or variations in carbonate ion concentrations. Here we compare the δ13C of two benthic foraminifer species, Cibicides kullenbergi and Cibicides wuellerstorfi, and their morphotypes, in three <span class="hlt">sub-Antarctic</span> Atlantic sediment cores over several glacial-interglacial transitions. These species are commonly assumed to be epibenthic, living above or directly below the sediment-<span class="hlt">water</span> interface. While this might be consistent with the small δ13C offset that we observe between these species during late Pleistocene interglacial periods (Δδ13C = -0.19 ± 0.31‰, N = 63), it is more difficult to reconcile with the significant δ13C offset that is found between these species during glacial periods (Δδ13C = -0.76 ± 0.44‰, N = 44). We test possible scenarios by analyzing Uvigerina spp. δ13C and benthic foraminifer abundances: (1) C. kullenbergi δ13C is biased to light values either due to microhabitat shifts or phytodetritus effects and (2) C. wuellerstorfi δ13C is biased to heavy values, relative to long-term average conditions, for instance by recording the sporadic occurrence of less depleted deepwater δ13CDIC. Neither of these scenarios can be ruled out unequivocally. However, our findings emphasize that supposedly epibenthic foraminifer δ13C in the <span class="hlt">sub-Antarctic</span> Atlantic may reflect several factors rather than being solely a function of bottom <span class="hlt">water</span> δ13CDIC. This could have a direct bearing on the interpretation of extremely light South Atlantic δ13C values at the Last Glacial Maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1613786T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1613786T"><span>Investigating the spring bloom initiation and net community production in the <span class="hlt">Subantarctic</span> Southern Ocean using high-resolution in situ glider data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>thomalla, sandy; Racault, Marie-Fanny; Swart, Sebastiaan; Monteiro, Pedro</p> <p>2014-05-01</p> <p>Phytoplankton bloom phenology has important consequences for marine ecosystems, fisheries and carbon export to the ocean interior. As such, it is important to examine the drivers of phytoplankton bloom initiation and their sensitivity to inter-annual climate variability and change. In this study we use ~6 months of in-situ high-resolution glider data to investigate the spring bloom initiation in the <span class="hlt">subantarctic</span> zone (SAZ) of the Southern Ocean by implementing three different methods; a rate of change method, a threshold method and a cumulative sum method. The bloom initiation dates are critically compared to one another and the drivers of discrepancies assessed to inform on the sensitivities of different methods to processes driving the seasonal evolution of phytoplankton biomass in the <span class="hlt">subantarctic</span>. The bloom initiation dates combined with in situ glider data of chlorophyll, light, and mixed layer depth allow us to resolve both Sverdrup's Critical Depth and Behrenfeld's Disturbance Recovery models through the <span class="hlt">water</span> column and thus determine the seasonal evolution of net community production and respiration rates and the potential for carbon export. The outputs of the two different models are compared to one another in the context of their sensitivities to <span class="hlt">water</span> column processes thereby refining their ability to address specific system scale questions. The novelty of this study is that gliders provide an unprecedented dataset to assess the seasonal cycle of phytoplankton biomass throughout the <span class="hlt">water</span> column at high resolution, thus enhancing our understanding of net community production and export processes at submeso-space and sub-seasonal time scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1519G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1519G"><span>Seismic Characterization of Oceanic <span class="hlt">Water</span> Masses, <span class="hlt">Water</span> Mass Boundaries, and Mesoscale Eddies SE of New Zealand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorman, Andrew R.; Smillie, Matthew W.; Cooper, Joanna K.; Bowman, M. Hamish; Vennell, Ross; Holbrook, W. Steven; Frew, Russell</p> <p>2018-02-01</p> <p>The Subtropical and <span class="hlt">Subantarctic</span> Fronts, which separate Subtropical, <span class="hlt">Subantarctic</span>, and Antarctic Intermediate <span class="hlt">Waters</span>, are diverted to the south of New Zealand by the submerged continental landmass of Zealandia. In the upper ocean of this region, large volumes of dissolved or suspended material are intermittently transported across the Subtropical Front; however, the mechanisms of such transport processes are enigmatic. Understanding these oceanic boundaries in three dimensions generally depends on measurements collected from stationary vessels and moorings. The details of these data sets, which are critical for understanding how <span class="hlt">water</span> masses interact and mix at the fine-scale (<10 m) to mesoscale (10-100 km), are inadequately constrained due to resolution considerations. Southeast of New Zealand, high-resolution seismic reflection images of oceanic <span class="hlt">water</span> masses have been produced using petroleum industry data. These seismic sections clearly show three main <span class="hlt">water</span> masses, the boundary zones (fronts) between them, and associated thermohaline fine structure that may be related to the mixing of <span class="hlt">water</span> masses in this region. Interpretations of the data suggest that the Subtropical Front in this region is a landward-dipping zone, with a width that can vary between 20 and 40 km. The boundary zone between <span class="hlt">Subantarctic</span> <span class="hlt">Waters</span> and the underlying Antarctic Intermediate <span class="hlt">Waters</span> is also observed to dip landward. Several isolated lenses have been identified on the three data sets, ranging in size from 9 to 30 km in diameter. These lenses are interpreted to be mesoscale eddies that form at relatively shallow depths along the south side of the Subtropical Front.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018QSRv..183..110J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018QSRv..183..110J"><span>Glacier extent in <span class="hlt">sub-Antarctic</span> Kerguelen archipelago from MIS 3 period: Evidence from 36Cl dating</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jomelli, Vincent; Schimmelpfennig, Irene; Favier, Vincent; Mokadem, Fatima; Landais, Amaelle; Rinterknecht, Vincent; Brunstein, Daniel; Verfaillie, Deborah; Legentil, Claude; Aumaitre, Georges; Bourlès, Didier L.; Keddadouche, Karim</p> <p>2018-03-01</p> <p>Documenting <span class="hlt">sub-Antarctic</span> glacier variations during the local last glacial maximum is of major interest to better understand their sensitivity to atmospheric and oceanic temperature changes in conjunction with Antarctic ice sheet changes. However, data are sparse because evidence of earlier glacier extents is for most <span class="hlt">sub-Antarctic</span> islands located offshore making their observation complex. Here, we present 22 cosmogenic 36Cl surface exposure ages obtained from five sites at Kerguelen to document the glacial history. The 36Cl ages from roche moutonnee surfaces, erratics and boulders collected on moraines span from 41.9 ± 4.4 ka to 14.3 ± 1.1 ka. Ice began to retreat on the eastern part of the main island before 41.4 ± 4.4 ka. Slow deglaciation occurred from ∼41 to ∼29 ka. There is no evidence of advances between 29 ka and the Antarctic Cold Reversal (ACR) period (∼14.5-12.9 ka) period. During the ACR, however, the Bontemps and possibly Belvedere moraines were formed by the advance of a Cook Ice Cap outlet glacier and a local glacier on the Presque Ile Jeanne d'Arc, respectively. This glacier evolution differs partly from that of glaciers in New Zealand and in Patagonia. These asynchronous glacier changes in the <span class="hlt">sub-Antarctic</span> region are however in agreement with sea surface temperature changes recorded around Antarctica, which suggest differences in the climate evolution of the Indo-Pacific and Atlantic sectors of Antarctica.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011DSRII..58..808P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011DSRII..58..808P"><span>The response of phytoplankton to iron enrichment in <span class="hlt">Sub-Antarctic</span> HNLCLSi <span class="hlt">waters</span>: Results from the SAGE experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Peloquin, Jill; Hall, Julie; Safi, Karl; Smith, Walker O., Jr.; Wright, Simon; van den Enden, Rick</p> <p>2011-03-01</p> <p>Areas of high nutrients and low chlorophyll a comprise nearly a third of the world's oceans, including the equatorial Pacific, the Southern Ocean and the Sub-Arctic Pacific. The SOLAS Sea- Air Gas Exchange (SAGE) experiment was conducted in late summer, 2004, off the east coast of the South Island of New Zealand. The objective was to assess the response of phytoplankton in <span class="hlt">waters</span> with low iron and silicic acid concentrations to iron enrichment. We monitored the quantum yield of photochemistry ( Fv/ Fm) with pulse amplitude modulated fluorometry, chlorophyll a, primary productivity, and taxonomic composition. Measurements of Fv/ Fm indicated that the phytoplankton within the amended patch were relieved from iron stress ( Fv/ Fm approached 0.65). Although there was no significant difference between IN and OUT stations at points during the experiment, the eventual enhancement in chlorophyll a and primary productivity was twofold by the end of the 15-day patch occupation. However, no change in particulate carbon or nitrogen pools was detected. Enhancement in primary productivity and chlorophyll a were approximately equal for all phytoplankton size classes, resulting in a stable phytoplankton size distribution. Initial seed stocks of diatoms were extremely low, <1% of the assemblage based on HPLC pigment analysis, and did not respond to iron enrichment. The most dominant groups before and after iron enrichment were type 8 haptophytes and prasinophytes that were associated with ˜75% of chlorophyll a. Twofold enhancement of biomass estimated by flow cytometry was detected only in eukaryotic picoplankton, likely prasinophytes, type 8 haptophytes and/or pelagophytes. These results suggest that factors other than iron, such as silicic acid, light or physical disturbance limited the phytoplankton assemblage during the SAGE experiment. Furthermore, these results suggest that additional iron supply to the <span class="hlt">Sub-Antarctic</span> under similar seasonal conditions and seed stock will most</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1351M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1351M"><span>Postglacial Records of Southern Hemisphere Climate and Oceanographic Change From the New Zealand <span class="hlt">Subantarctic</span> Auckland Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moy, C. M.; Gilmer, G.; Nichols, J. E.; Browne, I. M.; Curtin, L.; Vandergoes, M.; Aebig, C.; Wilson, G. S.</p> <p>2017-12-01</p> <p>The strength and latitudinal position of the Southern Hemisphere westerly winds (SHWW) play a fundamental role in influencing mid-latitude climate and CO2 exchange between the Southern Ocean and the atmosphere along seasonal to glaicial-interglacial timescales. Despite their importance, our understanding of past SHWW change is limited by the small number of paleoclimate records from the modern wind maximum, which are often not in agreement. The New Zealand <span class="hlt">subantarctic</span> Auckland Islands are located within the core of the modern wind belt (50°S), a key latitude where ocean-atmospheric linkages between the Antarctic and mid-latitudes are strong. In contrast to other <span class="hlt">subantarctic</span> islands on the Campbell Plateau, the Auckland Islands have multiple protected fjord sub-basins, deep lakes, and peatlands that are advantageous for the development of high-resolution paleoclimate records. We will present ongoing work towards the establishment of multi-proxy and multi-site reconstructions of past SHWW variability from the Auckland Islands. Modern process and paleoclimate studies suggest that in lacustrine and fjord settings, the degree of <span class="hlt">water</span> column mixing, the stable isotopic composition of n-alkanes and benthic foraminifera, and the influx of terrestrial organic matter are good indicators of wind-induced mixing of the <span class="hlt">water</span> column or precipitation-driven erosion within catchments. During the Late Glacial and early Holocene (15 to 9 ka), elevated long-chain n-alkane δD values from ombrotrophic peatlands and an increase in the concentration of redox-sensitive elements in fjord sediment cores, signal weakening of the SHWW that appears to be coincident with periods of rapid deglacial warming of West Antarctica. Since 5.5 ka, we interpret declining n-alkane δD values to indicate enhanced westerly flow. These interpretations are in broad agreement with terrestrial paleoclimate records developed from southern South America and argue for a symmetrical response of the SHWW during</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..11.5243F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..11.5243F"><span>Investigation of the late summer Si-budget in the <span class="hlt">Sub-Antarctic</span> and Polar Front Zones south of Tasmania (SAZ-SENSE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fripiat, F.; Leblanc, K.; Elskens, M.; Quéguiner, B.; Armand, L.; Cornet-Barthaux, V.; André, L.; Cardinal, D.</p> <p>2009-04-01</p> <p>In the surface ocean, the Si-biogeochemical budget can be estimated by the ratio between the integrated biogenic silica dissolution and production rates. However such data are scarce in the ocean mostly because of methodology limitation. This is especially true in the <span class="hlt">Sub-Antarctic</span> Zone (SAZ) where only two profiles were measured so far, exhibiting large variation (dissolution: production ratio of 0.3 and 3.1 for spring and summer, respectively). Though, the SAZ plays a crucial role in the efficiency of the silicate pump and the fertility of the <span class="hlt">Sub-Antarctic</span> <span class="hlt">Mode</span> <span class="hlt">Waters</span> which then replenish in nutrients the majority of the surface <span class="hlt">waters</span> of the world ocean. Therefore, better constraining the dissolution: production ratios in this region will certainly improve our understanding of these processes. During the SAZ-SENSE cruise (Jan.-Feb. 2007), the Si-budget of three stations (two in the SAZ and one in the Polar Frontal Zone, PFZ, for a total of nine profiles) covering different biogeochemical properties (e.g., Fe enriched vs. depleted conditions, dominance of diatoms vs. other phytoplankton,…) was investigated. This was implemented in the framework of an exhaustive characterization of the Si-biogeochemical cycle using different parameters: PDMPO labelling, 32Si and 30Si spiked incubations, and, taxonomy. We have developed a new method for the determination of the production and dissolution rates from the 30Si isotopic dilution technique. We now measure the changes of the 30Si-abundances in particulate and liquid phases by High Resolution Sector Field Inductively Coupled Plasma Mass Spectrometer (HR-SF-ICP-MS). This method, which is faster, more sensitive and more precise than the traditional ones using an Isotope Ratio Mass Spectrometer (IRMS) or Thermal Ionization Mass Spectrometer (TIMS), will significantly aid in expanding the biogenic silica production-dissolution dataset in the ocean. The results obtained on Si budget indicate that the Si</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO54C3262F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO54C3262F"><span>Is the Oceanography of the New Zealand <span class="hlt">Subantarctic</span> Region Responding to the Tropics?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Forcen-Vazquez, A. N.</p> <p>2016-02-01</p> <p>The Campbell Plateau, south of New Zealand plays an important role in New Zealand's regional climate and its oceanography may have a significant impact on fluctuations in fish stocks and marine mammal populations. It is located between the Subtropical and <span class="hlt">Subantarctic</span> Fronts and exhibits marked variability over long time scales. It has been previously assumed, because of its location, that the Campbell Plateau oceanography is driven by <span class="hlt">Subantarctic</span> and polar processes. Recent analysis, presented here, suggests this in not the case, and instead forcing comes from the tropics and subtropics. This is supported by positive correlations of Sea Level Anomalies (SLA) and Sea Surface Temperature (SST) with the Southern Oscillation Index (SOI) with SOI leading changes on the Campbell Plateau by two months for SLA and seven months for SST. Here we will present evidence of the similarity between the Campbell Plateau and the Tasman Sea SLA trends which suggests a closer relationship with the subtropical region. Satellite collected SLA data and SST from the last two decades are investigated to understand trends and long-term variability over the Campbell Plateau and its relationship with the surrounding open ocean, and other potential remote drivers of variability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.B24A0306N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.B24A0306N"><span>Annual Cycles of Deep-ocean, Biogeochemical Export Fluxes and Biological Pump Processes in Subtropical and <span class="hlt">Subantarctic</span> <span class="hlt">Waters</span>, Southwest Pacific Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nodder, S.; Chiswell, S.; Northcote, L.</p> <p>2016-02-01</p> <p>One of the key aspects of the global carbon cycle is the efficiency and spatio-temporal variability of the biological pump. In this paper, the annual cycles of particle fluxes, derived from moored sediment trap data collected from 2000-12 in subtropical (STW) and <span class="hlt">subantarctic</span> <span class="hlt">waters</span> (SAW), east of New Zealand, are presented. These observations are the most comprehensive export flux time-series from temperate Southern Hemisphere latitudes to date. With high levels of variability, fluxes in SAW were markedly lower than in STW, reflecting the picophytoplankton-dominated communities in the iron-limited, high nutrient-low chlorophyll SAW. Austral spring chlorophyll blooms in surface STW were near-synchronous with elevated fluxes of bio-siliceous, carbonate and organic carbon-rich materials to the deep ocean, probably facilitated by diatom sedimentation. Lithogenic fluxes were also high in STW, compared to SAW, reflecting proximity to the New Zealand landmass. In contrast, the highest biogenic fluxes in SAW occurred in spring when surface chlorophyll concentrations were low, while highest annual chlorophyll concentrations were in summer with no associated flux increase. We hypothesize that the high spring export in SAW occurs from subsurface chlorophyll accumulations that are not evident from remote-sensing satellites. This material was also rich in biogenic silica, perhaps related to the preferential export of diatoms and other silica-producing organisms, such as silicoflagellates and radiolarians. Particle fluxes in STW are similar to that of other mesotrophic to oligotrophic <span class="hlt">waters</span> ( 6-7 mgC m-2 d-1), whereas export from SAW is below global averages ( 3 mgC m-2 d-1), and is characterized by carbonate-dominated and prominent bio-siliceous deposition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1988DSRA...35..311F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1988DSRA...35..311F"><span><span class="hlt">Water</span> mass modification at the Agulhas retroflection: chlorofluoromethane studies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fine, Rana A.; Warner, Mark J.; Weiss, Ray F.</p> <p>1988-03-01</p> <p>Chlorofluoromethane (CFM) and hydrographic data from the 1983 Agulhas Retroflection cruise are used to show the importance of the region in ventilating thermocline and Intermediate <span class="hlt">Waters</span> of the southwest Indian ocean gyre. Generally South Atlantic <span class="hlt">waters</span> are more recently ventilated by at least two years than those of the South Indian Ocean, probably because the latter are farther downstream from the source regions near the South Atlantic <span class="hlt">subantarctic</span> sector. A two-component mixing model shows that the outflow from the Agulhas Retroflection (14-4°C) was composed of South Indian <span class="hlt">water</span> and at least 23% South Atlantic <span class="hlt">water</span>. However, at the density of Indian sector <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> the inflow into the Agulhas Retroflection was well preserved in the outflow, and the South Atlantic and Indian <span class="hlt">waters</span> appear to be ventilated by different <span class="hlt">water</span> masses. In addition, strong interleaving was found throughout the survey area (between 14 and 4°C), characterized by correlations of negative salinity anomalies with high CFM concentrations. At the density of Antarctic Intermediate <span class="hlt">Water</span> (AAIW) there was interleaving of both low salinity <span class="hlt">water</span> and higher salinity Red Sea <span class="hlt">Water</span>. Using estimates of past atmospheric ratios of two CFMs, we calculate that AAIW within the retroflection was 50-75% diluted by mixing with CFM-free <span class="hlt">water</span> since leaving the source region. Results from the two-component mixing model, which show substantial contributions of South Atlantic <span class="hlt">water</span> in the outflow, suggest that the return flow for the 10 Sv leakage of Indian Ocean <span class="hlt">water</span> via the Agulhas Current into the South Atlantic [ GORDON (1985) Science, 227, 1030-1033; GORDONet al. (1987) Deep-Sea Research, 34, 565-600] is occurring at thermocline and intermediate depths. A combination of active mixing in this region and similarity in the ventilation processes may be the reason that the South Atlantic and Indian thermoclines are coincident in temperature and salinity space (between 15 and 7°C) as noted</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMPP42B..02R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMPP42B..02R"><span>Development of a Regional Glycerol Dialkyl Glycerol Tetraether (GDGT) - Temperature Calibration for Antarctic and <span class="hlt">sub-Antarctic</span> Lakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roberts, S. J.; Foster, L. C.; Pearson, E. J.; Steve, J.; Hodgson, D.; Saunders, K. M.; Verleyen, E.</p> <p>2016-12-01</p> <p>Temperature calibration models based on the relative abundances of sedimentary glycerol dialkyl glycerol tetraethers (GDGTs) have been used to reconstruct past temperatures in both marine and terrestrial environments, but have not been widely applied in high latitude environments. This is mainly because the performance of GDGT-temperature calibrations at lower temperatures and GDGT provenance in many lacustrine settings remains uncertain. To address these issues, we examined surface sediments from 32 Antarctic, <span class="hlt">sub-Antarctic</span> and Southern Chilean lakes. First, we quantified GDGT compositions present and then investigated modern-day environmental controls on GDGT composition. GDGTs were found in all 32 lakes studied. Branched GDGTs (brGDGTs) were dominant in 31 lakes and statistical analyses showed that their composition was strongly correlated with mean summer air temperature (MSAT) rather than pH, conductivity or <span class="hlt">water</span> depth. Second, we developed the first regional brGDGT-temperature calibration for Antarctic and <span class="hlt">sub-Antarctic</span> lakes based on four brGDGT compounds (GDGT-Ib, GDGT-II, GDGT-III and GDGT-IIIb). Of these, GDGT-IIIb proved particularly important in cold lacustrine environments. Our brGDGT-Antarctic temperature calibration dataset has an improved statistical performance at low temperatures compared to previous global calibrations (r2=0.83, RMSE=1.45°C, RMSEP-LOO=1.68°C, n=36 samples), highlighting the importance of basing palaeotemperature reconstructions on regional GDGT-temperature calibrations, especially if specific compounds lead to improved model performance. Finally, we applied the new Antarctic brGDGT-temperature calibration to two key lake records from the Antarctic Peninsula and South Georgia. In both, downcore temperature reconstructions show similarities to known Holocene warm periods, providing proof of concept for the new Antarctic calibration model.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolE....5..705A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolE....5..705A"><span>Microbial biomass and basal respiration of selected <span class="hlt">Sub-Antarctic</span> and Antarctic soils in the areas of some Russian polar stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abakumov, E.; Mukhametova, N.</p> <p>2014-07-01</p> <p>Antarctica is a unique place for soil, biological, and ecological investigations. Soils of Antarctica have been studied intensively during the last century, when different national Antarctic expeditions visited the sixth continent with the aim of investigating nature and the environment. Antarctic investigations are comprised of field surveys mainly in the terrestrial landscapes, where the polar stations of different countries are situated. That is why the main and most detailed soil surveys were conducted in the McMurdo Valleys, Transantarctic Mountains, South Shetland Islands, Larsemann Hills and the Schirmacher Oasis. Our investigations were conducted during the 53rd and 55th Russian Antarctic expeditions in the base of soil pits, and samples were collected in <span class="hlt">Sub-Antarctic</span> and Antarctic regions. <span class="hlt">Sub-Antarctic</span> or maritime landscapes are considered to be very different from Antarctic landscapes due to differing climatic and geogenic conditions. Soils of diverse zonal landscapes were studied with the aim of assessing the microbial biomass level, basal respiration rates and metabolic activity of microbial communities. This investigation shows that Antarctic soils are quite diverse in profile organization and carbon content. In general, <span class="hlt">Sub-Antarctic</span> soils are characterized by more developed humus (sod) organo-mineral horizons as well as by an upper organic layer. The most developed organic layers were revealed in peat soils of King George Island, where its thickness reach, in some cases, was 80 cm. These soils as well as soils formed under guano are characterized by the highest amount of total organic carbon (TOC), between 7.22 and 33.70%. Coastal and continental Antarctic soils exhibit less developed Leptosols, Gleysols, Regolith and rare Ornhitosol, with TOC levels between 0.37 and 4.67%. The metabolic ratios and basal respiration were higher in <span class="hlt">Sub-Antarctic</span> soils than in Antarctic ones, which can be interpreted as a result of higher amounts of fresh organic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SolED...6..869A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SolED...6..869A"><span>Microbial biomass and basal respiration in <span class="hlt">Sub-Antarctic</span> and Antarctic soils in the areas of some Russian polar stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abakumov, E.; Mukhametova, N.</p> <p>2014-03-01</p> <p>Antarctica is the unique place for pedological investigations. Soils of Antarctica have been studied intensively during the last century. Antarctic logistic provides the possibility to scientists access the terrestrial landscapes mainly in the places of polar stations. That is why the main and most detailed pedological investigations were conducted in Mc Murdo Valleys, Transantarctic Mountains, South Shetland Islands, Larsemann hills and Schirmacher Oasis. Investigations were conducted during the 53rd and 55th Russian Antarctic expeditions on the base of soil pits and samples collected in <span class="hlt">Sub-Antarctic</span> and Antarctic regions. Soils of diverse Antarctic landscapes were studied with aim to assess the microbial biomass level, basal respiration rates and metabolic activity of microbial communities. The investigation conducted shows that soils of Antarctic are quite different in profile organization and carbon content. In general, <span class="hlt">Sub-Antarctic</span> soils are characterized by more developed humus (sod) organo-mineral horizons as well as the upper organic layer. The most developed organic layers were revealed in peat soils of King-George Island, where its thickness reach even 80 cm. These soils as well as soils under guano are characterized by the highest amount of total organic carbon (TOC) 7.22-33.70%. Coastal and continental soils of Antarctic are presented by less developed Leptosols, Gleysols, Regolith and rare Ornhitosol with TOC levels about 0.37-4.67%. The metabolic ratios and basal respiration were higher in <span class="hlt">Sub-Antarctic</span> soils than in Antarctic ones which can be interpreted as result of higher amounts of fresh organic remnants in organic and organo-mineral horizons. Also the soils of King-George island have higher portion of microbial biomass (max 1.54 mg g-1) than coastal (max 0.26 mg g-1) and continental (max 0.22 mg g-1) Antarctic soils. <span class="hlt">Sub-Antarctic</span> soils mainly differ from Antarctic ones in increased organic layers thickness and total organic carbon content</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4856368','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4856368"><span>Underwater Optics in <span class="hlt">Sub-Antarctic</span> and Antarctic Coastal Ecosystems</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huovinen, Pirjo; Ramírez, Jaime; Gómez, Iván</p> <p>2016-01-01</p> <p>Understanding underwater optics in natural <span class="hlt">waters</span> is essential in evaluating aquatic primary production and risk of UV exposure in aquatic habitats. Changing environmental conditions related with global climate change, which imply potential contrasting changes in underwater light climate further emphasize the need to gain insights into patterns related with underwater optics for more accurate future predictions. The present study evaluated penetration of solar radiation in six <span class="hlt">sub-Antarctic</span> estuaries and fjords in Chilean North Patagonian region (39–44°S) and in an Antarctic bay (62°S). Based on vertical diffuse attenuation coefficients (Kd), derived from measurements with a submersible multichannel radiometer, average summer UV penetration depth (z1%) in these <span class="hlt">water</span> bodies ranged 2–11 m for UV-B (313 nm), 4–27 m for UV-A (395 nm), and 7–30 m for PAR (euphotic zone). UV attenuation was strongest in the shallow Quempillén estuary, while Fildes Bay (Antarctica) exhibited the highest transparency. Optically non-homogeneous <span class="hlt">water</span> layers and seasonal variation in transparency (lower in winter) characterized Comau Fjord and Puyuhuapi Channel. In general, multivariate analysis based on Kd values of UV and PAR wavelengths discriminated strongly Quempillén estuary and Puyuhuapi Channel from other study sites. Spatial (horizontal) variation within the estuary of Valdivia river reflected stronger attenuation in zones receiving river impact, while within Fildes Bay a lower spatial variation in <span class="hlt">water</span> transparency could in general be related to closeness of glaciers, likely due to increased turbidity through ice-driven processes. Higher transparency and deeper UV-B penetration in proportion to UV-A/visible wavelengths observed in Fildes Bay suggests a higher risk for Antarctic ecosystems reflected by e.g. altered UV-B damage vs. photorepair under UV-A/PAR. Considering that damage repair processes often slow down under cool temperatures, adverse UV impact could be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMPP34B..06M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMPP34B..06M"><span>Millennial-scale variability in dust deposition, marine export production, and nutrient consumption in the glacial <span class="hlt">subantarctic</span> ocean (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martinez-Garcia, A.; Sigman, D. M.; Anderson, R. F.; Ren, H. A.; Hodell, D. A.; Straub, M.; Jaccard, S.; Eglinton, T. I.; Haug, G. H.</p> <p>2013-12-01</p> <p>Based on the limitation of modern Southern Ocean phytoplankton by iron and the evidence of higher iron-bearing dust fluxes to the ocean during ice ages, it has been proposed that iron fertilization of Southern Ocean phytoplankton contributed to the reduction in atmospheric CO2 during ice ages. In the <span class="hlt">Subantarctic</span> zone of the Atlantic Southern Ocean, glacial increases in dust flux and export production have been documented, supporting the iron fertilization hypothesis. However, these observations could be interpreted alternatively as resulting from the equatorward migration of Southern Ocean fronts during ice ages if the observed productivity rise was not accompanied by an increase in major nutrient consumption. Here, new 230Th-normalized lithogenic and opal fluxes are combined with high-resolution biomarker measurements to reconstruct millennial-scale changes in dust deposition and marine export production in the <span class="hlt">subantarctic</span> Atlantic over the last glacial cycle. In the same record foraminifera-bound nitrogen isotopes are used to reconstruct ice age changes in surface nitrate utilization, providing a comprehensive test of the iron fertilization hypothesis. Elevation in foraminifera-bound δ15N, indicating more complete nitrate consumption, coincides with times of surface cooling and greater dust flux and export production. These observations indicate that the ice age <span class="hlt">Subantarctic</span> was characterized by iron fertilized phytoplankton growth. The resulting strengthening of the Southern Ocean's biological pump can explain the ~40 ppm lowering of CO2 that characterizes the transitions from mid-climate states to full ice age conditions as well as the millennial-scale atmospheric CO2 fluctuations observed within the last ice age</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li class="active"><span>2</span></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_2 --> <div id="page_3" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="41"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19776248','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19776248"><span>Physiological response to extreme fasting in <span class="hlt">subantarctic</span> fur seal (Arctocephalus tropicalis) pups: metabolic rates, energy reserve utilization, and <span class="hlt">water</span> fluxes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Verrier, Delphine; Groscolas, René; Guinet, Christophe; Arnould, John P Y</p> <p>2009-11-01</p> <p>Surviving prolonged fasting requires various metabolic adaptations, such as energy and protein sparing, notably when animals are simultaneously engaged in energy-demanding processes such as growth. Due to the intermittent pattern of maternal attendance, <span class="hlt">subantarctic</span> fur seal pups have to repeatedly endure exceptionally long fasting episodes throughout the 10-mo rearing period while preparing for nutritional independence. Their metabolic responses to natural prolonged fasting (33.4 +/- 3.3 days) were investigated at 7 mo of age. Within 4-6 fasting days, pups shifted into a stage of metabolic economy characterized by a minimal rate of body mass loss (0.7%/day) and decreased resting metabolic rate (5.9 +/- 0.1 ml O(2)xkg(-1)xday(-1)) that was only 10% above the level predicted for adult terrestrial mammals. Field metabolic rate (289 +/- 10 kJxkg(-1)xday(-1)) and <span class="hlt">water</span> influx (7.9 +/- 0.9 mlxkg(-1)xday(-1)) were also among the lowest reported for any young otariid, suggesting minimized energy allocation to behavioral activity and thermoregulation. Furthermore, lean tissue degradation was dramatically reduced. High initial adiposity (>48%) and predominant reliance on lipid catabolism likely contributed to the exceptional degree of protein sparing attained. Blood chemistry supported these findings and suggested utilization of alternative fuels, such as beta-hydroxybutyrate and de novo synthesized glucose from fat-released glycerol. Regardless of sex and body condition, pups tended to adopt a convergent strategy of extreme energy and lean body mass conservation that appears highly adaptive for it allows some tissue growth during the repeated episodes of prolonged fasting they experience throughout their development.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018GeoRL..45.5002O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018GeoRL..45.5002O"><span>Episodic Southern Ocean Heat Loss and Its Mixed Layer Impacts Revealed by the Farthest South Multiyear Surface Flux Mooring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogle, S. E.; Tamsitt, V.; Josey, S. A.; Gille, S. T.; Cerovečki, I.; Talley, L. D.; Weller, R. A.</p> <p>2018-05-01</p> <p>The Ocean Observatories Initiative air-sea flux mooring deployed at 54.08°S, 89.67°W, in the southeast Pacific sector of the Southern Ocean, is the farthest south long-term open ocean flux mooring ever deployed. Mooring observations (February 2015 to August 2017) provide the first in situ quantification of annual net air-sea heat exchange from one of the prime <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> formation regions. Episodic turbulent heat loss events (reaching a daily mean net flux of -294 W/m2) generally occur when northeastward winds bring relatively cold, dry air to the mooring location, leading to large air-sea temperature and humidity differences. Wintertime heat loss events promote deep mixed layer formation that lead to <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> formation. However, these processes have strong interannual variability; a higher frequency of 2 σ and 3 σ turbulent heat loss events in winter 2015 led to deep mixed layers (>300 m), which were nonexistent in winter 2016.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12919686','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12919686"><span>Attenuation characteristics of the fundamental <span class="hlt">modes</span> that propagate in buried iron <span class="hlt">water</span> pipes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Long, R; Lowe, M; Cawley, P</p> <p>2003-09-01</p> <p>The attenuation of the fundamental non-torsional <span class="hlt">modes</span> that propagate down buried iron <span class="hlt">water</span> pipes has been studied. The <span class="hlt">mode</span> shapes, <span class="hlt">mode</span> attenuation due to leakage into the surrounding medium and the scattering of the <span class="hlt">modes</span> as they interact with pipe joints and fittings have been investigated. In the low frequency region the <span class="hlt">mode</span> predicted to dominate over significant propagation distances approximates a plane wave in the <span class="hlt">water</span> within the pipe. The established acoustic technique used to locate leaks in buried iron <span class="hlt">water</span> pipes assumes that leak noise propagates as a single non-dispersive <span class="hlt">mode</span> at a velocity related to the low frequency asymptote of this <span class="hlt">water</span> borne <span class="hlt">mode</span>. Experiments have been conducted on buried <span class="hlt">water</span> mains at test sites in the UK to verify the attenuation and velocity dispersion predictions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004HMR....58...11C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004HMR....58...11C"><span>Larval development of the <span class="hlt">subantarctic</span> king crabs Lithodes santolla and Paralomis granulosa reared in the laboratory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calcagno, J. A.; Anger, K.; Lovrich, G. A.; Thatje, S.; Kaffenberger, A.</p> <p>2004-02-01</p> <p>The larval development and survival in the two <span class="hlt">subantarctic</span> lithodid crabs Lithodes santolla (Jaquinot) and Paralomis granulosa (Molina) from the Argentine Beagle Channel were studied in laboratory cultures. In L. santolla, larval development lasted about 70 days, passing through three zoeal stages and the megalopa stage, with a duration of approximately 4, 7, 11 and 48 days, respectively. The larval development in P. granulosa is more abbreviated, comprising only two zoeal stages and the megalopa stage, with 6, 11 and 43 days' duration, respectively. In both species, we tested for effects of presence versus absence of food (Artemia nauplii) on larval development duration and survival rate. In P. granulosa, we also studied effects of different rearing conditions, such as individual versus mass cultures, as well as aerated versus unaerated cultures. No differences in larval development duration and survival were observed between animals subjected to those different rearing conditions. The lack of response to the presence or absence of potential food confirms, in both species, a complete lecithotrophic <span class="hlt">mode</span> of larval development. Since lithodid crabs are of high economic importance in the artisanal fishery in the southernmost parts of South America, the knowledge of optimal rearing conditions for lithodid larvae is essential for future attempts at repopulating the collapsing natural stocks off Tierra del Fuego.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19661523','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19661523"><span>Campylobacter subantarcticus sp. nov., isolated from birds in the <span class="hlt">sub-Antarctic</span> region.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Debruyne, Lies; Broman, Tina; Bergström, Sven; Olsen, Björn; On, Stephen L W; Vandamme, Peter</p> <p>2010-04-01</p> <p>Six Gram-stain-negative, spiral-shaped, microaerobic isolates were obtained during a sampling from wild birds in the <span class="hlt">sub-Antarctic</span> region. Based on initial observations, these isolates were classified as Campylobacter lari-like. The isolates were further characterized by whole-cell protein and amplified fragment length polymorphism (AFLP) analysis, which revealed that they were distinct from C. lari and all other known species of the genus Campylobacter. Here, we present comprehensive phylogenetic, genomic and phenotypic evidence that these isolates represent a novel species within the genus Campylobacter, for which the name Campylobacter subantarcticus sp. nov. is proposed. The type strain is R-3023(T) (=LMG 24377(T) =CCUG 38513(T)).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMOS34A..01P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMOS34A..01P"><span>Submarine glacial landforms and interactions with volcanism around <span class="hlt">Sub-Antarctic</span> Heard and McDonald Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Picard, K.; Watson, S. J.; Fox, J. M.; Post, A.; Whittaker, J. M.; Lucieer, V.; Carey, R.; Coffin, M. F.; Hodgson, D.; Hogan, K.; Graham, A. G. C.</p> <p>2017-12-01</p> <p>Unravelling the glacial history of <span class="hlt">Sub-Antarctic</span> islands can provide clues to past climate and Antarctic ice sheet stability. The glacial history of many <span class="hlt">sub-Antarctic</span> islands is poorly understood, including the Heard and McDonald Islands (HIMI) located on the Kerguelen Plateau in the southern Indian Ocean. The geomorphologic development of HIMI has involved a combination of construction via hotspot volcanism and mechanical erosion caused by waves, weather, and glaciers. Today, the 2.5 km2 McDonald Islands are not glacierised; in contrast, the 368 km2 Heard Island has 12 major glaciers, some extending from the summit of 2813 m to sea level. Historical accounts from Heard Island suggest that the glaciers were more extensive in the 1850s to 1870s, and have retreated at least 12% (33.89 km2) since 1997. However, surrounding bathymetry suggests a much more extensive previous glaciation of the HIMI region that encompassed 9,585 km2, likely dating back at least to the Last Glacial Maximum (LGM) ca. 26.5 -19 ka. We present analyses of multibeam bathymetry and backscatter data, acquired aboard RV Investigator in early 2016, that support the previous existence of an extensive icecap. These data reveal widespread ice-marginal and subglacial features including moraines, over-deepened troughs, drumlins and crag-and-tails. Glacial landforms suggest paleo-ice flow directions and a glacial extent that are consistent with previously documented broad scale morphological features. We identify >660 iceberg keel scours in <span class="hlt">water</span> depths ranging from 150 - 530 m. The orientations of the iceberg keel scours reflect the predominantly east-flowing Antarctic Circumpolar Current and westerly winds in the region. 40Ar/39Ar dating of volcanic rocks from submarine volcanoes around McDonald Islands suggests that volcanism and glaciation coincided. The flat-topped morphology of these volcanoes may result from lava-ice interaction or erosion by glaciers post eruption during a time of extensive ice</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24727293','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24727293"><span>Mercury exposure in a large <span class="hlt">subantarctic</span> avian community.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carravieri, Alice; Cherel, Yves; Blévin, Pierre; Brault-Favrou, Maud; Chastel, Olivier; Bustamante, Paco</p> <p>2014-07-01</p> <p>Mercury (Hg) contamination poses potential threats to ecosystems worldwide. In order to study Hg bioavailability in the poorly documented southern Indian Ocean, Hg exposure was investigated in the large avian community of Kerguelen Islands. Adults of 27 species (480 individuals) showed a wide range of feather Hg concentrations, from 0.4 ± 0.1 to 16.6 ± 3.8 μg g(-1) dry weight in Wilson's storm petrels and wandering albatrosses, respectively. Hg concentrations increased roughly in the order crustacean- < fish- ≤ squid- ≤ carrion-consumers, confirming that diet, rather than taxonomy, is an important driver of avian Hg exposure. Adults presented higher Hg concentrations than chicks, due to a longer duration of exposure, with the only exception being the <span class="hlt">subantarctic</span> skua, likely because of feeding habits' differences of the two age-classes in this species. High Hg concentrations were reported for three species of the poorly known gadfly petrels, which merit further investigation. Copyright © 2014 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003HMR....57..110T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003HMR....57..110T"><span>Extended hatching periods in the <span class="hlt">subantarctic</span> lithodid crabs Lithodes santolla and Paralomis granulosa (Crustacea: Decapoda: Lithodidae)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thatje, S.; Calcagno, J. A.; Lovrich, G. A.; Sartoris, F. J.; Anger, K.</p> <p>2003-06-01</p> <p>Temporal pattern of hatching was studied in the <span class="hlt">subantarctic</span> lithodid crabs Lithodes santolla (Molina) and Paralomis granulosa (Jaquinot) from the Argentine Beagle Channel. In both species, larval hatching occurred in low daily numbers over an extended period of up to several weeks, depending on hatch size. Low daily hatching activity and low oxygen-consumption rates in freshly hatched P. granulosa larvae are discussed as life history adaptations to, and/or physiological constraints by, the environmental conditions of high latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17070757','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17070757"><span>Isolation and molecular identification of free-living amoebae of the genus Naegleria from Arctic and <span class="hlt">sub-Antarctic</span> regions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>De Jonckheere, Johan F</p> <p>2006-07-01</p> <p>Twenty-three freshwater samples with sediment taken from two regions in the Arctic, Spitzbergen and Greenland, and one region in sub-Antarctica, Ile de la Possession, were cultured for amoebae at 37 degrees C and room temperature (RT). Only two samples yielded amoebae at 37 degrees C and the two isolates were identified from their morphological features to belong to the genus Acanthamoeba. Vahlkampfiid amoebae were isolated from 11 samples at RT. Morphological analysis of the cysts identified all 11 isolates as belonging to the genus Naegleria, although only about half of them (45%) transformed into flagellates. Ribosomal DNA sequence analysis demonstrated that these isolates represent novel species and that N. antarctica, N. dobsoni and N. chilensis are their closest relatives. Not surprisingly, these three species also grow at lower temperatures (<37 degrees C) than the majority of described Naegleria spp. Two of the eight new species were found in both Arctic and <span class="hlt">sub-Antarctic</span> regions, and other new species from the Arctic are closely related to new species from the <span class="hlt">sub-Antarctic</span>. Therefore, it seems the Naegleria gene pool present in the polar regions is different from that found in temperate and tropical regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26725363','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26725363"><span>The hydrogen-bond network of <span class="hlt">water</span> supports propagating optical phonon-like <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Elton, Daniel C; Fernández-Serra, Marivi</p> <p>2016-01-04</p> <p>The local structure of liquid <span class="hlt">water</span> as a function of temperature is a source of intense research. This structure is intimately linked to the dynamics of <span class="hlt">water</span> molecules, which can be measured using Raman and infrared spectroscopies. The assignment of spectral peaks depends on whether they are collective <span class="hlt">modes</span> or single-molecule motions. Vibrational <span class="hlt">modes</span> in liquids are usually considered to be associated to the motions of single molecules or small clusters. Using molecular dynamics simulations, here we find dispersive optical phonon-like <span class="hlt">modes</span> in the librational and OH-stretching bands. We argue that on subpicosecond time scales these <span class="hlt">modes</span> propagate through <span class="hlt">water</span>'s hydrogen-bond network over distances of up to 2 nm. In the long wavelength limit these optical <span class="hlt">modes</span> exhibit longitudinal-transverse splitting, indicating the presence of coherent long-range dipole-dipole interactions, as in ice. Our results indicate the dynamics of liquid <span class="hlt">water</span> have more similarities to ice than previously thought.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29891979','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29891979"><span>Identification of sources and bioaccumulation pathways of MeHg in <span class="hlt">subantarctic</span> penguins: a stable isotopic investigation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Renedo, Marina; Amouroux, David; Pedrero, Zoyne; Bustamante, Paco; Cherel, Yves</p> <p>2018-06-11</p> <p>Seabirds are widely used as bioindicators of mercury (Hg) contamination in marine ecosystems and the investigation of their foraging strategies is of key importance to better understand methylmercury (MeHg) exposure pathways and environmental sources within the different ecosystems. Here we report stable isotopic composition for both Hg mass-dependent (e.g. δ 202 Hg) and mass-independent (e.g. Δ 199 Hg) fractionation (proxies of Hg sources and transformations), carbon (δ 13 C, proxy of foraging habitat) and nitrogen (δ 15 N, proxy of trophic position) in blood of four species of sympatric penguins breeding at the <span class="hlt">subantarctic</span> Crozet Islands (Southern Indian Ocean). Penguins have species-specific foraging strategies, from coastal to oceanic <span class="hlt">waters</span> and from benthic to pelagic dives, and feed on different prey. A progressive increase to heavier Hg isotopic composition (δ 202 Hg and Δ 199 Hg, respectively) was observed from benthic (1.45 ± 0.12 and 1.41 ± 0.06‰) to epipelagic (1.93 ± 0.18 and 1.77 ± 0.13‰) penguins, indicating a benthic-pelagic gradient of MeHg sources close to Crozet Islands. The relative variations of MeHg concentration, δ 202 Hg and Δ 199 Hg with pelagic penguins feeding in Polar Front circumpolar <span class="hlt">waters</span> (1.66 ± 0.11 and 1.54 ± 0.06‰) support that different MeHg sources occur at large scales in Southern Ocean deep <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15858571','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15858571"><span>Increased productivity in the <span class="hlt">subantarctic</span> ocean during Heinrich events.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sachs, Julian P; Anderson, Robert F</p> <p>2005-04-28</p> <p>Massive iceberg discharges from the Northern Hemisphere ice sheets, 'Heinrich events', coincided with the coldest periods of the last ice age. There is widespread evidence for Heinrich events and their profound impact on the climate and circulation of the North Atlantic Ocean, but their influence beyond that region remains uncertain. Here we use a combination of molecular fingerprints of algal productivity and radioisotope tracers of sedimentation to document eight periods of increased productivity in the subpolar Southern Ocean during the past 70,000 years that occurred within 1,000-2,000 years of a Northern Hemisphere Heinrich event. We discuss possible causes for such a link, including increased supply of iron from upwelling and increased stratification during the growing season, which imply an alteration of the global ocean circulation during Heinrich events. The mechanisms linking North Atlantic iceberg discharges with <span class="hlt">subantarctic</span> productivity remain unclear at this point. We suggest that understanding how the Southern Ocean was altered during these extreme climate perturbations is critical to understanding the role of the ocean in climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22580956','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22580956"><span>Alkane biodegradation genes from chronically polluted <span class="hlt">subantarctic</span> coastal sediments and their shifts in response to oil exposure.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Guibert, Lilian M; Loviso, Claudia L; Marcos, Magalí S; Commendatore, Marta G; Dionisi, Hebe M; Lozada, Mariana</p> <p>2012-10-01</p> <p>Although sediments are the natural hydrocarbon sink in the marine environment, the ecology of hydrocarbon-degrading bacteria in sediments is poorly understood, especially in cold regions. We studied the diversity of alkane-degrading bacterial populations and their response to oil exposure in sediments of a chronically polluted <span class="hlt">Subantarctic</span> coastal environment, by analyzing alkane monooxygenase (alkB) gene libraries. Sequences from the sediment clone libraries were affiliated with genes described in Proteobacteria and Actinobacteria, with 67 % amino acid identity in average to sequences from isolated microorganisms. The majority of the sequences were most closely related to uncultured microorganisms from cold marine sediments or soils from high latitude regions, highlighting the role of temperature in the structuring of this bacterial guild. The distribution of alkB sequences among samples of different sites and years, and selection after experimental oil exposure allowed us to identify ecologically relevant alkB genes in <span class="hlt">Subantarctic</span> sediments, which could be used as biomarkers for alkane biodegradation in this environment. 16 S rRNA amplicon pyrosequencing indicated the abundance of several genera for which no alkB genes have yet been described (Oleispira, Thalassospira) or that have not been previously associated with oil biodegradation (Spongiibacter-formerly Melitea-, Maribius, Robiginitomaculum, Bizionia and Gillisia). These genera constitute candidates for future work involving identification of hydrocarbon biodegradation pathway genes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1242981-hydrogen-bond-network-water-supports-propagating-optical-phonon-like-modes','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1242981-hydrogen-bond-network-water-supports-propagating-optical-phonon-like-modes"><span>The hydrogen-bond network of <span class="hlt">water</span> supports propagating optical phonon-like <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Elton, Daniel C.; Fernández-Serra, Marivi</p> <p>2016-01-04</p> <p>The local structure of liquid <span class="hlt">water</span> as a function of temperature is a source of intense research. This structure is intimately linked to the dynamics of <span class="hlt">water</span> molecules, which can be measured using Raman and infrared spectroscopies. The assignment of spectral peaks depends on whether they are collective <span class="hlt">modes</span> or single-molecule motions. Vibrational <span class="hlt">modes</span> in liquids are usually considered to be associated to the motions of single molecules or small clusters. Using molecular dynamics simulations, here we find dispersive optical phonon-like <span class="hlt">modes</span> in the librational and OH-stretching bands. We argue that on subpicosecond time scales these <span class="hlt">modes</span> propagate through water’smore » hydrogen-bond network over distances of up to 2 nm. In the long wavelength limit these optical <span class="hlt">modes</span> exhibit longitudinal–transverse splitting, indicating the presence of coherent long-range dipole–dipole interactions, as in ice. Lastly, our results indicate the dynamics of liquid <span class="hlt">water</span> have more similarities to ice than previously thought.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG21A0152K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG21A0152K"><span>Normal <span class="hlt">modes</span> of the shallow <span class="hlt">water</span> system on the cubed sphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kang, H. G.; Cheong, H. B.; Lee, C. H.</p> <p>2017-12-01</p> <p>Spherical harmonics expressed as the Rossby-Haurwitz waves are the normal <span class="hlt">modes</span> of non-divergent barotropic model. Among the normal <span class="hlt">modes</span> in the numerical models, the most unstable <span class="hlt">mode</span> will contaminate the numerical results, and therefore the investigation of normal <span class="hlt">mode</span> for a given grid system and a discretiztaion method is important. The cubed-sphere grid which consists of six identical faces has been widely adopted in many atmospheric models. This grid system is non-orthogonal grid so that calculation of the normal <span class="hlt">mode</span> is quiet challenge problem. In the present study, the normal <span class="hlt">modes</span> of the shallow <span class="hlt">water</span> system on the cubed sphere discretized by the spectral element method employing the Gauss-Lobatto Lagrange interpolating polynomials as orthogonal basis functions is investigated. The algebraic equations for the shallow <span class="hlt">water</span> equation on the cubed sphere are derived, and the huge global matrix is constructed. The linear system representing the eigenvalue-eigenvector relations is solved by numerical libraries. The normal <span class="hlt">mode</span> calculated for the several horizontal resolution and lamb parameters will be discussed and compared to the normal <span class="hlt">mode</span> from the spherical harmonics spectral method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26202610','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26202610"><span>Soil invertebrate community change over fuel-contaminated sites on a <span class="hlt">subantarctic</span> island: An ecological field-based line of evidence for site risk assessment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wasley, Jane; Mooney, Thomas J; King, Catherine K</p> <p>2016-04-01</p> <p>A number of fuel spills, of both recent and historic origins, have occurred on World Heritage-listed <span class="hlt">subantarctic</span> Macquarie Island. Sites contaminated by mainly diesel fuels are undergoing remediation by the Australian Antarctic Division. The risks posed by these sites are being managed using a "weight of evidence" approach, for which this study provides a preliminary line of evidence for the ecological assessment component of this site management decision framework. This knowledge is pertinent, given the absence of environmental guidelines for fuel contaminants in <span class="hlt">subantarctic</span> ecosystems. We provide a field-based, site-specific ecological risk assessment for soil invertebrate communities across the fuel spill sites, before the commencement of in situ remediation activities. Springtails (Collembola) were the most abundant taxa. Springtail community patterns showed only limited correlations with the level of fuel contamination at the soil surface, even when elevated levels occurred in the substratum layers. Of the environmental variables measured, community patterns were most strongly correlated with vegetation cover. We identify a suite of 6 species that contribute most to the community dynamics across these sites. A subset of these we propose as useful candidates for future development of single-species toxicity tests: Folsomotoma punctata, Cryptopygus caecus, Cryptopygus antarcticus and Parisotoma insularis. Findings from this study advance our understanding of soil invertebrate community dynamics within these contaminated sites, directly contributing to the improved management and restoration of the sites. Not only does this study provide an important line of evidence for the island's ecological risk assessment for fuel contaminants, it also enhances our understanding of the potential impact of fuels at other <span class="hlt">subantarctic</span> islands. © 2015 SETAC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26842369','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26842369"><span>Different adaptations of Chinese winter-over expeditioners during prolonged Antarctic and <span class="hlt">sub-Antarctic</span> residence.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Nan; Wu, Quan; Li, Hao; Zhang, Tao; Xu, Chengli</p> <p>2016-05-01</p> <p>Prolonged residence in Antarctica is characterized by exposure to isolated, confined, and extreme (ICE) environment. Winter-over expeditioners at research stations often exhibit a complex of psychophysiological symptoms, which varied by stations and sociocultural backgrounds. To understand the different patterns of psychophysiological responses provoked by environmental stress, we conducted a longitudinal assessment of mood and endocrine function in two groups of Chinese expeditioners who were deployed to <span class="hlt">sub-Antarctic</span> (Great Wall Station, 62°S, N = 12) and Antarctic (Zhongshan Station, 66°S, N = 16) from December 2003 to 2005. Measures of mood, thyroid function, the levels of plasma catecholamine, and circulating interleukins were obtained at departure from China, mid-winter (Antarctica), end of winter (Antarctica), and return to China, respectively. The Zhongshan Station crew experienced significant increases in fatigue, anger, tension, confusion, and decrease in free thyroxine (FT4), norepinephrine (NE), and epinephrine (E) during the winter, increase in thyrotropin (TSH) and total triiodothyronine (TT3) when returning, whereas their counterparts at Great Wall Station only experienced increased TT3 after deployment. Moreover, compared with the Great Wall Station crew, the Zhongshan Station crew exhibited greater increase in anger, greater decrease in FT4, total thyroxine (TT4), NE and E over the winter, and greater increase in TSH when returning. Chinese expeditioners who lived and worked at the Antarctic station and the <span class="hlt">sub-Antarctic</span> station for over a year showed different change patterns in mood and endocrine hormones. Negative mood and endocrine dysfunction were positively associated with the severity of environment. The study is a supplement to scientific knowledge on psychophysiological variation under ICE environment, which has certain applied value for the development of preventive countermeasures or interventions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016IJBm...60..737C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016IJBm...60..737C"><span>Different adaptations of Chinese winter-over expeditioners during prolonged Antarctic and <span class="hlt">sub-Antarctic</span> residence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Nan; Wu, Quan; Li, Hao; Zhang, Tao; Xu, Chengli</p> <p>2016-05-01</p> <p>Prolonged residence in Antarctica is characterized by exposure to isolated, confined, and extreme (ICE) environment. Winter-over expeditioners at research stations often exhibit a complex of psychophysiological symptoms, which varied by stations and sociocultural backgrounds. To understand the different patterns of psychophysiological responses provoked by environmental stress, we conducted a longitudinal assessment of mood and endocrine function in two groups of Chinese expeditioners who were deployed to <span class="hlt">sub-Antarctic</span> (Great Wall Station, 62°S, N = 12) and Antarctic (Zhongshan Station, 66°S, N = 16) from December 2003 to 2005. Measures of mood, thyroid function, the levels of plasma catecholamine, and circulating interleukins were obtained at departure from China, mid-winter (Antarctica), end of winter (Antarctica), and return to China, respectively. The Zhongshan Station crew experienced significant increases in fatigue, anger, tension, confusion, and decrease in free thyroxine (FT4), norepinephrine (NE), and epinephrine (E) during the winter, increase in thyrotropin (TSH) and total triiodothyronine (TT3) when returning, whereas their counterparts at Great Wall Station only experienced increased TT3 after deployment. Moreover, compared with the Great Wall Station crew, the Zhongshan Station crew exhibited greater increase in anger, greater decrease in FT4, total thyroxine (TT4), NE and E over the winter, and greater increase in TSH when returning. Chinese expeditioners who lived and worked at the Antarctic station and the <span class="hlt">sub-Antarctic</span> station for over a year showed different change patterns in mood and endocrine hormones. Negative mood and endocrine dysfunction were positively associated with the severity of environment. The study is a supplement to scientific knowledge on psychophysiological variation under ICE environment, which has certain applied value for the development of preventive countermeasures or interventions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23219394','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23219394"><span>Daily accumulation rates of marine debris on <span class="hlt">sub-Antarctic</span> island beaches.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Eriksson, Cecilia; Burton, Harry; Fitch, Stuart; Schulz, Martin; van den Hoff, John</p> <p>2013-01-15</p> <p>The worlds' oceans contain a large but unknown amount of plastic debris. We made daily collections of marine debris stranded at two <span class="hlt">sub-Antarctic</span> islands to establish (a) physical causes of strandings, and (b) a sampling protocol to better estimate the oceans' plastic loading. Accumulation rates at some beaches were dependent on tide and onshore winds. Most of the 6389 items collected were plastic (Macquarie 95%, Heard 94%) and discarded or lost fishing gear comprised 22% of those plastic items. Stalked barnacles (Lepas spp.) were a regular attachment on Macquarie debris but not at Heard Island. The daily accumulation rate of plastic debris on Macquarie Island was an order of magnitude higher than that estimated from monthly surveys during the same 4 months in the previous 5 years. This finding suggests that estimates of the oceans' plastic loading are an order of magnitude too low. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1233183','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1233183"><span><span class="hlt">Mode</span> and Intermediate <span class="hlt">Waters</span> in Earth System Models</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>Gnanadesikan, Anand; Sarmiento, Jorge L.</p> <p></p> <p>This report describes work done as part of a joint Princeton-Johns Hopkins project to look at the impact of <span class="hlt">mode</span> and intermediate <span class="hlt">waters</span> in Earth System Models. The Johns Hopkins portion of this work focussed on the role of lateral mixing in ventilating such <span class="hlt">waters</span>, with important implications for hypoxia, the uptake of anthropogenic carbon, the dynamics of El Nino and carbon pumps. The Johns Hopkins group also collaborated with the Princeton Group to help develop a watermass diagnostics framework.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_1");'>1</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li class="active"><span>3</span></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_3 --> <div id="page_4" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="61"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3733920','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3733920"><span>Mapping <span class="hlt">Sub-Antarctic</span> Cushion Plants Using Random Forests to Combine Very High Resolution Satellite Imagery and Terrain Modelling</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bricher, Phillippa K.; Lucieer, Arko; Shaw, Justine; Terauds, Aleks; Bergstrom, Dana M.</p> <p>2013-01-01</p> <p>Monitoring changes in the distribution and density of plant species often requires accurate and high-resolution baseline maps of those species. Detecting such change at the landscape scale is often problematic, particularly in remote areas. We examine a new technique to improve accuracy and objectivity in mapping vegetation, combining species distribution modelling and satellite image classification on a remote <span class="hlt">sub-Antarctic</span> island. In this study, we combine spectral data from very high resolution WorldView-2 satellite imagery and terrain variables from a high resolution digital elevation model to improve mapping accuracy, in both pixel- and object-based classifications. Random forest classification was used to explore the effectiveness of these approaches on mapping the distribution of the critically endangered cushion plant Azorella macquariensis Orchard (Apiaceae) on <span class="hlt">sub-Antarctic</span> Macquarie Island. Both pixel- and object-based classifications of the distribution of Azorella achieved very high overall validation accuracies (91.6–96.3%, κ = 0.849–0.924). Both two-class and three-class classifications were able to accurately and consistently identify the areas where Azorella was absent, indicating that these maps provide a suitable baseline for monitoring expected change in the distribution of the cushion plants. Detecting such change is critical given the threats this species is currently facing under altering environmental conditions. The method presented here has applications to monitoring a range of species, particularly in remote and isolated environments. PMID:23940805</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610722','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5610722"><span>Nutritional Immunity Triggers the Modulation of Iron Metabolism Genes in the <span class="hlt">Sub-Antarctic</span> Notothenioid Eleginops maclovinus in Response to Piscirickettsia salmonis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Martínez, Danixa; Oyarzún, Ricardo; Pontigo, Juan Pablo; Romero, Alex; Yáñez, Alejandro J.; Vargas-Chacoff, Luis</p> <p>2017-01-01</p> <p>Iron deprivation is a nutritional immunity mechanism through which fish can limit the amount of iron available to invading bacteria. The aim of this study was to evaluate the modulation of iron metabolism genes in the liver and brain of <span class="hlt">sub-Antarctic</span> notothenioid Eleginops maclovinus challenged with Piscirickettsia salmonis. The specimens were inoculated with two P. salmonis strains: LF-89 (ATCC® VR-1361™) and Austral-005 (antibiotic resistant). Hepatic and brain samples were collected at intervals over a period of 35 days. Gene expression (by RT-qPCR) of proteins involved in iron storage, transport, and binding were statistically modulated in infected fish when compared with control counterparts. Specifically, the expression profiles of the transferrin and hemopexin genes in the liver, as well as the expression profiles of ferritin-M, ferritin-L, and transferrin in the brain, were similar for both experimental groups. Nevertheless, the remaining genes such as ferritin-H, ceruloplasmin, hepcidin, and haptoglobin presented tissue-specific expression profiles that varied in relation to the injected bacterial strain and sampling time-point. These results suggest that nutritional immunity could be an important immune defense mechanism for E. maclovinus against P. salmonis injection. This study provides relevant information for understanding iron metabolism of a <span class="hlt">sub-Antarctic</span> notothenioid fish. PMID:28974951</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012CPL...554..243K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012CPL...554..243K"><span>Local vibrational <span class="hlt">modes</span> of the <span class="hlt">water</span> dimer - Comparison of theory and experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kalescky, R.; Zou, W.; Kraka, E.; Cremer, D.</p> <p>2012-12-01</p> <p>Local and normal vibrational <span class="hlt">modes</span> of the <span class="hlt">water</span> dimer are calculated at the CCSD(T)/CBS level of theory. The local H-bond stretching frequency is 528 cm-1 compared to a normal <span class="hlt">mode</span> stretching frequency of just 143 cm-1. The adiabatic connection scheme between local and normal vibrational <span class="hlt">modes</span> reveals that the lowering is due to mass coupling, a change in the anharmonicity, and coupling with the local HOH bending <span class="hlt">modes</span>. The local <span class="hlt">mode</span> stretching force constant is related to the strength of the H-bond whereas the normal <span class="hlt">mode</span> stretching force constant and frequency lead to an erroneous underestimation of the H-bond strength.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JPhCS..79a2015F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JPhCS..79a2015F"><span><span class="hlt">Water</span>-sensitive positron trapping <span class="hlt">modes</span> in nanoporous magnesium aluminate ceramics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Filipecki, J.; Ingram, A.; Klym, H.; Shpotyuk, O.; Vakiv, M.</p> <p>2007-08-01</p> <p>The <span class="hlt">water</span>-sensitive positron trapping <span class="hlt">modes</span> in nanoporous MgAl2O4 ceramics with a spinel structure are studied. It is shown that <span class="hlt">water</span>-sorption processes in magnesium aluminate ceramics leads to corresponding increase in positron trapping rates of extended defects located near intergranual boundaries. This catalytic affect has reversible nature, being strongly dependent on sorption <span class="hlt">water</span> fluxes in ceramics. The fixation of all <span class="hlt">water</span>-dependent positron trapping inputs allow to refine the most significant changes in positron trapping rate of extended defects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002PalOc..17.1004B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002PalOc..17.1004B"><span>Late Oligocene to early Miocene geochronology and paleoceanography from the <span class="hlt">subantarctic</span> 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>Billups, K.; Channell, J. E. T.; Zachos, J.</p> <p>2002-01-01</p> <p>At Ocean Drilling Program (ODP) Site 1090 on the Agulhas Ridge (<span class="hlt">subantarctic</span> South Atlantic) benthic foraminiferal stable isotope records span the late Oligocene through the early Miocene (25-16 Ma) at a temporal resolution of ~10 kyr. In the same time interval a magnetic polarity stratigraphy can be unequivocally correlated to the geomagnetic polarity timescale (GPTS), thereby providing secure correlation of the isotope record to the GPTS. On the basis of the isotope-magnetostratigraphic correlation we provide refined age calibration of established oxygen isotope events Mi1 through Mi2 as well as several other distinctive isotope events. Our data suggest that the δ18O maximum commonly associated with the Oligocene/Miocene (O/M) boundary falls within C6Cn.2r (23.86 Ma). The δ13C maximum coincides, within the temporal resolution of our record, with C6Cn.2n/r boundary and hence to the O/M boundary. Comparison of the stable isotope record from ODP Site 1090 to the orbitally tuned stable isotope record from ODP Site 929 across the O/M boundary shows that variability in the two records is very similar and can be correlated at and below the O/M boundary. Site 1090 stable isotope records also provide the first deep Southern Ocean end-member for reconstructions of circulation patterns and late Oligocene to early Miocene climate change. Comparison to previously published records suggests that basin to basin carbon isotope gradients were small or nonexistent and are inconclusive with respect to the direction of deep <span class="hlt">water</span> flow. Oxygen isotope gradients between sites suggest that the deep Southern Ocean was cold in comparison to the North Atlantic, Indian, and the Pacific Oceans. Dominance of cold Southern Component Deep <span class="hlt">Water</span> at Site 1090, at least until 17 Ma, suggests that relatively cold circumpolar climatic conditions prevailed during the late Oligocene and early Miocene. We believe that a relatively cold Southern Ocean reflects unrestricted circumpolar flow through</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27389459','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27389459"><span>Assessing fuel spill risks in polar <span class="hlt">waters</span>: Temporal dynamics and behaviour of hydrocarbons from Antarctic diesel, marine gas oil and residual fuel oil.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Brown, Kathryn E; King, Catherine K; Kotzakoulakis, Konstantinos; George, Simon C; Harrison, Peter L</p> <p>2016-09-15</p> <p>As part of risk assessment of fuel oil spills in Antarctic and <span class="hlt">subantarctic</span> <span class="hlt">waters</span>, this study describes partitioning of hydrocarbons from three fuels (Special Antarctic Blend diesel, SAB; marine gas oil, MGO; and intermediate grade fuel oil, IFO 180) into seawater at 0 and 5°C and subsequent depletion over 7days. Initial total hydrocarbon content (THC) of <span class="hlt">water</span> accommodated fraction (WAF) in seawater was highest for SAB. Rates of THC loss and proportions in equivalent carbon number fractions differed between fuels and over time. THC was most persistent in IFO 180 WAFs and most rapidly depleted in MGO WAF, with depletion for SAB WAF strongly affected by temperature. Concentration and composition remained proportionate in dilution series over time. This study significantly enhances our understanding of fuel behaviour in Antarctic and <span class="hlt">subantarctic</span> <span class="hlt">waters</span>, enabling improved predictions for estimates of sensitivities of marine organisms to toxic contaminants from fuels in the region. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25947505','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25947505"><span>Description of Pseudingolfiella possessionis n. sp. (Crustacea, Amphipoda) from <span class="hlt">sub-Antarctic</span> Île de La Possession, Crozet archipelago: the second freshwater amphipod known from the Antarctic biome, a human introduction of Gondwanan ancestry?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Smet, Willem H De</p> <p>2015-03-31</p> <p>A new species of freshwater amphipod, Pseudingolfiella possessionis n. sp. (Senticaudata, Pseudingolfiellidae), is described from the submerged moss vegetation of small brooklets at <span class="hlt">sub-Antarctic</span> Île de La Possession, Crozet archipelago. It constitutes the second freshwater amphipod species known for the <span class="hlt">sub-Antarctic</span> and Antarctic region, and the fourth member of the genus. The main characters distinguishing it from all congeners are: the spine on the posterior margin of the dactylus, incisor and lamina mobilis of mandible each with 5 teeth, the setation of the maxilliped, the vestigial second article of pleopod 3 in the female, the undulate and laterally notched posterolateral margin of the external ramus of uropods 1 and 2 in the male, the spinulate dorsomedian projection of the telson.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP43B1459B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP43B1459B"><span>A multiproxy fjord sediment record of Holocene climate change from the <span class="hlt">subantarctic</span> Auckland Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Browne, I. M.; Moy, C. M.; Wilson, G. S.; Neil, H.; Riesselman, C. R.</p> <p>2014-12-01</p> <p>The Southern Hemisphere Westerly Winds (SHWW) and the associated oceanic fronts have a major influence on atmospheric and oceanic circulation in the Southern Hemisphere. Sediment cores recovered from fjords along the eastern margin of the <span class="hlt">sub-Antarctic</span> Auckland Islands (51°S, 166°E) are ideally located to sensitively record changes in the strength and position of the SHWW throughout the Holocene. A 5.75m core from Hanfield Inlet preserves both marine and terrestrial environmental components, which we use to develop a multiproxy record of past climatic conditions. This core, composed entirely of brown marine mud and silt, was recovered from a depth of 44m. Based on the entrance sill depth of the fjord (10mbsl) and our knowledge of regional sea level rise, we infer that the base of the core will be early Holocene in age, which will be confirmed using radiocarbon age dating. Benthic foraminiferal assemblages (125-500μm fraction) in surface and downcore samples are dominated by three taxa, Nonionellina flemingi, Cassidulina carinata and Quinqueloculina seminula. These species are either shallow infaunal or infaunal. We will use stable carbon (δ¹³C) and oxygen (δ¹⁸O) isotope geochemistry of the benthic foraminifera Nonionellina flemingi, Bolivina cf. earlandi, Trifarina angulosa, Bulimina marginata f. marginata and Cibicides species (all identified from Rose Bengal stained box-core samples) to reconstruct <span class="hlt">water</span> column fluctuations associated with frontal migration. These results will compliment bulk sediment C and N concentration and isotope reconstructions of terrestrial organic matter delivery to fjord sub-basins over the past 12,000 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010QSRv...29.1228H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010QSRv...29.1228H"><span>Intermediate and deep <span class="hlt">water</span> mass distribution in the Pacific during the Last Glacial Maximum inferred from oxygen and carbon stable isotopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Herguera, J. C.; Herbert, T.; Kashgarian, M.; Charles, C.</p> <p>2010-05-01</p> <p>Intermediate ocean circulation changes during the last Glacial Maximum (LGM) in the North Pacific have been linked with Northern Hemisphere climate through air-sea interactions, although the extent and the source of the variability of the processes forcing these changes are still not well resolved. The ventilated volumes and ages in the upper wind driven layer are related to the wind stress curl and surface buoyancy fluxes at mid to high latitudes in the North Pacific. In contrast, the deeper thermohaline layers are more effectively ventilated by direct atmosphere-sea exchange during convective formation of <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Waters</span> (SAMW) and Antarctic Intermediate <span class="hlt">Waters</span> (AAIW) in the Southern Ocean, the precursors of Pacific Intermediate <span class="hlt">Waters</span> (PIW) in the North Pacific. Results reported here show a fundamental change in the carbon isotopic gradient between intermediate and deep <span class="hlt">waters</span> during the LGM in the eastern North Pacific indicating a deepening of nutrient and carbon rich <span class="hlt">waters</span>. These observations suggest changes in the source and nature of intermediate <span class="hlt">waters</span> of Southern Ocean origin that feed PIW and enhanced ventilation processes in the North Pacific, further affecting paleoproductivity and export patters in this basin. Furthermore, oxygen isotopic results indicate these changes may have been accomplished in part by changes in circulation affecting the intermediate depths during the LGM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23086282','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23086282"><span>ATP regulation of the ligand-binding properties in temperate and cold-adapted haemoglobins. X-ray structure and ligand-binding kinetics in the <span class="hlt">sub-Antarctic</span> fish Eleginops maclovinus.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Coppola, Daniela; Abbruzzetti, Stefania; Nicoletti, Francesco; Merlino, Antonello; Gambacurta, Alessandra; Giordano, Daniela; Howes, Barry D; De Sanctis, Giampiero; Vitagliano, Luigi; Bruno, Stefano; di Prisco, Guido; Mazzarella, Lelio; Smulevich, Giulietta; Coletta, Massimo; Viappiani, Cristiano; Vergara, Alessandro; Verde, Cinzia</p> <p>2012-10-30</p> <p>The major haemoglobin of the <span class="hlt">sub-Antarctic</span> fish Eleginops maclovinus was structurally and functionally characterised with the aim to compare molecular environmental adaptations in the O(2)-transport system of <span class="hlt">sub-Antarctic</span> fishes of the suborder Notothenioidei with those of their high-latitude relatives. Ligand-binding kinetics of the major haemoglobin of E. maclovinus indicated strong stabilisation of the liganded quaternary T state, enhanced in the presence of the physiological allosteric effector ATP, compared to that of high-Antarctic Trematomus bernacchii. The activation enthalpy for O(2) dissociation was dramatically lower than that in T. bernacchii haemoglobin, suggesting remarkable differences in temperature sensitivity and structural changes associated with O(2) release and exit from the protein. The haemoglobin functional properties, together with the X-ray structure of the CO form at 1.49 Å resolution, the first of a temperate notothenioid, strongly support the hypothesis that in E. maclovinus, whose life-style varies according to changes in habitat, the mechanisms that regulate O(2) affinity and the ATP-induced Root effect differ from those of high-Antarctic Notothenioids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012CSR....43...36M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012CSR....43...36M"><span>Aspects of reproductive ecology and benthic-pelagic coupling in the <span class="hlt">sub-antarctic</span> sea cucumber Pseudostichopus mollis (Theel)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morgan, Andrew; Neal, Lance</p> <p>2012-07-01</p> <p>For deeper regions of the continental shelf environmental cues entraining reproduction in echinoderms are often absent, which contributes to adoption of continuous reproduction, having larger eggs, and a lecithotrophic <span class="hlt">mode</span> of larval development. In the present study the <span class="hlt">sub-Antarctic</span> sea cucumber Pseudostichopus mollis from the family Synallactidae was obtained during June (winter) and September (spring) from a depth of approximately 300 m north of the Auckland Islands in an area abundant in biogenic sediments. Samples were processed for body indices and gonad development. Features characteristic of non-continuous reproduction were exhibited. Although a larger egg size was found (212±14 μm), two distinct winter cohorts of oocytes occurred (41-81 and 161-201 μm) and body wall weight fluctuations (7.6% increase in males and 27.5% reduction in females) coincided with changes in gonad indices between sample dates. For males gonad as a proportion of body wall weight decreased from 3.31±0.9 to 2.11±0.37% and for females it increased from 1.59±0.28 to 2.5±0.30%. For both sample dates the gonad of males maintained mature spermatozoa whereas female gonad shifted from mainly recovery and growth of oocytes to growth and advanced growth of mature oocytes. In habitats with low or variable food availability intermittent reproduction is predicted as resources are too low for a high reproductive effort and too erratic for synchrony. A pattern of reproduction where fluctuations in seasonal organic input into an accumulated benthic food source initiates and synchronises gametogenesis for future spawning is proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15755885','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15755885"><span>Deleterious effects of repeated cold exposure in a freeze-tolerant <span class="hlt">sub-Antarctic</span> caterpillar.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sinclair, Brent J; Chown, Steven L</p> <p>2005-03-01</p> <p>Multiple freeze-thaw cycles are common in alpine, polar and temperate habitats. We investigated the effects of five consecutive cycles of approx. -5 degrees C on the freeze-tolerant larvae of Pringleophaga marioni Viette (Lepidoptera: Tineidae) on <span class="hlt">sub-Antarctic</span> Marion Island. The likelihood of freezing was positively correlated with body mass, and decreased from 70% of caterpillars that froze on initial exposure to 55% of caterpillars that froze on subsequent exposures; however, caterpillars retained their freeze tolerance and did not appear to switch to a freeze-avoiding strategy. Apart from an increase in gut <span class="hlt">water</span>, there was no difference in body composition of caterpillars frozen 0 to 5 times, suggesting that the observed effects were not due to freezing, but rather to exposure to cold per se. Repeated cold exposure did not result in mortality, but led to decreased mass, largely accounted for by a decreased gut mass caused by cessation of feeding by caterpillars. Treatment caterpillars had fragile guts with increased lipid content, suggesting damage to the gut epithelium. These effects persisted for 5 days after the final exposure to cold, and after 30 days, treatment caterpillars had regained their pre-exposure mass, whereas their control counterparts had significantly gained mass. We show that repeated cold exposure does occur in the field, and suggest that this may be responsible for the long life cycle in P. marioni. Although mean temperatures are increasing on Marion Island, several climate change scenarios predict an increase in exposures to sub-zero temperatures, which would result in an increased generation time for P. marioni. Coupled with increased predation from introduced house mice on Marion Island, this could have severe consequences for the P. marioni population.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4740428','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4740428"><span>Observing mesoscale eddy effects on <span class="hlt">mode-water</span> subduction and transport in the North Pacific</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Xu, Lixiao; Li, Peiliang; Xie, Shang-Ping; Liu, Qinyu; Liu, Cong; Gao, Wendian</p> <p>2016-01-01</p> <p>While modelling studies suggest that mesoscale eddies strengthen the subduction of <span class="hlt">mode</span> <span class="hlt">waters</span>, this eddy effect has never been observed in the field. Here we report results from a field campaign from March 2014 that captured the eddy effects on <span class="hlt">mode-water</span> subduction south of the Kuroshio Extension east of Japan. The experiment deployed 17 Argo floats in an anticyclonic eddy (AC) with enhanced daily sampling. Analysis of over 3,000 hydrographic profiles following the AC reveals that potential vorticity and apparent oxygen utilization distributions are asymmetric outside the AC core, with enhanced subduction near the southeastern rim of the AC. There, the southward eddy flow advects newly ventilated <span class="hlt">mode</span> <span class="hlt">water</span> from the north into the main thermocline. Our results show that subduction by eddy lateral advection is comparable in magnitude to that by the mean flow—an effect that needs to be better represented in climate models. PMID:26829888</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ClDy...48.4093M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ClDy...48.4093M"><span>Interannual variability of Indian Ocean subtropical <span class="hlt">mode</span> <span class="hlt">water</span> subduction rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Jie; Lan, Jian</p> <p>2017-06-01</p> <p>The interannual variation of Indian Ocean subtropical <span class="hlt">mode</span> <span class="hlt">water</span> (IOSTMW) subduction rate in the Southwest Indian Ocean from 1980 to 2007 is investigated in this paper based on Simple Ocean Data Assimilation (SODA) outputs. Climatology of subduction rate exceeds 75 m/year in the IOSTMW formation area. The renewal time of permanent pycnocline <span class="hlt">water</span> mass based on the subduction rate is calculated for each density class: 3-6 years for IOSTMW (25.8 < σ θ < 26.2 kg m-3). Subduction rate in the Southwest Indian Ocean subtropical gyre exhibits a great year-to-year variability. This interannual variations of the IOSTMW subduction rate is primarily dominated by the lateral induction term, associated with the interannual variations of strong meridional gradient of winter mixed layer depth (MLD). The slope of the mixed layer depth in the <span class="hlt">mode</span> <span class="hlt">water</span> is closely linked to the large variations of deep late winter MLD in the mid-latitudes and negligible variations of shallow winter MLD in lower latitudes. It is further identified that the interannual variation of late winter MLD in this area is largely controlled by the latent and sensible heat flux components. The <span class="hlt">water</span> volume of the permanent pycnocline in the IOSTMW distribution area is also found to show a significant interannual variability, and it is well correlated with the interannual variation of subduction rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70011199','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70011199"><span>Analysis of spurious oscillation <span class="hlt">modes</span> for the shallow <span class="hlt">water</span> and Navier-Stokes equations</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Walters, R.A.; Carey, G.F.</p> <p>1983-01-01</p> <p>The origin and nature of spurious oscillation <span class="hlt">modes</span> that appear in mixed finite element methods are examined. In particular, the shallow <span class="hlt">water</span> equations are considered and a modal analysis for the one-dimensional problem is developed. From the resulting dispersion relations we find that the spurious <span class="hlt">modes</span> in elevation are associated with zero frequency and large wave number (wavelengths of the order of the nodal spacing) and consequently are zero-velocity <span class="hlt">modes</span>. The spurious modal behavior is the result of the finite spatial discretization. By means of an artificial compressibility and limiting argument we are able to resolve the similar problem for the Navier-Stokes equations. The relationship of this simpler analysis to alternative consistency arguments is explained. This modal approach provides an explanation of the phenomenon in question and permits us to deduce the cause of the very complex behavior of spurious <span class="hlt">modes</span> observed in numerical experiments with the shallow <span class="hlt">water</span> equations and Navier-Stokes equations. Furthermore, this analysis is not limited to finite element formulations, but is also applicable to finite difference formulations. ?? 1983.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDM36006M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDM36006M"><span><span class="hlt">Modes</span> of elastic plates and shells in <span class="hlt">water</span> driven by modulated radiation pressure of focused ultrasound</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Marston, Philip L.; Daniel, Timothy D.; Abawi, Ahmad T.; Kirsteins, Ivars</p> <p>2015-11-01</p> <p>The modulated radiation pressure (MRP) of ultrasound has been used for decades to selectively excite low frequency <span class="hlt">modes</span> associated with surface tension of fluid objects in <span class="hlt">water</span>. Much less is known about the excitation of low frequency <span class="hlt">modes</span> of less compliant metallic objects. Here we use MRP of focused ultrasound to excite resonant flexural vibrations of a circular metal plate in <span class="hlt">water</span>. The source transducer was driven with a double-sideband suppressed carrier voltage as in. The response of the target (detected with a hydrophone) was at twice the modulation frequency and proportional to the square of the drive voltage. Since the radiation pressure of focused beams is spatially localized, <span class="hlt">mode</span> shapes could be identified by scanning the source along the target while measuring the target's response. Additional measurements were done with an open-ended <span class="hlt">water</span>-filled copper circular cylindrical shell in which resonant frequencies and <span class="hlt">mode</span> shapes were also identified. These experiments show how focused ultrasound can be used to identify low-frequency <span class="hlt">modes</span> of elastic objects without direct contact. Supported by ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23742520','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23742520"><span>Instantaneous normal <span class="hlt">mode</span> analysis of the vibrational relaxation of the amide I <span class="hlt">mode</span> of alanine dipeptide in <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Farag, Marwa H; Zúñiga, José; Requena, Alberto; Bastida, Adolfo</p> <p>2013-05-28</p> <p>Nonequilibrium Molecular Dynamics (MD) simulations coupled to instantaneous normal <span class="hlt">modes</span> (INMs) analysis are used to study the vibrational relaxation of the acetyl and amino-end amide I <span class="hlt">modes</span> of the alanine dipeptide (AlaD) molecule dissolved in <span class="hlt">water</span> (D2O). The INMs are assigned in terms of the equilibrium normal <span class="hlt">modes</span> using the Effective Atomic Min-Cost algorithm as adapted to make use of the outputs of standard MD packages, a method which is well suited for the description of flexible molecules. The relaxation energy curves of both amide I <span class="hlt">modes</span> show multiexponential decays, in good agreement with the experimental findings. It is found that ~85%-90% of the energy relaxes through intramolecular vibrational redistribution. The main relaxation pathways are also identified. The rate at which energy is transferred into the solvent is similar for the acetyl-end and amino-end amide I <span class="hlt">modes</span>. The conformational changes occurring during relaxation are investigated, showing that the populations of the alpha and beta region conformers are altered by energy transfer in such a way that it takes 15 ps for the equilibrium conformational populations to be recovered after the initial excitation of the AlaD molecule.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1015c2008A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1015c2008A"><span>Non-linear multi-objective model for planning <span class="hlt">water</span>-energy <span class="hlt">modes</span> of Novosibirsk Hydro Power Plant</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alsova, O. K.; Artamonova, A. V.</p> <p>2018-05-01</p> <p>This paper presents a non-linear multi-objective model for planning and optimizing of <span class="hlt">water</span>-energy <span class="hlt">modes</span> for the Novosibirsk Hydro Power Plant (HPP) operation. There is a very important problem of developing a strategy to improve the scheme of <span class="hlt">water</span>-power <span class="hlt">modes</span> and ensure the effective operation of hydropower plants. It is necessary to determine the methods and criteria for the optimal distribution of <span class="hlt">water</span> resources, to develop a set of models and to apply them to the software implementation of a DSS (decision-support system) for managing Novosibirsk HPP <span class="hlt">modes</span>. One of the possible versions of the model is presented and investigated in this paper. Experimental study of the model has been carried out with 2017 data and the task of ten-day period planning from April to July (only 12 ten-day periods) was solved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.V43F..08W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.V43F..08W"><span>Submarine geology and geomorphology of active <span class="hlt">Sub-Antarctic</span> volcanoes: Heard and McDonald Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Watson, S. J.; Coffin, M. F.; Whittaker, J. M.; Lucieer, V.; Fox, J. M.; Carey, R.; Arculus, R. J.; Bowie, A. R.; Chase, Z.; Robertson, R.; Martin, T.; Cooke, F.</p> <p>2016-12-01</p> <p>Heard and McDonald Islands (HIMI) are World Heritage listed <span class="hlt">sub-Antarctic</span> active volcanic islands in the Southern Indian Ocean. Built atop the Kerguelen Plateau by Neogene-Quaternary volcanism, HIMI represent subaerial exposures of the second largest submarine Large Igneous Province globally. Onshore, processes influencing island evolution include glaciers, weathering, volcanism, vertical tectonics and mass-wasting (Duncan et al. 2016). <span class="hlt">Waters</span> surrounding HIMI are largely uncharted, due to their remote location. Hence, the extent to which these same processes shape the submarine environment around HIMI has not been investigated. In early 2016, we conducted marine geophysical and geologic surveys around HIMI aboard RV Investigator (IN2016_V01). Results show that volcanic and sedimentary features prominently trend east-west, likely a result of erosion by the eastward flowing Antarctic Circumpolar Current and tidal currents. However, spatial patterns of submarine volcanism and sediment distribution differ substantially between the islands. >70 sea knolls surround McDonald Island suggesting substantial submarine volcanism. Geophysical data reveals hard volcanic seafloor around McDonald Island, whereas Heard Island is characterised by sedimentary sequences tens of meters or more thick and iceberg scours - indicative of glacial processes. Differences in submarine geomorphology are likely due to the active glaciation of Heard Island and differing rock types (Heard: alkali basalt, McDonald: phonolite), and dominant products (clastics vs. lava). Variations may also reflect different magmatic plumbing systems beneath the two active volcanoes (Heard produces larger volumes of more focused lava, whilst McDonald extrudes smaller volumes of more evolved lavas from multiple vents across the edifice). Using geophysical data, corroborated with new and existing geologic data, we present the first geomorphic map revealing the processes that shape the submarine environment around HIMI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26043371','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26043371"><span><span class="hlt">Water</span> reclamation from emulsified oily wastewater via effective forward osmosis hollow fiber membranes under the PRO <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Gang; de Wit, Jos S; Chung, Tai-Shung</p> <p>2015-09-15</p> <p>By using a novel hydrophilic cellulose acetate butyrate (CAB) as the membrane material for the hollow fiber substrate and modifying its outer surface by polydopamine (PDA) coating and inner surface by interfacial polymerization, we have demonstrated that the thin-film composite (TFC) membranes can be effectively used for sustainable <span class="hlt">water</span> reclamation from emulsified oil/<span class="hlt">water</span> streams via forward osmosis (FO) under the pressure retarded osmosis (PRO) <span class="hlt">mode</span>. The newly developed TFC-FO hollow fiber membrane shows characteristics of high <span class="hlt">water</span> flux, outstanding salt and oil rejection, and low fouling propensity. Under the PRO <span class="hlt">mode</span>, the newly developed TFC-FO membrane exhibits a <span class="hlt">water</span> flux of 37.1 L m(-2) h(-1) with an oil rejection of 99.9% using a 2000 ppm soybean oil/<span class="hlt">water</span> emulsion as the feed and 1 M NaCl as the draw solution. Remarkable anti-fouling behaviors have also been observed. Under the PRO <span class="hlt">mode</span>, the <span class="hlt">water</span> flux decline is only 10% of the initial value even after a 12 h test for oil/<span class="hlt">water</span> separation. The <span class="hlt">water</span> flux of the fouled membrane can be effectively restored to 97% of the original value by <span class="hlt">water</span> rinses on the fiber outer surface without using any chemicals. Furthermore, the flux declines are only 25% and 52% when the <span class="hlt">water</span> recovery of a 2000 ppm soybean oil/<span class="hlt">water</span> emulsion and a 2000 ppm petroleum oil/<span class="hlt">water</span> emulsion containing 0.04 M NaCl reaches 82%, respectively. This study may not only provide insightful guidelines for the fabrication of effective TFC-FO membranes with high performance and low fouling behaviors for oily wastewater under the PRO <span class="hlt">mode</span> but also add an alternative perspective to the design of new materials for <span class="hlt">water</span> purification purposes. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_2");'>2</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li class="active"><span>4</span></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_4 --> <div id="page_5" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="81"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMOS33E..03T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMOS33E..03T"><span><span class="hlt">Mode</span> <span class="hlt">Water</span> Formation via Cabbeling and Submesoscale Lateral Mixing at a Strained Thermohaline Front</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Thomas, L. N.; Shakespeare, C. J.</p> <p>2014-12-01</p> <p><span class="hlt">Mode</span> <span class="hlt">waters</span> play an important role in interannual climate variability through the temporary storage of heat and carbon in the ocean. The mechanisms explaining their formation are not well understood but appear to be shaped by the dynamics of the ocean fronts that mark their poleward extent. We explore a <span class="hlt">mode</span> <span class="hlt">water</span> formation mechanism that has a clear connection to fronts and involves cabbeling. Cabbeling refers to the process by which two <span class="hlt">water</span> masses of equal density but different temperature and salinity are combined to create a new, denser <span class="hlt">water</span> mass, as a result of nonlinearities in the equation of state for seawater. The work is motivated in part by recent observations of an extremely sharp, density-compensated front at the north wall of the Gulf Stream, the boundary between the subtropical and subpolar gyres. Here, the inter-gyre salinity/temperature difference is compressed into a span of a few kilometers, making the flow susceptible to cabbeling. The sharpness of the front is caused by frontogenetic strain, which is presumably balanced by submesoscale lateral mixing processes. We study this balance with a simple analytical model of a thermohaline front forced by uniform strain and derive a scaling for the amount of <span class="hlt">water</span> mass transformation resulting from the ensuing cabbeling. The theory suggests that this mechanism could be responsible for persistent, hence significant, <span class="hlt">mode</span> <span class="hlt">water</span> formation. As such, it represents a submesoscale process that impacts the ocean on basin scales that should be resolved or parameterized in realistic numerical simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..109M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..109M"><span>Four Years of North Pacific <span class="hlt">Mode</span> <span class="hlt">Water</span> Evolution: A Fukushima Tracer Perspective</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macdonald, Alison M.; Yoshida, Sachiko; Pike, Steven; Buesseler, Ken O.; Rypina, Irina I.; Jayne, Steven</p> <p>2017-04-01</p> <p>Here we presents the results of a investigation which uses the tracer information provided by the 2011 direct ocean release of radio-isotopes, (137Cs, 30-year half-life and 134Cs, 2-year half-life) from the Fukushima Daiichi nuclear power plant to better understand the pathways, mixing and transport of <span class="hlt">water</span> in the North Pacific Ocean. The main focus is the analysis of cesium observations obtained from the spring 2015 CLIVAR/GO-SHIP occupation of the P16N line in the eastern North Pacific. Nearly four hundred 20 L radionuclide samples were obtained on this cruise between 29 April and 26 June 2015 covering the 152°W line from 3°N to the Alaskan Shelf off Kodiak (56.4°N), crossing the Alaska Gyre at 55°N and making a short (200 nm) line extending from the outer edge of U.S. EEZ coming into Seattle, just to the south of the Canadian border and Line-P. Samples include both profiles from the surface to 1000 m and surface/subsurface pairs that provide an average 1° latitude spacing along 152°W. A clear Fukushima signal is apparent from the surface down to 400 m. The core signal lies at between 0-200 m at about 40°N where Subtropical <span class="hlt">Mode</span> <span class="hlt">Water</span> density <span class="hlt">water</span> outcrops. The densest <span class="hlt">waters</span> with Fukushima isotopes lie at 440 m in the bottom density range of Dense-Central <span class="hlt">Mode</span> <span class="hlt">Water</span>. There is a weak, but detectable signal in the Alaska Current to the north off both Kodiak and Sitka. The deepest detectable 137Cs (weapon's testing) signals are found at and to the north of 45°N at 900-1000 m. There is detectable, background level 137Cs as far south as 3°N, but as of spring 2015 the southernmost 134C signal was found above 200 m at 30°N. This horizontal and vertical pattern of Fukushima radionuclides traces the path of <span class="hlt">mode</span> <span class="hlt">waters</span> from their formation regions in the western North Pacific to their outcrop in eastern basin over the four years since their release.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhPl...24l3515L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhPl...24l3515L"><span>Discharge <span class="hlt">mode</span> transition and temporal-spatial evolution of an air-<span class="hlt">water</span> plasma jet generated by pulsating DC power</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lei, J.; Geng, Y.; Liu, K.; Zhu, W.; Zheng, Z.; Hu, H.</p> <p>2017-12-01</p> <p>In this paper, pulsating direct current air-<span class="hlt">water</span> plasma jet, which can increase the production of •OH and decrease the temperature, is studied. The results show that the discharge <span class="hlt">mode</span> changes in one cycle from corona discharge with steep Trichel current pulse to glow-like discharge. It is unknown whether the different discharge <span class="hlt">modes</span> and <span class="hlt">water</span> ratio have an effect on the transient process of the excited O and •OH production and the mechanism of plasma propagation. So, a series of experiments are done in this paper. The results show that the changing rules of both the excited state O and the discharge current reach their two peak values synchronously. And its maximum appears at the time of the first peak current value in corona <span class="hlt">mode</span>. However, the change of the excited state •OH is different. It increases to its maximum at the time of the second peak current value in glow-like <span class="hlt">mode</span>. Besides, the intensified charge coupled device photographs show that the luminous intensity of the discharge zone at the first peak current value in corona <span class="hlt">mode</span> is stronger than the second peak current value in glow-like <span class="hlt">mode</span>. At the same time, the discharge area of the former is larger than the latter. Nevertheless, with the increase in <span class="hlt">water</span> ratio, the discharge area change reversed. Additionally, the air plasma plume propagation depends on the gas flow. The initial propagation velocity decreases with the increase in <span class="hlt">water</span> ratio.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000JQS....15..101H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000JQS....15..101H"><span>Deglacial palaeoclimate at Puerto del Hambre, <span class="hlt">subantarctic</span> Patagonia, Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Heusser, Calvin J.; Heusser, Linda E.; Lowell, Thomas V.; Moreira M., Andrés; Moreira M., Simón</p> <p>2000-02-01</p> <p>The primary objective of this study is to further substantiate multistep climatic forcing of late-glacial vegetation in southern South America. A secondary objective is to establish the age of deglaciation in Estrecho de Magallanes-Bahía Inútil. Pollen assemblages at 2-cm intervals in a core of the mire at Puerto del Hambre (53°3621S, 70°5553W) provide the basis for reconstructing the vegetation and a detailed account of palaeoclimate in <span class="hlt">subantarctic</span> Patagonia. Chronology over the 262-cm length of core is regulated by 20 AMS radiocarbon dates between 14 455 and 10 089 14C yr BP. Of 13 pollen assemblage zones, the earliest representing the Oldest Dryas chronozone (14 455-13 000 14C yr BP) records impoverished steppe with decreasing frequencies and loss of southern beech (Nothofagus). Successive 100-yr-long episodes of grass/herbs and of heath (Empetrum/Ericaceae) before 14 000 14C yr BP infer deglacial successional communities under a climate of increased continentality prior to the establishment of grass-dominated steppe. The Bølling-Allerød (13 000-11 000 14C yr BP) is characterised by mesic grassland under moderating climate that with abrupt change to heath dominance after 12 000 14C yr BP was warmer and not as humid. At the time of the Younger Dryas (11 000-10 000 14C yr BP), grass steppe expanded with a return of colder, more humid climate. Later, with gradual warming, communities were invaded by southern beech. The Puerto del Hambre record parallels multistep, deglacial palaeoclimatic sequences reported elsewhere in the Southern Andes and at Taylor Dome in Antarctica. Deglaciation of Estrecho de Magallanes-Bahía Inútil is dated close to 14 455 14C yr BP, invalidating earlier dates of between 15 800 and 16 590 14C yr BP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.9572F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.9572F"><span>Satellite Altimetry and Current-Meter Velocities in the Malvinas Current at 41°S: Comparisons and <span class="hlt">Modes</span> of Variations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferrari, Ramiro; Artana, Camila; Saraceno, Martin; Piola, Alberto R.; Provost, Christine</p> <p>2017-12-01</p> <p>Three year long current-meter arrays were deployed in the Malvinas Current at 41°S below a satellite altimeter track at about 10 years intervals. Surface geostrophic velocities (SGV) derived from satellite altimetric data are compared with the in situ velocities at the upper current meter (˜300 m). Multisatellite gridded SGV compare better with in situ observations than along-track SGV. In spite of the proximity of the moorings to the complex Brazil-Malvinas Confluence (BMC) region, satellite SGV are significantly correlated with the 20 day low-passed in situ velocities (0.85 for along-isobaths velocities, 0.8 for cross-isobaths velocities). The recent in situ measurement period (2014-2015) stands out in the altimetry record with a long-lasting (4 months) high level of eddy kinetic energy at the mooring site and a southernmost location of the <span class="hlt">Subantarctic</span> Front (SAF). The first two <span class="hlt">modes</span> of variations of sea level anomaly (SLA) over the BMC remarkably match the first two <span class="hlt">modes</span> of the low-passed in situ velocities. The first <span class="hlt">mode</span> is associated with a latitudinal migration of the SAF, and the second with a longitudinal displacement of the Brazil Current overshoot. The two <span class="hlt">modes</span> dominate the 24 year long record of SLA in the BMC, with energy peaks at the annual and semiannual periods for the first <span class="hlt">mode</span> and at 3-5 months for the second <span class="hlt">mode</span>. The SLA over the Southwest Atlantic was regressed onto the two confluence <span class="hlt">modes</span> of SLA variations and showed remarkable standing wave train like structures in the Argentine Basin.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5357866','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5357866"><span>Major advance of South Georgia glaciers during the Antarctic Cold Reversal following extensive <span class="hlt">sub-Antarctic</span> glaciation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Graham, Alastair G. C.; Kuhn, Gerhard; Meisel, Ove; Hillenbrand, Claus-Dieter; Hodgson, Dominic A.; Ehrmann, Werner; Wacker, Lukas; Wintersteller, Paul; dos Santos Ferreira, Christian; Römer, Miriam; White, Duanne; Bohrmann, Gerhard</p> <p>2017-01-01</p> <p>The history of glaciations on Southern Hemisphere sub-polar islands is unclear. Debate surrounds the extent and timing of the last glacial advance and termination on <span class="hlt">sub-Antarctic</span> South Georgia in particular. Here, using sea-floor geophysical data and marine sediment cores, we resolve the record of glaciation offshore of South Georgia through the transition from the Last Glacial Maximum to Holocene. We show a sea-bed landform imprint of a shelf-wide last glacial advance and progressive deglaciation. Renewed glacier resurgence in the fjords between c. 15,170 and 13,340 yr ago coincided with a period of cooler, wetter climate known as the Antarctic Cold Reversal, revealing a cryospheric response to an Antarctic climate pattern extending into the Atlantic sector of the Southern Ocean. We conclude that the last glaciation of South Georgia was extensive, and the sensitivity of its glaciers to climate variability during the last termination more significant than implied by previous studies. PMID:28303885</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AcO....36..299H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AcO....36..299H"><span>Contrasting nurse plants and nurse rocks: The spatial distribution of seedlings of two <span class="hlt">sub-Antarctic</span> species</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haussmann, N. S.; McGeoch, M. A.; Boelhouwers, J. C.</p> <p>2010-05-01</p> <p>Positive plant interactions, such as those associated with nurse plants, have been suggested to dominate over negative interactions in environments with high abiotic stress. Here we demonstrate that the <span class="hlt">sub-Antarctic</span> cushion plant species, Azorella selago (Apiaceae), positively affects the distribution of both its own seedlings and those of the perennial grass, Agrostis magellanica (Poaceae). As a result of the light weight and small size of seeds of both species, coupled with strong winds experienced in the study area, we consider it unlikely that these patterns are the result of very localized seed dispersal from the study cushions themselves. Instead, we suggest that both cushions and rocks act as seed traps, trapping seeds dispersed by wind, runoff and/or downslope sediment transport through frost creep. In addition, increased A. selago seedling numbers around cushions, but not around rocks, suggest that cushions provide a biological nurse effect, such as improving soil nutrient status or providing mychorrizae, to seedlings of their own kind.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC14C2085A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC14C2085A"><span>Observed Temporal and Spatial Variability in the Marine Environment at the <span class="hlt">Sub-Antarctic</span> Prince Edward Islands - Evidence of a Changing Climate?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Asdar, S.; Deshayes, J.; Ansorge, I. J.</p> <p>2016-02-01</p> <p>The <span class="hlt">sub-Antarctic</span> Prince Edward Islands (PEI) (47°S,38°E) are classified as isolated, hostile, impoverished regions, in which the terrestrial and marine ecosystems are relatively simple and extremely sensitive to perturbations. Their location between the <span class="hlt">Sub-Antarctic</span> Front (SAF) and the Antarctic Polar Front (APF), bordering the Antarctic Circumpolar Current (ACC) provides an ideal natural laboratory for studying how organisms, ecological processes and ecosystems respond to a changing ocean climate in the Southern Ocean. Recent studies have proposed that climate changes reported at the PEI may correspond in time to a southward shift of the ACC and in particular of the SAF. This southward migration in the geographic position is likely to coincide with dramatic changes in the distribution of species and total productivity of this region. This study focuses on the inter-comparison of observations available at these islands. Using spectral analysis which is a study of the frequency domain characteristics of a process, we first determine the dominant characteristics of both the temporal and spatial variability of physical and biogeochemical properties. In doing so the authors are able to determine whether and how these indices of variability interact with one another in order to understand better the mechanisms underpinning this variability, i.e. the seasonal zonal migrations associated with the SAF. Additionally, we include in our analysis recent data from 2 ADCP moorings deployed between the islands from 2014 to 2015. These in-situ observations of circulation and hydrography in the vicinity of the islands provide a unique opportunity to establish a better understanding of how large scale climatic variability may impact local conditions, and more importantly its influence on the fragile ecosystem surrounding the PEI.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16346297','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16346297"><span>Bacterioplankton in antarctic ocean <span class="hlt">waters</span> during late austral winter: abundance, frequency of dividing cells, and estimates of production.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hanson, R B; Shafer, D; Ryan, T; Pope, D H; Lowery, H K</p> <p>1983-05-01</p> <p>Bacterioplankton productivity in Antarctic <span class="hlt">waters</span> of the eastern South Pacific Ocean and Drake Passage was estimated by direct counts and frequency of dividing cells (FDC). Total bacterioplankton assemblages were enumerated by epifluorescent microscopy. The experimentally determined relationship between in situ FDC and the potential instantaneous growth rate constant (mu) is best described by the regression equation ln mu = 0.081 FDC - 3.73. In the eastern South Pacific Ocean, bacterioplankton abundance (2 x 10 to 3.5 x 10 cells per ml) and FDC (11%) were highest at the Polar Front (Antarctic Convergence). North of the <span class="hlt">Subantarctic</span> Front, abundance and FDC were between 1 x 10 to 2 x 10 cells per ml and 3 to 5%, respectively, and were vertically homogeneous to a depth of 600 m. In Drake Passage, abundance (10 x 10 cells per ml) and FDC (16%) were highest in <span class="hlt">waters</span> south of the Polar Front and near the sea ice. <span class="hlt">Subantarctic</span> <span class="hlt">waters</span> in Drake Passage contained 4 x 10 cells per ml with 4 to 5% FDC. Instantaneous growth rate constants ranged between 0.029 and 0.088 h. Using estimates of potential mu and measured standing stocks, we estimated productivity to range from 0.62 mug of C per liter . day in the eastern South Pacific Ocean to 17.1 mug of C per liter . day in the Drake Passage near the sea ice.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24367536','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24367536"><span>Gene flow and hybridization between numerically imbalanced populations of two duck species on the <span class="hlt">subantarctic</span> island of South Georgia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McCracken, Kevin G; Wilson, Robert E; Martin, Anthony R</p> <p>2013-01-01</p> <p>Hybridization is common between species of animals, particularly in waterfowl (Anatidae). One factor shown to promote hybridization is restricted mate choice, which can occur when 2 species occur in sympatry but one is rare. According to the Hubbs principle, or "desperation hypothesis," the rarer species is more likely to mate with heterospecifics. We report the second of 2 independent examples of hybridization between 2 species of ducks inhabiting island ecosystems in the <span class="hlt">Subantarctic</span> and South Atlantic Ocean. Yellow-billed pintails (Anas georgica) and speckled teal (Anas flavirostris) are abundant in continental South America, where they are sympatric and coexist in mixed flocks. But on South Georgia, an isolated island in the <span class="hlt">Subantarctic</span>, the pintail population of approximately 6000 pairs outnumbers a small breeding population of speckled teal 300∶1. Using 6 genetic loci (mtDNA and 5 nuclear introns) and Bayesian assignment tests coupled with coalescent analyses, we identified hybrid-origin speckled teal alleles in 2 pintails on South Georgia. While it is unclear whether introgression has also occurred into the speckled teal population, our data suggest that this hybridization was not a recent event, but occurred some time ago. We also failed to identify unequivocal evidence of introgression in a much larger sample of pintails and speckled teal from Argentina using a 3-population "Isolation-with-Migration" coalescent analysis. Combined with parallel findings of hybridization between these same 2 duck species in the Falkland Islands, where population ratios are reversed and pintails are outnumbered by speckled teal 1:10, our results provide further support for the desperation hypothesis, which predicts that scarcity in one population and abundance of another will often lead to hybridization. While the South Georgia pintail population appears to be thriving, it's possible that low density of conspecific mates and inverse density dependence (Allee effect) may be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21072617-water-bag-theory-autoresonant-bernstein-greene-kruskal-modes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21072617-water-bag-theory-autoresonant-bernstein-greene-kruskal-modes"><span>A <span class="hlt">water</span> bag theory of autoresonant Bernstein-Greene-Kruskal <span class="hlt">modes</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>Khain, P.; Friedland, L.</p> <p>2007-08-15</p> <p>The adiabatic <span class="hlt">water</span> bag theory describing formation and passage through phase-space of driven, continuously phase-locked (autoresonant) coherent structures in plasmas [L. Friedland et al., Phys. Rev. Lett. 96, 225001 (2006)] and of the associated Bernstein-Greene-Kruskal (BGK) <span class="hlt">modes</span> is developed. The phase-locking is achieved by using a chirped frequency ponderomotive drive, passing through kinetic Cerenkov-type resonances. The theory uses the adiabatic invariants (conserved actions of limiting trajectories) in the problem and, for a flat-top initial distribution of the electrons, reduces the calculation of the self-field of the driven BGK <span class="hlt">mode</span> to solution of a few algebraic equations. The adiabatic multiwater bagmore » extension of the theory for applications to autoresonant BGK structures with more general initial distributions is suggested. The results of the theories are in very good agreement with numerical simulations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1344098-water-dissociation-ni-ni-ni-surfaces-reaction-path-approach-mode-selectivity','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1344098-water-dissociation-ni-ni-ni-surfaces-reaction-path-approach-mode-selectivity"><span><span class="hlt">Water</span> dissociation on Ni(100), Ni(110), and Ni(111) surfaces: Reaction path approach to <span class="hlt">mode</span> selectivity</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Seenivasan, H.; Jackson, Bret; Tiwari, Ashwani K.</p> <p>2017-02-17</p> <p>We performed a comparative study of <span class="hlt">mode</span>-selectivity of <span class="hlt">water</span> dissociation on Ni(100), Ni(110), and Ni(111) surfaces at the same level of theory using a fully quantum approach based on the reaction path Hamiltonian. Calculations show that the barrier to <span class="hlt">water</span> dissociation on the Ni(110) surface is significantly lower compared to its close-packed counterparts. Transition states for this reaction on all three surfaces involve the elongation of one of the O–H bonds. Furthermore, a significant decrease in the symmetric stretching and bending <span class="hlt">mode</span> frequencies near the transition state is observed in all three cases and in the vibrational adiabatic approximation, excitationmore » of these softened <span class="hlt">modes</span> results in a significant enhancement in reactivity. Inclusion of non-adiabatic couplings between <span class="hlt">modes</span> results in the asymmetric stretching <span class="hlt">mode</span> showing a similar enhancement of reactivity as the symmetric stretching <span class="hlt">mode</span>. Dissociation probabilities calculated at a surface temperature of 300 K showed higher reactivity at lower collision energies compared to that of the static surface case, underlining the importance of lattice motion in enhancing reactivity. <span class="hlt">Mode</span> selective behavior is similar on all the surfaces. Molecules with one-quantum of vibrational excitation in the symmetric stretch, at lower energies (up to 0.45 eV), are more reactive on Ni(110) than the Ni(100) and Ni(111) surfaces. But, the dissociation probabilities approach saturation on all the surfaces at higher incident energy values. Ultimately, Ni(110) is found to be highly reactive toward <span class="hlt">water</span> dissociation among the low-index nickel surfaces owing to a low reaction barrier resulting from the openness and corrugation of the surface. These results show that the <span class="hlt">mode</span>-selective behavior does not vary with different crystal facets of Ni qualitatively, but there is a significant quantitative effect.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1344098','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1344098"><span><span class="hlt">Water</span> dissociation on Ni(100), Ni(110), and Ni(111) surfaces: Reaction path approach to <span class="hlt">mode</span> selectivity</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>Seenivasan, H.; Jackson, Bret; Tiwari, Ashwani K.</p> <p></p> <p>We performed a comparative study of <span class="hlt">mode</span>-selectivity of <span class="hlt">water</span> dissociation on Ni(100), Ni(110), and Ni(111) surfaces at the same level of theory using a fully quantum approach based on the reaction path Hamiltonian. Calculations show that the barrier to <span class="hlt">water</span> dissociation on the Ni(110) surface is significantly lower compared to its close-packed counterparts. Transition states for this reaction on all three surfaces involve the elongation of one of the O–H bonds. Furthermore, a significant decrease in the symmetric stretching and bending <span class="hlt">mode</span> frequencies near the transition state is observed in all three cases and in the vibrational adiabatic approximation, excitationmore » of these softened <span class="hlt">modes</span> results in a significant enhancement in reactivity. Inclusion of non-adiabatic couplings between <span class="hlt">modes</span> results in the asymmetric stretching <span class="hlt">mode</span> showing a similar enhancement of reactivity as the symmetric stretching <span class="hlt">mode</span>. Dissociation probabilities calculated at a surface temperature of 300 K showed higher reactivity at lower collision energies compared to that of the static surface case, underlining the importance of lattice motion in enhancing reactivity. <span class="hlt">Mode</span> selective behavior is similar on all the surfaces. Molecules with one-quantum of vibrational excitation in the symmetric stretch, at lower energies (up to 0.45 eV), are more reactive on Ni(110) than the Ni(100) and Ni(111) surfaces. But, the dissociation probabilities approach saturation on all the surfaces at higher incident energy values. Ultimately, Ni(110) is found to be highly reactive toward <span class="hlt">water</span> dissociation among the low-index nickel surfaces owing to a low reaction barrier resulting from the openness and corrugation of the surface. These results show that the <span class="hlt">mode</span>-selective behavior does not vary with different crystal facets of Ni qualitatively, but there is a significant quantitative effect.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009JMS....78..547K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JMS....78..547K"><span>Ichthyoplankton in the neritic and coastal zone of Antarctica and <span class="hlt">Subantarctic</span> islands: A review</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Koubbi, Philippe; Duhamel, Guy; Hecq, Jean-Henri; Beans, Cristina; Loots, Christophe; Pruvost, Patrice; Tavernier, Eric; Vacchi, Marino; Vallet, Carole</p> <p>2009-11-01</p> <p>Since the article published by Loeb et al. [Loeb, V.J., Kellermann, A., Koubbi, P., North, A.W., White, M., 1993. Antarctic larval fish assemblages: a review. Bull. Mar. Sci. 53(2), 416-449.] about Antarctic ichthyoplankton, many surveys were carried out in different sectors of the Southern Ocean focusing on different aspects of the ecology of fish larvae. Some of these researches were conducted in the <span class="hlt">Subantarctic</span> Kerguelen Islands and others on the continental shelf off Terre Adélie and Georges V land. Oceanographic and geographic features influence fish larvae ecology such as island mass effects, gyres, canyons. Antarctic fishes show also temporal segregation of spawning which induces temporal succession of early stage larvae. This avoids competition and probably the predation on early stages for species having few recruits. In that case, we have to understand how these larvae can deal with the match-mismatch with their preys and how they find sufficient food to survive. But our knowledge on Antarctic fish larvae is still insufficient as we do not know larvae for quite a lot of species and because of the difficulty to sample during winter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.1533B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.1533B"><span>Three-Dimensional Ageostrophic Motion and <span class="hlt">Water</span> Mass Subduction in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buongiorno Nardelli, B.; Mulet, S.; Iudicone, D.</p> <p>2018-02-01</p> <p>Vertical velocities at the ocean mesoscale are several orders of magnitude smaller than corresponding horizontal flows, making their direct monitoring a still unsolved challenge. Vertical motion is generally retrieved indirectly by applying diagnostic equations to observation-based fields. The most common approach relies on the solution of an adiabatic version of the Omega equation, neglecting the ageostrophic secondary circulation driven by frictional effects and turbulent mixing in the boundary layers. Here we apply a diabatic semigeostrophic diagnostic model to two different 3-D reconstructions covering the Southern Ocean during the period 2010-2012. We incorporate the effect of vertical mixing through a modified K-profile parameterization and using ERA-interim data, and perform an indirect validation of the ageostrophic circulation with independent drifter observations. Even if horizontal gradients and associated vertical flow are likely underestimated at 1/4° × 1/4° resolution, the exercise provides an unprecedented relative quantification of the contribution of vertical mixing and adiabatic internal dynamics on the vertical exchanges along the Antarctic Circumpolar Current. Kinematic estimates of subduction rates show the destruction of poleward flowing <span class="hlt">waters</span> lighter than 26.6 kg/m3 (14 ÷ 15 Sv) and two main positive bands associated with the Antarctic Intermediate <span class="hlt">Water</span> (7 ÷ 11 Sv) and <span class="hlt">Sub-Antarctic</span> <span class="hlt">Mode</span> <span class="hlt">Waters</span> (4 ÷ 7 Sv) formation, while Circumpolar Deep <span class="hlt">Water</span> upwelling attains around 3 ÷ 6 Sv. Diabatic and adiabatic terms force distinct spatial responses and vertical velocity magnitudes along the <span class="hlt">water</span> column and the restratifying effect of adiabatic internal dynamics due to mesoscale eddies is shown to at least partly compensate the contribution of wind-driven vertical exchanges to net subduction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23598995','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23598995"><span>Imaging surface nanobubbles at graphite-<span class="hlt">water</span> interfaces with different atomic force microscopy <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Chih-Wen; Lu, Yi-Hsien; Hwang, Ing-Shouh</p> <p>2013-05-08</p> <p>We have imaged nanobubbles on highly ordered pyrolytic graphite (HOPG) surfaces in pure <span class="hlt">water</span> with different atomic force microscopy (AFM) <span class="hlt">modes</span>, including the frequency-modulation, the tapping, and the PeakForce techniques. We have compared the performance of these <span class="hlt">modes</span> in obtaining the surface profiles of nanobubbles. The frequency-modulation <span class="hlt">mode</span> yields a larger height value than the other two <span class="hlt">modes</span> and can provide more accurate measurement of the surface profiles of nanobubbles. Imaging with PeakForce <span class="hlt">mode</span> shows that a nanobubble appears smaller and shorter with increasing peak force and disappears above a certain peak force, but the size returns to the original value when the peak force is reduced. This indicates that imaging with high peak forces does not cause gas removal from the nanobubbles. Based on the presented findings and previous AFM observations, the existing models for nanobubbles are reviewed and discussed. The model of gas aggregate inside nanobubbles provides a better explanation for the puzzles of the high stability and the contact angle of surface nanobubbles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009DSRII..56.1004S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009DSRII..56.1004S"><span><span class="hlt">Water</span> masses in the Humboldt Current System: Properties, distribution, and the nitrate deficit as a chemical <span class="hlt">water</span> mass tracer for Equatorial Subsurface <span class="hlt">Water</span> off Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Silva, Nelson; Rojas, Nora; Fedele, Aldo</p> <p>2009-07-01</p> <p>Three sections are used to analyze the physical and chemical characteristics of the <span class="hlt">water</span> masses in the eastern South Pacific and their distributions. Oceanographic data were taken from the SCORPIO (May-June 1967), PIQUERO (May-June 1969), and KRILL (June 1974) cruises. Vertical sections of temperature, salinity, σ θ, dissolved oxygen, nitrate, nitrite, phosphate, and silicate were used to analyze the <span class="hlt">water</span> column structure. Five <span class="hlt">water</span> masses were identified in the zone through T- S diagrams: <span class="hlt">Subantarctic</span> <span class="hlt">Water</span>, Subtropical <span class="hlt">Water</span>, Equatorial Subsurface <span class="hlt">Water</span>, Antarctic Intermediate <span class="hlt">Water</span>, and Pacific Deep <span class="hlt">Water</span>. Their proportions in the sea <span class="hlt">water</span> mixture are calculated using the mixing triangle method. Vertical sections were used to describe the geographical distributions of the <span class="hlt">water</span> mass cores in the upper 1500 m. Several characteristic oceanographic features in the study area were analyzed: the shallow salinity minimum displacement towards the equator, the equatorial subsurface salinity maximum associated with a dissolved oxygen minimum zone and a high nutrient content displacement towards the south, and the equatorward intermediate Antarctic salinity minimum associated with a dissolved oxygen maximum. The nitrate deficit generated in the denitrification area off Peru and northern Chile is proposed as a conservative chemical tracer for the Equatorial Subsurface <span class="hlt">Waters</span> off the coast of Chile, south of 25°S.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26769702','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26769702"><span>Multiple <span class="hlt">modes</span> of <span class="hlt">water</span> quality impairment by fecal contamination in a rapidly developing coastal area: southwest Brunswick County, North Carolina.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cahoon, Lawrence B; Hales, Jason C; Carey, Erin S; Loucaides, Socratis; Rowland, Kevin R; Toothman, Byron R</p> <p>2016-02-01</p> <p>Fecal contamination of surface <span class="hlt">waters</span> is a significant problem, particularly in rapidly developing coastal watersheds. Data from a <span class="hlt">water</span> quality monitoring program in southwest Brunswick County, North Carolina, gathered in support of a regional wastewater and stormwater management program were used to examine likely <span class="hlt">modes</span> and sources of fecal contamination. Sampling was conducted at 42 locations at 3-4-week intervals between 1996 and 2003, including streams, ponds, and estuarine <span class="hlt">waters</span> in a variety of land use settings. Expected fecal sources included human wastewater systems (on-site and central), stormwater runoff, and direct deposition by animals. Fecal coliform levels were positively associated with rainfall measures, but frequent high fecal coliform concentrations at times of no rain indicated other <span class="hlt">modes</span> of contamination as well. Fecal coliform levels were also positively associated with silicate levels, a groundwater source signal, indicating that flux of fecal-contaminated groundwater was a <span class="hlt">mode</span> of contamination, potentially elevating FC levels in impacted <span class="hlt">waters</span> independent of stormwater runoff. Fecal contamination by failing septic or sewer systems at many locations was significant and in addition to effects of stormwater runoff. Rainfall was also linked to fecal contamination by central sewage treatment system failures. These results highlight the importance of considering multiple <span class="hlt">modes</span> of <span class="hlt">water</span> pollution and different ways in which human activities cause <span class="hlt">water</span> quality degradation. Management of <span class="hlt">water</span> quality in coastal regions must therefore recognize diverse drivers of fecal contamination to surface <span class="hlt">waters</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFD.H4008D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFD.H4008D"><span><span class="hlt">Modes</span> of targets in <span class="hlt">water</span> excited and identified using radiation pressure of modulated focused ultrasound</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Daniel, Timothy; Fortuner, Auberry; Abawi, Ahmad; Kirsteins, Ivars; Marston, Philip</p> <p>2016-11-01</p> <p>The modulated radiation pressure (MRP) of ultrasound has been widely used to selectively excite low frequency <span class="hlt">modes</span> of fluid objects. We previously used MRP to excite less compliant metallic object in <span class="hlt">water</span> including the low frequency <span class="hlt">modes</span> of a circular metal plate in <span class="hlt">water</span>. A larger focused ultrasonic transducer allows us to drive <span class="hlt">modes</span> of larger more-realistic targets. In our experiments solid targets are suspended by strings or supported on sand and the modulated ultrasound is focused on the target's surface. Target sound emissions were recorded and a laser vibrometer was used to measure the surface velocity of the target to give the magnitude of the target response. The source transducer was driven with a doublesideband suppressed carrier voltage as in. By varying the modulation frequency and monitoring target response, resonant frequencies can be measured and compared to finite element models. We also demonstrate the radiation torque of a focused first-order acoustic vortex beam associated with power absorption in the Stokes layer adjacent to a sphere. Funded by ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008HMR....62..143P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008HMR....62..143P"><span>Redescription of Terebellides kerguelensis stat. nov. (Polychaeta: Trichobranchidae) from Antarctic and <span class="hlt">subantarctic</span> <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Parapar, Julio; Moreira, Juan</p> <p>2008-06-01</p> <p>During the Spanish Antarctic expeditions “Bentart” 1994, 1995 and 2003, a number of trichobranchid (Annelida: Polychaeta) specimens were collected and identified initially as Terebellides stroemii kerguelensis McIntosh, 1885, the only known species of the genus widely recognised as valid in Antarctic <span class="hlt">waters</span>. In the framework of a worldwide revision of the genus Terebellides, a reconsideration of the taxonomic status of this subspecies of the boreal Terebellides stroemii Sars, 1835 is done through the examination of the syntypes of T. s. kerguelensis compared with recent descriptions of the nominal species from Norwegian <span class="hlt">waters</span> and material from Icelandic <span class="hlt">waters</span>. Thus, T. s. kerguelensis is regarded as a valid species, T. kerguelensis stat. nov., and redescribed designating a lectotype and paralectotypes. The species is mainly characterised by the presence of an anterior branchial extension (fifth lobe), lateral lappets in five anterior thoracic chaetigers, segmental organs in chaetigers 1, 4 and 5, and first thoracic acicular neurochaetae sharply bent with pointed tips. The biological role of the segmental organs, the presence and disposition of cilia in branchial lamellae and the finding of new structures located in dorsal part of thoracic notopodia are discussed.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148v2812M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148v2812M"><span><span class="hlt">Water</span>-separated ion pairs cause the slow dielectric <span class="hlt">mode</span> of magnesium sulfate solutions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mamatkulov, Shavkat I.; Rinne, Klaus F.; Buchner, Richard; Netz, Roland R.; Bonthuis, Douwe Jan</p> <p>2018-06-01</p> <p>We compare the dielectric spectra of aqueous MgSO4 and Na2SO4 solutions calculated from classical molecular dynamics simulations with experimental data, using an optimized thermodynamically consistent sulfate force field. Both the concentration-dependent shift of the static dielectric constant and the spectral shape match the experimental results very well for Na2SO4 solutions. For MgSO4 solutions, the simulations qualitatively reproduce the experimental observation of a slow <span class="hlt">mode</span>, the origin of which we trace back to the ion-pair relaxation contribution via spectral decomposition. The radial distribution functions show that Mg2+ and SO42 - ions form extensive <span class="hlt">water</span>-separated—and thus strongly dipolar—ion pairs, the orientational relaxation of which provides a simple physical explanation for the prominent slow dielectric <span class="hlt">mode</span> in MgSO4 solutions. Remarkably, the Mg2+-SO42 - ion-pair relaxation extends all the way into the THz range, which we rationalize by the vibrational relaxation of tightly bound <span class="hlt">water</span>-separated ion pairs. Thus, the relaxation of divalent ion pairs can give rise to widely separated orientational and vibrational spectroscopic features.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19937200','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19937200"><span><span class="hlt">Water</span> filtration rate and infiltration/accumulation of low density lipoproteins in 3 different <span class="hlt">modes</span> of endothelial/smooth muscle cell co-cultures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ding, ZuFeng; Fan, YuBo; Deng, XiaoYan</p> <p>2009-11-01</p> <p>Using different endothelial/smooth muscle cell co-culture <span class="hlt">modes</span> to simulate the intimal structure of blood vessels, the <span class="hlt">water</span> filtration rate and the infiltration/accumulation of LDL of the cultured cell layers were studied. The three cell culture <span class="hlt">modes</span> of the study were: (i) The endothelial cell monolayer (EC/Phi); (ii) endothelial cells directly co-cultured on the smooth muscle cell monolayer (EC-SMC); (iii) endothelial cells and smooth muscle cells cultured on different sides of a Millicell-CM membrane (EC/SMC). It was found that under the same condition, the <span class="hlt">water</span> filtration rate was the lowest for the EC/SMC <span class="hlt">mode</span> and the highest for the EC/Phi <span class="hlt">mode</span>, while the infiltration/accumulation of DiI-LDLs was the lowest in the EC/Phi <span class="hlt">mode</span> and the highest in the EC-SMC <span class="hlt">mode</span>. It was also found that DiI-LDL infiltration/accumulation in the cultured cell layers increased with the increasing <span class="hlt">water</span> filtration rate. The results from the in vitro model study therefore suggest that the infiltration/accumulation of the lipids within the arterial wall is positively correlated with concentration polarization of atherogenic lipids, and the integrity of the endothelium plays an important role in the penetration and accumulation of atherogenic lipids in blood vessel walls.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23372011','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23372011"><span>Recent changes in the ventilation of the southern oceans.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Waugh, Darryn W; Primeau, Francois; Devries, Tim; Holzer, Mark</p> <p>2013-02-01</p> <p>Surface westerly winds in the Southern Hemisphere have intensified over the past few decades, primarily in response to the formation of the Antarctic ozone hole, and there is intense debate on the impact of this on the ocean's circulation and uptake and redistribution of atmospheric gases. We used measurements of chlorofluorocarbon-12 (CFC-12) made in the southern oceans in the early 1990s and mid- to late 2000s to examine changes in ocean ventilation. Our analysis of the CFC-12 data reveals a decrease in the age of subtropical <span class="hlt">subantarctic</span> <span class="hlt">mode</span> <span class="hlt">waters</span> and an increase in the age of circumpolar deep <span class="hlt">waters</span>, suggesting that the formation of the Antarctic ozone hole has caused large-scale coherent changes in the ventilation of the southern oceans.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP51A1057T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP51A1057T"><span>Asymmetric Signature of Glacial Antarctic Intermediate <span class="hlt">Water</span> in the Central South Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tapia, R.; Nuernberg, D.; Ho, S. L.; Lamy, F.; Ullermann, J.; Gersonde, R.; Tiedemann, R.</p> <p>2017-12-01</p> <p>Southern Ocean Intermediate <span class="hlt">Waters</span> (SOIWs) play a key role in modulating the global climate on glacial-interglacial time scales as they connect the Southern Ocean and the tropics. Despite their importance, the past evolution of the SOIWs in the central South Pacific is largely unknown due to a dearth of sedimentary archives. Here we compare Mg/Ca-temperature, stable carbon and oxygen isotope records from surface-dwelling (G. bulloides) and deep-dwelling (G. inflata) planktic foraminifera at site PS75/059-2 (54°12.9' S, 125°25.53' W; recovery 13.98 m; 3.613 m <span class="hlt">water</span> depth), located north of the modern <span class="hlt">Subantarctic</span> Front. Our study focuses on the temperature and salinity variability controlled by SOIWs, which were subducted at the <span class="hlt">Subantarctic</span> Front during the Last Glacial Maximum (LGM; 29-17ka BP) and the Penultimate Glacial Maximum (PGM; 180-150ka BP). During both glacial periods conditions at the subsurface ocean were colder and fresher relative to the Holocene (<10ka) suggesting an enhanced presence of SOIWs. In spite of the comparable subsurface cooling during both glacial, the subsurface ocean during the PGM was saltier and 0.35‰ more depleted in δ13C in comparison to the LGM. Interestingly, the mean δ13C value of the PGM is comparable to the Carbon Isotope Minimum Events, which might suggests a larger contribution of "old" low δ13C deep <span class="hlt">waters</span> to the study site during the PGM. A Latitudinal comparison of subsurface proxies suggests glacial asymmetries in the advection of SOIWs into the central Pacific, plausibly related to glacial changes in the convection depth of SOIWs at the South Antarctic Front area rather than changes in production of the SOIWs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26457564','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26457564"><span>Suppressing interfacial <span class="hlt">water</span> signals to assist the peak assignment of the N⁺-H stretching <span class="hlt">mode</span> in sum frequency generation vibrational spectroscopy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nguyen, Khoi Tan; Nguyen, Anh V</p> <p>2015-11-21</p> <p>Amines are one of the common functional groups of interest due to their abundant presence in natural proteins, surfactants and other chemicals. However, their accurate spectral assignment of vibrational <span class="hlt">modes</span>, critical to interpreting SFG signals for characterizing various bio-interfaces such as protein-membrane interaction and surfactant adsorption, still remains elusive. Herein we present a systematic study to identify and justify the correct peak assignment of the N(+)-H stretching <span class="hlt">mode</span> at the air-<span class="hlt">water</span> interface. We used three special surfactants: hexadecylamine (a primary amine without counterions), dodecylamine hydrochloride (a primary amine with counterions) and hexadecyltrimethylammonium bromide as a control (the N(+)-H stretching <span class="hlt">mode</span> is absent in this quarternary amine). We suppressed the SFG interfacial <span class="hlt">water</span> signals using saturated NaCl solutions. Our designed experiments resolved the current controversy and concluded that the 3080 cm(-1) peak is from the N(+)-H vibrations, while the 3330 cm(-1) peak is not due to ammonium species but rather originates from the interfacial <span class="hlt">water</span> vibrational <span class="hlt">modes</span> or the backbone amide <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010cosp...38..274S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010cosp...38..274S"><span>Fronts and Thermohaline Structure of the Brazil Current Confluence System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Severov, Dimitri</p> <p></p> <p>and Thermohaline Structure of the Brazil Current Confluence System (BCCS) are stud-ied from climatic data, "Marathon Exp. Leg.8, 1984"data, and two Sea surface temperature (SST) data bases: "Meteor satellite"(1989-1994) and "ds277-Reynolds" (1981-2000).The South Atlantic Central <span class="hlt">Water</span> (SACW) is divided in two main types: tropical (TW) and subtropical <span class="hlt">water</span> (ST). <span class="hlt">Water</span> masses, fronts, inter-frontal and frontal zones are analysed and classified: a) the <span class="hlt">water</span> masses: Tropical Low-Salinity <span class="hlt">Water</span>, Tropical Surface <span class="hlt">Water</span>, Tropical Tropospheric <span class="hlt">Water</span>, Subtropical Low-Salinity <span class="hlt">Water</span>, Subtropical Surface <span class="hlt">Water</span>, Subtropical Tropospheric <span class="hlt">Water</span>. T,S characteristics of intermediate, deep and bottom <span class="hlt">water</span> defined by different authors are confirmed and completed; b) the Inter-frontal Zones: Tropical/Brazil Current Zone, Sub-tropical Zone and <span class="hlt">Subantarctic</span> Zone; c) the Frontal Zones: Subtropical, <span class="hlt">Subantarctic</span> and Polar, and d) the Fronts: Subtropical Front of the Brazil Current, Principal Subtropical Front, North Subtropical Front, Subtropical Surface Front, South Subtropical Front, <span class="hlt">Subantarctic</span> Surface Front, <span class="hlt">Subantarctic</span> Front and Polar Front. Several stable T-S relationships are found below the friction layer and at the Fronts. The maximum gradient of the oceanographic characteris-tics occurs at the Brazil Current Front, which can be any of the subtropical fronts, depending on season. Minimum mean depth of the pycnocline coincides with the fronts of the BCCS, indicating the paths of low-salinity shelf <span class="hlt">waters</span> into the open ocean. D. N. Severov (a) , V. Pshennikov (b) and A.V. Remeslo (c) a -Sección Oceanologé Facultad de Ciencia, Universidad de la Republica, Igué 4225, 11400 ıa, a Montevideo, Uruguay. Tel. (598-2) 525-8618, Fax (598-2) 525-8617, mail: dima@fcien.edu.uy b -Instituto de Física, Facultad de Ciencias, Universidad de la Republica, Igué 4225, 11400 Mon-a tevideo, Uruguay, mail: seva@fisica.edu.uy c -Atlantic Research Inst. For Fisheries Oceanology (Atlant</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..121..143W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..121..143W"><span>Biogeochemical flux and phytoplankton succession: A year-long sediment trap record in the Australian sector of the <span class="hlt">Subantarctic</span> Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilks, Jessica V.; Rigual-Hernández, Andrés S.; Trull, Thomas W.; Bray, Stephen G.; Flores, José-Abel; Armand, Leanne K.</p> <p>2017-03-01</p> <p>The <span class="hlt">Subantarctic</span> Zone (SAZ) plays a crucial role in global carbon cycling as a significant sink for atmospheric CO2. In the Australian sector, the SAZ exports large quantities of organic carbon from the surface ocean, despite lower algal biomass accumulation in surface <span class="hlt">waters</span> than other Southern Ocean sectors. We present the first analysis of diatom and coccolithophore assemblages and seasonality, as well as the first annual quantification of bulk organic components of captured material at the base of the mixed layer (500 m depth) in the SAZ. Sediment traps were moored in the SAZ southwest of Tasmania as part of the long-term SAZ Project for one year (September 2003 to September 2004). Annual mass flux at 500 m and 2000 m was composed mainly of calcium carbonate, while biogenic silica made up on average <10% of material captured in the traps. Organic carbon flux was estimated at 1.1 g m-2 y-1 at 500 m, close to the estimated global mean carbon flux. Low diatom fluxes and high fluxes of coccoliths were consistent with low biogenic silica and high calcium carbonate fluxes, respectively. Diatoms and coccoliths were identified to species level. Diatom and coccolithophore sinking assemblages reflected some seasonal ecological succession. A theoretical scheme of diatom succession in live assemblages is compared to successional patterns presented in sediment traps. This study provides a unique, direct measurement of the biogeochemical fluxes and their main biological carbon vectors just below the winter mixed layer depth at which effective sequestration of carbon occurs. Comparison of these results with previous sediment trap deployments at the same site at deeper depths (i.e. 1000, 2000 and 3800 m) documents the changes particle fluxes experience in the lower "twilight zone" where biological processes and remineralisation of carbon reduce the efficiency of carbon sequestration.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP41E..08T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP41E..08T"><span>140-year <span class="hlt">subantarctic</span> tree-ring temperature reconstruction reveals tropical forcing of increased Southern Ocean climate variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Turney, C. S.; Fogwill, C. J.; Palmer, J. G.; VanSebille, E.; Thomas, Z.; McGlone, M.; Richardson, S.; Wilmshurst, J.; Fenwick, P.; Zunz, V.; Goosse, H.; Wilson, K. J.; Carter, L.; Lipson, M.; Jones, R. T.; Harsch, M.; Clark, G.; Marzinelli, E.; Rogers, T.; Rainsley, E.; Ciasto, L.; Waterman, S.; Thomas, E. R.; Visbeck, M.</p> <p>2017-12-01</p> <p>Occupying about 14 % of the world's surface, the Southern Ocean plays a fundamental role in ocean and atmosphere circulation, carbon cycling and Antarctic ice-sheet dynamics. Unfortunately, high interannual variability and a dearth of instrumental observations before the 1950s limits our understanding of how marine-atmosphere-ice domains interact on multi-decadal timescales and the impact of anthropogenic forcing. Here we integrate climate-sensitive tree growth with ocean and atmospheric observations on south-west Pacific <span class="hlt">subantarctic</span> islands that lie at the boundary of polar and subtropical climates (52-54˚S). Our annually resolved temperature reconstruction captures regional change since the 1870s and demonstrates a significant increase in variability from the 1940s, a phenomenon predating the observational record, and coincident with major changes in mammalian and bird populations. Climate reanalysis and modelling show a parallel change in tropical Pacific sea surface temperatures that generate an atmospheric Rossby wave train which propagates across a large part of the Southern Hemisphere during the austral spring and summer. Our results suggest that modern observed high interannual variability was established across the mid-twentieth century, and that the influence of contemporary equatorial Pacific temperatures may now be a permanent feature across the mid- to high latitudes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26690744','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26690744"><span>Conformational Changes of Trialanine in <span class="hlt">Water</span> Induced by Vibrational Relaxation of the Amide I <span class="hlt">Mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bastida, Adolfo; Zúñiga, José; Requena, Alberto; Miguel, Beatriz; Candela, María Emilia; Soler, Miguel Angel</p> <p>2016-01-21</p> <p>Most of the protein-based diseases are caused by anomalies in the functionality and stability of these molecules. Experimental and theoretical studies of the conformational dynamics of proteins are becoming in this respect essential to understand the origin of these anomalies. However, a description of the conformational dynamics of proteins based on mechano-energetic principles still remains elusive because of the intrinsic high flexibility of the peptide chains, the participation of weak noncovalent interactions, and the role of the ubiquitous <span class="hlt">water</span> solvent. In this work, the conformational dynamics of trialanine dissolved in <span class="hlt">water</span> (D2O) is investigated through Molecular Dynamics (MD) simulations combined with instantaneous normal <span class="hlt">modes</span> (INMs) analysis both at equilibrium and after the vibrational excitation of the C-terminal amide I <span class="hlt">mode</span>. The conformational equilibrium between α and pPII conformers is found to be altered by the intramolecular relaxation of the amide I <span class="hlt">mode</span> as a consequence of the different relaxation pathways of each conformer which modify the amount of vibrational energy stored in the torsional motions of the tripeptide, so the α → pPII and pPII → α conversion rates are increased differently. The selectivity of the process comes from the shifts of the vibrational frequencies with the conformational changes that modify the resonance conditions driving the intramolecular energy flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006JChPh.124w4708L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006JChPh.124w4708L"><span>The environmental effect on the radial breathing <span class="hlt">mode</span> of carbon nanotubes in <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Longhurst, M. J.; Quirke, N.</p> <p>2006-06-01</p> <p>We investigate, using molecular dynamics, the effect on the radial breathing <span class="hlt">mode</span> (RBM) frequency of immersion in <span class="hlt">water</span> for a range of single-walled carbon nanotubes. We find that nanotube-<span class="hlt">water</span> interactions are responsible for an upshift in the RBM frequency of the order of 4-10 wave numbers. The upshift is comprised of two components: increased hydrostatic pressure on the nanotube due to curvature effects, and the dynamic coupling of the RBM with its solvation shell. In contrast to much of the current literature, we find that the latter of the two effects is dominant. This could serve as an innovative tool for determining the interaction potential between nanotubes/graphitic surfaces and fluids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhL.110z4102L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhL.110z4102L"><span>Controlled cytotoxicity of plasma treated <span class="hlt">water</span> formulated by open-air hybrid <span class="hlt">mode</span> discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, P.; Boehm, D.; Cullen, P.; Bourke, P.</p> <p>2017-06-01</p> <p>Plasma treated liquids (PTLs) provide a means to convey a broad range of effects of relevance for food, environmental, or clinical decontamination, plant growth promotion, and therapeutic applications. Devising the reactive species ingredients and controlling the biological response of PTLs are of great interest. We demonstrate an approach by using an open-air hybrid <span class="hlt">mode</span> discharge (HMD) to control the principal reactive species composition within plasma treated <span class="hlt">water</span> (PTW), which is then demonstrated to regulate the cytotoxicity of PTW. The cytotoxicity of HMD produced PTW demonstrates a non-monotonic change over the discharge time. Although hydrogen peroxide and nitrite are not the sole effectors for cell death caused by PTW, using them as principal reactive species indicators, cytotoxicity can be removed and/or enhanced by formulating their concentrations and composition through adjusting the discharge <span class="hlt">mode</span> and time on-line during PTW generation without the addition of additional working gas or chemical scavengers. This work demonstrates that a hybrid <span class="hlt">mode</span> discharge can be employed to generate a PTW formulation to control a biological response such as cytotoxicity. This provides insights into how plasma treated liquids may be harnessed for biological applications in a specific and controllable manner.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003ASAJ..113.2334O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003ASAJ..113.2334O"><span>Tilt angle dependence of backscattering enhancements from organ pipe <span class="hlt">modes</span> of open <span class="hlt">water</span>-filled cylinders: Measurements and models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Osterhoudt, Curtis F.; Marston, Philip L.</p> <p>2003-04-01</p> <p>A simple target for simulating narrow low-frequency resonances of cylinders is an open metal pipe completely filled with <span class="hlt">water</span>. We have previously described how the high-Q organ-pipe <span class="hlt">modes</span> having a pressure node near each end are easily observed in backscattering experiments with small cylinders [C. F. Osterhoudt and P. L. Marston, J. Acoust. Soc. Am. 110, 2773 (2001)]. The resonance occurs because of the strong reflection of internal acoustic waves from the open ends of the pipe [H. Levine and J. Schwinger, Phys. Rev. 73, 383-406 (1948)]. In the present research, the dependence of the backscattering amplitude on the orientation of the cylinder is measured and modeled. The tilt angle dependence is affected by the symmetry of the organ pipe <span class="hlt">mode</span>. An approximation was also developed for the backscattering amplitude at high Q resonances based on energy conservation, reciprocity, and the optical theorem. While this analysis applies to cylinders suspended in <span class="hlt">water</span> away from boundaries, the organ-pipe <span class="hlt">modes</span> studied may be useful for investigating scattering processes for buried or partially buried cylinders. [Research supported in part by ONR.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRC..123.2238P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRC..123.2238P"><span>Seasonal Variation of Barrier Layer in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pan, Li; Zhong, Yisen; Liu, Hailong; Zhou, Lei; Zhang, Zhaoru; Zhou, Meng</p> <p>2018-03-01</p> <p>The seasonal variability of barrier layer (BL) and its formation mechanism in the Southern Ocean are investigated using the most recent Argo data. The results reveal that the BL is a persistent feature in the Southern Ocean with a strong seasonal cycle. The thickest BL appears in winter with the maximum amplitude exceeding 250 m while it dramatically decreases to less than 50 m in summer. The spatial distribution of BL is zonally oriented in the Pacific and Indian Ocean sectors, which is in agreement with that of the mixed layer depth (MLD) and the isothermal layer depth (ILD). Two areas with the most prominent BL are identified. One is located south of Australia and the other in the southeastern Pacific. The BL formation in both areas is generally attributed to a shallow mixed layer controlled by surface freshwater intrusion and a deep isothermal layer modulated by seasonal vertical convection. In the former region, the cold and fresh Antarctic Surface <span class="hlt">Water</span> (ASW) is transported northward across the <span class="hlt">Subantarctic</span> Front (SAF) by the Ekman effect and overlies the warm <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> (SAMW). The resulting inverse temperature structure facilitates the development of thick BLs. In the latter region, the BL emerges in the ventilation area where the shallow Surface Salinity Minimum <span class="hlt">Water</span> (SSMW) coming from north leans against the deep vertical isotherms. In summer, positive surface heat flux into the ocean overwhelms other thermodynamic effects in the mixed layer heat budget. The MLD and ILD coincide and thus the BL is destroyed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21361418','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21361418"><span>Suppression of an acoustic <span class="hlt">mode</span> by an elastic <span class="hlt">mode</span> of a liquid-filled spherical shell resonator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lonzaga, Joel B; Raymond, Jason L; Mobley, Joel; Gaitan, D Felipe</p> <p>2011-02-01</p> <p>The purpose of this paper is to report on the suppression of an approximately radial (radially symmetric) acoustic <span class="hlt">mode</span> by an elastic <span class="hlt">mode</span> of a <span class="hlt">water</span>-filled, spherical shell resonator. The resonator, which has a 1-in. wall thickness and a 9.5-in. outer diameter, was externally driven by a small transducer bolted to the external wall. Experiments showed that for the range of drive frequencies (19.7-20.6 kHz) and sound speeds in <span class="hlt">water</span> (1520-1570 m/s) considered in this paper, a nonradial (radially nonsymmetric) <span class="hlt">mode</span> was also excited, in addition to the radial <span class="hlt">mode</span>. Furthermore, as the sound speed in the liquid was changed, the resonance frequency of the nonradial <span class="hlt">mode</span> crossed with that of the radial one and the amplitude of the latter was greatly reduced near the crossing point. The crossing of the eigenfrequency curves of these two <span class="hlt">modes</span> was also predicted theoretically. Further calculations demonstrated that while the radial <span class="hlt">mode</span> is an acoustic one associated with the interior fluid, the nonradial <span class="hlt">mode</span> is an elastic one associated with the shell. Thus, the suppression of the radial acoustic <span class="hlt">mode</span> is apparently caused by the overlapping with the nonradial elastic <span class="hlt">mode</span> near the crossing point.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4795697','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4795697"><span>Metagenomic Survey of Viral Diversity Obtained from Feces of <span class="hlt">Subantarctic</span> and South American Fur Seals</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Kluge, Mariana; Campos, Fabrício Souza; Tavares, Maurício; de Amorim, Derek Blaese; Valdez, Fernanda Pedone; Giongo, Adriana; Roehe, Paulo Michel; Franco, Ana Claudia</p> <p>2016-01-01</p> <p>The Brazilian South coast seasonally hosts numerous marine species, observed particularly during winter months. Some animals, including fur seals, are found dead or debilitated along the shore and may harbor potential pathogens within their microbiota. In the present study, a metagenomic approach was performed to evaluate the viral diversity in feces of fur seals found deceased along the coast of the state of Rio Grande do Sul. The fecal virome of two fur seal species was characterized: the South American fur seal (Arctocephalus australis) and the <span class="hlt">Subantarctic</span> fur seal (Arctocephalus tropicalis). Fecal samples from 10 specimens (A. australis, n = 5; A. tropicalis, n = 5) were collected and viral particles were purified, extracted and amplified with a random PCR. The products were sequenced through Ion Torrent and Illumina platforms and assembled reads were submitted to BLASTx searches. Both viromes were dominated by bacteriophages and included a number of potentially novel virus genomes. Sequences of picobirnaviruses, picornaviruses and a hepevirus-like were identified in A. australis. A rotavirus related to group C, a novel member of the Sakobuvirus and a sapovirus very similar to California sea lion sapovirus 1 were found in A. tropicalis. Additionally, sequences of members of the Anelloviridae and Parvoviridae families were detected in both fur seal species. This is the first metagenomic study to screen the fecal virome of fur seals, contributing to a better understanding of the complexity of the viral community present in the intestinal microbiota of these animals. PMID:26986573</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27211206','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27211206"><span>Seroprevalence of Toxoplasma gondii in mainland and <span class="hlt">sub-Antarctic</span> New Zealand sea lion (Phocarctos hookeri) populations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Michael, S A; Howe, L; Chilvers, B L; Morel, Pch; Roe, W D</p> <p>2016-09-01</p> <p>To investigate the seroprevalence of antibodies to Toxoplasma gondii in New Zealand sea lions (Phocarctos hookeri), as a potential contributor to reproductive failure. Archived sera were sourced from New Zealand sea lions from two recolonising mainland populations in the Otago Peninsula (n=15) and Stewart Island (n=12), as well as a declining population at Enderby Island (n=28) in the New Zealand <span class="hlt">sub-Antarctic</span>. Sera were tested for antibodies to T. gondii using a commercially available ELISA (with samples considered positive if the sample to positive ratio was >30%), and latex agglutination test (LAT; with titres ≥1:32 considered positive). Western blot analysis was used to validate the results of a subset of 14 samples. Five samples from sea lions in mainland locations were confirmed positive for antibodies to T. gondii. Two adult females exhibited high LAT antibody titres (min 1:2048, max 1:4096) on both occasions when sampled 1 and 2 years apart, respectively. No animals from Enderby Island were seropositive. Toxoplasma gondii infection is unlikely to be a major contributor to poor reproductive success in New Zealand sea lions. However, continued surveillance is pertinent to assess subclinical and clinical impacts of the parasite on these threatened populations. The commercial tests evaluated here, with further species-specific threshold refinement could provide a fast, inexpensive and reliable indicator of T. gondii exposure in New Zealand sea lions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ExFl...59...95V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ExFl...59...95V"><span>Experimental investigation of the sloshing motion of the <span class="hlt">water</span> free surface in the draft tube of a Francis turbine operating in synchronous condenser <span class="hlt">mode</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vagnoni, Elena; Favrel, Arthur; Andolfatto, Loïc; Avellan, François</p> <p>2018-06-01</p> <p>Hydropower units may be required to operate in condenser <span class="hlt">mode</span> to supply reactive power. In this operating <span class="hlt">mode</span>, the <span class="hlt">water</span> level in the turbine or pump-turbine is decreased below the runner by closing the guide vanes and injecting pressurized air. While operating in condenser <span class="hlt">mode</span> the machine experiences power losses due to several air-<span class="hlt">water</span> interaction phenomena which cause air losses. One of such phenomena is the sloshing motion of the <span class="hlt">water</span> free surface below the runner in the draft tube cone of a Francis turbine. The objective of the present work is to experimentally investigate the sloshing motion of the <span class="hlt">water</span> free surface in the draft tube cone of a reduced scale physical model of a Francis turbine operating in condenser <span class="hlt">mode</span>. Images acquisition and simultaneous pressure fluctuation measurements are performed and an image processing method is developed to investigate amplitude and frequency of the sloshing motion of the free surface. It is found that this motion is excited at the natural frequency of the <span class="hlt">water</span> volume and corresponds to the azimuthal wavenumber m = 1 of a rotating gravity wave. The amplitude of the motion is perturbed by wave breaking and it decreases by increasing the densimetric Froude number. The sloshing frequency slightly increases with respect to the natural frequency of the <span class="hlt">water</span> volume by increasing the densimetric Froude number. Moreover, it results that this resonant phenomenon is not related to the torque perturbation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1215562','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1215562"><span>Predicting the occurrence of mixed <span class="hlt">mode</span> failure associated with hydraulic fracturing, part 2 <span class="hlt">water</span> saturated tests</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>Bauer, Stephen J.; Broome, Scott Thomas; Choens, Charles</p> <p>2015-09-14</p> <p>Seven <span class="hlt">water</span>-saturated triaxial extension experiments were conducted on four sedimentary rocks. This experimental condition was hypothesized more representative of that existing for downhole hydrofracture and thus it may improve our understanding of the phenomena. In all tests the pore pressure was 10 MPa and confirming pressure was adjusted to achieve tensile and transitional failure <span class="hlt">mode</span> conditions. Using previous work in this LDRD for comparison, the law of effective stress is demonstrated in extension using this sample geometry. In three of the four lithologies, no apparent chemo-mechanical effect of <span class="hlt">water</span> is apparent, and in the fourth lithology test results indicate somemore » chemo-mechanical effect of <span class="hlt">water</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17..166S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17..166S"><span>Seabird guano enhances phytoplankton production in the Southern Ocean.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shatova, Olga; Wing, Stephen; Hoffmann, Linn; Jack, Lucy; Gault-Ringold, Melanie</p> <p>2015-04-01</p> <p>Great congregations of seabirds in <span class="hlt">sub-Antarctic</span> and Antarctic coastal areas result in delivery of nutrient-rich guano to marine ecosystems that potentially enhances productivity and supports biodiversity in the region. Guano-derived bio-available micronutrients and macronutrients might be utilized by marine phytoplankton for photosynthetic production, however, mechanisms and significance of guano fertilization in the Southern Ocean are largely understudied. Over austral summers of 2012 and 2013 we performed a series of guano-enrichment phytoplankton incubation experiments with <span class="hlt">water</span> samples collected from three different <span class="hlt">water</span> masses in the Southern Ocean: Antarctic <span class="hlt">waters</span> of the Ross sea and <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span> offshore the Otago Peninsula, both showing iron limitation of phytoplankton productivity in summer, and in the subtropical frontal zone offshore from the Snares Islands, which is generally micronutrient-repleted. Samples were enriched with known concentrations of guano-derived nutrients. Phytoplankton biomass increased significantly in guano-treated samples during all three incubation experiments (7-10 fold increase), while remained low in control samples. This response indicates that seabird guano provides nutrients that limit primary production in the Southern Ocean and that these nutrients are readily taken up by phytoplankton. Guano additions were compared to Fe and Macronutrient treatments (both added in quantities similar to those in the guano treatment). Phytoplankton biomass increased significantly in response to the Macronutrient treatment in the subtropical frontal zone, however, the response had a smaller magnitude compared to the guano treatment (2.8 µgL-1 vs 5.2 µgL-1) ; there was no significant effect of Fe on phytoplankton growth. This suggests the potential importance of synergistic effects of nutrients in guano. Incubation with <span class="hlt">sub-Antarctic</span> <span class="hlt">waters</span> showed that Fe and Macronutrients might be equally important for enhancement of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994HM.....48...79M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994HM.....48...79M"><span>Leucon parasiphonatus, a new species (Crustacea: Cumacea: Leuconidae) from Antarctic <span class="hlt">waters</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mühlenhardt-Siegel, U.</p> <p>1994-03-01</p> <p>Six specimens of Leucon parasiphonatus n. sp. were collected at depths ranging from 15 to 424 m in the vicinity of King George Island (South Shetland Islands, Antarctica) and the south eastern Weddell Sea. Leucon parasiphonatus belongs to the subgenus Leucon and differs from the other already known antarctic and <span class="hlt">Subantarctic</span> species of the genus, in the absence of a serrated dorsomedian line and in the presence of a long pseudorostrum with several fine setae at its tip, surrounding the very long branchial siphon. The surface of the carapace is granulated; the carapace displays no teeth except for a few at its antero-lateral margin and at its ventral margin. The species most similar to Leucon parasiphonatus is Leucon siphonatus, reported from Mediterranean and North Atlantic <span class="hlt">waters</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_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/1991CP....158..447K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1991CP....158..447K"><span>The effects of solvent on the conformation and the collective motions of protein: Normal <span class="hlt">mode</span> analysis and molecular dynamics simulations of melittin in <span class="hlt">water</span> and in vacuum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kitao, Akio; Hirata, Fumio; Gō, Nobuhiro</p> <p>1991-12-01</p> <p>The effects of solvent on the conformation and dynamics of protein is studied by computer simulation. The dynamics is studied by focusing mainly on collective motions of the protein molecule. Three types of simulation, normal <span class="hlt">mode</span> analysis, molecular dynamics in vacuum, and molecular dynamics in <span class="hlt">water</span> are applied to melittin, the major component of bee venom. To define collective motions principal, component analysis as well as normal <span class="hlt">mode</span> analysis has been carried out. The principal components with large fluctuation amplitudes have a very good correspondence with the low-frequency normal <span class="hlt">modes</span>. Trajectories of the molecular dynamics simulation are projected onto the principal axes. From the projected motions time correlation functions are calculated. The results indicate that the very-low-frequency <span class="hlt">modes</span>, whose frequencies are less than ≈ 50 cm -1, are overdamping in <span class="hlt">water</span> with relaxation times roushly twice as long as the period of the oscillatory motion. Effective Langevin <span class="hlt">mode</span> analysis is carried out by using the friction coefficient matrix determined from the velocity correlation function calculated from the molecular dynamics trajectory in <span class="hlt">water</span>. This analysis reproduces the results of the simulation in <span class="hlt">water</span> reasonably well. The presence of the solvent <span class="hlt">water</span> is found also to affect the shape of the potential energy surface in such a way that it produces many local minima with low-energy barriers in between, the envelope of which is given by the surface in vacuum. Inter-minimum transitions endow the conformational dynamics of proteins in <span class="hlt">water</span> another diffusive character, which already exists in the intra-minimum collective motions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H44G..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H44G..01H"><span>The different <span class="hlt">modes</span> of hydro-economic analysis (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harou, J. J.; Binions, O.; Erfani, T.</p> <p>2013-12-01</p> <p>In the face of growing <span class="hlt">water</span> demands, climate change and spatial and temporal <span class="hlt">water</span> access variability, accurately assessing the economic impacts of proposed <span class="hlt">water</span> resource management changes is useful. The objective of this project funded by UK <span class="hlt">Water</span> Industry Research was to present and demonstrate a framework for identifying and using the ';value of <span class="hlt">water</span>' to enable <span class="hlt">water</span> utilities and their regulators to make better decisions. A hydro-economic model can help evaluate <span class="hlt">water</span> management options in terms of their hydrological and economic impact at different locations throughout a catchment over time. In this talk we discuss three <span class="hlt">modes</span> in which hydro-economic models can be implemented: evaluative, behavioral and prescriptive. In evaluation <span class="hlt">mode</span> economic <span class="hlt">water</span> demand and benefit functions are used to post-process <span class="hlt">water</span> resource management model results to assess the economic impacts (over space and time) of a policy under consideration. In behavioral hydro-economic models users are represented as agents and the economics is used to help predict their actions. In prescriptive <span class="hlt">mode</span> optimization is used to find the most economically efficient management actions such as allocation patterns or source selection. These three types of hydro-economic analysis are demonstrated on a UK watershed (Great River Ouse) that includes 97 different <span class="hlt">water</span> abstractors from amongst the public <span class="hlt">water</span> supply, agriculture, industry and energy plant cooling sectors. The following issues under dry and normal historical conditions were investigated: Supply/demand investment planning, societal cost of environmental flows, <span class="hlt">water</span> market prices, and scarcity-sensitive charges for <span class="hlt">water</span> rights. The talk discusses which hydro-economic modeling <span class="hlt">mode</span> is used to study each of these issues and why; example results are shown and discussed. The topic of how hydro-economic models can be built and deployed effectively is covered along with how existing <span class="hlt">water</span> utility operational and planning tools can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE10150E..0OM','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE10150E..0OM"><span>Alcohol sensor based on single-<span class="hlt">mode-multimode-single-mode</span> fiber structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mefina Yulias, R.; Hatta, A. M.; Sekartedjo, Sekartedjo</p> <p>2016-11-01</p> <p>Alcohol sensor based on Single-<span class="hlt">mode</span> -Multimode-Single-<span class="hlt">mode</span> (SMS) fiber structure is being proposed to sense alcohol concentration in alcohol-<span class="hlt">water</span> mixtures. This proposed sensor uses refractive index sensing as its sensing principle. Fabricated SMS fiber structure had 40 m of multimode length. With power input -6 dBm and wavelength 1550 nm, the proposed sensor showed good response with sensitivity 1,983 dB per % v/v with measurement range 05 % v/v and measurement span 0,5% v/v.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27375948','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27375948"><span>Dynamic absorption and scattering of <span class="hlt">water</span> and hydrogel during high-repetition-rate (>100 MHz) burst-<span class="hlt">mode</span> ultrafast-pulse laser ablation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Qian, Zuoming; Covarrubias, Andrés; Grindal, Alexander W; Akens, Margarete K; Lilge, Lothar; Marjoribanks, Robin S</p> <p>2016-06-01</p> <p>High-repetition-rate burst-<span class="hlt">mode</span> ultrafast-laser ablation and disruption of biological tissues depends on interaction of each pulse with the sample, but under those particular conditions which persist from previous pulses. This work characterizes and compares the dynamics of absorption and scattering of a 133-MHz repetition-rate, burst-<span class="hlt">mode</span> ultrafast-pulse laser, in agar hydrogel targets and distilled <span class="hlt">water</span>. The differences in energy partition are quantified, pulse-by-pulse, using a time-resolving integrating-sphere-based device. These measurements reveal that high-repetition-rate burst-<span class="hlt">mode</span> ultrafast-laser ablation is a highly dynamical process affected by the persistence of ionization, dissipation of plasma plume, neutral material flow, tissue tensile strength, and the hydrodynamic oscillation of cavitation bubbles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1337232-diverse-bacterial-groups-contribute-alkane-degradation-potential-chronically-polluted-subantarctic-coastal-sediments','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1337232-diverse-bacterial-groups-contribute-alkane-degradation-potential-chronically-polluted-subantarctic-coastal-sediments"><span>Diverse Bacterial Groups Contribute to the Alkane Degradation Potential of Chronically Polluted <span class="hlt">Subantarctic</span> Coastal Sediments</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>Guibert, Lilian M.; Loviso, Claudia L.; Borglin, Sharon</p> <p></p> <p>We aimed to gain insight into the alkane degradation potential of microbial communities from chronically polluted sediments of a <span class="hlt">subantarctic</span> coastal environment using a combination of metagenomic approaches. A total of 6178 sequences annotated as alkane-1-monooxygenases (EC 1.14.15.3) were retrieved from a shotgun metagenomic dataset that included two sites analyzed in triplicate. The majority of the sequences binned with AlkB described in Bacteroidetes (32 ± 13 %) or Proteobacteria (29 ± 7 %), although a large proportion remained unclassified at the phylum level. Operational taxonomic unit (OTU)-based analyses showed small differences in AlkB distribution among samples that could be correlatedmore » with alkane concentrations, as well as with site-specific variations in pH and salinity. A number of low-abundance OTUs, mostly affiliated with Actinobacterial sequences, were found to be only present in the most contaminated samples. On the other hand, the molecular screening of a large-insert metagenomic library of intertidal sediments from one of the sampling sites identified two genomic fragments containing novel alkB gene sequences, as well as various contiguous genes related to lipid metabolism. Both genomic fragments were affiliated with the phylum Planctomycetes, and one could be further assigned to the genus Rhodopirellula due to the presence of a partial sequence of the 23S ribosomal RNA (rRNA) gene. This work highlights the diversity of bacterial groups contributing to the alkane degradation potential and reveals patterns of functional diversity in relation with environmental stressors in a chronically polluted, high-latitude coastal environment. In addition, alkane biodegradation genes are described for the first time in members of Planctomycetes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27634266','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27634266"><span>Isotope effects in liquid <span class="hlt">water</span> probed by transmission <span class="hlt">mode</span> x-ray absorption spectroscopy at the oxygen K-edge.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Schreck, Simon; Wernet, Philippe</p> <p>2016-09-14</p> <p>The effects of isotope substitution in liquid <span class="hlt">water</span> are probed by x-ray absorption spectroscopy at the O K-edge as measured in transmission <span class="hlt">mode</span>. Confirming earlier x-ray Raman scattering experiments, the D2O spectrum is found to be blue shifted with respect to H2O, and the D2O spectrum to be less broadened. Following the earlier interpretations of UV and x-ray Raman spectra, the shift is related to the difference in ground-state zero-point energies between D2O and H2O, while the difference in broadening is related to the difference in ground-state vibrational zero-point distributions. We demonstrate that the transmission-<span class="hlt">mode</span> measurements allow for determining the spectral shapes with unprecedented accuracy. Owing in addition to the increased spectral resolution and signal to noise ratio compared to the earlier measurements, the new data enable the stringent determination of blue shift and broadening in the O K-edge x-ray absorption spectrum of liquid <span class="hlt">water</span> upon isotope substitution. The results are compared to UV absorption data, and it is discussed to which extent they reflect the differences in zero-point energies and vibrational zero-point distributions in the ground-states of the liquids. The influence of the shape of the final-state potential, inclusion of the Franck-Condon structure, and differences between liquid H2O and D2O resulting from different hydrogen-bond environments in the liquids are addressed. The differences between the O K-edge absorption spectra of <span class="hlt">water</span> from our transmission-<span class="hlt">mode</span> measurements and from the state-of-the-art x-ray Raman scattering experiments are discussed in addition. The experimentally extracted values of blue shift and broadening are proposed to serve as a test for calculations of ground-state zero-point energies and vibrational zero-point distributions in liquid H2O and D2O. This clearly motivates the need for new calculations of the O K-edge x-ray absorption spectrum of liquid <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.7163F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.7163F"><span>Variability of the subtropical <span class="hlt">mode</span> <span class="hlt">water</span> in the Southwest Pacific</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fernandez, Denise; Sutton, Philip; Bowen, Melissa</p> <p>2017-09-01</p> <p>The variability of Subtropical <span class="hlt">Mode</span> <span class="hlt">Water</span> (STMW) in the Southwest Pacific is investigated using a 28 year-long time series (1986-2014) of high-resolution expendable bathythermograph data north of New Zealand (PX06) and a shorter time series, the Roemmich-Gilson monthly Argo optimal interpolation for the 2004-2014 period. The variability in STMW inventories is compared to the variability in air-sea heat fluxes, mixed layer depths and transport of the East Auckland Current (EAUC) to assess both the atmospheric and oceanic roles influencing the formation and decay of STMW. The STMW north of New Zealand has a short lifespan with little persistence of the <span class="hlt">water</span> mass from 1 year to the next one. Deeper mixed layers and negative anomalies in surface heat fluxes are correlated with increased formation of STMW. The heat content of the STMW layer is anticorrelated with inventories, particularly during the El Niño years. This suggests that large volumes of STMW are coincident with cooler conditions in the prior winter and less oceanic heat storage. There is significant seasonal and interannual variability in STMW inventories, however there are no trends in STMW properties, including its core layer temperature over the last decade. The variability of the winter EAUC transport is highly correlated with the STMW inventories and thermocline depth in the following spring, suggesting ocean dynamics deepen the thermocline and precondition for deeper mixed layers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BGeo...15...31T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BGeo...15...31T"><span>Distribution of planktonic biogenic carbonate organisms in the Southern Ocean south of Australia: a baseline for ocean acidification impact assessment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trull, Thomas W.; Passmore, Abraham; Davies, Diana M.; Smit, Tim; Berry, Kate; Tilbrook, Bronte</p> <p>2018-01-01</p> <p>The Southern Ocean provides a vital service by absorbing about one-sixth of humankind's annual emissions of CO2. This comes with a cost - an increase in ocean acidity that is expected to have negative impacts on ocean ecosystems. The reduced ability of phytoplankton and zooplankton to precipitate carbonate shells is a clearly identified risk. The impact depends on the significance of these organisms in Southern Ocean ecosystems, but there is very little information on their abundance or distribution. To quantify their presence, we used coulometric measurement of particulate inorganic carbonate (PIC) on particles filtered from surface seawater into two size fractions: 50-1000 µm to capture foraminifera (the most important biogenic carbonate-forming zooplankton) and 1-50 µm to capture coccolithophores (the most important biogenic carbonate-forming phytoplankton). Ancillary measurements of biogenic silica (BSi) and particulate organic carbon (POC) provided context, as estimates of the biomass of diatoms (the highest biomass phytoplankton in polar <span class="hlt">waters</span>) and total microbial biomass, respectively. Results for nine transects from Australia to Antarctica in 2008-2015 showed low levels of PIC compared to Northern Hemisphere polar <span class="hlt">waters</span>. Coccolithophores slightly exceeded the biomass of diatoms in <span class="hlt">subantarctic</span> <span class="hlt">waters</span>, but their abundance decreased more than 30-fold poleward, while diatom abundances increased, so that on a molar basis PIC was only 1 % of BSi in Antarctic <span class="hlt">waters</span>. This limited importance of coccolithophores in the Southern Ocean is further emphasized in terms of their associated POC, representing less than 1 % of total POC in Antarctic <span class="hlt">waters</span> and less than 10 % in <span class="hlt">subantarctic</span> <span class="hlt">waters</span>. NASA satellite ocean-colour-based PIC estimates were in reasonable agreement with the shipboard results in <span class="hlt">subantarctic</span> <span class="hlt">waters</span> but greatly overestimated PIC in Antarctic <span class="hlt">waters</span>. Contrastingly, the NASA Ocean Biogeochemical Model (NOBM) shows coccolithophores as overly</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRD..122.2008Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRD..122.2008Y"><span>Generation of real-time <span class="hlt">mode</span> high-resolution <span class="hlt">water</span> vapor fields from GPS observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Chen; Penna, Nigel T.; Li, Zhenhong</p> <p>2017-02-01</p> <p>Pointwise GPS measurements of tropospheric zenith total delay can be interpolated to provide high-resolution <span class="hlt">water</span> vapor maps which may be used for correcting synthetic aperture radar images, for numeral weather prediction, and for correcting Network Real-time Kinematic GPS observations. Several previous studies have addressed the importance of the elevation dependency of <span class="hlt">water</span> vapor, but it is often a challenge to separate elevation-dependent tropospheric delays from turbulent components. In this paper, we present an iterative tropospheric decomposition interpolation model that decouples the elevation and turbulent tropospheric delay components. For a 150 km × 150 km California study region, we estimate real-time <span class="hlt">mode</span> zenith total delays at 41 GPS stations over 1 year by using the precise point positioning technique and demonstrate that the decoupled interpolation model generates improved high-resolution tropospheric delay maps compared with previous tropospheric turbulence- and elevation-dependent models. Cross validation of the GPS zenith total delays yields an RMS error of 4.6 mm with the decoupled interpolation model, compared with 8.4 mm with the previous model. On converting the GPS zenith wet delays to precipitable <span class="hlt">water</span> vapor and interpolating to 1 km grid cells across the region, validations with the Moderate Resolution Imaging Spectroradiometer near-IR <span class="hlt">water</span> vapor product show 1.7 mm RMS differences by using the decoupled model, compared with 2.0 mm for the previous interpolation model. Such results are obtained without differencing the tropospheric delays or <span class="hlt">water</span> vapor estimates in time or space, while the errors are similar over flat and mountainous terrains, as well as for both inland and coastal areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29315935','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29315935"><span><span class="hlt">Water</span>-Tryptophan Interactions: Lone-pair⋅⋅⋅π or O-H⋅⋅⋅π? Molecular Dynamics Simulations of β-Galactosidase Suggest that Both <span class="hlt">Modes</span> Can Co-exist.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Durec, Matúš; Marek, Radek; Kozelka, Jiří</p> <p>2018-04-17</p> <p>In proteins, the indole side chain of tryptophan can interact with <span class="hlt">water</span> molecules either in-plane, forming hydrogen bonds, or out-of-plane, with the <span class="hlt">water</span> molecule contacting the aromatic π face. The latter interaction can be either of the lone pair⋅⋅⋅π (lp⋅⋅⋅π) type or corresponds to the O-H⋅⋅⋅π binding <span class="hlt">mode</span>, an ambiguity that X-ray structures usually do not resolve. Here, we report molecular dynamics (MD) simulations of a solvated β-galactosidase monomer, which illustrate how a <span class="hlt">water</span> molecule located at the π face of an indole side chain of tryptophan can adapt to the position of proximate residues and "select" its binding <span class="hlt">mode</span>. In one such site, the <span class="hlt">water</span> molecule is predicted to rapidly oscillate between the O-H⋅⋅⋅π and lp⋅⋅⋅π binding <span class="hlt">modes</span>, thus gaining entropic advantage. Our MD simulations provide support for the role of lp⋅⋅⋅π interactions in the stabilization of protein structures. © 2018 Wiley-VCH Verlag GmbH & Co. KGaA, Weinheim.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918288S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918288S"><span>A propagating freshwater <span class="hlt">mode</span> in the Arctic Ocean with multidecadal time scale</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmith, Torben; Malskær Olsen, Steffen; Margrethe Ringgaard, Ida</p> <p>2017-04-01</p> <p>We apply Principal Oscillatory Pattern analysis to the Arctic Ocean fresh <span class="hlt">water</span> content as simulated in a 500 year long control run with constant preindustrial forcing with the EC-Earth global climate model. Two <span class="hlt">modes</span> emerge from this analysis. One <span class="hlt">mode</span> is a standing <span class="hlt">mode</span> with decadal time scale describing accumulation and release of fresh <span class="hlt">water</span> in the Beaufort Gyre, known in the literature as the Beaufort Gyre flywheel. In addition, we identify a propagating <span class="hlt">mode</span> with a time scale around 80 years, propagating along the rim of the Canadian Basin. This <span class="hlt">mode</span> has maximum variability of the fresh <span class="hlt">water</span> content in the Transpolar Drift and represents the bulk of the total variability of the fresh <span class="hlt">water</span> content in the Arctic Ocean and also projects on the fresh <span class="hlt">water</span> through the Fram Strait. Therefore, potentially, it can introduce a multidecadal variability to the Atlantic meridional overturning circulation. We will discuss the physical origin of this propagating <span class="hlt">mode</span>. This include planetary-scale internal Rossby waves with multidecadal time scale, due to the slow variation of the Coriolis parameter at these high latitudes, as well as topographic steering of these Rossby waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24376821','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24376821"><span>Soil calcium availability influences shell ecophenotype formation in the <span class="hlt">sub-antarctic</span> land snail, Notodiscus hookeri.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Charrier, Maryvonne; Marie, Arul; Guillaume, Damien; Bédouet, Laurent; Le Lannic, Joseph; Roiland, Claire; Berland, Sophie; Pierre, Jean-Sébastien; Le Floch, Marie; Frenot, Yves; Lebouvier, Marc</p> <p>2013-01-01</p> <p>Ecophenotypes reflect local matches between organisms and their environment, and show plasticity across generations in response to current living conditions. Plastic responses in shell morphology and shell growth have been widely studied in gastropods and are often related to environmental calcium availability, which influences shell biomineralisation. To date, all of these studies have overlooked micro-scale structure of the shell, in addition to how it is related to species responses in the context of environmental pressure. This study is the first to demonstrate that environmental factors induce a bi-modal variation in the shell micro-scale structure of a land gastropod. Notodiscus hookeri is the only native land snail present in the Crozet Archipelago (<span class="hlt">sub-Antarctic</span> region). The adults have evolved into two ecophenotypes, which are referred to here as MS (mineral shell) and OS (organic shell). The MS-ecophenotype is characterised by a thick mineralised shell. It is primarily distributed along the coastline, and could be associated to the presence of exchangeable calcium in the clay minerals of the soils. The Os-ecophenotype is characterised by a thin organic shell. It is primarily distributed at high altitudes in the mesic and xeric fell-fields in soils with large particles that lack clay and exchangeable calcium. Snails of the Os-ecophenotype are characterised by thinner and larger shell sizes compared to snails of the MS-ecophenotype, indicating a trade-off between mineral thickness and shell size. This pattern increased along a temporal scale; whereby, older adult snails were more clearly separated into two clusters compared to the younger adult snails. The prevalence of glycine-rich proteins in the organic shell layer of N. hookeri, along with the absence of chitin, differs to the organic scaffolds of molluscan biominerals. The present study provides new insights for testing the adaptive value of phenotypic plasticity in response to spatial and temporal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GBioC..30.1682G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GBioC..30.1682G"><span>Anthropogenic carbon in the ocean—Surface to interior connections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Groeskamp, Sjoerd; Lenton, Andrew; Matear, Richard; Sloyan, Bernadette M.; Langlais, Clothilde</p> <p>2016-11-01</p> <p>Quantifying the surface to interior transport of anthropogenic carbon (CA) is critical for projecting future carbon uptake and for improved understanding of the role of the oceans in the global carbon cycle. Here we develop and apply a diagnostic tool that provides a volumetric stream function in (CA,σ0) coordinates to calculate the total diapycnal CA transport in the ocean, where σ0 is the surface referenced potential density anomaly. We combine this with air-sea fluxes of CA to infer the internal ocean mixing of CA to obtain a closed globally integrated budget analyses of the ocean's CA transport. This diagnostic separates the contribution from the mean flow, seasonal cycles, trend, surface fluxes, and mixing in the distribution and the accumulation of CA in the ocean. We find that the redistribution of CA from the surface to the interior of the ocean is due to an interplay between circulation and mixing. The circulation component is dominated by the mean flow; however, effects due to seasonal cycles are significant for the CA redistribution. The two most important pathways for CA subduction are through the transformation of thermocline <span class="hlt">water</span> (TW) into <span class="hlt">subantarctic</span> <span class="hlt">mode</span> <span class="hlt">water</span> and by transformation of Circumpolar Deep <span class="hlt">Water</span> (CDW) into lighter Antarctic Intermediate <span class="hlt">Water</span>. The results suggest that an accurate representation of intermediate and <span class="hlt">mode</span> <span class="hlt">water</span> formation, deep <span class="hlt">water</span> formation, and spatial and temporal distribution of ocean mixing in ocean models is essential to simulate and project the oceanic uptake of CA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1812878A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1812878A"><span>Extensive lake sediment coring survey on <span class="hlt">Sub-Antarctic</span> Indian Ocean Kerguelen Archipelago (French Austral and Antarctic Lands)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnaud, Fabien; Fanget, Bernard; Malet, Emmanuel; Poulenard, Jérôme; Støren, Eivind; Leloup, Anouk; Bakke, Jostein; Sabatier, Pierre</p> <p>2016-04-01</p> <p>Recent paleo-studies revealed climatic southern high latitude climate evolution patterns that are crucial to understand the global climate evolution(1,2). Among others the strength and north-south shifts of westerlies wind appeared to be a key parameter(3). However, virtually no lands are located south of the 45th South parallel between Southern Georgia (60°W) and New Zealand (170°E) precluding the establishment of paleoclimate records of past westerlies dynamics. Located around 50°S and 70°E, lost in the middle of the <span class="hlt">sub-Antarctic</span> Indian Ocean, Kerguelen archipelago is a major, geomorphologically complex, land-mass that is covered by hundreds lakes of various sizes. It hence offers a unique opportunity to reconstruct past climate and environment dynamics in a region where virtually nothing is known about it, except the remarkable recent reconstructions based on a Lateglacial peatbog sequence(4). During the 2014-2015 austral summer, a French-Norwegian team led the very first extensive lake sediment coring survey on Kerguelen Archipelago under the umbrella of the PALAS program supported by the French Polar Institute (IPEV). Two main areas were investigated: i) the southwest of the mainland, so-called Golfe du Morbihan, where glaciers are currently absent and ii) the northernmost Kerguelen mainland peninsula so-called Loranchet, where cirque glaciers are still present. This double-target strategy aims at reconstructing various independent indirect records of precipitation (glacier advance, flood dynamics) and wind speed (marine spray chemical species, wind-borne terrigenous input) to tackle the Holocene climate variability. Despite particularly harsh climate conditions and difficult logistics matters, we were able to core 6 lake sediment sites: 5 in Golfe du Morbihan and one in Loranchet peninsula. Among them two sequences taken in the 4km-long Lake Armor using a UWITEC re-entry piston coring system by 20 and 100m <span class="hlt">water</span>-depth (6 and 7m-long, respectively). One</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdAtS..34..521L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdAtS..34..521L"><span>On the response of subduction in the South Pacific to an intensification of westerlies and heat flux in an eddy permitting ocean model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Chengyan; Wang, Zhaomin; Li, Bingrui; Cheng, Chen; Xia, Ruibin</p> <p>2017-04-01</p> <p>Based on an eddy permitting ocean general circulation model, the response of <span class="hlt">water</span> masses to two distinct climate scenarios in the South Pacific is assessed in this paper. Under annually repeating atmospheric forcing that is characterized by different westerlies and associated heat flux, the response of <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> (SAMW) and Antarctic Intermediate <span class="hlt">Water</span> (AAIW) is quantitatively estimated. Both SAMW and AAIW are found to be warmer, saltier and denser under intensified westerlies and increased heat loss. The increase in the subduction volume of SAMW and AAIW is about 19.8 Sv (1 Sv = 106 m3 s-1). The lateral induction term plays a dominant role in the changes in the subduction volume due to the deepening of the mixed layer depth (MLD). Furthermore, analysis of the buoyancy budget is used to quantitatively diagnose the reason for the changes in the MLD. The deepening of the MLD is found to be primarily caused by the strengthening of heat loss from the ocean to the atmosphere in the formation region of SAMW and AAIW.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28576050','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28576050"><span>Extraction and characterization of collagen from Antarctic and <span class="hlt">Sub-Antarctic</span> squid and its potential application in hybrid scaffolds for tissue engineering.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Coelho, Rui C G; Marques, Ana L P; Oliveira, Sara M; Diogo, Gabriela S; Pirraco, Rogério P; Moreira-Silva, Joana; Xavier, José C; Reis, Rui L; Silva, Tiago H; Mano, João F</p> <p>2017-09-01</p> <p>Collagen is the most abundant protein found in mammals and it exhibits a low immunogenicity, high biocompatibility and biodegradability when compared with others natural polymers. For this reason, it has been explored for the development of biologically instructive biomaterials with applications for tissue substitution and regeneration. Marine origin collagen has been pursued as an alternative to the more common bovine and porcine origins. This study focused on squid (Teuthoidea: Cephalopoda), particularly the Antarctic squid Kondakovia longimana and the <span class="hlt">Sub-Antarctic</span> squid Illex argentinus as potential collagen sources. In this study, collagen has been isolated from the skins of the squids using acid-based and pepsin-based protocols, with the higher yield being obtained from I. argentinus in the presence of pepsin. The produced collagen has been characterized in terms of physicochemical properties, evidencing an amino acid profile similar to the one of calf collagen, but exhibiting a less preserved structure, with hydrolyzed portions and a lower melting temperature. Pepsin-soluble collagen isolated from I. argentinus was selected for further evaluation of biomedical potential, exploring its incorporation on poly-ε-caprolactone (PCL) 3D printed scaffolds for the development of hybrid scaffolds for tissue engineering, exhibiting hierarchical features. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28886939','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28886939"><span>Development of an on-line mixed-<span class="hlt">mode</span> gel liquid chromatography×reversed phase liquid chromatography method for separation of <span class="hlt">water</span> extract from Flos Carthami.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Yu-Qing; Tang, Xu; Li, Jia-Fu; Wu, Yun-Long; Sun, Yu-Ying; Fang, Mei-Juan; Wu, Zhen; Wang, Xiu-Min; Qiu, Ying-Kun</p> <p>2017-10-13</p> <p>A novel on-line comprehensive two-dimensional liquid chromatography (2D-LC) method by coupling mixed-<span class="hlt">mode</span> gel liquid chromatography (MMG-LC) with reversed phase liquid chromatography (RPLC) was developed. A mixture of 17 reference compounds was used to study the separation mechanism. A crude <span class="hlt">water</span> extract of Flos Carthami was applied to evaluate the performance of the novel 2D-LC system. In the first dimension, the extract was eluted with a gradient of <span class="hlt">water</span>/methanol over a cross-linked dextran gel Sephadex LH-20 column. Meanwhile, the advantages of size exclusion, reversed phase partition and adsorption separation mechanism were exploited before further on-line reversed phase purification on the second dimension. This novel on-line mixed-<span class="hlt">mode</span> Sephadex LH-20×RPLC method provided higher peak resolution, sample processing ability (2.5mg) and better orthogonality (72.9%) versus RPLC×RPLC and hydrophilic interaction liquid chromatography (HILIC)×RPLC. To the best of our knowledge, this is the first report of a mixed-<span class="hlt">mode</span> Sephadex LH-20×RPLC separation method with successful applications in on-line <span class="hlt">mode</span>, which might be beneficial for harvesting targets from complicated medicinal plants. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27733109','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27733109"><span>Dispersal in the <span class="hlt">sub-Antarctic</span>: king penguins show remarkably little population genetic differentiation across their range.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Clucas, Gemma V; Younger, Jane L; Kao, Damian; Rogers, Alex D; Handley, Jonathan; Miller, Gary D; Jouventin, Pierre; Nolan, Paul; Gharbi, Karim; Miller, Karen J; Hart, Tom</p> <p>2016-10-13</p> <p>Seabirds are important components of marine ecosystems, both as predators and as indicators of ecological change, being conspicuous and sensitive to changes in prey abundance. To determine whether fluctuations in population sizes are localised or indicative of large-scale ecosystem change, we must first understand population structure and dispersal. King penguins are long-lived seabirds that occupy a niche across the <span class="hlt">sub-Antarctic</span> zone close to the Polar Front. Colonies have very different histories of exploitation, population recovery, and expansion. We investigated the genetic population structure and patterns of colonisation of king penguins across their current range using a dataset of 5154 unlinked, high-coverage single nucleotide polymorphisms generated via restriction site associated DNA sequencing (RADSeq). Despite breeding at a small number of discrete, geographically separate sites, we find only very slight genetic differentiation among colonies separated by thousands of kilometers of open-ocean, suggesting migration among islands and archipelagos may be common. Our results show that the South Georgia population is slightly differentiated from all other colonies and suggest that the recently founded Falkland Island colony is likely to have been established by migrants from the distant Crozet Islands rather than nearby colonies on South Georgia, possibly as a result of density-dependent processes. The observed subtle differentiation among king penguin colonies must be considered in future conservation planning and monitoring of the species, and demographic models that attempt to forecast extinction risk in response to large-scale climate change must take into account migration. It is possible that migration could buffer king penguins against some of the impacts of climate change where colonies appear panmictic, although it is unlikely to protect them completely given the widespread physical changes projected for their Southern Ocean foraging grounds</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017DSRI..127...41H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017DSRI..127...41H"><span>Habitat associations and distribution of the hyperbenthic shrimp, Nauticaris marionis, around the <span class="hlt">sub-Antarctic</span> Prince Edward Islands</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haley, Craig; von der Meden, Charles; Atkinson, Lara; Reed, Cecile</p> <p>2017-09-01</p> <p>The association of organisms with particular habitats and habitat-forming organisms, can strongly influence species distributions, interactions and wider ecosystem services. At the <span class="hlt">sub-Antarctic</span> Prince Edward Islands, the caridean shrimp Nauticaris marionis is a principal part of the benthic ecosystem, occurring between ca. 50 m and 600 m. Its role as a trophic link between the primary productivity and higher predators is established, but little is understood of its in situ habitat usage and associations or of how these structure patterns of abundance. We investigated these aspects directly using a benthic camera sled, sampling 27 stations between 50 m and 500 m. Substratum type was characterised, and estimates of percentage cover of the 13 main groups of habitat-forming epibenthic taxa were made, alongside absolute counts of N. marionis within 'digital quadrats' drawn from 300 m transects. The distribution of N. marionis was influenced by depth, substratum type and overall biogenic cover, being limited to habitats between 50 and 160 m depth on mud or gravel substrata only, and having > 50% biogenic cover. The presence/absence of N. marionis related to significantly different epibenthic assemblages (termed biogenic habitats), but this effect was contingent on depth. Likewise, densities of N. marionis were significantly affected by biogenic habitat type, identifying an association with two biogenic habitat groups, one dominated by red-algae, the other by structurally complex bryozoan species. These associations likely relate to the structural complexity of the two habitat groups, rather than the specific taxa involved. The apparent absence of N. marionis at depths > 160 m contrasts with earlier records and poses questions about the trophic importance of the shrimp in deeper habitats.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..12210042B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..12210042B"><span>Southern Ocean Mixed-Layer Seasonal and Interannual Variations From Combined Satellite and In Situ Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Buongiorno Nardelli, B.; Guinehut, S.; Verbrugge, N.; Cotroneo, Y.; Zambianchi, E.; Iudicone, D.</p> <p>2017-12-01</p> <p>The depth of the upper ocean mixed layer provides fundamental information on the amount of seawater that directly interacts with the atmosphere. Its space-time variability modulates <span class="hlt">water</span> mass formation and carbon sequestration processes related to both the physical and biological pumps. These processes are particularly relevant in the Southern Ocean, where surface mixed-layer depth estimates are generally obtained either as climatological fields derived from in situ observations or through numerical simulations. Here we demonstrate that weekly observation-based reconstructions can be used to describe the variations of the mixed-layer depth in the upper ocean over a range of space and time scales. We compare and validate four different products obtained by combining satellite measurements of the sea surface temperature, salinity, and dynamic topography and in situ Argo profiles. We also compute an ensemble mean and use the corresponding spread to estimate mixed-layer depth uncertainties and to identify the more reliable products. The analysis points out the advantage of synergistic approaches that include in input the sea surface salinity observations obtained through a multivariate optimal interpolation. Corresponding data allow to assess mixed-layer depth seasonal and interannual variability. Specifically, the maximum correlations between mixed-layer anomalies and the Southern Annular <span class="hlt">Mode</span> are found at different time lags, related to distinct summer/winter responses in the Antarctic Intermediate <span class="hlt">Water</span> and <span class="hlt">Sub-Antarctic</span> <span class="hlt">Mode</span> <span class="hlt">Waters</span> main formation areas.</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/21607694','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21607694"><span>Characterization of MHC class I and II genes in a <span class="hlt">subantarctic</span> seabird, the blue petrel, Halobaena caerulea (Procellariiformes).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Strandh, Maria; Lannefors, Mimi; Bonadonna, Francesco; Westerdahl, Helena</p> <p>2011-10-01</p> <p>The great polymorphism observed in the major histocompatibility complex (MHC) genes is thought to be maintained by pathogen-mediated selection possibly combined with MHC-disassortative mating, guided by MHC-determined olfactory cues. Here, we partly characterize the MHC class I and II B of the blue petrel, Halobaena caerulea (Procellariiformes), a bird with significant olfactory abilities that lives under presumably low pathogen burdens in Subantarctica. Blue petrels are long-lived, monogamous birds which suggest the necessity of an accurate mate choice process. The species is ancestral to songbirds (Passeriformes; many MHC loci), although not to gamefowls (Galliformes; few MHC loci). Considering the phylogenetic relationships and the low <span class="hlt">subantarctic</span> pathogen burden, we expected few rather than many MHC loci in the blue petrel. However, when we analysed partial MHC class I and class II B cDNA and gDNA sequences we found evidence for as many as at least eight MHC class I loci and at least two class II B loci. These class I and II B sequences showed classical MHC characteristics, e.g. high nucleotide diversity, especially in putative peptide-binding regions where signatures of positive selection was detected. Trans-species polymorphism was found between MHC class II B sequences of the blue petrel and those of thin-billed prion, Pachyptila belcheri, two species that diverged ∼25 MYA. The observed MHC allele richness in the blue petrel may well serve as a basis for mate choice, especially since olfactory discrimination of MHC types may be possible in this species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19770016250','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19770016250"><span>Advanced high pressure engine study for mixed-<span class="hlt">mode</span> vehicle applications</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Luscher, W. P.; Mellish, J. A.</p> <p>1977-01-01</p> <p>High pressure liquid rocket engine design, performance, weight, envelope, and operational characteristics were evaluated for a variety of candidate engines for use in mixed-<span class="hlt">mode</span>, single-stage-to-orbit applications. Propellant property and performance data were obtained for candidate <span class="hlt">Mode</span> 1 fuels which included: RP-1, RJ-5, hydrazine, monomethyl-hydrazine, and methane. The common oxidizer was liquid oxygen. Oxygen, the candidate <span class="hlt">Mode</span> 1 fuels, and hydrogen were evaluated as thrust chamber coolants. Oxygen, methane, and hydrogen were found to be the most viable cooling candidates. <span class="hlt">Water</span>, lithium, and sodium-potassium were also evaluated as auxiliary coolant systems. <span class="hlt">Water</span> proved to be the best of these, but the system was heavier than those systems which cooled with the engine propellants. Engine weight and envelope parametric data were established for candidate <span class="hlt">Mode</span> 1, <span class="hlt">Mode</span> 2, and dual-fuel engines. Delivered engine performance data were also calculated for all candidate <span class="hlt">Mode</span> 1 and dual-fuel engines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMPP11B1792Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMPP11B1792Z"><span>Pleistocene atmospheric CO2 change linked to Southern Ocean nutrient utilization</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ziegler, M.; Diz, P.; Hall, I. R.; Zahn, R.</p> <p>2011-12-01</p> <p>Biological uptake of CO2 by the ocean and its subsequent storage in the abyss is intimately linked with the global carbon cycle and constitutes a significant climatic force1. The Southern Ocean is a particularly important region because its wind-driven upwelling regime brings CO2 laden abyssal <span class="hlt">waters</span> to the surface that exchange CO2 with the atmosphere. The <span class="hlt">Subantarctic</span> Zone (SAZ) is a CO2 sink and also drives global primary productivity as unutilized nutrients, advected with surface <span class="hlt">waters</span> from the south, are exported via <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> (SAMW) as preformed nutrients to the low latitudes where they fuel the biological pump in upwelling areas. Recent model estimates suggest that up to 40 ppm of the total 100 ppm atmospheric pCO2 reduction during the last ice age were driven by increased nutrient utilization in the SAZ and associated feedbacks on the deep ocean alkalinity. Micro-nutrient fertilization by iron (Fe), contained in the airborne dust flux to the SAZ, is considered to be the prime factor that stimulated this elevated photosynthetic activity thus enhancing nutrient utilization. We present a millennial-scale record of the vertical stable carbon isotope gradient between subsurface and deep <span class="hlt">water</span> (Δδ13C) in the SAZ spanning the past 350,000 years. The Δδ13C gradient, derived from planktonic and benthic foraminifera, reflects the efficiency of biological pump and is highly correlated (rxy = -0.67 with 95% confidence interval [0.63; 0.71], n=874) with the record of dust flux preserved in Antarctic ice cores6. This strongly suggests that nutrient utilization in the SAZ was dynamically coupled to dust-induced Fe fertilization across both glacial-interglacial and faster millennial timescales. In concert with ventilation changes of the deep Southern Ocean this drove ocean-atmosphere CO2 exchange and, ultimately, atmospheric pCO2 variability during the late Pleistocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3869943','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3869943"><span>Soil Calcium Availability Influences Shell Ecophenotype Formation in the <span class="hlt">Sub-Antarctic</span> Land Snail, Notodiscus hookeri</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Charrier, Maryvonne; Marie, Arul; Guillaume, Damien; Bédouet, Laurent; Le Lannic, Joseph; Roiland, Claire; Berland, Sophie; Pierre, Jean-Sébastien; Le Floch, Marie; Frenot, Yves; Lebouvier, Marc</p> <p>2013-01-01</p> <p>Ecophenotypes reflect local matches between organisms and their environment, and show plasticity across generations in response to current living conditions. Plastic responses in shell morphology and shell growth have been widely studied in gastropods and are often related to environmental calcium availability, which influences shell biomineralisation. To date, all of these studies have overlooked micro-scale structure of the shell, in addition to how it is related to species responses in the context of environmental pressure. This study is the first to demonstrate that environmental factors induce a bi-modal variation in the shell micro-scale structure of a land gastropod. Notodiscus hookeri is the only native land snail present in the Crozet Archipelago (<span class="hlt">sub-Antarctic</span> region). The adults have evolved into two ecophenotypes, which are referred to here as MS (mineral shell) and OS (organic shell). The MS-ecophenotype is characterised by a thick mineralised shell. It is primarily distributed along the coastline, and could be associated to the presence of exchangeable calcium in the clay minerals of the soils. The Os-ecophenotype is characterised by a thin organic shell. It is primarily distributed at high altitudes in the mesic and xeric fell-fields in soils with large particles that lack clay and exchangeable calcium. Snails of the Os-ecophenotype are characterised by thinner and larger shell sizes compared to snails of the MS- ecophenotype, indicating a trade-off between mineral thickness and shell size. This pattern increased along a temporal scale; whereby, older adult snails were more clearly separated into two clusters compared to the younger adult snails. The prevalence of glycine-rich proteins in the organic shell layer of N. hookeri, along with the absence of chitin, differs to the organic scaffolds of molluscan biominerals. The present study provides new insights for testing the adaptive value of phenotypic plasticity in response to spatial and temporal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhFl...25i7103C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhFl...25i7103C"><span>A semi-analytical method for near-trapped <span class="hlt">mode</span> and fictitious frequencies of multiple scattering by an array of elliptical cylinders in <span class="hlt">water</span> waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Jeng-Tzong; Lee, Jia-Wei</p> <p>2013-09-01</p> <p>In this paper, we focus on the <span class="hlt">water</span> wave scattering by an array of four elliptical cylinders. The null-field boundary integral equation method (BIEM) is used in conjunction with degenerate kernels and eigenfunctions expansion. The closed-form fundamental solution is expressed in terms of the degenerate kernel containing the Mathieu and the modified Mathieu functions in the elliptical coordinates. Boundary densities are represented by using the eigenfunction expansion. To avoid using the addition theorem to translate the Mathieu functions, the present approach can solve the <span class="hlt">water</span> wave problem containing multiple elliptical cylinders in a semi-analytical manner by introducing the adaptive observer system. Regarding <span class="hlt">water</span> wave problems, the phenomena of numerical instability of fictitious frequencies may appear when the BIEM/boundary element method (BEM) is used. Besides, the near-trapped <span class="hlt">mode</span> for an array of four identical elliptical cylinders is observed in a special layout. Both physical (near-trapped <span class="hlt">mode</span>) and mathematical (fictitious frequency) resonances simultaneously appear in the present paper for a <span class="hlt">water</span> wave problem by an array of four identical elliptical cylinders. Two regularization techniques, the combined Helmholtz interior integral equation formulation (CHIEF) method and the Burton and Miller approach, are adopted to alleviate the numerical resonance due to fictitious frequency.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15683175','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15683175"><span>Mercury concentrations in king penguin (Aptenodytes patagonicus) feathers at Crozet Islands (<span class="hlt">sub-Antarctic</span>): temporal trend between 1966--1974 and 2000--2001.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Scheifler, Renaud; Gauthier-Clerc, Michel; Le Bohec, Céline; Crini, Nadia; Coeurdassier, Michaël; Badot, Pierre-Marie; Giraudoux, Patrick; Le Maho, Yvon</p> <p>2005-01-01</p> <p>Remote <span class="hlt">sub-Antarctic</span> islands and their wildlife may be contaminated by mercury via atmospheric and oceanic currents. Because of mercury's high toxicity and its capacity to be biomagnified in marine food chains, top predators like seabirds may be threatened by secondary poisoning. The present study provides data regarding mercury concentrations in breast feathers sampled in 2000 and 2001 on king penguins (Aptenodytes patagonicus) living at Crozet Islands. These contemporary concentrations were compared to those measured in feathers of king penguins sampled in the same colony between 1966 and 1974 and preserved in a museum (1970s sample). The average concentration of the contemporary sample is 1.98 microg g(-1) (dry mass) and is significantly different than the concentrations reported in some other penguin species. The concentration of the contemporary sample is significantly lower than the concentration of the 1970s sample (2.66 microg g(-1)). This suggests that mercury concentrations in southern hemisphere seabirds do not increase, which conflicts with the trends observed in the northern hemisphere. This difference in temporal trends between the northern and southern hemispheres usually is attributed mainly to a higher degree of pollutant emission in the northern hemisphere. Parameters that may explain the interspecies differences in mercury concentrations are discussed. These first results may constitute a basis for further ecotoxicological and/or biomonitoring studies of king penguins in these remote ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AtmEn.123....9D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AtmEn.123....9D"><span>Surface greenhouse gas fluxes downwind of a penguin colony in the maritime <span class="hlt">sub-Antarctic</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Drewer, Julia; Braban, Christine F.; Tang, Y. Sim; Anderson, Margaret; Skiba, Ute M.; Dragosits, Ulrike; Trathan, Phil</p> <p>2015-12-01</p> <p>The relationship between ammonia (NH3) concentrations downwind from a penguin colony and local surface greenhouse gas (GHG) fluxes was investigated on the remote <span class="hlt">sub-Antarctic</span> Bird Island (54°00‧S, 38°03‧W) during summer 2010 (November and December). A Macaroni penguin (Eudyptes chrysolophus) colony (40,000 pairs) at Goldcrest Point is a large point source of NH3 on the island and a measurement transect of 23 m, 36 m, 70 m, 143 m and 338 m was set up downwind from the colony. Atmospheric NH3 concentrations measured by passive diffusion samplers declined from 23 μg m-3 close to the colony to less than 1 μg m-3 338 m downwind. As increased nitrogen (N) deposition can affect soil carbon (C) and N cycling, it can therefore potentially influence GHG and nitric oxide (NO) emission rates. However, in this study, a clear correlation between surface GHG fluxes and atmospheric NH3 concentrations could not be established. Average fluxes for nitrous oxide (N2O), methane (CH4) and carbon dioxide (CO2) over the entire transect and the eight week study period ranged from 7 to 23 μg N2O-N m-2 h-1, -5.5-245 μg CH4 m-2 h-1, and CO2 respiration rates averaged 2.2 μmol m-2 s-1. Laboratory studies using intact soil cores from the transect also did not show any significant correlation between atmospheric NH3 concentrations and N2O, NO, CH4 emissions or CO2 respiration rates. Overall, fluxes measured in the laboratory study reflected the high variability measured in the field. Large changes in soil depth along the transect, due to the topography of the island, possibly influenced fluxes more than NH3 concentration and seabirds appeared to have a more localised input (e.g. ground nesting birds). However, warmer temperatures might have a large potential to increase GHG fluxes in this ecosystem. This study confirms that GHG fluxes do occur in these ornithogenic ecosystems, however, the scale of the impact remains largely unquantified due to high uncertainties and high spatial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11554405','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11554405"><span>Study of matrix effects on the direct trace analysis of acidic pesticides in <span class="hlt">water</span> using various liquid chromatographic <span class="hlt">modes</span> coupled to tandem mass spectrometric detection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dijkman, E; Mooibroek, D; Hoogerbrugge, R; Hogendoorn, E; Sancho, J V; Pozo, O; Hernández, F</p> <p>2001-08-10</p> <p>This study investigated the effects of matrix interferences on the analytical performance of a triple quadrupole mass spectrometric (MS-MS) detector coupled to various reversed-phase liquid chromatographic (LC) <span class="hlt">modes</span> for the on-line determination of various types of acidic herbicides in <span class="hlt">water</span> using external calibration for quantification of the analytes tested at a level of 0.4 microg/l. The LC <span class="hlt">modes</span> included (i) a single-column configuration (LC), (ii) precolumn switching (PC-LC) and (iii) coupled-column LC (LC-LC). As regards detection, electrospray (ESI) and atmospheric pressure chemical ionization (APCI) in both positive (PI) and negative (NI) ionization <span class="hlt">modes</span> were examined. Salinity and dissolved organic carbon (DOC) were selected as interferences to study matrix effects in this type of analysis. Therefore, Milli-Q and tap <span class="hlt">water</span> samples both fortified with 12 mg/l DOC and spiked with sulfometuron-methyl, bentazone, bromoxynil, 2-methyl-4-chlorophenoxyacetic acid, and 2-methyl-4-chlorophenoxypropionic acid at a level of about 0.4 microg/l were analyzed with the various LC-MS approaches. Direct sample injection was performed with volumes of 0.25 ml or 2.0 ml on a column of 2.1 mm I.D. or 4.6 mm I.D. for the ESI and APCI <span class="hlt">modes</span>, respectively. The recovery data were used to compare and evaluate the analytical performance of the various LC approaches. As regards matrix effects, the salinity provided a dramatic decrease in response for early eluting analytes (k value of about 1) when using the LC <span class="hlt">mode</span>. Both PC-LC and LC-LC efficiently eliminated this problem. The high DOC content hardly effected the responses of analytes in the ESI <span class="hlt">mode</span>, while in most cases the responses increased when using APCI-MS-MS detection. Of all the tested configurations, LC-LC-ESI-MS-MS with the column combination Discovery C18/ABZ+ was the most favorable as regards elimination of matrix effects and provided reliable quantification of all compounds using external calibration at the tested</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16791191','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16791191"><span>The Southern Ocean biogeochemical divide.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Marinov, I; Gnanadesikan, A; Toggweiler, J R; Sarmiento, J L</p> <p>2006-06-22</p> <p>Modelling studies have demonstrated that the nutrient and carbon cycles in the Southern Ocean play a central role in setting the air-sea balance of CO(2) and global biological production. Box model studies first pointed out that an increase in nutrient utilization in the high latitudes results in a strong decrease in the atmospheric carbon dioxide partial pressure (pCO2). This early research led to two important ideas: high latitude regions are more important in determining atmospheric pCO2 than low latitudes, despite their much smaller area, and nutrient utilization and atmospheric pCO2 are tightly linked. Subsequent general circulation model simulations show that the Southern Ocean is the most important high latitude region in controlling pre-industrial atmospheric CO(2) because it serves as a lid to a larger volume of the deep ocean. Other studies point out the crucial role of the Southern Ocean in the uptake and storage of anthropogenic carbon dioxide and in controlling global biological production. Here we probe the system to determine whether certain regions of the Southern Ocean are more critical than others for air-sea CO(2) balance and the biological export production, by increasing surface nutrient drawdown in an ocean general circulation model. We demonstrate that atmospheric CO(2) and global biological export production are controlled by different regions of the Southern Ocean. The air-sea balance of carbon dioxide is controlled mainly by the biological pump and circulation in the Antarctic deep-<span class="hlt">water</span> formation region, whereas global export production is controlled mainly by the biological pump and circulation in the <span class="hlt">Subantarctic</span> intermediate and <span class="hlt">mode</span> <span class="hlt">water</span> formation region. The existence of this biogeochemical divide separating the Antarctic from the <span class="hlt">Subantarctic</span> suggests that it may be possible for climate change or human intervention to modify one of these without greatly altering the other.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19674310','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19674310"><span>Pleistocene refugia and polytopic replacement of diploids by tetraploids in the Patagonian and <span class="hlt">Subantarctic</span> plant Hypochaeris incana (Asteraceae, Cichorieae).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tremetsberger, Karin; Urtubey, Estrella; Terrab, Anass; Baeza, Carlos M; Ortiz, María Angeles; Talavera, María; König, Christiane; Temsch, Eva M; Kohl, Gudrun; Talavera, Salvador; Stuessy, Tod F</p> <p>2009-09-01</p> <p>We report the phylogeographic pattern of the Patagonian and <span class="hlt">Subantarctic</span> plant Hypochaeris incana endemic to southeastern South America. We applied amplified fragment length polymorphism (AFLP) and chloroplast DNA (cpDNA) analysis to 28 and 32 populations, respectively, throughout its distributional range and assessed ploidy levels using flow cytometry. While cpDNA data suggest repeated or simultaneous parallel colonization of Patagonia and Tierra del Fuego by several haplotypes and/or hybridization, AFLPs reveal three clusters corresponding to geographic regions. The central and northern Patagonian clusters (approximately 38-51 degrees S), which are closer to the outgroup, contain mainly tetraploid, isolated and highly differentiated populations with low genetic diversity. To the contrary, the southern Patagonian and Fuegian cluster (approximately 51-55 degrees S) contains mainly diploid populations with high genetic diversity and connected by high levels of gene flow. The data suggest that H. incana originated at the diploid level in central or northern Patagonia, from where it migrated south. All three areas, northern, central and southern, have similar levels of rare and private AFLP bands, suggesting that all three served as refugia for H. incana during glacial times. In southern Patagonia and Tierra del Fuego, the species seems to have expanded its populational system in postglacial times, when the climate became warmer and more humid. In central and northern Patagonia, the populations seem to have become restricted to favourable sites with increasing temperature and decreasing moisture and there was a parallel replacement of diploids by tetraploids in local populations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JMS...157...20S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JMS...157...20S"><span>Influence of oceanographic features on the spatial and seasonal patterns of mesozooplankton in the southern Patagonian shelf (Argentina, SW Atlantic)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sabatini, M. E.; Reta, R.; Lutz, V. A.; Segura, V.; Daponte, C.</p> <p>2016-05-01</p> <p>Surveys conducted during spring, summer and late winter in 2005-2006 over the southern Patagonian shelf have allowed the seasonal distribution of mesozooplankton communities in relation to <span class="hlt">water</span> masses and circulation to be investigated. In this system, most of the shelf is dominated by a distinct low salinity plume that is related to the runoff from the Magellan Strait (MSW), while the outer shelf is highly influenced by the cold and salty <span class="hlt">Subantarctic</span> <span class="hlt">water</span> (SAW) of the boundary Malvinas Current. Separating these two, the <span class="hlt">Subantarctic</span> Shelf <span class="hlt">water</span> mass (SASW) extends over the middle shelf. Correspondingly, the structure of the MSW and SAW mesozooplankton communities was found to be clearly different, while the former and the SASW assemblages were barely separable. This relatively fresh <span class="hlt">water</span> mass is actually a variant of <span class="hlt">Subantarctic</span> <span class="hlt">water</span> that enters into the region from the south and the shelf-break, and hence its mesozooplankton community was not significantly different from that of the SAW <span class="hlt">water</span> mass. Dissimilar species abundance, in turn associated with different life histories and population development, was more important than species composition in defining the assemblages. Total mesozooplankton abundance increased about 2.5-fold from the beginning of spring to late summer, and then decreased at least two orders of magnitude in winter. Across all seasons copepods represented > 70-80% of total mesozooplankton over most of the shelf. Copepod species best represented through all seasons, in terms of both relative abundance and occurrence, were Drepanopus forcipatus and Oithona helgolandica. Although seasonal differences in abundance were striking, the spatial distribution of mesozooplankton was largely similar across seasons, with relatively higher concentrations occurring mainly in Grande Bay and surroundings. The well defined spatial patterns of mesozooplankton that appear from our results in conjunction with the southward wide extension of the shelf and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22486789-new-water-soluble-heterometallic-complex-showing-unpredicted-coordination-modes-edta','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22486789-new-water-soluble-heterometallic-complex-showing-unpredicted-coordination-modes-edta"><span>New <span class="hlt">water</span> soluble heterometallic complex showing unpredicted coordination <span class="hlt">modes</span> of EDTA</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>Mudsainiyan, R.K., E-mail: mudsainiyanrk@gmail.com; Jassal, A.K.; Chawla, S.K., E-mail: sukhvinder.k.chawla@gmail.com</p> <p>2015-10-15</p> <p>A mesoporous 3D polymeric complex (I) having formula ([Zr(IV)O-μ{sup 3}-(EDTA)Fe(III)OH]·H{sub 2}O){sub n} has been crystallized and characterized by various techniques. Single-crystal X-ray diffraction analysis revealed that complex (I) crystallized in chiral monoclinic space group Cc (space group no. 9) with unexpected coordination <span class="hlt">modes</span> of EDTA and mixture of two transition metal ions. In this complex, the coordination number of Zr(IV) ion is seven where four carboxylate oxygen atoms, two nitrogen atoms, one oxide atom are coordinating with Zr(IV). Fe(III) is four coordinated and its coordination environment is composed of three different carboxylic oxygen atoms from three different EDTA and onemore » oxygen atom of –OH group. The structure consists of 4-c and 16-c (2-nodal) net with new topology and point symbol for net is (3{sup 36}·4{sup 54}·5{sup 30})·(3{sup 6}). TGA study and XRPD pattern showed that the coordination polymer is quite stable even after losing <span class="hlt">water</span> molecule and –OH ion. Quenching behavior in fluorescence of ligand is observed by complexation with transition metal ions is due to n–π⁎ transition. The SEM micrograph shows the morphology of complex (I) exhibits spherical shape with size ranging from 50 to 280 nm. The minimum N{sub 2} (S{sub BET}=8.7693 m{sup 2}/g) and a maximum amount of H{sub 2} (high surface area=1044.86 m{sup 2}/g (STP)) could be adsorbed at 77 K. From DLS study, zeta potential is calculated i.e. −7.94 shows the negative charges on the surface of complex. Hirshfeld surface analysis and fingerprint plots revealed influence of weak or non bonding interactions in crystal packing of complex. - Graphical abstract: The complex (I) crystallized with unexpected coordination <span class="hlt">modes</span> of EDTA having 4-c, 16-c net with new topology and point symbol is (3{sup 36}·4{sup 54}·5{sup 30})·(3{sup 6}). TGA study and XRPD pattern proved its stability with high preference of H{sub 2} uptake by complex. - Highlights: • 3D</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PSST...27a5002M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PSST...27a5002M"><span>Studying Townsend and glow <span class="hlt">modes</span> in an atmospheric-pressure DBD using mass spectrometry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>McKay, Kirsty; Donaghy, David; He, Feng; Bradley, James W.</p> <p>2018-01-01</p> <p>Ambient molecular beam mass spectrometry has been employed to examine the effects of the <span class="hlt">mode</span> of operation and the excitation waveform on the ionic content of a helium-based atmospheric-pressure parallel plate dielectric barrier discharge. By applying 10 kHz microsecond voltage pulses with a nanosecond rise times and 10 kHz sinusoidal voltage waveforms, distinctly different glow and Townsend <span class="hlt">modes</span> were produced, respectively. Results showed a significant difference in the dominant ion species between the two <span class="hlt">modes</span>. In the Townsend <span class="hlt">mode</span>, molecular oxygen ions, atomic oxygen anions and nitric oxide anions are the most abundant species, however, in the glow <span class="hlt">mode</span> <span class="hlt">water</span> clusters ions and hydrated nitric oxygen anions dominate. Several hypotheses are put forward to explain these differences, including low electron densities and energies in the Townsend <span class="hlt">mode</span>, more efficient ionization of <span class="hlt">water</span> molecules through penning ionization and charge exchange with other species in glow <span class="hlt">mode</span>, and large temperature gradients due to the pulsed nature of the glow <span class="hlt">mode</span>, leading to more favorable conditions for cluster formation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26814667','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26814667"><span>Long-Term Seasonal and Interannual Patterns of Marine Mammal Strandings in Subtropical Western South Atlantic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Prado, Jonatas H F; Mattos, Paulo H; Silva, Kleber G; Secchi, Eduardo R</p> <p>2016-01-01</p> <p>Understanding temporal patterns of marine mammal occurrence is useful for establishing conservation strategies. We used a 38 yr-long dataset spanning 1976 to 2013 to describe temporal patterns and trends in marine mammal strandings along a subtropical stretch of the east coast of South America. This region is influenced by a transitional zone between tropical and temperate <span class="hlt">waters</span> and is considered an important fishing ground off Brazil. Generalized Additive Models were used to evaluate the temporal stranding patterns of the most frequently stranded species. Forty species were documented in 12,540 stranding events. Franciscana (n = 4,574), South American fur seal, (n = 3,419), South American sea lion (n = 2,049), bottlenose dolphins (n = 293) and <span class="hlt">subantarctic</span> fur seal (n = 219) were the most frequently stranded marine mammals. The seasonality of strandings of franciscana and bottlenose dolphin coincided with periods of higher fishing effort and strandings of South American and <span class="hlt">subantarctic</span> fur seals with post-reproductive dispersal. For South American sea lion the seasonality of strandings is associated with both fishing effort and post-reproductive dispersal. Some clear seasonal patterns were associated with occurrence of cold- (e.g. <span class="hlt">subantarctic</span> fur seal) and warm-<span class="hlt">water</span> (e.g. rough-toothed dolphin) species in winter and summer, respectively. Inter-annual increases in stranding rate were observed for franciscana and South American fur seal and these are likely related to increased fishing effort and population growth, respectively. For <span class="hlt">subantarctic</span> fur seal the stranding rate showed a slight decline while for bottlenose dolphin it remained steady. No significant year to year variation in stranding rate was observed for South American sea lion. The slight decrease in frequency of temperate/polar marine mammals and the increased occurrence of subtropical/tropical species since the late 1990s might be associated with environmental changes linked to climate change</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4729480','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4729480"><span>Long-Term Seasonal and Interannual Patterns of Marine Mammal Strandings in Subtropical Western South Atlantic</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Prado, Jonatas H. F.; Mattos, Paulo H.; Silva, Kleber G.; Secchi, Eduardo R.</p> <p>2016-01-01</p> <p>Understanding temporal patterns of marine mammal occurrence is useful for establishing conservation strategies. We used a 38 yr-long dataset spanning 1976 to 2013 to describe temporal patterns and trends in marine mammal strandings along a subtropical stretch of the east coast of South America. This region is influenced by a transitional zone between tropical and temperate <span class="hlt">waters</span> and is considered an important fishing ground off Brazil. Generalized Additive Models were used to evaluate the temporal stranding patterns of the most frequently stranded species. Forty species were documented in 12,540 stranding events. Franciscana (n = 4,574), South American fur seal, (n = 3,419), South American sea lion (n = 2,049), bottlenose dolphins (n = 293) and <span class="hlt">subantarctic</span> fur seal (n = 219) were the most frequently stranded marine mammals. The seasonality of strandings of franciscana and bottlenose dolphin coincided with periods of higher fishing effort and strandings of South American and <span class="hlt">subantarctic</span> fur seals with post-reproductive dispersal. For South American sea lion the seasonality of strandings is associated with both fishing effort and post-reproductive dispersal. Some clear seasonal patterns were associated with occurrence of cold- (e.g. <span class="hlt">subantarctic</span> fur seal) and warm-<span class="hlt">water</span> (e.g. rough-toothed dolphin) species in winter and summer, respectively. Inter-annual increases in stranding rate were observed for franciscana and South American fur seal and these are likely related to increased fishing effort and population growth, respectively. For <span class="hlt">subantarctic</span> fur seal the stranding rate showed a slight decline while for bottlenose dolphin it remained steady. No significant year to year variation in stranding rate was observed for South American sea lion. The slight decrease in frequency of temperate/polar marine mammals and the increased occurrence of subtropical/tropical species since the late 1990s might be associated with environmental changes linked to climate change</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29507919','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29507919"><span>Influence of Application Time and Etching <span class="hlt">Mode</span> of Universal Adhesives on Enamel Adhesion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sai, Keiichi; Takamizawa, Toshiki; Imai, Arisa; Tsujimoto, Akimasa; Ishii, Ryo; Barkmeier, Wayne W; Latta, Mark A; Miyazaki, Masashi</p> <p>2018-01-01</p> <p>To investigate the influence of application time and etching <span class="hlt">mode</span> of universal adhesives on enamel adhesion. Five universal adhesives, Adhese Universal, Bondmer Lightless, Clearfil Universal Bond Quick, G-Premio Bond, and Scotchbond Universal, were used. Bovine incisors were prepared and divided into four groups of ten teeth each. SBS, Ra, and SFE were determined after the following procedures: 1. self-etch <span class="hlt">mode</span> with immediate air blowing after application (IA); 2. self-etch <span class="hlt">mode</span> with prolonged application time (PA); 3. etch-and-rinse <span class="hlt">mode</span> with IA; 4. etch-and-rinse <span class="hlt">mode</span> with PA. After 24-h <span class="hlt">water</span> storage, the bonded assemblies were subjected to shear bond strength (SBS) tests. For surface roughness (Ra) and surface free energy (SFE) measurements, the adhesives were simply applied to the enamel and rinsed with acetone and <span class="hlt">water</span> before the measurements were carried out. Significantly higher SBS and Ra values were obtained with etch-and-rinse <span class="hlt">mode</span> than with self-etch <span class="hlt">mode</span> regardless of the application time or type of adhesive. Although most adhesives showed decreased SFE values with increased application time in self-etch <span class="hlt">mode</span>, SFE values in etch-and-rinse <span class="hlt">mode</span> were dependent on the adhesive type and application time. Etching <span class="hlt">mode</span>, application time, and type of adhesive significantly influenced the SBS, Ra, and SFE values.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26PSL.491...48D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26PSL.491...48D"><span>Reduced oxygenation at intermediate depths of the southwest Pacific during the last glacial maximum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Durand, Axel; Chase, Zanna; Noble, Taryn L.; Bostock, Helen; Jaccard, Samuel L.; Townsend, Ashley T.; Bindoff, Nathaniel L.; Neil, Helen; Jacobsen, Geraldine</p> <p>2018-06-01</p> <p>To investigate changes in oxygenation at intermediate depths in the southwest Pacific between the Last Glacial Maximum (LGM) and the Holocene, redox sensitive elements uranium and rhenium were measured in 12 sediment cores located on the Campbell and Challenger plateaux offshore from New Zealand. The core sites are currently bathed by <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> (SAMW), Antarctic Intermediate <span class="hlt">Water</span> (AAIW) and Upper Circumpolar Deep <span class="hlt">Water</span> (UCDW). The sedimentary distributions of authigenic uranium and rhenium reveal reduced oxygen content at intermediate depths (800-1500 m) during the LGM compared to the Holocene. In contrast, data from deeper <span class="hlt">waters</span> (≥1500 m) indicate higher oxygen content during the LGM compared to the Holocene. These data, together with variations in benthic foraminiferal δ13C, are consistent with a shallower AAIW-UCDW boundary over the Campbell Plateau during the LGM. Whilst AAIW continued to bathe the intermediate depths (≤1500 m) of the Challenger Plateau during the LGM, the data suggest that the AAIW at these core sites contained less oxygen compared to the Holocene. These results are at odds with the general notion that AAIW was better oxygenated and expanded deeper during the LGM due to stronger westerlies and colder temperatures. These findings may be explained by an important change in AAIW formation and circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/869665','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/869665"><span>Reactor <span class="hlt">water</span> cleanup system</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Gluntz, Douglas M.; Taft, William E.</p> <p>1994-01-01</p> <p>A reactor <span class="hlt">water</span> cleanup system includes a reactor pressure vessel containing a reactor core submerged in reactor <span class="hlt">water</span>. First and second parallel cleanup trains are provided for extracting portions of the reactor <span class="hlt">water</span> from the pressure vessel, cleaning the extracted <span class="hlt">water</span>, and returning the cleaned <span class="hlt">water</span> to the pressure vessel. Each of the cleanup trains includes a heat exchanger for cooling the reactor <span class="hlt">water</span>, and a cleaner for cleaning the cooled reactor <span class="hlt">water</span>. A return line is disposed between the cleaner and the pressure vessel for channeling the cleaned <span class="hlt">water</span> thereto in a first <span class="hlt">mode</span> of operation. A portion of the cooled <span class="hlt">water</span> is bypassed around the cleaner during a second <span class="hlt">mode</span> of operation and returned through the pressure vessel for shutdown cooling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6890352','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/biblio/6890352"><span>Reactor <span class="hlt">water</span> cleanup system</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Gluntz, D.M.; Taft, W.E.</p> <p>1994-12-20</p> <p>A reactor <span class="hlt">water</span> cleanup system includes a reactor pressure vessel containing a reactor core submerged in reactor <span class="hlt">water</span>. First and second parallel cleanup trains are provided for extracting portions of the reactor <span class="hlt">water</span> from the pressure vessel, cleaning the extracted <span class="hlt">water</span>, and returning the cleaned <span class="hlt">water</span> to the pressure vessel. Each of the cleanup trains includes a heat exchanger for cooling the reactor <span class="hlt">water</span>, and a cleaner for cleaning the cooled reactor <span class="hlt">water</span>. A return line is disposed between the cleaner and the pressure vessel for channeling the cleaned <span class="hlt">water</span> thereto in a first <span class="hlt">mode</span> of operation. A portion of the cooled <span class="hlt">water</span> is bypassed around the cleaner during a second <span class="hlt">mode</span> of operation and returned through the pressure vessel for shutdown cooling. 1 figure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27420911','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27420911"><span>Fabrication of a novel hydrophobic/ion-exchange mixed-<span class="hlt">mode</span> adsorbent for the dispersive solid-phase extraction of chlorophenols from environmental <span class="hlt">water</span> samples.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gao, Li; Wei, Yinmao</p> <p>2016-08-01</p> <p>A novel mixed-<span class="hlt">mode</span> adsorbent was prepared by functionalizing silica with tris(2-aminoethyl)amine and 3-phenoxybenzaldehyde as the main mixed-<span class="hlt">mode</span> scaffold due to the presence of the plentiful amino groups and benzene rings in their molecules. The adsorption mechanism was probed with acidic, natural and basic compounds, and the mixed hydrophobic and ion-exchange interactions were found to be responsible for the adsorption of analytes. The suitability of dispersive solid-phase extraction was demonstrated in the determination of chlorophenols in environmental <span class="hlt">water</span>. Several parameters, including sample pH, desorption solvent, ionic strength, adsorbent dose, and extraction time were optimized. Under the optimal extraction conditions, the proposed dispersive solid-phase extraction coupled with high-performance liquid chromatography showed good linearity range and acceptable limits of detection (0.22∽0.54 ng/mL) for five chlorophenols. Notably, the higher extraction recoveries (88.7∽109.7%) for five chlorophenols were obtained with smaller adsorbent dose (10 mg) and shorter extraction time (15 min) compared with the reported methods. The proposed method might be potentially applied in the determination of trace chlorophenols in real <span class="hlt">water</span> samples. © 2016 WILEY-VCH Verlag GmbH & Co. KGaA, Weinheim.</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1280527','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1280527"><span>Low-frequency collective <span class="hlt">modes</span> in dry and hydrated proteins.</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bellissent-Funel, M C; Teixeira, J; Chen, S H; Dorner, B; Middendorf, H D; Crespi, H L</p> <p>1989-01-01</p> <p>We have observed Brillouin-like low frequency collective <span class="hlt">modes</span> in the scattering of 1 A neutrons from a fully in vivo deuterated protein. These <span class="hlt">modes</span> are tentatively interpreted as due to short-lived coherent excitations propagating with velocities between 2,000 and 4,000 m/s in elements of the secondary structure and patches of closely associated <span class="hlt">water</span>. PMID:2554989</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3219075','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3219075"><span>Recovering Greater Fungal Diversity from Pristine and Diesel Fuel Contaminated <span class="hlt">Sub-Antarctic</span> Soil Through Cultivation Using Both a High and a Low Nutrient Media Approach</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ferrari, Belinda C.; Zhang, Chengdong; van Dorst, Josie</p> <p>2011-01-01</p> <p>Novel cultivation strategies for bacteria are widespread and well described for recovering greater diversity from the “hitherto” unculturable majority. While similar approaches have not yet been demonstrated for fungi it has been suggested that of the 1.5 million estimated species less than 5% have been recovered into pure culture. Fungi are known to be involved in many degradative processes, including the breakdown of petroleum hydrocarbons, and it has been speculated that in Polar Regions they contribute significantly to bioremediation of contaminated soils. Given the biotechnological potential of fungi there is a need to increase efforts for greater species recovery, particularly from extreme environments such as <span class="hlt">sub-Antarctic</span> Macquarie Island. In this study, like the yet-to-be cultured bacteria, high concentrations of nutrients selected for predominantly different fungal species to that recovered using a low nutrient media. By combining both media approaches to the cultivation of fungi from contaminated and non-contaminated soils, 91 fungal species were recovered, including 63 unidentified species. A preliminary biodegradation activity assay on a selection of isolates found that a high proportion of novel and described fungal species from a range of soil samples were capable of hydrocarbon degradation and should be characterized further. PMID:22131985</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27517142','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27517142"><span>Evaluation of genotoxic effects of surface <span class="hlt">waters</span> using a battery of bioassays indicating different <span class="hlt">mode</span> of action.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Han, Yingnan; Li, Na; Oda, Yoshimitsu; Ma, Mei; Rao, Kaifeng; Wang, Zijian; Jin, Wei; Hong, Gang; Li, Zhiguo; Luo, Yi</p> <p>2016-11-01</p> <p>With the burgeoning contamination of surface <span class="hlt">waters</span> threatening human health, the genotoxic effects of surface <span class="hlt">waters</span> have received much attention. Because mutagenic and carcinogenic compounds in <span class="hlt">water</span> cause tumors by different mechanisms, a battery of bioassays that each indicate a different <span class="hlt">mode</span> of action (MOA) is required to evaluate the genotoxic effects of contaminants in <span class="hlt">water</span> samples. In this study, 15 <span class="hlt">water</span> samples from two source <span class="hlt">water</span> reservoirs and surrounding rivers in Shijiazhuang city of China were evaluated for genotoxic effects. Target chemical analyses of 14 genotoxic pollutants were performed according to the Environmental quality standards for surface <span class="hlt">water</span> of China. Then, the in vitro cytokinesis-block micronucleus (CBMN) assay, based on a high-content screening technique, was used to detect the effect of chromosome damage. The SOS/umu test using strain TA1535/pSK1002 was used to detect effects on SOS repair of gene expression. Additionally, two other strains, NM2009 and NM3009, which are highly sensitive to aromatic amines and nitroarenes, respectively, were used in the SOS/umu test to avoid false negative results. In the <span class="hlt">water</span> samples, only two of the genotoxic chemicals listed in the <span class="hlt">water</span> standards were detected in a few samples, with concentrations that were below <span class="hlt">water</span> quality standards. However, positive results for the CBMN assay were observed in two river samples, and positive results for the induction of umuC gene expression in TA1535/pSK1002 were observed in seven river samples. Moreover, positive results were observed for NM2009 with S9 and NM3009 without S9 in some samples that had negative results using the strain TA1535/pSK1002. Based on the results with NM2009 and NM3009, some unknown or undetected aromatic amines and nitroarenes were likely in the source <span class="hlt">water</span> reservoirs and the surrounding rivers. Furthermore, these compounds were most likely the causative pollutants for the genotoxic effect of these <span class="hlt">water</span> samples. Therefore</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptCo.393..244T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptCo.393..244T"><span>Relationship between height and width of resonance peaks in a whispering gallery <span class="hlt">mode</span> resonator immersed in <span class="hlt">water</span> and sucrose solutions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teraoka, Iwao; Yao, Haibei; Huiyi Luo, Natalie</p> <p>2017-06-01</p> <p>We employed a recently developed whispering gallery <span class="hlt">mode</span> (WGM) dip sensor made of silica to obtain spectra for many resonance peaks in <span class="hlt">water</span> and solutions of sucrose at different concentrations and thus having different refractive indices (RI). The apparent Q factor was estimated by fitting each peak profile in the busy resonance spectrum by a Lorentzian or a sum of Lorentzians. A plot of the Q factor as a function the peak height for all the peaks analyzed indicates a straight line with a negative slope as the upper limit, for each of <span class="hlt">water</span> and the solutions. A coupling model for a resonator and a pair of fiber tapers to feed and pick up light, developed here, supports the presence of the upper limit. We also found that the round-trip attenuation of WGM was greater than the one estimated from light absorption by <span class="hlt">water</span>, and the difference increased with the concentration of sucrose.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRC..120.4226K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRC..120.4226K"><span>Decadal and seasonal changes in temperature, salinity, nitrate, and chlorophyll in inshore and offshore <span class="hlt">waters</span> along southeast Australia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kelly, Paige; Clementson, Lesley; Lyne, Vincent</p> <p>2015-06-01</p> <p>Sixty years of oceanographic in situ data at Port Hacking (34°S) and Maria Island (42°S) and 15 years of satellite-derived chlorophyll a (chl a) in inshore and offshore <span class="hlt">waters</span> of southeast Australia show changes in the seasonality and trend of <span class="hlt">water</span> properties consistent with long-term intensification and southerly extensions of East Australian Current (EAC) <span class="hlt">water</span>. Decadal analyses reveal that the EAC extension <span class="hlt">water</span> at Maria Island increased gradually from the 1940s to 1980s, followed by a rapid increase since the 1990s. This acceleration coincided with enhanced winter nitrate, implying increased injections of <span class="hlt">subantarctic</span> <span class="hlt">water</span> at Maria Island. Satellite-derived chl a at six coastal sites and offshore companion sites in the western Tasman Sea showed significant inshore-offshore variations in seasonal cycle and long-term trend. After 2004-2005, the Maria Island seasonal cycle became increasingly similar to those of Bass Strait and St. Helens, suggesting that the EAC extension <span class="hlt">water</span> was extending further southward. Comparative analyses of inshore-offshore sites showed that the presence of EAC extension <span class="hlt">water</span> declined offshore. Seasonal cycles at Maria Island show a recent shift away from the traditional spring bloom, toward increased winter biomass, and enhanced primary productivity consistent with extensions of warm, energetic EAC extension <span class="hlt">water</span> and more frequent injections of cooler, fresher nitrate-replete <span class="hlt">waters</span>. Overall, we find complex temporal, latitudinal, and inshore-offshore changes in multiple <span class="hlt">water</span> masses, particularly at Maria Island, and changes in primary productivity that will profoundly impact fisheries and ecosystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1376289-instantaneous-normal-modes-protein-glass-transition','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1376289-instantaneous-normal-modes-protein-glass-transition"><span>Instantaneous Normal <span class="hlt">Modes</span> and the Protein Glass Transition</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>Schulz, Roland; Krishnan, Marimuthu; Daidone, Isabella</p> <p>2009-01-01</p> <p>In the instantaneous normal <span class="hlt">mode</span> method, normal <span class="hlt">mode</span> analysis is performed at instantaneous configurations of a condensed-phase system, leading to <span class="hlt">modes</span> with negative eigenvalues. These negative <span class="hlt">modes</span> provide a means of characterizing local anharmonicities of the potential energy surface. Here, we apply instantaneous normal <span class="hlt">mode</span> to analyze temperature-dependent diffusive dynamics in molecular dynamics simulations of a small protein (a scorpion toxin). Those characteristics of the negative <span class="hlt">modes</span> are determined that correlate with the dynamical (or glass) transition behavior of the protein, as manifested as an increase in the gradient with T of the average atomic mean-square displacement at ~ 220more » K. The number of negative eigenvalues shows no transition with temperature. Further, although filtering the negative <span class="hlt">modes</span> to retain only those with eigenvectors corresponding to double-well potentials does reveal a transition in the hydration <span class="hlt">water</span>, again, no transition in the protein is seen. However, additional filtering of the protein double-well <span class="hlt">modes</span>, so as to retain only those that, on energy minimization, escape to different regions of configurational space, finally leads to clear protein dynamical transition behavior. Partial minimization of instantaneous configurations is also found to remove nondiffusive imaginary <span class="hlt">modes</span>. In summary, examination of the form of negative instantaneous normal <span class="hlt">modes</span> is shown to furnish a physical picture of local diffusive dynamics accompanying the protein glass transition.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/950825-instantaneous-normal-modes-protein-glass-transition','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/950825-instantaneous-normal-modes-protein-glass-transition"><span>Instantaneous Normal <span class="hlt">Modes</span> and the Protein Glass Transition</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>Schultz, Roland; Krishnan, Marimuthu; Daidone, Isabella</p> <p>2009-01-01</p> <p>In the instantaneous normal <span class="hlt">mode</span> method, normal <span class="hlt">mode</span> analysis is performed at instantaneous configurations of a condensed-phase system, leading to <span class="hlt">modes</span> with negative eigenvalues. These negative <span class="hlt">modes</span> provide a means of characterizing local anharmonicities of the potential energy surface. Here, we apply instantaneous normal <span class="hlt">mode</span> to analyze temperature-dependent diffusive dynamics in molecular dynamics simulations of a small protein (a scorpion toxin). Those characteristics of the negative <span class="hlt">modes</span> are determined that correlate with the dynamical (or glass) transition behavior of the protein, as manifested as an increase in the gradient with T of the average atomic mean-square displacement at 220 K.more » The number of negative eigenvalues shows no transition with temperature. Further, although filtering the negative <span class="hlt">modes</span> to retain only those with eigenvectors corresponding to double-well potentials does reveal a transition in the hydration <span class="hlt">water</span>, again, no transition in the protein is seen. However, additional filtering of the protein double-well <span class="hlt">modes</span>, so as to retain only those that, on energy minimization, escape to different regions of configurational space, finally leads to clear protein dynamical transition behavior. Partial minimization of instantaneous configurations is also found to remove nondiffusive imaginary <span class="hlt">modes</span>. In summary, examination of the form of negative instantaneous normal <span class="hlt">modes</span> is shown to furnish a physical picture of local diffusive dynamics accompanying the protein glass transition.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018Icar..306..200M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018Icar..306..200M"><span>Excitation mechanisms for Jovian seismic <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Markham, Steve; Stevenson, Dave</p> <p>2018-05-01</p> <p>Recent (2011) results from the Nice Observatory indicate the existence of global seismic <span class="hlt">modes</span> on Jupiter in the frequency range between 0.7 and 1.5 mHz with amplitudes of tens of cm/s. Currently, the driving force behind these <span class="hlt">modes</span> is a mystery; the measured amplitudes are many orders of magnitude larger than anticipated based on theory analogous to helioseismology (that is, turbulent convection as a source of stochastic excitation). One of the most promising hypotheses is that these <span class="hlt">modes</span> are driven by Jovian storms. This work constructs a framework to analytically model the expected equilibrium normal <span class="hlt">mode</span> amplitudes arising from convective columns in storms. We also place rough constraints on Jupiter's seismic modal quality factor. Using this model, neither meteor strikes, turbulent convection, nor <span class="hlt">water</span> storms can feasibly excite the order of magnitude of observed amplitudes. Next we speculate about the potential role of rock storms deeper in Jupiter's atmosphere, because the rock storms' expected energy scales make them promising candidates to be the chief source of excitation for Jovian seismic <span class="hlt">modes</span>, based on simple scaling arguments. We also suggest some general trends in the expected partition of energy between different frequency <span class="hlt">modes</span>. Finally we supply some commentary on potential applications to gravity, Juno, Cassini and Saturn, and future missions to Uranus and Neptune.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptCo.383..525R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptCo.383..525R"><span>Three-<span class="hlt">mode</span> <span class="hlt">mode</span>-division-multiplexing passive optical network over 12-km low <span class="hlt">mode</span>-crosstalk FMF using all-fiber <span class="hlt">mode</span> MUX/DEMUX</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Fang; Li, Juhao; Wu, Zhongying; Hu, Tao; Yu, Jinyi; Mo, Qi; He, Yongqi; Chen, Zhangyuan; Li, Zhengbin</p> <p>2017-01-01</p> <p>We propose three-<span class="hlt">mode</span> <span class="hlt">mode</span>-division-multiplexing passive optical network (MDM-PON) based on low <span class="hlt">mode</span>-crosstalk few-<span class="hlt">mode</span> fiber (FMF) and all-fiber <span class="hlt">mode</span> multiplexer/demultiplexer (MUX/DEMUX). The FMF with step-index profile is designed and fabricated for effectively three-independent-spatial-<span class="hlt">mode</span> transmission and low <span class="hlt">mode</span>-crosstalk for MDM-PON transmission. The all-fiber <span class="hlt">mode</span> MUX/DEMUX are composed of cascaded <span class="hlt">mode</span> selective couplers (MSCs), which simultaneously multiplex or demultiplex multiple <span class="hlt">modes</span>. Based on the low <span class="hlt">mode</span>-crosstalk of the FMF and all-fiber <span class="hlt">mode</span> MUX/DEMUX, each optical network unit (ONU) communicates with the optical line terminal (OLT) independently utilizing a different optical linearly polarized (LP) spatial <span class="hlt">mode</span> in MDM-PON system. We experimentally demonstrate MDM-PON transmission of three independent-spatial-<span class="hlt">modes</span> over 12-km FMF with 10-Gb/s optical on-off keying (OOK) signal and direct detection.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26896669','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26896669"><span>Penguins as bioindicators of mercury contamination in the southern Indian Ocean: geographical and temporal trends.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carravieri, Alice; Cherel, Yves; Jaeger, Audrey; Churlaud, Carine; Bustamante, Paco</p> <p>2016-06-01</p> <p>Penguins have been recently identified as useful bioindicators of mercury (Hg) transfer to food webs in the Southern Ocean over different spatial and temporal scales. Here, feather Hg concentrations were measured in adults and chicks of all the seven penguin species breeding in the southern Indian Ocean, over a large latitudinal gradient spanning Antarctic, <span class="hlt">subantarctic</span> and subtropical sites. Hg was also measured in feathers of museum specimens of penguins collected at the same sites in the 1950s and 1970s. Our aim was to evaluate geographical and historical variations in Hg transfer to penguins, while accounting for feeding habits by using the stable isotope technique (δ(13)C, habitat; δ(15)N, diet/trophic level). Adult feather Hg concentrations in contemporary individuals ranged from 0.7 ± 0.2 to 5.9 ± 1.9 μg g(-1) dw in Adélie and gentoo penguins, respectively. Inter-specific differences in Hg accumulation were strong among both adults and chicks, and mainly linked to feeding habits. Overall, penguin species that feed in Antarctic <span class="hlt">waters</span> had lower feather Hg concentrations than those that feed in <span class="hlt">subantarctic</span> and subtropical <span class="hlt">waters</span>, irrespective of age class and dietary group, suggesting different Hg incorporation into food webs depending on the <span class="hlt">water</span> mass. While accounting for feeding habits, we detected different temporal variations in feather Hg concentrations depending on species. Notably, the <span class="hlt">subantarctic</span> gentoo and macaroni penguins had higher Hg burdens in the contemporary rather than in the historical sample, despite similar or lower trophic levels, respectively. Whereas increases in Hg deposition have been recently documented in the Southern Hemisphere, future monitoring is highly needed to confirm or not this temporal trend in penguins, especially in the context of actual changing Hg emission patterns and global warming. Copyright © 2016. Published by Elsevier Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMPP23D2084D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMPP23D2084D"><span>Eastern South Pacific <span class="hlt">water</span> mass geometry during the last glacial-interglacial transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De Pol-Holz, R.; Reyes, D.; Mohtadi, M.</p> <p>2012-12-01</p> <p>The eastern South Pacific is characterized today by a complex thermocline structure where large salinity and oxygen changes as a function of depth coexist. Surface <span class="hlt">waters</span> from tropical origin float on top of <span class="hlt">subantarctic</span> fresher <span class="hlt">water</span> (the so-called 'shallow salinity minimum of the eastern south Pacific'), which in turn, flow above aged equatorial and deeper recently ventilated Antarctic Intermediate <span class="hlt">waters</span>. Little is known however about the <span class="hlt">water</span> mass geometry changes that could have occurred during the last glacial maximum boundary conditions (about 20,000 years before the present), despite this information being critical for the assessment of potential mechanisms that have been proposed as explanations for the deglacial onset of low oxygen conditions in the area and the atmospheric CO2 increase during the same time. Here we present benthic and planktonic foraminifera stable isotope and radiocarbon data from a set of sediment cores from the Chilean continental margin covering a large -yet still limited- geographical area and depth range. Sedimentations rates were relatively high (>10 cm/kyr) precluding major caveats from bioturbation in all of our archives. The distribution of δ13C of ΣCO2 shows the presence of a very depleted (δ13C < -1‰ V-PDB) <span class="hlt">water</span> mass overlaying more recently ventilated <span class="hlt">waters</span> at intermediate depths as indicated by thermocline foraminifer dwellers being more depleted in 13C than the benthic species. The origin of this depleted end-member is probably upwelling from the Southern Ocean as expressed by the radiocarbon content and the large reservoir effect associated with the last glacial maximum and the beginning of the deglaciation along the margin. Our data suggest that the Tropical <span class="hlt">waters</span> that today bath the lower latitude cores was displaced by surface <span class="hlt">waters</span> of southern origin and therefore in line with the evidence of a latitudinal shift of the frontal systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25375329','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25375329"><span>Satellite tagging and biopsy sampling of killer whales at <span class="hlt">subantarctic</span> Marion Island: effectiveness, immediate reactions and long-term responses.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Reisinger, Ryan R; Oosthuizen, W Chris; Péron, Guillaume; Cory Toussaint, Dawn; Andrews, Russel D; de Bruyn, P J Nico</p> <p>2014-01-01</p> <p>Remote tissue biopsy sampling and satellite tagging are becoming widely used in large marine vertebrate studies because they allow the collection of a diverse suite of otherwise difficult-to-obtain data which are critical in understanding the ecology of these species and to their conservation and management. Researchers must carefully consider their methods not only from an animal welfare perspective, but also to ensure the scientific rigour and validity of their results. We report methods for shore-based, remote biopsy sampling and satellite tagging of killer whales Orcinus orca at <span class="hlt">Subantarctic</span> Marion Island. The performance of these methods is critically assessed using 1) the attachment duration of low-impact minimally percutaneous satellite tags; 2) the immediate behavioural reactions of animals to biopsy sampling and satellite tagging; 3) the effect of researcher experience on biopsy sampling and satellite tagging; and 4) the mid- (1 month) and long- (24 month) term behavioural consequences. To study mid- and long-term behavioural changes we used multievent capture-recapture models that accommodate imperfect detection and individual heterogeneity. We made 72 biopsy sampling attempts (resulting in 32 tissue samples) and 37 satellite tagging attempts (deploying 19 tags). Biopsy sampling success rates were low (43%), but tagging rates were high with improved tag designs (86%). The improved tags remained attached for 26±14 days (mean ± SD). Individuals most often showed no reaction when attempts missed (66%) and a slight reaction-defined as a slight flinch, slight shake, short acceleration, or immediate dive-when hit (54%). Severe immediate reactions were never observed. Hit or miss and age-sex class were important predictors of the reaction, but the method (tag or biopsy) was unimportant. Multievent trap-dependence modelling revealed considerable variation in individual sighting patterns; however, there were no significant mid- or long-term changes following</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4222950','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4222950"><span>Satellite Tagging and Biopsy Sampling of Killer Whales at <span class="hlt">Subantarctic</span> Marion Island: Effectiveness, Immediate Reactions and Long-Term Responses</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Reisinger, Ryan R.; Oosthuizen, W. Chris; Péron, Guillaume; Cory Toussaint, Dawn; Andrews, Russel D.; de Bruyn, P. J. Nico</p> <p>2014-01-01</p> <p>Remote tissue biopsy sampling and satellite tagging are becoming widely used in large marine vertebrate studies because they allow the collection of a diverse suite of otherwise difficult-to-obtain data which are critical in understanding the ecology of these species and to their conservation and management. Researchers must carefully consider their methods not only from an animal welfare perspective, but also to ensure the scientific rigour and validity of their results. We report methods for shore-based, remote biopsy sampling and satellite tagging of killer whales Orcinus orca at <span class="hlt">Subantarctic</span> Marion Island. The performance of these methods is critically assessed using 1) the attachment duration of low-impact minimally percutaneous satellite tags; 2) the immediate behavioural reactions of animals to biopsy sampling and satellite tagging; 3) the effect of researcher experience on biopsy sampling and satellite tagging; and 4) the mid- (1 month) and long- (24 month) term behavioural consequences. To study mid- and long-term behavioural changes we used multievent capture-recapture models that accommodate imperfect detection and individual heterogeneity. We made 72 biopsy sampling attempts (resulting in 32 tissue samples) and 37 satellite tagging attempts (deploying 19 tags). Biopsy sampling success rates were low (43%), but tagging rates were high with improved tag designs (86%). The improved tags remained attached for 26±14 days (mean ± SD). Individuals most often showed no reaction when attempts missed (66%) and a slight reaction–defined as a slight flinch, slight shake, short acceleration, or immediate dive–when hit (54%). Severe immediate reactions were never observed. Hit or miss and age-sex class were important predictors of the reaction, but the method (tag or biopsy) was unimportant. Multievent trap-dependence modelling revealed considerable variation in individual sighting patterns; however, there were no significant mid- or long-term changes following</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24216801','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24216801"><span>Two-<span class="hlt">mode</span> PLC-based <span class="hlt">mode</span> multi/demultiplexer for <span class="hlt">mode</span> and wavelength division multiplexed transmission.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hanzawa, Nobutomo; Saitoh, Kuimasa; Sakamoto, Taiji; Matsui, Takashi; Tsujikawa, Kyozo; Koshiba, Masanori; Yamamoto, Fumihiko</p> <p>2013-11-04</p> <p>We proposed a PLC-based <span class="hlt">mode</span> multi/demultiplexer (MUX/DEMUX) with an asymmetric parallel waveguide for <span class="hlt">mode</span> division multiplexed (MDM) transmission. The <span class="hlt">mode</span> MUX/DEMUX including a <span class="hlt">mode</span> conversion function with an asymmetric parallel waveguide can be realized by matching the effective indices of the LP(01) and LP(11) <span class="hlt">modes</span> of two waveguides. We report the design of a <span class="hlt">mode</span> MUX/DEMUX that can support C-band WDM-MDM transmission. The fabricated <span class="hlt">mode</span> MUX/DEMUX realized a low insertion loss of less than 1.3 dB and high a <span class="hlt">mode</span> extinction ratio that exceeded 15 dB. We used the fabricated <span class="hlt">mode</span> MUX/DEMUX to achieve a successful 2 <span class="hlt">mode</span> x 4 wavelength x 10 Gbps transmission over a 9 km two-<span class="hlt">mode</span> fiber with a penalty of less than 1 dB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMPP23A1376G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMPP23A1376G"><span>Ventilation of the deep Southern Ocean and changes in atmospheric CO2 during the last deglacial and glacial periods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gottschalk, J.; Skinner, L. C.; Lippold, J. A.; Jaccard, S.; Vogel, H.; Frank, N.; Waelbroeck, C.</p> <p>2014-12-01</p> <p>The Southern Ocean is thought to have played a key role in atmospheric CO2 (CO2,atm) variations, both via its role in bringing carbon-rich deep-<span class="hlt">waters</span> into contact with the atmosphere, and via its capacity for enhanced biologically mediated carbon export into the deep sea. The governing mechanisms of millennial scale rises in CO2,atm during the last deglacial and glacial periods have been linked controversially either with variations in biological export productivity, possibly driven by fluctuations in airborne dust supply, or to variations in southern high-latitude vertical mixing, possibly driven by changes in westerly wind stress or density stratification across the Southern Ocean <span class="hlt">water</span> column. However, the impact of these processes on deep, southern high-latitude carbon sequestration and ocean-atmosphere CO2 exchange remain ambiguous. We present proxy evidence for the link between deep carbon storage in the <span class="hlt">sub-Antarctic</span> Atlantic with changes in CO2,atm during the last 70 ka from sub-millennially resolved changes in bottom <span class="hlt">water</span> oxygenation based on the uranium accumulation in authigenic coatings on foraminiferal shells and the δ13C offset between epibenthic and infaunal foraminifera (Δδ13C). We compare our results with reconstructed opal fluxes and sediment model output data to assess the impact of physical and biological processes on Southern Ocean carbon storage. While variations in <span class="hlt">sub-Antarctic</span> Atlantic export production are intrinsically linked with changes in airborne dust supply supporting the major impact of dust on the biological soft-tissue pump, they cannot account for observed changes in pore <span class="hlt">water</span> organic carbon respiration indicated by increasing Δδ13C and therefore, bottom <span class="hlt">water</span> oxygen changes in the deep <span class="hlt">sub-Antarctic</span> Atlantic. This is in strong support of millennial-scale fluctuations in deep Southern Ocean carbon storage primarily controlled by the ventilation of the deep ocean by southern-sourced <span class="hlt">water</span> masses, which emphasize the strong</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28592891','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28592891"><span>Dynamic Triple-<span class="hlt">Mode</span> Sorption and Outgassing in Materials.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sharma, Hom N; Harley, Stephen J; Sun, Yunwei; Glascoe, Elizabeth A</p> <p>2017-06-07</p> <p>Moisture uptake and outgassing can be detrimental to a system by altering the chemical and mechanical properties of materials within the system over time. In this work, we conducted isotherm experiments to investigate dynamic moisture sorption and desorption in markedly different materials, i.e., a polymeric material, Sylgard-184 and a ceramic aluminosilicate material, Zircar RS-1200, at different temperatures (30 °C-70 °C) by varying the <span class="hlt">water</span> activity (0.0-0.90). Sylgard-184 showed a linear sorption and outgassing behavior with no-hysteresis over the entire temperature and <span class="hlt">water</span> activity range considered here. Whereas, the sorption and outgassing of Zircar RS-1200 was highly non-linear with significant hysteresis, especially at higher <span class="hlt">water</span> activities, at all temperatures considered here. The type of hysteresis suggested the presence of mesopores in Zircar RS-1200, whereas the lack of hysteresis in Sylgard-184 indicates that it has a nonporous structure. A diffusion model coupled with a dynamic, triple-<span class="hlt">mode</span> sorption (Langmuir, Henry, and pooling <span class="hlt">modes</span>) model employed in this study matched our experimental data very well and provides mechanistic insight into the processes. Our triple-<span class="hlt">mode</span> sorption model was adaptive enough to (1) model these distinctly different materials and (2) predict sorption and outgassing under conditions that are distinctly different from the parameterization experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1395470-dynamic-triple-mode-sorption-outgassing-materials','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1395470-dynamic-triple-mode-sorption-outgassing-materials"><span>Dynamic Triple-<span class="hlt">Mode</span> Sorption and Outgassing in Materials</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Sharma, Hom N.; Harley, Stephen J.; Sun, Yunwei; ...</p> <p>2017-06-07</p> <p>Moisture uptake and outgassing can be detrimental to a system by altering the chemical and mechanical properties of materials within the system over time. In this work, we conducted isotherm experiments to investigate dynamic moisture sorption and desorption in markedly different materials, i.e., a polymeric material, Sylgard-184 and a ceramic aluminosilicate material, Zircar RS-1200, at different temperatures (30 °C–70 °C) by varying the <span class="hlt">water</span> activity (0.0–0.90). Sylgard-184 showed a linear sorption and outgassing behavior with no-hysteresis over the entire temperature and <span class="hlt">water</span> activity range considered here. Whereas, the sorption and outgassing of Zircar RS-1200 was highly non-linear with significant hysteresis,more » especially at higher <span class="hlt">water</span> activities, at all temperatures considered here. The type of hysteresis suggested the presence of mesopores in Zircar RS-1200, whereas the lack of hysteresis in Sylgard-184 indicates that it has a nonporous structure. A diffusion model coupled with a dynamic, triple-<span class="hlt">mode</span> sorption (Langmuir, Henry, and pooling <span class="hlt">modes</span>) model employed in this study matched our experimental data very well and provides mechanistic insight into the processes. Our triple-<span class="hlt">mode</span> sorption model was adaptive enough to (1) model these distinctly different materials and (2) predict sorption and outgassing under conditions that are distinctly different from the parameterization experiments.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1395470','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1395470"><span>Dynamic Triple-<span class="hlt">Mode</span> Sorption and Outgassing in Materials</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>Sharma, Hom N.; Harley, Stephen J.; Sun, Yunwei</p> <p></p> <p>Moisture uptake and outgassing can be detrimental to a system by altering the chemical and mechanical properties of materials within the system over time. In this work, we conducted isotherm experiments to investigate dynamic moisture sorption and desorption in markedly different materials, i.e., a polymeric material, Sylgard-184 and a ceramic aluminosilicate material, Zircar RS-1200, at different temperatures (30 °C–70 °C) by varying the <span class="hlt">water</span> activity (0.0–0.90). Sylgard-184 showed a linear sorption and outgassing behavior with no-hysteresis over the entire temperature and <span class="hlt">water</span> activity range considered here. Whereas, the sorption and outgassing of Zircar RS-1200 was highly non-linear with significant hysteresis,more » especially at higher <span class="hlt">water</span> activities, at all temperatures considered here. The type of hysteresis suggested the presence of mesopores in Zircar RS-1200, whereas the lack of hysteresis in Sylgard-184 indicates that it has a nonporous structure. A diffusion model coupled with a dynamic, triple-<span class="hlt">mode</span> sorption (Langmuir, Henry, and pooling <span class="hlt">modes</span>) model employed in this study matched our experimental data very well and provides mechanistic insight into the processes. Our triple-<span class="hlt">mode</span> sorption model was adaptive enough to (1) model these distinctly different materials and (2) predict sorption and outgassing under conditions that are distinctly different from the parameterization experiments.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRC..122.1232M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRC..122.1232M"><span>Regional modeling of the <span class="hlt">water</span> masses and circulation annual variability at the Southern Brazilian Continental Shelf</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mendonça, L. F.; Souza, R. B.; Aseff, C. R. C.; Pezzi, L. P.; Möller, O. O.; Alves, R. C. M.</p> <p>2017-02-01</p> <p>The Southern Brazilian Continental Shelf (SBCS) is one of the more productive areas for fisheries in Brazilian <span class="hlt">waters</span>. The <span class="hlt">water</span> masses and the dynamical processes of the region present a very seasonal behavior that imprint strong effects in the ecosystem and the weather of the area and its vicinity. This paper makes use of the Regional Ocean Modeling System (ROMS) for studying the <span class="hlt">water</span> mass distribution and circulation variability in the SBCS during the year of 2012. Model outputs were compared to in situ, historical observations and to satellite data. The model was able to reproduce the main thermohaline characteristics of the <span class="hlt">waters</span> dominating the SBCS and the adjacent region. The mixing between the <span class="hlt">Subantarctic</span> Shelf <span class="hlt">Water</span> and the Subtropical Shelf <span class="hlt">Water</span>, known as the Subtropical Shelf Front (STSF), presented a clear seasonal change in volume. As a consequence of the mixing and of the seasonal oscillation of the STSF position, the stability of the <span class="hlt">water</span> column inside the SBCS also changes seasonally. Current velocities and associated transports estimated for the Brazil Current (BC) and for the Brazilian Coastal Current (BCC) agree with previous measurements and estimates, stressing the fact that the opposite flow of the BCC occurring during winter in the study region is about 2 orders of magnitude smaller than that of the BC. Seasonal maps of simulated Mean Kinetic Energy and Eddy Kinetic Energy demonstrate the known behavior of the BC and stressed the importance of the mean coastal flow off Argentina throughout the year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70156091','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70156091"><span><span class="hlt">Water</span> masses, ocean fronts, and the structure of Antarctic seabird communities: putting the eastern Bellingshausen Sea in perspective</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ribic, Christine A.; Ainley, David G.; Ford, R. Glenn; Fraser, William R.; Tynan, Cynthia T.; Woehler, Eric J.</p> <p>2015-01-01</p> <p><span class="hlt">Waters</span> off the western Antarctic Peninsula (i.e., the eastern Bellingshausen Sea) are unusually complex owing to the convergence of several major fronts. Determining the relative influence of fronts on occurrence patterns of top-trophic species in that area, therefore, has been challenging. In one of the few ocean-wide seabird data syntheses, in this case for the Southern Ocean, we analyzed ample, previously collected cruise data, Antarctic-wide, to determine seabird species assemblages and quantitative relationships to fronts as a way to provide context to the long-term Palmer LTER and the winter Southern Ocean GLOBEC studies in the eastern Bellingshausen Sea. Fronts investigated during both winter (April–September) and summer (October–March) were the southern boundary of the Antarctic Circumpolar Current (ACC), which separates the High Antarctic from the Low Antarctic <span class="hlt">water</span> mass, and within which are embedded the marginal ice zone and Antarctic Shelf Break Front; and the Antarctic Polar Front, which separates the Low Antarctic and the <span class="hlt">Subantarctic</span> <span class="hlt">water</span> masses. We used clustering to determine species' groupings with <span class="hlt">water</span> masses, and generalized additive models to relate species' densities, biomass and diversity to distance to respective fronts. Antarctic-wide, in both periods, highest seabird densities and lowest species diversity were found in the High Antarctic <span class="hlt">water</span> mass. In the eastern Bellingshausen, seabird density in the High Antarctic <span class="hlt">water</span> mass was lower (as low as half that of winter) than found in other Antarctic regions. During winter, Antarctic-wide, two significant species groups were evident: one dominated by Adélie penguins (Pygoscelis adeliae) (High Antarctic <span class="hlt">water</span> mass) and the other by petrels and prions (no differentiation among <span class="hlt">water</span> masses); in eastern Bellingshausen <span class="hlt">waters</span> during winter, the one significant species group was composed of species from both Antarctic-wide groups. In summer, Antarctic-wide, a High Antarctic group</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/2018OptCo.410..112W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptCo.410..112W"><span>Fundamental-<span class="hlt">mode</span> MMF transmission enabled by <span class="hlt">mode</span> conversion</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wu, Zhongying; Li, Juhao; Tian, Yu; Ge, Dawei; Zhu, Jinglong; Ren, Fang; Mo, Qi; Yu, Jinyi; Li, Zhengbin; Chen, Zhangyuan; He, Yongqi</p> <p>2018-03-01</p> <p>Modal dispersion in conventional multi-<span class="hlt">mode</span> fiber (MMF) will cause serious signal degradation and an effective solution is to restrict the signal transmission in the fundamental <span class="hlt">mode</span> of MMF. In this paper, unlike previous methods by filtering out higher-order <span class="hlt">modes</span>, we propose to adopt low-modal-crosstalk <span class="hlt">mode</span> converters to realize fundamental-<span class="hlt">mode</span> MMF transmission. We design and fabricate all-fiber <span class="hlt">mode</span>-selective couplers (MSC), which perform <span class="hlt">mode</span> conversion between the fundamental <span class="hlt">mode</span> in single-<span class="hlt">mode</span> fiber (SMF) and fundamental <span class="hlt">mode</span> in MMF. The proposed scheme is experimentally compared with center launching method under different MMF links and then its wavelength division multiplexing (WDM) transmission performance is investigated. Experimental results indicate that the proposed <span class="hlt">mode</span> conversion scheme could achieve better transmission performance and works well for the whole C-band.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004DSRII..51..513P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004DSRII..51..513P"><span>Distribution of siphonophores, chaetognaths, euphausiids and oceanographic conditions in the fjords and channels of southern Chile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Palma, Sergio; Silva, Nelson</p> <p>2004-03-01</p> <p>Interior <span class="hlt">waters</span> of the fjords and channels of southern Chile (41.5°S-56°S) receive inputs of <span class="hlt">Subantarctic</span> <span class="hlt">Water</span>, Equatorial Subsuperficial <span class="hlt">Water</span> and Western Pacific Subsurface <span class="hlt">Water</span> from the adjacent Pacific Ocean by means of numerous connecting channels that lead inward from the ocean margin. These <span class="hlt">waters</span> become mixed in the interior zone with freshwater from precipitation, river flow, and meltwater from cordilleran glaciers. A two-layered positive estuarine circulation becomes established, with a superficial layer having a net movement towards the adjacent ocean, and a deep layer with net movement towards the fjords. The biomass of the interior <span class="hlt">waters</span> is composed principally of planktonic crustaceans (copepods and euphausiids), chaetognaths, and gelatinous carnivores. In a southerly direction, decreases are observed in biomass, in relative abundance, and in species diversity of siphonophores, chaetognaths, and euphausiids. Only a few species have been able to adapt successfully to the extreme oceanographic conditions typical of the region, reflected in dominant monospecific populations such as Muggiaea atlantica, Sagitta tasmanica, and Euphausia vallentini. The zooplankton fauna of interior <span class="hlt">waters</span>, characterized by its low degree of specific richness, is made up of a mixture of species typical of <span class="hlt">Subantarctic</span> <span class="hlt">Water</span> (Sagitta tasmanica, S. decipiens, Euphausia lucens, Nematoscelis megalops, Thysanoessa gregaria), antarctic <span class="hlt">water</span> (Pyrosthephos vanhoeffeni, Dimophyes arctica, Sagitta marri, S. gazellae, Eukrohnia hamata, E. bathyantarctica, Euphausia vallentini), temperate and warm epipelagic <span class="hlt">waters</span> (Eudoxoides spiralis, Lensia conoidea, Chelophyes appendiculata, Muggiaea atlantica, Sphaeronectes gracilis, S. fragilis, Abylopsis tetragona, Sagitta enflata), and mesopelagic <span class="hlt">water</span> (Physophora hydrostatica, Stylocheiron maximum, Vogtia pentacantha, V. serrata).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=reasons+AND+breaking&pg=5&id=ED178304','ERIC'); return false;" href="https://eric.ed.gov/?q=reasons+AND+breaking&pg=5&id=ED178304"><span>Response <span class="hlt">Mode</span> Effects on Computer Based Problem Solving. Report Series 1979.</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>Brown, Bobby R.; Sustik, Joan M.</p> <p></p> <p>This response <span class="hlt">mode</span> study attempts to determine whether different response <span class="hlt">modes</span> are helpful or not in facilitating the thought process in a given problem solving situation. The Luchins <span class="hlt">Water</span> Jar Test (WJT) used in this study illustrates the phenomena "Einstelling" (mechanization of response) because it does not require any specialized content…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007PhRvE..75b1504H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007PhRvE..75b1504H"><span>Slow relaxation <span class="hlt">mode</span> in concentrated oil-in-<span class="hlt">water</span> microemulsions consisting of repulsive droplets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hattori, Y.; Ushiki, H.; Courbin, L.; Panizza, P.</p> <p>2007-02-01</p> <p>The present contribution reports on the observation of two diffusive relaxation <span class="hlt">modes</span> in a concentrated microemulsion made of repulsive droplets. These two <span class="hlt">modes</span> can be interpreted in the frame of Weissman’s and Pusey’s theoretical pioneering works. The fast <span class="hlt">mode</span> is associated to the collective diffusion of droplets whereas the slow one corresponds to the relaxation of droplet concentration fluctuations associated with composition and/or size. We show that (i) repulsive interactions considerably slow down the latter and (ii) a generalized Stokes Einstein relationship between its coefficient of diffusion and the Newtonian viscosity of the solutions, similar to the Walden’s rule for electrolytes, holds for concentrated microemulsion systems made of repulsive droplets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptFT..35...80S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptFT..35...80S"><span>PLC-based <span class="hlt">mode</span> multi/demultiplexers for <span class="hlt">mode</span> division multiplexing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saitoh, Kunimasa; Hanzawa, Nobutomo; Sakamoto, Taiji; Fujisawa, Takeshi; Yamashita, Yoko; Matsui, Takashi; Tsujikawa, Kyozo; Nakajima, Kazuhide</p> <p>2017-02-01</p> <p>Recently developed PLC-based <span class="hlt">mode</span> multi/demultiplexers (MUX/DEMUXs) for <span class="hlt">mode</span> division multiplexing (MDM) transmission are reviewed. We firstly show the operation principle and basic characteristics of PLC-based MUX/DEMUXs with an asymmetric directional coupler (ADC). We then demonstrate the 3-<span class="hlt">mode</span> (2LP-<span class="hlt">mode</span>) multiplexing of the LP01, LP11a, and LP11b <span class="hlt">modes</span> by using fabricated PLC-based <span class="hlt">mode</span> MUX/DEMUX on one chip. In order to excite LP11b <span class="hlt">mode</span> in the same plane, a PLC-based LP11 <span class="hlt">mode</span> rotator is introduced. Finally, we show the PLC-based 6-<span class="hlt">mode</span> (4LP-<span class="hlt">mode</span>) MUX/DEMUX with a uniform height by using ADCs, LP11 <span class="hlt">mode</span> rotators, and tapered waveguides. It is shown that the LP21a <span class="hlt">mode</span> can be excited from the LP11b <span class="hlt">mode</span> by using ADC, and the two nearly degenerated LP21b and LP02 <span class="hlt">modes</span> can be (de)multiplexed separately by using tapered <span class="hlt">mode</span> converter from E13 (E31) <span class="hlt">mode</span> to LP21b (LP02) <span class="hlt">mode</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25835902','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25835902"><span><span class="hlt">Mode</span> coupling at connectors in <span class="hlt">mode</span>-division multiplexed transmission over few-<span class="hlt">mode</span> fiber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vuong, Jordi; Ramantanis, Petros; Frignac, Yann; Salsi, Massimiliano; Genevaux, Philippe; Bendimerad, Djalal F; Charlet, Gabriel</p> <p>2015-01-26</p> <p>In <span class="hlt">mode</span>-division multiplexed (MDM) transmission systems, <span class="hlt">mode</span> coupling is responsible for inter-modal crosstalk. We consider the transmission of modulated signals over a few-<span class="hlt">mode</span> fiber (FMF) having low <span class="hlt">mode</span> coupling and large differential <span class="hlt">mode</span> group delay in the presence of a non-ideal fiber connection responsible for extra <span class="hlt">mode</span> coupling. In this context, we first analytically derive the coupling matrix of the multimode connector and we numerically study the dependence of the matrix coefficients as a function of the butt-joint connection characteristics. The numerical results are then validated through an experiment with a five-<span class="hlt">mode</span> setup. Finally, through numerical simulations, we assess the impact of the connector on the signal quality investigating different receiver digital signal processing (DSP) schemes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22329151','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22329151"><span>Assessing acute toxicity of effluent from a textile industry and nearby river <span class="hlt">waters</span> using sulfur-oxidizing bacteria in continuous <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gurung, Anup; Hassan, Sedky H A; Oh, Sang-Eun</p> <p>2011-10-01</p> <p>Bioassays are becoming an important tool for assessing the toxicity of complex mixtures of substances in aquatic environments in which Daphnia magna is routinely used as a test organism. Bioassays outweigh physicochemical analyses and are valuable in the decision-making process pertaining to the final discharge of effluents from wastewater treatment plants as they measure the total effect of the discharge which is ecologically relevant. In this study, the aquatic toxicity of a textile plant effluent and river <span class="hlt">water</span> downstream from the plant were evaluated with sulfur-oxidizing bacterial biosensors in continuous <span class="hlt">mode</span>. Collected samples were analysed for different physicochemical parameters and 1,4-dioxane was detected in the effluent. The effluent contained a relatively high chemical oxygen demand of 60 mg L(-1), which exceeded the limit set by the Korean government for industrial effluent discharges. Results showed that both the effluent and river <span class="hlt">waters</span> were toxic to sulfur-oxidizing bacteria. These results show the importance of incorporating bioassays to detect toxicity in wastewater effluents for the sustainable management of <span class="hlt">water</span> resources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19045637','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19045637"><span>Acoustic <span class="hlt">mode</span> coupling induced by shallow <span class="hlt">water</span> nonlinear internal waves: sensitivity to environmental conditions and space-time scales of internal waves.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Colosi, John A</p> <p>2008-09-01</p> <p>While many results have been intuited from numerical simulation studies, the precise connections between shallow-<span class="hlt">water</span> acoustic variability and the space-time scales of nonlinear internal waves (NLIWs) as well as the background environmental conditions have not been clearly established analytically. Two-dimensional coupled <span class="hlt">mode</span> propagation through NLIWs is examined using a perturbation series solution in which each order n is associated with nth-order multiple scattering. Importantly, the perturbation solution gives resonance conditions that pick out specific NLIW scales that cause coupling, and seabed attenuation is demonstrated to broaden these resonances, fundamentally changing the coupling behavior at low frequency. Sound-speed inhomogeneities caused by internal solitary waves (ISWs) are primarily considered and the dependence of <span class="hlt">mode</span> coupling on ISW amplitude, range width, depth structure, location relative to the source, and packet characteristics are delineated as a function of acoustic frequency. In addition, it is seen that significant energy transfer to <span class="hlt">modes</span> with initially low or zero energy involves at least a second order scattering process. Under moderate scattering conditions, comparisons of first order, single scattering theoretical predictions to direct numerical simulation demonstrate the accuracy of the approach for acoustic frequencies upto 400 Hz and for single as well as multiple ISW wave packets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008JPhCS.100e2021N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008JPhCS.100e2021N"><span>Tapping <span class="hlt">mode</span> SPM local oxidation nanolithography with sub-10 nm resolution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nishimura, S.; Ogino, T.; Takemura, Y.; Shirakashi, J.</p> <p>2008-03-01</p> <p>Tapping <span class="hlt">mode</span> SPM local oxidation nanolithography with sub-10 nm resolution is investigated by optimizing the applied bias voltage (V), scanning speed (S) and the oscillation amplitude of the cantilever (A). We fabricated Si oxide wires with an average width of 9.8 nm (V = 17.5 V, S = 250 nm/s, A = 292 nm). In SPM local oxidation with tapping <span class="hlt">mode</span> operation, it is possible to decrease the size of the <span class="hlt">water</span> meniscus by enhancing the oscillation amplitude of cantilever. Hence, it seems that the <span class="hlt">water</span> meniscus with sub-10 nm dimensions could be formed by precisely optimizing the oxidation conditions. Moreover, we quantitatively explain the size (width and height) of Si oxide wires with a model based on the oxidation ratio, which is defined as the oxidation time divided by the period of the cantilever oscillation. The model allows us to understand the mechanism of local oxidation in tapping <span class="hlt">mode</span> operation with amplitude modulation. The results imply that the sub-10 nm resolution could be achieved using tapping <span class="hlt">mode</span> SPM local oxidation technique with the optimization of the cantilever dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013OptCo.306..185X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013OptCo.306..185X"><span>Optimization of few-<span class="hlt">mode</span>-fiber based <span class="hlt">mode</span> converter for <span class="hlt">mode</span> division multiplexing transmission</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, Yiwei; Fu, Songnian; Zhang, Minming; Tang, M.; Shum, P.; Liu, Deming</p> <p>2013-10-01</p> <p>Few-<span class="hlt">mode</span>-fiber (FMF) based <span class="hlt">mode</span> division multiplexing (MDM) is a promising technique to further increase the transmission capacity of single <span class="hlt">mode</span> fibers. We propose and numerically investigate a fiber-optical <span class="hlt">mode</span> converter (MC) using long period gratings (LPGs) fabricated on the FMF by point-by-point CO2 laser inscription technique. In order to precisely excite three <span class="hlt">modes</span> (LP01, LP11, and LP02), both untilted LPG and tilted LPG are comprehensively optimized through the length, index modulation depth, and tilt angle of the LPG in order to achieve a <span class="hlt">mode</span> contrast ratio (MCR) of more than 20 dB with less wavelength dependence. It is found that the proposed MCs have obvious advantages of high MCR, low <span class="hlt">mode</span> crosstalk, easy fabrication and maintenance, and compact size.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22375854-constraining-primordial-vector-mode-from-mode-polarization','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22375854-constraining-primordial-vector-mode-from-mode-polarization"><span>Constraining primordial vector <span class="hlt">mode</span> from B-<span class="hlt">mode</span> polarization</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>Saga, Shohei; Ichiki, Kiyotomo; Shiraishi, Maresuke, E-mail: saga.shohei@nagoya-u.jp, E-mail: maresuke.shiraishi@pd.infn.it, E-mail: ichiki@a.phys.nagoya-u.ac.jp</p> <p></p> <p>The B-<span class="hlt">mode</span> polarization spectrum of the Cosmic Microwave Background (CMB) may be the smoking gun of not only the primordial tensor <span class="hlt">mode</span> but also of the primordial vector <span class="hlt">mode</span>. If there exist nonzero vector-<span class="hlt">mode</span> metric perturbations in the early Universe, they are known to be supported by anisotropic stress fluctuations of free-streaming particles such as neutrinos, and to create characteristic signatures on both the CMB temperature, E-<span class="hlt">mode</span>, and B-<span class="hlt">mode</span> polarization anisotropies. We place constraints on the properties of the primordial vector <span class="hlt">mode</span> characterized by the vector-to-scalar ratio r{sub v} and the spectral index n{sub v} of the vector-shear power spectrum,more » from the Planck and BICEP2 B-<span class="hlt">mode</span> data. We find that, for scale-invariant initial spectra, the ΛCDM model including the vector <span class="hlt">mode</span> fits the data better than the model including the tensor <span class="hlt">mode</span>. The difference in χ{sup 2} between the vector and tensor models is Δχ{sup 2} = 3.294, because, on large scales the vector <span class="hlt">mode</span> generates smaller temperature fluctuations than the tensor <span class="hlt">mode</span>, which is preferred for the data. In contrast, the tensor <span class="hlt">mode</span> can fit the data set equally well if we allow a significantly blue-tilted spectrum. We find that the best-fitting tensor <span class="hlt">mode</span> has a large blue tilt and leads to an indistinct reionization bump on larger angular scales. The slightly red-tilted vector <span class="hlt">mode</span> supported by the current data set can also create O(10{sup -22})-Gauss magnetic fields at cosmological recombination. Our constraints should motivate research that considers models of the early Universe that involve the vector <span class="hlt">mode</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870024418&hterms=4th&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D4th','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870024418&hterms=4th&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3D4th"><span>Computational <span class="hlt">modes</span> and the Machenauer N.L.N.M.I. of the GLAS 4th order model. [NonLinear Normal <span class="hlt">Mode</span> Initialization in numerical weather forecasting</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Navon, I. M.; Bloom, S.; Takacs, L. L.</p> <p>1985-01-01</p> <p>An attempt was made to use the GLAS global 4th order shallow <span class="hlt">water</span> equations to perform a Machenhauer nonlinear normal <span class="hlt">mode</span> initialization (NLNMI) for the external vertical <span class="hlt">mode</span>. A new algorithm was defined for identifying and filtering out computational <span class="hlt">modes</span> which affect the convergence of the Machenhauer iterative procedure. The computational <span class="hlt">modes</span> and zonal waves were linearly initialized and gravitational <span class="hlt">modes</span> were nonlinearly initialized. The Machenhauer NLNMI was insensitive to the absence of high zonal wave numbers. The effects of the Machenhauer scheme were evaluated by performing 24 hr integrations with nondissipative and dissipative explicit time integration models. The NLNMI was found to be inferior to the Rasch (1984) pseudo-secant technique for obtaining convergence when the time scales of nonlinear forcing were much smaller than the time scales expected from the natural frequency of the <span class="hlt">mode</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptLT.101...21R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptLT.101...21R"><span>Spatial-<span class="hlt">mode</span> switchable ring fiber laser based on low <span class="hlt">mode</span>-crosstalk all-fiber <span class="hlt">mode</span> MUX/DEMUX</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Fang; Yu, Jinyi; Wang, Jianping</p> <p>2018-05-01</p> <p>We report an all-fiber ring laser that emits linearly polarized (LP) <span class="hlt">modes</span> based on the intracavity all-fiber <span class="hlt">mode</span> multiplexer/demultiplexer (MUX/DEMUX). Multiple LP <span class="hlt">modes</span> in ring fiber laser are generated by taking advantage of <span class="hlt">mode</span> MUX/DEMUX. The all-fiber <span class="hlt">mode</span> MUX/DEMUX are composed of cascaded <span class="hlt">mode</span>-selective couplers (MSCs). The output lasing <span class="hlt">mode</span> of the ring fiber laser can be switched among the three lowest-order LP <span class="hlt">modes</span> by employing combination of a <span class="hlt">mode</span> MUX and a simple N × 1 optical switch. The slope efficiencies, optical spectra and <span class="hlt">mode</span> profiles are measured.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMSA31C..04E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMSA31C..04E"><span>Deep Orographic Gravity Wave Dynamics over <span class="hlt">Subantarctic</span> Islands as Observed and Modeled during the Deep Propagating Gravity Wave Experiment (DEEPWAVE)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eckermann, S. D.; Broutman, D.; Ma, J.; Doyle, J. D.; Pautet, P. D.; Taylor, M. J.; Bossert, K.; Williams, B. P.; Fritts, D. C.; Smith, R. B.; Kuhl, D.; Hoppel, K.; McCormack, J. P.; Ruston, B. C.; Baker, N. L.; Viner, K.; Whitcomb, T.; Hogan, T. F.; Peng, M.</p> <p>2016-12-01</p> <p>The Deep Propagating Gravity Wave Experiment (DEEPWAVE) was an international aircraft-based field program to observe and study the end-to-end dynamics of atmospheric gravity waves from 0-100 km altitude and the effects on atmospheric circulations. On 14 July 2014, aircraft remote-sensing instruments detected large-amplitude gravity-wave oscillations within mesospheric airglow and sodium layers downstream of the Auckland Islands, located 1000 km south of Christchurch, New Zealand. A high-altitude reanalysis and a three-dimensional Fourier gravity wave model are used to investigate the dynamics of this event from the surface to the mesosphere. At 0700 UTC when first observations were made, surface flow across the islands' terrain generated linear three-dimensional wavefields that propagated rapidly to ˜78 km altitude, where intense breaking occurred in a narrow layer beneath a zero-wind region at ˜83 km altitude. In the following hours, the altitude of weak winds descended under the influence of a large-amplitude migrating semidiurnal tide, leading to intense breaking of these wavefields in subsequent observations starting at 1000 UTC. The linear Fourier model constrained by upstream reanalysis reproduces the salient aspects of observed wavefields, including horizontal wavelengths, phase orientations, temperature and vertical displacement amplitudes, heights and locations of incipient wave breaking, and momentum fluxes. Wave breaking has huge effects on local circulations, with inferred layer-averaged westward mean-flow accelerations of ˜350 m s-1 hour-1 and dynamical heating rates of ˜8 K hour-1, supporting recent speculation of important impacts of orographic gravity waves from <span class="hlt">subantarctic</span> islands on the mean circulation and climate of the middle atmosphere during austral winter. We also study deep orographic gravity waves from islands during DEEPWAVE more widely using observations from the Atmospheric Infrared Sounder (AIRS) and high-resolution high</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29336503','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29336503"><span>Sappinia sp. (Amoebozoa: Thecamoebida) and Rosculus sp. (SAR: Cercozoa) Isolated From King Penguin Guano Collected in the <span class="hlt">Subantarctic</span> (South Georgia, Salisbury Plain) and their Coexistence in Culture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tyml, Tomáš; Dyková, Iva</p> <p>2018-01-16</p> <p>Two amoeboid organisms of the genera Sappinia Dangeard, 1896 and Rosculus Hawes, 1963 were identified in a sample containing king penguin guano. This sample, collected in the <span class="hlt">Subantarctic</span>, enlarges the list of fecal habitats known for the presence of coprophilic amoebae. The two organisms were co-isolated and subcultured for over 6 mo, with continuous efforts being invested to separate each one from the mixed culture. In the mixed culture, Rosculus cells were fast growing, tolerated changes in culturing conditions, formed cysts, and evidently were attracted by Sappinia trophozoites. The separation of the Rosculus strain was accomplished, whereas the Sappinia strain remained intermixed with inseparable Rosculus cells. Sappinia cell populations were sensitive to changes in culturing conditions; they improved with reduction of Rosculus cells in the mixed culture. Thick-walled cysts, reportedly formed by Sappinia species, were not seen. The ultrastructure of both organisms was congruent with the currently accepted generic characteristics; however, some details were remarkable at the species level. Combined with the results of phylogenetic analyses, our findings indicate that the ultrastructure of the glycocalyx and the presence/absence of the Golgi apparatus in differential diagnoses of Sappinia species require a critical re-evaluation. © 2018 The Author(s) Journal of Eukaryotic Microbiology © 2018 International Society of Protistologists.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29931807','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29931807"><span>Comparison of three different dispersive liquid-liquid microextraction <span class="hlt">modes</span> performed on their most usual configurations for the extraction of phenolic, neutral aromatic, and amino compounds from <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saraji, Mohammad; Ghambari, Hoda</p> <p>2018-06-21</p> <p>In this work we seek clues to select the appropriate dispersive liquid-liquid microextraction <span class="hlt">mode</span> for extracting three categories of compounds. For this purpose, three common dispersive liquid-liquid microextraction <span class="hlt">modes</span> were compared under optimized conditions. Traditional dispersive liquid-liquid microextraction, in situ ionic liquid dispersive liquid-liquid microextraction and conventional ionic liquid dispersive liquid-liquid microextraction using chloroform, 1-butyl-3-methylimidazolium tetrafluoroborate, and 1-hexyl-3-methylimidazolium hexafluorophosphate as the extraction solvent, respectively, were considered in this work. Phenolic, neutral aromatic and amino compounds (each category included six members) were studied as analytes. The analytes in the extracts were determined by high-performance liquid chromatography with UV detection. For the analytes with polar functionalities, the in situ ionic liquid dispersive liquid-liquid microextraction <span class="hlt">mode</span> mostly led to better results. In contrast, for neutral hydrocarbons without polar functionalities, traditional dispersive liquid-liquid microextraction using chloroform produced better results. In this case, where dispersion forces were the dominant interactions in the extraction, the refractive index of solvent and analyte predicted the extraction performance better than the octanol-<span class="hlt">water</span> partition coefficient. It was also revealed that none of the methods were successful in extracting very hydrophilic analytes (compounds with the log octanol-<span class="hlt">water</span> partition coefficient < 2). The results of this study could be helpful in selecting a dispersive liquid-liquid microextraction <span class="hlt">mode</span> for the extraction of various groups of compounds. This article is protected by copyright. All rights reserved. This article is protected by copyright. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011SPIE.8307E..2JY','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011SPIE.8307E..2JY"><span>Influence of photo- and thermal bleaching on pre-irradiation low <span class="hlt">water</span> peak single <span class="hlt">mode</span> fibers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, Jianchong; Wen, Jianxiang; Luo, Wenyun; Xiao, Zhongyin; Chen, Zhenyi; Wang, Tingyun</p> <p>2011-12-01</p> <p>Reducing the radiation-induced transmission loss in low <span class="hlt">water</span> peak single <span class="hlt">mode</span> fiber (LWP SMF) has been investigated by using photo-bleaching method with 980nm pump light source and using thermal-bleaching method with temperature control system. The results show that the radiation-induced loss of pre-irradiation optical fiber can be reduced effectively with the help of photo-bleaching or thermal-bleaching. Although the effort of photo-bleaching is not as significant as thermal-bleaching, by using photo-bleaching method, the loss of fiber caused by radiation-induced defects can be reduced best up to 49% at 1310nm and 28% at 1550nm in low pre-irradiation condition, the coating of the fiber are not destroyed, and the rehabilitating time is just several hours, while self-annealing usually costs months' time. What's more, the typical high power LASER for photo-bleaching can be 980nm pump Laser Diode, which is very accessible.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21587786-identification-developmentally-toxic-drinking-water-disinfection-byproducts-evaluation-data-relevant-mode-action','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21587786-identification-developmentally-toxic-drinking-water-disinfection-byproducts-evaluation-data-relevant-mode-action"><span>Identification of developmentally toxic drinking <span class="hlt">water</span> disinfection byproducts and evaluation of data relevant to <span class="hlt">mode</span> of action</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>Colman, Joan; Rice, Glenn E., E-mail: rice.glenn@epa.gov; Wright, J. Michael</p> <p></p> <p>Reactions between chemicals used to disinfect drinking <span class="hlt">water</span> and compounds present in source <span class="hlt">waters</span> produce chemical mixtures containing hundreds of disinfection byproducts (DBPs). Although the results have been somewhat inconsistent, some epidemiological studies suggest associations may exist between DBP exposures and adverse developmental outcomes. The potencies of individual DBPs in rodent and rabbit developmental bioassays suggest that no individual DBP can account for the relative risk estimates reported in the positive epidemiologic studies, leading to the hypothesis that these outcomes could result from the toxicity of DBP mixtures. As a first step in a mixtures risk assessment for DBP developmentalmore » effects, this paper identifies developmentally toxic DBPs and examines data relevant to the <span class="hlt">mode</span> of action (MOA) for DBP developmental toxicity. We identified 24 developmentally toxic DBPs and four adverse developmental outcomes associated with human DBP exposures: spontaneous abortion, cardiovascular defects, neural tube defects, and low birth weight infancy. A plausible MOA, involving hormonal disruption of pregnancy, is delineated for spontaneous abortion, which some epidemiologic studies associate with total trihalomethane and bromodichloromethane exposures. The DBP data for the other three outcomes were inadequate to define key MOA steps.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/20837765-multidimensional-mixing-behavior-steam-water-flow-downcomer-annulus-during-lbloca-reflood-phase-direct-vessel-injection-mode','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/20837765-multidimensional-mixing-behavior-steam-water-flow-downcomer-annulus-during-lbloca-reflood-phase-direct-vessel-injection-mode"><span>Multidimensional Mixing Behavior of Steam-<span class="hlt">Water</span> Flow in a Downcomer Annulus During LBLOCA Reflood Phase with a Direct Vessel Injection <span class="hlt">Mode</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>Kwon, Tae-Soon; Yun, Byong-Jo; Euh, Dong-Jin</p> <p></p> <p>Multidimensional thermal-hydraulic behavior in the downcomer annulus of a pressurized <span class="hlt">water</span> reactor (PWR) vessel with a direct vessel injection <span class="hlt">mode</span> is presented based on the experimental observation in the MIDAS (multidimensional investigation in downcomer annulus simulation) steam-<span class="hlt">water</span> test facility. From the steady-state test results to simulate the late reflood phase of a large-break loss-of-coolant accident (LBLOCA), isothermal lines show the multidimensional phenomena of a phasic interaction between steam and <span class="hlt">water</span> in the downcomer annulus very well. MIDAS is a steam-<span class="hlt">water</span> separate effect test facility, which is 1/4.93 linearly scaled down to a 1400-MW(electric) PWR type of a nuclear reactor, focusedmore » on understanding multidimensional thermal-hydraulic phenomena in a downcomer annulus with various types of safety injection during the refill or reflood phase of an LBLOCA. The initial and the boundary conditions are scaled from the pretest analysis based on the preliminary calculation using the TRAC code. The superheated steam with a superheating degree of 80 K at a given downcomer pressure of 180 kPa is injected equally through three intact cold legs into the downcomer.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JHyd..539..648J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JHyd..539..648J"><span>Managing the <span class="hlt">water</span>-energy-food nexus: Gains and losses from new <span class="hlt">water</span> development in Amu Darya River Basin</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jalilov, Shokhrukh-Mirzo; Keskinen, Marko; Varis, Olli; Amer, Saud; Ward, Frank A.</p> <p>2016-08-01</p> <p>According to the UN, the population of Central Asia will increase from its current approximately 65 million people to a well over 90 million by the end of this century. Taking this increasing population into consideration, it is impossible to project development strategies without considering three key factors in meeting the demands of a growing population: <span class="hlt">water</span>, food and energy. Societies will have to choose, for instance, between using land and fertilizer for food production or for bio-based or renewable energy production, and between using fresh <span class="hlt">water</span> for energy production or for irrigating crops. Thus <span class="hlt">water</span>, food and energy are inextricably linked and must be considered together as a system. Recently, tensions among the Central Asian countries over the use of <span class="hlt">water</span> for energy and energy production have increased with the building of Rogun Dam on the Vakhsh River, a tributary of the Amu Darya River. The dam will provide upstream Tajikistan with hydropower, while downstream countries fear it could negatively impact their irrigated agriculture. Despite recent peer reviewed literature on <span class="hlt">water</span> resources management in Amu Darya Basin, none to date have addressed the interconnection and mutual impacts within <span class="hlt">water</span>-energy-food systems in face of constructing the Rogun Dam. We examine two potential operation <span class="hlt">modes</span> of the dam: Energy <span class="hlt">Mode</span> (ensuring Tajikistan's hydropower needs) and Irrigation <span class="hlt">Mode</span> (ensuring <span class="hlt">water</span> for agriculture downstream). Results show that the Energy <span class="hlt">Mode</span> could ensure more than double Tajikistan's energy capacity, but would reduce <span class="hlt">water</span> availability during the growing season, resulting in an average 37% decline in agricultural benefits in downstream countries. The Irrigation <span class="hlt">Mode</span> could bring a surplus in agricultural benefits to Tajikistan and Uzbekistan in addition an increasing energy benefits in Tajikistan by two fold. However, energy production in the Irrigation <span class="hlt">Mode</span> would be non-optimally distributed over the seasons resulting in the most of</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('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3032774','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3032774"><span>Isotopic Investigation of Contemporary and Historic Changes in Penguin Trophic Niches and Carrying Capacity of the Southern Indian Ocean</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jaeger, Audrey; Cherel, Yves</p> <p>2011-01-01</p> <p>A temperature-defined regime shift occurred in the 1970s in the southern Indian Ocean, with simultaneous severe decreases in many predator populations. We tested a possible biological link between the regime shift and predator declines by measuring historic and contemporary feather isotopic signatures of seven penguin species with contrasted foraging strategies and inhabiting a large latitudinal range. We first showed that contemporary penguin isotopic variations and chlorophyll a concentration were positively correlated, suggesting the usefulness of predator δ13C values to track temporal changes in the ecosystem carrying capacity and its associated coupling to consumers. Having controlled for the Suess effect and for increase CO2 in seawater, δ13C values of Antarctic penguins and of king penguins did not change over time, while δ13C of other <span class="hlt">subantarctic</span> and subtropical species were lower in the 1970s. The data therefore suggest a decrease in ecosystem carrying capacity of the southern Indian Ocean during the temperature regime-shift in subtropical and <span class="hlt">subantarctic</span> <span class="hlt">waters</span> but not in the vicinity of the Polar Front and in southward high-Antarctic <span class="hlt">waters</span>. The resulting lower secondary productivity could be the main driving force explaining the decline of subtropical and <span class="hlt">subantarctic</span> (but not Antarctic) penguins that occurred in the 1970s. Feather δ15N values did not show a consistent temporal trend among species, suggesting no major change in penguins’ diet. This study highlights the usefulness of developing long-term tissue sampling and data bases on isotopic signature of key marine organisms to track potential changes in their isotopic niches and in the carrying capacity of the environment. PMID:21311756</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21311756','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21311756"><span>Isotopic investigation of contemporary and historic changes in penguin trophic niches and carrying capacity of the southern Indian ocean.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jaeger, Audrey; Cherel, Yves</p> <p>2011-02-02</p> <p>A temperature-defined regime shift occurred in the 1970s in the southern Indian Ocean, with simultaneous severe decreases in many predator populations. We tested a possible biological link between the regime shift and predator declines by measuring historic and contemporary feather isotopic signatures of seven penguin species with contrasted foraging strategies and inhabiting a large latitudinal range. We first showed that contemporary penguin isotopic variations and chlorophyll a concentration were positively correlated, suggesting the usefulness of predator δ¹³C values to track temporal changes in the ecosystem carrying capacity and its associated coupling to consumers. Having controlled for the Suess effect and for increase CO₂ in seawater, δ¹³C values of Antarctic penguins and of king penguins did not change over time, while δ¹³C of other <span class="hlt">subantarctic</span> and subtropical species were lower in the 1970s. The data therefore suggest a decrease in ecosystem carrying capacity of the southern Indian Ocean during the temperature regime-shift in subtropical and <span class="hlt">subantarctic</span> <span class="hlt">waters</span> but not in the vicinity of the Polar Front and in southward high-Antarctic <span class="hlt">waters</span>. The resulting lower secondary productivity could be the main driving force explaining the decline of subtropical and <span class="hlt">subantarctic</span> (but not Antarctic) penguins that occurred in the 1970s. Feather δ¹⁵N values did not show a consistent temporal trend among species, suggesting no major change in penguins' diet. This study highlights the usefulness of developing long-term tissue sampling and data bases on isotopic signature of key marine organisms to track potential changes in their isotopic niches and in the carrying capacity of the environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25423551','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25423551"><span>Wandering albatrosses document latitudinal variations in the transfer of persistent organic pollutants and mercury to Southern Ocean predators.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Carravieri, Alice; Bustamante, Paco; Tartu, Sabrina; Meillère, Alizée; Labadie, Pierre; Budzinski, Hélène; Peluhet, Laurent; Barbraud, Christophe; Weimerskirch, Henri; Chastel, Olivier; Cherel, Yves</p> <p>2014-12-16</p> <p>Top marine predators are effective tools to monitor bioaccumulative contaminants in remote oceanic environments. Here, we used the wide-ranging wandering albatross Diomedea exulans to investigate potential geographical variations of contaminant transfer to predators in the Southern Ocean. Blood concentrations of 19 persistent organic pollutants and 14 trace elements were measured in a large number of individuals (N = 180) of known age, sex and breeding status from the <span class="hlt">subantarctic</span> Crozet Islands. Wandering albatrosses were exposed to a wide range of contaminants, with notably high blood mercury concentrations. Contaminant burden was markedly influenced by latitudinal foraging habitats (inferred from blood δ(13)C values), with individuals feeding in warmer subtropical <span class="hlt">waters</span> having lower concentrations of pesticides, but higher concentrations of mercury, than those feeding in colder <span class="hlt">subantarctic</span> <span class="hlt">waters</span>. Sexual differences in contaminant burden seemed to be driven by gender specialization in feeding habitats, rather than physiological characteristics, with females foraging further north than males. Other individual traits, such as adult age and reproductive status, had little effect on blood contaminant concentrations. Our study provides further evidence of the critical role of global distillation on organic contaminant exposure to Southern Ocean avian predators. In addition, we document an unexpected high transfer of mercury to predators in subtropical <span class="hlt">waters</span>, which merits further investigation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.817a2035W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.817a2035W"><span>An SMS (single <span class="hlt">mode</span> - multi <span class="hlt">mode</span> - single <span class="hlt">mode</span>) fiber structure for vibration sensing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Waluyo, T. B.; Bayuwati, D.</p> <p>2017-04-01</p> <p>We describe an SMS (single <span class="hlt">mode</span> - multi <span class="hlt">mode</span> - single <span class="hlt">mode</span>) fiber structure to be used in a vibration sensing system. The fiber structure was fabricated by splicing a section (about 300 mm in length) of a step index multi <span class="hlt">mode</span> fiber between two single <span class="hlt">mode</span> fibers obtained from a communication grade fiber patchcord. Interference between higher order <span class="hlt">modes</span> occurs while light from a narrow band light source travels along the multi <span class="hlt">mode</span> fiber. When the multi <span class="hlt">mode</span> fiber vibrates, the refractive index profile is changed because of the photo-elastics effect and the amplitude of the interference pattern is changed accordingly. To simulate a vibrating structure we used a loudspeaker to vibrate a wooden table. By using a digital oscilloscope, we recorded and analysed the vibrating signals obtained from the SMS fiber structure as well as from a GS-32CT geophone for referencing. We observed that this SMS fiber structure was potential to be used in a vibration sensing system with a measurement range from 30 to 180 Hz with inherent optical fiber sensor advantages such as light weight, immune to electromagnetic interference, and no electricity in the sensing part.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1394448','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1394448"><span>Multi-<span class="hlt">mode</span> humidity sensing with <span class="hlt">water</span>-soluble copper phthalocyanine for increased sensitivity and dynamic range</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>Muckley, Eric S.; Jacobs, Christopher B.; Vidal, Keith</p> <p></p> <p>Aqueous solubility of copper phthalocyanine-3,4',4',4"'-tetrasulfonic acid tetrasodium salt (CuPcTs) enables fabrication of flexible electronic devices by low cost inkjet printing. We (1) investigate <span class="hlt">water</span> adsorption kinetics on CuPcTs for better understanding the effects of relative humidity (RH) on hydrophilic phthalocyanines, and (2) assess CuPcTs as a humidity-sensing material. Reaction models show that H 2O undergoes 2-site adsorption which can be represented by a pair of sequentially-occurring pseudo-first order reactions. Using high frequency (300–700 THz) and low frequency (1–8 MHz) dielectric spectroscopy combined with gravimetric measurements and principal component analysis, we observe that significant opto-electrical changes in CuPcTs occur at RHmore » ≈ 60%. The results suggest that rapid H 2O adsorption takes place at hydrophilic sulfonyl/salt groups on domain surfaces at low RH, while slow adsorption and diffusion of H 2O into CuPcTs crystallites leads to a mixed CuPcTs-H 2O phase at RH > 60%, resulting in high frequency dielectric screening of the film by <span class="hlt">water</span> and dissociation of Na+ from CuPc(SO 3-) 4 ions. Lastly, the CuPcTs-H 2O interaction can be tracked using a combination of gravimetric, optical, and electrical sensing <span class="hlt">modes</span>, enabling accurate ( ± 2.5%) sensing in the ~0–95% RH range with a detection limit of less than 0.1% RH.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1394448-multi-mode-humidity-sensing-water-soluble-copper-phthalocyanine-increased-sensitivity-dynamic-range','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1394448-multi-mode-humidity-sensing-water-soluble-copper-phthalocyanine-increased-sensitivity-dynamic-range"><span>Multi-<span class="hlt">mode</span> humidity sensing with <span class="hlt">water</span>-soluble copper phthalocyanine for increased sensitivity and dynamic range</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Muckley, Eric S.; Jacobs, Christopher B.; Vidal, Keith; ...</p> <p>2017-08-30</p> <p>Aqueous solubility of copper phthalocyanine-3,4',4',4"'-tetrasulfonic acid tetrasodium salt (CuPcTs) enables fabrication of flexible electronic devices by low cost inkjet printing. We (1) investigate <span class="hlt">water</span> adsorption kinetics on CuPcTs for better understanding the effects of relative humidity (RH) on hydrophilic phthalocyanines, and (2) assess CuPcTs as a humidity-sensing material. Reaction models show that H 2O undergoes 2-site adsorption which can be represented by a pair of sequentially-occurring pseudo-first order reactions. Using high frequency (300–700 THz) and low frequency (1–8 MHz) dielectric spectroscopy combined with gravimetric measurements and principal component analysis, we observe that significant opto-electrical changes in CuPcTs occur at RHmore » ≈ 60%. The results suggest that rapid H 2O adsorption takes place at hydrophilic sulfonyl/salt groups on domain surfaces at low RH, while slow adsorption and diffusion of H 2O into CuPcTs crystallites leads to a mixed CuPcTs-H 2O phase at RH > 60%, resulting in high frequency dielectric screening of the film by <span class="hlt">water</span> and dissociation of Na+ from CuPc(SO 3-) 4 ions. Lastly, the CuPcTs-H 2O interaction can be tracked using a combination of gravimetric, optical, and electrical sensing <span class="hlt">modes</span>, enabling accurate ( ± 2.5%) sensing in the ~0–95% RH range with a detection limit of less than 0.1% RH.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28855615','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28855615"><span>Multi-<span class="hlt">mode</span> humidity sensing with <span class="hlt">water</span>-soluble copper phthalocyanine for increased sensitivity and dynamic range.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Muckley, Eric S; Jacobs, Christopher B; Vidal, Keith; Lavrik, Nickolay V; Sumpter, Bobby G; Ivanov, Ilia N</p> <p>2017-08-30</p> <p>Aqueous solubility of copper phthalocyanine-3,4',4″,4″'-tetrasulfonic acid tetrasodium salt (CuPcTs) enables fabrication of flexible electronic devices by low cost inkjet printing. We (1) investigate <span class="hlt">water</span> adsorption kinetics on CuPcTs for better understanding the effects of relative humidity (RH) on hydrophilic phthalocyanines, and (2) assess CuPcTs as a humidity-sensing material. Reaction models show that H 2 O undergoes 2-site adsorption which can be represented by a pair of sequentially-occurring pseudo-first order reactions. Using high frequency (300-700 THz) and low frequency (1-8 MHz) dielectric spectroscopy combined with gravimetric measurements and principal component analysis, we observe that significant opto-electrical changes in CuPcTs occur at RH ≈ 60%. The results suggest that rapid H 2 O adsorption takes place at hydrophilic sulfonyl/salt groups on domain surfaces at low RH, while slow adsorption and diffusion of H 2 O into CuPcTs crystallites leads to a mixed CuPcTs-H 2 O phase at RH > 60%, resulting in high frequency dielectric screening of the film by <span class="hlt">water</span> and dissociation of Na + from CuPc(SO 3 - ) 4 ions. The CuPcTs-H 2 O interaction can be tracked using a combination of gravimetric, optical, and electrical sensing <span class="hlt">modes</span>, enabling accurate ( ± 2.5%) sensing in the ~0-95% RH range with a detection limit of less than 0.1% RH.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC14C2080G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC14C2080G"><span>Effects of Southern Hemispheric Wind Changes on Global Oxygen and the Pacific Oxygen Minimum Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Getzlaff, J.; Dietze, H.; Oschlies, A.</p> <p>2016-02-01</p> <p>We use a coupled ocean biogeochemistry-circulation model to compare the impact of changes in southern hemispheric winds with that of warming induced buoyancy fluxes on dissolved oxygen. Changes in the southern hemispheric wind fields, which are in line with an observed shift of the southern annual <span class="hlt">mode</span>, are a combination of a strengthening and poleward shift of the southern westerlies. We differentiate between effects caused by a strengthening of the westerlies and effects of a southward shift of the westerlies that is accompanied by a poleward expansion of the tropical trade winds. Our results confirm that the Southern Ocean plays an important role for the marine oxygen supply: a strengthening of the southern westerlies, that leads to an increase of the <span class="hlt">water</span> formation rates of the oxygen rich deep and intermediate <span class="hlt">water</span> masses, can counteract part of the warming-induced decline in marine oxygen levels. The wind driven intensification of the Southern Ocean meridional overturning circulation drives an increase of the global oxygen supply. Furthermore the results show that the shift of the boundary between westerlies and trades results in an increase of <span class="hlt">subantarctic</span> <span class="hlt">mode</span> <span class="hlt">water</span> and an anti-correlated decrease of deep <span class="hlt">water</span> formation and reduces the oceanic oxygen supply. In addition we find that the increased meridional extension of the southern trade winds, results in a strengthening and southward shift of the subtropical wind stress curl. This alters the subtropical gyre circulation (intensification and southward shift) and with it decreases the <span class="hlt">water</span> mass transport into the oxygen minimum zone. In a business-as-usual CO2 emission scenario, the poleward shift of the trade-to-westerlies boundary is as important for the future evolution of the suboxic volume as direct warming-induced changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDH13006K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDH13006K"><span>Ringin' the <span class="hlt">water</span> bell: dynamic <span class="hlt">modes</span> of curved fluid sheets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kolinski, John; Aharoni, Hillel; Fineberg, Jay; Sharon, Eran</p> <p>2015-11-01</p> <p>A <span class="hlt">water</span> bell is formed by fluid flowing in a thin, coherent sheet in the shape of a bell. Experimentally, a <span class="hlt">water</span> bell is created via the impact of a cylindrical jet on a flat surface. Its shape is set by the splash angle (the separation angle) of the resulting cylindrically symmetric <span class="hlt">water</span> sheet. The separation angle is altered by adjusting the height of a lip surrounding the impact point, as in a <span class="hlt">water</span> sprinkler. We drive the lip's height sinusoidally, altering the separation angle, and ringin' the <span class="hlt">water</span> bell. This forcing generates disturbances on the steady-state <span class="hlt">water</span> bell that propagate forward and backward in the fluid's reference frame at well-defined velocities, and interact, resulting in the emergence of an interference pattern unique to each steady-state geometry. We analytically model these dynamics by linearizing the amplitude of the bell's response about the underlying curved geometry. This simple model predicts the nodal structure over a wide range of steady-state <span class="hlt">water</span> bell configurations and driving frequencies. Due to the curved <span class="hlt">water</span> bell geometry, the nodal structure is quite complex; nevertheless, the predicted nodal structure agrees extremely well with the experimental data. When we drive the bell beyond perturbative separation angles, the nodal locations surprisingly persist, despite the strikingly altered underlying <span class="hlt">water</span> bell shape. At extreme driving amplitudes the <span class="hlt">water</span> sheet assumes a rich variety of tortuous, non-convex shapes; nevertheless, the fluid sheet remains intact.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/12243575','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/12243575"><span>Experimental investigation of leaky lamb <span class="hlt">modes</span> by an optically induced grating.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Van de Rostyne, Kris; Glorieux, Christ; Gao, Weimin; Lauriks, Walter; Thoen, Jan</p> <p>2002-09-01</p> <p>By removing the symmetry of a free plate configuration, fluid loading significantly modifies the nature of acoustic waves travelling along a plate, and it even gives existence to new acoustic <span class="hlt">modes</span>. We present theoretical predictions for the existence, dispersive behavior, and spatial distribution of leaky Lamb waves in a fluid-loaded film. Although Lamb <span class="hlt">modes</span> are often investigated by studying the radiated fluid waves resulting from their leakage, here their properties are assessed by detecting the wave displacements directly using laser beam deflection. By using crossed laser beam excitation, the detection and analysis of the different <span class="hlt">modes</span> is done at a fixed wavelength, allowing one to verify the existence, the velocity, and the damping of each predicted <span class="hlt">mode</span> in a simple and unambiguous way. Our theoretical predictions for the nature of the <span class="hlt">modes</span> in a <span class="hlt">water</span>-loaded Plexiglas film, including parts of looping <span class="hlt">modes</span>, are experimentally confirmed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17427957','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17427957"><span>Accuracy of binding <span class="hlt">mode</span> prediction with a cascadic stochastic tunneling method.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fischer, Bernhard; Basili, Serena; Merlitz, Holger; Wenzel, Wolfgang</p> <p>2007-07-01</p> <p>We investigate the accuracy of the binding <span class="hlt">modes</span> predicted for 83 complexes of the high-resolution subset of the ASTEX/CCDC receptor-ligand database using the atomistic FlexScreen approach with a simple forcefield-based scoring function. The median RMS deviation between experimental and predicted binding <span class="hlt">mode</span> was just 0.83 A. Over 80% of the ligands dock within 2 A of the experimental binding <span class="hlt">mode</span>, for 60 complexes the docking protocol locates the correct binding <span class="hlt">mode</span> in all of ten independent simulations. Most docking failures arise because (a) the experimental structure clashed in our forcefield and is thus unattainable in the docking process or (b) because the ligand is stabilized by crystal <span class="hlt">water</span>. 2007 Wiley-Liss, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFDA16002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDA16002H"><span>Analysis of <span class="hlt">water</span> microdroplet condensation on silicon surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Honda, Takuya; Fujimoto, Kenya; Yoshimoto, Yuta; Mogi, Katsuo; Kinefuchi, Ikuya; Sugii, Yasuhiko; Takagi, Shu; Univ. of Tokyo Team; Tokyo Inst. of Tech. Team</p> <p>2016-11-01</p> <p>We observed the condensation process of <span class="hlt">water</span> microdroplets on flat silicon (100) surfaces by means of the sequential visualization of the droplets using an environmental scanning electron microscope. As previously reported for nanostructured surfaces, the condensation process of <span class="hlt">water</span> microdroplets on the flat silicon surfaces also exhibits two <span class="hlt">modes</span>: the constant base (CB) area <span class="hlt">mode</span> and the constant contact angle (CCA) <span class="hlt">mode</span>. In the CB <span class="hlt">mode</span>, the contact angle increases with time while the base diameter is constant. Subsequently, in the CCA <span class="hlt">mode</span>, the base diameter increases with time while the contact angle remains constant. The dropwise condensation model regulated by subcooling temperature does not reproduce the experimental results. Because the subcooling temperature is not constant in the case of a slow condensation rate, this model is not applicable to the condensation of the long time scale ( several tens of minutes). The contact angle of <span class="hlt">water</span> microdroplets ( several μm) tended to be smaller than the macro contact angle. Two hypotheses are proposed as the cause of small contact angles: electrowetting and the coalescence of sub- μm <span class="hlt">water</span> droplets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE10019E..0NL','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE10019E..0NL"><span><span class="hlt">Mode</span> evolution in polarization maintain few <span class="hlt">mode</span> fibers and applications in <span class="hlt">mode</span>-division-multiplexing systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Yan; Zeng, Xinglin; Mo, Qi; Li, Wei; Liu, Zhijian; Wu, Jian</p> <p>2016-10-01</p> <p>In few-<span class="hlt">mode</span> polarization-maintaining-fiber (FM-PMF), the effective-index splitting exists not only between orthogonally polarization state but also between degenerated <span class="hlt">modes</span> within a high-order <span class="hlt">mode</span> group. Hence besides the polarization state evolution, the <span class="hlt">mode</span> patterns in each LP set are need to be analyzed. In this letter, the completed firstorder <span class="hlt">mode</span> (LP11 <span class="hlt">mode</span>) evolution in PM-FMF is analyzed and represented by analogous Jones vector and Poincarésphere respectively. Furthermore, with Jones matrix analysis, the modal dynamics in FM-PMFs is conveniently analyzed. The conclusions are used to propose a PM-FMF based LP11 <span class="hlt">mode</span> rotator and an PM-FMF based OAM generator. Both simulation and experiments are conducted to investigate performance of the two devices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22395778-dual-cavity-mode-converter-fundamental-mode-output-over-moded-relativistic-backward-wave-oscillator','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22395778-dual-cavity-mode-converter-fundamental-mode-output-over-moded-relativistic-backward-wave-oscillator"><span>Dual-cavity <span class="hlt">mode</span> converter for a fundamental <span class="hlt">mode</span> output in an over-<span class="hlt">moded</span> relativistic backward-wave oscillator</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>Li, Jiawei; Huang, Wenhua; Science and Technology on High Power Microwave Laboratory, Northwest Institute of Nuclear Technology, Xi'an 710024</p> <p>2015-03-16</p> <p>A dual-cavity TM{sub 02}–TM{sub 01} <span class="hlt">mode</span> converter is designed for a dual-<span class="hlt">mode</span> operation over-<span class="hlt">moded</span> relativistic backward-wave oscillator. With the converter, the fundamental <span class="hlt">mode</span> output is achieved. Particle-in-cell simulation shows that the efficiency of beam-wave conversion was over 46% and a pureTM{sub 01} <span class="hlt">mode</span> output was obtained. Effects of end reflection provided by the <span class="hlt">mode</span> converter were studied. Adequate TM{sub 01} <span class="hlt">mode</span> feedback provided by the converter enhances conversion efficiency. The distance between the <span class="hlt">mode</span> converter and extraction cavity critically affect the generation of microwaves depending on the reflection phase of TM{sub 01} <span class="hlt">mode</span> feedback.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006DSRI...53.1203H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006DSRI...53.1203H"><span>The seasonal succession of zooplankton in the Southern Ocean south of Australia, part II: The <span class="hlt">Sub-Antarctic</span> to Polar Frontal Zones</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hunt, Brian P. V.; Hosie, Graham W.</p> <p>2006-07-01</p> <p>Between October 2001 and March 2002 six transects were completed at monthly intervals in the <span class="hlt">Sub-Antarctic</span> Zone (SAZ) and Inter-Sub-Antarctic Front Zone (ISAFZ)/Polar Frontal Zone (PFZ) in the Southern Ocean south of Australia. Zooplankton were collected with a Continuous Plankton Recorder and NORPAC net and multivariate analysis was used to analyse the seasonal succession of communities. Despite strong, seasonally consistent, biogeographic differences between the SAZ and ISAFZ/PFZ, community structure in all zones was dominated by a suite of common taxa. These included the ubiquitous Oithona similis, foraminiferans and appendicularians (Core taxa), occurring in >97% of samples and contributing an average of 75% to total sample abundance, and Calanus simillimus, Rhincalanus gigas, Ctenocalanus citer, Clausocalanus brevipes, Clausocalanus laticeps, Oithona frigida, Limacina spp. and chaetognaths (Summer taxa), present in >57% of samples and occurring at seasonally high densities. Because of the dominance of the Core and Summer taxa, the seasonal succession was most clearly evident as a change in zooplankton densities. In October densities averaged <15 ind m -3, rising to 52 ind m -3 (max=92 ind m -3) in November, and subsequently increasing slowly through to January (ave=115 ind m -3; max=255 ind m -3). Densities peaked abruptly in February (ave=634 ind m -3; max=1593 ind m -3), and remained relatively high in March (ave=193 ind m -3; max=789 ind m -3). A latitudinal lag in seasonal development was observed with peak densities occurring first in the SAZ (February) and then in the ISAFZ/PFZ (March). The seasonal community succession was strongly influenced by species population cycles. The role of zooplankton in biogeochemical cycling in the SAZ and ISAFZ/PFZ was discussed in the light of past sediment trap data collected from the study area.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18278107','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18278107"><span>Single-<span class="hlt">mode</span> fiber laser based on core-cladding <span class="hlt">mode</span> conversion.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Suzuki, Shigeru; Schülzgen, Axel; Peyghambarian, N</p> <p>2008-02-15</p> <p>A single-<span class="hlt">mode</span> fiber laser based on an intracavity core-cladding <span class="hlt">mode</span> conversion is demonstrated. The fiber laser consists of an Er-doped active fiber and two fiber Bragg gratings. One Bragg grating is a core-cladding <span class="hlt">mode</span> converter, and the other Bragg grating is a narrowband high reflector that selects the lasing wavelength. Coupling a single core <span class="hlt">mode</span> and a single cladding <span class="hlt">mode</span> by the grating <span class="hlt">mode</span> converter, the laser operates as a hybrid single-<span class="hlt">mode</span> laser. This approach for designing a laser cavity provides a much larger <span class="hlt">mode</span> area than conventional large-<span class="hlt">mode</span>-area step-index fibers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3125541','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3125541"><span>Scaling Fiber Lasers to Large <span class="hlt">Mode</span> Area: An Investigation of Passive <span class="hlt">Mode</span>-Locking Using a Multi-<span class="hlt">Mode</span> Fiber</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ding, Edwin; Lefrancois, Simon; Kutz, Jose Nathan; Wise, Frank W.</p> <p>2011-01-01</p> <p>The <span class="hlt">mode</span>-locking of dissipative soliton fiber lasers using large <span class="hlt">mode</span> area fiber supporting multiple transverse <span class="hlt">modes</span> is studied experimentally and theoretically. The averaged <span class="hlt">mode</span>-locking dynamics in a multi-<span class="hlt">mode</span> fiber are studied using a distributed model. The co-propagation of multiple transverse <span class="hlt">modes</span> is governed by a system of coupled Ginzburg–Landau equations. Simulations show that stable and robust <span class="hlt">mode</span>-locked pulses can be produced. However, the <span class="hlt">mode</span>-locking can be destabilized by excessive higher-order <span class="hlt">mode</span> content. Experiments using large core step-index fiber, photonic crystal fiber, and chirally-coupled core fiber show that <span class="hlt">mode</span>-locking can be significantly disturbed in the presence of higher-order <span class="hlt">modes</span>, resulting in lower maximum single-pulse energies. In practice, spatial <span class="hlt">mode</span> content must be carefully controlled to achieve full pulse energy scaling. This paper demonstrates that <span class="hlt">mode</span>-locking performance is very sensitive to the presence of multiple waveguide <span class="hlt">modes</span> when compared to systems such as amplifiers and continuous-wave lasers. PMID:21731106</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21731106','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21731106"><span>Scaling Fiber Lasers to Large <span class="hlt">Mode</span> Area: An Investigation of Passive <span class="hlt">Mode</span>-Locking Using a Multi-<span class="hlt">Mode</span> Fiber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ding, Edwin; Lefrancois, Simon; Kutz, Jose Nathan; Wise, Frank W</p> <p>2011-01-01</p> <p>The <span class="hlt">mode</span>-locking of dissipative soliton fiber lasers using large <span class="hlt">mode</span> area fiber supporting multiple transverse <span class="hlt">modes</span> is studied experimentally and theoretically. The averaged <span class="hlt">mode</span>-locking dynamics in a multi-<span class="hlt">mode</span> fiber are studied using a distributed model. The co-propagation of multiple transverse <span class="hlt">modes</span> is governed by a system of coupled Ginzburg-Landau equations. Simulations show that stable and robust <span class="hlt">mode</span>-locked pulses can be produced. However, the <span class="hlt">mode</span>-locking can be destabilized by excessive higher-order <span class="hlt">mode</span> content. Experiments using large core step-index fiber, photonic crystal fiber, and chirally-coupled core fiber show that <span class="hlt">mode</span>-locking can be significantly disturbed in the presence of higher-order <span class="hlt">modes</span>, resulting in lower maximum single-pulse energies. In practice, spatial <span class="hlt">mode</span> content must be carefully controlled to achieve full pulse energy scaling. This paper demonstrates that <span class="hlt">mode</span>-locking performance is very sensitive to the presence of multiple waveguide <span class="hlt">modes</span> when compared to systems such as amplifiers and continuous-wave lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002EGSGA..27.2398H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002EGSGA..27.2398H"><span><span class="hlt">Water</span> On Mars: <span class="hlt">Mode</span> of Emplacement, Scale, Behavior and Fate.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Head, J. W.</p> <p></p> <p>There is clear evidence for standing bodies of <span class="hlt">water</span> in different places and at different times in the history of Mars. The martian outflow channels emptied into the northern lowlands primarily in the Late Hesperian Period and their characteristics suggest to many workers that a large standing body of <span class="hlt">water</span>, or ocean, was produced as a result. Characteristics of northern lowland deposits in the Early Amazonian Period suggest that by this time such an ocean was gone. We analyze the fate of such standing bodies of <span class="hlt">water</span> under climatic conditions similar to the present. The evolution of <span class="hlt">water</span> loaded with sediments emplaced by outflow channel formation would include three phases. (1) Violent emplacement of warm <span class="hlt">water</span> followed by a short period of intensive evaporation and convection. <span class="hlt">Water</span> vapor would strongly influence the climate, at least for a geologically short time; when the <span class="hlt">water</span> reached 277 K, boiling and intensive convection ceased and sediments were deposited. (2) Geologically fast (104 years) freezing accompanied by weak convective <span class="hlt">water</span> movement. (3) Sublimation of the ice lasted longer than freezing, but for a geologically short period. The rate and latitudinal dependence of sublimation, and locations of <span class="hlt">water</span> vapor condensation, crucially depend on planetary obliquity, climate, and sediment veneering of the ice. Several observations support the hypothesis that the Late Hesperian Vastitas Borealis Formation is the sublimation residue of the ocean. Geological evidence has been cited to support a `warm, wet' era in the earlier Noachian Period (e.g., valley networks, degradation rates, etc.) and standing bodies of <span class="hlt">water</span> under these earlier conditions have different origins and could have significantly longer residence times. Critical assessment of this evidence leads to several scenarios for the emplacement style, location and fate of <span class="hlt">water</span> on early Mars, and the important transition to conditions similar to those of today. Candidate early Mars emplacement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ascl.soft01006S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ascl.soft01006S"><span>Decoupling<span class="hlt">Modes</span>: Passive <span class="hlt">modes</span> amplitudes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shaw, J. Richard; Lewis, Antony</p> <p>2018-01-01</p> <p>Decoupling<span class="hlt">Modes</span> calculates the amplitude of the passive <span class="hlt">modes</span>, which requires solving the Einstein equations on superhorizon scales sourced by the anisotropic stress from the magnetic fields (prior to neutrino decoupling), and the magnetic and neutrino stress (after decoupling). The code is available as a Mathematica notebook.</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.ncbi.nlm.nih.gov/pubmed/21675047','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21675047"><span>[History of Polish botanical and mycological researches on sheets of land of Antarctic and <span class="hlt">Sub-Antarctic</span> in the years 1977-2009].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Köhler, Piotr; Olech, Maria</p> <p>2011-01-01</p> <p>The work includes a description of the period from the moment of setting up Polish Polar Station on King George Island (1977) to the end of International Polar Year IV in 2009. Researches on flower plants focused, among others, on plants' morphology, morphological composition of the pollen and anatomical ultra-structure of the leaves. There were also carried out biochemical and other searches for the internal mutability. Within physiological studies one concentrated on the problem of reaction to temperature stress. Biological researches focused mainly on solving taxonomic and bio-geographic problems. Finally, were published several monographs and, among others, the first in history complete description of moss' flora of the whole of Antarctic (2008). Research works over algae included also such issues as floristics, bio-geography, taxonomy and ecology (for instance, the rookery's impact on distribution of algae, or the influence of inanimate factors on dynamics of condensing the Diatoma in different <span class="hlt">water</span> and soil-bound tanks). Up till now, within mycological investigations has been identified a variety of lichen fungi that for the most part of Antarctic are a novelty. There were scientifically described new for science genera and species of Western Antarctic. Lichenological studies were made in the field of taxonomy, geography, lichenometry, biochemistry of lichens, lichenoindication, ecophysiology and from the point of analysis of base metals' content. There were also described new for science species. Since 1991, were published the results of searches for the base metals' content and vestigial chemical elements in lichens' thallus. Ecophysiological researches concerned both micro-climatic conditions' impact on primary production and lichens' adaptation to a very cold climate. One discovered a mechanism of two-phase hydratization/dehydratization of lichens' thallus. On the ground of palaeobotanical analyzes was reconstructed a development of flora in Western</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016CPL...652...50D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016CPL...652...50D"><span>Ultrafast vibrational energy flow in <span class="hlt">water</span> monomers in acetonitrile</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dahms, Fabian; Costard, Rene; Nibbering, Erik T. J.; Elsaesser, Thomas</p> <p>2016-05-01</p> <p>Vibrational relaxation of the OH stretching and bending <span class="hlt">modes</span> of <span class="hlt">water</span> monomers in acetonitrile is studied by two-color pump-probe experiments in a frequency range from 1400 to 3800 cm-1. Measurements with resonant infrared excitation reveal vibrational lifetimes of 6.4 ± 1.0 ps of the OH stretching <span class="hlt">modes</span> and 4.0 ± 0.5 ps of the OH bending <span class="hlt">mode</span>. After OH stretching excitation, the OH bending <span class="hlt">mode</span> shows an instantaneous response, a hallmark of the anharmonic coupling of stretching and bending <span class="hlt">modes</span>, and a delayed population buildup by relaxation of the stretching via the bending <span class="hlt">mode</span>. The relaxation steps are discussed within the framework of current theoretical pictures of <span class="hlt">water</span>'s vibrational relaxation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ECSS..191..125S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ECSS..191..125S"><span>Phytoplankton community structure is influenced by seabird guano enrichment in the Southern Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shatova, O. A.; Wing, S. R.; Hoffmann, L. J.; Wing, L. C.; Gault-Ringold, M.</p> <p>2017-05-01</p> <p>Phytoplankton biomass, productivity and community structure are strongly influenced by differences in nutrient concentrations among oceanographic <span class="hlt">water</span> masses. Changes in community composition, particularly in the distribution of cell sizes, can result in dramatic changes in the energetics of pelagic food webs and ecosystem function in terms of biogeochemical cycling and carbon sequestration. Here we examine responses of natural phytoplankton communities from four major <span class="hlt">water</span> masses in the Southern Ocean to enrichment from seabird guano, a concentrated source of bioactive metals (Mn, Fe, Co, Ni, Cu, Zn) and macronutrients (N, P), in a series of incubation experiments. Phytoplankton communities from sub-tropical <span class="hlt">water</span>, modified sub-tropical <span class="hlt">water</span> from the Snares Island wake, <span class="hlt">sub-Antarctic</span> <span class="hlt">water</span> and Antarctic <span class="hlt">water</span> from the Ross Sea, each showed dramatic changes in community structure following additions of seabird guano. We observed particularly high growth of prymnesiophytes in response to the guano-derived nutrients within <span class="hlt">sub-Antarctic</span> and sub-tropical frontal zones, resulting in communities dominated by larger cell sizes than in control incubations. Community changes within treatments enriched with guano were distinct, and in most cases more extensive, than those observed for treatments with additions of macronutrients (N, P) or iron (Fe) alone. These results provide the first empirical evidence that seabird guano enrichment can drive significant changes in the structure and composition of natural phytoplankton communities. Our findings have important implications for understanding the consequences of accumulation of bioactive metals and macronutrients within food webs and the role of seabirds as nutrient vectors within the Southern Ocean ecosystem.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29563248','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29563248"><span>Crossing the front: contrasting storm-forced dispersal dynamics revealed by biological, geological and genetic analysis of beach-cast kelp.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Waters, Jonathan M; King, Tania M; Fraser, Ceridwen I; Craw, Dave</p> <p>2018-03-01</p> <p>The subtropical front (STF) generally represents a substantial oceanographic barrier to dispersal between cold-sub-Antarctic and warm-temperate <span class="hlt">water</span> masses. Recent studies have suggested that storm events can drastically influence marine dispersal and patterns. Here we analyse biological and geological dispersal driven by two major, contrasting storm events in southern New Zealand, 2017. We integrate biological and physical data to show that a severe southerly system in July 2017 disrupted this barrier by promoting movement of substantial numbers of southern <span class="hlt">sub-Antarctic</span> Durvillaea kelp rafts across the STF, to make landfall in mainland NZ. By contrast, a less intense easterly storm (Cyclone Cook, April 2017) resulted in more moderate dispersal distances, with minimal dispersal between the <span class="hlt">sub-Antarctic</span> and mainland New Zealand. These quantitative analyses of approximately 200 freshly beach-cast kelp specimens indicate that storm intensity and wind direction can strongly influence marine dispersal and landfall outcomes. © 2018 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24369993','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24369993"><span>Benchmarking organic micropollutants in wastewater, recycled <span class="hlt">water</span> and drinking <span class="hlt">water</span> with in vitro bioassays.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Escher, Beate I; Allinson, Mayumi; Altenburger, Rolf; Bain, Peter A; Balaguer, Patrick; Busch, Wibke; Crago, Jordan; Denslow, Nancy D; Dopp, Elke; Hilscherova, Klara; Humpage, Andrew R; Kumar, Anu; Grimaldi, Marina; Jayasinghe, B Sumith; Jarosova, Barbora; Jia, Ai; Makarov, Sergei; Maruya, Keith A; Medvedev, Alex; Mehinto, Alvine C; Mendez, Jamie E; Poulsen, Anita; Prochazka, Erik; Richard, Jessica; Schifferli, Andrea; Schlenk, Daniel; Scholz, Stefan; Shiraishi, Fujio; Snyder, Shane; Su, Guanyong; Tang, Janet Y M; van der Burg, Bart; van der Linden, Sander C; Werner, Inge; Westerheide, Sandy D; Wong, Chris K C; Yang, Min; Yeung, Bonnie H Y; Zhang, Xiaowei; Leusch, Frederic D L</p> <p>2014-01-01</p> <p>Thousands of organic micropollutants and their transformation products occur in <span class="hlt">water</span>. Although often present at low concentrations, individual compounds contribute to mixture effects. Cell-based bioassays that target health-relevant biological endpoints may therefore complement chemical analysis for <span class="hlt">water</span> quality assessment. The objective of this study was to evaluate cell-based bioassays for their suitability to benchmark <span class="hlt">water</span> quality and to assess efficacy of <span class="hlt">water</span> treatment processes. The selected bioassays cover relevant steps in the toxicity pathways including induction of xenobiotic metabolism, specific and reactive <span class="hlt">modes</span> of toxic action, activation of adaptive stress response pathways and system responses. Twenty laboratories applied 103 unique in vitro bioassays to a common set of 10 <span class="hlt">water</span> samples collected in Australia, including wastewater treatment plant effluent, two types of recycled <span class="hlt">water</span> (reverse osmosis and ozonation/activated carbon filtration), stormwater, surface <span class="hlt">water</span>, and drinking <span class="hlt">water</span>. Sixty-five bioassays (63%) showed positive results in at least one sample, typically in wastewater treatment plant effluent, and only five (5%) were positive in the control (ultrapure <span class="hlt">water</span>). Each <span class="hlt">water</span> type had a characteristic bioanalytical profile with particular groups of toxicity pathways either consistently responsive or not responsive across test systems. The most responsive health-relevant endpoints were related to xenobiotic metabolism (pregnane X and aryl hydrocarbon receptors), hormone-mediated <span class="hlt">modes</span> of action (mainly related to the estrogen, glucocorticoid, and antiandrogen activities), reactive <span class="hlt">modes</span> of action (genotoxicity) and adaptive stress response pathway (oxidative stress response). This study has demonstrated that selected cell-based bioassays are suitable to benchmark <span class="hlt">water</span> quality and it is recommended to use a purpose-tailored panel of bioassays for routine monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27750127','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27750127"><span>Global resilience analysis of <span class="hlt">water</span> distribution systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Diao, Kegong; Sweetapple, Chris; Farmani, Raziyeh; Fu, Guangtao; Ward, Sarah; Butler, David</p> <p>2016-12-01</p> <p>Evaluating and enhancing resilience in <span class="hlt">water</span> infrastructure is a crucial step towards more sustainable urban <span class="hlt">water</span> management. As a prerequisite to enhancing resilience, a detailed understanding is required of the inherent resilience of the underlying system. Differing from traditional risk analysis, here we propose a global resilience analysis (GRA) approach that shifts the objective from analysing multiple and unknown threats to analysing the more identifiable and measurable system responses to extreme conditions, i.e. potential failure <span class="hlt">modes</span>. GRA aims to evaluate a system's resilience to a possible failure <span class="hlt">mode</span> regardless of the causal threat(s) (known or unknown, external or internal). The method is applied to test the resilience of four <span class="hlt">water</span> distribution systems (WDSs) with various features to three typical failure <span class="hlt">modes</span> (pipe failure, excess demand, and substance intrusion). The study reveals GRA provides an overview of a <span class="hlt">water</span> system's resilience to various failure <span class="hlt">modes</span>. For each failure <span class="hlt">mode</span>, it identifies the range of corresponding failure impacts and reveals extreme scenarios (e.g. the complete loss of <span class="hlt">water</span> supply with only 5% pipe failure, or still meeting 80% of demand despite over 70% of pipes failing). GRA also reveals that increased resilience to one failure <span class="hlt">mode</span> may decrease resilience to another and increasing system capacity may delay the system's recovery in some situations. It is also shown that selecting an appropriate level of detail for hydraulic models is of great importance in resilience analysis. The method can be used as a comprehensive diagnostic framework to evaluate a range of interventions for improving system resilience in future studies. Copyright © 2016 The Authors. Published by Elsevier Ltd.. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29530595','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29530595"><span>CW EPR parameters reveal cytochrome P450 ligand binding <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lockart, Molly M; Rodriguez, Carlo A; Atkins, William M; Bowman, Michael K</p> <p>2018-06-01</p> <p>Cytochrome P450 (CYP) monoxygenses utilize heme cofactors to catalyze oxidation reactions. They play a critical role in metabolism of many classes of drugs, are an attractive target for drug development, and mediate several prominent drug interactions. Many substrates and inhibitors alter the spin state of the ferric heme by displacing the heme's axial <span class="hlt">water</span> ligand in the resting enzyme to yield a five-coordinate iron complex, or they replace the axial <span class="hlt">water</span> to yield a nitrogen-ligated six-coordinate iron complex, which are traditionally assigned by UV-vis spectroscopy. However, crystal structures and recent pulsed electron paramagnetic resonance (EPR) studies find a few cases where molecules hydrogen bond to the axial <span class="hlt">water</span>. The <span class="hlt">water</span>-bridged drug-H 2 O-heme has UV-vis spectra similar to nitrogen-ligated, six-coordinate complexes, but are closer to "reverse type I" complexes described in older liteature. Here, pulsed and continuous wave (CW) EPR demonstrate that <span class="hlt">water</span>-bridged complexes are remarkably common among a range of nitrogenous drugs or drug fragments that bind to CYP3A4 or CYP2C9. Principal component analysis reveals a distinct clustering of CW EPR spectral parameters for <span class="hlt">water</span>-bridged complexes. CW EPR reveals heterogeneous mixtures of ligated states, including multiple directly-coordinated complexes and <span class="hlt">water</span>-bridged complexes. These results suggest that <span class="hlt">water</span>-bridged complexes are under-represented in CYP structural databases and can have energies similar to other ligation <span class="hlt">modes</span>. The data indicates that <span class="hlt">water</span>-bridged binding <span class="hlt">modes</span> can be identified and distinguished from directly-coordinated binding by CW EPR. Copyright © 2018 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1414098-low-frequency-ultrasonic-bessel-like-collimated-beam-generation-from-radial-modes-piezoelectric-transducers','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1414098-low-frequency-ultrasonic-bessel-like-collimated-beam-generation-from-radial-modes-piezoelectric-transducers"><span>Low-frequency ultrasonic Bessel-like collimated beam generation from radial <span class="hlt">modes</span> of piezoelectric transducers</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Chillara, Vamshi Krishna; Pantea, Cristian; Sinha, Dipen N.</p> <p>2017-02-06</p> <p>We present a very simple approach to generate a collimated ultrasonic beam that exploits the natural Bessel-like vibration pattern of the radial <span class="hlt">modes</span> of a piezoelectric disc with lateral clamping. This eliminates the need for the conventional annular Bessel pattern of the electrodes with individual electrode excitation on the piezo-disc, thus simplifying the transducer design. Numerical and experimental studies are carried out to investigate the Bessel-like vibration patterns of these radial <span class="hlt">modes</span> showing an excellent agreement between these two studies. Measured ultrasonic beam- pro les in <span class="hlt">water</span> from the radial <span class="hlt">modes</span> con rm the profile to be a Bessel beam.more » Collimated beam generation from radial <span class="hlt">modes</span> is investigated using a coupled electromechanical finite-element model. It is found that clamping the lateral edges of piezoelectric transducers results in a high-degree of collimation with practically no side-lobes similar to a parametric array beam. Ultrasonic beam- profile measurements in <span class="hlt">water</span> with both free and clamped piezoelectric transducer are presented. The collimated beam generation using the present technique of using the laterally clamped radial <span class="hlt">modes</span> finds significant applications in low-frequency imaging through highly attenuating materials.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1414098','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1414098"><span>Low-frequency ultrasonic Bessel-like collimated beam generation from radial <span class="hlt">modes</span> of piezoelectric transducers</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>Chillara, Vamshi Krishna; Pantea, Cristian; Sinha, Dipen N.</p> <p></p> <p>We present a very simple approach to generate a collimated ultrasonic beam that exploits the natural Bessel-like vibration pattern of the radial <span class="hlt">modes</span> of a piezoelectric disc with lateral clamping. This eliminates the need for the conventional annular Bessel pattern of the electrodes with individual electrode excitation on the piezo-disc, thus simplifying the transducer design. Numerical and experimental studies are carried out to investigate the Bessel-like vibration patterns of these radial <span class="hlt">modes</span> showing an excellent agreement between these two studies. Measured ultrasonic beam- pro les in <span class="hlt">water</span> from the radial <span class="hlt">modes</span> con rm the profile to be a Bessel beam.more » Collimated beam generation from radial <span class="hlt">modes</span> is investigated using a coupled electromechanical finite-element model. It is found that clamping the lateral edges of piezoelectric transducers results in a high-degree of collimation with practically no side-lobes similar to a parametric array beam. Ultrasonic beam- profile measurements in <span class="hlt">water</span> with both free and clamped piezoelectric transducer are presented. The collimated beam generation using the present technique of using the laterally clamped radial <span class="hlt">modes</span> finds significant applications in low-frequency imaging through highly attenuating materials.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JSSCh.230...61M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JSSCh.230...61M"><span>New <span class="hlt">water</span> soluble heterometallic complex showing unpredicted coordination <span class="hlt">modes</span> of EDTA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mudsainiyan, R. K.; Jassal, A. K.; Chawla, S. K.</p> <p>2015-10-01</p> <p>A mesoporous 3D polymeric complex (I) having formula {[Zr(IV)O-μ3-(EDTA)Fe(III)OH]·H2O}n has been crystallized and characterized by various techniques. Single-crystal X-ray diffraction analysis revealed that complex (I) crystallized in chiral monoclinic space group Cc (space group no. 9) with unexpected coordination <span class="hlt">modes</span> of EDTA and mixture of two transition metal ions. In this complex, the coordination number of Zr(IV) ion is seven where four carboxylate oxygen atoms, two nitrogen atoms, one oxide atom are coordinating with Zr(IV). Fe(III) is four coordinated and its coordination environment is composed of three different carboxylic oxygen atoms from three different EDTA and one oxygen atom of -OH group. The structure consists of 4-c and 16-c (2-nodal) net with new topology and point symbol for net is (336·454·530)·(36). TGA study and XRPD pattern showed that the coordination polymer is quite stable even after losing <span class="hlt">water</span> molecule and -OH ion. Quenching behavior in fluorescence of ligand is observed by complexation with transition metal ions is due to n-π* transition. The SEM micrograph shows the morphology of complex (I) exhibits spherical shape with size ranging from 50 to 280 nm. The minimum N2 (SBET=8.7693 m2/g) and a maximum amount of H2 (high surface area=1044.86 m2/g (STP)) could be adsorbed at 77 K. From DLS study, zeta potential is calculated i.e. -7.94 shows the negative charges on the surface of complex. Hirshfeld surface analysis and fingerprint plots revealed influence of weak or non bonding interactions in crystal packing of complex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OptCo.338..117K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OptCo.338..117K"><span>Lommel <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kovalev, Alexey A.; Kotlyar, Victor V.</p> <p>2015-03-01</p> <p>We study a non-paraxial family of nondiffracting laser beams whose complex amplitude is proportional to an n-th order Lommel function of two variables. These beams are referred to as Lommel <span class="hlt">modes</span>. Explicit analytical relations for the angular spectrum of plane waves and orbital angular momentum of the Lommel beams have been derived. The even (n=2p) and odd (n=2p+1) Lommel <span class="hlt">modes</span> are mutually orthogonal, as are the Lommel <span class="hlt">modes</span> characterized by different projections of the wave vector on the optical axis. At a definite parameter, the Lommel <span class="hlt">modes</span> change to conventional Bessel beams. Asymmetry of the Lommel <span class="hlt">modes</span> depends on a complex parameter с, with its modulus in the polar notation defining the intensity pattern in the beam‧s cross-section and the argument defining the angle of rotation of the intensity pattern about the optical axis. If the parameter с is real or purely imaginary, the transverse intensity component of the Lommel <span class="hlt">modes</span> is specularly symmetric about the Cartesian coordinate axes. Besides, with the modulus of the с parameter increasing from 0 to 1, the orbital angular momentum of the Lommel <span class="hlt">modes</span> increases from a finite value proportional to the topological charge n to infinity. The orbital angular momentum of the Lommel <span class="hlt">modes</span> undergoes continuous variations, in contrast to its discrete changes in the Bessel <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22308359-efficient-anharmonic-vibrational-spectroscopy-large-molecules-using-local-mode-coordinates','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22308359-efficient-anharmonic-vibrational-spectroscopy-large-molecules-using-local-mode-coordinates"><span>Efficient anharmonic vibrational spectroscopy for large molecules using local-<span class="hlt">mode</span> coordinates</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>Cheng, Xiaolu; Steele, Ryan P., E-mail: ryan.steele@utah.edu</p> <p></p> <p>This article presents a general computational approach for efficient simulations of anharmonic vibrational spectra in chemical systems. An automated local-<span class="hlt">mode</span> vibrational approach is presented, which borrows techniques from localized molecular orbitals in electronic structure theory. This approach generates spatially localized vibrational <span class="hlt">modes</span>, in contrast to the delocalization exhibited by canonical normal <span class="hlt">modes</span>. The method is rigorously tested across a series of chemical systems, ranging from small molecules to large <span class="hlt">water</span> clusters and a protonated dipeptide. It is interfaced with exact, grid-based approaches, as well as vibrational self-consistent field methods. Most significantly, this new set of reference coordinates exhibits a well-behavedmore » spatial decay of <span class="hlt">mode</span> couplings, which allows for a systematic, a priori truncation of <span class="hlt">mode</span> couplings and increased computational efficiency. Convergence can typically be reached by including <span class="hlt">modes</span> within only about 4 Å. The local nature of this truncation suggests particular promise for the ab initio simulation of anharmonic vibrational motion in large systems, where connection to experimental spectra is currently most challenging.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..133a2009H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..133a2009H"><span>Review on <span class="hlt">Water</span> Distribution of Cooling Tower in Power Station</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huichao, Zhang; Lei, Fang; Hao, Guang; Ying, Niu</p> <p>2018-04-01</p> <p>As the energy sources situation is becoming more and more severe, the importance of energy conservation and emissions reduction gets clearer. Since the optimization of <span class="hlt">water</span> distribution system of cooling tower in power station can save a great amount of energy, the research of <span class="hlt">water</span> distribution system gets more attention nowadays. This paper summarizes the development process of counter-flow type natural draft wet cooling tower and the <span class="hlt">water</span> distribution system, and introduces the related domestic and international research situation. Combining the current situation, we come to the conclusion about the advantages and disadvantages of the several major <span class="hlt">water</span> distribution <span class="hlt">modes</span>, and analyze the problems of the existing <span class="hlt">water</span> distribution ways in engineering application, furthermore, we put forward the direction of <span class="hlt">water</span> distribution <span class="hlt">mode</span> development on the basis knowledge of <span class="hlt">water</span> distribution of cooling tower. Due to the <span class="hlt">water</span> system can hardly be optimized again when it’s built, choosing an appropriate <span class="hlt">water</span> distribution <span class="hlt">mode</span> according to actual condition seems to be more significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29670417','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29670417"><span>Trophic ecology of two co-existing <span class="hlt">Sub-Antarctic</span> limpets of the genus Nacella: spatio-temporal variation in food availability and diet composition of Nacella magellanica and N. deaurata.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rosenfeld, Sebastián; Marambio, Johanna; Ojeda, Jaime; Juan Pablo Rodríguez; González-Wevar, Claudio; Gerard, Karin; Tamara Contador; Pizarro, Gemita; Mansilla, Andrés</p> <p>2018-01-01</p> <p>Interactions between algae and herbivores can be affected by various factors, such as seasonality and habitat structure. Among herbivores inhabiting marine systems, species of the order Patellogastropoda are considered key organisms in many rocky coasts of the world. Nacella species are one of the most dominant macro-herbivores on the rocky shores of the <span class="hlt">sub-Antarctic</span> ecoregion of Magellan. However, the importance of its key role must be associated with its trophic ecology. The objective of this work was to evaluate spatial and temporal variabilities in the dietary composition of two intertidal Nacella species, considering grazing on macro- (macroalgae) and microscopic (periphyton) food. The composition of periphyton and the availability of macroalgae in the winter and summer seasons were examined at two localities of the Magellanic province, alongside the gut contents of N. magellanica and N. deaurata . The dietary composition differed between the two Nacella species, as well as between seasons and locations. The differences observed in the diet of the two species of Nacella may be mainly due to their respective distributions in the intertidal zone. Both species presented a generalist strategy of grazing, which is relationed to the seasonality of micro- and macroalgae availability and to the variability of the assemblages between the localities. This research was the first to perform a detailed study of the diet of intertidal Nacella species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5904503','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5904503"><span>Trophic ecology of two co-existing <span class="hlt">Sub-Antarctic</span> limpets of the genus Nacella: spatio-temporal variation in food availability and diet composition of Nacella magellanica and N. deaurata</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rosenfeld, Sebastián; Marambio, Johanna; Ojeda, Jaime; Juan Pablo Rodríguez; González-Wevar, Claudio; Gerard, Karin; Tamara Contador; Pizarro, Gemita; Mansilla, Andrés</p> <p>2018-01-01</p> <p>Abstract Interactions between algae and herbivores can be affected by various factors, such as seasonality and habitat structure. Among herbivores inhabiting marine systems, species of the order Patellogastropoda are considered key organisms in many rocky coasts of the world. Nacella species are one of the most dominant macro-herbivores on the rocky shores of the <span class="hlt">sub-Antarctic</span> ecoregion of Magellan. However, the importance of its key role must be associated with its trophic ecology. The objective of this work was to evaluate spatial and temporal variabilities in the dietary composition of two intertidal Nacella species, considering grazing on macro- (macroalgae) and microscopic (periphyton) food. The composition of periphyton and the availability of macroalgae in the winter and summer seasons were examined at two localities of the Magellanic province, alongside the gut contents of N. magellanica and N. deaurata. The dietary composition differed between the two Nacella species, as well as between seasons and locations. The differences observed in the diet of the two species of Nacella may be mainly due to their respective distributions in the intertidal zone. Both species presented a generalist strategy of grazing, which is relationed to the seasonality of micro- and macroalgae availability and to the variability of the assemblages between the localities. This research was the first to perform a detailed study of the diet of intertidal Nacella species. PMID:29670417</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26832518','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26832518"><span>Adiabatically tapered microstructured <span class="hlt">mode</span> converter for selective excitation of the fundamental <span class="hlt">mode</span> in a few <span class="hlt">mode</span> fiber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Taher, Aymen Belhadj; Di Bin, Philippe; Bahloul, Faouzi; Tartaret-Josnière, Etienne; Jossent, Mathieu; Février, Sébastien; Attia, Rabah</p> <p>2016-01-25</p> <p>We propose a new technique to selectively excite the fundamental <span class="hlt">mode</span> in a few <span class="hlt">mode</span> fiber (FMF). This method of excitation is made from a single <span class="hlt">mode</span> fiber (SMF) which is inserted facing the FMF into an air-silica microstructured cane before the assembly is adiabatically tapered. We study theoretically and numerically this method by calculating the effective indices of the propagated <span class="hlt">modes</span>, their amplitudes along the taper and the adiabaticity criteria, showing the ability to achieve an excellent selective excitation of the fundamental <span class="hlt">mode</span> in the FMF with negligible loss. We experimentally demonstrate that the proposed solution provides a successful <span class="hlt">mode</span> conversion and allows an almost excellent fundamental <span class="hlt">mode</span> excitation in the FMF (representing 99.8% of the total power).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003Cryo...43..687Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003Cryo...43..687Y"><span>Investigation on the oscillation <span class="hlt">modes</span> in a thermoacoustic Stirling prime mover: <span class="hlt">mode</span> stability and <span class="hlt">mode</span> transition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Z. B.; Li, Q.; Chen, X.; Guo, F. Z.; Xie, X. J.; Wu, J. H.</p> <p>2003-12-01</p> <p>The purpose of this paper is to investigate the stability of oscillation <span class="hlt">modes</span> in a thermoacoustic Stirling prime mover, which is a combination of looped tube and resonator. Two <span class="hlt">modes</span>, with oscillation frequencies of 76 and 528 Hz, have been observed, stabilities of which are widely different. The stability of the high frequency <span class="hlt">mode</span> (HFM) is affected by low frequency <span class="hlt">mode</span> (LFM) strongly. Once the LFM is excited when the HFM is present, the HFM will be gradually slaved and suppressed by the LFM. The details of the transition from HFM to LFM have been described. The two stability curves of the two <span class="hlt">modes</span> have been measured. Mean pressure Pm is an important control parameter influencing the <span class="hlt">mode</span> stability in the tested system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APS..DFDE21004R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APS..DFDE21004R"><span>Characterization of Ventilatory <span class="hlt">Modes</span> in Dragonfly Nymph</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Roh, Chris; Saxton-Fox, Theresa; Gharib, Morteza</p> <p>2013-11-01</p> <p>A dragonfly nymph's highly modified hindgut has multiple ventilatory <span class="hlt">modes</span>: hyperventilation (i.e. jet propulsion), gulping ventilation (extended expiratory phase) and normal ventilation. Each <span class="hlt">mode</span> involves dynamic manipulation of the exit diameter and pressure. To study the different fluid dynamics associated with the three <span class="hlt">modes</span>, Anisopteran larvae of the family Aeshnidae were tethered onto a rod for flow visualization. The result showed distinct flow structures. The hyperventilation showed a highly turbulent and powerful jet that occurred at high frequency. The gulping ventilation produced a single vortex at a moderate frequency. The normal ventilation showed two distinct vortices, a low-Reynolds number vortex, followed by a high-Reynolds number vortex. Furthermore, a correlation of the formation of the vortices with the movement of the sternum showed that the dragonfly is actively controlling the timing and the speed of the vortices to have them at equal distance from the jet exit at the onset of inspiration. This behavior prevents inspiration of the oxygen deficient expirated <span class="hlt">water</span>, resulting in the maximization of the oxygen intake. Supported by NSF GRFP.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..186a2030E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..186a2030E"><span>Sliding <span class="hlt">mode</span> controller for a photovoltaic pumping system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>ElOugli, A.; Miqoi, S.; Boutouba, M.; Tidhaf, B.</p> <p>2017-03-01</p> <p>In this paper, a sliding <span class="hlt">mode</span> control scheme (SMC) for maximum power point tracking controller for a photovoltaic pumping system, is proposed. The main goal is to maximize the flow rate for a <span class="hlt">water</span> pump, by forcing the photovoltaic system to operate in its MPP, to obtain the maximum power that a PV system can deliver.And this, through the intermediary of a sliding <span class="hlt">mode</span> controller to track and control the MPP by overcoming the power oscillation around the operating point, which appears in most implemented MPPT techniques. The sliding <span class="hlt">mode</span> control approach is recognized as one of the efficient and powerful tools for nonlinear systems under uncertainty conditions.The proposed controller with photovoltaic pumping system is designed and simulated using MATLAB/SIMULINK environment. In addition, to evaluate its performances, a classical MPPT algorithm using perturb and observe (P&O) has been used for the same system to compare to our controller. Simulation results are shown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25320998','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25320998"><span>PLC-based LP₁₁ <span class="hlt">mode</span> rotator for <span class="hlt">mode</span>-division multiplexing transmission.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Saitoh, Kunimasa; Uematsu, Takui; Hanzawa, Nobutomo; Ishizaka, Yuhei; Masumoto, Kohei; Sakamoto, Taiji; Matsui, Takashi; Tsujikawa, Kyozo; Yamamoto, Fumihiko</p> <p>2014-08-11</p> <p>A PLC-based LP11 <span class="hlt">mode</span> rotator is proposed. The proposed <span class="hlt">mode</span> rotator is composed of a waveguide with a trench that provides asymmetry of the waveguide. Numerical simulations show that converting LP11a (LP11b) <span class="hlt">mode</span> to LP11b (LP11a) <span class="hlt">mode</span> can be achieved with high conversion efficiency (more than 90%) and little polarization dependence over a wide wavelength range from 1450 nm to 1650 nm. In addition, we fabricate the proposed LP11 <span class="hlt">mode</span> rotator using silica-based PLC. It is confirmed that the fabricated <span class="hlt">mode</span> rotator can convert LP11a <span class="hlt">mode</span> to LP11b <span class="hlt">mode</span> over a wide wavelength range.</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/2017EPJAP..8020501Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJAP..8020501Y"><span>Competition and evolution of dielectric waveguide <span class="hlt">mode</span> and plasmonic waveguide <span class="hlt">mode</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, Sheng-Nan; Fang, Yun-Tuan</p> <p>2017-10-01</p> <p>In order to study the coupling and evolution law of the waveguide <span class="hlt">mode</span> and two plasmonic surface <span class="hlt">modes</span>, we construct a line defect waveguide based on hexagonal honeycomb plasmonic photonic crystal. Through adjusting the radius of the edge dielectric rods, the competition and evolution behaviors occur between dielectric waveguide <span class="hlt">mode</span> and plasmonic waveguide <span class="hlt">mode</span>. There are three status: only plasmonic waveguide <span class="hlt">modes</span> occur for rA < 0.09a; only dielectric waveguide <span class="hlt">modes</span> occur for rA > 0.25a; two kinds of <span class="hlt">modes</span> coexist for 0.09a < rA < 0.25a. The plasmonic waveguide <span class="hlt">mode</span> has advantages in achieving slow light.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........50E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........50E"><span>Understanding the dielectric properties of <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elton, Daniel Christopher</p> <p></p> <p>Liquid <span class="hlt">water</span> is a complex material with many anomalous properties. Three of these anomalies are an abnormally high dielectric constant, an abnormally high boiling point, and a solid phase which is less dense than the liquid phase. Each of these anomalies is known to have been critically important in the development of life on Earth. All of <span class="hlt">water</span>'s special properties can be linked to <span class="hlt">water</span>'s unique ability to form hydrogen bonds. <span class="hlt">Water</span>'s hydrogen bonds form a transient network. Understanding the average structure of this network and how it changes through the phase diagram remains the focus of intense research. In this thesis we focus on understanding dielectric and infrared measurements, which measure the absorption and refraction of electromagnetic waves at different frequencies. Computer simulation is a necessary tool for correctly interpreting these measurements in terms of the microscopic dynamics of molecules. In the first part of this thesis we compare three classes of <span class="hlt">water</span> molecule model that are used in molecular dynamics simulation--rigid, flexible, and polarizable. We show how the inclusion of polarization is necessary to capture how <span class="hlt">water</span>'s properties change with pressure and temperature. This finding is relevant to biophysical simulation. In the next part, we conduct a detailed study of <span class="hlt">water</span>'s dielectric properties to discover vibrational <span class="hlt">modes</span> that propagate through the hydrogen bond network. Parts of the absorption spectrum of <span class="hlt">water</span> are due to electromagnetic waves coupling to these <span class="hlt">modes</span>. Previously, vibrational motions in <span class="hlt">water</span> were thought to be confined to small clusters of perhaps five molecules. Our work upends this view by arguing that dynamics occur on the hydrogen bond network, resulting in <span class="hlt">modes</span> that can propagate surprisingly long distances of up to two nanometers. These <span class="hlt">modes</span> bear many similarities to optical phonon <span class="hlt">modes</span> in ice. We show how the LO-TO splitting of these <span class="hlt">modes</span> provides a new window into the structure of the hydrogen bond</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013vftl.book..119L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013vftl.book..119L"><span>Single-<span class="hlt">Mode</span> VCSELs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Larsson, Anders; Gustavsson, Johan S.</p> <p></p> <p>The only active transverse <span class="hlt">mode</span> in a truly single-<span class="hlt">mode</span> VCSEL is the fundamental <span class="hlt">mode</span> with a near Gaussian field distribution. A single-<span class="hlt">mode</span> VCSEL produces a light beam of higher spectral purity, higher degree of coherence and lower divergence than a multimode VCSEL and the beam can be more precisely shaped and focused to a smaller spot. Such beam properties are required in many applications. In this chapter, after discussing applications of single-<span class="hlt">mode</span> VCSELs, we introduce the basics of fields and <span class="hlt">modes</span> in VCSELs and review designs implemented for single-<span class="hlt">mode</span> emission from VCSELs in different materials and at different wavelengths. This includes VCSELs that are inherently single-<span class="hlt">mode</span> as well as inherently multimode VCSELs where higher-order <span class="hlt">modes</span> are suppressed by <span class="hlt">mode</span> selective gain or loss. In each case we present the current state-of-the-art and discuss pros and cons. At the end, a specific example with experimental results is provided and, as a summary, the most promising designs based on current technologies are identified.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012APS..DFDH15009Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012APS..DFDH15009Y"><span>Jumping of <span class="hlt">water</span> striders on <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Eunjin; Son, Jaehak; Jablonski, Piotr; Kim, Ho-Young</p> <p>2012-11-01</p> <p>Small insects such as <span class="hlt">water</span> striders, springtails, fishing spiders freely move on <span class="hlt">water</span> by adopting various <span class="hlt">modes</span> of locomotion, such as rowing, galloping, jumping and meniscus-climbing. As the physics of jumping have not yet been fully understood among those ways of semi-aquatic propulsion, here we present the results of a combined experimental and theoretical investigation of the dynamics of <span class="hlt">water</span> striders leaping off <span class="hlt">water</span>. We first image and analyze the trajectories of the legs and body of jumping <span class="hlt">water</span> striders of three different species with a high-speed camera. We then theoretically compute the forces acting on the body by considering the capillary interaction between the flexible legs and deforming <span class="hlt">water</span> meniscus. Our theory enables us to predict the maximum take-off speed for given leg lengths. The experimental measurements suggest that the <span class="hlt">water</span> striders drive their legs near the optimal speed to gain the maximum take-off speed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1999JGR...10420949M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1999JGR...10420949M"><span>Distribution of oxygen isotopes in the <span class="hlt">water</span> masses of Drake Passage and 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>Meredith, Michael P.; Grose, Katie E.; McDonagh, Elaine L.; Heywood, Karen J.; Frew, Russell D.; Dennis, Paul F.</p> <p>1999-09-01</p> <p>Measurements of the ratio of stable isotopes of oxygen (18O and 16O) from samples collected on World Ocean Circulation Experiment sections SR1b (eastern Drake Passage) and A11 (Punta Arenas to Cape Town) are used, together with hydrographic data, to deduce information about the formation and variability of South Atlantic and Southern Ocean <span class="hlt">water</span> masses. The Drake Passage surface <span class="hlt">waters</span> south of the Polar Front (PF) are isotopically light (δ18O around -0.4‰) owing to the influence of meteoric <span class="hlt">waters</span>. The salinity and δ18O of the A11 surface <span class="hlt">waters</span> yield an apparent freshwater end-member which is much isotopically lighter than the local precipitation, thus advection of these <span class="hlt">waters</span> from farther south dominates over local effects in determining the surface <span class="hlt">water</span> properties. The Drake Passage section shows unusual proximity of the two main fronts of the Antarctic Circumpolar Current (the PF and <span class="hlt">Subantarctic</span> Front (SAF)), and we observe cold, fresh, and isotopically light <span class="hlt">water</span> derived from the temperature-minimum Winter <span class="hlt">Water</span> at the SAF. This <span class="hlt">water</span> is of the correct density to freshen the intermediate <span class="hlt">water</span> north of the SAF and thus play a role in the formation of the comparatively fresh Antarctic Intermediate <span class="hlt">Water</span> (AAIW) of the South Atlantic. This confirms the role of Antarctic <span class="hlt">water</span> in forming the South Atlantic variety of AAIW. Across the A11 section the oxygen isotope and salinity data at the AAIW core show very similar traces, with <span class="hlt">waters</span> in the Malvinas Current loop showing lowest values of both. At the eastern boundary of the South Atlantic, the input of Red Sea <span class="hlt">Water</span> from east of South Africa is observed via the presence of anomalously isotopically heavy AAIW. We deduce potentially significant temporal variability in the isotopic composition of Weddell Sea Deep <span class="hlt">Water</span> (WSDW) by comparing the Drake Passage data to earlier data covering the outflow of the Weddell Sea. The A11 data show WSDW consistent with such variability, indicating that its effects could</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JGRD..11723110S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JGRD..11723110S"><span>Validation of <span class="hlt">Mode-S</span> Meteorological Routine Air Report aircraft observations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strajnar, B.</p> <p>2012-12-01</p> <p>The success of mesoscale data assimilation depends on the availability of three-dimensional observations with high spatial and temporal resolution. This paper describes an example of such observations, available through <span class="hlt">Mode-S</span> air traffic control system composed of ground radar and transponders on board the aircraft. The meteorological information is provided by interrogation of a dedicated meteorological data register, called Meteorological Routine Air Report (MRAR). MRAR provides direct measurements of temperature and wind, but is only returned by a small fraction of aircraft. The quality of <span class="hlt">Mode-S</span> MRAR data, collected at the Ljubljana Airport, Slovenia, is assessed by its comparison with AMDAR and high-resolution radiosonde data sets, which enable high- and low-level validation, respectively. The need for temporal smoothing of raw <span class="hlt">Mode-S</span> MRAR data is also studied. The standard deviation of differences between smoothed <span class="hlt">Mode-S</span> MRAR and AMDAR is 0.35°C for temperature, 0.8 m/s for wind speed and below 10 degrees for wind direction. The differences with respect to radiosondes are larger, with standard deviations of approximately 1.7°C, 3 m/s and 25 degrees for temperature, wind speed and wind direction, respectively. It is concluded that both wind and temperature observations from <span class="hlt">Mode-S</span> MRAR are accurate and therefore potentially very useful for data assimilation in numerical weather prediction models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17578590','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17578590"><span>Parasites as biological tags for stock discrimination in marine fish from South American Atlantic <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Timi, Juan T</p> <p>2007-06-01</p> <p>The use of parasites as biological tags in population studies of marine fish in the south-western Atlantic has proved to be a successful tool for discriminating stocks for all species to which it has been applied, namely: Scomber japonicus, Engraulis anchoita, Merluccius hubbsi and Cynoscion guatucupa, the latter studied on a broader geographic scale, including samples from Uruguayan and Brazilian <span class="hlt">waters</span>. The distribution patterns of marine parasites are determined mainly by temperature-salinity profiles and by their association with specific masses of <span class="hlt">water</span>. Analyses of distribution patterns of some parasite species in relation to gradients in environmental (oceanographic) conditions showed that latitudinal gradients in parasite distribution are common in the study area, and are probably directly related to <span class="hlt">water</span> temperature. Indeed, temperature, which is a good predictor of latitudinal gradients of richness and diversity of species, shows a latitudinal pattern in south-western Atlantic coasts, decreasing southwards, due to the influence of subtropical and <span class="hlt">subantarctic</span> marine currents flowing along the edge of the continental slope. This pattern also determines the distribution of zooplankton, with a characteristic specific composition in different <span class="hlt">water</span> masses. The gradient in the distribution of parasites determines differential compositions of their communities at different latitudes, which makes possible the identification of different stocks of their fish hosts. Other features of the host-parasite systems contributing to the success of the parasitological method are: (1) parasites identified as good biological tags (i.e. anisakids) are widely distributed in the local fauna; (2) many of these species show low specificity and use paratenic hosts; and (3) the structure of parasite communities are, to a certain degree, predictable in time and space.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E3SWC..3804011Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E3SWC..3804011Z"><span>Connection Analysis of Different <span class="hlt">Modes</span> in Multimodal Transport</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhao, Zhi; Lu, Ya Ya; Liu, Xing Hua; Jiang, Ying; Zhang, Yan Zhou</p> <p>2018-06-01</p> <p>As the most advanced way of transport organization, container multimodal transport provides high quality and efficient systematic logistics transportation services in a wide range of freight transport activities. So it has been widely promoted worldwide. China is in a period of sustained and rapid economic development, which needs greater support from logistics, while the rationalization of multimodal transport enables the best transport area of each transportation <span class="hlt">mode</span> to be reflected. This paper makes an analysis of the connection between united transportation of railway and highway, rail and <span class="hlt">water</span> transport and untied transportation of highway and <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28788733','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28788733"><span>Linearly polarized vector <span class="hlt">modes</span>: enabling MIMO-free <span class="hlt">mode</span>-division multiplexing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Lixian; Nejad, Reza Mirzaei; Corsi, Alessandro; Lin, Jiachuan; Messaddeq, Younès; Rusch, Leslie; LaRochelle, Sophie</p> <p>2017-05-15</p> <p>We experimentally investigate <span class="hlt">mode</span>-division multiplexing in an elliptical ring core fiber (ERCF) that supports linearly polarized vector <span class="hlt">modes</span> (LPV). Characterization show that the ERCF exhibits good polarization maintaining properties over eight LPV <span class="hlt">modes</span> with effective index difference larger than 1 × 10 -4 . The ERCF further displays stable <span class="hlt">mode</span> power and polarization extinction ratio when subjected to external perturbations. Crosstalk between the LPV <span class="hlt">modes</span>, after propagating through 0.9 km ERCF, is below -14 dB. By using six LPV <span class="hlt">modes</span> as independent data channels, we achieved the transmission of 32 Gbaud QPSK over 0.9 km ERCF without any multiple-input-multiple-output (MIMO) or polarization-division multiplexing (PDM) signal processing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100014091','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100014091"><span>Few-<span class="hlt">Mode</span> Whispering-Gallery-<span class="hlt">Mode</span> Resonators</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Savchenkov, Anatoliy; Strekalov, Dmitry; Matsko, Andrey; Iltchenko, Vladimir; Maleki, Lute</p> <p>2006-01-01</p> <p>Whispering-gallery-<span class="hlt">mode</span> (WGM) optical resonators of a type now under development are designed to support few well-defined waveguide <span class="hlt">modes</span>. In the simplest case, a resonator of this type would support one equatorial family of WGMs; in a more complex case, such a resonator would be made to support two, three, or some other specified finite number of <span class="hlt">modes</span>. Such a resonator can be made of almost any transparent material commonly used in optics. The nature of the supported <span class="hlt">modes</span> does not depend on which material is used, and the geometrical dispersion of this resonator is much smaller than that of a typical prior WGM resonator. Moreover, in principle, many such resonators could be fabricated as integral parts of a single chip. Basically, a resonator of this type consists of a rod, made of a suitable transparent material, from which protrudes a thin circumferential belt of the same material. The belt is integral with the rest of the rod (see figure) and acts as a circumferential waveguide. If the depth (d) and width (w) of the belt are made appropriately small, then the belt acts as though it were the core of a single-<span class="hlt">mode</span> optical fiber: the belt and its adjacent supporting rod material support a single, circumferentially propagating <span class="hlt">mode</span> or family of <span class="hlt">modes</span>. It has been shown theoretically that the fiber-optic-like behavior of the belton- rod resonator structure can be summarized, in part, by the difference, Dn, between (1) an effective index of refraction of an imaginary fiber core and (2) the index of refraction (n) of the transparent rod/belt material. It has also been shown theoretically that for a given required value of Dn, the required depth of the belt can be estimated as d R Dn, where R is the radius of the rod. It must be emphasized that this estimated depth is independent of n and, hence, is independent of the choice of rod material. As in the cases of prior WGM resonators, input/output optical coupling involves utilization of evanescent fields. In the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=278258&Lab=NHEERL&keyword=bioremediation&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=278258&Lab=NHEERL&keyword=bioremediation&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>Integrated <span class="hlt">water</span> quality, emergy and economic evaluation of three bioremediation treatment systems for eutrophic <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>This study was targeted at finding one or more environmentally efficient, economically feasible and ecologically sustainable bioremediation treatment <span class="hlt">modes</span> for eutrophic <span class="hlt">water</span>. Three biological species, i.e. <span class="hlt">water</span> spinach (Ipomoea aquatica), loach (Misgurus anguillicaudatus) and ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29028041','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29028041"><span>Comparing <span class="hlt">mode</span>-crosstalk and <span class="hlt">mode</span>-dependent loss of laterally displaced orbital angular momentum and Hermite-Gaussian <span class="hlt">modes</span> for free-space optical communication.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ndagano, Bienvenu; Mphuthi, Nokwazi; Milione, Giovanni; Forbes, Andrew</p> <p>2017-10-15</p> <p>There is interest in using orbital angular momentum (OAM) <span class="hlt">modes</span> to increase the data speed of free-space optical communication. A prevalent challenge is the mitigation of <span class="hlt">mode</span>-crosstalk and <span class="hlt">mode</span>-dependent loss that is caused by the <span class="hlt">modes</span>' lateral displacement at the data receiver. Here, the <span class="hlt">mode</span>-crosstalk and <span class="hlt">mode</span>-dependent loss of laterally displaced OAM <span class="hlt">modes</span> (LG 0,+1 , LG 0,-1 ) are experimentally compared to that of a Hermite-Gaussian (HG) <span class="hlt">mode</span> subset (HG 0,1 , HG 1,0 ). It is shown, for an aperture larger than the <span class="hlt">modes</span>' waist sizes, some of the HG <span class="hlt">modes</span> can experience less <span class="hlt">mode</span>-crosstalk and <span class="hlt">mode</span>-dependent loss when laterally displaced along a symmetry axis. It is also shown, over a normal distribution of lateral displacements whose standard deviation is 2× the <span class="hlt">modes</span>' waist sizes, on average, the HG <span class="hlt">modes</span> experience 66% less <span class="hlt">mode</span>-crosstalk and 17% less <span class="hlt">mode</span>-dependent loss.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMPP41C..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMPP41C..07W"><span>Pacific patterns of dust deposition, iron supply and export production</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Winckler, G.; Anderson, R. F.; Park, J.; Schwartz, R.; Pahnke, K.; Struve, T.; Lamy, F.; Gersonde, R.</p> <p>2015-12-01</p> <p>The scarcity of iron limits marine export production and carbon uptake in about a quarter of the global ocean where the surface concentration of nitrate and phosphate is high, as biological utilization of these macronutrients is incomplete. Of these high nutrient low chlorophyll (HNLC) regions, the Southern Ocean is the region where variations in iron availability can have the largest effect on Earth's carbon cycle through its fertilizing effect on marine ecosystems, both in the modern and in the past. Recent work in the <span class="hlt">Subantarctic</span> South Atlantic (Martínez-Garcia et al., 2009, 2014, Anderson et al., 2014) suggests that dust-driven iron fertilization lowered atmospheric CO2 by up to 40 ppm in the latter half of each glacial cycle of the late Pleistocene, with the increase in <span class="hlt">Subantarctic</span> productivity consuming a greater fraction of the surface nutrients and thus driving more storage of carbon in the ocean interior. The other sectors of the Southern Ocean remain poorly constrained, including the Pacific Sector, that accounts for the largest surface area of the <span class="hlt">Subantarctic</span> Southern Ocean. Here we report records of dust deposition, iron supply and export production from a set of cores from the <span class="hlt">Subantarctic</span> Pacific (PS75, Lamy et al 2014) and initial results about the origin of dust transported to the <span class="hlt">Subantarctic</span> Pacific Ocean from radiogenic isotopes and rare earth elements. We test how tightly dust and biological productivity are coupled over glacial/interglacial and millennial timescales in the <span class="hlt">Subantarctic</span> Pacific and place the region in a context of global patterns of biological productivity, nutrient utilization and iron fertilization by dust, including comparisons to the other Pacific HNLC regions, the Subarctic North Pacific and equatorial Pacific.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25606998','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25606998"><span>Variable optical attenuator and dynamic <span class="hlt">mode</span> group equalizer for few <span class="hlt">mode</span> fibers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Blau, Miri; Weiss, Israel; Gerufi, Jonathan; Sinefeld, David; Bin-Nun, Moran; Lingle, Robert; Grüner-Nielsen, Lars; Marom, Dan M</p> <p>2014-12-15</p> <p>Variable optical attenuation (VOA) for three-<span class="hlt">mode</span> fiber is experimentally presented, utilizing an amplitude spatial light modulator (SLM), achieving up to -28dB uniform attenuation for all <span class="hlt">modes</span>. Using the ability to spatially vary the attenuation distribution with the SLM, we also achieve up to 10dB differential attenuation between the fiber's two supported <span class="hlt">mode</span> group (LP₀₁ and LP₁₁). The spatially selective attenuation serves as the basis of a dynamic <span class="hlt">mode</span>-group equalizer (DME), potentially gain-balancing <span class="hlt">mode</span> dependent optical amplification. We extend the experimental three <span class="hlt">mode</span> DME functionality with a performance analysis of a fiber supporting 6 spatial <span class="hlt">modes</span> in four <span class="hlt">mode</span> groups. The spatial <span class="hlt">modes</span>' distribution and overlap limit the available dynamic range and performance of the DME in the higher <span class="hlt">mode</span> count case.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28433032','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28433032"><span>IR spectral assignments for the hydrated excess proton in liquid <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Biswas, Rajib; Carpenter, William; Fournier, Joseph A; Voth, Gregory A; Tokmakoff, Andrei</p> <p>2017-04-21</p> <p>The local environmental sensitivity of infrared (IR) spectroscopy to a hydrogen-bonding structure makes it a powerful tool for investigating the structure and dynamics of excess protons in <span class="hlt">water</span>. Although of significant interest, the line broadening that results from the ultrafast evolution of different solvated proton-<span class="hlt">water</span> structures makes the assignment of liquid-phase IR spectra a challenging task. In this work, we apply a normal <span class="hlt">mode</span> analysis using density functional theory of thousands of proton-<span class="hlt">water</span> clusters taken from reactive molecular dynamics trajectories of the latest generation multistate empirical valence bond proton model (MS-EVB 3.2). These calculations are used to obtain a vibrational density of states and IR spectral density, which are decomposed on the basis of solvated proton structure and the frequency dependent <span class="hlt">mode</span> character. Decompositions are presented on the basis of the proton sharing parameter δ, often used to distinguish Eigen and Zundel species, the stretch and bend character of the <span class="hlt">modes</span>, the <span class="hlt">mode</span> delocalization, and the vibrational <span class="hlt">mode</span> symmetry. We find there is a wide distribution of vibrational frequencies spanning 1200-3000 cm -1 for every local proton configuration, with the region 2000-2600 cm -1 being mostly governed by the distorted Eigen-like configuration. We find a continuous red shift of the special-pair O⋯H + ⋯O stretching frequency, and an increase in the flanking <span class="hlt">water</span> bending intensity with decreasing δ. Also, we find that the flanking <span class="hlt">water</span> stretch <span class="hlt">mode</span> of the Zundel-like species is strongly mixed with the flanking <span class="hlt">water</span> bend, and the special pair proton oscillation band is strongly coupled with the bend <span class="hlt">modes</span> of the central H 5 O2+moiety.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JChPh.146o4507B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JChPh.146o4507B"><span>IR spectral assignments for the hydrated excess proton in liquid <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Biswas, Rajib; Carpenter, William; Fournier, Joseph A.; Voth, Gregory A.; Tokmakoff, Andrei</p> <p>2017-04-01</p> <p>The local environmental sensitivity of infrared (IR) spectroscopy to a hydrogen-bonding structure makes it a powerful tool for investigating the structure and dynamics of excess protons in <span class="hlt">water</span>. Although of significant interest, the line broadening that results from the ultrafast evolution of different solvated proton-<span class="hlt">water</span> structures makes the assignment of liquid-phase IR spectra a challenging task. In this work, we apply a normal <span class="hlt">mode</span> analysis using density functional theory of thousands of proton-<span class="hlt">water</span> clusters taken from reactive molecular dynamics trajectories of the latest generation multistate empirical valence bond proton model (MS-EVB 3.2). These calculations are used to obtain a vibrational density of states and IR spectral density, which are decomposed on the basis of solvated proton structure and the frequency dependent <span class="hlt">mode</span> character. Decompositions are presented on the basis of the proton sharing parameter δ, often used to distinguish Eigen and Zundel species, the stretch and bend character of the <span class="hlt">modes</span>, the <span class="hlt">mode</span> delocalization, and the vibrational <span class="hlt">mode</span> symmetry. We find there is a wide distribution of vibrational frequencies spanning 1200-3000 cm-1 for every local proton configuration, with the region 2000-2600 cm-1 being mostly governed by the distorted Eigen-like configuration. We find a continuous red shift of the special-pair O⋯H+⋯O stretching frequency, and an increase in the flanking <span class="hlt">water</span> bending intensity with decreasing δ. Also, we find that the flanking <span class="hlt">water</span> stretch <span class="hlt">mode</span> of the Zundel-like species is strongly mixed with the flanking <span class="hlt">water</span> bend, and the special pair proton oscillation band is strongly coupled with the bend <span class="hlt">modes</span> of the central H5+O2 moiety.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhPl...22i2111U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhPl...22i2111U"><span>Helicon <span class="hlt">modes</span> in uniform plasmas. I. Low m <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Urrutia, J. M.; Stenzel, R. L.</p> <p>2015-09-01</p> <p>Helicons are whistler <span class="hlt">modes</span> with azimuthal wave numbers. They arise in bounded gaseous and solid state plasmas, but the present work shows that very similar <span class="hlt">modes</span> also exist in unbounded uniform plasmas. The antenna properties determine the <span class="hlt">mode</span> structure. A simple antenna is a magnetic loop with dipole moment aligned either along or across the ambient background magnetic field B0. For such configurations, the wave magnetic field has been measured in space and time in a large and uniform laboratory plasma. The observed wave topology for a dipole along B0 is similar to that of an m = 0 helicon <span class="hlt">mode</span>. It consists of a sequence of alternating whistler vortices. For a dipole across B0, an m = 1 <span class="hlt">mode</span> is excited which can be considered as a transverse vortex which rotates around B0. In m = 0 <span class="hlt">modes</span>, the field lines are confined to each half-wavelength vortex while for m = 1 <span class="hlt">modes</span> they pass through the entire wave train. A subset of m = 1 field lines forms two nested helices which rotate in space and time like corkscrews. Depending on the type of the antenna, both m = + 1 and m = -1 <span class="hlt">modes</span> can be excited. Helicons in unbounded plasmas also propagate transverse to B0. The transverse and parallel wave numbers are about equal and form oblique phase fronts as in whistler Gendrin <span class="hlt">modes</span>. By superimposing small amplitude fields of several loop antennas, various antenna combinations have been created. These include rotating field antennas, helical antennas, and directional antennas. The radiation efficiency is quantified by the radiation resistance. Since helicons exist in unbounded laboratory plasmas, they can also arise in space plasmas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29428168','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29428168"><span>Pulmonary Capillary Hemorrhage Induced by Different Imaging <span class="hlt">Modes</span> of Diagnostic Ultrasound.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Miller, Douglas L; Dong, Zhihong; Dou, Chunyan; Raghavendran, Krishnan</p> <p>2018-05-01</p> <p>The induction of pulmonary capillary hemorrhage (PCH) is a well-established non-thermal biological effect of pulsed ultrasound in animal models. Typically, research has been done using laboratory pulsed ultrasound systems with a fixed beam and, recently, by B-<span class="hlt">mode</span> diagnostic ultrasound. In this study, a GE Vivid 7 Dimension ultrasound machine with 10 L linear array probe was used at 6.6 MHz to explore the relative PCH efficacy of B-<span class="hlt">mode</span> imaging, M-<span class="hlt">mode</span> (fixed beam), color angio <span class="hlt">mode</span> Doppler imaging and pulsed Doppler <span class="hlt">mode</span> (fixed beam). Anesthetized rats were scanned in a warmed <span class="hlt">water</span> bath, and thresholds were determined by scanning at different power steps, 2 dB apart, in different groups of six rats. Exposures were performed for 5 min, except for a 15-s M-<span class="hlt">mode</span> group. Peak rarefactional pressure amplitude thresholds were 1.5 MPa for B-<span class="hlt">mode</span> and 1.1 MPa for angio Doppler <span class="hlt">mode</span>. For the non-scanned <span class="hlt">modes</span>, thresholds were 1.1 MPa for M-<span class="hlt">mode</span> and 0.6 MPa for pulsed Doppler <span class="hlt">mode</span> with its relatively high duty cycle (7.7 × 10 -3 vs. 0.27 × 10 -3 for M-<span class="hlt">mode</span>). Reducing the duration of M-<span class="hlt">mode</span> to 15 s (from 300 s) did not significantly reduce PCH (area, volume or depth) for some power settings, but the threshold was increased to 1.4 MPa. Pulmonary sonographers should be aware of this unique adverse bio-effect of diagnostic ultrasound and should consider reduced on-screen mechanical index settings for potentially vulnerable patients. Copyright © 2018 World Federation for Ultrasound in Medicine and Biology. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Hydrology&pg=7&id=ED067252','ERIC'); return false;" href="https://eric.ed.gov/?q=Hydrology&pg=7&id=ED067252"><span>Scientific Allocation of <span class="hlt">Water</span> Resources.</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>Buras, Nathan</p> <p></p> <p>Oriented for higher education students, researchers, practicing engineers and planners, this book surveys the state of the art of <span class="hlt">water</span> resources engineering. A broad spectrum of issues is embraced in the treatment of <span class="hlt">water</span> resources: quantity aspects as well as quality aspects within a systems approach. Using a rational <span class="hlt">mode</span> for <span class="hlt">water</span> resources…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013JChPh.138q4108C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JChPh.138q4108C"><span>Computational IR spectroscopy of <span class="hlt">water</span>: OH stretch frequencies, transition dipoles, and intermolecular vibrational coupling constants</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Choi, Jun-Ho; Cho, Minhaeng</p> <p>2013-05-01</p> <p>The Hessian matrix reconstruction method initially developed to extract the basis <span class="hlt">mode</span> frequencies, vibrational coupling constants, and transition dipoles of the delocalized amide I, II, and III vibrations of polypeptides and proteins from quantum chemistry calculation results is used to obtain those properties of delocalized O-H stretch <span class="hlt">modes</span> in liquid <span class="hlt">water</span>. Considering the <span class="hlt">water</span> symmetric and asymmetric O-H stretch <span class="hlt">modes</span> as basis <span class="hlt">modes</span>, we here develop theoretical models relating vibrational frequencies, transition dipoles, and coupling constants of basis <span class="hlt">modes</span> to local <span class="hlt">water</span> configuration and solvent electric potential. Molecular dynamics simulation was performed to generate an ensemble of <span class="hlt">water</span> configurations that was in turn used to construct vibrational Hamiltonian matrices. Obtaining the eigenvalues and eigenvectors of the matrices and using the time-averaging approximation method, which was developed by the Skinner group, to calculating the vibrational spectra of coupled oscillator systems, we could numerically simulate the O-H stretch IR spectrum of liquid <span class="hlt">water</span>. The asymmetric line shape and weak shoulder bands were quantitatively reproduced by the present computational procedure based on vibrational exciton model, where the polarization effects on basis <span class="hlt">mode</span> transition dipoles and inter-<span class="hlt">mode</span> coupling constants were found to be crucial in quantitatively simulating the vibrational spectra of hydrogen-bond networking liquid <span class="hlt">water</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_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('https://www.osti.gov/biblio/22590538-mode-coupling-hybrid-square-rectangular-lasers-single-mode-operation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22590538-mode-coupling-hybrid-square-rectangular-lasers-single-mode-operation"><span><span class="hlt">Mode</span> coupling in hybrid square-rectangular lasers for single <span class="hlt">mode</span> operation</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>Ma, Xiu-Wen; Huang, Yong-Zhen, E-mail: yzhuang@semi.ac.cn; Yang, Yue-De</p> <p></p> <p><span class="hlt">Mode</span> coupling between a square microcavity and a Fabry-Pérot (FP) cavity is proposed and demonstrated for realizing single <span class="hlt">mode</span> lasers. The modulations of the <span class="hlt">mode</span> Q factor as simulation results are observed and single <span class="hlt">mode</span> operation is obtained with a side <span class="hlt">mode</span> suppression ratio of 46 dB and a single <span class="hlt">mode</span> fiber coupling loss of 3.2 dB for an AlGaInAs/InP hybrid laser as a 300-μm-length and 1.5-μm-wide FP cavity connected to a vertex of a 10-μm-side square microcavity. Furthermore, tunable single <span class="hlt">mode</span> operation is demonstrated with a continuous wavelength tuning range over 10 nm. The simple hybrid structure may shed light on practicalmore » applications of whispering-gallery <span class="hlt">mode</span> microcavities in large-scale photonic integrated circuits and optical communication and interconnection.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22878956','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22878956"><span><span class="hlt">Water</span>- and nitrogen-dependent alterations in the inheritance <span class="hlt">mode</span> of transpiration efficiency in winter wheat at the leaf and whole-plant level.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ratajczak, Dominika; Górny, Andrzej G</p> <p>2012-11-01</p> <p>The effects of contrasting <span class="hlt">water</span> and nitrogen (N) supply on the observed inheritance <span class="hlt">mode</span> of transpiration efficiency (TE) at the flag-leaf and whole-season levels were examined in winter wheat. Major components of the photosynthetic capacity of leaves and the season-integrated efficiency of <span class="hlt">water</span> use in vegetative and grain mass formation were evaluated in parental lines of various origins and their diallel F(2)-hybrids grown in a factorial experiment under different moisture and N status of the soil. A broad genetic variation was mainly found for the season-long TE measures. The variation range in the leaf photosynthetic indices was usually narrow, but tended to slightly enhance under <span class="hlt">water</span> and N shortage. Genotype-treatment interaction effects were significant for most characters. No consistency between the leaf- and season-long TE measures was observed. Preponderance of additivity-dependent variance was mainly identified for the season-integrated TE and leaf CO(2) assimilation rate. Soil treatments exhibited considerable influence on the phenotypic expression of gene action for the residual leaf measures. The contribution of non-additive gene effects and degree of dominance tended to increase in <span class="hlt">water</span>- and N-limited plants, especially for the leaf transpiration rate and stomatal conductance. The results indicate that promise exists to improve the season-integrated TE. However, selection for TE components should be prolonged for later hybrid generations to eliminate the masking of non-additive causes. Such evaluation among families grown under sub-optimal <span class="hlt">water</span> and nitrogen supply seems to be the most promising strategy in winter wheat.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhPl...21e6103W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhPl...21e6103W"><span>Edge-localized <span class="hlt">mode</span> avoidance and pedestal structure in I-<span class="hlt">mode</span> plasmasa)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Walk, J. R.; Hughes, J. W.; Hubbard, A. E.; Terry, J. L.; Whyte, D. G.; White, A. E.; Baek, S. G.; Reinke, M. L.; Theiler, C.; Churchill, R. M.; Rice, J. E.; Snyder, P. B.; Osborne, T.; Dominguez, A.; Cziegler, I.</p> <p>2014-05-01</p> <p>I-<span class="hlt">mode</span> is a high-performance tokamak regime characterized by the formation of a temperature pedestal and enhanced energy confinement, without an accompanying density pedestal or drop in particle and impurity transport. I-<span class="hlt">mode</span> operation appears to have naturally occurring suppression of large Edge-Localized <span class="hlt">Modes</span> (ELMs) in addition to its highly favorable scalings of pedestal structure and overall performance. Extensive study of the ELMy H-<span class="hlt">mode</span> has led to the development of the EPED model, which utilizes calculations of coupled peeling-ballooning MHD <span class="hlt">modes</span> and kinetic-ballooning <span class="hlt">mode</span> (KBM) stability limits to predict the pedestal structure preceding an ELM crash. We apply similar tools to the structure and ELM stability of I-<span class="hlt">mode</span> pedestals. Analysis of I-<span class="hlt">mode</span> discharges prepared with high-resolution pedestal data from the most recent C-Mod campaign reveals favorable pedestal scalings for extrapolation to large machines—pedestal temperature scales strongly with power per particle Pnet/n ¯e, and likewise pedestal pressure scales as the net heating power (consistent with weak degradation of confinement with heating power). Matched discharges in current, field, and shaping demonstrate the decoupling of energy and particle transport in I-<span class="hlt">mode</span>, increasing fueling to span nearly a factor of two in density while maintaining matched temperature pedestals with consistent levels of Pnet/n ¯e. This is consistent with targets for increased performance in I-<span class="hlt">mode</span>, elevating pedestal βp and global performance with matched increases in density and heating power. MHD calculations using the ELITE code indicate that I-<span class="hlt">mode</span> pedestals are strongly stable to edge peeling-ballooning instabilities. Likewise, numerical modeling of the KBM turbulence onset, as well as scalings of the pedestal width with poloidal beta, indicates that I-<span class="hlt">mode</span> pedestals are not limited by KBM turbulence—both features identified with the trigger for large ELMs, consistent with the observed suppression of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100035662','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100035662"><span>Flexible <span class="hlt">Modes</span> Control Using Sliding <span class="hlt">Mode</span> Observers: Application to Ares I</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shtessel, Yuri B.; Hall, Charles E.; Baev, Simon; Orr, Jeb S.</p> <p>2010-01-01</p> <p>The launch vehicle dynamics affected by bending and sloshing <span class="hlt">modes</span> are considered. Attitude measurement data that are corrupted by flexible <span class="hlt">modes</span> could yield instability of the vehicle dynamics. Flexible body and sloshing <span class="hlt">modes</span> are reconstructed by sliding <span class="hlt">mode</span> observers. The resultant estimates are used to remove the undesirable dynamics from the measurements, and the direct effects of sloshing and bending <span class="hlt">modes</span> on the launch vehicle are compensated by means of a controller that is designed without taking the bending and sloshing <span class="hlt">modes</span> into account. A linearized mathematical model of Ares I launch vehicle was derived based on FRACTAL, a linear model developed by NASA/MSFC. The compensated vehicle dynamics with a simple PID controller were studied for the launch vehicle model that included two bending <span class="hlt">modes</span>, two slosh <span class="hlt">modes</span> and actuator dynamics. A simulation study demonstrated stable and accurate performance of the flight control system with the augmented simple PID controller without the use of traditional linear bending filters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26480436','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26480436"><span><span class="hlt">Mode</span> selection in square resonator microlasers for widely tunable single <span class="hlt">mode</span> lasing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tang, Ming-Ying; Sui, Shao-Shuai; Yang, Yue-De; Xiao, Jin-Long; Du, Yun; Huang, Yong-Zhen</p> <p>2015-10-19</p> <p><span class="hlt">Mode</span> selection in square resonator semiconductor microlasers is demonstrated by adjusting the width of the output waveguide coupled to the midpoint of one side. The simulation and experimental results reveal that widely tunable single <span class="hlt">mode</span> lasing can be realized in square resonator microlasers. Through adjusting the width of the output waveguide, the <span class="hlt">mode</span> interval of the high-Q <span class="hlt">modes</span> can reach four times of the longitudinal <span class="hlt">mode</span> interval. Therefore, <span class="hlt">mode</span> hopping can be efficiently avoided and the lasing wavelength can be tuned continuously by tuning the injection current. For a 17.8-μm-side-length square microlaser with a 1.4-μm-width output waveguide, <span class="hlt">mode</span>-hopping-free single-<span class="hlt">mode</span> operation is achieved with a continuous tuning range of 9.2 nm. As a result, the control of the lasing <span class="hlt">mode</span> is realized for the square microlasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MSSP..107...53L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MSSP..107...53L"><span>Adaptive variational <span class="hlt">mode</span> decomposition method for signal processing based on <span class="hlt">mode</span> characteristic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lian, Jijian; Liu, Zhuo; Wang, Haijun; Dong, Xiaofeng</p> <p>2018-07-01</p> <p>Variational <span class="hlt">mode</span> decomposition is a completely non-recursive decomposition model, where all the <span class="hlt">modes</span> are extracted concurrently. However, the model requires a preset <span class="hlt">mode</span> number, which limits the adaptability of the method since a large deviation in the number of <span class="hlt">mode</span> set will cause the discard or mixing of the <span class="hlt">mode</span>. Hence, a method called Adaptive Variational <span class="hlt">Mode</span> Decomposition (AVMD) was proposed to automatically determine the <span class="hlt">mode</span> number based on the characteristic of intrinsic <span class="hlt">mode</span> function. The method was used to analyze the simulation signals and the measured signals in the hydropower plant. Comparisons have also been conducted to evaluate the performance by using VMD, EMD and EWT. It is indicated that the proposed method has strong adaptability and is robust to noise. It can determine the <span class="hlt">mode</span> number appropriately without modulation even when the signal frequencies are relatively close.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4598738','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4598738"><span><span class="hlt">Mode</span> division multiplexing using an orbital angular momentum <span class="hlt">mode</span> sorter and MIMO-DSP over a graded-index few-<span class="hlt">mode</span> optical fibre</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huang, Hao; Milione, Giovanni; Lavery, Martin P. J.; Xie, Guodong; Ren, Yongxiong; Cao, Yinwen; Ahmed, Nisar; An Nguyen, Thien; Nolan, Daniel A.; Li, Ming-Jun; Tur, Moshe; Alfano, Robert R.; Willner, Alan E.</p> <p>2015-01-01</p> <p><span class="hlt">Mode</span> division multiplexing (MDM)– using a multimode optical fiber’s N spatial <span class="hlt">modes</span> as data channels to transmit N independent data streams – has received interest as it can potentially increase optical fiber data transmission capacity N-times with respect to single <span class="hlt">mode</span> optical fibers. Two challenges of MDM are (1) designing <span class="hlt">mode</span> (de)multiplexers with high <span class="hlt">mode</span> selectivity (2) designing <span class="hlt">mode</span> (de)multiplexers without cascaded beam splitting’s 1/N insertion loss. One spatial <span class="hlt">mode</span> basis that has received interest is that of orbital angular momentum (OAM) <span class="hlt">modes</span>. In this paper, using a device referred to as an OAM <span class="hlt">mode</span> sorter, we show that OAM <span class="hlt">modes</span> can be (de)multiplexed over a multimode optical fiber with higher than −15 dB <span class="hlt">mode</span> selectivity and without cascaded beam splitting’s 1/N insertion loss. As a proof of concept, the OAM <span class="hlt">modes</span> of the LP11 <span class="hlt">mode</span> group (OAM−1,0 and OAM+1,0), each carrying 20-Gbit/s polarization division multiplexed and quadrature phase shift keyed data streams, are transmitted 5km over a graded-index, few-<span class="hlt">mode</span> optical fibre. Channel crosstalk is mitigated using 4 × 4 multiple-input-multiple-output digital-signal-processing with <1.5 dB power penalties at a bit-error-rate of 2 × 10−3. PMID:26450398</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26450398','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26450398"><span><span class="hlt">Mode</span> division multiplexing using an orbital angular momentum <span class="hlt">mode</span> sorter and MIMO-DSP over a graded-index few-<span class="hlt">mode</span> optical fibre.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huang, Hao; Milione, Giovanni; Lavery, Martin P J; Xie, Guodong; Ren, Yongxiong; Cao, Yinwen; Ahmed, Nisar; An Nguyen, Thien; Nolan, Daniel A; Li, Ming-Jun; Tur, Moshe; Alfano, Robert R; Willner, Alan E</p> <p>2015-10-09</p> <p><span class="hlt">Mode</span> division multiplexing (MDM)- using a multimode optical fiber's N spatial <span class="hlt">modes</span> as data channels to transmit N independent data streams - has received interest as it can potentially increase optical fiber data transmission capacity N-times with respect to single <span class="hlt">mode</span> optical fibers. Two challenges of MDM are (1) designing <span class="hlt">mode</span> (de)multiplexers with high <span class="hlt">mode</span> selectivity (2) designing <span class="hlt">mode</span> (de)multiplexers without cascaded beam splitting's 1/N insertion loss. One spatial <span class="hlt">mode</span> basis that has received interest is that of orbital angular momentum (OAM) <span class="hlt">modes</span>. In this paper, using a device referred to as an OAM <span class="hlt">mode</span> sorter, we show that OAM <span class="hlt">modes</span> can be (de)multiplexed over a multimode optical fiber with higher than -15 dB <span class="hlt">mode</span> selectivity and without cascaded beam splitting's 1/N insertion loss. As a proof of concept, the OAM <span class="hlt">modes</span> of the LP11 <span class="hlt">mode</span> group (OAM-1,0 and OAM+1,0), each carrying 20-Gbit/s polarization division multiplexed and quadrature phase shift keyed data streams, are transmitted 5km over a graded-index, few-<span class="hlt">mode</span> optical fibre. Channel crosstalk is mitigated using 4 × 4 multiple-input-multiple-output digital-signal-processing with <1.5 dB power penalties at a bit-error-rate of 2 × 10(-3).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...514931H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...514931H"><span><span class="hlt">Mode</span> division multiplexing using an orbital angular momentum <span class="hlt">mode</span> sorter and MIMO-DSP over a graded-index few-<span class="hlt">mode</span> optical fibre</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Hao; Milione, Giovanni; Lavery, Martin P. J.; Xie, Guodong; Ren, Yongxiong; Cao, Yinwen; Ahmed, Nisar; An Nguyen, Thien; Nolan, Daniel A.; Li, Ming-Jun; Tur, Moshe; Alfano, Robert R.; Willner, Alan E.</p> <p>2015-10-01</p> <p><span class="hlt">Mode</span> division multiplexing (MDM)- using a multimode optical fiber’s N spatial <span class="hlt">modes</span> as data channels to transmit N independent data streams - has received interest as it can potentially increase optical fiber data transmission capacity N-times with respect to single <span class="hlt">mode</span> optical fibers. Two challenges of MDM are (1) designing <span class="hlt">mode</span> (de)multiplexers with high <span class="hlt">mode</span> selectivity (2) designing <span class="hlt">mode</span> (de)multiplexers without cascaded beam splitting’s 1/N insertion loss. One spatial <span class="hlt">mode</span> basis that has received interest is that of orbital angular momentum (OAM) <span class="hlt">modes</span>. In this paper, using a device referred to as an OAM <span class="hlt">mode</span> sorter, we show that OAM <span class="hlt">modes</span> can be (de)multiplexed over a multimode optical fiber with higher than -15 dB <span class="hlt">mode</span> selectivity and without cascaded beam splitting’s 1/N insertion loss. As a proof of concept, the OAM <span class="hlt">modes</span> of the LP11 <span class="hlt">mode</span> group (OAM-1,0 and OAM+1,0), each carrying 20-Gbit/s polarization division multiplexed and quadrature phase shift keyed data streams, are transmitted 5km over a graded-index, few-<span class="hlt">mode</span> optical fibre. Channel crosstalk is mitigated using 4 × 4 multiple-input-multiple-output digital-signal-processing with <1.5 dB power penalties at a bit-error-rate of 2 × 10-3.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24576599','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24576599"><span><span class="hlt">Mode</span> perturbation method for optimal guided wave <span class="hlt">mode</span> and frequency selection.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Philtron, J H; Rose, J L</p> <p>2014-09-01</p> <p>With a thorough understanding of guided wave mechanics, researchers can predict which guided wave <span class="hlt">modes</span> will have a high probability of success in a particular nondestructive evaluation application. However, work continues to find optimal <span class="hlt">mode</span> and frequency selection for a given application. This "optimal" <span class="hlt">mode</span> could give the highest sensitivity to defects or the greatest penetration power, increasing inspection efficiency. Since material properties used for modeling work may be estimates, in many cases guided wave <span class="hlt">mode</span> and frequency selection can be adjusted for increased inspection efficiency in the field. In this paper, a novel <span class="hlt">mode</span> and frequency perturbation method is described and used to identify optimal <span class="hlt">mode</span> points based on quantifiable wave characteristics. The technique uses an ultrasonic phased array comb transducer to sweep in phase velocity and frequency space. It is demonstrated using guided interface waves for bond evaluation. After searching nearby <span class="hlt">mode</span> points, an optimal <span class="hlt">mode</span> and frequency can be selected which has the highest sensitivity to a defect, or gives the greatest penetration power. The optimal <span class="hlt">mode</span> choice for a given application depends on the requirements of the inspection. Copyright © 2014 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014IAUS..301..477P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014IAUS..301..477P"><span><span class="hlt">Mode</span> identification from spectroscopy of gravity-<span class="hlt">mode</span> pulsators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollard, K. R.; Brunsden, E.; Cottrell, P. L.; Davie, M.; Greenwood, A.; Wright, D. J.; De Cat, P.</p> <p>2014-02-01</p> <p>The gravity <span class="hlt">modes</span> present in γ Doradus stars probe the deep stellar interiors and are thus of particular interest in asteroseismology. For the MUSICIAN programme at the University of Canterbury, we obtain extensive high-resolution echelle spectra of γ Dor stars from the Mt John University Observatory in New Zealand. We analyze these to obtain the pulsational frequencies and identify these with the multiple pulsational <span class="hlt">modes</span> excited in the star. A summary of recent results from our spectroscopic <span class="hlt">mode</span>-identification programme is given.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017QSRv..162..128J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017QSRv..162..128J"><span><span class="hlt">Sub-Antarctic</span> glacier extensions in the Kerguelen region (49°S, Indian Ocean) over the past 24,000 years constrained by 36Cl moraine dating</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jomelli, Vincent; Mokadem, Fatima; Schimmelpfennig, Irene; Chapron, Emmanuel; Rinterknecht, Vincent; Favier, Vincent; Verfaillie, Deborah; Brunstein, Daniel; Legentil, Claude; Michel, Elisabeth; Swingedouw, Didier; Jaouen, Alain; Aumaitre, Georges; Bourlès, Didier L.; Keddadouche, Karim</p> <p>2017-04-01</p> <p>Similar to many other regions in the world, glaciers in the southern sub-polar regions are currently retreating. In the Kerguelen Islands (49°S, 69°E), the mass balance of the Cook Ice Cap (CIC), the largest ice cap in this region, experienced dramatic shrinking between 1960 and 2013 with retreat rates among the highest in the world. This observation needs to be evaluated in a long-term context. However, data on the past glacier extents are sparse in the <span class="hlt">sub-Antarctic</span> regions. To investigate the deglaciation pattern since the Last Glacial Maximum (LGM) period, we present the first 13 cosmogenic 36Cl surface exposure ages from four sites in the Kerguelen Islands. The 36Cl ages from erratic and moraine boulders span from 24.4 ± 2.7 ka to 0.3 ± 0.1 ka. We combined these ages with existing glacio-marine radiocarbon ages and bathymetric data to document the temporal and spatial changes of the island's glacial history. Ice began to retreat on the main island before 24.4 ± 2.7 ka until around the time of the Antarctic Cold Reversal (ACR) period (∼14.5-12.9 ka), during which the Bontemps moraine was formed by the advance of a CIC outlet glacier. Deglaciation continued during the Holocene probably until 3 ka with evidence of minor advances during the last millennium. This chronology is in pace with major changes in δ18O in a recent West Antarctica ice core record, showing that Kerguelen Islands glaciers are particularly sensitive and relevant to document climate change in the southern polar regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPO21A..06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPO21A..06B"><span>Inference and Biogeochemical Response of Vertical Velocities inside a <span class="hlt">Mode</span> <span class="hlt">Water</span> Eddy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Barceló-Llull, B.; Pallas Sanz, E.; Sangrà, P.</p> <p>2016-02-01</p> <p>With the aim to study the modulation of the biogeochemical fluxes by the ageostrophic secondary circulation in anticyclonic mesoscale eddies, a typical eddy of the Canary Eddy Corridor was interdisciplinary surveyed on September 2014 in the framework of the PUMP project. The eddy was elliptical shaped, 4 month old, 110 km diameter and 400 m depth. It was an intrathermocline type often also referred as <span class="hlt">mode</span> <span class="hlt">water</span> eddy type. We inferred the mesoscale vertical velocity field resolving a generalized omega equation from the 3D density and ADCP velocity fields of a five-day sampled CTD-SeaSoar regular grid centred on the eddy. The grid transects where 10 nautical miles apart. Although complex, in average, the inferred omega velocity field (hereafter w) shows a dipolar structure with downwelling velocities upstream of the propagation path (west) and upwelling velocities downstream. The w at the eddy center was zero and maximum values were located at the periphery attaining ca. 6 m day-1. Coinciding with the occurrence of the vertical velocities cells a noticeable enhancement of phytoplankton biomass was observed at the eddy periphery respect to the far field. A corresponding upward diapycnal flux of nutrients was also observed at the periphery. As minimum velocities where reached at the eddy center, lineal Ekman pumping mechanism was discarded. Minimum values of phytoplankton biomass where also observed at the eddy center. The possible mechanisms for such dipolar w cell are still being investigated, but an analysis of the generalized omega equation forcing terms suggest that it may be a combination of horizontal deformation and advection of vorticity by the ageostrophic current (related to nonlinear Ekman pumping). As expected for Trades, the wind was rather constant and uniform with a speed of ca. 5 m s-1. Diagnosed nonlinear Ekman pumping leaded also to a dipolar cell that mirrors the omega w dipolar cell.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011QSRv...30..876R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011QSRv...30..876R"><span>Environmental reconstructions of the upper 500 m of the southern Indian Ocean over the last 40 ka using Radiolarian (Protista) proxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rogers, John; De Deckker, Patrick</p> <p>2011-04-01</p> <p>In 2007, we demonstrated that radiolarians are proxies for a wide range of oceanic physico-chemical properties from the surface to depths of up to 500 m below sea level. In this study, our results are refined and Correspondence Analysis (CA) scores derived from census counts of radiolarian subfossils from southern Indian Ocean core-tops are correlated with the physico-chemical properties of the region obtained from the 2005 World Ocean Database. Calibration and regression techniques are employed to reconstruct palaeoenvironmental conditions spanning the last 40 ka for four Indian Ocean cores MD88-769 [46°04'S 90°06'E], MD88-770 [46°01'S 96°27'E], MD94-102 [43°30'S 79°50'E], and MD94-103 [45°35'S 86°31'E], all from close to the Southeast Indian Ridge. For the first time, reconstructions of temperature, salinity, dissolved oxygen, and the silicate, nitrate, and phosphate concentrations for a range of <span class="hlt">water</span> depths are proved possible. Changes of the oceanic environment and the movement of <span class="hlt">water</span> masses over the last 40 ka, as suggested by these reconstructions, are discussed. During Marine Isotope Stages 2 and 3 (MIS-2 and MIS-3), the <span class="hlt">water</span> column at some of the core sites has similar characteristics to the <span class="hlt">waters</span> south of the Polar Front today. At the MIS-1/MIS-2 transition, the development of the <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> is apparent. Temperature reconstructions include evidence of the Antarctic Cold Reversal and the Holocene Optimum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21421249-averaged-variational-principle-autoresonant-bernstein-greene-kruskal-modes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21421249-averaged-variational-principle-autoresonant-bernstein-greene-kruskal-modes"><span>Averaged variational principle for autoresonant Bernstein-Greene-Kruskal <span class="hlt">modes</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>Khain, P.; Friedland, L.</p> <p>2010-10-15</p> <p>Whitham's averaged variational principle is applied in studying dynamics of formation of autoresonant (continuously phase-locked) Bernstein-Greene-Kruskal (BGK) <span class="hlt">modes</span> in a plasma driven by a chirped frequency ponderomotive wave. A flat-top electron velocity distribution is used as a model allowing a variational formulation within the <span class="hlt">water</span> bag theory. The corresponding Lagrangian, averaged over the fast phase variable yields evolution equations for the slow field variables, allows uniform description of all stages of excitation of driven-chirped BGK <span class="hlt">modes</span>, and predicts modulational stability of these nonlinear phase-space structures. Numerical solutions of the system of slow variational equations are in good agreement with Vlasov-Poissonmore » simulations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25321749','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25321749"><span>Single <span class="hlt">mode</span> tapered fiber-optic interferometer based refractive index sensor and its application to protein sensing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yadav, T K; Narayanaswamy, R; Abu Bakar, M H; Kamil, Y Mustapha; Mahdi, M A</p> <p>2014-09-22</p> <p>We demonstrate refractive index sensors based on single <span class="hlt">mode</span> tapered fiber and its application as a biosensor. We utilize this tapered fiber optic biosensor, operating at 1550 nm, for the detection of protein (gelatin) concentration in <span class="hlt">water</span>. The sensor is based on the spectroscopy of <span class="hlt">mode</span> coupling based on core <span class="hlt">modes</span>-fiber cladding <span class="hlt">modes</span> excited by the fundamental core <span class="hlt">mode</span> of an optical fiber when it transitions into tapered regions from untapered regions. The changes are determined from the wavelength shift of the transmission spectrum. The proposed fiber sensor has sensitivity of refractive index around 1500 nm/RIU and for protein concentration detection, its highest sensitivity is 2.42141 nm/%W/V.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22253079-edge-localized-mode-avoidance-pedestal-structure-mode-plasmas','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22253079-edge-localized-mode-avoidance-pedestal-structure-mode-plasmas"><span>Edge-localized <span class="hlt">mode</span> avoidance and pedestal structure in I-<span class="hlt">mode</span> plasmas</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>Walk, J. R., E-mail: jrwalk@psfc.mit.edu; Hughes, J. W.; Hubbard, A. E.</p> <p></p> <p>I-<span class="hlt">mode</span> is a high-performance tokamak regime characterized by the formation of a temperature pedestal and enhanced energy confinement, without an accompanying density pedestal or drop in particle and impurity transport. I-<span class="hlt">mode</span> operation appears to have naturally occurring suppression of large Edge-Localized <span class="hlt">Modes</span> (ELMs) in addition to its highly favorable scalings of pedestal structure and overall performance. Extensive study of the ELMy H-<span class="hlt">mode</span> has led to the development of the EPED model, which utilizes calculations of coupled peeling-ballooning MHD <span class="hlt">modes</span> and kinetic-ballooning <span class="hlt">mode</span> (KBM) stability limits to predict the pedestal structure preceding an ELM crash. We apply similar tools to themore » structure and ELM stability of I-<span class="hlt">mode</span> pedestals. Analysis of I-<span class="hlt">mode</span> discharges prepared with high-resolution pedestal data from the most recent C-Mod campaign reveals favorable pedestal scalings for extrapolation to large machines—pedestal temperature scales strongly with power per particle P{sub net}/n{sup ¯}{sub e}, and likewise pedestal pressure scales as the net heating power (consistent with weak degradation of confinement with heating power). Matched discharges in current, field, and shaping demonstrate the decoupling of energy and particle transport in I-<span class="hlt">mode</span>, increasing fueling to span nearly a factor of two in density while maintaining matched temperature pedestals with consistent levels of P{sub net}/n{sup ¯}{sub e}. This is consistent with targets for increased performance in I-<span class="hlt">mode</span>, elevating pedestal β{sub p} and global performance with matched increases in density and heating power. MHD calculations using the ELITE code indicate that I-<span class="hlt">mode</span> pedestals are strongly stable to edge peeling-ballooning instabilities. Likewise, numerical modeling of the KBM turbulence onset, as well as scalings of the pedestal width with poloidal beta, indicates that I-<span class="hlt">mode</span> pedestals are not limited by KBM turbulence—both features identified with the trigger for large ELMs</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24714732','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24714732"><span>Correlated evolution between <span class="hlt">mode</span> of larval development and habitat in muricid gastropods.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pappalardo, Paula; Rodríguez-Serrano, Enrique; Fernández, Miriam</p> <p>2014-01-01</p> <p>Larval <span class="hlt">modes</span> of development affect evolutionary processes and influence the distribution of marine invertebrates in the ocean. The decrease in pelagic development toward higher latitudes is one of the patterns of distribution most frequently discussed in marine organisms (Thorson's rule), which has been related to increased larval mortality associated with long pelagic durations in colder <span class="hlt">waters</span>. However, the type of substrate occupied by adults has been suggested to influence the generality of the latitudinal patterns in larval development. To help understand how the environment affects the evolution of larval types we evaluated the association between larval development and habitat using gastropods of the Muricidae family as a model group. To achieve this goal, we collected information on latitudinal distribution, sea <span class="hlt">water</span> temperature, larval development and type of substrate occupied by adults. We constructed a molecular phylogeny for 45 species of muricids to estimate the ancestral character states and to assess the relationship between traits using comparative methods in a Bayesian framework. Our results showed high probability for a common ancestor of the muricids with nonpelagic (and nonfeeding) development, that lived in hard bottoms and cold temperatures. From this ancestor, a pelagic feeding larva evolved three times, and some species shifted to warmer temperatures or sand bottoms. The evolution of larval development was not independent of habitat; the most probable evolutionary route reconstructed in the analysis of correlated evolution showed that type of larval development may change in soft bottoms but in hard bottoms this change is highly unlikely. Lower sea <span class="hlt">water</span> temperatures were associated with nonpelagic <span class="hlt">modes</span> of development, supporting Thorson's rule. We show how environmental pressures can favor a particular <span class="hlt">mode</span> of larval development or transitions between larval <span class="hlt">modes</span> and discuss the reacquisition of feeding larva in muricids gastropods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE10158E..0GY','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE10158E..0GY"><span>Low-bending loss and single-<span class="hlt">mode</span> operation in few-<span class="hlt">mode</span> optical fiber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yin, Ping; Wang, Hua; Chen, Ming-Yang; Wei, Jin; Cai, Zhi-Min; Li, Lu-Ming; Yang, Ji-Hai; Zhu, Yuan-Feng</p> <p>2016-10-01</p> <p>The technique of eliminating the higher-order <span class="hlt">modes</span> in a few-<span class="hlt">mode</span> optical fiber is proposed. The fiber is designed with a group of defect <span class="hlt">modes</span> in the cladding. The higher-order <span class="hlt">modes</span> in the fiber can be eliminated by bending the fiber to induce strong coupling between the defect <span class="hlt">modes</span> and the higher-order <span class="hlt">modes</span>. Numerical simulation shows the bending losses of the LP01 <span class="hlt">mode</span> are lower than 1.5×10-4 dB/turn for the wavelength shorter than 1.625 μm. The proposed fiber can be bent multiple turns at small bending radius which are preferable for FTTH related applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016tcp..book..195D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016tcp..book..195D"><span>Plasma <span class="hlt">Modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dubin, D. H. E.</p> <p></p> <p>This chapter explores several aspects of the linear electrostatic normal <span class="hlt">modes</span> of oscillation for a single-species non-neutral plasma in a Penning trap. Linearized fluid equations of motion are developed, assuming the plasma is cold but collisionless, which allow derivation of the cold plasma dielectric tensor and the electrostatic wave equation. Upper hybrid and magnetized plasma waves in an infinite uniform plasma are described. The effect of the plasma surface in a bounded plasma system is considered, and the properties of surface plasma waves are characterized. The normal <span class="hlt">modes</span> of a cylindrical plasma column are discussed, and finally, <span class="hlt">modes</span> of spheroidal plasmas, and finite temperature effects on the <span class="hlt">modes</span>, are briefly described.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_14 --> <div id="page_15" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="281"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9739E..0HR','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9739E..0HR"><span>A burst-<span class="hlt">mode</span> photon counting receiver with automatic channel estimation and bit rate detection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rao, Hemonth G.; DeVoe, Catherine E.; Fletcher, Andrew S.; Gaschits, Igor D.; Hakimi, Farhad; Hamilton, Scott A.; Hardy, Nicholas D.; Ingwersen, John G.; Kaminsky, Richard D.; Moores, John D.; Scheinbart, Marvin S.; Yarnall, Timothy M.</p> <p>2016-04-01</p> <p>We demonstrate a multi-rate burst-<span class="hlt">mode</span> photon-counting receiver for undersea communication at data rates up to 10.416 Mb/s over a 30-foot <span class="hlt">water</span> channel. To the best of our knowledge, this is the first demonstration of burst-<span class="hlt">mode</span> photon-counting communication. With added attenuation, the maximum link loss is 97.1 dB at λ=517 nm. In clear ocean <span class="hlt">water</span>, this equates to link distances up to 148 meters. For λ=470 nm, the achievable link distance in clear ocean <span class="hlt">water</span> is 450 meters. The receiver incorporates soft-decision forward error correction (FEC) based on a product code of an inner LDPC code and an outer BCH code. The FEC supports multiple code rates to achieve error-free performance. We have selected a burst-<span class="hlt">mode</span> receiver architecture to provide robust performance with respect to unpredictable channel obstructions. The receiver is capable of on-the-fly data rate detection and adapts to changing levels of signal and background light. The receiver updates its phase alignment and channel estimates every 1.6 ms, allowing for rapid changes in <span class="hlt">water</span> quality as well as motion between transmitter and receiver. We demonstrate on-the-fly rate detection, channel BER within 0.2 dB of theory across all data rates, and error-free performance within 1.82 dB of soft-decision capacity across all tested code rates. All signal processing is done in FPGAs and runs continuously in real time.</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 Ocean 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 <span class="hlt">waters</span> flowing from the Pacific and the marginal seas through the Indian Ocean (IO) on their way toward the South Atlantic within a high-resolution ocean/sea-ice model. The model fields are analysed from a Lagrangian perspective where <span class="hlt">water</span> 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 basin within 1-3 decades. <span class="hlt">Waters</span> entering the IO south of Australia are at intermediate depths and maintain their temperature-salinity properties as they exit the basin within 1.5-3.5 decades. Of these <span class="hlt">waters</span>, the contribution from Tasman leakage is 1.4 Sv. The rest stem from recirculation of <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> formed within the IO. The marginal seas export 1.0 Sv into the Atlantic within 1.5-4 decades, and the <span class="hlt">waters</span> cool and freshen on-route. However, the model's simulation of <span class="hlt">waters</span> from the Gulfs of Aden and Oman are too light and hence overly susceptible to upper ocean circulations. In the Cape Basin, 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('https://www.ncbi.nlm.nih.gov/pubmed/23927230','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23927230"><span>Passive estimation of the waveguide invariant per pair of <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Le Gall, Yann; Bonnel, Julien</p> <p>2013-08-01</p> <p>In many oceanic waveguides, acoustic propagation is characterized by a parameter called waveguide invariant. This property is used in many passive and active sonar applications where knowledge of the waveguide invariant value is required. The waveguide invariant is classically considered as scalar but several studies show that it is better modeled by a distribution because of its dependence on frequency and <span class="hlt">mode</span> pairs. This paper presents a new method for estimating the waveguide invariant distribution. Using the noise radiated by a distant ship and a single hydrophone, the proposed methodology allows estimating the waveguide invariant for each pair of <span class="hlt">modes</span> in shallow <span class="hlt">water</span>. Performance is evaluated on simulated data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015OptL...40.1980M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015OptL...40.1980M"><span>4 × 20 Gbit/s <span class="hlt">mode</span> division multiplexing over free space using vector <span class="hlt">modes</span> and a q-plate <span class="hlt">mode</span> (de)multiplexer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milione, Giovanni; Lavery, Martin P. J.; Huang, Hao; Ren, Yongxiong; Xie, Guodong; Nguyen, Thien An; Karimi, Ebrahim; Marrucci, Lorenzo; Nolan, Daniel A.; Alfano, Robert R.; Willner, Alan E.</p> <p>2015-05-01</p> <p>Vector <span class="hlt">modes</span> are spatial <span class="hlt">modes</span> that have spatially inhomogeneous states of polarization, such as, radial and azimuthal polarization. They can produce smaller spot sizes and stronger longitudinal polarization components upon focusing. As a result, they are used for many applications, including optical trapping and nanoscale imaging. In this work, vector <span class="hlt">modes</span> are used to increase the information capacity of free space optical communication via the method of optical communication referred to as <span class="hlt">mode</span> division multiplexing. A <span class="hlt">mode</span> (de)multiplexer for vector <span class="hlt">modes</span> based on a liquid crystal technology referred to as a q-plate is introduced. As a proof of principle, using the <span class="hlt">mode</span> (de)multiplexer four vector <span class="hlt">modes</span> each carrying a 20 Gbit/s quadrature phase shift keying signal on a single wavelength channel (~1550nm), comprising an aggregate 80 Gbit/s, were transmitted ~1m over the lab table with <-16.4 dB (<2%) <span class="hlt">mode</span> crosstalk. Bit error rates for all vector <span class="hlt">modes</span> were measured at the forward error correction threshold with power penalties < 3.41dB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28640618','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28640618"><span>Dynamic Roughness Ratio-Based Framework for Modeling Mixed <span class="hlt">Mode</span> of Droplet Evaporation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gunjan, Madhu Ranjan; Raj, Rishi</p> <p>2017-07-18</p> <p>The spatiotemporal evolution of an evaporating sessile droplet and its effect on lifetime is crucial to various disciplines of science and technology. Although experimental investigations suggest three distinct <span class="hlt">modes</span> through which a droplet evaporates, namely, the constant contact radius (CCR), the constant contact angle (CCA), and the mixed, only the CCR and the CCA <span class="hlt">modes</span> have been modeled reasonably. Here we use experiments with <span class="hlt">water</span> droplets on flat and micropillared silicon substrates to characterize the mixed <span class="hlt">mode</span>. We visualize that a perfect CCA <span class="hlt">mode</span> after the initial CCR <span class="hlt">mode</span> is an idealization on a flat silicon substrate, and the receding contact line undergoes intermittent but recurring pinning (CCR <span class="hlt">mode</span>) as it encounters fresh contaminants on the surface. The resulting increase in roughness lowers the contact angle of the droplet during these intermittent CCR <span class="hlt">modes</span> until the next depinning event, followed by the CCA <span class="hlt">mode</span> of evaporation. The airborne contaminants in our experiments are mostly loosely adhered to the surface and travel along with the receding contact line. The resulting gradual increase in the apparent roughness and hence the extent of CCR <span class="hlt">mode</span> over CCA <span class="hlt">mode</span> forces appreciable decrease in the contact angle observed during the mixed <span class="hlt">mode</span> of evaporation. Unlike loosely adhered airborne contaminants on flat samples, micropillars act as fixed roughness features. The apparent roughness fluctuates about the mean value as the contact line recedes between pillars. Evaporation on these surfaces exhibits stick-jump motion with a short-duration mixed <span class="hlt">mode</span> toward the end when the droplet size becomes comparable to the pillar spacing. We incorporate this dynamic roughness into a classical evaporation model to accurately predict the droplet evolution throughout the three <span class="hlt">modes</span>, for both flat and micropillared silicon surfaces. We believe that this framework can also be extended to model the evaporation of nanofluids and the coffee-ring effect, among</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8601E..0SK','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8601E..0SK"><span>Femtosecond pulse inscription of a selective <span class="hlt">mode</span> filter in large <span class="hlt">mode</span> area fibers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krämer, Ria G.; Voigtländer, Christian; Freier, Erik; Liem, Andreas; Thomas, Jens U.; Richter, Daniel; Schreiber, Thomas; Tünnermann, Andreas; Nolte, Stefan</p> <p>2013-02-01</p> <p>We present a selective <span class="hlt">mode</span> filter inscribed with ultrashort pulses directly into a few <span class="hlt">mode</span> large <span class="hlt">mode</span> area (LMA) fiber. The <span class="hlt">mode</span> filter consists of two refractive index modifications alongside the fiber core in the cladding. The refractive index modifications, which were of approximately the same order of magnitude as the refractive index difference between core and cladding have been inscribed by nonlinear absorption of femtosecond laser pulses (800 nm wavelength, 120 fs pulse duration). If light is guided in the core, it will interact with the inscribed modifications causing <span class="hlt">modes</span> to be coupled out of the core. In order to characterize the <span class="hlt">mode</span> filter, we used a femtosecond inscribed fiber Bragg grating (FBG), which acts as a wavelength and therefore <span class="hlt">mode</span> selective element in the LMA fiber. Since each <span class="hlt">mode</span> has different Bragg reflection wavelengths, an FBG in a multimode fiber will exhibit multiple Bragg reflection peaks. In our experiments, we first inscribed the FBG using the phase mask scanning technique. Then the <span class="hlt">mode</span> filter was inscribed. The reflection spectrum of the FBG was measured in situ during the inscription process using a supercontinuum source. The reflectivities of the LP01 and LP11 <span class="hlt">modes</span> show a dependency on the length of the <span class="hlt">mode</span> filter. Two stages of the filter were obtained: one, in which the LP11 <span class="hlt">mode</span> was reduced by 60% and one where the LP01 <span class="hlt">mode</span> was reduced by 80%. The other <span class="hlt">mode</span> respectively showed almost no losses. In conclusion, we could selectively filter either the fundamental or higher order <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840014003&hterms=4th&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D4th','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840014003&hterms=4th&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D4th"><span>Computational aspects of the nonlinear normal <span class="hlt">mode</span> initialization of the GLAS 4th order GCM</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Navon, I. M.; Bloom, S. C.; Takacs, L.</p> <p>1984-01-01</p> <p>Using the normal <span class="hlt">modes</span> of the GLAS 4th Order Model, a Machenhauer nonlinear normal <span class="hlt">mode</span> initialization (NLNMI) was carried out for the external vertical <span class="hlt">mode</span> using the GLAS 4th Order shallow <span class="hlt">water</span> equations model for an equivalent depth corresponding to that associated with the external vertical <span class="hlt">mode</span>. A simple procedure was devised which was directed at identifying computational <span class="hlt">modes</span> by following the rate of increase of BAL sub M, the partial (with respect to the zonal wavenumber m) sum of squares of the time change of the normal <span class="hlt">mode</span> coefficients (for fixed vertical <span class="hlt">mode</span> index) varying over the latitude index L of symmetric or antisymmetric gravity waves. A working algorithm is presented which speeds up the convergence of the iterative Machenhauer NLNMI. A 24 h integration using the NLNMI state was carried out using both Matsuno and leap-frog time-integration schemes; these runs were then compared to a 24 h integration starting from a non-initialized state. The maximal impact of the nonlinear normal <span class="hlt">mode</span> initialization was found to occur 6-10 hours after the initial time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5664630','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5664630"><span>The Study of Titanium and Zirconium Ions in <span class="hlt">Water</span> by MPT-LTQ Mass Spectrometry in Negative <span class="hlt">Mode</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>Yang, Junqing; Zheng, Mei; Liu, Qiuju; Zhu, Meiling; Yang, Chushan; Zhang, Yan; Zhu, Zhiqiang</p> <p>2017-01-01</p> <p>Microwave plasma torches (MPTs) can be used as simple and low power-consumption ambient ion sources. When MPT-mass spectrometry (MPT-MS) is applied in the detection of some metal elements, the metallic ions exhibit some novel features which are significantly different with those obtained by the traditional inductively coupled plasma (ICP)-mass spectrometry (ICP-MS) and may be helpful for metal element analysis. As the representative elements of group IVA, titanium and zirconium are both of importance and value in modern industry, and they have impacts on human health. Here, we first provide a study on the complex anions of titanium and zirconium in <span class="hlt">water</span> by using the MPT as ion source and a linear ion trap mass spectrometer (LTQ-MS). These complex anions were produced in the plasma flame by an aqueous solution flowing through the central tube of the MPT, and were introduced into the inlet of the mass spectrometry working in negative ion <span class="hlt">mode</span> to get the feature mass spectrometric signals. Moreover, the feature fragment patterns of these ions in multi-step collision- induced dissociation processes have been explained. Under the optimized conditions, the limit of detection (LOD) using the MS2 (the second tandem mass spectrometry) procedure was estimated to be at the level of 10 μg/L for titanium and 20 μg/L for zirconium with linear dynamics ranges that cover at least two orders of magnitude, i.e., between 0–500 μg/L and 20–200 μg/L, respectively. These experimental data demonstrated that the MPT-MS is a promising and useful tool in field analysis of titanium and zirconium ions in <span class="hlt">water</span>, and can be applied in many fields, such as environmental control, hydrogeology, and <span class="hlt">water</span> quality inspection. In addition, MPT-MS could also be used as a supplement of ICP-MS for the rapid and on-site analysis of metal ions. PMID:28954404</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28954404','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28954404"><span>The Study of Titanium and Zirconium Ions in <span class="hlt">Water</span> by MPT-LTQ Mass Spectrometry in Negative <span class="hlt">Mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Junqing; Zheng, Mei; Liu, Qiuju; Yang, Meiling Zhu Chushan; Zhang, Yan; Zhu, Zhiqiang</p> <p>2017-09-26</p> <p>Microwave plasma torches (MPTs) can be used as simple and low power-consumption ambient ion sources. When MPT-mass spectrometry (MPT-MS) is applied in the detection of some metal elements, the metallic ions exhibit some novel features which are significantly different with those obtained by the traditional inductively coupled plasma (ICP)-mass spectrometry (ICP-MS) and may be helpful for metal element analysis. As the representative elements of group IVA, titanium and zirconium are both of importance and value in modern industry, and they have impacts on human health. Here, we first provide a study on the complex anions of titanium and zirconium in <span class="hlt">water</span> by using the MPT as ion source and a linear ion trap mass spectrometer (LTQ-MS). These complex anions were produced in the plasma flame by an aqueous solution flowing through the central tube of the MPT, and were introduced into the inlet of the mass spectrometry working in negative ion <span class="hlt">mode</span> to get the feature mass spectrometric signals. Moreover, the feature fragment patterns of these ions in multi-step collision- induced dissociation processes have been explained. Under the optimized conditions, the limit of detection (LOD) using the MS² (the second tandem mass spectrometry) procedure was estimated to be at the level of 10μg/L for titanium and 20 μg/L for zirconium with linear dynamics ranges that cover at least two orders of magnitude, i.e., between 0-500 μg/L and 20-200 μg/L, respectively. These experimental data demonstrated that the MPT-MS is a promising and useful tool in field analysis of titanium and zirconium ions in <span class="hlt">water</span>, and can be applied in many fields, such as environmental control, hydrogeology, and <span class="hlt">water</span> quality inspection. In addition, MPT-MS could also be used as a supplement of ICP-MS for the rapid and on-site analysis of metal ions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SurSc.669..103A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SurSc.669..103A"><span>Study of the <span class="hlt">modes</span> of adsorption and electronic structure of hydrogen peroxide and ethanol over TiO2 rutile (110) surface within the context of <span class="hlt">water</span> splitting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alghamdi, H.; Idriss, H.</p> <p>2018-03-01</p> <p>While photocatalytic <span class="hlt">water</span> splitting over many materials is favourable thermodynamically the kinetic of the reaction is very slow. One of the proposed reasons linked to the slow oxidation reaction rate is H2O2 formation as a reaction intermediate. Using Density Functional Theory (DFT) H2O2 is investigated on TiO2 rutile (110) surface to determine its most stable adsorption <span class="hlt">modes</span>: molecular, (H)O(H)O - (a), partially dissociated, (H)OO - (a), and fully dissociated (a) - OO - (a). We then compare H2O2 interaction to that of a fast hole scavenger molecule, ethanol. Geometry, electronic structure, charge density difference and work function determination of both adsorbates are presented and compared using DFT with different functionals (PBE, PBE-D, PBE-U, and HSE + D). H2O2 is found to be strongly adsorbed on TiO2 rutile (110) surface with adsorption energies reaching 0.95 eV, comparable to that of ethanol (0.89 eV); using GGA PBE. The negative changes in the work function upon adsorption were found to be highest for molecular adsorption ( - 1.23 eV) and lowest for the fully dissociated <span class="hlt">mode</span> ( - 0.54 eV) of H2O2. This may indicate that electrons flow from the surface to the adsorbate in order to make O(s)-H partially offset the overall magnitude of the oxygen lone pair interaction (of H2O2) with Ti4+ cations. Examination of the electronic structure through density of states (DOS) at the PBE level of computation, indicates that the H2O2 highest occupied molecular orbital (HOMO) level is not overlapping with oxygen atoms of TiO2 surface at any of its adsorption <span class="hlt">modes</span> and at any of the computation methods. Some overlap is seen using the HSE + D computational method. On the other hand the dissociated <span class="hlt">mode</span> of ethanol (ethoxides) does overlap with all computational methods used. The high adsorption energy and the absence of overlapping of the HOMO level of H2O2 with TiO2 rutile (110) surface may explain why <span class="hlt">water</span> splitting is slow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016LaPhL..13h5301C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016LaPhL..13h5301C"><span>Inter-comb synchronization by <span class="hlt">mode-to-mode</span> locking</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chun, Byung Jae; Kim, Young-Jin; Kim, Seung-Woo</p> <p>2016-08-01</p> <p>Two combs of fiber femtosecond lasers are synchronized through the optical frequency reference created by injection-locking of a diode laser to a single comb <span class="hlt">mode</span>. Maintaining a mHz-level narrow linewidth, the optical frequency reference permits two combs to be stabilized by <span class="hlt">mode-to-mode</span> locking with a relative stability of 1.52  ×  10-16 at 10 s with a frequency slip of 2.46 mHz. This inter-comb synchronization can be utilized for applications such as dual-comb spectroscopy or ultra-short pulse synthesis without extra narrow-linewidth lasers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29088162','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29088162"><span>Design of elliptical-core <span class="hlt">mode</span>-selective photonic lanterns with six <span class="hlt">modes</span> for MIMO-free <span class="hlt">mode</span> division multiplexing systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sai, Xiaowei; Li, Yan; Yang, Chen; Li, Wei; Qiu, Jifang; Hong, Xiaobin; Zuo, Yong; Guo, Hongxiang; Tong, Weijun; Wu, Jian</p> <p>2017-11-01</p> <p>Elliptical-core few <span class="hlt">mode</span> fiber (EC-FMF) is used in a <span class="hlt">mode</span> division multiplexing (MDM) transmission system to release multiple-input-multiple-output (MIMO) digital-signal-processing, which reduces the cost and the complexity of the receiver. However, EC-FMF does not match with conventional multiplexers/de-multiplexers (MUXs/DeMUXs) such as a photonic lantern, leading to extra <span class="hlt">mode</span> coupling loss and crosstalk. We design elliptical-core <span class="hlt">mode</span>-selective photonic lanterns (EC-MSPLs) with six <span class="hlt">modes</span>, which can match well with EC-FMF in MIMO-free MDM systems. Simulation of the EC-MSPL using the beam propagation method was demonstrated employing a combination of either step-index or graded-index fibers with six different sizes of cores, and the taper transition length of 8 cm or 4 cm. Through numerical simulations and optimizations, both types of photonic lanterns can realize low loss transmission and low crosstalk of below -20.0  dB for all <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ThEng..63..592B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ThEng..63..592B"><span>Definition of hydraulic stability of KVGM-100 hot-<span class="hlt">water</span> boiler and minimum <span class="hlt">water</span> flow rate</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belov, A. A.; Ozerov, A. N.; Usikov, N. V.; Shkondin, I. A.</p> <p>2016-08-01</p> <p>In domestic power engineering, the methods of quantitative and qualitative-quantitative adjusting the load of the heat supply systems are widely distributed; furthermore, during the greater part of the heating period, the actual discharge of network <span class="hlt">water</span> is less than estimated values when changing to quantitative adjustment. Hence, the hydraulic circuits of hot-<span class="hlt">water</span> boilers should ensure the <span class="hlt">water</span> velocities, minimizing the scale formation and excluding the formation of stagnant zones. The results of the calculations of hot-<span class="hlt">water</span> KVGM-100 boiler and minimum <span class="hlt">water</span> flow rate for the basic and peak <span class="hlt">modes</span> at the fulfillment of condition of the lack of surface boil are presented in the article. The minimal flow rates of <span class="hlt">water</span> at its underheating to the saturation state and the thermal flows in the furnace chamber were defined. The boiler hydraulic calculation was performed using the "Hydraulic" program, and the analysis of permissible and actual velocities of the <span class="hlt">water</span> movement in the pipes of the heating surfaces was carried out. Based on the thermal calculations of furnace chamber and thermal- hydraulic calculations of heating surfaces, the following conclusions were drawn: the minimum velocity of <span class="hlt">water</span> movement (by condition of boiling surface) at lifting movement of environment increases from 0.64 to 0.79 m/s; it increases from 1.14 to 1.38 m/s at down movement of environmental; the minimum <span class="hlt">water</span> flow rate by the boiler in the basic <span class="hlt">mode</span> (by condition of the surface boiling) increased from 887 t/h at the load of 20% up to 1074 t/h at the load of 100%. The minimum flow rate is 1074 t/h at nominal load and is achieved at the pressure at the boiler outlet equal to 1.1 MPa; the minimum <span class="hlt">water</span> flow rate by the boiler in the peak <span class="hlt">mode</span> by condition of surface boiling increases from 1669 t/h at the load of 20% up to 2021 t/h at the load of 100%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016isms.confETI02T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016isms.confETI02T"><span>Influence of Aromatic Molecules on the Structure and Spectroscopy of <span class="hlt">Water</span> Clusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tabor, Daniel P.; Sibert, Edwin; Walsh, Patrick S.; Zwier, Timothy S.</p> <p>2016-06-01</p> <p>Isomer-specific resonant ion-dip infrared spectra are presented for benzene-(<span class="hlt">water</span>)_n, 1-2-diphenoxyethane-(<span class="hlt">water</span>)_n, and tricyclophane-(<span class="hlt">water</span>)_n clusters. The IR spectra are modeled with a local <span class="hlt">mode</span> Hamiltonian that was originally formulated for the analysis of benzene-(<span class="hlt">water</span>)_n clusters with up to seven <span class="hlt">waters</span>. The model accounts for stretch-bend Fermi coupling, which can complicate the IR spectra in the 3150-3300 cm-1 region. When the <span class="hlt">water</span> clusters interact with each of the solutes, the hydrogen bond lengths between the <span class="hlt">water</span> molecules change in a characteristic way, reflecting the strength of the solute-<span class="hlt">water</span> interaction. These structural effects are also reflected spectroscopically in the shifts of the local <span class="hlt">mode</span> OH stretch frequencies. When diphenoxyethane is the solute, the <span class="hlt">water</span> clusters distort more significantly than when bound to benzene. Tricyclophane's structure provides an aromatic-rich binding pocket for the <span class="hlt">water</span> clusters. The local <span class="hlt">mode</span> model is used to extract Hamiltonians for individual <span class="hlt">water</span> molecules. These monomer Hamiltonians divide into groups based on their local H-bonding architecture, allowing for further classification of the wide variety of <span class="hlt">water</span> environments encountered in this study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JSMTE..05..013R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JSMTE..05..013R"><span><span class="hlt">Mode</span>-coupling theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reichman, David R.; Charbonneau, Patrick</p> <p>2005-05-01</p> <p>In this set of lecture notes we review the <span class="hlt">mode</span>-coupling theory of the glass transition from several perspectives. First, we derive <span class="hlt">mode</span>-coupling equations for the description of density fluctuations from microscopic considerations with the use the Mori Zwanzig projection operator technique. We also derive schematic <span class="hlt">mode</span>-coupling equations of a similar form from a field-theoretic perspective. We review the successes and failures of <span class="hlt">mode</span>-coupling theory, and discuss recent advances in the applications of the theory.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.5802S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.5802S"><span>Directional Analysis of <span class="hlt">Sub-Antarctic</span> Climate Change on South Georgia 1905-2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sakamoto Ferranti, Emma Jayne; Solera Garcia, Maria Angeles; Timmis, Roger James; Gerrard McKenna, Paul; Whyatt, James Duncan</p> <p>2010-05-01</p> <p>Directional analysis has been used to study changes in the sub-polar climate of the mountainous and glacierised <span class="hlt">sub-Antarctic</span> island of South Georgia (54-55°S, 36-38°W). Significantly for climate change studies, South Georgia lies in the Scotia Sea between polar and temperate latitudes, and approximately 1000 km northeast and downwind of the Antarctic Peninsula - one of the fastest-warming regions on Earth (Vaughan et al., 2001). South Georgia was chosen for directional analysis because its climate is substantially advected by predominantly westerly circulations, and because it has a long (since 1905) meteorological record from King Edward Point (KEP) on its eastern side. Additional shorter records from Bird Island at the northwest tip of South Georgia allow comparison between windward (Bird Island) and leeward (KEP) climate regimes. The variation of mountain barrier heights with direction from KEP allows climate changes to be studied under different amounts of orographic influence (from ~700 m to ~2200 m). Records of glacier advance and retreat provide further independent evidence of climate change for comparison with the meteorological record. Directional climate analysis is based on a series of monthly-mean pressure fields defining the orientation and strength of synoptic-scale air-mass advection over the Scotia Sea. These fields are used to define directional climatologies for six 30° sectors with bearings from 150-180° to 300-330°; these sectors encompass 99% of recorded months since 1905. The climatologies summarise the frequencies of air masses from each sector, and the accompanying temperatures and precipitation. The 6 sectors can be broadly associated with 4 air-mass types and source regions: (i) sectors 150-210° advect cold polar maritime air that originated over the Antarctic continent before passing over the Weddell Sea, (ii) sectors 210-270° advect warmer, more stable polar maritime air from the Bellingshausen Sea/Antarctic Peninsula region</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750020647','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750020647"><span>Advanced <span class="hlt">water</span> iodinating system. [for potable <span class="hlt">water</span> aboard manned spacecraft</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Davenport, R. J.; Schubert, F. H.; Wynveen, R. A.</p> <p>1975-01-01</p> <p>Potable <span class="hlt">water</span> stores aboard manned spacecraft must remain sterile. Suitable sterilization techniques are needed to prevent microbial growth. The development of an advanced <span class="hlt">water</span> iodinating system for possible application to the shuttle orbiter and other advanced spacecraft, is considered. The AWIS provides a means of automatically dispensing iodine and controlling iodination levels in potable <span class="hlt">water</span> stores. In a recirculation <span class="hlt">mode</span> test, simulating application of the AWIS to a <span class="hlt">water</span> management system of a long term six man capacity space mission, noniodinated feed <span class="hlt">water</span> flowing at 32.2 cu cm min was iodinated to 5 + or - ppm concentrations after it was mixed with previously iodinated <span class="hlt">water</span> recirculating through a potable <span class="hlt">water</span> storage tank. Also, the AWIS was used to successfully demonstrate its capability to maintain potable <span class="hlt">water</span> at a desired I2 concentration level while circulating through the <span class="hlt">water</span> storage tank, but without the addition of noniodinated <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1918401P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1918401P"><span>Drivers of Antarctic sea-ice expansion and Southern Ocean surface cooling over the past four decades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Purich, Ariaan; England, Matthew</p> <p>2017-04-01</p> <p>Despite global warming, total Antarctic sea-ice coverage has increased overall during the past four decades. In contrast, the majority of CMIP5 models simulate a decline. In addition, Southern Ocean surface <span class="hlt">waters</span> have largely cooled, in stark contrast to almost all historical CMIP5 simulations. <span class="hlt">Subantarctic</span> Surface <span class="hlt">Waters</span> have cooled and freshened while <span class="hlt">waters</span> to the north of the Antarctic Circumpolar Current have warmed and increased in salinity. It remains unclear as to what extent the cooling and Antarctic sea-ice expansion is due to natural variability versus anthropogenic forcing; due for example to changes in the Southern Annular <span class="hlt">Mode</span> (SAM). It is also unclear what the respective role of surface buoyancy fluxes is compared to internal ocean circulation changes, and what the implications are for longer-term climate change in the region. In this presentation we will outline three distinct drivers of recent Southern Ocean surface trends that have each made a significant contribution to regional cooling: (1) wind-driven surface cooling and sea-ice expansion due to shifted westerly winds, (2) teleconnections of decadal variability from the tropical Pacific, and (3) surface cooling and ice expansion due to large-scale Southern Ocean freshening, most likely driven by SAM-related precipitation trends over the open ocean. We will also outline the main reasons why climate models for the most part miss these Southern Ocean cooling trends, despite capturing overall trends in the SAM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22489541-dissociative-chemisorption-water-ni-mode-bond-selective-chemistry-metal-surfaces','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22489541-dissociative-chemisorption-water-ni-mode-bond-selective-chemistry-metal-surfaces"><span>The dissociative chemisorption of <span class="hlt">water</span> on Ni(111): <span class="hlt">Mode</span>- and bond-selective chemistry on metal surfaces</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>Farjamnia, Azar; Jackson, Bret, E-mail: jackson@chem.umass.edu</p> <p></p> <p>A fully quantum approach based on an expansion in vibrationally adiabatic eigenstates is used to explore the dissociative chemisorption of H{sub 2}O, HOD, and D{sub 2}O on Ni(111). For this late barrier system, excitation of both the bending and stretching <span class="hlt">modes</span> significantly enhances dissociative sticking. The vibrational efficacies vary somewhat from <span class="hlt">mode-to-mode</span> but are all relatively close to one, in contrast to methane dissociation, where the behavior is less statistical. Similar to methane dissociation, the motion of lattice atoms near the dissociating molecule can significantly modify the height of the barrier to dissociation, leading to a strong variation in dissociativemore » sticking with substrate temperature. Given a rescaling of the barrier height, our results are in reasonable agreement with measurements of the dissociative sticking of D{sub 2}O on Ni(111), for both laser-excited molecules with one or two quanta of excitation in the antisymmetric stretch and in the absence of laser excitation. Even without laser excitation, the beam contains vibrationally excited molecules populated at the experimental source temperature, and these make significant contributions to the sticking probability. At high collision energies, above the adiabatic barrier heights, our results correlate with these barrier heights and <span class="hlt">mode</span> softening effects. At lower energies, dissociative sticking occurs primarily via vibrationally nonadiabatic pathways. We find a preference for O–H over O–D bond cleavage for ground state HOD molecules at all but the highest collision energies, and excitation of the O–H stretch gives close to 100% O–H selectivity at lower energies. Excitation of the O–D stretch gives a lower O–D cleavage selectivity, as the interaction with the surface leads to energy transfer from the O–D stretch into the O–H bond, when <span class="hlt">mode</span> softening makes these vibrations nearly degenerate.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22493814-particle-simulations-mode-conversion-between-slow-mode-fast-mode-lower-hybrid-range-frequencies','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22493814-particle-simulations-mode-conversion-between-slow-mode-fast-mode-lower-hybrid-range-frequencies"><span>Particle simulations of <span class="hlt">mode</span> conversion between slow <span class="hlt">mode</span> and fast <span class="hlt">mode</span> in lower hybrid range of frequencies</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>Jia, Guozhang; Xiang, Nong; Huang, Yueheng</p> <p>2016-01-15</p> <p>The propagation and <span class="hlt">mode</span> conversion of lower hybrid waves in an inhomogeneous plasma are investigated by using the nonlinear δf algorithm in a two-dimensional particle-in-cell simulation code based on the gyrokinetic electron and fully kinetic ion (GeFi) scheme [Lin et al., Plasma Phys. Controlled Fusion 47, 657 (2005)]. The characteristics of the simulated waves, such as wavelength, frequency, phase, and group velocities, agree well with the linear theoretical analysis. It is shown that a significant reflection component emerges in the conversion process between the slow <span class="hlt">mode</span> and the fast <span class="hlt">mode</span> when the scale length of the density variation is comparablemore » to the local wavelength. The dependences of the reflection coefficient on the scale length of the density variation are compared with the results based on the linear full wave model for cold plasmas. It is indicated that the <span class="hlt">mode</span> conversion for the waves with a frequency of 2.45 GHz (ω ∼ 3ω{sub LH}, where ω{sub LH} represents the lower hybrid resonance) and within Tokamak relevant amplitudes can be well described in the linear scheme. As the frequency decreases, the modification due to the nonlinear term becomes important. For the low-frequency waves (ω ∼ 1.3ω{sub LH}), the generations of the high harmonic <span class="hlt">modes</span> and sidebands through nonlinear <span class="hlt">mode-mode</span> coupling provide new power channels and thus could reduce the reflection significantly.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29092317','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29092317"><span>Accurate <span class="hlt">mode</span> characterization of two-<span class="hlt">mode</span> optical fibers by in-fiber acousto-optics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Alcusa-Sáez, E; Díez, A; Andrés, M V</p> <p>2016-03-07</p> <p>Acousto-optic interaction in optical fibers is exploited for the accurate and broadband characterization of two-<span class="hlt">mode</span> optical fibers. Coupling between LP 01 and LP 1m <span class="hlt">modes</span> is produced in a broadband wavelength range. Difference in effective indices, group indices, and chromatic dispersions between the guided <span class="hlt">modes</span>, are obtained from experimental measurements. Additionally, we show that the technique is suitable to investigate the fine <span class="hlt">modes</span> structure of LP <span class="hlt">modes</span>, and some other intriguing features related with <span class="hlt">modes</span>' cut-off.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19940024966','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19940024966"><span>Transient analysis <span class="hlt">mode</span> participation for modal survey target <span class="hlt">mode</span> selection using MSC/NASTRAN DMAP</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Barnett, Alan R.; Ibrahim, Omar M.; Sullivan, Timothy L.; Goodnight, Thomas W.</p> <p>1994-01-01</p> <p>Many methods have been developed to aid analysts in identifying component <span class="hlt">modes</span> which contribute significantly to component responses. These <span class="hlt">modes</span>, typically targeted for dynamic model correlation via a modal survey, are known as target <span class="hlt">modes</span>. Most methods used to identify target <span class="hlt">modes</span> are based on component global dynamic behavior. It is sometimes unclear if these methods identify all <span class="hlt">modes</span> contributing to responses important to the analyst. These responses are usually those in areas of hardware design concerns. One method used to check the completeness of target <span class="hlt">mode</span> sets and identify <span class="hlt">modes</span> contributing significantly to important component responses is <span class="hlt">mode</span> participation. With this method, the participation of component <span class="hlt">modes</span> in dynamic responses is quantified. Those <span class="hlt">modes</span> which have high participation are likely modal survey target <span class="hlt">modes</span>. <span class="hlt">Mode</span> participation is most beneficial when it is used with responses from analyses simulating actual flight events. For spacecraft, these responses are generated via a structural dynamic coupled loads analysis. Using MSC/NASTRAN DMAP, a method has been developed for calculating <span class="hlt">mode</span> participation based on transient coupled loads analysis results. The algorithm has been implemented to be compatible with an existing coupled loads methodology and has been used successfully to develop a set of modal survey target <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DFDA16002H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DFDA16002H"><span>Performance enhancing <span class="hlt">water</span> skipping: successive free surface impacts of elastic spheres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hurd, Randy; Truscott, Tadd; Belden, Jesse</p> <p>2014-11-01</p> <p>From naval gunners skipping cannonballs to children skipping stones, physicists have long been enamored with the repeated ricochet of objects on the <span class="hlt">water</span> surface. Elastic spheres, such as the toy Waboba ball, make <span class="hlt">water</span> skipping more accessible to the masses by expanding the range of impact parameters over which objects can be skipped. For example, it is not difficult to achieve more than twenty skips with such spheres, where skipping a stone twenty times is very difficult. In this talk we discuss the dynamics of <span class="hlt">water</span> skipping elastic spheres over several successive skips. High-speed video captured using a unique experimental setup reveals how dynamics change with each skip as a result of lost kinetic energy. We place these observations in the context of previous work on single oblique impacts to identify material vibration <span class="hlt">modes</span> that are excited during ricochet. The material <span class="hlt">modes</span> excited with each successive impact are seen to decay from high-energy <span class="hlt">modes</span> to low energy <span class="hlt">modes</span> until <span class="hlt">water</span> entry finally occurs. A model for estimating skipping outcome from initial conditions is proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1007911','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1007911"><span><span class="hlt">Water</span>-heating dehumidifier</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Tomlinson, John J.</p> <p>2006-04-18</p> <p>A <span class="hlt">water</span>-heating dehumidifier includes a refrigerant loop including a compressor, at least one condenser, an expansion device and an evaporator including an evaporator fan. The condenser includes a <span class="hlt">water</span> inlet and a <span class="hlt">water</span> outlet for flowing <span class="hlt">water</span> therethrough or proximate thereto, or is affixed to the tank or immersed into the tank to effect <span class="hlt">water</span> heating without flowing <span class="hlt">water</span>. The immersed condenser design includes a self-insulated capillary tube expansion device for simplicity and high efficiency. In a <span class="hlt">water</span> heating <span class="hlt">mode</span> air is drawn by the evaporator fan across the evaporator to produce cooled and dehumidified air and heat taken from the air is absorbed by the refrigerant at the evaporator and is pumped to the condenser, where <span class="hlt">water</span> is heated. When the tank of <span class="hlt">water</span> heater is full of hot <span class="hlt">water</span> or a humidistat set point is reached, the <span class="hlt">water</span>-heating dehumidifier can switch to run as a dehumidifier.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11580674','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11580674"><span>Direct observation of terahertz surface <span class="hlt">modes</span> in nanometer-sized liquid <span class="hlt">water</span> pools.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Boyd, J E; Briskman, A; Colvin, V L; Mittleman, D M</p> <p>2001-10-01</p> <p>The far-infrared absorption spectrum of nanometer-sized <span class="hlt">water</span> pools at the core of AOT micelles exhibits a pronounced resonance which is absent in bulk <span class="hlt">water</span>. The amplitude and spectral position of this resonance are sensitive to the size of the confined <span class="hlt">water</span> core. This resonance results from size-dependent modifications in the vibrational density of states, and thus has far-reaching implications for chemical processes which involve <span class="hlt">water</span> sequestered within small cavities. These data represent the first study of the terahertz dielectric properties of confined liquids.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17789444','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17789444"><span>Interhemispheric correlation of late pleistocene glacial events.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lowell, T V; Heusser, C J; Andersen, B G; Moreno, P I; Hauser, A; Heusser, L E; Schlüchter, C; Marchant, D R; Denton, G H</p> <p>1995-09-15</p> <p>A radiocarbon chronology shows that piedmont glacier lobes in the Chilean Andes achieved maxima during the last glaciation at 13,900 to 14,890, 21,000, 23,060, 26,940, 29,600, and >/=33,500 carbon-14 years before present ((14)C yr B.P.) in a cold and wet <span class="hlt">Subantarctic</span> Parkland environment. The last glaciation ended with massive collapse of ice lobes close to 14,000(14)C yr B.P., accompanied by an influx of North Patagonian Rain Forest species. In the Southern Alps of New Zealand, additional glacial maxima are registered at 17,720(14)C yr B.P., and at the beginning of the Younger Dryas at 11,050 (14)C yr B. P. These glacial maxima in mid-latitude mountains rimming the South Pacific were coeval with ice-rafting pulses in the North Atlantic Ocean. Furthermore, the last termination began suddenly and simultaneously in both polar hemispheres before the resumption of the modern <span class="hlt">mode</span> of deep-<span class="hlt">water</span> production in the Nordic Seas. Such interhemispheric coupling implies a global atmospheric signal rather than regional climatic changes caused by North Atlantic thermohaline switches or Laurentide ice surges.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMNG43A1670T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMNG43A1670T"><span>Evaluation of Oceanic Transport Statistics By Use of Transient Tracers and Bayesian Methods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Trossman, D. S.; Thompson, L.; Mecking, S.; Bryan, F.; Peacock, S.</p> <p>2013-12-01</p> <p>Key variables that quantify the time scales over which atmospheric signals penetrate into the oceanic interior and their uncertainties are computed using Bayesian methods and transient tracers from both models and observations. First, the mean residence times, subduction rates, and formation rates of Subtropical <span class="hlt">Mode</span> <span class="hlt">Water</span> (STMW) and Subpolar <span class="hlt">Mode</span> <span class="hlt">Water</span> (SPMW) in the North Atlantic and <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span> (SAMW) in the Southern Ocean are estimated by combining a model and observations of chlorofluorocarbon-11 (CFC-11) via Bayesian Model Averaging (BMA), statistical technique that weights model estimates according to how close they agree with observations. Second, a Bayesian method is presented to find two oceanic transport parameters associated with the age distribution of ocean <span class="hlt">waters</span>, the transit-time distribution (TTD), by combining an eddying global ocean model's estimate of the TTD with hydrographic observations of CFC-11, temperature, and salinity. Uncertainties associated with objectively mapping irregularly spaced bottle data are quantified by making use of a thin-plate spline and then propagated via the two Bayesian techniques. It is found that the subduction of STMW, SPMW, and SAMW is mostly an advective process, but up to about one-third of STMW subduction likely owes to non-advective processes. Also, while the formation of STMW is mostly due to subduction, the formation of SPMW is mostly due to other processes. About half of the formation of SAMW is due to subduction and half is due to other processes. A combination of air-sea flux, acting on relatively short time scales, and turbulent mixing, acting on a wide range of time scales, is likely the dominant SPMW erosion mechanism. Air-sea flux is likely responsible for most STMW erosion, and turbulent mixing is likely responsible for most SAMW erosion. Two oceanic transport parameters, the mean age of a <span class="hlt">water</span> parcel and the half-variance associated with the TTD, estimated using the model's tracers as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013Ap%26SS.345...41H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013Ap%26SS.345...41H"><span>Determination of intrinsic <span class="hlt">mode</span> and linear <span class="hlt">mode</span> coupling in solar microwave bursts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Guangli; Song, Qiwu; Li, Jianping</p> <p>2013-05-01</p> <p>An explicit equation of the propagational angle of microwave emission between the line-of-sight and the local magnetic field is newly derived based on the approximated formulae of nonthermal gyrosynchrotron emission (Dulk and Marsh in Astrophys. J. 259, 350, 1982). The existence of the solution of propagational angle is clearly shown under a series of typical parameters in solar microwave observations. It could be used to determine the intrinsic <span class="hlt">mode</span> and linear <span class="hlt">mode</span> coupling in solar microwave bursts by three steps. (1) The <span class="hlt">mode</span> coupling may happen only when the angle approximately equals to 90 degrees, i.e., when the emission propagates through the quasi-transverse region (Cohen in Astrophys. J. 131, 664, 1960). (2) The inversion of polarization sense due to the weakly <span class="hlt">mode</span> coupling takes place only when the transition frequency defined by Cohen (1960) is larger than the frequency of microwave emission, and an observable criterion of the weakly <span class="hlt">mode</span> coupling in flaring loops was indicated by the same polarization sense in the two footpoints of a flaring loop (Melrose and Robinson in Proc. Astron. Soc. Aust. 11, 16, 1994). (3) Finally, the intrinsic <span class="hlt">mode</span> of microwave emission is determined by the observed polarization and the calculated direction of local magnetic field according to the general plasma dispersion relation, together with the <span class="hlt">mode</span> coupling process. However, a 180-degree ambiguity still exists in the direction of longitudinal magnetic field, to produce an uncertainty of the intrinsic <span class="hlt">mode</span>. One example is selected to check the feasibility of the method in the 2001 September 25 event with a loop-like structure nearby the central meridian passage observed by Nobeyama Radio Heliograph and Polarimeters. The calculated angle in one footpoint (FP) varied around 90∘ in two time intervals of the maximum phase, which gives a direct evidence of the emission propagating through a quasi-transverse region where the linear <span class="hlt">mode</span> coupling took place, while, the angle</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140016593','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140016593"><span>Dual-<span class="hlt">Mode</span> Combustor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Trefny, Charles J (Inventor); Dippold, Vance F (Inventor)</p> <p>2013-01-01</p> <p>A new dual-<span class="hlt">mode</span> ramjet combustor used for operation over a wide flight Mach number range is described. Subsonic combustion <span class="hlt">mode</span> is usable to lower flight Mach numbers than current dual-<span class="hlt">mode</span> scramjets. High speed <span class="hlt">mode</span> is characterized by supersonic combustion in a free-jet that traverses the subsonic combustion chamber to a variable nozzle throat. Although a variable combustor exit aperture is required, the need for fuel staging to accommodate the combustion process is eliminated. Local heating from shock-boundary-layer interactions on combustor walls is also eliminated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22364771','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22364771"><span>Capacitive deionization coupled with microbial fuel cells to desalinate low-concentration salt <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yuan, Lulu; Yang, Xufei; Liang, Peng; Wang, Lei; Huang, Zheng-Hong; Wei, Jincheng; Huang, Xia</p> <p>2012-04-01</p> <p>A new technology (CDI-MFC) that combined capacitive deionization (CDI) and microbial fuel cell (MFC) was developed to treat low-concentration salt <span class="hlt">water</span> with NaCl concentration of 60mg/L. The <span class="hlt">water</span> desalination rate was 35.6mg/(Lh), meanwhile the charge efficiency was 21.8%. Two desorption <span class="hlt">modes</span> were investigated: discharging (DC) <span class="hlt">mode</span> and short circuit (SC) <span class="hlt">mode</span>. The desalination rate in the DC <span class="hlt">mode</span> was 200.6±3.1mg/(Lh), 47.8% higher than that in the SC <span class="hlt">mode</span> [135.7±15.3mg/(Lh)]. The average current in the DC <span class="hlt">mode</span> was also much higher than that of the SC <span class="hlt">mode</span>. The energy stored in the CDI cell has been reused to enhance the electron production of MFC by the discharging desorption <span class="hlt">mode</span> (DC <span class="hlt">mode</span>), which offers an approach to recover the electrostatic energy in the CDI cell. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16771322','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16771322"><span>Thermal diffusion behavior of nonionic surfactants in <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ning, Hui; Kita, Rio; Kriegs, Hartmut; Luettmer-Strathmann, Jutta; Wiegand, Simone</p> <p>2006-06-08</p> <p>We studied the thermal diffusion behavior of hexaethylene glycol monododecyl ether (C12E6) in <span class="hlt">water</span> by means of thermal diffusion forced Rayleigh scattering (TDFRS) and determined Soret coefficients, thermal diffusion coefficients, and diffusion constants at different temperatures and concentrations. At low surfactant concentrations, the measured Soret coefficient is positive, which implies that surfactant micelles move toward the cold region in a temperature gradient. For C12E6/<span class="hlt">water</span> at a high surfactant concentration of w1 = 90 wt % and a temperature of T = 25 degrees C, however, a negative Soret coefficient S(T) was observed. Because the concentration part of the TDFRS diffraction signal for binary systems is expected to consist of a single <span class="hlt">mode</span>, we were surprised to find a second, slow <span class="hlt">mode</span> for C12E6/<span class="hlt">water</span> system in a certain temperature and concentration range. To clarify the origin of this second <span class="hlt">mode</span>, we investigated also, tetraethylene glycol monohexyl ether (C6E4), tetraethylene glycol monooctyl ether (C8E4), pentaethylene glycol monododecyl ether (C12E5), and octaethylene glycol monohexadecyl ether (C16E8) and compared the results with the previous results for octaethylene glycol monodecyl ether (C10E8). Except for C6E4 and C10E8, a second slow <span class="hlt">mode</span> was observed in all systems usually for state points close to the phase boundary. The diffusion coefficient and Soret coefficient derived from the fast <span class="hlt">mode</span> can be identified as the typical mutual diffusion and Soret coefficients of the micellar solutions and compare well with the independently determined diffusion coefficients in a dynamic light scattering experiment. Experiments with added salt show that the slow <span class="hlt">mode</span> is suppressed by the addition of w(NaCl) = 0.02 mol/L sodium chloride. This suggests that the slow <span class="hlt">mode</span> is related to the small amount of absorbing ionic dye, less than 10(-5) by weight, which is added in TDFRS experiments to create a temperature grating. The origin of the slow <span class="hlt">mode</span> of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1176124','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1176124"><span>Zero-<span class="hlt">mode</span> waveguides</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Levene, Michael J.; Korlach, Jonas; Turner, Stephen W.; Craighead, Harold G.; Webb, Watt W.</p> <p>2007-02-20</p> <p>The present invention is directed to a method and an apparatus for analysis of an analyte. The method involves providing a zero-<span class="hlt">mode</span> waveguide which includes a cladding surrounding a core where the cladding is configured to preclude propagation of electromagnetic energy of a frequency less than a cutoff frequency longitudinally through the core of the zero-<span class="hlt">mode</span> waveguide. The analyte is positioned in the core of the zero-<span class="hlt">mode</span> waveguide and is then subjected, in the core of the zero-<span class="hlt">mode</span> waveguide, to activating electromagnetic radiation of a frequency less than the cut-off frequency under conditions effective to permit analysis of the analyte in an effective observation volume which is more compact than if the analysis were carried out in the absence of the zero-<span class="hlt">mode</span> waveguide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AMT.....9.2253K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AMT.....9.2253K"><span>Retrieving atmospheric turbulence information from regular commercial aircraft using <span class="hlt">Mode-S</span> and ADS-B</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kopeć, Jacek M.; Kwiatkowski, Kamil; de Haan, Siebren; Malinowski, Szymon P.</p> <p>2016-05-01</p> <p>Navigational information broadcast by commercial aircraft in the form of <span class="hlt">Mode-S</span> EHS (<span class="hlt">Mode-S</span> Enhanced Surveillance) and ADS-B (Automatic Dependent Surveillance-Broadcast) messages can be considered a new source of upper tropospheric and lower stratospheric turbulence estimates. A set of three processing methods is proposed and analysed using a quality record of turbulence encounters made by a research aircraft.The proposed methods are based on processing the vertical acceleration or the background wind into the eddy dissipation rate. Turbulence intensity can be estimated using the standard content of the <span class="hlt">Mode-S</span> EHS/ADS-B.The results are based on a <span class="hlt">Mode-S</span> EHS/ADS-B data set generated synthetically based on the transmissions from the research aircraft. This data set was validated using the overlapping record of the <span class="hlt">Mode-S</span> EHS/ADS-B received from the same research aircraft. The turbulence intensity, meaning the eddy dissipation rate, obtained from the proposed methods based on the <span class="hlt">Mode-S</span> EHS/ADS-B is compared with the value obtained using on-board accelerometer. The results of the comparison indicate the potential of the methods. The advantages and limitation of the presented approaches are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NPGeo..24..645K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NPGeo..24..645K"><span>Kinematic parameters of internal waves of the second <span class="hlt">mode</span> in 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>Kurkina, Oxana; Talipova, Tatyana; Soomere, Tarmo; Giniyatullin, Ayrat; Kurkin, Andrey</p> <p>2017-10-01</p> <p>Spatial distributions of the main properties of the <span class="hlt">mode</span> function and kinematic and non-linear parameters of internal waves of the second <span class="hlt">mode</span> are derived for the South China Sea for typical summer conditions in July. The calculations are based on the Generalized Digital Environmental Model (GDEM) climatology of hydrological variables, from which the local stratification is evaluated. The focus is on the phase speed of long internal waves and the coefficients at the dispersive, quadratic and cubic terms of the weakly non-linear Gardner model. Spatial distributions of these parameters, except for the coefficient at the cubic term, are qualitatively similar for waves of both <span class="hlt">modes</span>. The dispersive term of Gardner's equation and phase speed for internal waves of the second <span class="hlt">mode</span> are about a quarter and half, respectively, of those for waves of the first <span class="hlt">mode</span>. Similarly to the waves of the first <span class="hlt">mode</span>, the coefficients at the quadratic and cubic terms of Gardner's equation are practically independent of <span class="hlt">water</span> depth. In contrast to the waves of the first <span class="hlt">mode</span>, for waves of the second <span class="hlt">mode</span> the quadratic term is mostly negative. The results can serve as a basis for expressing estimates of the expected parameters of internal waves for the South China Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AdAtS..35..540Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AdAtS..35..540Y"><span>Organizational <span class="hlt">Modes</span> of Severe Wind-producing Convective Systems over North China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Xinlin; Sun, Jianhua</p> <p>2018-05-01</p> <p>Severe weather reports and composite radar reflectivity data from 2010-14 over North China were used to analyze the distribution of severe convective wind (SCW) events and their organizational <span class="hlt">modes</span> of radar reflectivity. The six organizational <span class="hlt">modes</span> for SCW events (and their proportions) were cluster cells (35.4%), squall lines (18.4%), nonlinear-shaped systems (17.8%), broken lines (11.6%), individual cells (1.2%), and bow echoes (0.5%). The peak month for both squall lines and broken lines was June, whereas it was July for the other four <span class="hlt">modes</span>. The highest numbers of SCW events were over the mountains, which were generally associated with disorganized systems of cluster cells. In contrast, SCW associated with linear systems occurred mainly over the plains, where stations recorded an average of less than one SCW event per year. Regions with a high frequency of SCW associated with nonlinear-shaped systems also experienced many SCW events associated with squall lines. Values of convective available potential energy, precipitable <span class="hlt">water</span>, 0-3-km shear, and 0-6-km shear, were demonstrably larger over the plains than over the mountains, which had an evident effect on the organizational <span class="hlt">modes</span> of SCW events. Therefore, topography may be an important factor in the organizational <span class="hlt">modes</span> for SCW events over North China.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..MARG14003T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..MARG14003T"><span><span class="hlt">Water</span> Bouncing Balls: how material stiffness affects <span class="hlt">water</span> entry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Truscott, Tadd</p> <p>2014-03-01</p> <p>It is well known that one can skip a stone across the <span class="hlt">water</span> surface, but less well known that a ball can also be skipped on <span class="hlt">water</span>. Even though 17th century ship gunners were aware that cannonballs could be skipped on the <span class="hlt">water</span> surface, they did not know that using elastic spheres rather than rigid ones could greatly improve skipping performance (yet would have made for more peaceful volleys). The <span class="hlt">water</span> bouncing ball (Waboba®) is an elastic ball used in a game of aquatic keep away in which players pass the ball by skipping it along the <span class="hlt">water</span> surface. The ball skips easily along the surface creating a sense that breaking the world record for number of skips could easily be achieved (51 rock skips Russell Byers 2007). We investigate the physics of skipping elastic balls to elucidate the mechanisms by which they bounce off of the <span class="hlt">water</span>. High-speed video reveals that, upon impact with the <span class="hlt">water</span>, the balls create a cavity and deform significantly due to the extreme elasticity; the flattened spheres resemble skipping stones. With an increased wetted surface area, a large hydrodynamic lift force is generated causing the ball to launch back into the air. Unlike stone skipping, the elasticity of the ball plays an important roll in determining the success of the skip. Through experimentation, we demonstrate that the deformation timescale during impact must be longer than the collision time in order to achieve a successful skip. Further, several material deformation <span class="hlt">modes</span> can be excited upon free surface impact. The effect of impact velocity and angle on the two governing timescales and material wave <span class="hlt">modes</span> are also experimentally investigated. Scaling for the deformation and collision times are derived and used to establish criteria for skipping in terms of relevant physical parameters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011SPIE.7903E..2PM','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011SPIE.7903E..2PM"><span>Multiphoton endoscopy based on a <span class="hlt">mode</span>-filtered single-<span class="hlt">mode</span> fiber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moon, Sucbei; Liu, Gangjun; Chen, Zhongping</p> <p>2011-03-01</p> <p>We present a new low-nonlinearity fiber of <span class="hlt">mode</span>-filtered large-core fiber for flexible beam delivery of intense pulsed light aiming at multi-photon endoscopy application. A multimode fiber of a large core diameter (20 μm) equips a <span class="hlt">mode</span> filtering means in the middle of the fiber link to suppress the high-order <span class="hlt">modes</span> selectively. A large effective core area of ~200 μm2 has been achieved at 0.8-μm and 1.0-μm bands. This is 8 times larger than the core area of a conventional SMF used for those spectral bands. Various advantages of our large-<span class="hlt">mode</span> area fiber will be demonstrated and discussed in this report.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14503384','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14503384"><span>Urban community perception towards intermittent <span class="hlt">water</span> supply system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Joshi, M W; Talkhande, A V; Andey, S P; Kelkar, P S</p> <p>2002-04-01</p> <p>While evaluating intermittent and continuous <span class="hlt">water</span> supply systems, consumers opinion survey was undertaken for critical appraisal of both <span class="hlt">modes</span> of operation. With the help of a pre-designed set of questions relating to various aspects of <span class="hlt">water</span> supply and the opinion of consumers regarding degree of service, a house to house survey was conducted in the study area of Ghaziabad and Jaipur. The consumer opinion survey clearly indicated a satisfactory degree of service wherever adequate quantity of <span class="hlt">water</span> was made available irrespective of the <span class="hlt">mode</span> of <span class="hlt">water</span> supply. Number of complaints regarding quality of <span class="hlt">water</span> supplied, timings of supply, low pressures and breakdowns in supply were reported during intermittent <span class="hlt">water</span> supply. Every family stored <span class="hlt">water</span> for drinking and other uses. Most of the families discard drinking <span class="hlt">water</span> once the fresh <span class="hlt">water</span> supply is resumed next day. Discarded drinking <span class="hlt">water</span> is usually used in kitchen for washing and gardening. Storage for other purposes depends on economic status and availability of other sources like open dug well in the house. While most of the respondents had no complaints on <span class="hlt">water</span> tariff, all of them were in favour of continuous <span class="hlt">water</span> supply.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhLA..382.1176A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhLA..382.1176A"><span>Dynamics of a camphoric acid boat at the air-<span class="hlt">water</span> interface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Akella, V. S.; Singh, Dhiraj K.; Mandre, Shreyas; Bandi, M. M.</p> <p>2018-05-01</p> <p>We report experiments on an agarose gel tablet loaded with camphoric acid (c-boat) spontaneously set into motion by surface tension gradients on the <span class="hlt">water</span> surface. We observe three distinct <span class="hlt">modes</span> of c-boat motion: harmonic <span class="hlt">mode</span> where the c-boat speed oscillates sinusoidally in time, a steady <span class="hlt">mode</span> where the c-boat maintains constant speed, and an intermittent <span class="hlt">mode</span> where the c-boat maintains near-zero speed between sudden jumps in speed. Whereas all three <span class="hlt">modes</span> have been separately reported before in different systems, controlled release of Camphoric Acid (CA) from the agarose gel matrix allowed the observation of all the three <span class="hlt">modes</span> in the same system. These three <span class="hlt">modes</span> are a result of a competition between the driving (surface tension gradients) and drag forces acting on the c-boat. Moreover we suggest that there exist two time scales corresponding to spreading of CA and boat motion and the mismatch of these two time scales give rise to the three <span class="hlt">modes</span> in boat motion. We reproduced all the <span class="hlt">modes</span> of motion by varying the air-<span class="hlt">water</span> interfacial tension using Sodium Dodecyl Sulfate (SDS).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/902761','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/902761"><span>Multi-<span class="hlt">mode</span> radio frequency device</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Gilbert, Ronald W [Morgan Hill, CA; Carrender, Curtis Lee [Morgan Hill, CA; Anderson, Gordon A [Benton City, WA; Steele, Kerry D [Kennewick, WA</p> <p>2007-02-13</p> <p>A transponder device having multiple <span class="hlt">modes</span> of operation, such as an active <span class="hlt">mode</span> and a passive <span class="hlt">mode</span>, wherein the <span class="hlt">modes</span> of operation are selected in response to the strength of a received radio frequency signal. A communication system is also provided having a transceiver configured to transmit a radio frequency signal and to receive a responsive signal, and a transponder configured to operate in a plurality of <span class="hlt">modes</span> and to activate <span class="hlt">modes</span> of operation in response to the radio frequency signal. Ideally, each <span class="hlt">mode</span> of operation is activated and deactivated independent of the other <span class="hlt">modes</span>, although two or more <span class="hlt">modes</span> may be concurrently operational.</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/2018OptCo.408...58I','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptCo.408...58I"><span>All-fiber-based selective <span class="hlt">mode</span> multiplexer and demultiplexer for weakly-coupled <span class="hlt">mode</span>-division multiplexed systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Igarashi, Koji; Park, Kyung Jun; Tsuritani, Takahiro; Morita, Itsuro; Kim, Byoung Yoon</p> <p>2018-02-01</p> <p>We show all-fiber-based selective <span class="hlt">mode</span> multiplexers and demultiplexers for weakly-coupled <span class="hlt">mode</span>-division multiplexed systems. We fabricate a set of six-<span class="hlt">mode</span> multiplexer and demultiplexer based on fiber <span class="hlt">mode</span> selective couplers, and experimentally evaluate the performance for the six-<span class="hlt">mode</span> dual-polarization (DP) quadrature phase shift keying (QPSK) optical signals. In the <span class="hlt">mode</span> multiplexer and demultiplexer, the <span class="hlt">mode</span> couplings between the lower three <span class="hlt">modes</span> and the higher three <span class="hlt">modes</span> are suppressed to be less than -20 dB, which enables us to apply partial 6 ×6 MIMO equalizers even for the six-<span class="hlt">mode</span> demultiplexing. For the six-<span class="hlt">mode</span> DP-QPSK signals, the penalty of optical signal-to-noise ratio by replacing the full 12 ×12MIMO to the partial 6 ×6 MIMO is suppressed by less than 1 dB.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/913583','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/913583"><span>List <span class="hlt">mode</span> multichannel analyzer</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Archer, Daniel E [Livermore, CA; Luke, S John [Pleasanton, CA; Mauger, G Joseph [Livermore, CA; Riot, Vincent J [Berkeley, CA; Knapp, David A [Livermore, CA</p> <p>2007-08-07</p> <p>A digital list <span class="hlt">mode</span> multichannel analyzer (MCA) built around a programmable FPGA device for onboard data analysis and on-the-fly modification of system detection/operating parameters, and capable of collecting and processing data in very small time bins (<1 millisecond) when used in histogramming <span class="hlt">mode</span>, or in list <span class="hlt">mode</span> as a list <span class="hlt">mode</span> MCA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JEOS....6E1009N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JEOS....6E1009N"><span>Partially coherent surface plasmon <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Niconoff, G. M.; Vara, P. M.; Munoz-Lopez, J.; Juárez-Morales, J. C.; Carbajal-Dominguez, A.</p> <p>2011-04-01</p> <p>Elementary long-range plasmon <span class="hlt">modes</span> are described assuming an exponential dependence of the refractive index in the neighbourhood of the interface dielectric-metal thin film. The study is performed using coupling <span class="hlt">mode</span> theory. The interference between two long-range plasmon <span class="hlt">modes</span> generated that way allows the synthesis of surface sinusoidal plasmon <span class="hlt">modes</span>, which can be considered as completely coherent generalized plasmon <span class="hlt">modes</span>. These sinusoidal plasmon <span class="hlt">modes</span> are used for the synthesis of new partially coherent surface plasmon <span class="hlt">modes</span>, which are obtained by means of an incoherent superposition of sinusoidal plasmon <span class="hlt">modes</span> where the period of each one is considered as a random variable. The kinds of surface <span class="hlt">modes</span> generated have an easily tuneable profile controlled by means of the probability density function associated to the period. We show that partially coherent plasmon <span class="hlt">modes</span> have the remarkable property to control the length of propagation which is a notable feature respect to the completely coherent surface plasmon <span class="hlt">mode</span>. The numerical simulation for sinusoidal, Bessel, Gaussian and Dark Hollow plasmon <span class="hlt">modes</span> are presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ThEng..63..222S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ThEng..63..222S"><span>Mathematical model for calculation of the heat-hydraulic <span class="hlt">modes</span> of heating points of heat-supplying systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shalaginova, Z. I.</p> <p>2016-03-01</p> <p>The mathematical model and calculation method of the thermal-hydraulic <span class="hlt">modes</span> of heat points, based on the theory of hydraulic circuits, being developed at the Melentiev Energy Systems Institute are presented. The redundant circuit of the heat point was developed, in which all possible connecting circuits (CC) of the heat engineering equipment and the places of possible installation of control valve were inserted. It allows simulating the operating <span class="hlt">modes</span> both at central heat points (CHP) and individual heat points (IHP). The configuration of the desired circuit is carried out automatically by removing the unnecessary links. The following circuits connecting the heating systems (HS) are considered: the dependent circuit (direct and through mixing elevator) and independent one (through the heater). The following connecting circuits of the load of hot <span class="hlt">water</span> supply (HWS) were considered: open CC (direct <span class="hlt">water</span> pumping from pipelines of heat networks) and a closed CC with connecting the HWS heaters on single-level (serial and parallel) and two-level (sequential and combined) circuits. The following connecting circuits of the ventilation systems (VS) were also considered: dependent circuit and independent one through a common heat exchanger with HS load. In the heat points, <span class="hlt">water</span> temperature regulators for the hot <span class="hlt">water</span> supply and ventilation and flow regulators for the heating system, as well as to the inlet as a whole, are possible. According to the accepted decomposition, the model of the heat point is an integral part of the overall heat-hydraulic model of the heat-supplying system having intermediate control stages (CHP and IHP), which allows to consider the operating <span class="hlt">modes</span> of the heat networks of different levels connected with each other through CHP as well as connected through IHP of consumers with various connecting circuits of local systems of heat consumption: heating, ventilation and hot <span class="hlt">water</span> supply. The model is implemented in the Angara data</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptLT.101..433E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptLT.101..433E"><span><span class="hlt">Mode</span> coupling in vortex beams</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eyyuboğlu, Halil T.</p> <p>2018-05-01</p> <p>We examine the <span class="hlt">mode</span> coupling in vortex beams. <span class="hlt">Mode</span> coupling also known as the crosstalk takes place due to turbulent characteristics of the atmospheric communication medium. This way, the transmitted intrinsic <span class="hlt">mode</span> of the vortex beam leaks power to other extrinsic <span class="hlt">modes</span>, thus preventing the correct detection of the transmitted symbol which is usually encoded into the <span class="hlt">mode</span> index or the orbital angular momentum state of the vortex beam. Here we investigate the normalized power <span class="hlt">mode</span> coupling ratios of several types of vortex beams, namely, Gaussian vortex beam, Bessel Gaussian beam, hypergeometric Gaussian beam and Laguerre Gaussian beam. It is found that smaller <span class="hlt">mode</span> numbers lead to less <span class="hlt">mode</span> coupling. The same is partially observed for increasing source sizes. Comparing the vortex beams amongst themselves, it is seen that hypergeometric Gaussian beam is the one retaining the most power in intrinsic <span class="hlt">mode</span> during propagation, but only at lowest <span class="hlt">mode</span> index of unity. At higher <span class="hlt">mode</span> indices this advantage passes over to the Gaussian vortex beam.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A43J..02S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A43J..02S"><span>Propagating annular <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sheshadri, A.; Plumb, R. A.</p> <p>2017-12-01</p> <p>The leading "annular <span class="hlt">mode</span>", defined as the dominant EOF of surface pressure or of zonal mean zonal wind variability, appears as a dipolar structure straddling the mean midlatitude jet and thus seems to describe north-south wobbling of the jet latitude. However, extratropical zonal wind anomalies frequently tend to migrate poleward. This behavior can be described by the first two EOFs, the first (AM1) being the dipolar structure, and the second (AM2) having a tripolar structure centered on the mean jet. Taken in isolation, AM1 thus describes a north-south wobbling of the jet position, while AM2 describes a strengthening and narrowing of the jet. However, despite the fact that they are spatially orthogonal, and their corresponding time series temporally orthogonal, AM1 and AM2 are not independent, but show significant lag-correlations which reveal the propagation. The EOFs are not <span class="hlt">modes</span> of the underlying dynamical system governing the zonal flow evolution. The true <span class="hlt">modes</span> can be estimated using principal oscillation pattern (POP) analysis. In the troposphere, the leading POPs manifest themselves as a pair of complex conjugate structures with conjugate eigenvalues thus, in reality, constituting a single, complex, <span class="hlt">mode</span> that describes propagating anomalies. Even though the principal components associated with the two leading EOFs decay at different rates, each decays faster than the true <span class="hlt">mode</span>. These facts have implications for eddy feedback and the susceptibility of the <span class="hlt">mode</span> to external perturbations. If one interprets the annular <span class="hlt">modes</span> as the <span class="hlt">modes</span> of the system, then simple theory predicts that the response to steady forcing will usually be dominated by AM1 (with the longest time scale). However, such arguments should really be applied to the true <span class="hlt">modes</span>. Experiments with a simplified GCM show that climate response to perturbations do not necessarily have AM1 structures. Implications of these results for stratosphere-troposphere interactions are explored. The POP</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H13I1526G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H13I1526G"><span>The evaluation of basin <span class="hlt">water</span> resources utilization efficiency based on Chaos projection <span class="hlt">mode</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guan, X.; Liang, S.; Meng, Y.; Wang, H.</p> <p>2017-12-01</p> <p>To promote the coordinated development of a healthy economy, society, and environment, and the sustainable development of <span class="hlt">water</span> resources comprehensive utilization efficiency (WRCUE), this study investigated appropriate indicators using the trapezoidal fuzzy number method, and constructed an evaluation index system for WRCUE. A WRCUE evaluation model is applied to the areas in the Yellow River Basin in China using a genetic projection pursuit method. The comprehensive evaluation index system of <span class="hlt">water</span> use efficiency includes 6 indicators: <span class="hlt">Water</span> consumption per unit industrial value added, <span class="hlt">water</span> consumption per unit GDP, eliminate the climate effect on agricultural <span class="hlt">water</span> use efficiency, irrigation <span class="hlt">water</span> consumption per unit area, domestic <span class="hlt">water</span> use per capita and industrial <span class="hlt">water</span> ratio. Then, multiple indexes in the index system are transformed to a comprehensive index by the combined model, which is used to represent the total <span class="hlt">water</span> resources utilization efficiency. Results show that the WRCUE in Yellow River basin and the provinces have a great distance. WRCUE is well developed in Shanxi, Shandong, and Henan provinces, moderately developed in Shaanxi, Inner Mongolia, and Sichuan provinces, and poorly developed in the Ningxia Autonomous Region, Gansu Province, and Qinghai Province. According to the capacities of provinces, related measures are proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=308207','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=308207"><span>New steady-state models for <span class="hlt">water</span>-limited cropping systems using saline irrigation <span class="hlt">waters</span>: Analytical solutions and applications</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Due to the diminishing availability of good quality <span class="hlt">water</span> for irrigation, it is increasingly important that irrigation and salinity management tools be able to target submaximal crop yields and support the use of marginal quality <span class="hlt">waters</span>. In this work, we present a steady-state irrigated systems <span class="hlt">mode</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22454441-investigation-metallic-photonic-crystal-high-power-microwave-mode-converter','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22454441-investigation-metallic-photonic-crystal-high-power-microwave-mode-converter"><span>Investigation of a metallic photonic crystal high power microwave <span class="hlt">mode</span> converter</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>Wang, Dong, E-mail: mr20001@sina.com; Qin, Fen; Xu, Sha</p> <p>2015-02-15</p> <p>It is demonstrated that an L band metallic photonic crystal TEM-TE{sub 11} <span class="hlt">mode</span> converter is suitable for narrow band high power microwave application. The proposed <span class="hlt">mode</span> converter is realized by partially filling metallic photonic crystals along azimuthal direction in a coaxial transmission line for phase-shifting. A three rows structure is designed and simulated by commercial software CST Microwave Studio. Simulation results show that its conversion efficiency is 99% at the center frequency 1.58 GHz. Over the frequency range of 1.56-1.625 GHz, the conversion efficiency exceeds 90 %, with a corresponding bandwidth of 4.1 %. This <span class="hlt">mode</span> converter has a gigawattmore » level power handling capability which is suitable for narrow band high power microwave application. Using magnetically insulated transmission line oscillator(MILO) as a high power microwave source, particle-in-cell simulation is carried out to test the performance of the <span class="hlt">mode</span> converter. The expected TE{sub 11} <span class="hlt">mode</span> microwave output is obtained and the MILO works well. <span class="hlt">Mode</span> conversion performance of the converter is tested by far-field measurement method. And the experimental result confirms the validity of our design. Then, high power microwave experiment is carried out on a Marx-driven Blumlein <span class="hlt">water</span> line pulsed power accelerator. Microwave frequency, radiated pattern and power are measured in the far-field region and the results agree well with simulation results. The experiment also reveals that no microwave breakdown or pulse shortening took place in the experimental setup.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22871399','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22871399"><span>Phylogeny and colonization history of Pringlea antiscorbutica (Brassicaceae), an emblematic endemic from the South Indian Ocean Province.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bartish, Igor V; Aïnouche, Abdelkader; Jia, Dongrui; Bergstrom, Dana; Chown, Steven L; Winkworth, Richard C; Hennion, Françoise</p> <p>2012-11-01</p> <p>The origins and evolution of <span class="hlt">sub-Antarctic</span> island floras are not well understood. In particular there is uncertainty about the ages of the contemporary floras and the ultimate origins of the lineages they contain. Pringlea R. Br. (Brassicaceae) is a monotypic genus endemic to four <span class="hlt">sub-Antarctic</span> island groups in the southern Indian Ocean. Here we used sequences from both the chloroplast and nuclear genomes to examine the phylogenetic position of this enigmatic genus. Our analyses confirm that Pringlea falls within the tribe Thelypodieae and provide a preliminary view of its relationships within the group. Divergence time estimates and ancestral area reconstructions imply Pringlea diverged from a South American ancestor ~5 Myr ago. It remains unclear whether the ancestor of Pringlea dispersed directly to the South Indian Ocean Province (SIOP) or used Antarctica as a stepping-stone; what is clear, however, is that following arrival in the SIOP several additional long-distance dispersal events must be inferred to explain the current distribution of this species. Our analyses also suggest that although Pringlea is likely to have inherited cold tolerance from its closest relatives, the distinctive morphology of this species evolved only after it split from the South American lineage. More generally, our results lend support to the hypothesis that angiosperms persisted on the <span class="hlt">sub-Antarctic</span> islands throughout the Pliocene and Pleistocene. Taken together with evidence from other <span class="hlt">sub-Antarctic</span> island plant groups, they suggest the extant flora of <span class="hlt">sub-Antarctic</span> is likely to have been assembled over a broad time period and from lineages with distinctive biogeographic histories. Copyright © 2012 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930068154&hterms=lime&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dlime','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930068154&hterms=lime&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dlime"><span>Subcritical crack growth in soda-lime glass in combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Singh, Dileep; Shetty, Dinesh K.</p> <p>1990-01-01</p> <p>Subcritical crack growth under mixed-<span class="hlt">mode</span> loading was studied in soda-lime glass. Pure <span class="hlt">mode</span> I, combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II, and pure <span class="hlt">mode</span> II loadings were achieved in precracked disk specimens by loading in diametral compression at selected angles with respect to the symmetric radial crack. Crack growth was monitored by measuring the resistance changes in a microcircuit grid consisting of parallel, electrically conducting grid lines deposited on the surface of the disk specimens by photolithography. Subcritical crack growth rates in pure <span class="hlt">mode</span> I, pure <span class="hlt">mode</span> II, and combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading could be described by an exponential relationship between crack growth rate and an effective crack driving force derived from a <span class="hlt">mode</span> I-<span class="hlt">mode</span> II fracture toughness envelope. The effective crack driving force was based on an empirical representation of the noncoplanar strain energy release rate. Stress intensities for kinked cracks were assessed using the method of caustics and an initial decrease and a subsequent increase in the subcritical crack growth rates of kinked cracks were shown to correlate with the variations of the <span class="hlt">mode</span> I and the <span class="hlt">mode</span> II stress intensities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS.956a2008K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS.956a2008K"><span>Sensitivity optimization in whispering gallery <span class="hlt">mode</span> optical cylindrical biosensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Khozeymeh, F.; Razaghi, M.</p> <p>2018-01-01</p> <p>Whispering-gallery-<span class="hlt">mode</span> resonances propagated in cylindrical resonators have two angular and radial orders of l and i. In this work, the higher radial order whispering-gallery-<span class="hlt">mode</span> resonances, (i = 1 - 4), at a fixed l are examined. The sensitivity of theses resonances is analysed as a function of the structural parameters of the cylindrical resonator like different radii and refractive index of composed material of the resonator. A practical application where cylindrical resonators are used for the measurement of glucose concentration in <span class="hlt">water</span> is presented as a biosensor demonstrator. We calculate the wavelength shifts of the WG1-4, in several glucose/<span class="hlt">water</span> solutions, with concentrations spanning from 0.0% to 9.0.% (weight/weight). Improved sensitivity can be achieved using multi-WGM cylindrical resonators with radius of R = 100 μm and resonator composed material of MgF 2 with refractive index of nc = 1.38. Also the effect of polarization on sensitivity is considered for all four WGMs. The best sensitivity of 83.07 nm/RIU for the fourth WGM with transverse magnetic polarization, is reported. These results propose optimized parameters aimed to fast designing of cylindrical resonators as optical biosensors, where both the sensitivity and the geometries can be optimized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21304696-vibrational-excitation-water-electron-impact','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21304696-vibrational-excitation-water-electron-impact"><span>Vibrational excitation of <span class="hlt">water</span> by electron impact</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>Khakoo, M. A.; Winstead, C.; McKoy, V.</p> <p>2009-05-15</p> <p>Experimental and calculated differential cross sections (DCSs) for electron-impact excitation of the (010) bending <span class="hlt">mode</span> and unresolved (100) symmetric and (001) antisymmetric stretching <span class="hlt">modes</span> of <span class="hlt">water</span> are presented. Measurements are reported at incident energies of 1-100 eV and scattering angles of 10 deg. - 130 deg. and are normalized to the elastic-scattering DCSs for <span class="hlt">water</span> determined earlier by our group. The calculated cross sections are obtained in the adiabatic approximation from fixed-nuclei, electronically elastic scattering calculations using the Schwinger multichannel method. The present results are compared to available experimental and theoretical data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25399183','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25399183"><span>Simulations of <span class="hlt">water</span> transport through carbon nanotubes: how different <span class="hlt">water</span> models influence the conduction rate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, L; Patey, G N</p> <p>2014-11-14</p> <p>The conduction rate of <span class="hlt">water</span> through (8,8) and (9,9) carbon nanotubes at 300 K and a pressure difference of 220 MPa is investigated using molecular dynamics simulations. The TIP3P, SPC/E, and TIP4P/2005 <span class="hlt">water</span> models are considered. The pressure-driven flow rate is found to be strongly model dependent for both nanotubes. The fastest model (TIP3P) has a flow rate that is approximately five times faster than the slowest (TIP4P/2005). It is shown that the flow rate is significantly influenced by the structure taken on by the <span class="hlt">water</span> molecules confined in the nanotube channels. The slower models, TIP4P/2005 and SPC/E, tend to favor stacked ring arrangements, with the molecules of a ring moving together through the nanotube, in what we term a "cluster-by-cluster" conduction <span class="hlt">mode</span>. Confined TIP3P <span class="hlt">water</span> has a much weaker tendency to form ring structures, and those that do form are fragile and break apart under flow conditions. This creates a much faster "diffusive" conduction <span class="hlt">mode</span> where the <span class="hlt">water</span> molecules mainly move through the tube as individual particles, rather than as components of a larger cluster. Our results demonstrate that <span class="hlt">water</span> models developed to describe the properties of bulk <span class="hlt">water</span> can behave very differently in confined situations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1176850-tof-sims-depth-profiling-insulating-samples-interlaced-mode-non-interlaced-mode','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1176850-tof-sims-depth-profiling-insulating-samples-interlaced-mode-non-interlaced-mode"><span>ToF-SIMS Depth Profiling Of Insulating Samples, Interlaced <span class="hlt">Mode</span> Or Non-interlaced <span class="hlt">Mode</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>Wang, Zhaoying; Jin, Ke; Zhang, Yanwen</p> <p>2014-11-01</p> <p>Dual beam depth profiling strategy has been widely adopted in ToF-SIMS depth profiling, in which two basic operation <span class="hlt">modes</span>, interlaced <span class="hlt">mode</span> and non-interlaced <span class="hlt">mode</span>, are commonly used. Generally, interlaced <span class="hlt">mode</span> is recommended for conductive or semi-conductive samples, whereas non-interlaced <span class="hlt">mode</span> is recommended for insulating samples, where charge compensation can be an issue. Recent publications, however, show that the interlaced <span class="hlt">mode</span> can be used effectively for glass depth profiling, despite the fact that glass is an insulator. In this study, we provide a simple guide for choosing between interlaced <span class="hlt">mode</span> and non-interlaced <span class="hlt">mode</span> for insulator depth profiling. Two representative cases aremore » presented: (1) depth profiling of a leached glass sample, and (2) depth profiling of a single crystal MgO sample. In brief, the interlaced <span class="hlt">mode</span> should be attempted first, because (1) it may provide reasonable-quality data, and (2) it is time-saving for most cases, and (3) it introduces low H/C/O background. If data quality is the top priority and measurement time is flexible, non-interlaced <span class="hlt">mode</span> is recommended because interlaced <span class="hlt">mode</span> may suffer from low signal intensity and poor mass resolution. A big challenge is tracking trace H/C/O in a highly insulating sample (e.g., MgO), because non-interlaced <span class="hlt">mode</span> may introduce strong H/C/O background but interlaced <span class="hlt">mode</span> may suffer from low signal intensity. Meanwhile, a C or Au coating is found to be very effective to improve the signal intensity. Surprisingly, the best analyzing location is not on the C or Au coating, but at the edge (outside) of the coating.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28789230','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28789230"><span><span class="hlt">Mode</span> conversion efficiency to Laguerre-Gaussian OAM <span class="hlt">modes</span> using spiral phase optics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Longman, Andrew; Fedosejevs, Robert</p> <p>2017-07-24</p> <p>An analytical model for the conversion efficiency from a TEM 00 <span class="hlt">mode</span> to an arbitrary Laguerre-Gaussian (LG) <span class="hlt">mode</span> with null radial index spiral phase optics is presented. We extend this model to include the effects of stepped spiral phase optics, spiral phase optics of non-integer topological charge, and the reduction in conversion efficiency due to broad laser bandwidth. We find that through optimization, an optimal beam waist ratio of the input and output <span class="hlt">modes</span> exists and is dependent upon the output azimuthal <span class="hlt">mode</span> number.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3097177','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3097177"><span>Out of Their Depth? Isolated Deep Populations of the Cosmopolitan Coral Desmophyllum dianthus May Be Highly Vulnerable to Environmental Change</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Miller, Karen J.; Rowden, Ashley A.; Williams, Alan; Häussermann, Vreni</p> <p>2011-01-01</p> <p>Deep sea scleractinian corals will be particularly vulnerable to the effects of climate change, facing loss of up to 70% of their habitat as the Aragonite Saturation Horizon (below which corals are unable to form calcium carbonate skeletons) rises. Persistence of deep sea scleractinian corals will therefore rely on the ability of larvae to disperse to, and colonise, suitable shallow-<span class="hlt">water</span> habitat. We used DNA sequence data of the internal transcribed spacer (ITS), the mitochondrial ribosomal subunit (16S) and mitochondrial control region (MtC) to determine levels of gene flow both within and among populations of the deep sea coral Desmophyllum dianthus in SE Australia, New Zealand and Chile to assess the ability of corals to disperse into different regions and habitats. We found significant genetic subdivision among the three widely separated geographic regions consistent with isolation and limited contemporary gene flow. Furthermore, corals from different depth strata (shallow <600 m, mid 1000–1500 m, deep >1500 m) even on the same or nearby seamounts were strongly differentiated, indicating limited vertical larval dispersal. Genetic differentiation with depth is consistent with the stratification of the <span class="hlt">Subantarctic</span> <span class="hlt">Mode</span> <span class="hlt">Water</span>, Antarctic Intermediate <span class="hlt">Water</span>, the Circumpolar Deep and North Pacific Deep <span class="hlt">Waters</span> in the Southern Ocean, and we propose that coral larvae will be retained within, and rarely migrate among, these <span class="hlt">water</span> masses. The apparent absence of vertical larval dispersal suggests deep populations of D. dianthus are unlikely to colonise shallow <span class="hlt">water</span> as the aragonite saturation horizon rises and deep <span class="hlt">waters</span> become uninhabitable. Similarly, assumptions that deep populations will act as refuges for shallow populations that are impacted by activities such as fishing or mining are also unlikely to hold true. Clearly future environmental management strategies must consider both regional and depth-related isolation of deep-sea coral populations. PMID</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JHyd..543..386S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JHyd..543..386S"><span>An ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources in the northern Tianshan Mountains, China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shang, Haimin; Wang, Wenke; Dai, Zhenxue; Duan, Lei; Zhao, Yaqian; Zhang, Jing</p> <p>2016-12-01</p> <p>In recent years, ecological degradation caused by irrational groundwater exploitation has been of growing concern in arid and semiarid regions. To address the groundwater-ecological issues, this paper proposes a groundwater-resource exploitation <span class="hlt">mode</span> to evaluate the tradeoff between groundwater development and ecological environment in the northern Tianshan Mountains, northwest China's Xinjiang Uygur Autonomous Region. Field surveys and remote sensing studies were conducted to analyze the relation between the distribution of hydrological conditions and the occurrence of ecological types. The results show that there is a good correlation between groundwater depth and the supergene ecological type. Numerical simulations and ecological assessment models were applied to develop an ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources. The <span class="hlt">mode</span> allows the groundwater levels in different zones to be regulated by optimizing groundwater exploitation <span class="hlt">modes</span>. The prediction results show that the supergene ecological quality will be better in 2020 and even more groundwater can be exploited in this <span class="hlt">mode</span>. This study provides guidance for regional groundwater management, especially in regions with an obvious <span class="hlt">water</span> scarcity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19910050203&hterms=lime&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlime','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19910050203&hterms=lime&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dlime"><span>Slow crack growth in glass in combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shetty, D. K.; Rosenfield, A. R.</p> <p>1991-01-01</p> <p>Slow crack growth in soda-lime glass under combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading was investigated in precracked disk specimens in which pure <span class="hlt">mode</span> I, pure <span class="hlt">mode</span> II, and various combinations of <span class="hlt">mode</span> I and <span class="hlt">mode</span> II were achieved by loading in diametral compression at selected angles with respect to symmetric radial cracks. It is shown that slow crack growth under these conditions can be described by a simple exponential relationship with elastic strain energy release rate as the effective crack-driving force parameter. It is possible to interpret this equation in terms of theoretical models that treat subcritical crack growth as a thermally activated bond-rupture process with an activation energy dependent on the environment, and the elastic energy release rate as the crack-driving force parameter.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFD.R2004V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFD.R2004V"><span>Sloshing motion dynamics of a free surface in the draft tube cone of a Francis turbine operating in synchronous condenser <span class="hlt">mode</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vagnoni, Elena; Andolfatto, Loïc; Favrel, Arthur; Avellan, François</p> <p>2016-11-01</p> <p>The penetration of the electrical grid by intermittent renewable energy sources induces grid fluctuations which must be compensated in order to guarantee the stability of the grid. Hydropower plants can supply reactive power to ensure the grid stabilization by operating in condenser <span class="hlt">mode</span>. In this operating <span class="hlt">mode</span>, the turbine operates with the tail <span class="hlt">water</span> depressed to let the runner spin in air to reduce the power consumption. Pressurized air is injected in the draft tube cone to maintain the <span class="hlt">water</span> level below the runner and this induces air-<span class="hlt">water</span> interaction phenomena which cause important power losses. Flow visualization and pressure fluctuation measurements are performed in a reduced scale physical model of a Francis turbine operating in condenser <span class="hlt">mode</span> to investigate the dynamics of the air-<span class="hlt">water</span> interaction in the draft tube cone which causes the sloshing motion of the free surface. An image post-processing method is developed, enabling a quantitative description of the sloshing motion. The latter depends on the Froude number. By increasing the value of the Froude number, the amplitude of the sloshing motion decreases, as well as the amplitude of the pressure fluctuations. The frequency of the sloshing motion corresponds to the first natural frequency of the <span class="hlt">water</span> volume.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10132E..52L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10132E..52L"><span>Comparison of detectability in step-and-shoot <span class="hlt">mode</span> and continuous <span class="hlt">mode</span> digital tomosynthesis systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Changwoo; Han, Minah; Baek, Jongduk</p> <p>2017-03-01</p> <p>Digital tomosynthesis system has been widely used in chest, dental, and breast imaging. Since the digital tomosynthesis system provides volumetric images from multiple projection data, structural noise inherent in X-ray radiograph can be reduced, and thus signal detection performance is improved. Currently, tomosynthesis system uses two data acquisition <span class="hlt">modes</span>: step-and-shoot <span class="hlt">mode</span> and continuous <span class="hlt">mode</span>. Several studies have been conducted to compare the system performance of two acquisition <span class="hlt">modes</span> with respect to spatial resolution and contrast. In this work, we focus on signal detectability in step-and-shoot <span class="hlt">mode</span> and continuous <span class="hlt">mode</span>. For evaluation, uniform background is considered, and eight spherical objects with diameters of 0.5, 0.8, 1, 2, 3, 5, 8, 10 mm are used as signals. Projection data with and without spherical objects are acquired in step-and-shoot <span class="hlt">mode</span> and continuous <span class="hlt">mode</span>, respectively, and quantum noise are added. Then, noisy projection data are reconstructed by FDK algorithm. To compare the detection performance of two acquisition <span class="hlt">modes</span>, we calculate task signal-to-noise ratio (SNR) of channelized Hotelling observer with Laguerre-Gauss channels for each spherical object. While the task-SNR values of two acquisition <span class="hlt">modes</span> are similar for spherical objects larger than 1 mm diameter, step-and-shoot <span class="hlt">mode</span> yields higher detectability for small signal sizes. The main reason of this behavior is that small signal is more affected by X-ray tube motion blur than large signal. Our results indicate that it is beneficial to use step-and-shoot data acquisition <span class="hlt">mode</span> to improve the detectability of small signals (i.e., less than 1 mm diameter) in digital tomosynthesis systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25074819','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25074819"><span><span class="hlt">Mode</span> of action of dopamine in inducing hyperglycemia in the fresh <span class="hlt">water</span> edible crab, Oziothelphusa senex senex.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Swetha, Ch; Sainath, S B; Reddy, P Sreenivasula</p> <p>2014-11-01</p> <p>The objective of this study was to investigate the <span class="hlt">mode</span> of action of dopamine in regulating hemolymph sugar level in the fresh <span class="hlt">water</span> edible crab, Oziothelphusa senex senex. Injection of dopamine produced hyperglycemia in a dose-dependent manner in intact crabs but not in eyestalkless crabs. Administration of dopamine resulted in a significant decrease in total carbohydrates and glycogen levels with a significant increase in glycogen phosphorylase activity levels in hepatopancreas and muscle of intact crabs, indicating dopamine-induced glycogenolysis resulting in hyperglycemia. Bilateral eyestalk ablation resulted in significant increase in the total carbohydrates and glycogen levels with a significant decrease in the activity levels of phosphorylase in the hepatopancreas and muscle of the crabs. Eyestalk ablation resulted in significant decrease in hemolymph hyperglycemic hormone levels. The levels of hyperglycemic hormone in the hemolymph of dopamine injected crabs were significantly higher than in control crabs. However, no significant changes in the levels of hemolymph hyperglycemic hormone and sugar and tissue carbohydrate and phosphorylase activity were observed in dopamine injected eyestalk ablated crabs when compared with eyestalk ablated crabs. These results support an earlier hypothesis in crustaceans that dopamine acts as a neurotransmitter and induces hyperglycemia by triggering the release of hyperglycemic hormone in the crab, O. senex senex. © 2014 Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992ApPhL..60.2735N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992ApPhL..60.2735N"><span>Observation of a new surface <span class="hlt">mode</span> on a fluid-saturated permeable solid</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nagy, Peter B.</p> <p>1992-06-01</p> <p>Almost ten years ago, S. Feng and D. L. Johnson predicted the presence of a new surface <span class="hlt">mode</span> on a fluid/fluid-saturated porous solid interface with closed surface pores [J. Acoust. Soc. Am. 74, 906 (1983)]. We found that, due to surface tension, practically closed-pore boundary conditions can prevail at an interface between a nonwetting fluid (e.g., air) and a porous solid saturated with a wetting fluid (e.g., <span class="hlt">water</span> or alcohol). Surface wave velocity and attenuation measurements were made on alcohol-saturated porous sintered glass at 100 kHz. The experimental results show clear evidence of the new ``slow'' surface <span class="hlt">mode</span> predicted by Feng and Johnson.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22695223','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22695223"><span>Processing <span class="hlt">mode</span> during repetitive thinking in socially anxious individuals: evidence for a maladaptive experiential <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wong, Quincy J J; Moulds, Michelle L</p> <p>2012-12-01</p> <p>Evidence from the depression literature suggests that an analytical processing <span class="hlt">mode</span> adopted during repetitive thinking leads to maladaptive outcomes relative to an experiential processing <span class="hlt">mode</span>. To date, in socially anxious individuals, the impact of processing <span class="hlt">mode</span> during repetitive thinking related to an actual social-evaluative situation has not been investigated. We thus tested whether an analytical processing <span class="hlt">mode</span> would be maladaptive relative to an experiential processing <span class="hlt">mode</span> during anticipatory processing and post-event rumination. High and low socially anxious participants were induced to engage in either an analytical or experiential processing <span class="hlt">mode</span> during: (a) anticipatory processing before performing a speech (Experiment 1; N = 94), or (b) post-event rumination after performing a speech (Experiment 2; N = 74). Mood, cognition, and behavioural measures were employed to examine the effects of processing <span class="hlt">mode</span>. For high socially anxious participants, the <span class="hlt">modes</span> had a similar effect on self-reported anxiety during both anticipatory processing and post-event rumination. Unexpectedly, relative to the analytical <span class="hlt">mode</span>, the experiential <span class="hlt">mode</span> led to stronger high standard and conditional beliefs during anticipatory processing, and stronger unconditional beliefs during post-event rumination. These experiments are the first to investigate processing <span class="hlt">mode</span> during anticipatory processing and post-event rumination. Hence, these results are novel and will need to be replicated. These findings suggest that an experiential processing <span class="hlt">mode</span> is maladaptive relative to an analytical processing <span class="hlt">mode</span> during repetitive thinking characteristic of socially anxious individuals. Copyright © 2012 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015MSSP...62..490O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015MSSP...62..490O"><span>Pad-<span class="hlt">mode</span>-induced instantaneous <span class="hlt">mode</span> instability for simple models of brake systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Oberst, S.; Lai, J. C. S.</p> <p>2015-10-01</p> <p>Automotive disc brake squeal is fugitive, transient and remains difficult to predict. In particular, instantaneous <span class="hlt">mode</span> squeal observed experimentally does not seem to be associated with <span class="hlt">mode</span> coupling and its mechanism is not clear. The effects of contact pressures, friction coefficients as well as material properties (pressure and temperature dependency and anisotropy) for brake squeal propensity have not been systematically explored. By analysing a finite element model of an isotropic pad sliding on a plate similar to that of a previously reported experimental study, pad <span class="hlt">modes</span> have been identified and found to be stable using conventional complex eigenvalue analysis. However, by subjecting the model to contact pressure harmonic excitation for a range of pressures and friction coefficients, a forced response analysis reveals that the dissipated energy for pad <span class="hlt">modes</span> is negative and becomes more negative with increasing contact pressures and friction coefficients, indicating the potential for instabilities. The frequency of the pad <span class="hlt">mode</span> in the sliding direction is within the range of squeal frequencies observed experimentally. Nonlinear time series analysis of the vibration velocity also confirms the evolution of instabilities induced by pad <span class="hlt">modes</span> as the friction coefficient increases. By extending this analysis to a more realistic but simple brake model in the form of a pad-on-disc system, in-plane pad-<span class="hlt">modes</span>, which a complex eigenvalue analysis predicts to be stable, have also been identified by negative dissipated energy for both isotropic and anisotropic pad material properties. The influence of contact pressures on potential instabilities has been found to be more dominant than changes in material properties owing to changes in pressure or temperature. Results here suggest that instantaneous <span class="hlt">mode</span> squeal is likely caused by in-plane pad-<span class="hlt">mode</span> instabilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOS.A34A2617Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOS.A34A2617Z"><span>Numerical Investigations of Subduction of Eighteen Degree <span class="hlt">Water</span> in the Subtropical Northwest Atlantic Ocean</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhai, P.; He, R.</p> <p>2016-02-01</p> <p><span class="hlt">Mode</span> <span class="hlt">waters</span> are upper-ocean <span class="hlt">water</span> masses with nearly uniform <span class="hlt">water</span> properties over a thickness of a few hundred meters. Subduction of <span class="hlt">mode</span> <span class="hlt">waters</span> plays an important role in changing atmospheric and oceanic long-term variability because they store "memory" of wintertime air-sea interaction. In this study, we investigated dynamic processes associated with subduction of the Eighteen Degree <span class="hlt">Water</span> (EDW, the principal <span class="hlt">mode</span> <span class="hlt">water</span>) in the subtropical Northwest Atlantic during January to June 2007. Numerical simulations of the temporal and spatial evolutions of EDW were performed using both uncoupled (ocean only) and air-sea coupled configurations and results were contrasted. We find the coupled simulation produced deeper mixed layer depth, stronger eddy kinetic energy, and larger subduction areas than their counterparts in the uncoupled ocean simulation. In both configurations, mesoscale eddies enhance the total subduction and eddy-induced subduction has the same order as the mean component. Resolving strong air-sea coupling and mesoscale eddies is therefore important for understanding EDW dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960047103','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960047103"><span>The Integrated <span class="hlt">Mode</span> Management Interface</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hutchins, Edwin</p> <p>1996-01-01</p> <p><span class="hlt">Mode</span> management is the processes of understanding the character and consequences of autoflight <span class="hlt">modes</span>, planning and selecting the engagement, disengagement and transitions between <span class="hlt">modes</span>, and anticipating automatic <span class="hlt">mode</span> transitions made by the autoflight system itself. The state of the art is represented by the latest designs produced by each of the major airframe manufacturers, the Boeing 747-400, the Boeing 777, the McDonnell Douglas MD-11, and the Airbus A320/A340 family of airplanes. In these airplanes autoflight <span class="hlt">modes</span> are selected by manipulating switches on the control panel. The state of the autoflight system is displayed on the flight <span class="hlt">mode</span> annunciators. The integrated <span class="hlt">mode</span> management interface (IMMI) is a graphical interface to autoflight <span class="hlt">mode</span> management systems for aircraft equipped with flight management computer systems (FMCS). The interface consists of a vertical <span class="hlt">mode</span> manager and a lateral <span class="hlt">mode</span> manager. Autoflight <span class="hlt">modes</span> are depicted by icons on a graphical display. <span class="hlt">Mode</span> selection is accomplished by touching (or mousing) the appropriate icon. The IMMI provides flight crews with an integrated interface to autoflight systems for aircraft equipped with flight management computer systems (FMCS). The current version is modeled on the Boeing glass-cockpit airplanes (747-400, 757/767). It runs on the SGI Indigo workstation. A working prototype of this graphics-based crew interface to the autoflight <span class="hlt">mode</span> management tasks of glass cockpit airplanes has been installed in the Advanced Concepts Flight Simulator of the CSSRF of NASA Ames Research Center. This IMMI replaces the devices in FMCS equipped airplanes currently known as <span class="hlt">mode</span> control panel (Boeing), flight guidance control panel (McDonnell Douglas), and flight control unit (Airbus). It also augments the functions of the flight <span class="hlt">mode</span> annunciators. All glass cockpit airplanes are sufficiently similar that the IMMI could be tailored to the <span class="hlt">mode</span> management system of any modern cockpit. The IMMI does not replace the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JChPh.137h4114Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JChPh.137h4114Z"><span>Relating normal vibrational <span class="hlt">modes</span> to local vibrational <span class="hlt">modes</span> with the help of an adiabatic connection scheme</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zou, Wenli; Kalescky, Robert; Kraka, Elfi; Cremer, Dieter</p> <p>2012-08-01</p> <p>Information on the electronic structure of a molecule and its chemical bonds is encoded in the molecular normal vibrational <span class="hlt">modes</span>. However, normal vibrational <span class="hlt">modes</span> result from a coupling of local vibrational <span class="hlt">modes</span>, which means that only the latter can provide detailed insight into bonding and other structural features. In this work, it is proven that the adiabatic internal coordinate vibrational <span class="hlt">modes</span> of Konkoli and Cremer [Int. J. Quantum Chem. 67, 29 (1998)], 10.1002/(SICI)1097-461X(1998)67:1<29::AID-QUA3>3.0.CO;2-0 represent a unique set of local <span class="hlt">modes</span> that is directly related to the normal vibrational <span class="hlt">modes</span>. The missing link between these two sets of <span class="hlt">modes</span> are the compliance constants of Decius, which turn out to be the reciprocals of the local <span class="hlt">mode</span> force constants of Konkoli and Cremer. Using the compliance constants matrix, the local <span class="hlt">mode</span> frequencies of any molecule can be converted into its normal <span class="hlt">mode</span> frequencies with the help of an adiabatic connection scheme that defines the coupling of the local <span class="hlt">modes</span> in terms of coupling frequencies and reveals how avoided crossings between the local <span class="hlt">modes</span> lead to changes in the character of the normal <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptCo.383...42L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptCo.383...42L"><span>Coupling analysis of non-circular-symmetric <span class="hlt">modes</span> and design of orientation-insensitive few-<span class="hlt">mode</span> fiber couplers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Jiaxiong; Du, Jiangbing; Ma, Lin; Li, Ming-Jun; Jiang, Shoulin; Xu, Xiao; He, Zuyuan</p> <p>2017-01-01</p> <p>We study the coupling between two identical weakly-coupled few-<span class="hlt">mode</span> fibers based on coupled-<span class="hlt">mode</span> theory. The coupling behavior of non-circular-symmetric <span class="hlt">modes</span>, such as LP11 and LP21, is investigated analytically and numerically. By carefully choosing the fiber core separation and coupler length, we can design orientation-insensitive fiber couplers for non-circular-symmetric <span class="hlt">modes</span> at arbitrary coupling ratios. Based on the design method, we propose an orientation-insensitive two-<span class="hlt">mode</span> fiber coupler at 850 nm working as a <span class="hlt">mode</span> multiplexer/demultiplexer for two-<span class="hlt">mode</span> transmission using standard single-<span class="hlt">mode</span> fiber. Within the band from 845 to 855 nm, the insertion losses of LP01 and LP11 <span class="hlt">modes</span> are less than 0.03 dB and 0.24 dB, respectively. When the two-<span class="hlt">mode</span> fiber coupler is used as <span class="hlt">mode</span> demultiplexer, the LP01/LP11 and LP11/LP01 extinction ratios in the separated branches are respectively above 12.6 dB and 21.2 dB. Our design method can be extended to two-<span class="hlt">mode</span> communication or sensing systems at other wavelengths.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26291340','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26291340"><span>Contact Freezing of <span class="hlt">Water</span> by Salts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Niehaus, Joseph; Cantrell, Will</p> <p>2015-09-03</p> <p><span class="hlt">Water</span> is unlikely to crystallize homogeneously at temperatures greater than -34 °C. Freezing at higher temperatures is heterogeneous-catalyzed by the presence of a second substance. If that substance is at an air-<span class="hlt">water</span> interface, then the <span class="hlt">mode</span> is called contact freezing, and it typically will trigger nucleation at a higher temperature than if the substance were wholly immersed within the liquid. We find that the impact of salt particles initiates freezing in experiments using <span class="hlt">water</span> droplets at supercoolings of 9 to 16 °C. These results show that contact freezing nuclei need not be effective as immersion <span class="hlt">mode</span> nuclei. We discuss our results in the context of proposed mechanisms of contact freezing. Finally, we use the time scales for diffusion of heat and of ions and the propagation of a sound wave through the droplet to estimate that contact freezing occurs within 10 ns of impact.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10620E..1MZ','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10620E..1MZ"><span>Moving target detection in flash <span class="hlt">mode</span> against stroboscopic <span class="hlt">mode</span> by active range-gated laser imaging</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Xuanyu; Wang, Xinwei; Sun, Liang; Fan, Songtao; Lei, Pingshun; Zhou, Yan; Liu, Yuliang</p> <p>2018-01-01</p> <p>Moving target detection is important for the application of target tracking and remote surveillance in active range-gated laser imaging. This technique has two operation <span class="hlt">modes</span> based on the difference of the number of pulses per frame: stroboscopic <span class="hlt">mode</span> with the accumulation of multiple laser pulses per frame and flash <span class="hlt">mode</span> with a single shot of laser pulse per frame. In this paper, we have established a range-gated laser imaging system. In the system, two types of lasers with different frequency were chosen for the two <span class="hlt">modes</span>. Electric fan and horizontal sliding track were selected as the moving targets to compare the moving blurring between two <span class="hlt">modes</span>. Consequently, the system working in flash <span class="hlt">mode</span> shows more excellent performance in motion blurring against stroboscopic <span class="hlt">mode</span>. Furthermore, based on experiments and theoretical analysis, we presented the higher signal-to-noise ratio of image acquired by stroboscopic <span class="hlt">mode</span> than flash <span class="hlt">mode</span> in indoor and underwater environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A41F3114A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A41F3114A"><span>The Aerosol Coarse <span class="hlt">Mode</span> Initiative</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnott, W. P.; Adhikari, N.; Air, D.; Kassianov, E.; Barnard, J.</p> <p>2014-12-01</p> <p>Many areas of the world show an aerosol volume distribution with a significant coarse <span class="hlt">mode</span> and sometimes a dominant coarse <span class="hlt">mode</span>. The large coarse <span class="hlt">mode</span> is usually due to dust, but sea salt aerosol can also play an important role. However, in many field campaigns, the coarse <span class="hlt">mode</span> tends to be ignored, because it is difficult to measure. This lack of measurements leads directly to a concomitant "lack of analysis" of this <span class="hlt">mode</span>. Because, coarse <span class="hlt">mode</span> aerosols can have significant effects on radiative forcing, both in the shortwave and longwave spectrum, the coarse <span class="hlt">mode</span> -- and these forcings -- should be accounted for in atmospheric models. Forcings based only on fine <span class="hlt">mode</span> aerosols have the potential to be misleading. In this paper we describe examples of large coarse <span class="hlt">modes</span> that occur in areas of large aerosol loading (Mexico City, Barnard et al., 2010) as well as small loadings (Sacramento, CA; Kassianov et al., 2012; and Reno, NV). We then demonstrate that: (1) the coarse <span class="hlt">mode</span> can contribute significantly to radiative forcing, relative to the fine <span class="hlt">mode</span>, and (2) neglecting the coarse <span class="hlt">mode</span> may result in poor comparisons between measurements and models. Next we describe -- in general terms -- the limitations of instrumentation to measure the coarse <span class="hlt">mode</span>. Finally, we suggest a new initiative aimed at examining coarse <span class="hlt">mode</span> aerosol generation mechanisms; transport and deposition; chemical composition; visible and thermal IR refractive indices; morphology; microphysical behavior when deposited on snow and ice; and specific instrumentation needs. Barnard, J. C., J. D. Fast, G. Paredes-Miranda, W. P. Arnott, and A. Laskin, 2010: Technical Note: Evaluation of the WRF-Chem "Aerosol Chemical to Aerosol Optical Properties" Module using data from the MILAGRO campaign, Atmospheric Chemistry and Physics, 10, 7325-7340. Kassianov, E. I., M. S. Pekour, and J. C. Barnard, 2012: Aerosols in Central California: Unexpectedly large contribution of coarse <span class="hlt">mode</span> to aerosol radiative forcing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900055334&hterms=Boussinesq+system&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBoussinesq%2Bsystem','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900055334&hterms=Boussinesq+system&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBoussinesq%2Bsystem"><span>Recurrence in truncated Boussinesq models for nonlinear waves in shallow <span class="hlt">water</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Elgar, Steve; Freilich, M. H.; Guza, R. T.</p> <p>1990-01-01</p> <p>The rapid spatial recurrence of weakly nonlinear and weakly dispersive progressive shallow-<span class="hlt">water</span> waves is examined using a numerical integration technique on the discretized and truncated form of the Boussinesq equations. This study primarily examines recurrence in wave fields with Ursell number O(1) and characterizes the sensitivity of recurrence to initial spectral shape and number of allowed frequency <span class="hlt">modes</span>. It is shown that the rapid spatial recurrence is not an inherent property of the considered Boussinesq systems for evolution distances of 10-50 wavelengths. The main result of the study is that highly truncated Boussinesq models of resonant shallow-<span class="hlt">water</span> ocean surface gravity waves predict rapid multiple recurrence cycles, but that this is an artifact dependent on the number of allowed <span class="hlt">modes</span>. For initial conditions consisting of essentially all energy concentrated in a single <span class="hlt">mode</span>, damping of the recurrence cycles increases as the number of low-power background <span class="hlt">modes</span> increases. When more than 32 <span class="hlt">modes</span> are allowed, the recurrence behavior is relatively insensitive to the number of allowed <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.813a2042P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.813a2042P"><span>Dynamics of large-diameter <span class="hlt">water</span> pipes in hydroelectric power plants</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pavić, G.; Chevillotte, F.; Heraud, J.</p> <p>2017-04-01</p> <p>An outline is made of physical behaviour of <span class="hlt">water</span> - filled large pipes. The fluid-wall coupling, the key factor governing the pipe dynamics, is discussed in some detail. Different circumferential pipe <span class="hlt">modes</span> and the associated cut-on frequencies are addressed from a theoretical as well as practical point of view. Major attention is paid to the breathing <span class="hlt">mode</span> in view of its importance regarding main dynamic phenomena, such as <span class="hlt">water</span> hammer. Selected measurement results done at EDF are presented to demonstrate how an external, non-intrusive sensor can detect pressure pulsations of the breathing <span class="hlt">mode</span> in a pressure pipe. Differences in the pressure measurement using intrusive and non-intrusive sensors reveal the full complexity of large-diameter pipe dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018HydJ..tmp...38T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018HydJ..tmp...38T"><span><span class="hlt">Water</span> quality responses to the interaction between surface <span class="hlt">water</span> and groundwater along the Songhua River, NE China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Teng, Yanguo; Hu, Bin; Zheng, Jieqiong; Wang, Jinsheng; Zhai, Yuanzheng; Zhu, Chen</p> <p>2018-03-01</p> <p>Investigation of surface <span class="hlt">water</span> and groundwater interaction (SW-GW interaction) provides basic information for regional <span class="hlt">water</span>-resource protection, management, and development. In this survey of a 10-km-wide area along both sides of the Songhua River, northeast China, the hydrogeochemical responses to different SW-GW interactions were studied. Three types of SW-GW interactions were identified—"recharge", "discharge", and "flow-through"—according to the hydraulic connection between the surface <span class="hlt">water</span> and groundwater. The single factor index, principal component analysis, and hierarchical cluster analysis of the hydrogeochemistry and pollutant data illuminated the hydrogeochemical response to the various SW-GW interactions. Clear SW-GW interactions along the Songhua River were revealed: (1) upstream in the study area, groundwater usually discharges into the surface <span class="hlt">water</span>, (2) groundwater is recharged by surface <span class="hlt">water</span> downstream, and (3) discharge and flow-through coexist in between. Statistical analysis indicated that the degree of hydrogeochemical response in different types of hydraulic connection varied, being clear in recharge and flow-through <span class="hlt">modes</span>, and less obvious in discharge <span class="hlt">mode</span>. During the interaction process, dilution, adsorption, redox reactions, nitrification, denitrification, and biodegradation contributed to the pollutant concentration and affected hydrogeochemical response in the hyporheic zone.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=341071&Lab=NHEERL&keyword=information&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=341071&Lab=NHEERL&keyword=information&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>Relationships between aquatic toxicity, chemical hydrophobicity and <span class="hlt">mode</span> of action: log kow QSARs revisited</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>Relationships between chemical hydrophobicity and toxicity have been shown for nearly 100 years in both mammals and fish, typically using the log of the octanol:<span class="hlt">water</span> partition coefficient (kow). The current study reassessed the influence of <span class="hlt">mode</span> of action (MOA) on aquatic toxici...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22310638-probing-plasmonic-breathing-modes-optically','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22310638-probing-plasmonic-breathing-modes-optically"><span>Probing plasmonic breathing <span class="hlt">modes</span> optically</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>Krug, Markus K., E-mail: markus.krug@uni-graz.at; Reisecker, Michael; Hohenau, Andreas</p> <p>2014-10-27</p> <p>The confinement of surface plasmon <span class="hlt">modes</span> in flat nanoparticles gives rise to plasmonic breathing <span class="hlt">modes</span>. With a vanishing net dipole moment, breathing <span class="hlt">modes</span> do not radiate, i.e., they are optically dark. Having thus escaped optical detection, breathing <span class="hlt">modes</span> were only recently revealed in silver nanodisks with electron energy loss spectroscopy in an electron microscope. We show that for disk diameters >200 nm, retardation induced by oblique optical illumination relaxes the optically dark character. This makes breathing <span class="hlt">modes</span> and thus the full plasmonic <span class="hlt">mode</span> spectrum accessible to optical spectroscopy. The experimental spectroscopy data are in excellent agreement with numerical simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7774M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7774M"><span>Transformation of fault slip <span class="hlt">modes</span> in laboratory experiments</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martynov, Vasilii; Alexey, Ostapchuk; Markov, Vadim</p> <p>2017-04-01</p> <p>Slip <span class="hlt">mode</span> of crust fault can vary because of many reasons. It's well known that fault structure, material of fault gouge, pore fluid et al. in many ways determines slip <span class="hlt">modes</span> from creep and slow slip events to mega-earthquakes [1-3]. Therefore, the possibility of fault slip transformation due to external action is urgent question. There is popular and developing approach of fluid injection into central part of fault. The phenomenon of earthquakes induced due to pumping of <span class="hlt">water</span> was investigated on small and large scales [4, 5]. In this work the laboratory experiments were conducted to study the evolution of the experimental fault slip when changing the properties of the interstitial fluid. The scheme of experiments is the classical slider-model set-up, in which the block under the shear force slips along the interface. In our experiments the plexiglas block 8x8x3 cm3 in size was put on the plexiglas base. The contact of the blocks was filled with a thin layer (about 3 mm thick) of a granular material. The normal load varied from 31 to 156 kPa. The shear load was applied through a spring with stiffness 60 kN/m, and the rate of spring deformation was 20 or 5 mcm/s. Two parameters were recorded during experiments: the shear force acting on the upper block (with an accuracy of 1 N) and its displacement relatively the base (with an accuracy of 0.1 μm). The gouge was composed of quartz sand (97.5%) and clay (2.5%). As a moisturizer were used different fluids with viscosity varying from 1 to 103 mPa x s. Different slip <span class="hlt">modes</span> were simulated during slider-experiments. In our experiments slip <span class="hlt">mode</span> is the act of instability manifested in an increase of slip velocity and a drop of shear stress acting on a movable block. The amplitude of a shear stress drop and the peak velocity of the upper block were chosen as the characteristics of the slip <span class="hlt">mode</span>. In the laboratory experiments, slip events of one type can be achieved either as regularly recurring (regular <span class="hlt">mode</span>) or as random</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880067067&hterms=lime&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlime','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880067067&hterms=lime&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dlime"><span>Microstructural effects on fracture toughness of polycrystalline ceramics in combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Singh, D.; Shetty, D. K.</p> <p>1988-01-01</p> <p>Fracture toughness of polycrystalline alumina and ceria partially-stabilized tetragonal zirconia (CeO2-TZP) ceramics were assessed in combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II loading using precracked disk specimens in diametral compression. Stress states ranging from pure <span class="hlt">mode</span> I, combined <span class="hlt">mode</span> I and <span class="hlt">mode</span> II, and pure <span class="hlt">mode</span> II were obtained by aligning the center crack at specific angles relative to the loading diameter. The resulting mixed-<span class="hlt">mode</span> fracture toughness envelope showed significant deviation to higher fracture toughness in <span class="hlt">mode</span> II relative to the predictions of the linear elastic fracture mechanics theory. Critical comparison with corresponding results on soda-lime glass and fracture surface observations showed that crack surface resistance arising from grain interlocking and abrasion was the main source of the increased fracture toughness in <span class="hlt">mode</span> II loading of the polycrystalline ceramics. The normalized fracture toughness for pure <span class="hlt">mode</span> II loading, (KII/KIc), increased with increasing grain size for the CeO2-TZP ceramics. Quantitative fractography confirmed an increased percentage of transgranular fracture of the grains in <span class="hlt">mode</span> II loading.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28861744','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28861744"><span>Bond durability of universal adhesive to bovine enamel using self-etch <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Suzuki, Soshi; Takamizawa, Toshiki; Imai, Arisa; Tsujimoto, Akimasa; Sai, Keiichi; Takimoto, Masayuki; Barkmeier, Wayne W; Latta, Mark A; Miyazaki, Masashi</p> <p>2018-04-01</p> <p>The purpose of this study was to examine the enamel bond durability of universal adhesives in the self-etch <span class="hlt">mode</span> under 2-year <span class="hlt">water</span> storage and thermal cycling conditions. Three commercially available universal adhesives and a gold standard two-step self-etch adhesive were used. Ten specimens of bovine enamel were prepared per test group, and shear bond strength (SBS) was measured to determine the bonding durability after thermal cycling (TC) or long-term <span class="hlt">water</span> storage (WS). The bonded specimens were divided into three groups: (1) specimens subjected to TC, where the bonded specimens were stored in 37 °C distilled <span class="hlt">water</span> for 24 h before being subjected to 3000, 10,000, 20,000 or 30,000 TC; (2) specimens stored in 37 °C distilled <span class="hlt">water</span> for 3 months, 6 months, 1 year or 2 year; and (3) specimens stored in 37 °C distilled <span class="hlt">water</span> for 24 h, serving as a baseline. The two-step self-etch adhesive showed significantly higher SBS than the universal adhesives tested, regardless of the type of degradation method. All universal adhesives showed no significant enamel SBS reductions in TC and WS, when compared to baseline and the other degradation conditions. Compared to the bond strengths obtained with the two-step self-etch adhesive, significantly lower bond strengths were obtained with universal adhesives. However, the enamel bond durability of universal adhesives was relatively stable under both degradation conditions tested. The present data indicate that the enamel bond durability of universal adhesives in the self-etch <span class="hlt">mode</span> might be sufficient for clinical use.</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.ncbi.nlm.nih.gov/pubmed/25835653','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25835653"><span>Nonlinear interaction in differential <span class="hlt">mode</span> delay managed <span class="hlt">mode</span>-division multiplexed transmission systems.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rademacher, Georg; Warm, Stefan; Petermann, Klaus</p> <p>2015-01-12</p> <p>We analyze the impact of Differential <span class="hlt">Mode</span> Delay (DMD) Management on the nonlinear impairments in <span class="hlt">mode</span>-division multiplexed transmission systems. It is found out that DMD Management can lead to a degraded performance, due to enhanced intermodal nonlinear interaction. This can be attributed to an increased correlation of co-propagating channels, similar to the effects that show up in dispersion managed single-<span class="hlt">mode</span> systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1352N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1352N"><span>Cryptic outgassing from the Southern Ocean during the Holocene</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nichols, J. E.; Moy, C. M.; Peteet, D. M.; Vandergoes, M.; Curtin, L.; Gilmer, G.</p> <p>2017-12-01</p> <p>The Southern Ocean is an important pre-anthropogenic source of carbon to the atmosphere. When Southern Hemisphere Westerly Winds are shifted poleward, wind-driven upwelling brings carbon-rich deep <span class="hlt">water</span> to the surface. Multiple studies have shown that this mechanism is particularly important during the last deglaciation and is partly influenced by climate and oceanographic change triggered by the Northern Hemisphere high latitudes and the tropics. Here we show that the middle Holocene, too, was an important time for increased upwelling. New paleoecological reconstructions, inorganic and organic geochemical data, and stable isotope data from lakes and peatlands on New Zealand's South Island and <span class="hlt">Subantarctic</span> Islands show strong evidence for poleward-shifted Southern Hemisphere Westerly Winds during the middle Holocene. Warming in the northern hemisphere either weakens westerlies or shifts them southward, reinvigorating the CO2 outgassing from the Southern Ocean. However, if, like in the deglacial period, the Southern Ocean was a source of carbon to the atmosphere in the middle Holocene, why do we not see ice-core evidence for increased pCO2 of the atmosphere? To answer this question, we look north, to the peatlands of the sub-Boreal, Boreal, and Arctic regions. We find, using a new compilation of peatland carbon accumulation rate data, that the northern peatland carbon sink, which was not a factor in the deglacial carbon cycle, could be strong enough in the mid Holocene to counterbalance the increased outgassing. The peatland carbon sink is strongest at the same time as our records from the <span class="hlt">subantarctic</span> show that the SHWW are in a weakened or poleward-shifted state. Our work shows how the <span class="hlt">subantarctic</span> has revealed a globally important mechanism impacting the carbon cycle of the Holocene.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29578579','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29578579"><span>Intensity modulated operating <span class="hlt">mode</span> of the rotating gamma system.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sengupta, Bishwambhar; Gulyas, Laszlo; Medlin, Donald; Koroknai, Tibor; Takacs, David; Filep, Gyorgy; Panko, Peter; Godo, Bence; Hollo, Tamas; Zheng, Xiao Ran; Fedorcsak, Imre; Dobai, Jozsef; Bognar, Laszlo; Takacs, Endre</p> <p>2018-05-01</p> <p>The purpose of this work was to explore two novel operation modalities of the rotating gamma systems (RGS) that could expand its clinical application to lesions in close proximity to critical organs at risk (OAR). The approach taken in this study consists of two components. First, a Geant4-based Monte Carlo (MC) simulation toolkit is used to model the dosimetric properties of the RGS Vertex 360™ for the normal, intensity modulated radiosurgery (IMRS), and speed modulated radiosurgery (SMRS) operation modalities. Second, the RGS Vertex 360™ at the Rotating Gamma Institute in Debrecen, Hungary is used to collect experimental data for the normal and IMRS operation <span class="hlt">modes</span>. An ion chamber is used to record measurements of the absolute dose. The dose profiles are measured using Gafchromic EBT3 films positioned within a spherical <span class="hlt">water</span> equivalent phantom. A strong dosimetric agreement between the measured and simulated dose profiles and penumbra was found for both the normal and IMRS operation <span class="hlt">modes</span> for all collimator sizes (4, 8, 14, and 18 mm diameter). The simulated falloff and maximum dose regions agree better with the experimental results for the 4 and 8 mm diameter collimators. Although the falloff regions align well in the 14 and 18 mm collimators, the maximum dose regions have a larger difference. For the IMRS operation <span class="hlt">mode</span>, the simulated and experimental dose distributions are ellipsoidal, where the short axis aligns with the blocked angles. Similarly, the simulated dose distributions for the SMRS operation <span class="hlt">mode</span> also adopt an ellipsoidal shape, where the short axis aligns with the angles where the orbital speed is highest. For both modalities, the dose distribution is highly constrained with a sharper penumbra along the short axes. Dose modulation of the RGS can be achieved with the IMRS and SMRS <span class="hlt">modes</span>. By providing a highly constrained dose distribution with a sharp penumbra, both <span class="hlt">modes</span> could be clinically applicable for the treatment of lesions in close</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1025987','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1025987"><span>Extending <span class="hlt">Mode</span> Areas of Single-<span class="hlt">mode</span> All-solid Photonic Bandgap Fibers</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2015-04-02</p> <p>T. Tunnermann, R. Iliew, F. Lederer, J. Broeng, G. Vienne, A. Petersson, and C. Jakobsen, “High-power air-clad large-<span class="hlt">mode</span>-area photonic crystal ...Yvernault, and F. Salin, “Extended single-<span class="hlt">mode</span> photonic crystal fiber lasers,” Opt. Express 14(7), 2715–2720 (2006). 10. L. Dong, T. Wu, H. McKay, L. Fu...progress in <span class="hlt">mode</span> area scaling of optical fibers. One notable area is in photonic crystal fibers (PCF) [3–5, 8, 9]. The short straight PCF rods used in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28033494','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28033494"><span>Forward osmosis as an approach to manage oil sands tailings <span class="hlt">water</span> and on-site basal depressurization <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhu, Shu; Li, Mingyu; Gamal El-Din, Mohamed</p> <p>2017-04-05</p> <p>As the volume of oil sands process-affected <span class="hlt">water</span> (OSPW) stored in tailings ponds increases, it is urgent to seek for <span class="hlt">water</span> management approaches to alleviate the environmental impact caused by large quantity of toxic <span class="hlt">water</span>. Forward osmosis (FO) utilizes osmotic pressure difference between two solutions, thereby giving a potential to manage two wastewaters. In this study, FO was proposed to manage OSPW, using on-site waste basal depressurization <span class="hlt">water</span> (BDW) as draw solution. To investigate its feasibility, both short and long-term OSPW desalination experiments were carried out. By applying this process, the volume of OSPW was decreased>40% and high rejections were achieved, especially, the major organic toxicity source - naphthenic acids (NAs). Although comparative low <span class="hlt">water</span> flux (≤3L/m 2 h) was obtained, <span class="hlt">water</span> flux caused by membrane fouling can be completely recovered using <span class="hlt">water</span> physical cleaning. Moreover, calcium carbonate precipitation was observed on the OSPW-oriented membrane side. With respect to flux decline, the active layer facing the feed solution (FO <span class="hlt">mode</span>) and active layer facing draw solution (PRO <span class="hlt">mode</span>) did not demonstrate a significant difference on anti-fouling performance. The advantages provided by this approach include zero draw solution cost, less reversible membrane fouling and beneficial reuse/recycle of diluted BDW. Copyright © 2016 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5247482','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5247482"><span>Normal <span class="hlt">modes</span> and <span class="hlt">mode</span> transformation of pure electron vortex beams</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Thirunavukkarasu, G.; Mousley, M.; Babiker, M.</p> <p>2017-01-01</p> <p>Electron vortex beams constitute the first class of matter vortex beams which are currently routinely produced in the laboratory. Here, we briefly review the progress of this nascent field and put forward a natural quantum basis set which we show is suitable for the description of electron vortex beams. The normal <span class="hlt">modes</span> are truncated Bessel beams (TBBs) defined in the aperture plane or the Fourier transform of the transverse structure of the TBBs (FT-TBBs) in the focal plane of a lens with the said aperture. As these <span class="hlt">modes</span> are eigenfunctions of the axial orbital angular momentum operator, they can provide a complete description of the two-dimensional transverse distribution of the wave function of any electron vortex beam in such a system, in analogy with the prominent role Laguerre–Gaussian (LG) beams played in the description of optical vortex beams. The characteristics of the normal <span class="hlt">modes</span> of TBBs and FT-TBBs are described, including the quantized orbital angular momentum (in terms of the winding number l) and the radial index p>0. We present the experimental realization of such beams using computer-generated holograms. The <span class="hlt">mode</span> analysis can be carried out using astigmatic transformation optics, demonstrating close analogy with the astigmatic <span class="hlt">mode</span> transformation between LG and Hermite–Gaussian beams. This article is part of the themed issue ‘Optical orbital angular momentum’. PMID:28069769</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28069769','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28069769"><span>Normal <span class="hlt">modes</span> and <span class="hlt">mode</span> transformation of pure electron vortex beams.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thirunavukkarasu, G; Mousley, M; Babiker, M; Yuan, J</p> <p>2017-02-28</p> <p>Electron vortex beams constitute the first class of matter vortex beams which are currently routinely produced in the laboratory. Here, we briefly review the progress of this nascent field and put forward a natural quantum basis set which we show is suitable for the description of electron vortex beams. The normal <span class="hlt">modes</span> are truncated Bessel beams (TBBs) defined in the aperture plane or the Fourier transform of the transverse structure of the TBBs (FT-TBBs) in the focal plane of a lens with the said aperture. As these <span class="hlt">modes</span> are eigenfunctions of the axial orbital angular momentum operator, they can provide a complete description of the two-dimensional transverse distribution of the wave function of any electron vortex beam in such a system, in analogy with the prominent role Laguerre-Gaussian (LG) beams played in the description of optical vortex beams. The characteristics of the normal <span class="hlt">modes</span> of TBBs and FT-TBBs are described, including the quantized orbital angular momentum (in terms of the winding number l) and the radial index p>0. We present the experimental realization of such beams using computer-generated holograms. The <span class="hlt">mode</span> analysis can be carried out using astigmatic transformation optics, demonstrating close analogy with the astigmatic <span class="hlt">mode</span> transformation between LG and Hermite-Gaussian beams.This article is part of the themed issue 'Optical orbital angular momentum'. © 2017 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017A%26A...601A.130R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017A%26A...601A.130R"><span>Frequency regularities of acoustic <span class="hlt">modes</span> and multi-colour <span class="hlt">mode</span> identification in rapidly rotating stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reese, D. R.; Lignières, F.; Ballot, J.; Dupret, M.-A.; Barban, C.; van't Veer-Menneret, C.; MacGregor, K. B.</p> <p>2017-05-01</p> <p>Context. <span class="hlt">Mode</span> identification has remained a major obstacle in the interpretation of pulsation spectra in rapidly rotating stars. This has motivated recent work on calculating realistic multi-colour <span class="hlt">mode</span> visibilities in this type of star. Aims: We would like to test <span class="hlt">mode</span> identification methods and seismic diagnostics in rapidly rotating stars, using oscillation spectra that are based on these new theoretical predictions. Methods: We investigate the auto-correlation function and Fourier transform of theoretically calculated frequency spectra, in which <span class="hlt">modes</span> are selected according to their visibilities. Given that intrinsic <span class="hlt">mode</span> amplitudes are determined by non-linear saturation and cannot currently be theoretically predicted, we experimented with various ad-hoc prescriptions for setting the <span class="hlt">mode</span> amplitudes, including using random values. Furthermore, we analyse the ratios between <span class="hlt">mode</span> amplitudes observed in different photometric bands to see up to what extent they can identify <span class="hlt">modes</span>. Results: When non-random intrinsic <span class="hlt">mode</span> amplitudes are used, our results show that it is possible to extract a mean value for the large frequency separation or half its value and, sometimes, twice the rotation rate, from the auto-correlation of the frequency spectra. Furthermore, the Fourier transforms are mostly sensitive to the large frequency separation or half its value. The combination of the two methods may therefore measure and distinguish the two types of separations. When the intrinsic <span class="hlt">mode</span> amplitudes include random factors, which seems more representative of real stars, the results are far less favourable. It is only when the large separation or half its value coincides with twice the rotation rate, that it might be possible to detect the signature of a frequency regularity. We also find that amplitude ratios are a good way of grouping together <span class="hlt">modes</span> with similar characteristics. By analysing the frequencies of these groups, it is possible to constrain <span class="hlt">mode</span> identification, as</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1413924-switching-off-hydrogen-bond-driven-excitation-modes-liquid-methanol','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1413924-switching-off-hydrogen-bond-driven-excitation-modes-liquid-methanol"><span>Switching off hydrogen-bond-driven excitation <span class="hlt">modes</span> in liquid methanol</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bellissima, Stefano; González, Miguel A.; Bafile, Ubaldo; ...</p> <p>2017-08-30</p> <p>Hydrogen bonding plays an essential role on intermolecular forces, and consequently on the thermodynamics of materials defined by this elusive bonding character. It determines the property of a vital liquid as <span class="hlt">water</span> as well as many processes crucial for life. The longstanding controversy on the nature of the hydrogen bond (HB) can be settled by looking at the effect of a vanishing HB interaction on the microscopic properties of a given hydrogen-bonded fluid. This task suits the capabilities of computer simulations techniques, which allow to easily switch off HB interactions. We then use molecular dynamics to study the microscopic propertiesmore » of methanol, a prototypical HB liquid. Fundamental aspects of the dynamics of methanol at room temperature were contextualised only very recently and its rich dynamics was found to have striking analogies with that of <span class="hlt">water</span>. The lower temperature (200 K) considered in the present study led us to observe that the molecular centre-of-mass dynamics is dominated by four <span class="hlt">modes</span>. Most importantly, the computational ability to switch on and off hydrogen bonds permitted us to identify which, among these <span class="hlt">modes</span>, have a pure HB-origin. This clarifies the role of hydrogen bonds in liquid dynamics, disclosing new research opportunities and unexplored interpretation schemes.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21500607','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21500607"><span>Failure <span class="hlt">mode</span> and effects analysis: an empirical comparison of failure <span class="hlt">mode</span> scoring procedures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ashley, Laura; Armitage, Gerry</p> <p>2010-12-01</p> <p>To empirically compare 2 different commonly used failure <span class="hlt">mode</span> and effects analysis (FMEA) scoring procedures with respect to their resultant failure <span class="hlt">mode</span> scores and prioritization: a mathematical procedure, where scores are assigned independently by FMEA team members and averaged, and a consensus procedure, where scores are agreed on by the FMEA team via discussion. A multidisciplinary team undertook a Healthcare FMEA of chemotherapy administration. This included mapping the chemotherapy process, identifying and scoring failure <span class="hlt">modes</span> (potential errors) for each process step, and generating remedial strategies to counteract them. Failure <span class="hlt">modes</span> were scored using both an independent mathematical procedure and a team consensus procedure. Almost three-fifths of the 30 failure <span class="hlt">modes</span> generated were scored differently by the 2 procedures, and for just more than one-third of cases, the score discrepancy was substantial. Using the Healthcare FMEA prioritization cutoff score, almost twice as many failure <span class="hlt">modes</span> were prioritized by the consensus procedure than by the mathematical procedure. This is the first study to empirically demonstrate that different FMEA scoring procedures can score and prioritize failure <span class="hlt">modes</span> differently. It found considerable variability in individual team members' opinions on scores, which highlights the subjective and qualitative nature of failure <span class="hlt">mode</span> scoring. A consensus scoring procedure may be most appropriate for FMEA as it allows variability in individuals' scores and rationales to become apparent and to be discussed and resolved by the team. It may also yield team learning and communication benefits unlikely to result from a mathematical procedure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28414955','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28414955"><span>Influence of relaxation <span class="hlt">modes</span> on membrane fouling in submerged membrane bioreactor for domestic wastewater treatment.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Habib, Rasikh; Asif, Muhammad Bilal; Iftekhar, Sidra; Khan, Zahiruddin; Gurung, Khum; Srivastava, Varsha; Sillanpää, Mika</p> <p>2017-08-01</p> <p>Relaxation and backwashing have become an integral part of membrane bioreactor (MBR) operations for fouling control. This study was carried out on real municipal wastewater to evaluate the influence of different operational strategies on membrane fouling at equivalent <span class="hlt">water</span> yield. Four relaxation <span class="hlt">modes</span> (MBR 10+0, MBR 10+1 , MBR 10+1.5 and MBR 10+2 ) were tested to analyze membrane fouling behavior. For the optimization of relaxation <span class="hlt">modes</span>, fouling rate in terms of trans-membrane pressure, hydraulic resistances and characteristics of fouling fractions were analyzed. It has been observed that cake layer resistance was minimum in MBR 10+1.5 but pore blockage resistance was increased in all relaxation <span class="hlt">modes</span>. Moreover, high instantaneous flux contributed significantly to fouling rate at the initial stage of MBR operations. Relaxation <span class="hlt">modes</span> were also efficient in removing irreversible fouling to some extent. Under all relaxation <span class="hlt">modes</span>, COD removal efficiency ranged from 92 to 96.5%. Ammonium and TP removal were on the lower side due to the short solids and hydraulic retention time. Copyright © 2017 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..DFDQ20005H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDQ20005H"><span><span class="hlt">Water</span> walking - an evolution of <span class="hlt">water</span> surface skipping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hurd, Randy; Belden, Jesse; Jandron, Michael; Bower, Allan; Holekamp, Sean; Truscott, Tadd</p> <p>2017-11-01</p> <p>Previous work has shown that elastomeric spheres skip more easily than disk-shaped stones. This is due to increased lift stemming from sphere deformation, which provides an increased cross-sectional area and favorable attack angle upon impact. We extend lift models developed for individual impacts to long-range multiple impact events and compare the estimates to experimental results, which show good agreement. Additionally, a surprising new <span class="hlt">mode</span> of skipping is observed that resembles <span class="hlt">water</span>-walking, wherein a quickly rotating sphere produces small successive impacts allowing it to move parallel to the <span class="hlt">water</span> surface. The dynamics of this new multiple skip behavior are rationalized analytically and tested experimentally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.916a2019X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.916a2019X"><span>Performance analysis of underwater pump for <span class="hlt">water</span>-air dual-use engine</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xia, Jun; Wang, Yun; Chen, Yu</p> <p>2017-10-01</p> <p>To make <span class="hlt">water</span>-air dual-use engine work both in air and under <span class="hlt">water</span>, the compressor of the engine should not only meet the requirements of air flight, but also must have the ability to work underwater. To verify the performance of the compressor when the <span class="hlt">water</span>-air dual-use engine underwater propulsion <span class="hlt">mode</span>, the underwater pumping <span class="hlt">water</span> model of the air compressor is simulated by commercial CFD software, and the flow field analysis is carried out. The results show that conventional air compressors have a certain ability to work in the <span class="hlt">water</span> environment, however, the blade has a great influence on the flow, and the compressor structure also affects the pump performance. Compressor can initially take into account the two <span class="hlt">modes</span> of <span class="hlt">water</span> and air. In order to obtain better performance, the structure of the compressor needs further improvement and optimization.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GPC...144..252D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GPC...144..252D"><span>Interglacial/glacial changes in coccolith-rich deposition in the SW Pacific Ocean: An analogue for a warmer world?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Duncan, Bella; Carter, Lionel; Dunbar, Gavin; Bostock, Helen; Neil, Helen; Scott, George; Hayward, Bruce W.; Sabaa, Ashwaq</p> <p>2016-09-01</p> <p>Satellite observations of middle to high latitudes show that modern ocean warming is accompanied by increased frequency and poleward expansion of coccolithophore blooms. However, the outcomes of such events and their causal processes are unclear. In this study, marine sediment cores are used to investigate past coccolithophore production north and south of the Subtropical Front. Calcareous pelagites from subtropical <span class="hlt">waters</span> off northernmost New Zealand (site P71) and from <span class="hlt">subantarctic</span> <span class="hlt">waters</span> on Campbell Plateau (Ocean Drilling Program [ODP] site 1120C) record marked changes in pelagite deposition. At both locations, foraminiferal-rich sediments dominate glacial periods whereas coccolith-rich sediments characterise specific interglacial periods. Sediment grain size has been used to determine relative abundances of coccoliths and foraminifers. Results show coccoliths prevailed around certain Marine Isotope Stage (MIS) transitions, at MIS 7b/a and MIS 2/1 at P71, and at MIS 6/5e at ODP 1120C. Palaeo-environmental proxies suggest that coccolithophore production and deposition at P71 reflect enhanced nutrient availability associated with intense winter mixing in the subtropical Tasman Sea. An increased inflow of that warm, micronutrient-bearing subtropical <span class="hlt">water</span> in concert with upper ocean thermal stratification in late spring/summer, led to peak phytoplankton production. At ODP 1120C during MIS 6/5e, an increased inflow of subtropical <span class="hlt">water</span>, warm sea surface temperatures and a thermally stratified upper ocean also favoured coccolithophore production. These palaeo-environmental reconstructions together with model simulations suggest that (i) future subtropical coccolithophore production at P71 is unlikely to reach abundances recorded during MIS 7b/a but (ii) future <span class="hlt">subantarctic</span> production is likely to dominate sedimentation over Campbell Plateau as modern conditions trend towards those prevalent during MIS 5e.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21935029','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21935029"><span>Dual-LP11 <span class="hlt">mode</span> 4×4 MIMO-OFDM transmission over a two-<span class="hlt">mode</span> fiber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Al Amin, Abdullah; Li, An; Chen, Simin; Chen, Xi; Gao, Guanjun; Shieh, William</p> <p>2011-08-15</p> <p>We report successful transmission of dual-LP(11) <span class="hlt">mode</span> (LP(11a) and LP(11b)), dual polarization coherent optical orthogonal frequency-division multiplexing (CO-OFDM) signals over two-<span class="hlt">mode</span> fibers (TMF) using all-fiber <span class="hlt">mode</span> converters. <span class="hlt">Mode</span> converters based on mechanically induced long-period grating with better than 20 dB extinction ratios are realized and used for interfacing single-<span class="hlt">mode</span> fiber transmitter and receivers to the TMF. We demonstrate that by using 4×4 MIMO-OFDM processing, the random coupling of the two LP(11) spatial <span class="hlt">modes</span> can be successfully tracked and equalized with a one-tap frequency-domain equalizer. We achieve successful transmission of 35.3 Gb/s over 26-km two-<span class="hlt">mode</span> fiber with less than 3 dB penalty. © 2011 Optical Society of America</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20030032968','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20030032968"><span><span class="hlt">Mode</span> I, <span class="hlt">Mode</span> II, and Mixed-<span class="hlt">Mode</span> Fracture of Plasma-sprayed Thermal Barrier Coatings at Ambient and Elevated Temperatures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Choi, Sung R.; Zhu, Dongming; Miller, Robert A.</p> <p>2003-01-01</p> <p>The mixed-<span class="hlt">mode</span> fracture behavior of plasma-sprayed ZrO2-8 wt% Y2O3 thermal barrier coatings was determined in air at 25 and 1316 C in asymmetric four-point flexure with single edge v-notched beam (SEVNB) test specimens. The <span class="hlt">mode</span> I fracture toughness was found to be K(sub Ic) = 1.15 plus or minus 0.07 and 0.98 plus or minus 0.13 MPa the square root of m, respectively, at 25 and 1316 C. The respective <span class="hlt">mode</span> II fracture toughness values were K(sub IIc) = 0.73 plus or minus 0.10 and 0.65 plus or minus 0.04 MPa the square root of m. Hence, there was an insignificant difference in either K(sub Ic or K(sub IIc) between 25 and 1316 C for the coating material, whereas there was a noticeable distinction between K(sub Ic) and K(sub IIc), resulting in K(sub IIc) per K(sub Ic) = 0.65 at both temperatures. The empirical mixed-<span class="hlt">mode</span> fracture criterion best described the coatings' mixed-<span class="hlt">mode</span> fracture behavior among the four mixed-<span class="hlt">mode</span> fracture theories considered. The angle of crack propagation was in reasonable agreement with the minimum strain energy density criterion. The effect of the directionality of the coating material in on K(sub Ic) was observed to be insignificant, while its sintering effect at 1316 C on K(sub Ic) was significant.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015SPIE.9343E..1DN','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015SPIE.9343E..1DN"><span>Resonator <span class="hlt">modes</span> and <span class="hlt">mode</span> dynamics for an external cavity-coupled laser array</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nair, Niketh; Bochove, Erik J.; Aceves, Alejandro B.; Zunoubi, Mohammad R.; Braiman, Yehuda</p> <p>2015-03-01</p> <p>Employing a Fox-Li approach, we derived the cold-cavity <span class="hlt">mode</span> structure and a coupled <span class="hlt">mode</span> theory for a phased array of N single-transverse-<span class="hlt">mode</span> active waveguides with feedback from an external cavity. We applied the analysis to a system with arbitrary laser lengths, external cavity design and coupling strengths to the external cavity. The entire system was treated as a single resonator. The effect of the external cavity was modeled by a set of boundary conditions expressed by an N-by-N frequency-dependent matrix relation between incident and reflected fields at the interface with the external cavity. The coupled <span class="hlt">mode</span> theory can be adapted to various types of gain media and internal and external cavity designs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28059185','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28059185"><span><span class="hlt">Mode</span> analysis of higher-order transverse-<span class="hlt">mode</span> correlation beams in a turbulent atmosphere.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Avetisyan, H; Monken, C H</p> <p>2017-01-01</p> <p>Due to the transfer of the angular spectrum of the pump beam to the two-photon state in spontaneous parametric downconversion, the generated twin photons are entangled in their spatial degrees of freedom. This spatial entanglement can be observed through correlation measurements in any set of <span class="hlt">modes</span> in which one may choose to perform measurements. Choosing, e.g., a Hermite-Gaussian (HG) set of spatial <span class="hlt">modes</span> as a basis, one can observe correlations present in their spatial degrees of freedom. In addition, these <span class="hlt">modes</span> can be used as alphabets for quantum communication. For global quantum communication purposes, we derive an analytic expression for two-photon detection probability in terms of HG <span class="hlt">modes</span>, taking into account the effects of the turbulent atmosphere. Our result is more general as it accounts for the propagation of both signal and idler photons through the atmosphere, as opposed to other works considering one photon's propagation in vacuum. We show that while the restrictions on both the parity and order of the downconverted HG fields no longer hold, due to the crosstalk between <span class="hlt">modes</span> when propagating in the atmosphere, the crosstalk is not uniform: there are more robust <span class="hlt">modes</span> that tend to keep the photons in them. These <span class="hlt">modes</span> can be employed in order to increase the fidelity of quantum communication.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1029946-fractographic-study-epoxy-fractured-under-mode-loading-mixed-mode-iii-loading','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1029946-fractographic-study-epoxy-fractured-under-mode-loading-mixed-mode-iii-loading"><span>Fractographic study of epoxy fractured under <span class="hlt">mode</span> I loading and mixed <span class="hlt">mode</span> I/III loading</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>Ren, Fei; Wang, Jy-An John; Bertelsen, Williams D.</p> <p>2011-01-01</p> <p>Fiber reinforced polymeric composite materials are widely used in structural components such as wind turbine blades, which are typically subject to complicated loading conditions. Thus, material response under mixed <span class="hlt">mode</span> loading is of great significance to the reliability of these structures. Epoxy is a thermosetting polymer that is currently used in manufacturing wind turbine blades. The fracture behavior of epoxy is relevant to the mechanical integrity of the wind turbine composite materials. In this study, a novel fracture testing methodology, the spiral notch torsion test (SNTT), was applied to study the fracture behavior of an epoxy material. SNTT samples weremore » tested using either monotonic loading or cyclic loading, while both <span class="hlt">mode</span> I and mixed <span class="hlt">mode</span> I/III loading conditions were used. Fractographic examination indicated the epoxy samples included in this study were prone to <span class="hlt">mode</span> I failure even when the samples were subject to mixed <span class="hlt">mode</span> loading. Different fatigue precracks were observed on <span class="hlt">mode</span> I and mixed <span class="hlt">mode</span> samples, i.e. precracks appeared as a uniform band under <span class="hlt">mode</span> I loading, and a semi-ellipse under mixed <span class="hlt">mode</span> loading. Fracture toughness was also estimated using quantitative fractography.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29143215','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29143215"><span>Combining cationic and anionic mixed-<span class="hlt">mode</span> sorbents in a single cartridge to extract basic and acidic pharmaceuticals simultaneously from environmental <span class="hlt">waters</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Salas, Daniela; Borrull, Francesc; Fontanals, Núria; Marcé, Rosa Maria</p> <p>2018-01-01</p> <p>The aim of the present study is to broaden the applications of mixed-<span class="hlt">mode</span> ion-exchange solid-phase extraction sorbents to extract both basic and acidic compounds simultaneously by combining the sorbents in a single cartridge and developing a simplified extraction procedure. Four different cartridges containing negative and positive charges in the same configuration were evaluated and compared to extract a group of basic, neutral, and acidic pharmaceuticals selected as model compounds. After a thorough optimization of the extraction conditions, the four different cartridges showed to be capable of retaining basic and acidic pharmaceuticals simultaneously through ionic interactions, allowing the introduction of a washing step with 15 mL methanol to eliminate interferences retained by hydrophobic interactions. Using the best combined cartridge, a method was developed, validated, and further applied to environmental <span class="hlt">waters</span> to demonstrate that the method is promising for the extraction of basic and acidic compounds from very complex samples.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016IAUFM..29B.509P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016IAUFM..29B.509P"><span>Spectroscopic <span class="hlt">mode</span> identification of γ Doradus stars: frequencies, <span class="hlt">modes</span>, rotation and wave leakage</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pollard, Karen R.; Brunsden, E.; Davie, M.; Greenwood, A.; Cottrell, P. L.</p> <p></p> <p>The gravity <span class="hlt">modes</span> present in γ Doradus stars probe the deep stellar interiors and are thus of particular interest in asteroseismology. The MUSICIAN programme at the University of Canterbury has been successfully identifying frequencies and pulsation <span class="hlt">modes</span> in many γ Doradus stars using hundreds of precise, high resolution spectroscopic observations obtained with the 1.0 m telescope and HERCULES spectrograph at the Mt John Observatory in New Zealand. In this paper we present a summary of our spectroscopic frequency and <span class="hlt">mode</span> identifications. Of particular interest from our spectroscopic analyses are: the prevalence of (l, m) = 1, 1 <span class="hlt">modes</span> in many γ Dor stars; the importance of stellar rotation in the interpretation of the frequency and <span class="hlt">mode</span> identification; and finally, possible evidence of wave leakage in one of these stars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JaJAP..53hMB10T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JaJAP..53hMB10T"><span>Proposal of optical <span class="hlt">mode</span> switch</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takakura, Ryuta; Jizodo, Makoto; Fujino, Asuka; Tanaka, Tatsushi; Hamamoto, Kiichi</p> <p>2014-08-01</p> <p>Here, we propose a novel optical <span class="hlt">mode</span> switch, which is a new concept of the optical switch. It can overcome the matrix size limitation issue, which has been a general issue for the waveguide optical space switch, because of its simple fiber coupling configuration. In addition, it contributes to the lossless mux/demux function such as wavelength multiplexing with powerless <span class="hlt">mode</span> conversion unlike wavelength conversion. In this paper, we propose the principle of the optical <span class="hlt">mode</span> switch. The simulation results showed less than -30 dB <span class="hlt">mode</span> crosstalk, with less than only 0.1 dB excess loss for a two-<span class="hlt">mode</span> optical switch. Moreover, the scalable configuration up to four <span class="hlt">modes</span> is also proposed in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29323869','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29323869"><span>Dual-Functional Superhydrophobic Textiles with Asymmetric Roll-Down/Pinned States for <span class="hlt">Water</span> Droplet Transportation and Oil-<span class="hlt">Water</span> Separation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Su, Xiaojing; Li, Hongqiang; Lai, Xuejun; Zhang, Lin; Liao, Xiaofeng; Wang, Jing; Chen, Zhonghua; He, Jie; Zeng, Xingrong</p> <p>2018-01-31</p> <p>Superhydrophobic surfaces with tunable adhesion from lotus-leaf to rose-petal states have generated much attention for their potential applications in self-cleaning, anti-icing, oil-<span class="hlt">water</span> separation, microdroplet transportation, and microfluidic devices. Herein we report a facile magnetic-field-manipulation strategy to fabricate dual-functional superhydrophobic textiles with asymmetric roll-down/pinned states on the two surfaces of the textile simultaneously. Upon exposure to a static magnetic field, fluoroalkylsilane-modified iron oxide (F-Fe 3 O 4 ) nanoparticles in polydimethylsiloxane (PDMS) moved along the magnetic field to construct discrepant hierarchical structures and roughnesses on the two sides of the textile. The positive surface (closer to the magnet, or P-surface) showed a <span class="hlt">water</span> contact angle up to 165°, and the opposite surface (or O-surface) had a <span class="hlt">water</span> contact angle of 152.5°. The P-surface where <span class="hlt">water</span> droplets easily slid off with a sliding angle of 7.5° appeared in the "roll-down" state as Cassie <span class="hlt">mode</span>, while the O-surface was in the "pinned" state as Wenzel <span class="hlt">mode</span>, where <span class="hlt">water</span> droplets firmly adhered even at vertical (90°) and inverted (180°) angles. The surface morphology and wetting <span class="hlt">mode</span> were adjustable by varying the ratios of F-Fe 3 O 4 nanoparticles and PDMS. By taking advantage of the asymmetric adhesion behaviors, the as-fabricated superhydrophobic textile was successfully applied in no-loss microdroplet transportation and oil-<span class="hlt">water</span> separation. Our method is simple and cost-effective. The fabricated textile has the characteristics of superhydrophobicity, magnetic responsiveness, excellent chemical stability, adjustable surface morphology, and controllable adhesion. Our findings conceivably stand out as a new tool to fabricate functional superhydrophobic materials with asymmetric surface properties for various potential applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.tmp..865S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.tmp..865S"><span>Investigating light curve modulation via kernel smoothing. II. New additional <span class="hlt">modes</span> in single-<span class="hlt">mode</span> OGLE classical Cepheids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Süveges, Maria; Anderson, Richard I.</p> <p>2018-04-01</p> <p>Detailed knowledge of the variability of classical Cepheids, in particular their modulations and <span class="hlt">mode</span> composition, provides crucial insight into stellar structure and pulsation. However, tiny modulations of the dominant radial-<span class="hlt">mode</span> pulsation were recently found to be very frequent, possibly ubiquitous in Cepheids, which makes secondary <span class="hlt">modes</span> difficult to detect and analyse, since these modulations can easily mask the potentially weak secondary <span class="hlt">modes</span>. The aim of this study is to re-investigate the secondary <span class="hlt">mode</span> content in the sample of OGLE-III and -IV single-<span class="hlt">mode</span> classical Cepheids using kernel regression with adaptive kernel width for pre-whitening, instead of using a constant-parameter model. This leads to a more precise removal of the modulated dominant pulsation, and enables a more complete survey of secondary <span class="hlt">modes</span> with frequencies outside a narrow range around the primary. Our analysis reveals that significant secondary <span class="hlt">modes</span> occur more frequently among first overtone Cepheids than previously thought. The <span class="hlt">mode</span> composition appears significantly different in the Large and Small Magellanic Clouds, suggesting a possible dependence on chemical composition. In addition to the formerly identified non-radial <span class="hlt">mode</span> at P2 ≈ 0.6…0.65P1 (0.62-<span class="hlt">mode</span>), and a cluster of <span class="hlt">modes</span> with near-primary frequency, we find two more candidate non-radial <span class="hlt">modes</span>. One is a numerous group of secondary <span class="hlt">modes</span> with P2 ≈ 1.25P1, which may represent the fundamental of the 0.62-<span class="hlt">mode</span>, supposed to be the first harmonic of an l ∈ {7, 8, 9} non-radial <span class="hlt">mode</span>. The other new <span class="hlt">mode</span> is at P2 ≈ 1.46P1, possibly analogous to a similar, rare <span class="hlt">mode</span> recently discovered among first overtone RR Lyrae stars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JSV...333.2812C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JSV...333.2812C"><span>Facing rim cavities fluctuation <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Casalino, Damiano; Ribeiro, André F. P.; Fares, Ehab</p> <p>2014-06-01</p> <p>Cavity <span class="hlt">modes</span> taking place in the rims of two opposite wheels are investigated through Lattice-Boltzmann CFD simulations. Based on previous observations carried out by the authors during the BANC-II/LAGOON landing gear aeroacoustic study, a resonance <span class="hlt">mode</span> can take place in the volume between the wheels of a two-wheel landing gear, involving a coupling between shear-layer vortical fluctuations and acoustic <span class="hlt">modes</span> resulting from the combination of round cavity <span class="hlt">modes</span> and wheel-to-wheel transversal acoustic <span class="hlt">modes</span>. As a result, side force fluctuations and tonal noise side radiation take place. A parametric study of the cavity <span class="hlt">mode</span> properties is carried out in the present work by varying the distance between the wheels. Moreover, the effects due to the presence of the axle are investigated by removing the axle from the two-wheel assembly. The azimuthal properties of the <span class="hlt">modes</span> are scrutinized by filtering the unsteady flow in narrow bands around the tonal frequencies and investigating the azimuthal structure of the filtered fluctuation <span class="hlt">modes</span>. Estimation of the tone frequencies with an ad hoc proposed analytical formula confirms the observed modal properties of the filtered unsteady flow solutions. The present study constitutes a primary step in the description of facing rim cavity <span class="hlt">modes</span> as a possible source of landing gear tonal noise.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApPhL.112o1101Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApPhL.112o1101Y"><span>Giant plasmonic <span class="hlt">mode</span> splitting in THz metamaterials mediated by coupling with Lorentz phonon <span class="hlt">mode</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Leilei; Huang, Yuanyuan; Liu, Changji; Hu, Fangrong; Jin, Yanping; Yan, Yi; Xu, Xinlong</p> <p>2018-04-01</p> <p>Giant plasmonic <span class="hlt">mode</span> splitting has been observed in THz metamaterials due to the mediation by the Lorentz phonon dielectric material. This splitting <span class="hlt">mode</span> is confirmed by the surface current distribution, indicating that plasmonic <span class="hlt">modes</span> behave like dipole resonances, while the phonon <span class="hlt">mode</span> behaves like multipole resonance due to coupling. The splitting of the plasmonic <span class="hlt">modes</span> demonstrates an anti-crossing behavior with the change in Lorentz central frequency, which suggests that there is energy redistribution between plasmon and phonon <span class="hlt">modes</span>. Similar to the Stark effect, the splitting frequency difference increases with the increasing direct current dielectric function. We also propose an interaction Hamiltonian to understand the physical mechanism of the plasmonic splitting. Furthermore, the splitting is convincible for small Lorentz dielectrics such as sugar and amino acid in the THz region, which could be used for biomolecular sensing applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NucFu..56i2007K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NucFu..56i2007K"><span>Neoclassical tearing <span class="hlt">mode</span> seeding by coupling with infernal <span class="hlt">modes</span> in low-shear tokamaks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kleiner, A.; Graves, J. P.; Brunetti, D.; Cooper, W. A.; Halpern, F. D.; Luciani, J.-F.; Lütjens, H.</p> <p>2016-09-01</p> <p>A numerical and an analytical study of the triggering of resistive MHD <span class="hlt">modes</span> in tokamak plasmas with low magnetic shear core is presented. Flat q profiles give rise to fast growing pressure driven MHD <span class="hlt">modes</span>, such as infernal <span class="hlt">modes</span>. It has been shown that infernal <span class="hlt">modes</span> drive fast growing islands on neighbouring rational surfaces. Numerical simulations of such instabilities in a MAST-like configuration are performed with the initial value stability code XTOR-2F in the resistive frame. The evolution of magnetic islands are computed from XTOR-2F simulations and an analytical model is developed based on Rutherford’s theory in combination with a model of resistive infernal <span class="hlt">modes</span>. The parameter {{Δ }\\prime} is extended from the linear phase to the non-linear phase. Additionally, the destabilising contribution due to a helically perturbed bootstrap current is considered. Comparing the numerical XTOR-2F simulations to the model, we find that coupling has a strong destabilising effect on (neoclassical) tearing <span class="hlt">modes</span> and is able to seed 2/1 magnetic islands in situations when the standard NTM theory predicts stability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17679335','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17679335"><span>Vibration <span class="hlt">mode</span> imaging.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Xiaoming; Zeraati, Mohammad; Kinnick, Randall R; Greenleaf, James F; Fatemi, Mostafa</p> <p>2007-06-01</p> <p>A new method for imaging the vibration <span class="hlt">mode</span> of an object is investigated. The radiation force of ultrasound is used to scan the object at a resonant frequency of the object. The vibration of the object is measured by laser and the resulting acoustic emission from the object is measured by a hydrophone. It is shown that the measured signal is proportional to the value of the <span class="hlt">mode</span> shape at the focal point of the ultrasound beam. Experimental studies are carried out on a mechanical heart valve and arterial phantoms. The <span class="hlt">mode</span> images on the valve are made by the hydrophone measurement and confirmed by finite-element method simulations. Compared with conventional B-scan imaging on arterial phantoms, the <span class="hlt">mode</span> imaging can show not only the interface of the artery and the gelatin, but also the vibration <span class="hlt">modes</span> of the artery. The images taken on the phantom surface suggest that an image of an interior artery can be made by vibration measurements on the surface of the body. However, the image of the artery can be improved if the vibration of the artery is measured directly. Imaging of the structure in the gelatin or tissue can be enhanced by small bubbles and contrast agents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20087168','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20087168"><span>A clinical comparison between a new dual-chamber pacing <span class="hlt">mode</span>-AAIsafeR and DDD <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xue-Jun, Ren; Zhihong, Han; Ye, Wang; Huifeng, Du; Jinrong, Zhang; Fang, Chen; Jihong, Guo</p> <p>2010-02-01</p> <p>The aim of this study was to compare the cross-follow-up results in DDD or AAISafeR <span class="hlt">mode</span> and to describe the safety and effectiveness of this pacing <span class="hlt">mode</span>. The Symphony 2450/2550 cardiac pacemakers were implanted in 30 patients with sick sinus syndrome between February 2006 and September 2006. They were randomized to the DDD <span class="hlt">mode</span> or AAISafeR <span class="hlt">mode</span> for 3 months and then crossed over to the alternate pacing modality for an additional 3 months. No AAISafeR-related adverse event was observed. All documented episodes of paroxysmal atrial ventricular block caused the immediate switch of the pacing <span class="hlt">mode</span> from AAI to DDD. The cumulative percent ventricular pacing was significantly reduced in the AAISafeR <span class="hlt">mode</span> compared with the DDD <span class="hlt">mode</span> (0.9% [0%-3%] versus 51.3% [2%-91%] P = 0.001; 2.94% [0%-18%] versus 41.18% [0%-65%] P = 0.0001). After 3 months in DDD <span class="hlt">mode</span>, left atrial diameter, left ventricular enddiastolic diameter, and left ventricular end-systolic diameter increased significantly and left ventricular ejection fraction decreased. However, no obvious changes appeared in 3 months of AAISafeR <span class="hlt">mode</span>. Switches to DDD occurred during follow-up in 21 patients due to different-degree atrial ventricular block. The AAISafeR <span class="hlt">mode</span> substantially reduces the amount of unnecessary right ventricular pacing in the bradycardia population and effectively prevents the deleterious effects on cardiac performance. An international randomized study will further ascertain the efficacy of this new pacing <span class="hlt">mode</span> specifically in the prevention of heart failure hospitalization and atrial fibrillation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870024439&hterms=water+filters&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dwater%2Bfilters','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870024439&hterms=water+filters&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D90%26Ntt%3Dwater%2Bfilters"><span>High-latitude filtering in a global grid-point model using model normal <span class="hlt">modes</span>. [Fourier filters for synoptic weather forecasting</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Takacs, L. L.; Kalnay, E.; Navon, I. M.</p> <p>1985-01-01</p> <p>A normal <span class="hlt">modes</span> expansion technique is applied to perform high latitude filtering in the GLAS fourth order global shallow <span class="hlt">water</span> model with orography. The maximum permissible time step in the solution code is controlled by the frequency of the fastest propagating <span class="hlt">mode</span>, which can be a gravity wave. Numerical methods are defined for filtering the data to identify the number of gravity <span class="hlt">modes</span> to be included in the computations in order to obtain the appropriate zonal wavenumbers. The performances of the model with and without the filter, and with a time tendency and a prognostic field filter are tested with simulations of the Northern Hemisphere winter. The normal <span class="hlt">modes</span> expansion technique is shown to leave the Rossby <span class="hlt">modes</span> intact and permit 3-5 day predictions, a range not possible with the other high-latitude filters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1083954','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1083954"><span><span class="hlt">Mode</span> synthesizing atomic force microscopy and <span class="hlt">mode</span>-synthesizing sensing</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Passian, Ali; Thundat, Thomas George; Tetard, Laurene</p> <p>2013-05-17</p> <p>A method of analyzing a sample that includes applying a first set of energies at a first set of frequencies to a sample and applying, simultaneously with the applying the first set of energies, a second set of energies at a second set of frequencies, wherein the first set of energies and the second set of energies form a multi-<span class="hlt">mode</span> coupling. The method further includes detecting an effect of the multi-<span class="hlt">mode</span> coupling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1149602','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1149602"><span><span class="hlt">Mode</span>-synthesizing atomic force microscopy and <span class="hlt">mode</span>-synthesizing sensing</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Passain, Ali; Thundat, Thomas George; Tetard, Laurene</p> <p>2014-07-22</p> <p>A method of analyzing a sample that includes applying a first set of energies at a first set of frequencies to a sample and applying, simultaneously with the applying the first set of energies, a second set of energies at a second set of frequencies, wherein the first set of energies and the second set of energies form a multi-<span class="hlt">mode</span> coupling. The method further includes detecting an effect of the multi-<span class="hlt">mode</span> coupling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23038511','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23038511"><span>GaN microwires as optical microcavities: whispering gallery <span class="hlt">modes</span> Vs Fabry-Perot <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Coulon, Pierre-Marie; Hugues, Maxime; Alloing, Blandine; Beraudo, Emmanuel; Leroux, Mathieu; Zuniga-Perez, Jesus</p> <p>2012-08-13</p> <p>GaN microwires grown by metalorganic vapour phase epitaxy and with radii typically on the order of 1-5 micrometers exhibit a number of resonances in their photoluminescence spectra. These resonances include whispering gallery <span class="hlt">modes</span> and transverse Fabry-Perot <span class="hlt">modes</span>. A detailed spectroscopic study by polarization-resolved microphotoluminescence, in combination with electron microscopy images, has enabled to differentiate both kinds of <span class="hlt">modes</span> and determined their main spectral properties. Finally, the dispersion of the ordinary and extraordinary refractive indices of strain-free GaN in the visible-UV range has been obtained thanks to the numerical simulation of the observed <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008ESASP.665E..15R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008ESASP.665E..15R"><span>AADL <span class="hlt">Modes</span> for Space Software</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rolland, J.-F.; Filali, M.; Bodeveixm, J.-P.; Chemouil, D.; Thomas, D.; Rossignol, A.</p> <p>2008-08-01</p> <p>In this paper we study the <span class="hlt">mode</span> concept in AADL. First we present briefly this language and we define the subset that we use. Then, we propose an abstract TLA+ specification of the <span class="hlt">mode</span> transition. Then, we discuss how the <span class="hlt">mode</span> concepts proposed AADL could be related to this abstraction. We also present different issues related to the <span class="hlt">mode</span> transition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1224435','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1224435"><span>Waveguides having patterned, flattened <span class="hlt">modes</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>Messerly, Michael J.; Pax, Paul H.; Dawson, Jay W.</p> <p></p> <p>Field-flattening strands may be added to and arbitrarily positioned within a field-flattening shell to create a waveguide that supports a patterned, flattened <span class="hlt">mode</span>. Patterning does not alter the effective index or flattened nature of the <span class="hlt">mode</span>, but does alter the characteristics of other <span class="hlt">modes</span>. Compared to a telecom fiber, a hexagonal pattern of strands allows for a three-fold increase in the flattened <span class="hlt">mode</span>'s area without reducing the separation between its effective index and that of its bend-coupled <span class="hlt">mode</span>. Hexagonal strand and shell elements prove to be a reasonable approximation, and, thus, to be of practical benefit vis-a-vis fabrication, to thosemore » of circular cross section. Patterned flattened <span class="hlt">modes</span> offer a new and valuable path to power scaling.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25494003','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25494003"><span>Simultaneous spectral and temporal analyses of kinetic energies in nonequilibrium systems: theory and application to vibrational relaxation of O-D stretch <span class="hlt">mode</span> of HOD in <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jeon, Jonggu; Lim, Joon Hyung; Kim, Seongheun; Kim, Heejae; Cho, Minhaeng</p> <p>2015-05-28</p> <p>A time series of kinetic energies (KE) from classical molecular dynamics (MD) simulation contains fundamental information on system dynamics. It can also be analyzed in the frequency domain through Fourier transformation (FT) of velocity correlation functions, providing energy content of different spectral regions. By limiting the FT time span, we have previously shown that spectral resolution of KE evolution is possible in the nonequilibrium situations [Jeon and Cho, J. Chem. Phys. 2011, 135, 214504]. In this paper, we refine the method by employing the concept of instantaneous power spectra, extending it to reflect an instantaneous time-correlation of velocities with those in the future as well as with those in the past, and present a new method to obtain the instantaneous spectral density of KE (iKESD). This approach enables the simultaneous spectral and temporal resolution of KE with unlimited time precision. We discuss the formal and novel properties of the new iKESD approaches and how to optimize computational methods and determine parameters for practical applications. The method is specifically applied to the nonequilibrium MD simulation of vibrational relaxation of the OD stretch <span class="hlt">mode</span> in a hydrated HOD molecule by employing a hybrid quantum mechanical/molecular mechanical (QM/MM) potential. We directly compare the computational results with the OD band population relaxation time profiles extracted from the IR pump-probe measurements for 5% HOD in <span class="hlt">water</span>. The calculated iKESD yields the OD bond relaxation time scale ∼30% larger than the experimental value, and this decay is largely frequency-independent if the classical anharmonicity is accounted for. From the integrated iKESD over intra- and intermolecular bands, the major energy transfer pathways were found to involve the HOD bending <span class="hlt">mode</span> in the subps range, then the internal <span class="hlt">modes</span> of the solvent until 5 ps after excitation, and eventually the solvent intermolecular <span class="hlt">modes</span>. Also, strong hydrogen</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018FrES...12...52T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018FrES...12...52T"><span>Nitrogen uptake by phytoplankton in surface <span class="hlt">waters</span> of the Indian sector of Southern Ocean during austral summer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tripathy, S. C.; Patra, Sivaji; Vishnu Vardhan, K.; Sarkar, A.; Mishra, R. K.; Anilkumar, N.</p> <p>2018-03-01</p> <p>This study reports the nitrogen uptake rate (using 15N tracer) of phytoplankton in surface <span class="hlt">waters</span> of different frontal zones in the Indian sector of the Southern Ocean (SO) during austral summer of 2013. The investigated area encompasses four major frontal systems, i.e., the subtropical front (STF), <span class="hlt">subantarctic</span> front (SAF), polar front-1 (PF1) and polar front-2 (PF2). Southward decrease of surface <span class="hlt">water</span> temperature was observed, whereas surface salinity did not show any significant trend. Nutrient (NO3 - and SiO4 4-) concentrations increased southward from STF to PF; while ammonium (NH4 +), nitrite (NO2 -) and phosphate (PO4 3-) remained comparatively stable. Analysis of nutrient ratios indicated potential N-limited conditions at the STF and SAF but no such scenario was observed for PF. In terms of phytoplankton biomass, PF1 was found to be the most productive followed by SAF, whereas PF2 was the least productive region. Nitrate uptake rate increased with increasing latitude, as no systematic spatial variation was discerned for NH4 + and urea (CO(NH2)2). Linear relationship between nitrate and total N-uptake reveals that the studied area is capable of exporting up to 60% of the total production to the deep ocean if the environmental settings are favorable. Like N-uptake rates the f-ratio also increased towards PF region indicating comparatively higher new production in the PF than in the subtropics. The moderately high average f-ratio (0.53) indicates potentially near equal contributions by new production and regenerated production to the total productivity in the study area. Elevation in N-uptake rates with declining temperature suggests that the SO with its vast quantity of cool <span class="hlt">water</span> could play an important role in drawing down the atmospheric CO2 through the "solubility pump".</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997PhDT.......240S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997PhDT.......240S"><span>Time-domain study of acoustic pulse propagation in an ocean waveguide using a new normal <span class="hlt">mode</span> model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sidorovskaia, Natalia Anatol'evna</p> <p>1997-11-01</p> <p>This study is focused on issues of numerical modeling of sound propagation in diverse ocean waveguides. A new normal <span class="hlt">mode</span> acoustical model (Shallow <span class="hlt">Water</span> Acoustic <span class="hlt">Mode</span> Propagation-SWAMP) has been developed. The algorithm for obtaining the vertical modal solution is based on a warping matrix transformation of the solution of an isovelocity (reference) waveguide to one of arbitrary velocity profile. An efficient <span class="hlt">mode</span> coupling scheme with an adaptive step-size in range has been implemented for range-dependent environments. The new algorithm allows fairly arbitrary ocean layering and readily works at high frequency. An important advantage of the new procedure is that vertical modal eigenfunctions can easily be transformed to a spherical representation suitable for coupling in object scattering problems. Benchmarking results of the new code against established acoustic models based on parabolic equation and existing normal <span class="hlt">mode</span> approaches show good agreement for range-independent and up-slope and down-slope bathymetries and a very competitive calculation speed. Broad-band pulse propagation in deep and shallow <span class="hlt">water</span> with double (surface and bottom) ducts has been modeled using the new normal <span class="hlt">mode</span> model for a variety of ocean waveguide parameters and different frequency bands. The surface duct generates a series of the surface-duct-trapped- <span class="hlt">modes</span>, which form amplitude-modulated precursors in the far field pulse response. It has been found that the arrival times of the precursors could not be explained by the conventional concept of group velocity so that a more general principle based on the rate of energy transfer has been used. The Airy function solution was found to explain the amplitude modulation of the precursors. It has been learned from the numerical simulation that for a range-independent environment the time separation between precursors is fixed and any variations from this have been a result of range-dependence and <span class="hlt">mode</span> coupling in the model. The time</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhRvL.106q8103R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhRvL.106q8103R"><span>Paddling <span class="hlt">Mode</span> of Forward Flight in Insects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ristroph, Leif; Bergou, Attila J.; Guckenheimer, John; Wang, Z. Jane; Cohen, Itai</p> <p>2011-04-01</p> <p>By analyzing high-speed video of the fruit fly, we discover a swimminglike <span class="hlt">mode</span> of forward flight characterized by paddling wing motions. We develop a new aerodynamic analysis procedure to show that these insects generate drag-based thrust by slicing their wings forward at low angle of attack and pushing backwards at a higher angle. Reduced-order models and simulations reveal that the law for flight speed is determined by these wing motions but is insensitive to material properties of the fluid. Thus, paddling is as effective in air as in <span class="hlt">water</span> and represents a common strategy for propulsion through aquatic and aerial environments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JSV...422....1S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JSV...422....1S"><span>Deconvolution of azimuthal <span class="hlt">mode</span> detection measurements</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sijtsma, Pieter; Brouwer, Harry</p> <p>2018-05-01</p> <p>Unequally spaced transducer rings make it possible to extend the range of detectable azimuthal <span class="hlt">modes</span>. The disadvantage is that the response of the <span class="hlt">mode</span> detection algorithm to a single <span class="hlt">mode</span> is distributed over all detectable <span class="hlt">modes</span>, similarly to the Point Spread Function of Conventional Beamforming with microphone arrays. With multiple <span class="hlt">modes</span> the response patterns interfere, leading to a relatively high "noise floor" of spurious <span class="hlt">modes</span> in the detected <span class="hlt">mode</span> spectrum, in other words, to a low dynamic range. In this paper a deconvolution strategy is proposed for increasing this dynamic range. It starts with separating the measured sound into shaft tones and broadband noise. For broadband noise <span class="hlt">modes</span>, a standard Non-Negative Least Squares solver appeared to be a perfect deconvolution tool. For shaft tones a Matching Pursuit approach is proposed, taking advantage of the sparsity of dominant <span class="hlt">modes</span>. The deconvolution methods were applied to <span class="hlt">mode</span> detection measurements in a fan rig. An increase in dynamic range of typically 10-15 dB was found.</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/2011SPIE.7913E..04N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011SPIE.7913E..04N"><span>Constructing petal <span class="hlt">modes</span> from the coherent superposition of Laguerre-Gaussian <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naidoo, Darryl; Forbes, Andrew; Ait-Ameur, Kamel; Brunel, Marc</p> <p>2011-03-01</p> <p>An experimental approach in generating Petal-like transverse <span class="hlt">modes</span>, which are similar to what is seen in porro-prism resonators, has been successfully demonstrated. We hypothesize that the petal-like structures are generated from a coherent superposition of Laguerre-Gaussian <span class="hlt">modes</span> of zero radial order and opposite azimuthal order. To verify this hypothesis, visually based comparisons such as petal peak to peak diameter and the angle between adjacent petals are drawn between experimental data and simulated data. The beam quality factor of the Petal-like transverse <span class="hlt">modes</span> and an inner product interaction is also experimentally compared to numerical results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017WRCM...27....1X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017WRCM...27....1X"><span>Multi-soliton solutions and Bäcklund transformation for a two-<span class="hlt">mode</span> KdV equation in a fluid</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xiao, Zi-Jian; Tian, Bo; Zhen, Hui-Ling; Chai, Jun; Wu, Xiao-Yu</p> <p>2017-01-01</p> <p>In this paper, we investigate a two-<span class="hlt">mode</span> Korteweg-de Vries equation, which describes the one-dimensional propagation of shallow <span class="hlt">water</span> waves with two <span class="hlt">modes</span> in a weakly nonlinear and dispersive fluid system. With the binary Bell polynomial and an auxiliary variable, bilinear forms, multi-soliton solutions in the two-wave <span class="hlt">modes</span> and Bell polynomial-type Bäcklund transformation for such an equation are obtained through the symbolic computation. Soliton propagation and collisions between the two solitons are presented. Based on the graphic analysis, it is shown that the increase in s can lead to the increase in the soliton velocities under the condition of ?, but the soliton amplitudes remain unchanged when s changes, where s means the difference between the phase velocities of two-<span class="hlt">mode</span> waves, ? and ? are the nonlinearity parameter and dispersion parameter respectively. Elastic collisions between the two solitons in both two <span class="hlt">modes</span> are analyzed with the help of graphic analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AdSpR..54.2218K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AdSpR..54.2218K"><span>A simulation study on the <span class="hlt">mode</span> conversion process from slow Z-<span class="hlt">mode</span> to LO <span class="hlt">mode</span> by the tunneling effect and variations of beaming angle</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kalaee, Mohammad Javad; Katoh, Yuto</p> <p>2014-12-01</p> <p>For a particular angle of incidence wave, it is possible for a slow Z-<span class="hlt">mode</span> wave incident on an inhomogeneous plasma slab to be converted into an LO <span class="hlt">mode</span> wave. But for another wave normal angle of the incident wave, it has been considered impossible, since an evanescence region exists between two <span class="hlt">mode</span> branches. In this case we expect that the <span class="hlt">mode</span> conversion takes place through the tunneling effect. We investigate the effect of the spatial scale of the density gradient on the <span class="hlt">mode</span> conversion efficiency in an inhomogeneous plasma where the <span class="hlt">mode</span> conversion can occur only by the tunneling effect. We use the computer simulation solving Maxwell's equations and the motion of a cold electron fluid. By considering the steepness of the density gradient, the simulation results show the efficient <span class="hlt">mode</span> conversion could be expected even in the case that the mismatch of the refractive indexes prevents the close coupling of plasma waves. Also, we show for these cases the beaming angle does not correspond to Jones' formula. This effect leads to the angles larger and smaller than the angle estimated by the formula. This type of <span class="hlt">mode</span> conversion process becomes important in a case where the different plasmas form a discontinuity at their contact boundary.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22149799','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22149799"><span>Redistribution of carbonyl stretch <span class="hlt">mode</span> energy in isolated and solvated N-methylacetamide: kinetic energy spectral density analyses.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jeon, Jonggu; Cho, Minhaeng</p> <p>2011-12-07</p> <p>The vibrational energy transfer from the excited carbonyl stretch <span class="hlt">mode</span> in N-deuterated N-methylacetamide (NMA-d), both in isolation and in a heavy <span class="hlt">water</span> cluster, is studied with nonequilibrium molecular dynamics (NEMD) simulations, employing a quantum mechanical/molecular mechanical (QM∕MM) force field at the semiempirical PM3 level. The nonequilibrium ensemble of vibrationally excited NMA-d is prepared by perturbing the positions and velocities of the carbonyl C and O atoms and its NEMD trajectories are obtained with a leap-frog algorithm properly modified for the initial perturbation. In addition to the time-domain analysis of the kinetic and potential energies, a novel method for the spectral analysis of the atomic kinetic energies is developed, in terms of the spectral density of kinetic energy, which provides the time-dependent changes of the frequency-resolved kinetic energies without the complications of normal <span class="hlt">mode</span> analysis at every MD time step. Due to the QM description of the solute electronic structure, the couplings among the normal <span class="hlt">modes</span> are captured more realistically than with classical force fields. The energy transfer in the isolated NMA-d is found to proceed first from the carbonyl bond to other <span class="hlt">modes</span> with time scales of 3 ps or less, and then among the other <span class="hlt">modes</span> over 3-21 ps. In the solvated NMA-d, most of the excess energy is first transferred to other intramolecular <span class="hlt">modes</span> within 5 ps, which is subsequently dissipated to solvent with 7-19 ps time scales. The contribution of the direct energy transfer from the carbonyl bond to solvent was only 5% with ~7 ps time scale. Solvent reorganization that leads to destabilization of the electrostatic interactions is found to be crucial in the long time relaxation of the excess energy, while the <span class="hlt">water</span> intramolecular <span class="hlt">modes</span> do not contribute significantly. Detailed <span class="hlt">mode</span>-specific energy transfer pathways are deduced for the isolated and solvated NMA-d and they show that the energy transfer in NMA-d is a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20596193','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20596193"><span>Passive harmonic <span class="hlt">mode</span> locking by <span class="hlt">mode</span> selection in Fabry-Perot diode lasers with patterned effective index.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bitauld, David; Osborne, Simon; O'Brien, Stephen</p> <p>2010-07-01</p> <p>We demonstrate passive harmonic <span class="hlt">mode</span> locking of a quantum-well laser diode designed to support a discrete comb of Fabry-Perot <span class="hlt">modes</span>. Spectral filtering of the <span class="hlt">mode</span> spectrum was achieved using a nonperiodic patterning of the cavity effective index. By selecting six <span class="hlt">modes</span> spaced at twice the fundamental <span class="hlt">mode</span> spacing, near-transform-limited pulsed output with 2 ps pulse duration was obtained at a repetition rate of 100 GHz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19488314','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19488314"><span>Coupling of small, low-loss hexapole <span class="hlt">mode</span> with photonic crystal slab waveguide <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kim, Guk-Hyun; Lee, Yong-Hee; Shinya, Akihiko; Notomi, Masaya</p> <p>2004-12-27</p> <p>Coupling characteristics between the single-cell hexapole <span class="hlt">mode</span> and the triangular-lattice photonic crystal slab waveguide <span class="hlt">mode</span> is studied by the finite-difference time-domain method. The single-cell hexapole <span class="hlt">mode</span> has a high quality factor (Q) of 3.3Chi106 and a small modal volume of 1.18(lambda/n)3. Based on the symmetry, three representative types of coupling geometries (shoulder-couple, butt-couple and side-couple structures) are selected and tested. The coupling efficiency shows strong dependence on the transverse overlap of the cavity <span class="hlt">mode</span> and the waveguide <span class="hlt">mode</span> over the region of the waveguide. The shoulder-couple structure shows best coupling characteristics among three tested structures. For example, two shouldercouple waveguides and a hexapole cavity result in a high performance resonant-tunneling-filter with Q of 9.7Chi105 and transmittance of 0.48. In the side-couple structure, the coupling strength is much weaker than that of the shoulder-couple structure because of the poor spatial overlap between the <span class="hlt">mode</span> profiles. In the direct-couple structure, the energy transfer from the cavity to the waveguide is prohibited because of the symmetry mismatch and no coupling is observed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850012960','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850012960"><span>Characterization of <span class="hlt">mode</span> 1 and mixed-<span class="hlt">mode</span> failure of adhesive bonds between composite adherends</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mall, S.; Johnson, W. S.</p> <p>1985-01-01</p> <p>A combined experimental and analytical investigation of an adhesively bonded composite joint was conducted to characterize both the static and fatigue beyond growth mechanism under <span class="hlt">mode</span> 1 and mixed-<span class="hlt">mode</span> 1 and 2 loadings. Two bonded systems were studied: graphite/epoxy adherends bonded with EC 3445 and FM-300 adhesives. For each bonded system, two specimen types were tested: a double-cantilever-beam specimen for <span class="hlt">mode</span> 1 loading and a cracked-lapshear specimen for mixed-<span class="hlt">mode</span> 1 and 2 loading. In all specimens tested, failure occurred in the form of debond growth. Debonding always occurred in a cohesive manner with EC 3445 adhesive. The FM-300 adhesive debonded in a cohesive manner under mixed-<span class="hlt">mode</span> 1 and 2 loading, but in a cohesive, adhesive, or combined cohesive and adhesive manner under <span class="hlt">mode</span> 1 loading. Total strain-energy release rate appeared to be the driving parameter for debond growth under static and fatigue loadings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19850052525&hterms=pollen&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dpollen','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19850052525&hterms=pollen&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dpollen"><span>Does the ocean-atmosphere system have more than one stable <span class="hlt">mode</span> of operation?</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Broecker, W. S.; Peteet, D. M.; Rind, D.</p> <p>1985-01-01</p> <p>The climate record obtained from two long Greenland ice cores reveals several brief climate oscillations during glacial time. The most recent of these oscillations, also found in continental pollen records, has greatest impact in the area under the meteorological influence of the northern Atlantic, but none in the United States. This suggests that these oscillations are caused by fluctuations in the formation rate of deep <span class="hlt">water</span> in the northern Atlantic. As the present production of deep <span class="hlt">water</span> in this area is driven by an excess of evaporation over precipitation and continental runoff, atmospheric <span class="hlt">water</span> transport may be an important element in climate change. Changes in the production rate of deep <span class="hlt">water</span> in this sector of the ocean may push the climate system from one quasi-stable <span class="hlt">mode</span> of operation to another.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AIPC.1706c0003H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AIPC.1706c0003H"><span>Guided wave propagation in metallic and resin plates loaded with <span class="hlt">water</span> on single surface</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hayashi, Takahiro; Inoue, Daisuke</p> <p>2016-02-01</p> <p>Our previous papers reported dispersion curves for leaky Lamb waves in a <span class="hlt">water</span>-loaded plate and wave structures for several typical <span class="hlt">modes</span> including quasi-Scholte waves [1,2]. The calculations were carried out with a semi-analytical finite element (SAFE) method developed for leaky Lamb waves. This study presents SAFE calculations for transient guided waves including time-domain waveforms and animations of wave propagation in metallic and resin <span class="hlt">water</span>-loaded plates. The results show that non-dispersive and non-attenuated waves propagating along the interface between the fluid and the plate are expected for effective non-destructive evaluation of such fluid-loaded plates as storage tanks and transportation pipes. We calculated transient waves in both steel and polyvinyl chloride (PVC) plates loaded with <span class="hlt">water</span> on a single side and input dynamic loading from a point source on the other <span class="hlt">water</span>-free surface as typical examples of metallic and resin plates. For a steel plate, there exists a non-dispersive and non-attenuated <span class="hlt">mode</span>, called the quasi-Scholte wave, having an almost identical phase velocity to that of <span class="hlt">water</span>. The quasi-Scholte wave has superior generation efficiency in the low frequency range due to its broad energy distribution across the plate, whereas it is localized near the plate-<span class="hlt">water</span> interface at higher frequencies. This means that it has superior detectability of inner defects. For a PVC plate, plural non-attenuated <span class="hlt">modes</span> exist. One of the non-attenuated <span class="hlt">modes</span> similar to the A0 <span class="hlt">mode</span> of the Lamb wave in the form of a group velocity dispersion curve is promising for the non-destructive evaluation of the PVC plate because it provides prominent characteristics of generation efficiency and low dispersion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23188368','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23188368"><span>Adaptive frequency-domain equalization for the transmission of the fundamental <span class="hlt">mode</span> in a few-<span class="hlt">mode</span> fiber.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Bai, Neng; Xia, Cen; Li, Guifang</p> <p>2012-10-08</p> <p>We propose and experimentally demonstrate single-carrier adaptive frequency-domain equalization (SC-FDE) to mitigate multipath interference (MPI) for the transmission of the fundamental <span class="hlt">mode</span> in a few-<span class="hlt">mode</span> fiber. The FDE approach reduces computational complexity significantly compared to the time-domain equalization (TDE) approach while maintaining the same performance. Both FDE and TDE methods are evaluated by simulating long-haul fundamental-<span class="hlt">mode</span> transmission using a few-<span class="hlt">mode</span> fiber. For the fundamental <span class="hlt">mode</span> operation, the required tap length of the equalizer depends on the differential <span class="hlt">mode</span> group delay (DMGD) of a single span rather than DMGD of the entire link.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27410274','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27410274"><span>Discrimination of orbital angular momentum <span class="hlt">modes</span> of the terahertz vortex beam using a diffractive <span class="hlt">mode</span> transformer.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Changming; Wei, Xuli; Niu, Liting; Wang, Kejia; Yang, Zhengang; Liu, Jinsong</p> <p>2016-06-13</p> <p>We present an efficient method to discriminate orbital angular momentum (OAM) of the terahertz (THz) vortex beam using a diffractive <span class="hlt">mode</span> transformer. The <span class="hlt">mode</span> transformer performs a log-polar coordinate transformation of the input THz vortex beam, which consists of two 3D-printed diffractive elements. A following lens separates each transformed OAM <span class="hlt">mode</span> to a different lateral position in its focal plane. This method enables a simultaneous measurement over multiple OAM <span class="hlt">modes</span> of the THz vortex beam. We experimentally demonstrate the measurement of seven individual OAM <span class="hlt">modes</span> and two multiplexed OAM <span class="hlt">modes</span>, which is in good agreement with simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1034356','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1034356"><span>Dual <span class="hlt">Mode</span> Slotted Monopole Antenna</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-01-05</p> <p>of 15 DUAL <span class="hlt">MODE</span> SLOTTED MONOPOLE ANTENNA STATEMENT OF GOVERNMENT INTEREST [0001] The invention described herein may be manufactured and used by...to a dual <span class="hlt">mode</span> antenna having one <span class="hlt">mode</span> as a slotted cylinder antenna and another <span class="hlt">mode</span> as a monopole antenna . (2) Description of the Prior Art...0004] Slotted cylinder antennas are popular antennas for use in line of sight communications systems, especially where the carrier frequency exceeds</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20100028909','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20100028909"><span><span class="hlt">Mode</span> Tracker for <span class="hlt">Mode</span>-Hop-Free Operation of a Laser</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wysocki, Gerard; Tittel, Frank K.; Curl, Robert F.</p> <p>2010-01-01</p> <p>A <span class="hlt">mode</span>-tracking system that includes a <span class="hlt">mode</span>-controlling subsystem has been incorporated into an external-cavity (EC) quantum cascade laser that operates in a mid-infrared wavelength range. The <span class="hlt">mode</span>-tracking system makes it possible to perform <span class="hlt">mode</span>-hop-free wavelength scans, as needed for high-resolution spectroscopy and detection of trace gases. The laser includes a gain chip, a beam-collimating lens, and a diffraction grating. The grating is mounted on a platform, the position of which can be varied to effect independent control of the EC length and the grating angle. The position actuators include a piezoelectric stage for translation control and a motorized stage for coarse rotation control equipped with a piezoelectric actuator for fine rotation control. Together, these actuators enable control of the EC length over a range of about 90 m with a resolution of 0.9 nm, and control of the grating angle over a coarse-tuning range of +/-6.3deg and a fine-tuning range of +/-520 microrad with a resolution of 10 nrad. A mirror mounted on the platform with the grating assures always the same direction of the output laser beam.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26228144','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26228144"><span>BIOMECHANICS. Jumping on <span class="hlt">water</span>: Surface tension-dominated jumping of <span class="hlt">water</span> striders and robotic insects.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Koh, Je-Sung; Yang, Eunjin; Jung, Gwang-Pil; Jung, Sun-Pill; Son, Jae Hak; Lee, Sang-Im; Jablonski, Piotr G; Wood, Robert J; Kim, Ho-Young; Cho, Kyu-Jin</p> <p>2015-07-31</p> <p>Jumping on <span class="hlt">water</span> is a unique locomotion <span class="hlt">mode</span> found in semi-aquatic arthropods, such as <span class="hlt">water</span> striders. To reproduce this feat in a surface tension-dominant jumping robot, we elucidated the hydrodynamics involved and applied them to develop a bio-inspired impulsive mechanism that maximizes momentum transfer to <span class="hlt">water</span>. We found that <span class="hlt">water</span> striders rotate the curved tips of their legs inward at a relatively low descending velocity with a force just below that required to break the <span class="hlt">water</span> surface (144 millinewtons/meter). We built a 68-milligram at-scale jumping robotic insect and verified that it jumps on <span class="hlt">water</span> with maximum momentum transfer. The results suggest an understanding of the hydrodynamic phenomena used by semi-aquatic arthropods during <span class="hlt">water</span> jumping and prescribe a method for reproducing these capabilities in artificial systems. Copyright © 2015, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3821357','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3821357"><span>A Refractive Index Sensor Based on the Resonant Coupling to Cladding <span class="hlt">Modes</span> in a Fiber Loop</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Reyes, Mauricio; Monzón-Hernández, David; Martínez-Ríos, Alejandro; Silvestre, Enrique; Díez, Antonio; Cruz, José Luis; Andrés, Miguel V.</p> <p>2013-01-01</p> <p>We report an easy-to-build, compact, and low-cost optical fiber refractive index sensor. It consists of a single fiber loop whose transmission spectra exhibit a series of notches produced by the resonant coupling between the fundamental <span class="hlt">mode</span> and the cladding <span class="hlt">modes</span> in a uniformly bent fiber. The wavelength of the notches, distributed in a wavelength span from 1,400 to 1,700 nm, can be tuned by adjusting the diameter of the fiber loop and are sensitive to refractive index changes of the external medium. Sensitivities of 170 and 800 nm per refractive index unit for <span class="hlt">water</span> solutions and for the refractive index interval 1.40–1.442, respectively, are demonstrated. We estimate a long range resolution of 3 × 10−4 and a short range resolution of 2 × 10−5 for <span class="hlt">water</span> solutions. PMID:23979478</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990ElL....26.2112L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990ElL....26.2112L"><span>TM triple-<span class="hlt">mode</span> microwave filter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lai, S.-L.; Lin, W.-G.</p> <p>1990-12-01</p> <p>A novel realization of triple-<span class="hlt">mode</span> six-pole microwave filters that use only TM <span class="hlt">modes</span> is presented. The application involves TM triple degeneracies in cylindrical cavities using triple-<span class="hlt">mode</span> elliptic function filter synthesis. Experimental results are reported.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016OptCo.367..161H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016OptCo.367..161H"><span>A novel MUX/DEMUX based on few-<span class="hlt">mode</span> FBG for <span class="hlt">mode</span> division multiplexing system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Han, Yueyu; Hu, Guijun</p> <p>2016-05-01</p> <p>In this paper, a novel <span class="hlt">mode</span> multiplexer/demultiplexer (MUX/DEMUX) based on few-<span class="hlt">mode</span> fiber Bragg gratings (FBG) has been proposed. The principle of the MUX/DEMUX based on few-<span class="hlt">mode</span> FBG has been described in detail, and crosstalk of better than -20 dB is obtained experimentally. Then a 2×2 division multiplexing (MDM) system has been established with the MUX/DEMUX we proposed. The transmission experiment of 2×10 Gbps PRBS has been achieved successfully, which are carried by LP01 <span class="hlt">mode</span> and LP11 <span class="hlt">mode</span>, respectively. When the receiver sensitivity is greater than -14 dB m and -10 dB m, the BER can both reach 10-3 for B2B and 10 km transmission, respectively.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080006929','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080006929"><span><span class="hlt">Mode</span>-routed fiber-optic add-drop filter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moslehi, Behzad (Inventor); Black, Richard James (Inventor); Shaw, Herbert John (Inventor)</p> <p>2000-01-01</p> <p>New elements <span class="hlt">mode</span>-converting two-<span class="hlt">mode</span> grating and <span class="hlt">mode</span>-filtering two-<span class="hlt">mode</span> coupler are disclosed and used as elements in a system for communications, add-drop filtering, and strain sensing. Methods of fabrication for these new two-<span class="hlt">mode</span> gratings and <span class="hlt">mode</span>-filtering two-<span class="hlt">mode</span> couplers are also disclosed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005PhDT........75M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhDT........75M"><span>Parametric effects on pinch-off <span class="hlt">modes</span> in liquid/liquid jet systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Milosevic, Ilija N.</p> <p></p> <p>Many industries rely on liquid/liquid extraction systems, where jet pinch off occurs on a regular basis. Inherent short time and length scales make analytical and numerical simulation of the process very challenging. A main objective of this work was to document the details of various pinch-off <span class="hlt">modes</span> at different length scales using Laser Induced Fluorescence and Particle Image Velocimetry. A <span class="hlt">water</span> glycerine mixture was injected into ambient either silicone oil or 1-octanol. The resultant viscosity ratios, inner to outer fluid, were 1.6 and 2.8, respectively. Ohnesorge numbers were 0.013 for ambient silicone oil and 0.08 for ambient 1-octanol. Reynolds and Strouhal numbers ranged from 30 to 100 and 0.5 to 3.5, respectively. Decreasing the Strouhal number increased the number of drops formed per forcing. Increasing the Reynolds number suppressed satellite formation, and in some cases the number of drops decreased from two to one per cycle. Increasing the Ohnesorge number to 0.08 suppressed the pinch off yielding a longer jet with three-dimensional threads. At Ohnesorge number 0.013, increasing the forcing amplitude shortened the jet, and eventually led to a dripping <span class="hlt">mode</span>. High-resolution measurements of pinch-off angles were compared to results from similarity theory. Two <span class="hlt">modes</span> were investigated: drops breaking from the jet (jet/drop) and, one drop splitting into two (splitting drop). The jet/drop <span class="hlt">mode</span> angle measurements agreed with similarity predictions. The splitting drop <span class="hlt">mode</span> converged towards smaller angles. Scaling analysis showed that a Stokesian similarity regime applied for a neck radius of 6 microns or less. The smallest radius observed in experiments was 15 microns. Therefore, it is not known whether splitting drop <span class="hlt">mode</span> might still converge to same behavior.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27063089','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27063089"><span>Theory of psychological adaptive <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lehti, Juha</p> <p>2016-05-01</p> <p>When an individual is facing a stressor and normal stress-response mechanism cannot guarantee sufficient adaptation, special emotional states, adaptive <span class="hlt">modes</span>, are activated (for example a depressive reaction). Adaptive <span class="hlt">modes</span> are involuntary states of mind, they are of comprehensive nature, they interfere with normal functioning, and they cannot be repressed or controlled the same way as many emotions. Their transformational nature differentiates them from other emotional states. The object of the adaptive <span class="hlt">mode</span> is to optimize the problem-solving abilities according to the situation that has provoked the <span class="hlt">mode</span>. Cognitions and emotions during the adaptive <span class="hlt">mode</span> are different than in a normal mental state. These altered cognitions and emotional reactions guide the individual to use the correct coping skills in order to deal with the stressor. Successful adaptation will cause the adaptive <span class="hlt">mode</span> to fade off since the adaptive <span class="hlt">mode</span> is no longer necessary, and the process as a whole will lead to raised well-being. However, if the adaptation process is inadequate, then the transformation period is prolonged, and the adaptive <span class="hlt">mode</span> will turn into a dysfunctional state. Many psychiatric disorders are such maladaptive processes. The maladaptive processes can be turned into functional ones by using adaptive skills that are used in functional adaptive processes. Copyright © 2016 Elsevier Ltd. All rights reserved.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1329854-ecology-oriented-exploitation-mode-groundwater-resources-northern-foot-tianshan-mountain-china','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1329854-ecology-oriented-exploitation-mode-groundwater-resources-northern-foot-tianshan-mountain-china"><span>An ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources in the northern foot of Tianshan Mountain, China</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Shang, Haimin; Wang, Wenke; Dai, Zhenxue; ...</p> <p>2016-10-10</p> <p>In recent years, ecological degradation caused by irrational groundwater exploitation has been of growing concern in arid and semiarid regions. To address the groundwater-ecological issues, this paper proposes a groundwater-resource exploitation <span class="hlt">mode</span> to evaluate the tradeoff between groundwater development and ecological environment in the northern Tianshan Mountains, northwest China’s Xinjiang Uygur Autonomous Region. Field surveys and remote sensing studies were conducted to analyze the relation between the distribution of hydrological conditions and the occurrence of ecological types. The results show that there is a good correlation between groundwater depth and the supergene ecological type. Numerical simulations and ecological assessment modelsmore » were applied to develop an ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources. The <span class="hlt">mode</span> allows the groundwater levels in different zones to be regulated by optimizing groundwater exploitation <span class="hlt">modes</span>. The prediction results show that the supergene ecological quality will be better in 2020 and even more groundwater can be exploited in this <span class="hlt">mode</span>. This study provides guidance for regional groundwater management, especially in regions with an obvious <span class="hlt">water</span> scarcity.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1329854','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1329854"><span>An ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources in the northern foot of Tianshan Mountain, China</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>Shang, Haimin; Wang, Wenke; Dai, Zhenxue</p> <p></p> <p>In recent years, ecological degradation caused by irrational groundwater exploitation has been of growing concern in arid and semiarid regions. To address the groundwater-ecological issues, this paper proposes a groundwater-resource exploitation <span class="hlt">mode</span> to evaluate the tradeoff between groundwater development and ecological environment in the northern Tianshan Mountains, northwest China’s Xinjiang Uygur Autonomous Region. Field surveys and remote sensing studies were conducted to analyze the relation between the distribution of hydrological conditions and the occurrence of ecological types. The results show that there is a good correlation between groundwater depth and the supergene ecological type. Numerical simulations and ecological assessment modelsmore » were applied to develop an ecology-oriented exploitation <span class="hlt">mode</span> of groundwater resources. The <span class="hlt">mode</span> allows the groundwater levels in different zones to be regulated by optimizing groundwater exploitation <span class="hlt">modes</span>. The prediction results show that the supergene ecological quality will be better in 2020 and even more groundwater can be exploited in this <span class="hlt">mode</span>. This study provides guidance for regional groundwater management, especially in regions with an obvious <span class="hlt">water</span> scarcity.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..301a2137L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..301a2137L"><span>The Design of an Autonomous Underwater Vehicle for <span class="hlt">Water</span> Quality Monitoring</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Yulong; Liu, Rong; Liu, Shujin</p> <p>2018-01-01</p> <p>This paper describes the development of a civilian-used autonomous underwater vehicle (AUV) for <span class="hlt">water</span> quality monitoring at reservoirs and watercourses that can obtain realtime visual and locational information. The mechanical design was completed with CAD software Solidworks. Four thrusters—two horizontal and two vertical—on board enable the vehicle to surge, heave, yaw, and pitch. A specialized <span class="hlt">water</span> sample collection compartment is designed to perform <span class="hlt">water</span> collection at target locations. The vehicle has a central controller—STM32—and a sub-coordinate controller—Arduino MEGA 2560—that coordinates multiple sensors including an inertial sensor, ultrasonic sensors, etc. Global Navigation Satellite System (GNSS) and the inertial sensor enable the vehicle’s localization. Remote operators monitor and control the vehicle via a host computer system. Operators choose either semi-autonomous <span class="hlt">mode</span> in which they set target locations or manual <span class="hlt">mode</span>. The experimental results show that the vehicle is able to perform well in either <span class="hlt">mode</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRA..121.2755C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRA..121.2755C"><span>Two-dimensional numerical simulation of O-<span class="hlt">mode</span> to Z-<span class="hlt">mode</span> conversion in the ionosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cannon, P. D.; Honary, F.; Borisov, N.</p> <p>2016-03-01</p> <p>Experiments in the illumination of the F region of the ionosphere via radio frequency waves polarized in the ordinary <span class="hlt">mode</span> (O-<span class="hlt">mode</span>) have revealed that the magnitude of artificial heating-induced effects depends strongly on the inclination angle of the pump beam, with a greater modification to the plasma observed when the heating beam is directed close to or along the magnetic zenith direction. Numerical simulations performed using a recently developed finite-difference time-domain (FDTD) code are used to investigate the contribution of the O-<span class="hlt">mode</span> to Z-<span class="hlt">mode</span> conversion process to this effect. The aspect angle dependence and angular size of the radio window for which conversion of an O-<span class="hlt">mode</span> pump wave to the Z-<span class="hlt">mode</span> occurs is simulated for a variety of plasma density profiles including 2-D linear gradients representative of large-scale plasma depletions, density-depleted plasma ducts, and periodic field-aligned irregularities. The angular shape of the conversion window is found to be strongly influenced by the background plasma profile. If the Z-<span class="hlt">mode</span> wave is reflected, it can propagate back toward the O-<span class="hlt">mode</span> reflection region leading to resonant enhancement of the electric field in this region. Simulation results presented in this paper demonstrate that this process can make a significant contribution to the magnitude of electron density depletion and temperature enhancement around the resonance height and contributes to a strong dependence of the magnitude of plasma perturbation with the direction of the pump wave.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004ApOpt..43.2337H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004ApOpt..43.2337H"><span><span class="hlt">Mode</span> Behavior in Ultralarge Ring Lasers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hurst, Robert B.; Dunn, Robert W.; Schreiber, K. Ulrich; Thirkettle, Robert J.; MacDonald, Graeme K.</p> <p>2004-04-01</p> <p>Contrary to expectations based on <span class="hlt">mode</span> spacing, single-<span class="hlt">mode</span> operation in very large He-Ne ring lasers may be achieved at intracavity power levels up to ~0.15 times the saturation intensity for the He-Ne transition. Homogeneous line broadening at a high total gas pressure of 4-6 Torr allows a single-peaked gain profile that suppresses closely spaced multiple <span class="hlt">modes</span>. At startup, decay of initial multiple <span class="hlt">modes</span> may take tens of seconds. The single remaining <span class="hlt">mode</span> in each direction persists metastably as the cavity is detuned by many times the <span class="hlt">mode</span> frequency spacing. A theoretical explanation requires the gain profile to be concave down and to satisfy an inequality related to slope and saturation at the operating frequency. Calculated metastable frequency ranges are greater than 150 MHz at 6 Torr and depend strongly on pressure. Examples of unusual stable <span class="hlt">mode</span> configurations are shown, with differently numbered <span class="hlt">modes</span> in the two directions and with multiple <span class="hlt">modes</span> at a spacing of ~100 MHz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15098837','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15098837"><span><span class="hlt">Mode</span> behavior in ultralarge ring lasers.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hurst, Robert B; Dunn, Robert W; Schreiber, K Ulrich; Thirkettle, Robert J; MacDonald, Graeme K</p> <p>2004-04-10</p> <p>Contrary to expectations based on <span class="hlt">mode</span> spacing, single-<span class="hlt">mode</span> operation in very large He-Ne ring lasers may be achieved at intracavity power levels up to approximately0.15 times the saturation intensity for the He-Ne transition. Homogeneous line broadening at a high total gas pressure of 4-6 Torr allows a single-peaked gain profile that suppresses closely spaced multiple <span class="hlt">modes</span>. At startup, decay of initial multiple <span class="hlt">modes</span> may take tens of seconds. The single remaining <span class="hlt">mode</span> in each direction persists metastably as the cavity is detuned by many times the <span class="hlt">mode</span> frequency spacing. A theoretical explanation requires the gain profile to be concave down and to satisfy an inequality related to slope and saturation at the operating frequency. Calculated metastable frequency ranges are > 150 MHz at 6 Torr and depend strongly on pressure. Examples of unusual stable <span class="hlt">mode</span> configurations are shown, with differently numbered <span class="hlt">modes</span> in the two directions and with multiple <span class="hlt">modes</span> at a spacing of approximately 100 MHz.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28717132','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28717132"><span>Fiber cavities with integrated <span class="hlt">mode</span> matching optics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gulati, Gurpreet Kaur; Takahashi, Hiroki; Podoliak, Nina; Horak, Peter; Keller, Matthias</p> <p>2017-07-17</p> <p>In fiber based Fabry-Pérot Cavities (FFPCs), limited spatial <span class="hlt">mode</span> matching between the cavity <span class="hlt">mode</span> and input/output <span class="hlt">modes</span> has been the main hindrance for many applications. We have demonstrated a versatile <span class="hlt">mode</span> matching method for FFPCs. Our novel design employs an assembly of a graded-index and large core multimode fiber directly spliced to a single <span class="hlt">mode</span> fiber. This all-fiber assembly transforms the propagating <span class="hlt">mode</span> of the single <span class="hlt">mode</span> fiber to match with the <span class="hlt">mode</span> of a FFPC. As a result, we have measured a <span class="hlt">mode</span> matching of 90% for a cavity length of ~400 μm. This is a significant improvement compared to conventional FFPCs coupled with just a single <span class="hlt">mode</span> fiber, especially at long cavity lengths. Adjusting the parameters of the assembly, the fundamental cavity <span class="hlt">mode</span> can be matched with the <span class="hlt">mode</span> of almost any single <span class="hlt">mode</span> fiber, making this approach highly versatile and integrable.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25918549','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25918549"><span>Non-invasive assessment of leaf <span class="hlt">water</span> status using a dual-<span class="hlt">mode</span> microwave resonator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dadshani, Said; Kurakin, Andriy; Amanov, Shukhrat; Hein, Benedikt; Rongen, Heinz; Cranstone, Steve; Blievernicht, Ulrich; Menzel, Elmar; Léon, Jens; Klein, Norbert; Ballvora, Agim</p> <p>2015-01-01</p> <p>The <span class="hlt">water</span> status in plant leaves is a good indicator for the <span class="hlt">water</span> status in the whole plant revealing stress if the <span class="hlt">water</span> supply is reduced. The analysis of dynamic aspects of <span class="hlt">water</span> availability in plant tissues provides useful information for the understanding of the mechanistic basis of drought stress tolerance, which may lead to improved plant breeding and management practices. The determination of the <span class="hlt">water</span> content in plant tissues during plant development has been a challenge and is currently feasible based on destructive analysis only. We present here the application of a non-invasive quantitative method to determine the volumetric <span class="hlt">water</span> content of leaves and the ionic conductivity of the leaf juice from non-invasive microwave measurements at two different frequencies by one sensor device. A semi-open microwave cavity loaded with a ceramic dielectric resonator and a metallic lumped-element capacitor- and inductor structure was employed for non-invasive microwave measurements at 150 MHz and 2.4 Gigahertz on potato, maize, canola and wheat leaves. Three leaves detached from each plant were chosen, representing three developmental stages being representative for tissue of various age. Clear correlations between the leaf- induced resonance frequency shifts and changes of the inverse resonator quality factor at 2.4 GHz to the gravimetrically determined drying status of the leaves were found. Moreover, the ionic conductivity of Maize leaves, as determined from the ratio of the inverse quality factor and frequency shift at 150 MHz by use of cavity perturbation theory, was found to be in good agreement with direct measurements on plant juice. In conjunction with a compact battery- powered circuit board- microwave electronic module and a user-friendly software interface, this method enables rapid in-vivo <span class="hlt">water</span> amount assessment of plants by a handheld device for potential use in the field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23388946','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23388946"><span>Splice loss requirements in multi-<span class="hlt">mode</span> fiber <span class="hlt">mode</span>-division-multiplex transmission links.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Warm, Stefan; Petermann, Klaus</p> <p>2013-01-14</p> <p>We investigate numerically the influence of fiber splices and fiber connectors to the statistics of <span class="hlt">mode</span> dependent loss (MDL) and multiple-input multiple-output (MIMO) outage capacity in <span class="hlt">mode</span> multiplexed multi-<span class="hlt">mode</span> fiber links. Our results indicate required splice losses much lower than currently feasible to achieve a reasonable outage capacity in long-haul transmission systems. Splice losses as low as 0.03dB may effectively lead to an outage of MIMO channels after only a few hundred kilometers transmission length. In a first approximation, the relative capacity solely depends on the accumulated splice loss and should be less than ≈ 2dB to ensure a relative capacity of 90%. We also show that discrete <span class="hlt">mode</span> permutation (mixing) within the transmission line may effectively increase the maximum transmission distance by a factor of 5 for conventional splice losses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6012553-modal-split-model-considering-carpool-mode','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6012553-modal-split-model-considering-carpool-mode"><span>Modal split model considering carpool <span class="hlt">mode</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>Lyles, R.W.</p> <p>1979-03-01</p> <p>Modal split remains a primary concern of transportation planners as the state-of-the art has developed from diversion curves to behavioral models. The approach taken here is to formulate the <span class="hlt">mode</span>-choice decision for the work trip as a linear combination of real and perceived characteristics of the <span class="hlt">modes</span> considered. The logit formulation is used with three <span class="hlt">modes</span> being considered: two automobile <span class="hlt">modes</span> (drive-alone and carpool) and a public transit <span class="hlt">mode</span> (bus). The final model provides insight into which factors are important in travel decisions among these three <span class="hlt">modes</span> and the importance of examining traveler's perceptions of the differences among <span class="hlt">modes</span> relativemore » to actual measurable differences.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JChPh.134d4905M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JChPh.134d4905M"><span>Structure and dynamics of <span class="hlt">water</span> in mixed solutions including laponite and PEO</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Morikubo, Satoshi; Sekine, Yurina; Ikeda-Fukazawa, Tomoko</p> <p>2011-01-01</p> <p>To investigate the structure and dynamics of <span class="hlt">water</span> in mixed solutions including laponite clay particles and poly(ethylene oxide) (PEO), we measured the Raman spectra of the mixed solutions in the temperature range 283-313 K. The results show that the vibrational energies of the O-H stretching <span class="hlt">modes</span> in the mixed solutions depend on the <span class="hlt">water</span> content and temperature. The energy shifts of the O-H stretching <span class="hlt">modes</span> are attributed to changes in the <span class="hlt">water</span> structure. By applying a structural model of bulk <span class="hlt">water</span> to the spectra in the O-H stretching region, the local structures of <span class="hlt">water</span> in the solutions were analyzed. The result shows that the formation probability of hydrogen bonds in the solutions decreases as the <span class="hlt">water</span> content decreases. Laponite and PEO have effects to disrupt the network structure of hydrogen bonds between <span class="hlt">water</span> molecules. Further, it was found that laponite and PEO cause increase in the strength of hydrogen bonds of surrounding <span class="hlt">water</span>,although the strength of the hydrogen bonds increases with the order <span class="hlt">water</span>-laponite < <span class="hlt">water-water</span> < <span class="hlt">water</span>-PEO. It is concluded that <span class="hlt">water</span> in laponite-PEO mixed solutions has a less-networked structure with strong hydrogen bonds compared with bulk <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1441318-generalization-soft-phonon-modes','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1441318-generalization-soft-phonon-modes"><span>Generalization of soft phonon <span class="hlt">modes</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>Rudin, Sven P.</p> <p></p> <p>Soft phonon <span class="hlt">modes</span> describe a collective movement of atoms that transform a higher-symmetry crystal structure into a lower-symmetry crystal structure. Such structural transformations occur at finite temperatures, where the phonons (i.e., the low-temperature vibrational <span class="hlt">modes</span>) and the static perfect crystal structures provide an incomplete picture of the dynamics. In this paper, principal vibrational <span class="hlt">modes</span> (PVMs) are introduced as descriptors of the dynamics of a material system withmore » $N$ atoms. The PVMs represent the independent collective movements of the atoms at a given temperature. Molecular dynamics (MD) simulations, here in the form of quantum MD using density functional theory calculations, provide both the data describing the atomic motion and the data used to construct the PVMs. The leading <span class="hlt">mode</span>, $${\\mathrm{PVM}}_{0}$$, represents the $3N$-dimensional direction in which the system moves with greatest amplitude. For structural phase transitions, $${\\mathrm{PVM}}_{0}$$ serves as a generalization of soft phonon <span class="hlt">modes</span>. At low temperatures, $${\\mathrm{PVM}}_{0}$$ reproduces the soft phonon <span class="hlt">mode</span> in systems where one phonon dominates the phase transformation. In general, multiple phonon <span class="hlt">modes</span> combine to describe a transformation, in which case $${\\mathrm{PVM}}_{0}$$ culls these phonon <span class="hlt">modes</span>. Moreover, while soft phonon <span class="hlt">modes</span> arise in the higher-symmetry crystal structure, $${\\mathrm{PVM}}_{0}$$ can be equally well calculated on either side of the structural phase transition. Finally, two applications demonstrate these properties: first, transitions into and out of bcc titanium, and, second, the two crystal structures proposed for the $${\\beta}$$ phase of uranium, the higher-symmetry structure of which stabilizes with temperature.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1441318-generalization-soft-phonon-modes','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1441318-generalization-soft-phonon-modes"><span>Generalization of soft phonon <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Rudin, Sven P.</p> <p>2018-04-27</p> <p>Soft phonon <span class="hlt">modes</span> describe a collective movement of atoms that transform a higher-symmetry crystal structure into a lower-symmetry crystal structure. Such structural transformations occur at finite temperatures, where the phonons (i.e., the low-temperature vibrational <span class="hlt">modes</span>) and the static perfect crystal structures provide an incomplete picture of the dynamics. In this paper, principal vibrational <span class="hlt">modes</span> (PVMs) are introduced as descriptors of the dynamics of a material system withmore » $N$ atoms. The PVMs represent the independent collective movements of the atoms at a given temperature. Molecular dynamics (MD) simulations, here in the form of quantum MD using density functional theory calculations, provide both the data describing the atomic motion and the data used to construct the PVMs. The leading <span class="hlt">mode</span>, $${\\mathrm{PVM}}_{0}$$, represents the $3N$-dimensional direction in which the system moves with greatest amplitude. For structural phase transitions, $${\\mathrm{PVM}}_{0}$$ serves as a generalization of soft phonon <span class="hlt">modes</span>. At low temperatures, $${\\mathrm{PVM}}_{0}$$ reproduces the soft phonon <span class="hlt">mode</span> in systems where one phonon dominates the phase transformation. In general, multiple phonon <span class="hlt">modes</span> combine to describe a transformation, in which case $${\\mathrm{PVM}}_{0}$$ culls these phonon <span class="hlt">modes</span>. Moreover, while soft phonon <span class="hlt">modes</span> arise in the higher-symmetry crystal structure, $${\\mathrm{PVM}}_{0}$$ can be equally well calculated on either side of the structural phase transition. Finally, two applications demonstrate these properties: first, transitions into and out of bcc titanium, and, second, the two crystal structures proposed for the $${\\beta}$$ phase of uranium, the higher-symmetry structure of which stabilizes with temperature.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvB..97m4114R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvB..97m4114R"><span>Generalization of soft phonon <span class="hlt">modes</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rudin, Sven P.</p> <p>2018-04-01</p> <p>Soft phonon <span class="hlt">modes</span> describe a collective movement of atoms that transform a higher-symmetry crystal structure into a lower-symmetry crystal structure. Such structural transformations occur at finite temperatures, where the phonons (i.e., the low-temperature vibrational <span class="hlt">modes</span>) and the static perfect crystal structures provide an incomplete picture of the dynamics. Here, principal vibrational <span class="hlt">modes</span> (PVMs) are introduced as descriptors of the dynamics of a material system with N atoms. The PVMs represent the independent collective movements of the atoms at a given temperature. Molecular dynamics (MD) simulations, here in the form of quantum MD using density functional theory calculations, provide both the data describing the atomic motion and the data used to construct the PVMs. The leading <span class="hlt">mode</span>, PVM0, represents the 3 N -dimensional direction in which the system moves with greatest amplitude. For structural phase transitions, PVM0 serves as a generalization of soft phonon <span class="hlt">modes</span>. At low temperatures, PVM0 reproduces the soft phonon <span class="hlt">mode</span> in systems where one phonon dominates the phase transformation. In general, multiple phonon <span class="hlt">modes</span> combine to describe a transformation, in which case PVM0 culls these phonon <span class="hlt">modes</span>. Moreover, while soft phonon <span class="hlt">modes</span> arise in the higher-symmetry crystal structure, PVM0 can be equally well calculated on either side of the structural phase transition. Two applications demonstrate these properties: first, transitions into and out of bcc titanium, and, second, the two crystal structures proposed for the β phase of uranium, the higher-symmetry structure of which stabilizes with temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5859740','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5859740"><span><span class="hlt">Mode</span> Equivalence of Health Indicators Between Data Collection <span class="hlt">Modes</span> and Mixed-<span class="hlt">Mode</span> Survey Designs in Population-Based Health Interview Surveys for Children and Adolescents: Methodological Study</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hoffmann, Robert; Houben, Robin; Krause, Laura; Kamtsiuris, Panagiotis; Gößwald, Antje</p> <p>2018-01-01</p> <p>Background The implementation of an Internet option in an existing public health interview survey using a mixed-<span class="hlt">mode</span> design is attractive because of lower costs and faster data availability. Additionally, mixed-<span class="hlt">mode</span> surveys can increase response rates and improve sample composition. However, mixed-<span class="hlt">mode</span> designs can increase the risk of measurement error (<span class="hlt">mode</span> effects). Objective This study aimed to determine whether the prevalence rates or mean values of self- and parent-reported health indicators for children and adolescents aged 0-17 years differ between self-administered paper-based questionnaires (SAQ-paper) and self-administered Web-based questionnaires (SAQ-Web), as well as between a single-<span class="hlt">mode</span> control group and different mixed-<span class="hlt">mode</span> groups. Methods Data were collected for a methodological pilot of the third wave of the "German Health Interview and Examination Survey for Children and Adolescents". Questionnaires were completed by parents or adolescents. A population-based sample of 11,140 children and adolescents aged 0-17 years was randomly allocated to 4 survey designs—a single-<span class="hlt">mode</span> control group with paper-and-pencil questionnaires only (n=970 parents, n=343 adolescents)—and 3 mixed-<span class="hlt">mode</span> designs, all of which offered Web-based questionnaire options. In the concurrent mixed-<span class="hlt">mode</span> design, both questionnaires were offered at the same time (n=946 parents, n=290 adolescents); in the sequential mixed-<span class="hlt">mode</span> design, the SAQ-Web was sent first, followed by the paper questionnaire along with a reminder (n=854 parents, n=269 adolescents); and in the preselect mixed-<span class="hlt">mode</span> design, both options were offered and the respondents were asked to request the desired type of questionnaire (n=698 parents, n=292 adolescents). In total, 3468 questionnaires of parents of children aged 0-17 years (SAQ-Web: n=708; SAQ-paper: n=2760) and 1194 questionnaires of adolescents aged 11-17 years (SAQ-Web: n=299; SAQ-paper: n=895) were analyzed. Sociodemographic characteristics and a broad</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApPhL.111b1603L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApPhL.111b1603L"><span><span class="hlt">Water</span> droplet evaporation from sticky superhydrophobic surfaces</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Moonchan; Kim, Wuseok; Lee, Sanghee; Baek, Seunghyeon; Yong, Kijung; Jeon, Sangmin</p> <p>2017-07-01</p> <p>The evaporation dynamics of <span class="hlt">water</span> from sticky superhydrophobic surfaces was investigated using a quartz crystal microresonator and an optical microscope. Anodic aluminum oxide (AAO) layers with different pore sizes were directly fabricated onto quartz crystal substrates and hydrophobized via chemical modification. The resulting AAO layers exhibited hydrophobic or superhydrophobic characteristics with strong adhesion to <span class="hlt">water</span> due to the presence of sealed air pockets inside the nanopores. After placing a <span class="hlt">water</span> droplet on the AAO membranes, variations in the resonance frequency and Q-factor were measured throughout the evaporation process, which were related to changes in mass and viscous damping, respectively. It was found that droplet evaporation from a sticky superhydrophobic surface followed a constant contact radius (CCR) <span class="hlt">mode</span> in the early stage of evaporation and a combination of CCR and constant contact angle <span class="hlt">modes</span> without a Cassie-Wenzel transition in the final stage. Furthermore, AAO membranes with larger pore sizes exhibited longer evaporation times, which were attributed to evaporative cooling at the droplet interface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990084057&hterms=sliding+mode+control&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsliding%2Bmode%2Bcontrol','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990084057&hterms=sliding+mode+control&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dsliding%2Bmode%2Bcontrol"><span>Sliding <span class="hlt">Mode</span> Control of the X-33 Vehicle in Launch <span class="hlt">Mode</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shtessel, Yuri; Jackson, Mark; Hall, Charles; Krupp, Don; Hendrix, N. Douglas</p> <p>1998-01-01</p> <p>The "nested" structure of the control system for the X33 vehicle in launch <span class="hlt">mode</span> is developed. Employing backstopping concepts, the outer loop (guidance) and the Inner loop (rates) continuous sliding <span class="hlt">mode</span> controllers are designed. Simulations of the 3-DOF model of the X33 launch vehicle showed an accurate, robust, de-coupled tracking performance.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17590259','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17590259"><span>Cluster analysis and quality assessment of logged <span class="hlt">water</span> at an irrigation project, eastern Saudi Arabia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hussain, Mahbub; Ahmed, Syed Munaf; Abderrahman, Walid</p> <p>2008-01-01</p> <p>A multivariate statistical technique, cluster analysis, was used to assess the logged surface <span class="hlt">water</span> quality at an irrigation project at Al-Fadhley, Eastern Province, Saudi Arabia. The principal idea behind using the technique was to utilize all available hydrochemical variables in the quality assessment including trace elements and other ions which are not considered in conventional techniques for <span class="hlt">water</span> quality assessments like Stiff and Piper diagrams. Furthermore, the area belongs to an irrigation project where <span class="hlt">water</span> contamination associated with the use of fertilizers, insecticides and pesticides is expected. This quality assessment study was carried out on a total of 34 surface/logged <span class="hlt">water</span> samples. To gain a greater insight in terms of the seasonal variation of <span class="hlt">water</span> quality, 17 samples were collected from both summer and winter seasons. The collected samples were analyzed for a total of 23 <span class="hlt">water</span> quality parameters including pH, TDS, conductivity, alkalinity, sulfate, chloride, bicarbonate, nitrate, phosphate, bromide, fluoride, calcium, magnesium, sodium, potassium, arsenic, boron, copper, cobalt, iron, lithium, manganese, molybdenum, nickel, selenium, mercury and zinc. Cluster analysis in both Q and R <span class="hlt">modes</span> was used. Q-<span class="hlt">mode</span> analysis resulted in three distinct <span class="hlt">water</span> types for both the summer and winter seasons. Q-<span class="hlt">mode</span> analysis also showed the spatial as well as temporal variation in <span class="hlt">water</span> quality. R-<span class="hlt">mode</span> cluster analysis led to the conclusion that there are two major sources of contamination for the surface/shallow groundwater in the area: fertilizers, micronutrients, pesticides, and insecticides used in agricultural activities, and non-point natural sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=311249','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=311249"><span>Evaluation of neural network <span class="hlt">modeing</span> to calculate well-<span class="hlt">watered</span> leaf temperature of wine grape</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>Mild to moderate <span class="hlt">water</span> stress is desirable in wine grape for controlling vine vigor and optimizing fruit yield and quality, but precision irrigation management is hindered by the lack of a reliable method to easily quantify and monitor vine <span class="hlt">water</span> status. The crop <span class="hlt">water</span> stress index (CWSI) that effec...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AcSpA.188...26F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AcSpA.188...26F"><span>Anharmonic vibrational spectra and <span class="hlt">mode-mode</span> couplings analysis of 2-aminopyridine</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Faizan, Mohd; Alam, Mohammad Jane; Afroz, Ziya; Bhat, Sheeraz Ahmad; Ahmad, Shabbir</p> <p>2018-01-01</p> <p>Vibrational spectra of 2-aminopyridine (2AP) have been analyzed using the vibrational self-consistence field theory (VSCF), correlated corrected vibrational self-consistence field theory (CC-VSCF) and vibrational perturbation theory (VPT2) at B3LYP/6-311G(d,p) framework. The <span class="hlt">mode-mode</span> couplings affect the vibrational frequencies and intensities. The coupling integrals between pairs of normal <span class="hlt">modes</span> have been obtained on the basis of quartic force field (2MR-QFF) approximation. The overtone and combination bands are also assigned in the FTIR spectrum with the help of anharmonic calculation at VPT2 method. A statistical analysis of deviations shows that estimated anharmonic frequencies are closer to the experiment over harmonic approximation. Furthermore, the anharmonic correction has also been carried out for the dimeric structure of 2AP. The fundamental vibration bands have been assigned on the basis of potential energy distribution (PED) and visual look over the animated <span class="hlt">modes</span>. Other important molecular properties such as frontier molecular orbitals and molecular electrostatics potential mapping have also been analyzed.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_22 --> <div id="page_23" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li class="active"><span>23</span></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>25</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="441"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MNRAS.469.4034O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MNRAS.469.4034O"><span>Broad-band, radio spectro-polarimetric study of 100 radiative-<span class="hlt">mode</span> and jet-<span class="hlt">mode</span> AGN</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Sullivan, S. P.; Purcell, C. R.; Anderson, C. S.; Farnes, J. S.; Sun, X. H.; Gaensler, B. M.</p> <p>2017-08-01</p> <p>We present the results from a broad-band (1 to 3 GHz), spectro-polarimetry study of the integrated emission from 100 extragalactic radio sources with the Australia Telescope Compact Array, selected to be highly linearly polarized at 1.4 GHz. We use a general-purpose, polarization model-fitting procedure that describes the Faraday rotation measure (RM) and intrinsic polarization structure of up to three distinct polarized emission regions or `RM components' of a source. Overall, 37 per cent/52 per cent/11 per cent of sources are best fitted by one/two/three RM components. However, these fractions are dependent on the signal-to-noise ratio (S/N) in polarization (more RM components more likely at higher S/N). In general, our analysis shows that sources with high integrated degrees of polarization at 1.4 GHz have low Faraday depolarization, are typically dominated by a single RM component, have a steep spectral index and have a high intrinsic degree of polarization. After classifying our sample into radiative-<span class="hlt">mode</span> and jet-<span class="hlt">mode</span> AGN, we find no significant difference between the Faraday rotation or Faraday depolarization properties of jet-<span class="hlt">mode</span> and radiative-<span class="hlt">mode</span> AGN. However, there is a statistically significant difference in the intrinsic degree of polarization between the two types, with the jet-<span class="hlt">mode</span> sources having more intrinsically ordered magnetic field structures than the radiative-<span class="hlt">mode</span> sources. We also find a preferred perpendicular orientation of the intrinsic magnetic field structure of jet-<span class="hlt">mode</span> AGN with respect to the jet direction, while no clear preference is found for the radiative-<span class="hlt">mode</span> sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9753E..0TZ','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9753E..0TZ"><span>Analysis of multi-<span class="hlt">mode</span> to single-<span class="hlt">mode</span> conversion at 635 nm and 1550 nm</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zamora, Vanessa; Bogatzki, Angelina; Arndt-Staufenbiel, Norbert; Hofmann, Jens; Schröder, Henning</p> <p>2016-03-01</p> <p>We propose two low-cost and robust optical fiber systems based on the photonic lantern (PL) technology for operating at 635 nm and 1550 nm. The PL is an emerging technology that couples light from a multi-<span class="hlt">mode</span> (MM) fiber to several single-<span class="hlt">mode</span> (SM) fibers via a low-loss adiabatic transition. This bundle of SM fibers is observed as a MM fiber system whose spatial <span class="hlt">modes</span> are the degenerate supermodes of the bundle. The adiabatic transition allows that those supermodes evolve into the <span class="hlt">modes</span> of the MM fiber. Simulations of the MM fiber end structure and its taper transition have been performed via functional <span class="hlt">mode</span> solver tools in order to understand the modal evolution in PLs. The modelled design consists of 7 SM fibers inserted into a low-index capillary. The material and geometry of the PLs are chosen such that the supermodes match to the spatial <span class="hlt">modes</span> of the desired step-index MM fiber in a moderate loss transmission. The dispersion of materials is also considered. These parameters are studied in two PL systems in order to reach a spectral transmission from 450 nm to 1600 nm. Additionally, an analysis of the geometry and losses due to the mismatching of <span class="hlt">modes</span> is presented. PLs are typically used in the fields of astrophotonics and space photonics. Recently, they are demonstrated as <span class="hlt">mode</span> converters in telecommunications, especially focusing on spatial division multiplexing. In this study, we show the use of PLs as a promising interconnecting tool for the development of miniaturized spectrometers operating in a broad wavelength range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22648878-su-dosimetric-characteristics-cine-acquisition-mode-si-epid','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22648878-su-dosimetric-characteristics-cine-acquisition-mode-si-epid"><span>SU-F-T-263: Dosimetric Characteristics of the Cine Acquisition <span class="hlt">Mode</span> of An A-Si EPID</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>Bawazeer, O; Deb, P; Sarasanandarajah, S</p> <p>2016-06-15</p> <p>Purpose: To investigate the dosimetric characteristics of Varian a-Si-500 electronic portal imaging device (EPID) operated in cine <span class="hlt">mode</span> particularly considering linearity with delivered dose, dose rate, field size, phantom thickness, MLC speed and common IMRT fields. Methods: The EPID that attached to a Varian Clinac 21iX linear accelerator, was irradiated with 6 and 18 MV using 600 MU/min. Image acquisition is controlled by the IAS3 software, Trigger delay was 6 ms, BeamOnDelay and FrameStartDelay were zero. Different frame rates were utilized. Cine <span class="hlt">mode</span> response was calculated using MATLAB as summation of mean pixel values in a region of interest ofmore » the acquired images. The performance of cine <span class="hlt">mode</span> was compared to integrated <span class="hlt">mode</span> and dose measurements in <span class="hlt">water</span> using CC13 ionization chamber. Results: Figure1 illustrates that cine <span class="hlt">mode</span> has nonlinear response for small MU, when delivering 10 MU was about 0.5 and 0.64 for 6 and 18 MV respectively. This is because the missing acquired images that were calculated around four images missing in each delivery. With the increase MU the response became linear and comparable with integrated <span class="hlt">mode</span> and ionization chamber within 2%. Figure 2 shows that cine <span class="hlt">mode</span> has comparable response with integrated <span class="hlt">mode</span> and ionization chamber within 2% with changing dose rate for 10 MU delivered. This indicates that the dose rate change has no effect on nonlinearity of cine <span class="hlt">mode</span> response. Except nonlinearity, cine <span class="hlt">mode</span> is well matched to integrated <span class="hlt">mode</span> response within 2% for field size, phantom thickness, MLC speed dependences. Conclusion: Cine <span class="hlt">mode</span> has similar dosimetric characteristics to integrated <span class="hlt">mode</span> with open and IMRT fields, and the main limitation with cine <span class="hlt">mode</span> is missing images. Therefore, the calibration of EPID images with this <span class="hlt">mode</span> should be run with large MU, and when IMRT verification field has low MU, the correction for missing images are required.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1234227','DOE-PATENT-XML'); return false;" href="https://www.osti.gov/servlets/purl/1234227"><span>Path planning during combustion <span class="hlt">mode</span> switch</span></a></p> <p><a target="_blank" href="http://www.osti.gov/doepatents">DOEpatents</a></p> <p>Jiang, Li; Ravi, Nikhil</p> <p>2015-12-29</p> <p>Systems and methods are provided for transitioning between a first combustion <span class="hlt">mode</span> and a second combustion <span class="hlt">mode</span> in an internal combustion engine. A current operating point of the engine is identified and a target operating point for the internal combustion engine in the second combustion <span class="hlt">mode</span> is also determined. A predefined optimized transition operating point is selected from memory. While operating in the first combustion <span class="hlt">mode</span>, one or more engine actuator settings are adjusted to cause the operating point of the internal combustion engine to approach the selected optimized transition operating point. When the engine is operating at the selected optimized transition operating point, the combustion <span class="hlt">mode</span> is switched from the first combustion <span class="hlt">mode</span> to the second combustion <span class="hlt">mode</span>. While operating in the second combustion <span class="hlt">mode</span>, one or more engine actuator settings are adjusted to cause the operating point of the internal combustion to approach the target operating point.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/EJ1082802.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/EJ1082802.pdf"><span>ACCA College English Teaching <span class="hlt">Mode</span></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>Ding, Renlun</p> <p>2008-01-01</p> <p>This paper elucidates a new college English teaching <span class="hlt">mode</span>--"ACCA" (Autonomous Cooperative Class-teaching All-round College English Teaching <span class="hlt">Mode</span>). Integrated theories such as autonomous learning and cooperative learning into one teaching <span class="hlt">mode</span>, "ACCA", which is being developed and advanced in practice as well, is the achievement…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CPL...684...53S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CPL...684...53S"><span>Theoretical study on electronic and vibrational properties of hydrogen bonds in glycine-<span class="hlt">water</span> clusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Yulei; Zhang, Zhiyuan; Jiang, Wanrun; Wang, Zhigang</p> <p>2017-09-01</p> <p>The hydrogen bond (H-bond) in organic-<span class="hlt">water</span> molecules is essential in nature, and it present unique properties distinct from those in pure <span class="hlt">water</span> or organic clusters. Combining with the charge-transfer and energy decomposition analyses, we investigated the penetrating molecular-orbitals in glycine-<span class="hlt">water</span> clusters, which give evidences of the covalent-like characteristics of H-bonds in this system. Besides, the infrared spectral features provide a rare opportunity to discover the exceedingly-evident redshifts of symmetric stretching <span class="hlt">modes</span> (Symst) in <span class="hlt">water</span> on forming H-bond, in contrast to the slightly-redshifted asymmetric stretching <span class="hlt">modes</span> (Asyst) in <span class="hlt">water</span>. To explain these intriguing behaviors, we further analyzed the nuclear vibrating patterns, which clearly reveal that H-bond retains two unexpected effects on nuclear motions in <span class="hlt">water</span>: (i) Intensifying donor Symst, and (ii) Inhibiting donor Asyst. Furthermore, we also quantified the impact of anharmonic quantum fluctuations on each hydrogen bond. For the stretching <span class="hlt">modes</span> involved in H-bonds, red shifts up to more than one hundred wave numbers are observed under anharmonic vibration, explicitly indicating the increased 'covalency' of H-bonds. These finds shed light on the essential understanding of H-bonding comprehensively, and should provide incentives for future experimental studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JAP...123d3303H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JAP...123d3303H"><span>Fluorescence quenching and the "ring-<span class="hlt">mode</span>" to "red-<span class="hlt">mode</span>" transition in alkali inductively coupled plasmas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, M.; Bazurto, R.; Camparo, J.</p> <p>2018-01-01</p> <p>The ring-<span class="hlt">mode</span> to red-<span class="hlt">mode</span> transition in alkali metal inductively coupled plasmas (ICPs) (i.e., rf-discharge lamps) is perhaps the most important physical phenomenon affecting these devices as optical pumping light sources for atomic clocks and magnetometers. It sets the limit on useful ICP operating temperature, thereby setting a limit on ICP light output for atomic-clock/magnetometer signal generation, and it is a temperature region of ICP operation associated with discharge instability. Previous work has suggested that the mechanism driving the ring-<span class="hlt">mode</span> to red-<span class="hlt">mode</span> transition is associated with radiation trapping, but definitive experimental evidence validating that hypothesis has been lacking. Based on that hypothesis, one would predict that the introduction of an alkali-fluorescence quenching gas (i.e., N2) into the ICP would increase the ring-<span class="hlt">mode</span> to red-<span class="hlt">mode</span> transition temperature. Here, we test that prediction, finding direct evidence supporting the radiation-trapping hypothesis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5583638','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5583638"><span>Hospital <span class="hlt">water</span> and opportunities for infection prevention</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Decker, Brooke K.; Palmore, Tara N.</p> <p>2017-01-01</p> <p>Nosocomial waterborne pathogens may reach patients through several <span class="hlt">modes</span> of transmission. Colonization of healthcare facility waterworks can occur in the proximal infrastructure, in the distal <span class="hlt">water</span> outlets, or both. Infections with waterborne organisms such as Legionella, mycobacteria, Pseudomonas, and others cause significant morbidity and mortality, particularly in immunocomprised patients. Hospitals should have prospective <span class="hlt">water</span> safety plans that include preventive measures, as prevention is preferable to remediation of contaminated hospital <span class="hlt">water</span> distribution system. Whole genome sequencing may provide more informative epidemiologic data to link patient infections with hospital <span class="hlt">water</span> isolates. PMID:25217106</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.C43D0652S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.C43D0652S"><span>Atlantic <span class="hlt">water</span> variability on the SE Greenland continental shelf and its relationship to SST</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sutherland, D. A.; Straneo, F.; Rosing-Asvid, A.; Stenson, G.; Davidson, F. J.; Hammill, M.</p> <p>2012-12-01</p> <p>Interaction of warm, Atlantic-origin <span class="hlt">water</span> (AW) and colder, polar origin <span class="hlt">water</span> (PW) advecting southward in the East Greenland Current (EGC) influences the heat content of <span class="hlt">water</span> entering Greenland's outlet glacial fjords. Here we use depth and temperature data derived from deep-diving seals to map out <span class="hlt">water</span> mass variability across the continental shelf and to augment existing bathymetric products. We find two dominant <span class="hlt">modes</span> in the vertical temperature structure: a cold <span class="hlt">mode</span>, with the typical AW/PW layering observed in the EGC, and a warm <span class="hlt">mode</span>, where AW is present throughout the <span class="hlt">water</span> column. The prevalence of these <span class="hlt">modes</span> varies seasonally and spatially across the continental shelf, implying distinct AW pathways. In addition, we find that satellite sea surface temperatures (SST) correlate significantly with temperatures in the upper 50 m (R=0.54), but this correlation decreases with depth (R=0.22 at 200 m), and becomes insignificant below 250 m. Thus, care must be taken in using SST as a proxy for heat content, as AW mainly resides in these deeper layers. Regional map showing the location of all seal tracks originating from Canada and Greenland (stars). Tracks passing inside (red) or outside (blue) the SE Greenland region (black) were subdivided into continental shelf regions (green boxes) near Sermilik Fjord (SF), Cape Farewell (CF) and Kangerdlugssuaq Fjord (KG). GEBCO bathymetry is contoured at 200, 1000, 2000, and 3000 m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28202830','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28202830"><span>[Usefulness of Bolus Administration Using the FLEX <span class="hlt">Mode</span>(Bolus Infusion <span class="hlt">Mode</span>)for Baclofen Tolerance].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tanaka, Kazunori</p> <p>2017-02-01</p> <p>Intrathecal baclofen(ITB)is used to treat intractable spasticity of various etiologies and can provide better control of spasticity through the adjustment of the dose administered through the pump. However, in patients who develop tolerance to baclofen with the standard simple continuous <span class="hlt">mode</span>, a sharp increase in dose becomes necessary, and spasticity can become harder to control. We investigated whether switching from the simple continuous <span class="hlt">mode</span> to the bolus infusion <span class="hlt">mode</span> was effective in controlling spasticity in patients with baclofen tolerance. We reported four patients undergoing ITB therapy at our facility who were considered to have developed baclofen tolerance. We observed the number of bolus infusions and total dose suitable for maintaining spasticity control after switching from the simple continuous <span class="hlt">mode</span> to the bolus infusion <span class="hlt">mode</span>. After switching to the bolus infusion <span class="hlt">mode</span>, the total dose could be reduced in the short term; however, in the long term, the frequency of bolus infusions had to be increased to maintain spasticity control. Two years after changing to bolus infusion six times a day, the total dose was higher than that in the simple continuous <span class="hlt">mode</span> for two of the four patients, and was the same level in the other two patients. Our four cases suggest that bolus infusion is effective in patients with baclofen tolerance during ITB therapy. Therefore, the conditions of bolus infusion should be further investigated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhPl...25d2505M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhPl...25d2505M"><span>Verification of GENE and GYRO with L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasmas in Alcator C-Mod</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mikkelsen, D. R.; Howard, N. T.; White, A. E.; Creely, A. J.</p> <p>2018-04-01</p> <p>Verification comparisons are carried out for L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasma conditions in Alcator C-Mod. We compare linear and nonlinear ion-scale calculations by the gyrokinetic codes GENE and GYRO to each other and to the experimental power balance analysis. The two gyrokinetic codes' linear growth rates and real frequencies are in good agreement throughout all the ion temperature gradient <span class="hlt">mode</span> branches and most of the trapped electron <span class="hlt">mode</span> branches of the kyρs spectra at r/a = 0.65, 0.7, and 0.8. The shapes of the toroidal <span class="hlt">mode</span> spectra of heat fluxes in nonlinear simulations are very similar for kyρs ≤ 0.5, but in most cases GENE has a relatively higher heat flux than GYRO at higher <span class="hlt">mode</span> numbers. The ratio of ion to electron heat flux is similar in the two codes' simulations, but the heat fluxes themselves do not agree in almost all cases. In the I-<span class="hlt">mode</span> regime, GENE's heat fluxes are ˜3 times those from GYRO, and they are ˜60%-100% higher than GYRO in the L-<span class="hlt">mode</span> conditions. The GYRO under-prediction of Qe is much reduced in GENE's L-<span class="hlt">mode</span> simulations, and it is eliminated in the I-<span class="hlt">mode</span> simulations. This largely improved agreement with the experimental electron heat flux is offset, however, by the large overshoot of GENE's ion heat fluxes, which are 2-3 times the experimental level, and its electron heat flux overshoot at r/a = 0.80 in the I-<span class="hlt">mode</span>. Rotation effects can explain part of the difference between the two codes' predictions, but very significant differences remain in simulations without any rotation effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/14525074','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/14525074"><span>Correlations, soliton <span class="hlt">modes</span>, and non-Hermitian linear <span class="hlt">mode</span> transmutation in the one-dimensional noisy Burgers equation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fogedby, Hans C</p> <p>2003-08-01</p> <p>Using the previously developed canonical phase space approach applied to the noisy Burgers equation in one dimension, we discuss in detail the growth morphology in terms of nonlinear soliton <span class="hlt">modes</span> and superimposed linear <span class="hlt">modes</span>. We moreover analyze the non-Hermitian character of the linear <span class="hlt">mode</span> spectrum and the associated dynamical pinning, and <span class="hlt">mode</span> transmutation from diffusive to propagating behavior induced by the solitons. We discuss the anomalous diffusion of growth <span class="hlt">modes</span>, switching and pathways, correlations in the multisoliton sector, and in detail the correlations and scaling properties in the two-soliton sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..113a2119L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..113a2119L"><span>Study on the Flexibility in Cross-Border <span class="hlt">Water</span> Resources Cooperation Governance</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Zongrui; Wang, Teng; Zhou, Li</p> <p>2018-02-01</p> <p>Flexible strategy is very important to cross-border cooperation in international rivers <span class="hlt">water</span> resources, which may be employed to reconcile contradictions and ease conflicts. Flexible characters of cross-border cooperation in international rivers <span class="hlt">water</span> resources could be analyzed and revealed, using flexible strategic management framework, by taking international cooperation protocols related to <span class="hlt">water</span> from Transboundary Freshwater Disputes Database (TFDD) as samples from the number of cooperation issues, the amount of management layers and regulator agencies in cooperation organization and the categories of income (cost) distribution (allocation) <span class="hlt">mode</span>. The research demonstrates that there are some flexible features of cross-border cooperation in international rivers <span class="hlt">water</span> resources: Riparian countries would select relative diversification strategies related to <span class="hlt">water</span>, tend to construct a flexible cooperation organization featured with moderate hierarchies from vertical perspective and simplified administrations from horizontal perspective, and adopt selective inducement <span class="hlt">modes</span> to respect ‘joint and several liability’.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10132E..3JF','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10132E..3JF"><span>Renal stone characterization using high resolution imaging <span class="hlt">mode</span> on a photon counting detector CT system</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ferrero, A.; Gutjahr, R.; Henning, A.; Kappler, S.; Halaweish, A.; Abdurakhimova, D.; Peterson, Z.; Montoya, J.; Leng, S.; McCollough, C.</p> <p>2017-03-01</p> <p>In addition to the standard-resolution (SR) acquisition <span class="hlt">mode</span>, a high-resolution (HR) <span class="hlt">mode</span> is available on a research photon-counting-detector (PCD) whole-body CT system. In the HR <span class="hlt">mode</span> each detector consists of a 2x2 array of 0.225 mm x 0.225 mm subpixel elements. This is in contrast to the SR <span class="hlt">mode</span> that consists of a 4x4 array of the same subelements, and results in 0.25 mm isotropic resolution at iso-center for the HR <span class="hlt">mode</span>. In this study, we quantified ex vivo the capabilities of the HR <span class="hlt">mode</span> to characterize renal stones in terms of morphology and mineral composition. Forty pure stones - 10 uric acid (UA), 10 cystine (CYS), 10 calcium oxalate monohydrate (COM) and 10 apatite (APA) - and 14 mixed stones were placed in a 20 cm <span class="hlt">water</span> phantom and scanned in HR <span class="hlt">mode</span>, at radiation dose matched to that of routine dual-energy stone exams. Data from micro CT provided a reference for the quantification of morphology and mineral composition of the mixed stones. The area under the ROC curve was 1.0 for discriminating UA from CYS, 0.89 for CYS vs COM and 0.84 for COM vs APA. The root mean square error (RMSE) of the percent UA in mixed stones was 11.0% with a medium-sharp kernel and 15.6% with the sharpest kernel. The HR showed qualitatively accurate characterization of stone morphology relative to micro CT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28458443','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28458443"><span>Renal Stone Characterization using High Resolution Imaging <span class="hlt">Mode</span> on a Photon Counting Detector CT System.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ferrero, A; Gutjahr, R; Henning, A; Kappler, S; Halaweish, A; Abdurakhimova, D; Peterson, Z; Montoya, J; Leng, S; McCollough, C</p> <p>2017-03-09</p> <p>In addition to the standard-resolution (SR) acquisition <span class="hlt">mode</span>, a high-resolution (HR) <span class="hlt">mode</span> is available on a research photon-counting-detector (PCD) whole-body CT system. In the HR <span class="hlt">mode</span> each detector consists of a 2x2 array of 0.225 mm × 0.225 mm subpixel elements. This is in contrast to the SR <span class="hlt">mode</span> that consists of a 4x4 array of the same sub-elements, and results in 0.25 mm isotropic resolution at iso-center for the HR <span class="hlt">mode</span>. In this study, we quantified ex vivo the capabilities of the HR <span class="hlt">mode</span> to characterize renal stones in terms of morphology and mineral composition. Forty pure stones - 10 uric acid (UA), 10 cystine (CYS), 10 calcium oxalate monohydrate (COM) and 10 apatite (APA) - and 14 mixed stones were placed in a 20 cm <span class="hlt">water</span> phantom and scanned in HR <span class="hlt">mode</span>, at radiation dose matched to that of routine dual-energy stone exams. Data from micro CT provided a reference for the quantification of morphology and mineral composition of the mixed stones. The area under the ROC curve was 1.0 for discriminating UA from CYS, 0.89 for CYS vs COM and 0.84 for COM vs APA. The root mean square error (RMSE) of the percent UA in mixed stones was 11.0% with a medium-sharp kernel and 15.6% with the sharpest kernel. The HR showed qualitatively accurate characterization of stone morphology relative to micro CT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29760985','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29760985"><span>Terahertz time-domain spectroscopy for non-invasive assessment of <span class="hlt">water</span> content in biological samples.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Borovkova, Mariia; Khodzitsky, Mikhail; Demchenko, Petr; Cherkasova, Olga; Popov, Alexey; Meglinski, Igor</p> <p>2018-05-01</p> <p>We apply terahertz time-domain spectroscopy for the quantitative non-invasive assessment of the <span class="hlt">water</span> content in biological samples, such as Carpinus caroliniana tree leaves and pork muscles. The developed experimental terahertz time-domain spectroscopy system operates both in transmission and reflection <span class="hlt">modes</span>. The Landau-Looyenga-Lifshitz-based model is used for the calculation of the <span class="hlt">water</span> concentration within the samples. The results of the <span class="hlt">water</span> concentration measurements are compared with the results of the gravimetric measurements. The obtained results show that the <span class="hlt">water</span> content in biological samples can be measured non-invasively, with a high accuracy, utilizing terahertz waves in transmission and reflection <span class="hlt">modes</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2699686','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2699686"><span>Resonant <span class="hlt">Mode</span>-hopping Micromixing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jang, Ling-Sheng; Chao, Shih-Hui; Holl, Mark R.; Meldrum, Deirdre R.</p> <p>2009-01-01</p> <p>A common micromixer design strategy is to generate interleaved flow topologies to enhance diffusion. However, problems with these designs include complicated structures and dead volumes within the flow fields. We present an active micromixer using a resonating piezoceramic/silicon composite diaphragm to generate acoustic streaming flow topologies. Circulation patterns are observed experimentally and correlate to the resonant <span class="hlt">mode</span> shapes of the diaphragm. The dead volumes in the flow field are eliminated by rapidly switching from one discrete resonant <span class="hlt">mode</span> to another (i.e., resonant <span class="hlt">mode</span>-hop). Mixer performance is characterized by mixing buffer with a fluorescence tracer containing fluorescein. Movies of the mixing process are analyzed by converting fluorescent images to two-dimensional fluorescein concentration distributions. The results demonstrate that <span class="hlt">mode</span>-hopping operation rapidly homogenized chamber contents, circumventing diffusion-isolated zones. PMID:19551159</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.A31D0082W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.A31D0082W"><span>Interactions between large-scale <span class="hlt">modes</span> of climate and their relationship with Australian climate and hydrology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Whan, K. R.; Lindesay, J. A.; Timbal, B.; Raupach, M. R.; Williams, E.</p> <p>2010-12-01</p> <p>Australia’s natural environment is adapted to low rainfall availability and high variability but human systems are less able to adapt to variability in the hydrological cycle. Understanding the mechanisms underlying drought persistence and severity is vital to contextualising future climate change. Multiple external forcings mean the mechanisms of drought occurrence in south-eastern Australian are complex. The key influences on SEA climate are El Niño-Southern Oscillation (ENSO), the Indian Ocean Dipole (IOD), the Southern Annular <span class="hlt">Mode</span> (SAM) and the sub-tropical ridge (STR); each of these large-scale climate <span class="hlt">modes</span> (LSCM) has been studied widely. The need for research into the interactions among the <span class="hlt">modes</span> has been noted [1], although to date this has received limited attention. Relationships between LSCM and hydrometeorological variability are nonlinear, making linearity assumptions underlying usual statistical techniques (e.g. correlation, principle components analysis) questionable. In the current research a statistical technique that can deal with nonlinear interactions is applied to a new dataset enabling a full examination of the Australian <span class="hlt">water</span> balance. The Australian <span class="hlt">Water</span> Availability Project (AWAP) dataset models the Australian <span class="hlt">water</span> balance on a fine grid [2]. Hydrological parameters (e.g. soil moisture, evaporation, runoff) are modelled from meteorological data, allowing the complete Australian <span class="hlt">water</span> balance (climate and hydrology) to be examined and the mechanisms of drought to be studied holistically. Classification and regression trees (CART) are a powerful regression-based technique that is capable of accounting for nonlinear effects. Although it has limited previous application in climate research [3] this methodology is particularly informative in cases with multiple predictors and nonlinear relationships such as climate variability. Statistical relationships between variables are the basis for the decision rules in CART that are used to split</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2963764','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2963764"><span>Suffering for <span class="hlt">Water</span>, Suffering from <span class="hlt">Water</span>: Access to Drinking-<span class="hlt">water</span> and Associated Health Risks in Cameroon</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p></p> <p>2010-01-01</p> <p>Although many African countries, along the equator, receive a great amount of rainfall and possess a dense hydrographic network, access to drinking-<span class="hlt">water</span> remains a great challenge. In many households, <span class="hlt">water</span> is used for various purposes, including domestic and crafts activities. According to the World Health Organization, an estimated four billion cases of diarrheoa occurs worldwide, of which 88% are ascribed to unsafe drinking-<span class="hlt">water</span>. This study aimed at evaluating health risks in the usage of contaminated drinking-<span class="hlt">water</span> and its relationship with the prevalence of diarrhoeal diseases in Yaoundé, Cameroon. In this cross-sectional epidemiological design, 3,034 households with children aged less than five years were investigated. Households were selected from among 20 representative neighbourhoods out of 105 that made up the city. The study revealed a diarrheoa prevalence of 14.4% (437 diarrheoa cases out of 3,034 children tested). Among various risk factors examined, <span class="hlt">water</span>-supply <span class="hlt">modes</span> and quality of drinking-<span class="hlt">water</span> were statistically associated with diarrheoa cases. Moreover, levels of diarrheoa attacks varied considerably from one neighbourhood to the other. The spatial analysis helped determine neighbourhoods of higher and lower prevalence of diarrheoa in the city. PMID:20941893</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20941893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20941893"><span>Suffering for <span class="hlt">water</span>, suffering from <span class="hlt">water</span>: access to drinking-<span class="hlt">water</span> and associated health risks in Cameroon.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yongsi, H Blaise Nguendo</p> <p>2010-10-01</p> <p>Although many African countries, along the equator, receive a great amount of rainfall and possess a dense hydrographic network, access to drinking-<span class="hlt">water</span> remains a great challenge. In many households, <span class="hlt">water</span> is used for various purposes, including domestic and crafts activities. According to the World Health Organization, an estimated four billion cases of diarrheoa occurs worldwide, of which 88% are ascribed to unsafe drinking-<span class="hlt">water</span>. This study aimed at evaluating health risks in the usage of contaminated drinking-<span class="hlt">water</span> and its relationship with the prevalence of diarrhoeal diseases in Yaound6, Cameroon. In this cross-sectional epidemiological design, 3,034 households with children aged less than five years were investigated. Households were selected from among 20 representative neighbourhoods out of 105 that made up the city. The study revealed a diarrheoa prevalence of 14.4% (437 diarrheoa cases out of 3,034 children tested). Among various risk factors examined, <span class="hlt">water</span>-supply <span class="hlt">modes</span> and quality of drinking-<span class="hlt">water</span> were statistically associated with diarrheoa cases. Moreover, levels of diarrheoa attacks varied considerably from one neighbourhood to the other. The spatial analysis helped determine neighbourhoods of higher and lower prevalence of diarrheoa in the city.</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://ntrs.nasa.gov/search.jsp?R=19930061401&hterms=1073&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231073','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930061401&hterms=1073&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3D%2526%25231073"><span>Absorption coefficients for <span class="hlt">water</span> vapor at 193 nm from 300 to 1073 K</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kessler, W. J.; Carleton, K. L.; Marinelli, W. J.</p> <p>1993-01-01</p> <p>Measurements of the <span class="hlt">water</span> absorption coefficient at 193 nm from 300 to 1073 K are reported. The measurements were made using broadband VUV radiation and a monochromator-based detection system. The <span class="hlt">water</span> vapor was generated by a saturator and metered into a flowing, 99 cm absorption cell via a <span class="hlt">water</span> vapor mass flow meter. The 193 nm absorption coefficient measurements are compared to room temperature and high temperature shock tube measurements with good agreement. The absorption can be parameterized by a nu3 vibrational <span class="hlt">mode</span> reaction coordinate and the thermal population of the nu3 <span class="hlt">mode</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22569882','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22569882"><span>The dynamic crossover in <span class="hlt">water</span> does not require bulk <span class="hlt">water</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Turton, David A; Corsaro, Carmelo; Martin, David F; Mallamace, Francesco; Wynne, Klaas</p> <p>2012-06-14</p> <p>Many of the anomalous properties of <span class="hlt">water</span> may be explained by invoking a second critical point that terminates the coexistence line between the low- and high-density amorphous states in the liquid. Direct experimental evidence of this point, and the associated polyamorphic liquid-liquid transition, is elusive as it is necessary for liquid <span class="hlt">water</span> to be cooled below its homogeneous-nucleation temperature. To avoid crystallization, <span class="hlt">water</span> in the eutectic LiCl solution has been studied but then it is generally considered that "bulk" <span class="hlt">water</span> cannot be present. However, recent computational and experimental studies observe cooperative hydration in which case it is possible that sufficient hydrogen-bonded <span class="hlt">water</span> is present for the essential characteristics of <span class="hlt">water</span> to be preserved. For femtosecond optical Kerr-effect and nuclear magnetic resonance measurements, we observe in each case a fractional Stokes-Einstein relation with evidence of the dynamic crossover appearing near 220 K and 250 K respectively. Spectra obtained in the glass state also confirm the complex nature of the hydrogen-bonding <span class="hlt">modes</span> reported for neat room-temperature <span class="hlt">water</span> and support predictions of anomalous diffusion due to "worm-hole" structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvE..95f3110P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvE..95f3110P"><span>Experimental investigations on characteristics of stable <span class="hlt">water</span> electrospray in air without discharge</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Inyong; Hong, Won Seok; Kim, Sang Bok; Kim, Sang Soo</p> <p>2017-06-01</p> <p>An experimental study was conducted to resolve previous conflicting results on <span class="hlt">water</span> electrospray in air at atmospheric pressure. Using a small flow rate relative to that used in previous studies and a small nonmetallic nozzle, we observed stable electrospray of <span class="hlt">water</span> in air without discharge and distinguished three distinct operating regimes for applied voltage and flow rate. The well-known cone-jet <span class="hlt">mode</span> was observed and the general scaling law of the generated droplet size in the cone-jet <span class="hlt">mode</span> was confirmed by direct visualization of the meniscus, jet, and generated droplets. We also observed and analyzed whipping motion in the electrified <span class="hlt">water</span> jet.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatSR...743855N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatSR...743855N"><span>Center Frequency Stabilization in Planar Dual-<span class="hlt">Mode</span> Resonators during <span class="hlt">Mode</span>-Splitting Control</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Naji, Adham; Soliman, Mina H.</p> <p>2017-03-01</p> <p>Shape symmetry in dual-<span class="hlt">mode</span> planar electromagnetic resonators results in their ability to host two degenerate resonant <span class="hlt">modes</span>. As the designer enforces a controllable break in the symmetry, the degeneracy is removed and the two <span class="hlt">modes</span> couple, exchanging energy and elevating the resonator into its desirable second-order resonance operation. The amount of coupling is controlled by the degree of asymmetry introduced. However, this <span class="hlt">mode</span> coupling (or splitting) usually comes at a price. The centre frequency of the perturbed resonator is inadvertently drifted from its original value prior to coupling. Maintaining centre frequency stability during <span class="hlt">mode</span> splitting is a nontrivial geometric design problem. In this paper, we analyse the problem and propose a novel method to compensate for this frequency drift, based on field analysis and perturbation theory, and we validate the solution through a practical design example and measurements. The analytical method used works accurately within the perturbational limit. It may also be used as a starting point for further numerical optimization algorithms, reducing the required computational time during design, when larger perturbations are made to the resonator. In addition to enabling the novel design example presented, it is hoped that the findings will inspire akin designs for other resonator shapes, in different disciplines and applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29455285','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29455285"><span>Characterization of a novel miniaturized burst-<span class="hlt">mode</span> infrared laser system for IR-MALDESI mass spectrometry imaging.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ekelöf, Måns; Manni, Jeffrey; Nazari, Milad; Bokhart, Mark; Muddiman, David C</p> <p>2018-03-01</p> <p>Laser systems are widely used in mass spectrometry as sample probes and ionization sources. Mid-infrared lasers are particularly suitable for analysis of high <span class="hlt">water</span> content samples such as animal and plant tissues, using <span class="hlt">water</span> as a resonantly excited sacrificial matrix. Commercially available mid-IR lasers have historically been bulky and expensive due to cooling requirements. This work presents a novel air-cooled miniature mid-IR laser with adjustable burst-<span class="hlt">mode</span> output and details an evaluation of its performance for mass spectrometry imaging. The miniature laser was found capable of generating sufficient energy for complete ablation of animal tissue in the context of an IR-MALDESI experiment with exogenously added ice matrix, yielding several hundred confident metabolite identifications. Graphical abstract The use of a novel miniature 2.94 μm burst-<span class="hlt">mode</span> laser in IR-MALDESI allows for rapid and sensitive mass spectrometry imaging of a whole mouse.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29506967','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29506967"><span><span class="hlt">Mode</span> Equivalence of Health Indicators Between Data Collection <span class="hlt">Modes</span> and Mixed-<span class="hlt">Mode</span> Survey Designs in Population-Based Health Interview Surveys for Children and Adolescents: Methodological Study.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mauz, Elvira; Hoffmann, Robert; Houben, Robin; Krause, Laura; Kamtsiuris, Panagiotis; Gößwald, Antje</p> <p>2018-03-05</p> <p>The implementation of an Internet option in an existing public health interview survey using a mixed-<span class="hlt">mode</span> design is attractive because of lower costs and faster data availability. Additionally, mixed-<span class="hlt">mode</span> surveys can increase response rates and improve sample composition. However, mixed-<span class="hlt">mode</span> designs can increase the risk of measurement error (<span class="hlt">mode</span> effects). This study aimed to determine whether the prevalence rates or mean values of self- and parent-reported health indicators for children and adolescents aged 0-17 years differ between self-administered paper-based questionnaires (SAQ-paper) and self-administered Web-based questionnaires (SAQ-Web), as well as between a single-<span class="hlt">mode</span> control group and different mixed-<span class="hlt">mode</span> groups. Data were collected for a methodological pilot of the third wave of the "German Health Interview and Examination Survey for Children and Adolescents". Questionnaires were completed by parents or adolescents. A population-based sample of 11,140 children and adolescents aged 0-17 years was randomly allocated to 4 survey designs-a single-<span class="hlt">mode</span> control group with paper-and-pencil questionnaires only (n=970 parents, n=343 adolescents)-and 3 mixed-<span class="hlt">mode</span> designs, all of which offered Web-based questionnaire options. In the concurrent mixed-<span class="hlt">mode</span> design, both questionnaires were offered at the same time (n=946 parents, n=290 adolescents); in the sequential mixed-<span class="hlt">mode</span> design, the SAQ-Web was sent first, followed by the paper questionnaire along with a reminder (n=854 parents, n=269 adolescents); and in the preselect mixed-<span class="hlt">mode</span> design, both options were offered and the respondents were asked to request the desired type of questionnaire (n=698 parents, n=292 adolescents). In total, 3468 questionnaires of parents of children aged 0-17 years (SAQ-Web: n=708; SAQ-paper: n=2760) and 1194 questionnaires of adolescents aged 11-17 years (SAQ-Web: n=299; SAQ-paper: n=895) were analyzed. Sociodemographic characteristics and a broad range of health indicators for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27958427','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27958427"><span>Single-<span class="hlt">mode</span> large-<span class="hlt">mode</span>-area laser fiber with ultralow numerical aperture and high beam quality.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Peng, Kun; Zhan, Huan; Ni, Li; Wang, Xiaolong; Wang, Yuying; Gao, Cong; Li, Yuwei; Wang, Jianjun; Jing, Feng; Lin, Aoxiang</p> <p>2016-12-10</p> <p>By using the chelate precursor doping technique, we report on an ytterbium-doped aluminophosphosilicate (APS) large-<span class="hlt">mode</span>-area fiber with ultralow numerical aperture of 0.036 and effective fundamental <span class="hlt">mode</span> area of ∼550  μm<sup>2</sup>. With a bend diameter of 600 mm, the bending loss of fundamental <span class="hlt">mode</span> LP<sub>01</sub> was measured to be <10<sup>-3</sup>  dB/m, in agreement with the corresponding simulation results, while that of higher order <span class="hlt">mode</span> LP<sub>11</sub> is >100  dB/m at 1080 nm. Measured in an all-fiber oscillator laser cavity, 592 W single-<span class="hlt">mode</span> laser output was obtained at 1079.64 nm with high-beam quality M<sup>2</sup> of 1.12. The results indicate that the chelate precursor doping technique is a competitive method for ultralow numerical aperture fiber fabrication, which is very suitable for developing single-<span class="hlt">mode</span> seed lasers for high power laser systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017OptEn..56k6101R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017OptEn..56k6101R"><span>Fused-fiber-based 3-dB <span class="hlt">mode</span> insensitive power splitters for few-<span class="hlt">mode</span> optical fiber networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ren, Fang; Huang, Xiaoshan; Wang, Jianping</p> <p>2017-11-01</p> <p>We propose a 3-dB <span class="hlt">mode</span> insensitive power splitter (MIPS) capable of broadcasting and combining optical signals. It is fabricated with two identical few-<span class="hlt">mode</span> fibers (FMFs) by a heating and pulling technique. The <span class="hlt">mode</span>-dependent power transfer characteristic as a function of pulling length is investigated. For exploiting its application, we experimentally demonstrate both FMF-based transmissive and reflective star couplers consisting of multiple 3-dB <span class="hlt">mode</span> insensitive power splitters, which perform broadcasting and routing signals in few-<span class="hlt">mode</span> optical fiber networks such as <span class="hlt">mode</span>-division multiplexing (MDM) local area networks using star topology. For experimental demonstration, optical on-off keying signals at 10 Gb/s carried on three spatial <span class="hlt">modes</span> are successfully processed with open and clear eye diagrams. Measured bit error ratio results show reasonable power penalties. It is found that a reflective star coupler in MDM networks can reduce half of the total amount of required fibers comparing to that of a transmissive star coupler. This MIPS is more efficient, more reliable, more flexible, and more cost-effective for future expansion and application in few-<span class="hlt">mode</span> optical fiber networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011JChPh.134k4704T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011JChPh.134k4704T"><span>Spontaneous <span class="hlt">mode</span>-selection in the self-propelled motion of a solid/liquid composite driven by interfacial instability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takabatake, Fumi; Magome, Nobuyuki; Ichikawa, Masatoshi; Yoshikawa, Kenichi</p> <p>2011-03-01</p> <p>Spontaneous motion of a solid/liquid composite induced by a chemical Marangoni effect, where an oil droplet attached to a solid soap is placed on a <span class="hlt">water</span> phase, was investigated. The composite exhibits various characteristic motions, such as revolution (orbital motion) and translational motion. The results showed that the <span class="hlt">mode</span> of this spontaneous motion switches with a change in the size of the solid scrap. The essential features of this <span class="hlt">mode</span>-switching were reproduced by ordinary differential equations by considering nonlinear friction with proper symmetry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1990PhLA..144..479G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1990PhLA..144..479G"><span>Nonlinear surface elastic <span class="hlt">modes</span> in crystals</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gorentsveig, V. I.; Kivshar, Yu. S.; Kosevich, A. M.; Syrkin, E. S.</p> <p>1990-03-01</p> <p>The influence of nonlinearity on shear horizontal surface elastic waves in crystals is described on the basis of the effective nonlinear Schrödinger equation. It is shown that the corresponding solutions form a set of surface <span class="hlt">modes</span> and the simplest <span class="hlt">mode</span> coincides with the solution proposed by Mozhaev. The higher order <span class="hlt">modes</span> have internal frequencies caused by the nonlinearity. All these <span class="hlt">modes</span> decay in the crystal as uoexp(- z/ zo) atz≫ zo- u o-1 ( z is the distance from the crystal surface, uo the wave amplitude at the surface). The creation of the <span class="hlt">modes</span> from a localized surface excitation has a threshold. The stability of the <span class="hlt">modes</span> is discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19730028611&hterms=1092&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3D%2526%25231092','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730028611&hterms=1092&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3D%2526%25231092"><span>Dual <span class="hlt">mode</span> nuclear rocket system applications.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Boretz, J. E.; Bell, J. M.; Plebuch, R. K.; Priest, C. C.</p> <p>1972-01-01</p> <p>Mission areas where the dual-<span class="hlt">mode</span> nuclear rocket system is superior to nondual-<span class="hlt">mode</span> systems are demonstrated. It is shown that the dual-<span class="hlt">mode</span> system is competitive with the nondual-<span class="hlt">mode</span> system even for those specific missions and particular payload configurations where it does not have a clear-cut advantage.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7043060-fully-three-dimensional-ideal-magnetohydrodynamic-stability-analysis-low-modes-mercier-modes-stellarators','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7043060-fully-three-dimensional-ideal-magnetohydrodynamic-stability-analysis-low-modes-mercier-modes-stellarators"><span>Fully three-dimensional ideal magnetohydrodynamic stability analysis of low- n <span class="hlt">modes</span> and Mercier <span class="hlt">modes</span> in stellarators</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>Fu, G.Y.; Cooper, W.A.; Gruber, R.</p> <p>1992-06-01</p> <p>The TERPSICHORE three-dimensional linear ideal magnetohydrodynamic (MHD) stability code ({ital Theory} {ital of} {ital Fusion} {ital Plasmas}, Proceedings of the Joint Varenna--Lausanne International Workshop, Chexbres, Switzerland, 1988 (Editrice Compositori, Bologna, Italy, 1989), p. 93; {ital Controlled} {ital Fusion} {ital and} {ital Plasma} {ital Heating}, Proceedings of the 17th European Conference, Amsterdam, The Netherlands (European Physical Society, Petit-Lancy, Switzerland, 1990), Vol. 14B, Part II, p. 931; {ital Theory} {ital of} {ital Fusion} {ital Plasmas}, Proceedings of the Joint Varenna--Lausanne International Workshop, Valla Monastero, Varenna, Italy, 1990 (Editrice Compositori, Bologna, Italy, 1990), p. 655) has been extended to the full MHD equations.more » The new code is used to calculate the physical growth rates of nonlocal low-{ital n} <span class="hlt">modes</span> for {ital l}=2 torsatron configurations. A comprehensive investigation of the relation between the Mercier <span class="hlt">modes</span> and the low-{ital n} <span class="hlt">modes</span> has been performed. The unstable localized low-{ital n} <span class="hlt">modes</span> are found to be correlated with the Mercier criterion. Finite growth rates of the low-{ital n} <span class="hlt">modes</span> correspond to finite values of the Mercier criterion parameter. Near the Mercier marginal stability boundary, the low-{ital n} <span class="hlt">modes</span> tend to be weakly unstable with very small growth rates. However, the stability of global-type low-{ital n} <span class="hlt">modes</span> is found to be decorrelated from that of Mercier <span class="hlt">modes</span>. The low-{ital n} <span class="hlt">modes</span> with global radial structures can be more stable or more unstable than Mercier <span class="hlt">modes</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=search&pg=3&id=EJ887028','ERIC'); return false;" href="https://eric.ed.gov/?q=search&pg=3&id=EJ887028"><span>Standardization of Keyword Search <span class="hlt">Mode</span></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>Su, Di</p> <p>2010-01-01</p> <p>In spite of its popularity, keyword search <span class="hlt">mode</span> has not been standardized. Though information professionals are quick to adapt to various presentations of keyword search <span class="hlt">mode</span>, novice end-users may find keyword search confusing. This article compares keyword search <span class="hlt">mode</span> in some major reference databases and calls for standardization. (Contains 3…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E..32A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E..32A"><span>Fine <span class="hlt">mode</span> aerosol chemistry over a rural atmosphere near the north-east coast of Bay of Bengal in India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Adak, Anandamay; Chatterjee, Abhijit; Ghosh, Sanjay; Raha, Sibaji; Roy, Arindam</p> <p>2016-07-01</p> <p>A study was conducted on the chemical characterization of fine <span class="hlt">mode</span> aerosol or PM2.5 over a rural atmosphere near the coast of Bay of Bengal in eastern India. Samples were collected and analyzed during March 2013 - February 2014. The concentration of PM2.5 was found span over a wide range from as low as 3 µg m-3 to as high as 180 µg m-3. The average concentration of PM2.5 was 62 µg m-3. Maximum accumulation of fine <span class="hlt">mode</span> aerosol was observed during winter whereas minimum was observed during monsoon. <span class="hlt">Water</span> soluble ionic species of fine <span class="hlt">mode</span> aerosol were characterized over this rural atmosphere. In spite of being situated near the coast of Bay of Bengal, we observed significantly higher concentrations for anthropogenic species like ammonium and sulphate. The concentrations of these two species were much higher than the sea-salt aerosols. Ammonium and sulphate contributed around 30 % to the total fine <span class="hlt">mode</span> aerosols. Even dust aerosol species like calcium also showed higher concentrations. Chloride to sodium ratio was found to be much less than that in standard sea-<span class="hlt">water</span> indicating strong interaction between sea-salt and anthropogenic aerosols. Use of fertilizers in various crop fields and human and animal wastes significantly increased ammonium in fine <span class="hlt">mode</span> aerosols. Dust aerosol species were accumulated in the atmosphere which could be due to transport of finer dust species from nearby metropolis or locally generated. Non-sea-sulphate and nitrate showed significant contributions in fine <span class="hlt">mode</span> aerosols having both local and transported sources. Source apportionment shows prominent emission sources of anthropogenic aerosols from local anthropogenic activities and transported from nearby Kolkata metropolis as well.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H11H1311T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H11H1311T"><span>Benefit Assessment for Urban Rainwater Measure Configuration <span class="hlt">Mode</span> in Beijing Based on PROMETHEE Method</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tian, L.; Shu, A. P.; Huang, L.</p> <p>2017-12-01</p> <p>Along with accelerating in Chinese urbanization, a increasing number of urban construction projects have been built, which cause the growth of impervious surface ratio in cities. Large areas of impervious surface hinders city normal natural <span class="hlt">water</span> cycles, increases surface runoff coefficient, brings flood peak forward, and increases risk of flooding . Therefore, with the view of reducing risk of urban waterlogging disaster, improving <span class="hlt">water</span> resource cyclic utilization, and maximizing recovery of urban eco-hydrological process, China begins to promote Sponge city construction using LID as core idea. The paper take five kinds of collecting and utilization rainwater measure as research example, analysis their characteristic ,take investment cost, economic benefit and enviromental benefit as principle of assessment. The weight of the evaluation criterion are gained by entropy method. The final evaluation of urban stormwater measures configuration <span class="hlt">mode</span> based on the low impact development with PROMETHEE method . The sensitivity of evaluation criterion are analysised by GAIA. Finally, the examples are given to explain the feasibility . The result shows that comprehensive benefit of the <span class="hlt">mode</span> containing green roof, permeable pavement, Sunken green space and rainwater harvesting tank is the highest. It turn out that reasonable and various types rainwater measures and high land utilization is significant for increasing the its comprehensive efficiency. Besides, the environmental benefit of urban rainwater measures is significantly greater than the economic benefit. There is a positive correlation between plant significantly greater than the economic benefit. There is a positive correlation between plant shallow groove, sunken green space and comprehensive benefit of rainwater measure. Because they can effectively removes <span class="hlt">water</span> pollutants in stormwater. The studies not only have a great significance in optimizing configuration <span class="hlt">mode</span> of urban rainwater measures, but also push</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1437592-verification-gene-gyro-mode-mode-plasmas-alcator-mod','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1437592-verification-gene-gyro-mode-mode-plasmas-alcator-mod"><span>Verification of GENE and GYRO with L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasmas in Alcator C-Mod</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Mikkelsen, D. R.; Howard, N. T.; White, A. E.; ...</p> <p>2018-04-25</p> <p>Here, verification comparisons are carried out for L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasma conditions in Alcator C-Mod. We compare linear and nonlinear ion-scale calculations by the gyrokinetic codes GENE and GYRO to each other and to the experimental power balance analysis. The two gyrokinetic codes' linear growth rates and real frequencies are in good agreement throughout all the ion temperature gradient <span class="hlt">mode</span> branches and most of the trapped electron <span class="hlt">mode</span> branches of the kyρs spectra at r/a = 0.65, 0.7, and 0.8. The shapes of the toroidal <span class="hlt">mode</span> spectra of heat fluxes in nonlinear simulations are very similar for k yρ smore » ≤ 0.5, but in most cases GENE has a relatively higher heat flux than GYRO at higher <span class="hlt">mode</span> numbers.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1437592-verification-gene-gyro-mode-mode-plasmas-alcator-mod','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1437592-verification-gene-gyro-mode-mode-plasmas-alcator-mod"><span>Verification of GENE and GYRO with L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasmas in Alcator C-Mod</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>Mikkelsen, D. R.; Howard, N. T.; White, A. E.</p> <p></p> <p>Here, verification comparisons are carried out for L-<span class="hlt">mode</span> and I-<span class="hlt">mode</span> plasma conditions in Alcator C-Mod. We compare linear and nonlinear ion-scale calculations by the gyrokinetic codes GENE and GYRO to each other and to the experimental power balance analysis. The two gyrokinetic codes' linear growth rates and real frequencies are in good agreement throughout all the ion temperature gradient <span class="hlt">mode</span> branches and most of the trapped electron <span class="hlt">mode</span> branches of the kyρs spectra at r/a = 0.65, 0.7, and 0.8. The shapes of the toroidal <span class="hlt">mode</span> spectra of heat fluxes in nonlinear simulations are very similar for k yρ smore » ≤ 0.5, but in most cases GENE has a relatively higher heat flux than GYRO at higher <span class="hlt">mode</span> numbers.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=56913&searchall=children's+health+or+children's+environmental+health+or+adolescence+or+adolescent+or+child+or+childhood+or+children+or+developmental+or+daycare+or+early%20life+or+epigenetic+or+fetal+or+in%20utero+or+infant+or+maternal+or+paternal+or+perinatal+or+postnatal+or+pregnancy+or+pregnant+or+prenatal+or+school+or+young%20adult&sortby=fy','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=56913&searchall=children's+health+or+children's+environmental+health+or+adolescence+or+adolescent+or+child+or+childhood+or+children+or+developmental+or+daycare+or+early%20life+or+epigenetic+or+fetal+or+in%20utero+or+infant+or+maternal+or+paternal+or+perinatal+or+postnatal+or+pregnancy+or+pregnant+or+prenatal+or+school+or+young%20adult&sortby=fy"><span>A Summary of Publications on the Development of <span class="hlt">Mode</span>-of ...</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>Chemical contaminants are formed as a consequence of chemical disinfection of public drinking <span class="hlt">waters</span>. Chemical disinfectants, which are used to kill harmful microorganisms, react with natural organic matter (NOM), bromide, iodide, and other compounds, forming complex mixtures of potentially toxic disinfection byproducts (DBPs). The types and concentrations of DBPs formed during disinfection and the relative proportions of the components vary depending on factors such as source <span class="hlt">water</span> conditions (e.g., types of NOM present), disinfectant type (e.g., chlorine, ozone, chloramine), and treatment conditions (e.g., pH and temperature). To date, over 500 DBPs have been detected in treated <span class="hlt">waters</span>. However, typically more than 50% of the organic halide mass produced by chlorination disinfection consists of unidentified chemicals, which are not measured by routine analyses of DBPs. The protocols and methods typically used to evaluate chemical mixtures are best applied to simple defined mixtures consisting of relatively few chemicals. These approaches rely on assumptions (e.g., common <span class="hlt">mode</span> of action, independent toxic action) regarding the type of joint toxic action (e.g., dose-additivity, synergism) that might be observed. Such methods, used for site assessments or toxicological studies, are often not sufficient to estimate health risk for complex drinking <span class="hlt">water</span> DBP mixtures. Actual drinking <span class="hlt">water</span> exposures involve multiple chemicals, many of w</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5512674','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5512674"><span>Microfluidic Flows and Heat Transfer and Their Influence on Optical <span class="hlt">Modes</span> in Microstructure Fibers</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Davies, Edward; Christodoulides, Paul; Florides, George; Kalli, Kyriacos</p> <p>2014-01-01</p> <p>A finite element analysis (FEA) model has been constructed to predict the thermo-fluidic and optical properties of a microstructure optical fiber (MOF) accounting for changes in external temperature, input <span class="hlt">water</span> velocity and optical fiber geometry. Modeling a <span class="hlt">water</span> laminar flow within a <span class="hlt">water</span> channel has shown that the steady-state temperature is dependent on the <span class="hlt">water</span> channel radius while independent of the input velocity. There is a critical channel radius below which the steady-state temperature of the <span class="hlt">water</span> channel is constant, while above, the temperature decreases. However, the distance required to reach steady state within the <span class="hlt">water</span> channel is dependent on both the input velocity and the channel radius. The MOF has been found capable of supporting multiple <span class="hlt">modes</span>. Despite the large thermo-optic coefficient of <span class="hlt">water</span>, the bound modes’ response to temperature was dominated by the thermo-optic coefficient of glass. This is attributed to the majority of the light being confined within the glass, which increased with increasing external temperature due to a larger difference in the refractive index between the glass core and the <span class="hlt">water</span> channel. PMID:28788263</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018TDM.....5a5025B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018TDM.....5a5025B"><span>Touch-<span class="hlt">mode</span> capacitive pressure sensor with graphene-polymer heterostructure membrane</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berger, Christian; Phillips, Rory; Pasternak, Iwona; Sobieski, Jan; Strupinski, Wlodek; Vijayaraghavan, Aravind</p> <p>2018-01-01</p> <p>We describe the fabrication and characterisation of a touch-<span class="hlt">mode</span> capacitive pressure sensor (TMCPS) with a robust design that comprises a graphene-polymer heterostructure film, laminated onto the silicon dioxide surface of a silicon wafer, incorporating a SU-8 spacer grid structure. The spacer grid structure allows the flexible graphene-polymer film to be partially suspended above the substrate, such that a pressure on the membrane results in a reproducible deflection, even after exposing the membrane to pressures over 10 times the operating range. Sensors show reproducible pressure transduction in <span class="hlt">water</span> submersion at varying depths under static and dynamic loading. The measured capacitance change in response to pressure is in good agreement with an analytical model of clamped plates in touch <span class="hlt">mode</span>. The device shows a pressure sensitivity of 27.1 +/- 0.5 fF Pa-1 over a pressure range of 0.5 kPa-8.5 kPa. In addition, we demonstrate the operation of this device as a force-touch sensor in air.</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/2015ISPAr.XL1..363L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ISPAr.XL1..363L"><span>Validation of Spaceborne Radar Surface <span class="hlt">Water</span> Mapping with Optical sUAS Images</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li-Chee-Ming, J.; Murnaghan, K.; Sherman, D.; Poncos, V.; Brisco, B.; Armenakis, C.</p> <p>2015-08-01</p> <p>The Canada Centre for Remote Sensing (CCRS) has over 40 years of experience with airborne and spaceborne sensors and is now starting to use small Unmanned Aerial Systems (sUAS) to validate products from large coverage area sensors and create new methodologies for very high resolution products. Wetlands have several functions including <span class="hlt">water</span> storage and retention which can reduce flooding and provide continuous flow for hydroelectric generation and irrigation for agriculture. Synthetic Aperture Radar is well suited as a tool for monitoring surface <span class="hlt">water</span> by supplying acquisitions irrespective of cloud cover or time of day. Wetlands can be subdivided into three classes: open <span class="hlt">water</span>, flooded vegetation and upland which can vary seasonally with time and <span class="hlt">water</span> level changes. RADARSAT-2 data from the Wide-Ultra Fine, Spotlight and Fine Quad-Pol <span class="hlt">modes</span> has been used to map the open <span class="hlt">water</span> in the Peace-Athabasca Delta, Alberta using intensity thresholding. We also use spotlight <span class="hlt">modes</span> for higher resolution and the fully polarimetric <span class="hlt">mode</span> (FQ) for polarimetric decomposition. Validation of these products will be done using a low altitude flying sUAS to generate optical georeferenced images. This project provides methodologies which could be used for flood mapping as well as ecological monitoring.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27749870','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27749870"><span>PT-symmetric <span class="hlt">mode</span>-locking.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Longhi, S</p> <p>2016-10-01</p> <p>Parity-time (PT) symmetry is one of the most important accomplishments in optics over the past decade. Here the concept of PT <span class="hlt">mode</span>-locking (ML) of a laser is introduced, in which active phase-locking of cavity axial <span class="hlt">modes</span> is realized by asymmetric <span class="hlt">mode</span> coupling in a complex time crystal. PT ML shows a transition from single- to double-pulse emission as the PT symmetry breaking point is crossed. The transition can show a turbulent behavior, depending on a dimensionless modulation parameter that plays the same role as the Reynolds number in hydrodynamic flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMMR43A0457N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMMR43A0457N"><span>Raman Spectroscopy of <span class="hlt">Water</span>-rich Stishovite and Dense High-Pressure Silica up to 55 GPa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nisr, C.; Shim, S. H.; Leinenweber, K. D.; Chizmeshya, A. V.</p> <p>2017-12-01</p> <p>Recent studies have shown that mineral phases such as δ-AlOOH, (Mg,Si)OOH, (Mg,Si,Al)OOH, (Al,Si)O2 and SiO2 with rutile-type or modified rutile-type crystal structures can store large amounts of <span class="hlt">water</span> and be stable at high pressure and high temperature relevant to the Earth's lower mantle. The Al-H charge coupled substitution has been proposed to explain the large storage capacity of these phases. However, the substitution cannot explain the large <span class="hlt">water</span> storage found in pure stishovite (Spektor et al., 2011). Instead, an octahedral version of hydrogarnet-like substitution has been proposed for the incorporation of hydrogen in pure stishovite. We have performed Raman spectroscopy measurements on pure hydrous stishovite with 3.2 wt% <span class="hlt">water</span> up to 55 GPa. At ambient pressure, we found that the OH stretching <span class="hlt">mode</span> frequencies range between those of low-<span class="hlt">water</span> aluminous stishovite and δ-AlOOH, suggesting an intermediate strength of hydrogen bonding between these two phases. In the lattice <span class="hlt">mode</span> range, we observe <span class="hlt">modes</span> similar to the IR-active <span class="hlt">modes</span> of anhydrous stishovite after decompression to 1 bar, suggesting Si defects in the crystal structure that activate the inactive <span class="hlt">modes</span>. Our data show a series of changes at pressures between 24 and 28 GPa, supporting our observation of a phase transition (likely to the CaCl2 type) in X-Ray diffraction measurements (Nisr et al., 2017, JGR). We found that the OH <span class="hlt">mode</span> of hydrous stishovite has a positive frequency shift with an increase in pressure. The behavior is the opposite to that found in δ-AlOOH, indicating that the OH incorporation mechanism in hydrous silica is different from that of aluminous low-<span class="hlt">water</span> stishovite and δ-AlOOH, likely through direct substitution (Si ⇄ 4H+). Because the mantle hydrous phases would have complex compositions, our study suggests that the direct substitution should also be considered together with the Al substitution for the deep mantle storage of <span class="hlt">water</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/57720','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/57720"><span>Ground <span class="hlt">water</span> in Oklahoma</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Leonard, A.R.</p> <p>1960-01-01</p> <p>One of the first requisites for the intelligent planning of utilization and control of <span class="hlt">water</span> and for the administration of laws relating to its use is data on the quantity, quality, and <span class="hlt">mode</span> of occurrence of the available supplies. The collection, evaluation and interpretation, and publication of such data are among the primary functions of the U. S. Geological Survey, Since 1895 the Congress has made appropriations to the Survey for investigation of the <span class="hlt">water</span> resources of the Nation. In 1929 the Congress adopted the policy of dollar-for-dollar cooperation with the States and local governmental agencies in <span class="hlt">water</span> resources investigations of the U. S. Geological Survey, In 1937 a program of ground-<span class="hlt">water</span> investigations was started in cooperation with the Oklahoma Geological Survey, and in 1949 this program was expanded to include cooperation with the Oklahoma Planning and Resources Board, In 1957 the State Legislature created the Oklahoma <span class="hlt">Water</span> Resources Board as the principal State <span class="hlt">water</span> agency and it became the principal local cooperator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5431931-parasitic-modes-removal-out-operating-mode-neighbourhood-daw-accelerating-structure','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5431931-parasitic-modes-removal-out-operating-mode-neighbourhood-daw-accelerating-structure"><span>Parasitic <span class="hlt">modes</span> removal out of operating <span class="hlt">mode</span> neighbourhood in the DAW accelerating structure</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>Andreev, V.G.; Belugin, V.M.; Esin, S.K.</p> <p>1983-08-01</p> <p>The disk and washer (DAW) accelerating structure finds its use in a number of new projects (PIGMI, SNQ etc ). It composes the main part of the accelerating structure of the meson factory now under construction in the Institute for Nuclear Research (INR), Moscow. It is known that the parasitic <span class="hlt">modes</span> with azimuthal field variations exist at the operating <span class="hlt">mode</span> region. In this report different methods of the parasitic <span class="hlt">modes</span> frequency shift are considered. The main attention is given to the resonant methods, which are the most efficient.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018APExp..11e2702Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018APExp..11e2702Z"><span>Few-<span class="hlt">mode</span> vertical-cavity surface-emitting laser: Optional emission of transverse <span class="hlt">modes</span> with different polarizations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhong, Chuyu; Zhang, Xing; Hofmann, Werner; Yu, Lijuan; Liu, Jianguo; Ning, Yongqiang; Wang, Lijun</p> <p>2018-05-01</p> <p>Few-<span class="hlt">mode</span> vertical-cavity surface-emitting lasers that can be controlled to emit certain <span class="hlt">modes</span> and polarization states simply by changing the biased contacts are proposed and fabricated. By directly etching trenches in the p-doped distributed Bragg reflector, the upper mesa is separated into several submesas above the oxide layer. Individual contacts are then deposited. Each contact is used to control certain transverse <span class="hlt">modes</span> with different polarization directions emitted from the corresponding submesa. These new devices can be seen as a prototype of compact laser sources in <span class="hlt">mode</span> division multiplexing communications systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.4618H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.4618H"><span>Partitioning of ice nucleating particles: Which <span class="hlt">modes</span> matter?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hande, Luke; Hoose, Corinna</p> <p>2017-04-01</p> <p>Ice particles in clouds have a large impact on cloud lifetime, precipitation amount, and cloud radiative properties through the indirect aerosol effect. Thus, correctly modelling ice formation processes is important for simulations preformed on all spatial and temporal scales. Ice forms on aerosol particles through several different mechanisms, namely deposition nucleation, immersion freezing, and contact freezing. However there is conflicting evidence as to which <span class="hlt">mode</span> dominates, and the relative importance of the three heterogeneous ice nucleation mechanisms, as well as homogeneous nucleation, remains an open question. The environmental conditions, and hence the cloud type, have a large impact on determining which nucleation <span class="hlt">mode</span> dominates. In order to understand this, simulations were performed with the COSMO-LES model, utilising state of the art parameterisations to describe the different nucleation mechanisms for several semi-idealised cloud types commonly occurring over central Europe. The cloud types investigated include a semi-idealised, and an idealised convective cloud, an orographic cloud, and a stratiform cloud. Results show that immersion and contact freezing dominate at warmer temperatures, and under most conditions, deposition nucleation plays only a minor role. In clouds where sufficiently high levels of <span class="hlt">water</span> vapour are present at colder temperatures, deposition nucleation can play a role, however in general homogeneous nucleation dominates at colder temperatures. Since contact nucleation depends on the environmental relative humidity, enhancements in this nucleation <span class="hlt">mode</span> can be seen in areas of dry air entrainment. The results indicate that ice microphysical processes are somewhat sensitve to the environmental conditions and therefore the cloud type.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5751620','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5751620"><span>Repetitively <span class="hlt">Mode</span>-Locked Cavity-Enhanced Absorption Spectroscopy (RML-CEAS) for Near-Infrared Gas Sensing</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zheng, Chuantao; Wang, Yiding</p> <p>2017-01-01</p> <p>A Pound-Drever-Hall (PDH)-based <span class="hlt">mode</span>-locked cavity-enhanced sensor system was developed using a distributed feedback diode laser centered at 1.53 µm as the laser source. Laser temperature scanning, bias control of the piezoelectric ceramic transducer (PZT) and proportional-integral-derivative (PID) feedback control of diode laser current were used to repetitively lock the laser <span class="hlt">modes</span> to the cavity <span class="hlt">modes</span>. A gas absorption spectrum was obtained by using a series of absorption data from the discrete <span class="hlt">mode</span>-locked points. The 15 cm-long Fabry-Perot cavity was sealed using an enclosure with an inlet and outlet for gas pumping and a PZT for cavity length tuning. The performance of the sensor system was evaluated by conducting <span class="hlt">water</span> vapor measurements. A linear relationship was observed between the measured absorption signal amplitude and the H2O concentration. A minimum detectable absorption coefficient of 1.5 × 10–8 cm–1 was achieved with an averaging time of 700 s. This technique can also be used for the detection of other trace gas species by targeting the corresponding gas absorption line. PMID:29207470</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23964420','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23964420"><span>Are two hands (from different people) better than one? <span class="hlt">Mode</span> effects and differential transfer between manual coordination <span class="hlt">modes</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gorman, Jamie C; Crites, Michael J</p> <p>2013-08-01</p> <p>We report an experiment in which we investigated differential transfer between unimanual (one-handed), bimanual (two-handed), and intermanual (different peoples' hands) coordination <span class="hlt">modes</span>. People perform some manual tasks faster than others ("<span class="hlt">mode</span> effects"). However, little is known about transfer between coordination <span class="hlt">modes</span>. To investigate differential transfer, we draw hypotheses from two perspectives--information based and constraint based--of bimanual and interpersonal coordination and skill acquisition. Participants drove a teleoperated rover around a circular path in sets of two 2-min trials using two of the different coordination <span class="hlt">modes</span>. Speed and variability of the rover's path were measured. Order of coordination <span class="hlt">modes</span> was manipulated to examine differential transfer and <span class="hlt">mode</span> effects. Differential transfer analyses revealed patterns of positive transfer from simpler (localized spatiotemporal constraints) to more complex (distributed spatiotemporal constraints) coordination <span class="hlt">modes</span> paired with negative transfer in the opposite direction. <span class="hlt">Mode</span> effects indicated that intermanual performance was significantly faster than unimanual performance, and bimanual performance was intermediate. Importantly, all of these effects disappeared with practice. The observed patterns of differential transfer between coordination <span class="hlt">modes</span> may be better accounted for by a constraint-based explanation of differential transfer than by an information-based one. <span class="hlt">Mode</span> effects may be attributable to anticipatory movements based on dyads' access to mutual visual information. Although people may be faster using more-complex coordination <span class="hlt">modes</span>, when operators transition between <span class="hlt">modes</span>, they may be more effective transitioning from simpler (e.g., bimanual) to more complex (e.g., intermanual) <span class="hlt">modes</span> than vice versa. However, this difference may be critical only for novel or rarely practiced tasks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AIPC.1842c0024L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AIPC.1842c0024L"><span>Q-<span class="hlt">mode</span> versus R-<span class="hlt">mode</span> principal component analysis for linear discriminant analysis (LDA)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, Loong Chuen; Liong, Choong-Yeun; Jemain, Abdul Aziz</p> <p>2017-05-01</p> <p>Many literature apply Principal Component Analysis (PCA) as either preliminary visualization or variable con-struction methods or both. Focus of PCA can be on the samples (R-<span class="hlt">mode</span> PCA) or variables (Q-<span class="hlt">mode</span> PCA). Traditionally, R-<span class="hlt">mode</span> PCA has been the usual approach to reduce high-dimensionality data before the application of Linear Discriminant Analysis (LDA), to solve classification problems. Output from PCA composed of two new matrices known as loadings and scores matrices. Each matrix can then be used to produce a plot, i.e. loadings plot aids identification of important variables whereas scores plot presents spatial distribution of samples on new axes that are also known as Principal Components (PCs). Fundamentally, the scores matrix always be the input variables for building classification model. A recent paper uses Q-<span class="hlt">mode</span> PCA but the focus of analysis was not on the variables but instead on the samples. As a result, the authors have exchanged the use of both loadings and scores plots in which clustering of samples was studied using loadings plot whereas scores plot has been used to identify important manifest variables. Therefore, the aim of this study is to statistically validate the proposed practice. Evaluation is based on performance of external error obtained from LDA models according to number of PCs. On top of that, bootstrapping was also conducted to evaluate the external error of each of the LDA models. Results show that LDA models produced by PCs from R-<span class="hlt">mode</span> PCA give logical performance and the matched external error are also unbiased whereas the ones produced with Q-<span class="hlt">mode</span> PCA show the opposites. With that, we concluded that PCs produced from Q-<span class="hlt">mode</span> is not statistically stable and thus should not be applied to problems of classifying samples, but variables. We hope this paper will provide some insights on the disputable issues.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24526721','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24526721"><span>Olfactory foraging in temperate <span class="hlt">waters</span>: sensitivity to dimethylsulphide of shearwaters in the Atlantic Ocean and Mediterranean Sea.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dell'Ariccia, Gaia; Célérier, Aurélie; Gabirot, Marianne; Palmas, Pauline; Massa, Bruno; Bonadonna, Francesco</p> <p>2014-05-15</p> <p>Many procellariiforms use olfactory cues to locate food patches over the seemingly featureless ocean surface. In particular, some of them are able to detect and are attracted by dimethylsulphide (DMS), a volatile compound naturally occurring over worldwide oceans in correspondence with productive feeding areas. However, current knowledge is restricted to <span class="hlt">sub-Antarctic</span> species and to only one study realized under natural conditions at sea. Here, for the first time, we investigated the response to DMS in parallel in two different environments in temperate <span class="hlt">waters</span>, the Atlantic Ocean and the Mediterranean Sea, employing Cory's (Calonectris borealis) and Scopoli's (Calonectris diomedea) shearwaters as models. To test whether these birds can detect and respond to DMS, we presented them with this substance in a Y-maze. Then, to determine whether they use this molecule in natural conditions, we tested the response to DMS at sea. The number of birds that chose DMS in the Y-maze and that were recruited at DMS-scented slicks at sea suggests that these shearwaters are attracted to DMS in both non-foraging and natural contexts. Our findings show that the use of DMS as a foraging cue may be a strategy adopted by procellariiforms across oceans but that regional differences may exist, giving a worldwide perspective to previous hypotheses concerning the use of DMS as a chemical cue. © 2014. Published by The Company of Biologists Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018OptEL..14...88L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018OptEL..14...88L"><span>LP01 to LP11 <span class="hlt">mode</span> convertor based on side-polished small-core single-<span class="hlt">mode</span> fiber</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Yan; Li, Yang; Li, Wei-dong</p> <p>2018-03-01</p> <p>An all-fiber LP01-LP11 <span class="hlt">mode</span> convertor based on side-polished small-core single-<span class="hlt">mode</span> fibers (SMFs) is numerically demonstrated. The linearly polarized incident beam in one arm experiences π shift through a fiber half waveplate, and the side-polished parts merge into an equivalent twin-core fiber (TCF) which spatially shapes the incident LP01 <span class="hlt">modes</span> to the LP11 <span class="hlt">mode</span> supported by the step-index few-<span class="hlt">mode</span> fiber (FMF). Optimum conditions for the highest conversion efficiency are investigated using the beam propagation method (BPM) with an approximate efficiency as high as 96.7%. The proposed scheme can operate within a wide wavelength range from 1.3 μm to1.7 μm with overall conversion efficiency greater than 95%. The effective <span class="hlt">mode</span> area and coupling loss are also characterized in detail by finite element method (FEM).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1413558','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1413558"><span>Streambed microstructure predicts evolution of development and life history <span class="hlt">mode</span> in the plethodontid salamander Eurycea tynerensis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bonett, Ronald M; Chippindale, Paul T</p> <p>2006-01-01</p> <p>Background Habitat variation strongly influences the evolution of developmentally flexible traits, and may drive speciation and diversification. The plethodontid salamander Eurycea tynerensis is endemic to the geologically diverse Ozark Plateau of south-central North America, and comprises both strictly aquatic paedomorphic populations (achieving reproductive maturity while remaining in the larval form) and more terrestrial metamorphic populations. The switch between developmental <span class="hlt">modes</span> has occurred many times, but populations typically exhibit a single life history <span class="hlt">mode</span>. This unique system offers an opportunity to study the specific ecological circumstances under which alternate developmental and life history <span class="hlt">modes</span> evolve. We use phylogenetic independent contrasts to test for relationships between a key microhabitat feature (streambed sediment) and this major life history polymorphism. Results We find streambed microstructure (sediment particle size, type and degree of sorting) to be highly correlated with life-history <span class="hlt">mode</span>. Eurycea tynerensis is paedomorphic in streams containing large chert gravel, but metamorphoses in nearby streams containing poorly sorted, clastic material such as sandstone or siltstone. Conclusion Deposits of large chert gravel create loosely associated streambeds, which provide access to subsurface <span class="hlt">water</span> during dry summer months. Conversely, streambeds composed of more densely packed sandstone and siltstone sediments leave no subterranean refuge when surface <span class="hlt">water</span> dries, presumably necessitating metamorphosis and use of terrestrial habitats. This represents a clear example of the relationship between microhabitat structure and evolution of a major developmental and life history trait, and has broad implications for the role of localized ecological conditions on larger-scale evolutionary processes. PMID:16512919</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011Freq...65...47S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011Freq...65...47S"><span>A Current-<span class="hlt">Mode</span> Common-<span class="hlt">Mode</span> Feedback Circuit (CMFB) with Rail-to-Rail Operation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suadet, Apirak; Kasemsuwan, Varakorn</p> <p>2011-03-01</p> <p>This paper presents a current-<span class="hlt">mode</span> common-<span class="hlt">mode</span> feedback (CMFB) circuit with rail-to-rail operation. The CMFB is a stand-alone circuit, which can be connected to any low voltage transconductor without changing or upsetting the existing circuit. The proposed CMFB employs current mirrors, operating as common-<span class="hlt">mode</span> detector and current amplifier to enhance the loop gain of the CMFB. The circuit employs positive feedback to enhance the output impedance and gain. The circuit has been designed using a 0.18 <italic>μ</italic>m CMOS technology under 1V supply and analyzed using HSPICE with BSIM3V3 device models. A pseudo-differential amplifier using two common sources and the proposed CMFB shows rail to rail output swing (± 0.7 V) with low common-<span class="hlt">mode</span> gain (-36 dB) and power dissipation of 390 <italic>μ</italic>W.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24836232','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24836232"><span>Did BICEP2 see vector <span class="hlt">modes</span>? First B-<span class="hlt">mode</span> constraints on cosmic defects.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Moss, Adam; Pogosian, Levon</p> <p>2014-05-02</p> <p>Scaling networks of cosmic defects, such as strings and textures, actively generate scalar, vector, and tensor metric perturbations throughout the history of the Universe. In particular, vector <span class="hlt">modes</span> sourced by defects are an efficient source of the cosmic microwave background B-<span class="hlt">mode</span> polarization. We use the recently released BICEP2 and POLARBEAR B-<span class="hlt">mode</span> polarization spectra to constrain properties of a wide range of different types of cosmic strings networks. We find that in order for strings to provide a satisfactory fit on their own, the effective interstring distance needs to be extremely large--spectra that fit the data best are more representative of global strings and textures. When a local string contribution is considered together with the inflationary B-<span class="hlt">mode</span> spectrum, the fit is improved. We discuss implications of these results for theories that predict cosmic defects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18999836','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18999836"><span>Energetic-particle-induced geodesic acoustic <span class="hlt">mode</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fu, G Y</p> <p>2008-10-31</p> <p>A new energetic particle-induced geodesic acoustic <span class="hlt">mode</span> (EGAM) is shown to exist. The <span class="hlt">mode</span> frequency and <span class="hlt">mode</span> structure are determined nonperturbatively by energetic particle kinetic effects. In particular the EGAM frequency is found to be substantially lower than the standard GAM frequency. The radial <span class="hlt">mode</span> width is determined by the energetic particle drift orbit width and can be fairly large for high energetic particle pressure and large safety factor. These results are consistent with the recent experimental observation of the beam-driven n=0 <span class="hlt">mode</span> in DIII-D.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JChPh.148k4506H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JChPh.148k4506H"><span>Collective excitations and ultrafast dipolar solvation dynamics in <span class="hlt">water</span>-ethanol binary mixture</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hazra, Milan K.; Bagchi, Biman</p> <p>2018-03-01</p> <p>In order to understand the intermolecular vibrational spectrum and the collective excitations of <span class="hlt">water</span>-ethanol binary mixture, we investigate the density of states and the power spectrum using computer simulations aided by theory. We investigate in particular the spectra at intermediate to low frequencies (a few hundreds to few tens of cm-1) by calculating (i) the density of states from quenched normal <span class="hlt">modes</span>, (ii) the power spectrum from velocity time correlation function, and (iii) the far infrared and dielectric spectra (that is, the Cole-Cole plot) from the total dipole moment time correlation function. The different spectra are in broad agreement with each other and at the same time reveal unique characteristics of the <span class="hlt">water</span>-ethanol mixture. Inverse participation ratio reveals several interesting features. Libration of pure ethanol is more localized than that of pure <span class="hlt">water</span>. With increasing ethanol content, we observe localization of the collective libration <span class="hlt">mode</span> as well as of the hindered translational and rotational <span class="hlt">mode</span>. An interesting mixing between the libration of <span class="hlt">water</span> and ethanol is observed. Solvation dynamics of tryptophan measured by equilibrium energy fluctuation time correlation function show surprisingly strong non-linear dependence on composition that can be tested against experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29566531','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29566531"><span>Collective excitations and ultrafast dipolar solvation dynamics in <span class="hlt">water</span>-ethanol binary mixture.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hazra, Milan K; Bagchi, Biman</p> <p>2018-03-21</p> <p>In order to understand the intermolecular vibrational spectrum and the collective excitations of <span class="hlt">water</span>-ethanol binary mixture, we investigate the density of states and the power spectrum using computer simulations aided by theory. We investigate in particular the spectra at intermediate to low frequencies (a few hundreds to few tens of cm -1 ) by calculating (i) the density of states from quenched normal <span class="hlt">modes</span>, (ii) the power spectrum from velocity time correlation function, and (iii) the far infrared and dielectric spectra (that is, the Cole-Cole plot) from the total dipole moment time correlation function. The different spectra are in broad agreement with each other and at the same time reveal unique characteristics of the <span class="hlt">water</span>-ethanol mixture. Inverse participation ratio reveals several interesting features. Libration of pure ethanol is more localized than that of pure <span class="hlt">water</span>. With increasing ethanol content, we observe localization of the collective libration <span class="hlt">mode</span> as well as of the hindered translational and rotational <span class="hlt">mode</span>. An interesting mixing between the libration of <span class="hlt">water</span> and ethanol is observed. Solvation dynamics of tryptophan measured by equilibrium energy fluctuation time correlation function show surprisingly strong non-linear dependence on composition that can be tested against experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EnMan..51..882C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EnMan..51..882C"><span>Evaluating Adaptive Governance Approaches to Sustainable <span class="hlt">Water</span> Management in North-West Thailand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clark, Julian R. A.; Semmahasak, Chutiwalanch</p> <p>2013-04-01</p> <p>Adaptive governance is advanced as a potent means of addressing institutional fit of natural resource systems with prevailing <span class="hlt">modes</span> of political-administrative management. Its advocates also argue that it enhances participatory and learning opportunities for stakeholders over time. Yet an increasing number of studies demonstrate real difficulties in implementing adaptive governance `solutions'. This paper builds on these debates by examining the introduction of adaptive governance to <span class="hlt">water</span> management in Chiang Mai province, north-west Thailand. The paper considers, first, the limitations of current <span class="hlt">water</span> governance <span class="hlt">modes</span> at the provincial scale, and the rationale for implementation of an adaptive approach. The new approach is then critically examined, with its initial performance and likely future success evaluated by (i) analysis of <span class="hlt">water</span> stakeholders' opinions of its first year of operation; and (ii) comparison of its governance attributes against recent empirical accounts of implementation difficulty and failure of adaptive governance of natural resource management more generally. The analysis confirms the potentially significant role that the new approach can play in brokering and resolving the underlying differences in stakeholder representation and knowledge construction at the heart of the prevailing <span class="hlt">water</span> governance <span class="hlt">modes</span> in north-west Thailand.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2672048','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2672048"><span>Processing <span class="hlt">Mode</span> Causally Influences Emotional Reactivity</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Watkins, Ed; Moberly, Nicholas J.; Moulds, Michelle L.</p> <p>2008-01-01</p> <p>Three studies are reported showing that emotional responses to stress can be modified by systematic prior practice in adopting particular processing <span class="hlt">modes</span>. Participants were induced to think about positive and negative scenarios in a <span class="hlt">mode</span> either characteristic of or inconsistent with the abstract-evaluative mind-set observed in depressive rumination, via explicit instructions (Experiments 1 and 2) and via implicit induction of interpretative biases (Experiment 3), before being exposed to a failure experience. In all three studies, participants trained into the <span class="hlt">mode</span> antithetical to depressive rumination demonstrated less emotional reactivity following failure than participants trained into the <span class="hlt">mode</span> consistent with depressive rumination. These findings provide evidence consistent with the hypothesis that processing <span class="hlt">mode</span> modifies emotional reactivity and support the processing-<span class="hlt">mode</span> theory of rumination. 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