Sample records for air reveals large-scale

  1. Sensitivity of local air quality to the interplay between small- and large-scale circulations: a large-eddy simulation study

    NASA Astrophysics Data System (ADS)

    Wolf-Grosse, Tobias; Esau, Igor; Reuder, Joachim

    2017-06-01

    Street-level urban air pollution is a challenging concern for modern urban societies. Pollution dispersion models assume that the concentrations decrease monotonically with raising wind speed. This convenient assumption breaks down when applied to flows with local recirculations such as those found in topographically complex coastal areas. This study looks at a practically important and sufficiently common case of air pollution in a coastal valley city. Here, the observed concentrations are determined by the interaction between large-scale topographically forced and local-scale breeze-like recirculations. Analysis of a long observational dataset in Bergen, Norway, revealed that the most extreme cases of recurring wintertime air pollution episodes were accompanied by increased large-scale wind speeds above the valley. Contrary to the theoretical assumption and intuitive expectations, the maximum NO2 concentrations were not found for the lowest 10 m ERA-Interim wind speeds but in situations with wind speeds of 3 m s-1. To explain this phenomenon, we investigated empirical relationships between the large-scale forcing and the local wind and air quality parameters. We conducted 16 large-eddy simulation (LES) experiments with the Parallelised Large-Eddy Simulation Model (PALM) for atmospheric and oceanic flows. The LES accounted for the realistic relief and coastal configuration as well as for the large-scale forcing and local surface condition heterogeneity in Bergen. They revealed that emerging local breeze-like circulations strongly enhance the urban ventilation and dispersion of the air pollutants in situations with weak large-scale winds. Slightly stronger large-scale winds, however, can counteract these local recirculations, leading to enhanced surface air stagnation. Furthermore, this study looks at the concrete impact of the relative configuration of warmer water bodies in the city and the major transport corridor. We found that a relatively small local water

  2. DESIGN OF LARGE-SCALE AIR MONITORING NETWORKS

    EPA Science Inventory

    The potential effects of air pollution on human health have received much attention in recent years. In the U.S. and other countries, there are extensive large-scale monitoring networks designed to collect data to inform the public of exposure risks to air pollution. A major crit...

  3. Polar firn air reveals large-scale impact of anthropogenic mercury emissions during the 1970s

    PubMed Central

    Faïn, Xavier; Ferrari, Christophe P.; Dommergue, Aurélien; Albert, Mary R.; Battle, Mark; Severinghaus, Jeff; Arnaud, Laurent; Barnola, Jean-Marc; Cairns, Warren; Barbante, Carlo; Boutron, Claude

    2009-01-01

    Mercury (Hg) is an extremely toxic pollutant, and its biogeochemical cycle has been perturbed by anthropogenic emissions during recent centuries. In the atmosphere, gaseous elemental mercury (GEM; Hg°) is the predominant form of mercury (up to 95%). Here we report the evolution of atmospheric levels of GEM in mid- to high-northern latitudes inferred from the interstitial air of firn (perennial snowpack) at Summit, Greenland. GEM concentrations increased rapidly after World War II from ≈1.5 ng m−3 reaching a maximum of ≈3 ng m−3 around 1970 and decreased until stabilizing at ≈1.7 ng m−3 around 1995. This reconstruction reproduces real-time measurements available from the Arctic since 1995 and exhibits the same general trend observed in Europe since 1990. Anthropogenic emissions caused a two-fold rise in boreal atmospheric GEM concentrations before the 1970s, which likely contributed to higher deposition of mercury in both industrialized and remotes areas. Once deposited, this toxin becomes available for methylation and, subsequently, the contamination of ecosystems. Implementation of air pollution regulations, however, enabled a large-scale decline in atmospheric mercury levels during the 1980s. The results shown here suggest that potential increases in emissions in the coming decades could have a similar large-scale impact on atmospheric Hg levels. PMID:19805267

  4. Polar firn air reveals large-scale impact of anthropogenic mercury emissions during the 1970s.

    PubMed

    Faïn, Xavier; Ferrari, Christophe P; Dommergue, Aurélien; Albert, Mary R; Battle, Mark; Severinghaus, Jeff; Arnaud, Laurent; Barnola, Jean-Marc; Cairns, Warren; Barbante, Carlo; Boutron, Claude

    2009-09-22

    Mercury (Hg) is an extremely toxic pollutant, and its biogeochemical cycle has been perturbed by anthropogenic emissions during recent centuries. In the atmosphere, gaseous elemental mercury (GEM; Hg degrees ) is the predominant form of mercury (up to 95%). Here we report the evolution of atmospheric levels of GEM in mid- to high-northern latitudes inferred from the interstitial air of firn (perennial snowpack) at Summit, Greenland. GEM concentrations increased rapidly after World War II from approximately 1.5 ng m(-3) reaching a maximum of approximately 3 ng m(-3) around 1970 and decreased until stabilizing at approximately 1.7 ng m(-3) around 1995. This reconstruction reproduces real-time measurements available from the Arctic since 1995 and exhibits the same general trend observed in Europe since 1990. Anthropogenic emissions caused a two-fold rise in boreal atmospheric GEM concentrations before the 1970s, which likely contributed to higher deposition of mercury in both industrialized and remotes areas. Once deposited, this toxin becomes available for methylation and, subsequently, the contamination of ecosystems. Implementation of air pollution regulations, however, enabled a large-scale decline in atmospheric mercury levels during the 1980s. The results shown here suggest that potential increases in emissions in the coming decades could have a similar large-scale impact on atmospheric Hg levels.

  5. Effects of Large-Scale Solar Installations on Dust Mobilization and Air Quality

    NASA Astrophysics Data System (ADS)

    Pratt, J. T.; Singh, D.; Diffenbaugh, N. S.

    2012-12-01

    Large-scale solar projects are increasingly being developed worldwide and many of these installations are located in arid, desert regions. To examine the effects of these projects on regional dust mobilization and air quality, we analyze aerosol product data from NASA's Multi-angle Imaging Spectroradiometer (MISR) at annual and seasonal time intervals near fifteen photovoltaic and solar thermal stations ranging from 5-200 MW (12-4,942 acres) in size. The stations are distributed over eight different countries and were chosen based on size, location and installation date; most of the installations are large-scale, took place in desert climates and were installed between 2006 and 2010. We also consider air quality measurements of particulate matter between 2.5 and 10 micrometers (PM10) from the Environmental Protection Agency (EPA) monitoring sites near and downwind from the project installations in the U.S. We use monthly wind data from the NOAA's National Center for Atmospheric Prediction (NCEP) Global Reanalysis to select the stations downwind from the installations, and then perform statistical analysis on the data to identify any significant changes in these quantities. We find that fourteen of the fifteen regions have lower aerosol product after the start of the installations as well as all six PM10 monitoring stations showing lower particulate matter measurements after construction commenced. Results fail to show any statistically significant differences in aerosol optical index or PM10 measurements before and after the large-scale solar installations. However, many of the large installations are very recent, and there is insufficient data to fully understand the long-term effects on air quality. More data and higher resolution analysis is necessary to better understand the relationship between large-scale solar, dust and air quality.

  6. Landsat 7 Reveals Large-scale Fractal Motion of Clouds

    NASA Technical Reports Server (NTRS)

    2002-01-01

    get carried along within the vortices, but these are soon mixed into the surrounding clouds. Landsat is unique in its ability to image both the small-scale eddies that mix clear and cloudy air, down to the 30 meter pixel size of Landsat, but also having a wide enough field-of-view, 180 km, to reveal the connection of the turbulence to large-scale flows such as the subtropical oceanic gyres. Landsat 7, with its new onboard digital recorder, has extended this capability away from the few Landsat ground stations to remote areas such as Alejandro Island, and thus is gradually providing a global dynamic picture of evolving human-scale phenomena. (For more details on von Karman vortices, refer to http://climate.gsfc.nasa.gov/cahalan) Image and caption courtesy Bob Cahalan, NASA GSFC

  7. Large-scale exact diagonalizations reveal low-momentum scales of nuclei

    NASA Astrophysics Data System (ADS)

    Forssén, C.; Carlsson, B. D.; Johansson, H. T.; Sääf, D.; Bansal, A.; Hagen, G.; Papenbrock, T.

    2018-03-01

    Ab initio methods aim to solve the nuclear many-body problem with controlled approximations. Virtually exact numerical solutions for realistic interactions can only be obtained for certain special cases such as few-nucleon systems. Here we extend the reach of exact diagonalization methods to handle model spaces with dimension exceeding 1010 on a single compute node. This allows us to perform no-core shell model (NCSM) calculations for 6Li in model spaces up to Nmax=22 and to reveal the 4He+d halo structure of this nucleus. Still, the use of a finite harmonic-oscillator basis implies truncations in both infrared (IR) and ultraviolet (UV) length scales. These truncations impose finite-size corrections on observables computed in this basis. We perform IR extrapolations of energies and radii computed in the NCSM and with the coupled-cluster method at several fixed UV cutoffs. It is shown that this strategy enables information gain also from data that is not fully UV converged. IR extrapolations improve the accuracy of relevant bound-state observables for a range of UV cutoffs, thus making them profitable tools. We relate the momentum scale that governs the exponential IR convergence to the threshold energy for the first open decay channel. Using large-scale NCSM calculations we numerically verify this small-momentum scale of finite nuclei.

  8. Linking Low-Frequency Large-Scale Circulation Patterns to Cold Air Outbreak Formation in the Northeastern North Atlantic

    NASA Astrophysics Data System (ADS)

    Papritz, L.; Grams, C. M.

    2018-03-01

    The regional variability of wintertime marine cold air outbreaks (CAOs) in the northeastern North Atlantic is studied focusing on the role of weather regimes in modulating the large-scale circulation. Each regime is characterized by a typical CAO frequency anomaly pattern and a corresponding imprint in air-sea heat fluxes. Cyclonically dominated regimes, Greenland blocking and the Atlantic ridge regime are found to provide favorable conditions for CAO formation in at least one major sea of the study region; CAO occurrence is suppressed, however, by blocked regimes whose associated anticyclones are centered over northern Europe (European / Scandinavian blocking). Kinematic trajectories reveal that strength and location of the storm tracks are closely linked to the pathways of CAO air masses and, thus, CAO occurrence. Finally, CAO frequencies are also linked to the strength of the stratospheric polar vortex, which is understood in terms of associated variations in the frequency of weather regimes.

  9. Analysis and experimental study on formation conditions of large-scale barrier-free diffuse atmospheric pressure air plasmas in repetitive pulse mode

    NASA Astrophysics Data System (ADS)

    Li, Lee; Liu, Lun; Liu, Yun-Long; Bin, Yu; Ge, Ya-Feng; Lin, Fo-Chang

    2014-01-01

    Atmospheric air diffuse plasmas have enormous application potential in various fields of science and technology. Without dielectric barrier, generating large-scale air diffuse plasmas is always a challenging issue. This paper discusses and analyses the formation mechanism of cold homogenous plasma. It is proposed that generating stable diffuse atmospheric plasmas in open air should meet the three conditions: high transient power with low average power, excitation in low average E-field with locally high E-field region, and multiple overlapping electron avalanches. Accordingly, an experimental configuration of generating large-scale barrier-free diffuse air plasmas is designed. Based on runaway electron theory, a low duty-ratio, high voltage repetitive nanosecond pulse generator is chosen as a discharge excitation source. Using the wire-electrodes with small curvature radius, the gaps with highly non-uniform E-field are structured. Experimental results show that the volume-scaleable, barrier-free, homogeneous air non-thermal plasmas have been obtained between the gap spacing with the copper-wire electrodes. The area of air cold plasmas has been up to hundreds of square centimeters. The proposed formation conditions of large-scale barrier-free diffuse air plasmas are proved to be reasonable and feasible.

  10. Group Centric Networking: Large Scale Over the Air Testing of Group Centric Networking

    DTIC Science & Technology

    2016-11-01

    protocol designed to support groups of devices in a local region [4]. It attempts to use the wireless medium to broadcast minimal control information...1) Group Discovery: The goal of the group discovery algo- rithm is to find group nodes without globally flooding control messages. To facilitate this...Large Scale Over-the-Air Testing of Group Centric Networking Logan Mercer, Greg Kuperman, Andrew Hunter, Brian Proulx MIT Lincoln Laboratory

  11. Large scale air pollution estimation method combining land use regression and chemical transport modeling in a geostatistical framework.

    PubMed

    Akita, Yasuyuki; Baldasano, Jose M; Beelen, Rob; Cirach, Marta; de Hoogh, Kees; Hoek, Gerard; Nieuwenhuijsen, Mark; Serre, Marc L; de Nazelle, Audrey

    2014-04-15

    In recognition that intraurban exposure gradients may be as large as between-city variations, recent air pollution epidemiologic studies have become increasingly interested in capturing within-city exposure gradients. In addition, because of the rapidly accumulating health data, recent studies also need to handle large study populations distributed over large geographic domains. Even though several modeling approaches have been introduced, a consistent modeling framework capturing within-city exposure variability and applicable to large geographic domains is still missing. To address these needs, we proposed a modeling framework based on the Bayesian Maximum Entropy method that integrates monitoring data and outputs from existing air quality models based on Land Use Regression (LUR) and Chemical Transport Models (CTM). The framework was applied to estimate the yearly average NO2 concentrations over the region of Catalunya in Spain. By jointly accounting for the global scale variability in the concentration from the output of CTM and the intraurban scale variability through LUR model output, the proposed framework outperformed more conventional approaches.

  12. The perfect ash-storm: large-scale Pyroclastic Density Current experiments reveal highly mobile, self-fluidising and air-cushioned flow transport regime

    NASA Astrophysics Data System (ADS)

    Lube, G.; Cronin, S. J.; Breard, E.; Valentine, G.; Bursik, M. I.; Hort, M. K.; Freundt, A.

    2013-12-01

    We report on the first systematic series of large-scale Pyroclastic Density Current (PDC) experiments using the New Zealand PDC Generator, a novel international research facility in Physical Volcanology recently commissioned at Massey University. Repeatable highly energetic and hot PDCs are synthesized by the controlled ';eruption column-collapse' of up to 3500 kg of homogenously aerated Taupo ignimbrite material from a 15 m-elevated hopper onto an instrumented inclined flume. At discharge rates between 250-1300 kg/s and low- to moderate gas injection rates (yielding initial solids concentration of 15-70 vol%) channelized gas-particle mixture flows life-scaled to dense PDCs can be generated. The flow fronts of the currents reach velocities of up to 9.5 m/s over their first 12 m of travel and rapidly develop strong vertical density stratification. The PDCs typically form a highly mobile, <60 cm-thick dense and channel-confined underflow, with an overriding dilute and turbulent ash cloud surge that also laterally escapes the flume boundaries. Depending on the PDC starting conditions underflows with 1-45 vol% solids concentration are formed, while the upper surge contains <<1 vol.% solids. A characteristic feature of the underflow is the occurrence of 'ignitive' front breakouts, producing jetted lobes that accelerate outward from the flow front, initially forming a lobe-cleft structure, followed by segregation downslope into multiple flow pulses. Depending on initial solids concentration and discharge rate, stratified, dune-bedded and inversely graded bedforms are created whose thicknesses are remarkably uniform along the medial to distal runout path characterising highly mobile flow runout. Along with high-speed video footage we present time-series data of basal arrays of load- and gas-pore pressure transducers to characterise the mobile dense underflows. Data shows that the PDCs are comprised of a turbulent coarse-grained and air-ingesting front with particle

  13. Large-Scale Disasters

    NASA Astrophysics Data System (ADS)

    Gad-El-Hak, Mohamed

    "Extreme" events - including climatic events, such as hurricanes, tornadoes, and drought - can cause massive disruption to society, including large death tolls and property damage in the billions of dollars. Events in recent years have shown the importance of being prepared and that countries need to work together to help alleviate the resulting pain and suffering. This volume presents a review of the broad research field of large-scale disasters. It establishes a common framework for predicting, controlling and managing both manmade and natural disasters. There is a particular focus on events caused by weather and climate change. Other topics include air pollution, tsunamis, disaster modeling, the use of remote sensing and the logistics of disaster management. It will appeal to scientists, engineers, first responders and health-care professionals, in addition to graduate students and researchers who have an interest in the prediction, prevention or mitigation of large-scale disasters.

  14. LARGE-SCALE PREDICTIONS OF MOBILE SOURCE CONTRIBUTIONS TO CONCENTRATIONS OF TOXIC AIR POLLUTANTS

    EPA Science Inventory

    This presentation shows concentrations and deposition of toxic air pollutants predicted by a 3-D air quality model, the Community Multi Scale Air Quality (CMAQ) modeling system. Contributions from both on-road and non-road mobile sources are analyzed.

  15. Cytology of DNA Replication Reveals Dynamic Plasticity of Large-Scale Chromatin Fibers.

    PubMed

    Deng, Xiang; Zhironkina, Oxana A; Cherepanynets, Varvara D; Strelkova, Olga S; Kireev, Igor I; Belmont, Andrew S

    2016-09-26

    In higher eukaryotic interphase nuclei, the 100- to >1,000-fold linear compaction of chromatin is difficult to reconcile with its function as a template for transcription, replication, and repair. It is challenging to imagine how DNA and RNA polymerases with their associated molecular machinery would move along the DNA template without transient decondensation of observed large-scale chromatin "chromonema" fibers [1]. Transcription or "replication factory" models [2], in which polymerases remain fixed while DNA is reeled through, are similarly difficult to conceptualize without transient decondensation of these chromonema fibers. Here, we show how a dynamic plasticity of chromatin folding within large-scale chromatin fibers allows DNA replication to take place without significant changes in the global large-scale chromatin compaction or shape of these large-scale chromatin fibers. Time-lapse imaging of lac-operator-tagged chromosome regions shows no major change in the overall compaction of these chromosome regions during their DNA replication. Improved pulse-chase labeling of endogenous interphase chromosomes yields a model in which the global compaction and shape of large-Mbp chromatin domains remains largely invariant during DNA replication, with DNA within these domains undergoing significant movements and redistribution as they move into and then out of adjacent replication foci. In contrast to hierarchical folding models, this dynamic plasticity of large-scale chromatin organization explains how localized changes in DNA topology allow DNA replication to take place without an accompanying global unfolding of large-scale chromatin fibers while suggesting a possible mechanism for maintaining epigenetic programming of large-scale chromatin domains throughout DNA replication. Copyright © 2016 Elsevier Ltd. All rights reserved.

  16. Drought Variability in Eastern Part of Romania and its Connection with Large-Scale Air Circulation

    NASA Astrophysics Data System (ADS)

    Barbu, Nicu; Stefan, Sabina; Georgescu, Florinela

    2014-05-01

    Drought is a phenomenon that appears due to precipitation deficit and it is intensified by strong winds, high temperatures, low relative humidity and high insolation; in fact, all these factors lead to increasing of evapotranspiration processes that contribute to soil water deficit. The Standardized Precipitation Evapotranspiration Index (SPEI) take into account all this factors listed above. The temporal variability of the drought in Eastern part of Romania for 50 years, during the period 1961-2010, is investigated. This study is focused on the drought variability related to large scale air circulation. The gridded dataset with spatial resolution of 0.5º lat/lon of SPEI, (https://digital.csic.es/handle/10261/72264) were used to analyze drought periods in connection with large scale air circulation determinate from the two catalogues (GWT - GrossWetter-Typen and WLK - WetterLargenKlassifikation) defined in COST733Action. The GWT catalogue uses at input dataset the sea level pressure and the WLK catalogue uses as input dataset the geopotential field at 925 hPa and 500 hPa, wind at 700 hPa and total water content for entire atmospheric column. In this study we use the GWT catalogue with 18 circulation types and the WLK catalogue with 40 circulation types. The analysis for Barlad Hydrological Basin indicated that the negative values (that means water deficit - drought period) of SPEI are associated with prevailing anticyclonic regime and positive values (that means water excess - rainy period) of SPEI are associated with prevailing cyclonic regime as was expected. In last decade was observed an increase of dry period associated with an increase of anticyclonic activity over Romania. Using GWT18 catalogue the drought are associated with the north-eastern anticyclonic circulation type (NE-A). According to the WLK40 catalogue, the dominant circulation type associated with the drought is north-west-anticyclonic-dry anticyclonic (NW-AAD) type. keywords: drought, SPEI

  17. Revealing Large-Scale Asymetries in the Winds of Hot, Luminous Stars Using Spectroscopy and Polarimetry

    NASA Astrophysics Data System (ADS)

    St-Louis, Nicole

    2015-08-01

    The winds of hot, luminous stars are known to show small but also large scale density structures. Ultimately, these departures from spherical symmetry are important for the understanding of the loss of angular momentum from the star and are crucial in determining its rotation rate. There are many observational signatures of these departures from a uniform and spherically symmetric outflow. This poster will present results from spectroscopic and polarimetric observations of Wolf-Rayet stars, the descendants of massive O stars, that reveal large-scale asymmetries in their winds and discuss what can be learned about the structure of these winds and about the the physical mechanism responsible for generating them. Very little is known about the rotation rates of these small, He-burning stars which are the direct progenitors of at least some supernova explosions. If enough angular momentum is retained in the core, some may also very well be the progenitors of long gamma-ray bursts.

  18. Skin Friction Reduction Through Large-Scale Forcing

    NASA Astrophysics Data System (ADS)

    Bhatt, Shibani; Artham, Sravan; Gnanamanickam, Ebenezer

    2017-11-01

    Flow structures in a turbulent boundary layer larger than an integral length scale (δ), referred to as large-scales, interact with the finer scales in a non-linear manner. By targeting these large-scales and exploiting this non-linear interaction wall shear stress (WSS) reduction of over 10% has been achieved. The plane wall jet (PWJ), a boundary layer which has highly energetic large-scales that become turbulent independent of the near-wall finer scales, is the chosen model flow field. It's unique configuration allows for the independent control of the large-scales through acoustic forcing. Perturbation wavelengths from about 1 δ to 14 δ were considered with a reduction in WSS for all wavelengths considered. This reduction, over a large subset of the wavelengths, scales with both inner and outer variables indicating a mixed scaling to the underlying physics, while also showing dependence on the PWJ global properties. A triple decomposition of the velocity fields shows an increase in coherence due to forcing with a clear organization of the small scale turbulence with respect to the introduced large-scale. The maximum reduction in WSS occurs when the introduced large-scale acts in a manner so as to reduce the turbulent activity in the very near wall region. This material is based upon work supported by the Air Force Office of Scientific Research under Award Number FA9550-16-1-0194 monitored by Dr. Douglas Smith.

  19. Semi-Automated Air-Coupled Impact-Echo Method for Large-Scale Parkade Structure.

    PubMed

    Epp, Tyler; Svecova, Dagmar; Cha, Young-Jin

    2018-03-29

    Structural Health Monitoring (SHM) has moved to data-dense systems, utilizing numerous sensor types to monitor infrastructure, such as bridges and dams, more regularly. One of the issues faced in this endeavour is the scale of the inspected structures and the time it takes to carry out testing. Installing automated systems that can provide measurements in a timely manner is one way of overcoming these obstacles. This study proposes an Artificial Neural Network (ANN) application that determines intact and damaged locations from a small training sample of impact-echo data, using air-coupled microphones from a reinforced concrete beam in lab conditions and data collected from a field experiment in a parking garage. The impact-echo testing in the field is carried out in a semi-autonomous manner to expedite the front end of the in situ damage detection testing. The use of an ANN removes the need for a user-defined cutoff value for the classification of intact and damaged locations when a least-square distance approach is used. It is postulated that this may contribute significantly to testing time reduction when monitoring large-scale civil Reinforced Concrete (RC) structures.

  20. Semi-Automated Air-Coupled Impact-Echo Method for Large-Scale Parkade Structure

    PubMed Central

    Epp, Tyler; Svecova, Dagmar; Cha, Young-Jin

    2018-01-01

    Structural Health Monitoring (SHM) has moved to data-dense systems, utilizing numerous sensor types to monitor infrastructure, such as bridges and dams, more regularly. One of the issues faced in this endeavour is the scale of the inspected structures and the time it takes to carry out testing. Installing automated systems that can provide measurements in a timely manner is one way of overcoming these obstacles. This study proposes an Artificial Neural Network (ANN) application that determines intact and damaged locations from a small training sample of impact-echo data, using air-coupled microphones from a reinforced concrete beam in lab conditions and data collected from a field experiment in a parking garage. The impact-echo testing in the field is carried out in a semi-autonomous manner to expedite the front end of the in situ damage detection testing. The use of an ANN removes the need for a user-defined cutoff value for the classification of intact and damaged locations when a least-square distance approach is used. It is postulated that this may contribute significantly to testing time reduction when monitoring large-scale civil Reinforced Concrete (RC) structures. PMID:29596332

  1. Outbreaks associated to large open air festivals, including music festivals, 1980 to 2012.

    PubMed

    Botelho-Nevers, E; Gautret, P

    2013-03-14

    In the minds of many, large scale open air festivals have become associated with spring and summer, attracting many people, and in the case of music festivals, thousands of music fans. These festivals share the usual health risks associated with large mass gatherings, including transmission of communicable diseases and risk of outbreaks. Large scale open air festivals have however specific characteristics, including outdoor settings, on-site housing and food supply and the generally young age of the participants. Outbreaks at large scale open air festivals have been caused by Cryptosporium parvum, Campylobacter spp., Escherichia coli, Salmonella enterica, Shigella sonnei, Staphylococcus aureus, hepatitis A virus, influenza virus, measles virus, mumps virus and norovirus. Faecal-oral and respiratory transmissions of pathogens result from non-compliance with hygiene rules, inadequate sanitation and insufficient vaccination coverage. Sexual transmission of infectious diseases may also occur and is likely to be underestimated and underreported. Enhanced surveillance during and after festivals is essential. Preventive measures such as immunisations of participants and advice on-site and via social networks should be considered to reduce outbreaks at these large scale open air festivals.

  2. Large scale features and energetics of the hybrid subtropical low `Duck' over the Tasman Sea

    NASA Astrophysics Data System (ADS)

    Pezza, Alexandre Bernardes; Garde, Luke Andrew; Veiga, José Augusto Paixão; Simmonds, Ian

    2014-01-01

    New aspects of the genesis and partial tropical transition of a rare hybrid subtropical cyclone on the eastern Australian coast are presented. The `Duck' (March 2001) attracted more recent attention due to its underlying genesis mechanisms being remarkably similar to the first South Atlantic hurricane (March 2004). Here we put this cyclone in climate perspective, showing that it belongs to a class within the 1 % lowest frequency percentile in the Southern Hemisphere as a function of its thermal evolution. A large scale analysis reveals a combined influence from an existing tropical cyclone and a persistent mid-latitude block. A Lagrangian tracer showed that the upper level air parcels arriving at the cyclone's center had been modified by the blocking. Lorenz energetics is used to identify connections with both tropical and extratropical processes, and reveal how these create the large scale environment conducive to the development of the vortex. The results reveal that the blocking exerted the most important influence, with a strong peak in barotropic generation of kinetic energy over a large area traversed by the air parcels just before genesis. A secondary peak also coincided with the first time the cyclone developed an upper level warm core, but with insufficient amplitude to allow for a full tropical transition. The applications of this technique are numerous and promising, particularly on the use of global climate models to infer changes in environmental parameters associated with severe storms.

  3. Experimental study of rotating wind turbine breakdown characteristics in large scale air gaps

    NASA Astrophysics Data System (ADS)

    Wang, Yu; Qu, Lu; Si, Tianjun; Ni, Yang; Xu, Jianwei; Wen, Xishan

    2017-06-01

    When a wind turbine is struck by lightning, its blades are usually rotating. The effect of blade rotation on a turbine’s ability to trigger a lightning strike is unclear. Therefore, an arching electrode was used in a wind turbine lightning discharge test to investigate the difference in lightning triggering ability when blades are rotating and stationary. A negative polarity switching waveform of 250/2500 μs was applied to the arching electrode and the up-and-down method was used to calculate the 50% discharge voltage. Lightning discharge tests of a 1:30 scale wind turbine model with 2, 4, and 6 m air gaps were performed and the discharge process was observed. The experimental results demonstrated that when a 2 m air gap was used, the breakdown voltage increased as the blade speed was increased, but when the gap length was 4 m or longer, the trend was reversed and the breakdown voltage decreased. The analysis revealed that the rotation of the blades changes the charge distribution in the blade-tip region, promotes upward leader development on the blade tip, and decreases the breakdown voltage. Thus, the blade rotation of a wind turbine increases its ability to trigger lightning strikes.

  4. The application of liquid air energy storage for large scale long duration solutions to grid balancing

    NASA Astrophysics Data System (ADS)

    Brett, Gareth; Barnett, Matthew

    2014-12-01

    Liquid Air Energy Storage (LAES) provides large scale, long duration energy storage at the point of demand in the 5 MW/20 MWh to 100 MW/1,000 MWh range. LAES combines mature components from the industrial gas and electricity industries assembled in a novel process and is one of the few storage technologies that can be delivered at large scale, with no geographical constraints. The system uses no exotic materials or scarce resources and all major components have a proven lifetime of 25+ years. The system can also integrate low grade waste heat to increase power output. Founded in 2005, Highview Power Storage, is a UK based developer of LAES. The company has taken the concept from academic analysis, through laboratory testing, and in 2011 commissioned the world's first fully integrated system at pilot plant scale (300 kW/2.5 MWh) hosted at SSE's (Scottish & Southern Energy) 80 MW Biomass Plant in Greater London which was partly funded by a Department of Energy and Climate Change (DECC) grant. Highview is now working with commercial customers to deploy multi MW commercial reference plants in the UK and abroad.

  5. Operational design and pressure response of large-scale compressed air energy storage in porous formations

    NASA Astrophysics Data System (ADS)

    Wang, Bo; Bauer, Sebastian

    2017-04-01

    With the rapid growth of energy production from intermittent renewable sources like wind and solar power plants, large-scale energy storage options are required to compensate for fluctuating power generation on different time scales. Compressed air energy storage (CAES) in porous formations is seen as a promising option for balancing short-term diurnal fluctuations. CAES is a power-to-power energy storage, which converts electricity to mechanical energy, i.e. highly pressurized air, and stores it in the subsurface. This study aims at designing the storage setup and quantifying the pressure response of a large-scale CAES operation in a porous sandstone formation, thus assessing the feasibility of this storage option. For this, numerical modelling of a synthetic site and a synthetic operational cycle is applied. A hypothetic CAES scenario using a typical anticline structure in northern Germany was investigated. The top of the storage formation is at 700 m depth and the thickness is 20 m. The porosity and permeability were assumed to have a homogenous distribution with a value of 0.35 and 500 mD, respectively. According to the specifications of the Huntorf CAES power plant, a gas turbine producing 321 MW power with a minimum inlet pressure of 43 bars at an air mass flowrate of 417 kg/s was assumed. Pressure loss in the gas wells was accounted for using an analytical solution, which defines a minimum bottom hole pressure of 47 bars. Two daily extraction cycles of 6 hours each were set to the early morning and the late afternoon in order to bypass the massive solar energy production around noon. A two-year initial filling of the reservoir with air and ten years of daily cyclic operation were numerically simulated using the Eclipse E300 reservoir simulator. The simulation results show that using 12 wells the storage formation with a permeability of 500 mD can support the required 6-hour continuous power output of 321MW, which corresponds an energy output of 3852 MWh per

  6. Assessment of long-term and large-scale even-odd license plate controlled plan effects on urban air quality and its implication

    NASA Astrophysics Data System (ADS)

    Zhao, Suping; Yu, Ye; Qin, Dahe; Yin, Daiying; He, Jianjun

    2017-12-01

    To solve traffic congestion and to improve urban air quality, long-lasting and large-scale even-odd license plate controlled plan was implemented by local government during 20 November to 26 December 2016 in urban Lanzhou, a semi-arid valley city of northwest China. The traffic control measures provided an invaluable opportunity to evaluate its effects on urban air quality in less developed cities of northwest China. Based on measured simultaneously air pollutants and meteorological parameters, the abatement of traffic-related pollutants induced by the implemented control measures such as CO, PM2.5 and PM10 (the particulate matter with diameter less than 2.5 μm and 10 μm) concentrations were firstly quantified by comparing the air quality data in urban areas with those in rural areas (uncontrolled zones). The concentrations of CO, NO2 from motor vehicles and fine particulate matter (PM2.5) were shown to have significant decreases of 15%-23% during traffic control period from those measured before control period with hourly maximum CO, PM2.5, and NO2/SO2 reduction of 43%, 35% and 141.4%, respectively. The influence of the control measures on AQI (air quality index) and ozone was less as compared to its effect on other air pollutants. Therefore, to alleviate serious winter haze pollution in China and to protect human health, the stringent long-term and large-scale even-odd license plate controlled plan should be implemented aperiodically in urban areas, especially for the periods with poor diffusion conditions.

  7. Open-air direct current plasma jet: Scaling up, uniformity, and cellular control

    NASA Astrophysics Data System (ADS)

    Wu, S.; Wang, Z.; Huang, Q.; Lu, X.; Ostrikov, K.

    2012-10-01

    Atmospheric-pressure plasma jets are commonly used in many fields from medicine to nanotechnology, yet the issue of scaling the discharges up to larger areas without compromising the plasma uniformity remains a major challenge. In this paper, we demonstrate a homogenous cold air plasma glow with a large cross-section generated by a direct current power supply. There is no risk of glow-to-arc transitions, and the plasma glow appears uniform regardless of the gap between the nozzle and the surface being processed. Detailed studies show that both the position of the quartz tube and the gas flow rate can be used to control the plasma properties. Further investigation indicates that the residual charges trapped on the inner surface of the quartz tube may be responsible for the generation of the air plasma plume with a large cross-section. The spatially resolved optical emission spectroscopy reveals that the air plasma plume is uniform as it propagates out of the nozzle. The remarkable improvement of the plasma uniformity is used to improve the bio-compatibility of a glass coverslip over a reasonably large area. This improvement is demonstrated by a much more uniform and effective attachment and proliferation of human embryonic kidney 293 (HEK 293) cells on the plasma-treated surface.

  8. Large-scale physical activity data reveal worldwide activity inequality

    PubMed Central

    Althoff, Tim; Sosič, Rok; Hicks, Jennifer L.; King, Abby C.; Delp, Scott L.; Leskovec, Jure

    2018-01-01

    Understanding the basic principles that govern physical activity is needed to curb the global pandemic of physical inactivity1–7 and the 5.3 million deaths per year associated with in-activity2. Our knowledge, however, remains limited owing to the lack of large-scale measurements of physical activity patterns across free-living populations worldwide1, 6. Here, we leverage the wide usage of smartphones with built-in accelerometry to measure physical activity at planetary scale. We study a dataset consisting of 68 million days of physical activity for 717,527 people, giving us a window into activity in 111 countries across the globe. We find inequality in how activity is distributed within countries and that this inequality is a better predictor of obesity prevalence in the population than average activity volume. Reduced activity in females contributes to a large portion of the observed activity inequality. Aspects of the built environment, such as the walkability of a city, were associated with less gender gap in activity and activity inequality. In more walkable cities, activity is greater throughout the day and throughout the week, across age, gender, and body mass index (BMI) groups, with the greatest increases in activity for females. Our findings have implications for global public health policy and urban planning and highlight the role of activity inequality and the built environment for improving physical activity and health. PMID:28693034

  9. Large-Scale Hybrid Motor Testing. Chapter 10

    NASA Technical Reports Server (NTRS)

    Story, George

    2006-01-01

    Hybrid rocket motors can be successfully demonstrated at a small scale virtually anywhere. There have been many suitcase sized portable test stands assembled for demonstration of hybrids. They show the safety of hybrid rockets to the audiences. These small show motors and small laboratory scale motors can give comparative burn rate data for development of different fuel/oxidizer combinations, however questions that are always asked when hybrids are mentioned for large scale applications are - how do they scale and has it been shown in a large motor? To answer those questions, large scale motor testing is required to verify the hybrid motor at its true size. The necessity to conduct large-scale hybrid rocket motor tests to validate the burn rate from the small motors to application size has been documented in several place^'^^.^. Comparison of small scale hybrid data to that of larger scale data indicates that the fuel burn rate goes down with increasing port size, even with the same oxidizer flux. This trend holds for conventional hybrid motors with forward oxidizer injection and HTPB based fuels. While the reason this is occurring would make a great paper or study or thesis, it is not thoroughly understood at this time. Potential causes include the fact that since hybrid combustion is boundary layer driven, the larger port sizes reduce the interaction (radiation, mixing and heat transfer) from the core region of the port. This chapter focuses on some of the large, prototype sized testing of hybrid motors. The largest motors tested have been AMROC s 250K-lbf thrust motor at Edwards Air Force Base and the Hybrid Propulsion Demonstration Program s 250K-lbf thrust motor at Stennis Space Center. Numerous smaller tests were performed to support the burn rate, stability and scaling concepts that went into the development of those large motors.

  10. Rhythms of Consciousness: Binocular Rivalry Reveals Large-Scale Oscillatory Network Dynamics Mediating Visual Perception

    PubMed Central

    Doesburg, Sam M.; Green, Jessica J.; McDonald, John J.; Ward, Lawrence M.

    2009-01-01

    Consciousness has been proposed to emerge from functionally integrated large-scale ensembles of gamma-synchronous neural populations that form and dissolve at a frequency in the theta band. We propose that discrete moments of perceptual experience are implemented by transient gamma-band synchronization of relevant cortical regions, and that disintegration and reintegration of these assemblies is time-locked to ongoing theta oscillations. In support of this hypothesis we provide evidence that (1) perceptual switching during binocular rivalry is time-locked to gamma-band synchronizations which recur at a theta rate, indicating that the onset of new conscious percepts coincides with the emergence of a new gamma-synchronous assembly that is locked to an ongoing theta rhythm; (2) localization of the generators of these gamma rhythms reveals recurrent prefrontal and parietal sources; (3) theta modulation of gamma-band synchronization is observed between and within the activated brain regions. These results suggest that ongoing theta-modulated-gamma mechanisms periodically reintegrate a large-scale prefrontal-parietal network critical for perceptual experience. Moreover, activation and network inclusion of inferior temporal cortex and motor cortex uniquely occurs on the cycle immediately preceding responses signaling perceptual switching. This suggests that the essential prefrontal-parietal oscillatory network is expanded to include additional cortical regions relevant to tasks and perceptions furnishing consciousness at that moment, in this case image processing and response initiation, and that these activations occur within a time frame consistent with the notion that conscious processes directly affect behaviour. PMID:19582165

  11. Extreme air pollution events in Hokkaido, Japan, traced back to early snowmelt and large-scale wildfires over East Eurasia: Case studies.

    PubMed

    Yasunari, Teppei J; Kim, Kyu-Myong; da Silva, Arlindo M; Hayasaki, Masamitsu; Akiyama, Masayuki; Murao, Naoto

    2018-04-25

    To identify the unusual climate conditions and their connections to air pollutions in a remote area due to wildfires, we examine three anomalous large-scale wildfires in May 2003, April 2008, and July 2014 over East Eurasia, as well as how products of those wildfires reached an urban city, Sapporo, in the northern part of Japan (Hokkaido), significantly affecting the air quality. NASA's MERRA-2 (the Modern-Era Retrospective analysis for Research and Applications, Version 2) aerosol re-analysis data closely reproduced the PM 2.5 variations in Sapporo for the case of smoke arrival in July 2014. Results show that all three cases featured unusually early snowmelt in East Eurasia, accompanied by warmer and drier surface conditions in the months leading to the fires, inducing long-lasting soil dryness and producing climate and environmental conditions conducive to active wildfires. Due to prevailing anomalous synoptic-scale atmospheric motions, smoke from those fires eventually reached a remote area, Hokkaido, and worsened the air quality in Sapporo. In future studies, continuous monitoring of the timing of Eurasian snowmelt and the air quality from the source regions to remote regions, coupled with the analysis of atmospheric and surface conditions, may be essential in more accurately predicting the effects of wildfires on air quality.

  12. Relationship between climate extremes in Romania and their connection to large-scale air circulation

    NASA Astrophysics Data System (ADS)

    Barbu, Nicu; Ştefan, Sabina

    2015-04-01

    The aim of this paper is to investigate the connection between climate extremes (temperature and precipitation) in Romania and large-scale air circulation. Daily observational data of maximum air temperature and amount of precipitation for the period 1961-2010 were used to compute two seasonal indices associated with temperature and precipitation, quantifying their frequency, as follows: frequency of very warm days (FTmax90 ≥ 90th percentile), frequency of very wet days (FPp90; daily precipitation amount ≥ 90th percentile). Seasonally frequency of circulation types were calculated from daily circulation types determined by using two objective catalogues (GWT - GrossWetter-Typen and WLK - WetterLargenKlassifikation) from the COST733Action. Daily reanalysis data sets (sea level pressure, geopotential height at 925 and 500 hPa, u and v components of wind vector at 700 hPa and precipitable water content for the entire atmospheric column) build up by NCEP/NCAR, with 2.5°/2.5° lat/lon spatial resolution, were used to determine the circulation types. In order to select the optimal domain size related to the FTmax90 and the FPp90, the explained variance (EV) has been used. The EV determines the relation between the variance among circulation types and the total variance of the variable under consideration. This method quantifies the discriminatory power of a classification. The relationships between climate extremes in Romania and large-scale air circulation were investigated by using multiple linear regression model (MLRM), the predictands are FTmax90 and FPp90 and the circulation types were used as predictors. In order to select the independent predictors to build the MLRM the collinearity and multicollinearity analysis were performed. The study period is dividend in two periods: the period 1961-2000 is used to train the MLRM and the period 2001-2010 is used to validate the MLRM. The analytical relationship obtained by using MLRM can be used for future projection

  13. 78 FR 11632 - Record of Decision for Land Acquisition and Airspace Establishment To Support Large-Scale Marine...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-02-19

    ... Establishment To Support Large-Scale Marine Air Ground Task Force Live- Fire and Maneuver Training at the Marine...), announces its decision to establish a large-scale Marine Air Ground Task Force (MAGTF) training facility at... through the Federal Aviation Administration the establishment and modification of military Special Use...

  14. Evolution of scaling emergence in large-scale spatial epidemic spreading.

    PubMed

    Wang, Lin; Li, Xiang; Zhang, Yi-Qing; Zhang, Yan; Zhang, Kan

    2011-01-01

    Zipf's law and Heaps' law are two representatives of the scaling concepts, which play a significant role in the study of complexity science. The coexistence of the Zipf's law and the Heaps' law motivates different understandings on the dependence between these two scalings, which has still hardly been clarified. In this article, we observe an evolution process of the scalings: the Zipf's law and the Heaps' law are naturally shaped to coexist at the initial time, while the crossover comes with the emergence of their inconsistency at the larger time before reaching a stable state, where the Heaps' law still exists with the disappearance of strict Zipf's law. Such findings are illustrated with a scenario of large-scale spatial epidemic spreading, and the empirical results of pandemic disease support a universal analysis of the relation between the two laws regardless of the biological details of disease. Employing the United States domestic air transportation and demographic data to construct a metapopulation model for simulating the pandemic spread at the U.S. country level, we uncover that the broad heterogeneity of the infrastructure plays a key role in the evolution of scaling emergence. The analyses of large-scale spatial epidemic spreading help understand the temporal evolution of scalings, indicating the coexistence of the Zipf's law and the Heaps' law depends on the collective dynamics of epidemic processes, and the heterogeneity of epidemic spread indicates the significance of performing targeted containment strategies at the early time of a pandemic disease.

  15. The influence of large-scale wind power on global climate.

    PubMed

    Keith, David W; Decarolis, Joseph F; Denkenberger, David C; Lenschow, Donald H; Malyshev, Sergey L; Pacala, Stephen; Rasch, Philip J

    2004-11-16

    Large-scale use of wind power can alter local and global climate by extracting kinetic energy and altering turbulent transport in the atmospheric boundary layer. We report climate-model simulations that address the possible climatic impacts of wind power at regional to global scales by using two general circulation models and several parameterizations of the interaction of wind turbines with the boundary layer. We find that very large amounts of wind power can produce nonnegligible climatic change at continental scales. Although large-scale effects are observed, wind power has a negligible effect on global-mean surface temperature, and it would deliver enormous global benefits by reducing emissions of CO(2) and air pollutants. Our results may enable a comparison between the climate impacts due to wind power and the reduction in climatic impacts achieved by the substitution of wind for fossil fuels.

  16. Iron-Air Rechargeable Battery: A Robust and Inexpensive Iron-Air Rechargeable Battery for Grid-Scale Energy Storage

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

    None

    2010-10-01

    GRIDS Project: USC is developing an iron-air rechargeable battery for large-scale energy storage that could help integrate renewable energy sources into the electric grid. Iron-air batteries have the potential to store large amounts of energy at low cost—iron is inexpensive and abundant, while oxygen is freely obtained from the air we breathe. However, current iron-air battery technologies have suffered from low efficiency and short life spans. USC is working to dramatically increase the efficiency of the battery by placing chemical additives on the battery’s iron-based electrode and restructuring the catalysts at the molecular level on the battery’s air-based electrode. Thismore » can help the battery resist degradation and increase life span. The goal of the project is to develop a prototype iron-air battery at significantly cost lower than today’s best commercial batteries.« less

  17. Large-Scale Sidereal Anisotropy of Galactic Cosmic-Ray Intensity Observed by the Tibet Air Shower Array

    NASA Astrophysics Data System (ADS)

    Amenomori, M.; Ayabe, S.; Cui, S. W.; Danzengluobu; Ding, L. K.; Ding, X. H.; Feng, C. F.; Feng, Z. Y.; Gao, X. Y.; Geng, Q. X.; Guo, H. W.; He, H. H.; He, M.; Hibino, K.; Hotta, N.; Hu, Haibing; Hu, H. B.; Huang, J.; Huang, Q.; Jia, H. Y.; Kajino, F.; Kasahara, K.; Katayose, Y.; Kato, C.; Kawata, K.; Labaciren; Le, G. M.; Li, J. Y.; Lu, H.; Lu, S. L.; Meng, X. R.; Mizutani, K.; Mu, J.; Munakata, K.; Nagai, A.; Nanjo, H.; Nishizawa, M.; Ohnishi, M.; Ohta, I.; Onuma, H.; Ouchi, T.; Ozawa, S.; Ren, J. R.; Saito, T.; Sakata, M.; Sasaki, T.; Shibata, M.; Shiomi, A.; Shirai, T.; Sugimoto, H.; Takita, M.; Tan, Y. H.; Tateyama, N.; Torii, S.; Tsuchiya, H.; Udo, S.; Utsugi, T.; Wang, B. S.; Wang, H.; Wang, X.; Wang, Y. G.; Wu, H. R.; Xue, L.; Yamamoto, Y.; Yan, C. T.; Yang, X. C.; Yasue, S.; Ye, Z. H.; Yu, G. C.; Yuan, A. F.; Yuda, T.; Zhang, H. M.; Zhang, J. L.; Zhang, N. J.; Zhang, X. Y.; Zhang, Y.; Zhang, Yi; Zhaxisangzhu; Zhou, X. X.; Tibet Asγ Collaboration

    2005-06-01

    We present the large-scale sidereal anisotropy of Galactic cosmic-ray intensity in the multi-TeV region observed with the Tibet-III air shower array during the period from 1999 through 2003. The sidereal daily variation of cosmic rays observed in this experiment shows an excess of relative intensity around 4-7 hr local sidereal time as well as a deficit around 12 hr local sidereal time. While the amplitude of the excess is not significant when averaged over all declinations, the excess in individual declination bands becomes larger and clearer as the viewing direction moves toward the south. The maximum phase of the excess intensity changes from ~7 hr at the Northern Hemisphere to ~4 hr at the equatorial region. We also show that both the amplitude and the phase of the first harmonic vector of the daily variation are remarkably independent of primary energy in the multi-TeV region. This is the first result determining the energy and declination dependences of the full 24 hr profiles of the sidereal daily variation in the multi-TeV region with a single air shower experiment.

  18. Large-scale analysis reveals populational contributions of cortical spike rate and synchrony to behavioural functions.

    PubMed

    Kimura, Rie; Saiki, Akiko; Fujiwara-Tsukamoto, Yoko; Sakai, Yutaka; Isomura, Yoshikazu

    2017-01-01

    spike synchrony does exist, and that some neuron pairs exhibit a dependence on movement phase during task performance. However, the population-wide analysis revealed that spike synchrony was statistically independent of the movement phase and the spike rate-based preferences of the pair for behavioural functions, whereas spike rates were clearly dependent on the movement phase. In fact, mutual information analyses revealed that the contribution of spike synchrony to the behavioural functions was small relative to the contribution of spike rate. Our large-scale analysis revealed that cortical spike rate, rather than spike synchrony, contributes to population coding for movement. © 2016 The Authors. The Journal of Physiology © 2016 The Physiological Society.

  19. Evolution of Scaling Emergence in Large-Scale Spatial Epidemic Spreading

    PubMed Central

    Wang, Lin; Li, Xiang; Zhang, Yi-Qing; Zhang, Yan; Zhang, Kan

    2011-01-01

    Background Zipf's law and Heaps' law are two representatives of the scaling concepts, which play a significant role in the study of complexity science. The coexistence of the Zipf's law and the Heaps' law motivates different understandings on the dependence between these two scalings, which has still hardly been clarified. Methodology/Principal Findings In this article, we observe an evolution process of the scalings: the Zipf's law and the Heaps' law are naturally shaped to coexist at the initial time, while the crossover comes with the emergence of their inconsistency at the larger time before reaching a stable state, where the Heaps' law still exists with the disappearance of strict Zipf's law. Such findings are illustrated with a scenario of large-scale spatial epidemic spreading, and the empirical results of pandemic disease support a universal analysis of the relation between the two laws regardless of the biological details of disease. Employing the United States domestic air transportation and demographic data to construct a metapopulation model for simulating the pandemic spread at the U.S. country level, we uncover that the broad heterogeneity of the infrastructure plays a key role in the evolution of scaling emergence. Conclusions/Significance The analyses of large-scale spatial epidemic spreading help understand the temporal evolution of scalings, indicating the coexistence of the Zipf's law and the Heaps' law depends on the collective dynamics of epidemic processes, and the heterogeneity of epidemic spread indicates the significance of performing targeted containment strategies at the early time of a pandemic disease. PMID:21747932

  20. Large Scale Variability of Mid-Tropospheric Carbon Dioxide as Observed by the Atmospheric Infrared Sounder (AIRS) on the NASA EOS Aqua Platform

    NASA Technical Reports Server (NTRS)

    Pagano, Thomas S.; Olsen, Edward T.

    2012-01-01

    The Atmospheric Infrared Sounder (AIRS) is a hyperspectral infrared instrument on the EOS Aqua Spacecraft, launched on May 4, 2002. AIRS has 2378 infrared channels ranging from 3.7 microns to 15.4 microns and a 13.5 km footprint. AIRS, in conjunction with the Advanced Microwave Sounding Unit (AMSU), produces temperature profiles with 1K/km accuracy, water vapor profiles (20%/2km), infrared cloud height and fraction, and trace gas amounts for CO2, CO, SO2, O3 and CH4 in the mid to upper troposphere. AIRS wide swath(cedilla) +/-49.5 deg , enables daily global daily coverage for over 95% of the Earth's surface. AIRS data are used for weather forecasting, validating climate model distribution and processes, and observing long-range transport of greenhouse gases. In this study, we examine the large scale and regional horizontal variability in the AIRS Mid-tropospheric Carbon Dioxide product as a function of season and associate the observed variability with known atmospheric transport processes, and sources and sinks of CO2.

  1. Toward Instructional Leadership: Principals' Perceptions of Large-Scale Assessment in Schools

    ERIC Educational Resources Information Center

    Prytula, Michelle; Noonan, Brian; Hellsten, Laurie

    2013-01-01

    This paper describes a study of the perceptions that Saskatchewan school principals have regarding large-scale assessment reform and their perceptions of how assessment reform has affected their roles as principals. The findings revealed that large-scale assessments, especially provincial assessments, have affected the principal in Saskatchewan…

  2. Cloud-based large-scale air traffic flow optimization

    NASA Astrophysics Data System (ADS)

    Cao, Yi

    The ever-increasing traffic demand makes the efficient use of airspace an imperative mission, and this paper presents an effort in response to this call. Firstly, a new aggregate model, called Link Transmission Model (LTM), is proposed, which models the nationwide traffic as a network of flight routes identified by origin-destination pairs. The traversal time of a flight route is assumed to be the mode of distribution of historical flight records, and the mode is estimated by using Kernel Density Estimation. As this simplification abstracts away physical trajectory details, the complexity of modeling is drastically decreased, resulting in efficient traffic forecasting. The predicative capability of LTM is validated against recorded traffic data. Secondly, a nationwide traffic flow optimization problem with airport and en route capacity constraints is formulated based on LTM. The optimization problem aims at alleviating traffic congestions with minimal global delays. This problem is intractable due to millions of variables. A dual decomposition method is applied to decompose the large-scale problem such that the subproblems are solvable. However, the whole problem is still computational expensive to solve since each subproblem is an smaller integer programming problem that pursues integer solutions. Solving an integer programing problem is known to be far more time-consuming than solving its linear relaxation. In addition, sequential execution on a standalone computer leads to linear runtime increase when the problem size increases. To address the computational efficiency problem, a parallel computing framework is designed which accommodates concurrent executions via multithreading programming. The multithreaded version is compared with its monolithic version to show decreased runtime. Finally, an open-source cloud computing framework, Hadoop MapReduce, is employed for better scalability and reliability. This framework is an "off-the-shelf" parallel computing model

  3. Large-scale weather dynamics during the 2015 haze event in Singapore

    NASA Astrophysics Data System (ADS)

    Djamil, Yudha; Lee, Wen-Chien; Tien Dat, Pham; Kuwata, Mikinori

    2017-04-01

    The 2015 haze event in South East Asia is widely considered as a period of the worst air quality in the region in more than a decade. The source of the haze was from forest and peatland fire in Sumatra and Kalimantan Islands, Indonesia. The fires were mostly came from the practice of forest clearance known as slash and burn, to be converted to palm oil plantation. Such practice of clearance although occurs seasonally but at 2015 it became worst by the impact of strong El Nino. The long period of dryer atmosphere over the region due to El Nino makes the fire easier to ignite, spread and difficult to stop. The biomass emission from the forest and peatland fire caused large-scale haze pollution problem in both Islands and further spread into the neighboring countries such as Singapore and Malaysia. In Singapore, for about two months (September-October, 2015) the air quality was in the unhealthy level. Such unfortunate condition caused some socioeconomic losses such as school closure, cancellation of outdoor events, health issues and many more with total losses estimated as S700 million. The unhealthy level of Singapore's air quality is based on the increasing pollutant standard index (PSI>120) due to the haze arrival, it even reached a hazardous level (PSI= 300) for several days. PSI is a metric of air quality in Singapore that aggregate six pollutants (SO2, PM10, PM2.5, NO2, CO and O3). In this study, we focused on PSI variability in weekly-biweekly time scales (periodicity < 30 days) since it is the least understood compare to their diurnal and seasonal scales. We have identified three dominant time scales of PSI ( 5, 10 and 20 days) using Wavelet method and investigated their large-scale atmospheric structures. The PSI associated large-scale column moisture horizontal structures over the Indo-Pacific basin are dominated by easterly propagating gyres in synoptic (macro) scale for the 5 days ( 10 and 20 days) time scales. The propagating gyres manifest as cyclical

  4. Large scale particle image velocimetry with helium filled soap bubbles

    NASA Astrophysics Data System (ADS)

    Bosbach, Johannes; Kühn, Matthias; Wagner, Claus

    2009-03-01

    The application of Particle Image Velocimetry (PIV) to measurement of flows on large scales is a challenging necessity especially for the investigation of convective air flows. Combining helium filled soap bubbles as tracer particles with high power quality switched solid state lasers as light sources allows conducting PIV on scales of the order of several square meters. The technique was applied to mixed convection in a full scale double aisle aircraft cabin mock-up for validation of Computational Fluid Dynamics simulations.

  5. Preservation of large-scale chromatin structure in FISH experiments

    PubMed Central

    Hepperger, Claudia; Otten, Simone; von Hase, Johann

    2006-01-01

    The nuclear organization of specific endogenous chromatin regions can be investigated only by fluorescence in situ hybridization (FISH). One of the two fixation procedures is typically applied: (1) buffered formaldehyde or (2) hypotonic shock with methanol acetic acid fixation followed by dropping of nuclei on glass slides and air drying. In this study, we compared the effects of these two procedures and some variations on nuclear morphology and on FISH signals. We analyzed mouse erythroleukemia and mouse embryonic stem cells because their clusters of subcentromeric heterochromatin provide an easy means to assess preservation of chromatin. Qualitative and quantitative analyses revealed that formaldehyde fixation provided good preservation of large-scale chromatin structures, while classical methanol acetic acid fixation after hypotonic treatment severely impaired nuclear shape and led to disruption of chromosome territories, heterochromatin structures, and large transgene arrays. Our data show that such preparations do not faithfully reflect in vivo nuclear architecture. Electronic supplementary material Supplementary material is available in the online version of this article at http://dx.doi.org/10.1007/s00412-006-0084-2 and is accessible for authorized users. PMID:17119992

  6. Allometric scaling of UK urban emissions: interpretation and implications for air quality management

    NASA Astrophysics Data System (ADS)

    MacKenzie, Rob; Barnes, Matt; Whyatt, Duncan; Hewitt, Nick

    2016-04-01

    Allometry uncovers structures and patterns by relating the characteristics of complex systems to a measure of scale. We present an allometric analysis of air quality for UK urban settlements, beginning with emissions and moving on to consider air concentrations. We consider both airshed-average 'urban background' concentrations (cf. those derived from satellites for NO2) and local pollution 'hotspots'. We show that there is a strong and robust scaling (with respect to population) of the non-point-source emissions of the greenhouse gases carbon dioxide and methane, as well as the toxic pollutants nitrogen dioxide, PM2.5, and 1,3-butadiene. The scaling of traffic-related emissions is not simply a reflection of road length, but rather results from the socio-economic patterning of road-use. The recent controversy regarding diesel vehicle emissions is germane to our study but does not affect our overall conclusions. We next develop an hypothesis for the population-scaling of airshed-average air concentrations, with which we demonstrate that, although average air quality is expected to be worse in large urban centres compared to small urban centres, the overall effect is an economy of scale (i.e., large cities reduce the overall burden of emissions compared to the same population spread over many smaller urban settlements). Our hypothesis explains satellite-derived observations of airshed-average urban NO2 concentrations. The theory derived also explains which properties of nature-based solutions (urban greening) can make a significant contribution at city scale, and points to a hitherto unforeseen opportunity to make large cities cleaner than smaller cities in absolute terms with respect to their airshed-average pollutant concentration.

  7. Large-Scale Cognitive GWAS Meta-Analysis Reveals Tissue-Specific Neural Expression and Potential Nootropic Drug Targets.

    PubMed

    Lam, Max; Trampush, Joey W; Yu, Jin; Knowles, Emma; Davies, Gail; Liewald, David C; Starr, John M; Djurovic, Srdjan; Melle, Ingrid; Sundet, Kjetil; Christoforou, Andrea; Reinvang, Ivar; DeRosse, Pamela; Lundervold, Astri J; Steen, Vidar M; Espeseth, Thomas; Räikkönen, Katri; Widen, Elisabeth; Palotie, Aarno; Eriksson, Johan G; Giegling, Ina; Konte, Bettina; Roussos, Panos; Giakoumaki, Stella; Burdick, Katherine E; Payton, Antony; Ollier, William; Chiba-Falek, Ornit; Attix, Deborah K; Need, Anna C; Cirulli, Elizabeth T; Voineskos, Aristotle N; Stefanis, Nikos C; Avramopoulos, Dimitrios; Hatzimanolis, Alex; Arking, Dan E; Smyrnis, Nikolaos; Bilder, Robert M; Freimer, Nelson A; Cannon, Tyrone D; London, Edythe; Poldrack, Russell A; Sabb, Fred W; Congdon, Eliza; Conley, Emily Drabant; Scult, Matthew A; Dickinson, Dwight; Straub, Richard E; Donohoe, Gary; Morris, Derek; Corvin, Aiden; Gill, Michael; Hariri, Ahmad R; Weinberger, Daniel R; Pendleton, Neil; Bitsios, Panos; Rujescu, Dan; Lahti, Jari; Le Hellard, Stephanie; Keller, Matthew C; Andreassen, Ole A; Deary, Ian J; Glahn, David C; Malhotra, Anil K; Lencz, Todd

    2017-11-28

    Here, we present a large (n = 107,207) genome-wide association study (GWAS) of general cognitive ability ("g"), further enhanced by combining results with a large-scale GWAS of educational attainment. We identified 70 independent genomic loci associated with general cognitive ability. Results showed significant enrichment for genes causing Mendelian disorders with an intellectual disability phenotype. Competitive pathway analysis implicated the biological processes of neurogenesis and synaptic regulation, as well as the gene targets of two pharmacologic agents: cinnarizine, a T-type calcium channel blocker, and LY97241, a potassium channel inhibitor. Transcriptome-wide and epigenome-wide analysis revealed that the implicated loci were enriched for genes expressed across all brain regions (most strongly in the cerebellum). Enrichment was exclusive to genes expressed in neurons but not oligodendrocytes or astrocytes. Finally, we report genetic correlations between cognitive ability and disparate phenotypes including psychiatric disorders, several autoimmune disorders, longevity, and maternal age at first birth. Copyright © 2017 The Author(s). Published by Elsevier Inc. All rights reserved.

  8. Revealing the Hidden Relationship by Sparse Modules in Complex Networks with a Large-Scale Analysis

    PubMed Central

    Jiao, Qing-Ju; Huang, Yan; Liu, Wei; Wang, Xiao-Fan; Chen, Xiao-Shuang; Shen, Hong-Bin

    2013-01-01

    One of the remarkable features of networks is module that can provide useful insights into not only network organizations but also functional behaviors between their components. Comprehensive efforts have been devoted to investigating cohesive modules in the past decade. However, it is still not clear whether there are important structural characteristics of the nodes that do not belong to any cohesive module. In order to answer this question, we performed a large-scale analysis on 25 complex networks with different types and scales using our recently developed BTS (bintree seeking) algorithm, which is able to detect both cohesive and sparse modules in the network. Our results reveal that the sparse modules composed by the cohesively isolated nodes widely co-exist with the cohesive modules. Detailed analysis shows that both types of modules provide better characterization for the division of a network into functional units than merely cohesive modules, because the sparse modules possibly re-organize the nodes in the so-called cohesive modules, which lack obvious modular significance, into meaningful groups. Compared with cohesive modules, the sizes of sparse ones are generally smaller. Sparse modules are also found to have preferences in social and biological networks than others. PMID:23762457

  9. Polymer Physics of the Large-Scale Structure of Chromatin.

    PubMed

    Bianco, Simona; Chiariello, Andrea Maria; Annunziatella, Carlo; Esposito, Andrea; Nicodemi, Mario

    2016-01-01

    We summarize the picture emerging from recently proposed models of polymer physics describing the general features of chromatin large scale spatial architecture, as revealed by microscopy and Hi-C experiments.

  10. NATIONAL-SCALE ASSESSMENT OF AIR TOXICS RISKS ...

    EPA Pesticide Factsheets

    The national-scale assessment of air toxics risks is a modeling assessment which combines emission inventory development, atmospheric fate and transport modeling, exposure modeling, and risk assessment to characterize the risk associated with inhaling air toxics from outdoor sources. This national-scale effort will be initiated for the base year 1996 and repeated every three years thereafter to track trends and inform program development. Provide broad-scale understanding of inhalation risks for a subset of atmospherically-emitted air toxics to inform further data-gathering efforts and priority-setting for the EPA's Air Toxics Programs.

  11. Scale-Free Networks and Commercial Air Carrier Transportation in the United States

    NASA Technical Reports Server (NTRS)

    Conway, Sheila R.

    2004-01-01

    Network science, or the art of describing system structure, may be useful for the analysis and control of large, complex systems. For example, networks exhibiting scale-free structure have been found to be particularly well suited to deal with environmental uncertainty and large demand growth. The National Airspace System may be, at least in part, a scalable network. In fact, the hub-and-spoke structure of the commercial segment of the NAS is an often-cited example of an existing scale-free network After reviewing the nature and attributes of scale-free networks, this assertion is put to the test: is commercial air carrier transportation in the United States well explained by this model? If so, are the positive attributes of these networks, e.g. those of efficiency, flexibility and robustness, fully realized, or could we effect substantial improvement? This paper first outlines attributes of various network types, then looks more closely at the common carrier air transportation network from perspectives of the traveler, the airlines, and Air Traffic Control (ATC). Network models are applied within each paradigm, including discussion of implied strengths and weaknesses of each model. Finally, known limitations of scalable networks are discussed. With an eye towards NAS operations, utilizing the strengths and avoiding the weaknesses of scale-free networks are addressed.

  12. Biohazards Assessment in Large-Scale Zonal Centrifugation

    PubMed Central

    Baldwin, C. L.; Lemp, J. F.; Barbeito, M. S.

    1975-01-01

    A study was conducted to determine the biohazards associated with use of the large-scale zonal centrifuge for purification of moderate risk oncogenic viruses. To safely and conveniently assess the hazard, coliphage T3 was substituted for the virus in a typical processing procedure performed in a National Cancer Institute contract laboratory. Risk of personnel exposure was found to be minimal during optimal operation but definite potential for virus release from a number of centrifuge components during mechanical malfunction was shown by assay of surface, liquid, and air samples collected during the processing. High concentration of phage was detected in the turbine air exhaust and the seal coolant system when faulty seals were employed. The simulant virus was also found on both centrifuge chamber interior and rotor surfaces. Images PMID:1124921

  13. Local-Scale Air Quality Modeling in Support of Human Health and Exposure Research (Invited)

    NASA Astrophysics Data System (ADS)

    Isakov, V.

    2010-12-01

    Spatially- and temporally-sparse information on air quality is a key concern for air-pollution-related environmental health studies. Monitor networks are sparse in both space and time, are costly to maintain, and are often designed purposely to avoid detecting highly localized sources. Recent studies have shown that more narrowly defining the geographic domain of the study populations and improvements in the measured/estimated ambient concentrations can lead to stronger associations between air pollution and hospital admissions and mortality records. Traditionally, ambient air quality measurements have been used as a primary input to support human health and exposure research. However, there is increasing evidence that the current ambient monitoring network is not capturing sharp gradients in exposure due to the presence of high concentration levels near, for example, major roadways. Many air pollutants exhibit large concentration gradients near large emitters such as major roadways, factories, ports, etc. To overcome these limitations, researchers are now beginning to use air quality models to support air pollution exposure and health studies. There are many advantages to using air quality models over traditional approaches based on existing ambient measurements alone. First, models can provide spatially- and temporally-resolved concentrations as direct input to exposure and health studies and thus better defining the concentration levels for the population in the geographic domain. Air quality models have a long history of use in air pollution regulations, and supported by regulatory agencies and a large user community. Also, models can provide bidirectional linkages between sources of emissions and ambient concentrations, thus allowing exploration of various mitigation strategies to reduce risk to exposure. In order to provide best estimates of air concentrations to support human health and exposure studies, model estimates should consider local-scale features

  14. Acoustic telemetry reveals large-scale migration patterns of walleye in Lake Huron

    USGS Publications Warehouse

    Hayden, Todd A.; Holbrook, Christopher; Fielder, David G.; Vandergoot, Christopher S.; Bergstedt, Roger A.; Dettmers, John M.; Krueger, Charles C.; Cooke, Steven J.

    2014-01-01

    Fish migration in large freshwater lacustrine systems such as the Laurentian Great Lakes is not well understood. The walleye (Sander vitreus) is an economically and ecologically important native fish species throughout the Great Lakes. In Lake Huron walleye has recently undergone a population expansion as a result of recovery of the primary stock, stemming from changing food web dynamics. During 2011 and 2012, we used acoustic telemetry to document the timing and spatial scale of walleye migration in Lake Huron and Saginaw Bay. Spawning walleye (n = 199) collected from a tributary of Saginaw Bay were implanted with acoustic tags and their migrations were documented using acoustic receivers (n = 140) deployed throughout U.S. nearshore waters of Lake Huron. Three migration pathways were described using multistate mark-recapture models. Models were evaluated using the Akaike Information Criterion. Fish sex did not influence migratory behavior but did affect migration rate and walleye were detected on all acoustic receiver lines. Most (95%) tagged fish migrated downstream from the riverine tagging and release location to Saginaw Bay, and 37% of these fish emigrated from Saginaw Bay into Lake Huron. Remarkably, 8% of walleye that emigrated from Saginaw Bay were detected at the acoustic receiver line located farthest from the release location more than 350 km away. Most (64%) walleye returned to the Saginaw River in 2012, presumably for spawning. Our findings reveal that fish from this stock use virtually the entirety of U.S. nearshore waters of Lake Huron.

  15. Acoustic telemetry reveals large-scale migration patterns of walleye in Lake Huron.

    PubMed

    Hayden, Todd A; Holbrook, Christopher M; Fielder, David G; Vandergoot, Christopher S; Bergstedt, Roger A; Dettmers, John M; Krueger, Charles C; Cooke, Steven J

    2014-01-01

    Fish migration in large freshwater lacustrine systems such as the Laurentian Great Lakes is not well understood. The walleye (Sander vitreus) is an economically and ecologically important native fish species throughout the Great Lakes. In Lake Huron walleye has recently undergone a population expansion as a result of recovery of the primary stock, stemming from changing food web dynamics. During 2011 and 2012, we used acoustic telemetry to document the timing and spatial scale of walleye migration in Lake Huron and Saginaw Bay. Spawning walleye (n = 199) collected from a tributary of Saginaw Bay were implanted with acoustic tags and their migrations were documented using acoustic receivers (n = 140) deployed throughout U.S. nearshore waters of Lake Huron. Three migration pathways were described using multistate mark-recapture models. Models were evaluated using the Akaike Information Criterion. Fish sex did not influence migratory behavior but did affect migration rate and walleye were detected on all acoustic receiver lines. Most (95%) tagged fish migrated downstream from the riverine tagging and release location to Saginaw Bay, and 37% of these fish emigrated from Saginaw Bay into Lake Huron. Remarkably, 8% of walleye that emigrated from Saginaw Bay were detected at the acoustic receiver line located farthest from the release location more than 350 km away. Most (64%) walleye returned to the Saginaw River in 2012, presumably for spawning. Our findings reveal that fish from this stock use virtually the entirety of U.S. nearshore waters of Lake Huron.

  16. Satellite measurements of large-scale air pollution - Methods

    NASA Technical Reports Server (NTRS)

    Kaufman, Yoram J.; Ferrare, Richard A.; Fraser, Robert S.

    1990-01-01

    A technique for deriving large-scale pollution parameters from NIR and visible satellite remote-sensing images obtained over land or water is described and demonstrated on AVHRR images. The method is based on comparison of the upward radiances on clear and hazy days and permits simultaneous determination of aerosol optical thickness with error Delta tau(a) = 0.08-0.15, particle size with error + or - 100-200 nm, and single-scattering albedo with error + or - 0.03 (for albedos near 1), all assuming accurate and stable satellite calibration and stable surface reflectance between the clear and hazy days. In the analysis of AVHRR images of smoke from a forest fire, good agreement was obtained between satellite and ground-based (sun-photometer) measurements of aerosol optical thickness, but the satellite particle sizes were systematically greater than those measured from the ground. The AVHRR single-scattering albedo agreed well with a Landsat albedo for the same smoke.

  17. Interaction of a cumulus cloud ensemble with the large-scale environment

    NASA Technical Reports Server (NTRS)

    Arakawa, A.; Schubert, W.

    1973-01-01

    Large-scale modification of the environment by cumulus clouds is discussed in terms of entrainment, detrainment, evaporation, and subsidence. Drying, warming, and condensation by vertical displacement of air are considered as well as budget equations for mass, static energy, water vapor, and liquid water.

  18. Modeling large-scale adoption of intercropping as a sustainable agricultural practice for food security and air pollution mitigation around the globe

    NASA Astrophysics Data System (ADS)

    Fung, K. M.; Tai, A. P. K.; Yong, T.; Liu, X.

    2017-12-01

    The fast-growing world population will impose a severe pressure on our current global food production system. Meanwhile, boosting crop yield by increasing fertilizer use comes with a cascade of environmental problems including air pollution. In China, agricultural activities contribute to 95% of total ammonia emissions. Such emissions are attributable to 20% of the fine particulate matter (PM2.5) formed in the downwind regions, which imposes severe health risks to the citizens. Field studies of soybean intercropping have demonstrated its potential to enhance crop yield, lower fertilizer use, and thus reduce ammonia emissions by taking advantage of legume nitrogen fixation and enabling mutualistic crop-crop interactions between legumes and non-legume crops. In our work, we revise the process-based biogeochemical model, DeNitrification-DeComposition (DNDC) to capture the belowground interactions of intercropped crops and show that with intercropping, only 58% of fertilizer is required to yield the same maize production of its monoculture counterpart, corresponding to a reduction in ammonia emission by 43% over China. Using the GEOS-Chem global 3-D chemical transport model, we estimate that such ammonia reduction can lessen downwind inorganic PM2.5 by up to 2.1% (equivalent to 1.3 μg m-3), which saves the Chinese air pollution-related health costs by up to US$1.5 billion each year. With the more enhanced crop growth and land management algorithms in the Community Land Model (CLM), we also implement into CLM the new parametrization of the belowground interactions to simulate large-scale adoption of intercropping around the globe and study their beneficial effects on food production, fertilizer usage and ammonia reduction. This study can serve as a scientific basis for policy makers and intergovernmental organizations to consider promoting large-scale intercropping to maintain a sustainable global food supply to secure both future crop production and air quality.

  19. Air fluorescence detection of large air showers below the horizon

    NASA Technical Reports Server (NTRS)

    Halverson, P.; Bowen, T.

    1985-01-01

    In the interest of exploring the cosmic ray spectrum at energies greater than 10 to the 18th power eV, where flux rates at the Earth's surface drop below 100 yr(-1) km(-2) sr(-1), cosmic ray physicists have been forced to construct ever larger detectors in order to collect useful amounts of data in reasonable lengths of time. At present, the ultimate example of this trend is the Fly's Eye system in Utah, which uses the atmosphere around an array of skyward-looking photomultiplier tubes. The air acts as a scintillator to give detecting areas as large as 5000 square kilometers sr (for highest energy events). This experiment has revealed structure (and a possible cutoff) in the ultra-high energy region above 10 o the 19th power eV. The success of the Fly's Eye experiment provides impetus for continuing the development of larger detectors to make accessible even higher energies. However, due to the rapidly falling flux, a tenfold increase in observable energy would call for a hundredfold increase in the detecting area. But, the cost of expanding the Fly's Eye detecting area will approximately scale linearly with area. It is for these reasons that the authors have proposed a new approach to using the atmosphere as a scintillator; one which will require fewer photomultipliers, less hardware (thus being less extensive), yet will provide position and shower size information.

  20. Engineering a Large Scale Indium Nanodot Array for Refractive Index Sensing.

    PubMed

    Xu, Xiaoqing; Hu, Xiaolin; Chen, Xiaoshu; Kang, Yangsen; Zhang, Zhiping; B Parizi, Kokab; Wong, H-S Philip

    2016-11-23

    In this work, we developed a simple method to fabricate 12 × 4 mm 2 large scale nanostructure arrays and investigated the feasibility of indium nanodot (ND) array with different diameters and periods for refractive index sensing. Absorption resonances at multiple wavelengths from the visible to the near-infrared range were observed for various incident angles in a variety of media. Engineering the ND array with a centered square lattice, we successfully enhanced the sensitivity by 60% and improved the figure of merit (FOM) by 190%. The evolution of the resonance dips in the reflection spectra, of square lattice and centered square lattice, from air to water, matches well with the results of Lumerical FDTD simulation. The improvement of sensitivity is due to the enhancement of local electromagnetic field (E-field) near the NDs with centered square lattice, as revealed by E-field simulation at resonance wavelengths. The E-field is enhanced due to coupling between the two square ND arrays with [Formula: see text]x period at phase matching. This work illustrates an effective way to engineer and fabricate a refractive index sensor at a large scale. This is the first experimental demonstration of poor-metal (indium) nanostructure array for refractive index sensing. It also demonstrates a centered square lattice for higher sensitivity and as a better basic platform for more complex sensor designs.

  1. Modeling multi-scale aerosol dynamics and micro-environmental air quality near a large highway intersection using the CTAG model.

    PubMed

    Wang, Yan Jason; Nguyen, Monica T; Steffens, Jonathan T; Tong, Zheming; Wang, Yungang; Hopke, Philip K; Zhang, K Max

    2013-01-15

    A new methodology, referred to as the multi-scale structure, integrates "tailpipe-to-road" (i.e., on-road domain) and "road-to-ambient" (i.e., near-road domain) simulations to elucidate the environmental impacts of particulate emissions from traffic sources. The multi-scale structure is implemented in the CTAG model to 1) generate process-based on-road emission rates of ultrafine particles (UFPs) by explicitly simulating the effects of exhaust properties, traffic conditions, and meteorological conditions and 2) to characterize the impacts of traffic-related emissions on micro-environmental air quality near a highway intersection in Rochester, NY. The performance of CTAG, evaluated against with the field measurements, shows adequate agreement in capturing the dispersion of carbon monoxide (CO) and the number concentrations of UFPs in the near road micro-environment. As a proof-of-concept case study, we also apply CTAG to separate the relative impacts of the shutdown of a large coal-fired power plant (CFPP) and the adoption of the ultra-low-sulfur diesel (ULSD) on UFP concentrations in the intersection micro-environment. Although CTAG is still computationally expensive compared to the widely-used parameterized dispersion models, it has the potential to advance our capability to predict the impacts of UFP emissions and spatial/temporal variations of air pollutants in complex environments. Furthermore, for the on-road simulations, CTAG can serve as a process-based emission model; Combining the on-road and near-road simulations, CTAG becomes a "plume-in-grid" model for mobile emissions. The processed emission profiles can potentially improve regional air quality and climate predictions accordingly. Copyright © 2012 Elsevier B.V. All rights reserved.

  2. Large-scale structure of randomly jammed spheres

    NASA Astrophysics Data System (ADS)

    Ikeda, Atsushi; Berthier, Ludovic; Parisi, Giorgio

    2017-05-01

    We numerically analyze the density field of three-dimensional randomly jammed packings of monodisperse soft frictionless spherical particles, paying special attention to fluctuations occurring at large length scales. We study in detail the two-point static structure factor at low wave vectors in Fourier space. We also analyze the nature of the density field in real space by studying the large-distance behavior of the two-point pair correlation function, of density fluctuations in subsystems of increasing sizes, and of the direct correlation function. We show that such real space analysis can be greatly improved by introducing a coarse-grained density field to disentangle genuine large-scale correlations from purely local effects. Our results confirm that both Fourier and real space signatures of vanishing density fluctuations at large scale are absent, indicating that randomly jammed packings are not hyperuniform. In addition, we establish that the pair correlation function displays a surprisingly complex structure at large distances, which is however not compatible with the long-range negative correlation of hyperuniform systems but fully compatible with an analytic form for the structure factor. This implies that the direct correlation function is short ranged, as we also demonstrate directly. Our results reveal that density fluctuations in jammed packings do not follow the behavior expected for random hyperuniform materials, but display instead a more complex behavior.

  3. Acoustic Telemetry Reveals Large-Scale Migration Patterns of Walleye in Lake Huron

    PubMed Central

    Hayden, Todd A.; Holbrook, Christopher M.; Fielder, David G.; Vandergoot, Christopher S.; Bergstedt, Roger A.; Dettmers, John M.; Krueger, Charles C.; Cooke, Steven J.

    2014-01-01

    Fish migration in large freshwater lacustrine systems such as the Laurentian Great Lakes is not well understood. The walleye (Sander vitreus) is an economically and ecologically important native fish species throughout the Great Lakes. In Lake Huron walleye has recently undergone a population expansion as a result of recovery of the primary stock, stemming from changing food web dynamics. During 2011 and 2012, we used acoustic telemetry to document the timing and spatial scale of walleye migration in Lake Huron and Saginaw Bay. Spawning walleye (n = 199) collected from a tributary of Saginaw Bay were implanted with acoustic tags and their migrations were documented using acoustic receivers (n = 140) deployed throughout U.S. nearshore waters of Lake Huron. Three migration pathways were described using multistate mark-recapture models. Models were evaluated using the Akaike Information Criterion. Fish sex did not influence migratory behavior but did affect migration rate and walleye were detected on all acoustic receiver lines. Most (95%) tagged fish migrated downstream from the riverine tagging and release location to Saginaw Bay, and 37% of these fish emigrated from Saginaw Bay into Lake Huron. Remarkably, 8% of walleye that emigrated from Saginaw Bay were detected at the acoustic receiver line located farthest from the release location more than 350 km away. Most (64%) walleye returned to the Saginaw River in 2012, presumably for spawning. Our findings reveal that fish from this stock use virtually the entirety of U.S. nearshore waters of Lake Huron. PMID:25506913

  4. Metaproteomics reveals major microbial players and their biodegradation functions in a large-scale aerobic composting plant

    PubMed Central

    Liu, Dongming; Li, Mingxiao; Xi, Beidou; Zhao, Yue; Wei, Zimin; Song, Caihong; Zhu, Chaowei

    2015-01-01

    Composting is an appropriate management alternative for municipal solid waste; however, our knowledge about the microbial regulation of this process is still scare. We employed metaproteomics to elucidate the main biodegradation pathways in municipal solid waste composting system across the main phases in a large-scale composting plant. The investigation of microbial succession revealed that Bacillales, Actinobacteria and Saccharomyces increased significantly with respect to abundance in composting process. The key microbiologic population for cellulose degradation in different composting stages was different. Fungi were found to be the main producers of cellulase in earlier phase. However, the cellulolytic fungal communities were gradually replaced by a purely bacterial one in active phase, which did not support the concept that the thermophilic fungi are active through the thermophilic phase. The effective decomposition of cellulose required the synergy between bacteria and fungi in the curing phase. PMID:25989417

  5. Use of a large-scale rainfall simulator reveals novel insights into stemflow generation

    NASA Astrophysics Data System (ADS)

    Levia, D. F., Jr.; Iida, S. I.; Nanko, K.; Sun, X.; Shinohara, Y.; Sakai, N.

    2017-12-01

    Detailed knowledge of stemflow generation and its effects on both hydrological and biogoechemical cycling is important to achieve a holistic understanding of forest ecosystems. Field studies and a smaller set of experiments performed under laboratory conditions have increased our process-based knowledge of stemflow production. Building upon these earlier works, a large-scale rainfall simulator was employed to deepen our understanding of stemflow generation processes. The use of the large-scale rainfall simulator provides a unique opportunity to examine a range of rainfall intensities under constant conditions that are difficult under natural conditions due to the variable nature of rainfall intensities in the field. Stemflow generation and production was examined for three species- Cryptomeria japonica D. Don (Japanese cedar), Chamaecyparis obtusa (Siebold & Zucc.) Endl. (Japanese cypress), Zelkova serrata Thunb. (Japanese zelkova)- under both leafed and leafless conditions at several different rainfall intensities (15, 20, 30, 40, 50, and 100 mm h-1) using a large-scale rainfall simulator in National Research Institute for Earth Science and Disaster Resilience (Tsukuba, Japan). Stemflow production and rates and funneling ratios were examined in relation to both rainfall intensity and canopy structure. Preliminary results indicate a dynamic and complex response of the funneling ratios of individual trees to different rainfall intensities among the species examined. This is partly the result of different canopy structures, hydrophobicity of vegetative surfaces, and differential wet-up processes across species and rainfall intensities. This presentation delves into these differences and attempts to distill them into generalizable patterns, which can advance our theories of stemflow generation processes and ultimately permit better stewardship of forest resources. ________________ Funding note: This research was supported by JSPS Invitation Fellowship for Research in

  6. Large and small-scale structures in Saturn's rings

    NASA Astrophysics Data System (ADS)

    Albers, N.; Rehnberg, M. E.; Brown, Z. L.; Sremcevic, M.; Esposito, L. W.

    2017-09-01

    Observations made by the Cassini spacecraft have revealed both large and small scale structures in Saturn's rings in unprecedented detail. Analysis of high-resolution measurements by the Cassini Ultraviolet Spectrograph (UVIS) High Speed Photometer (HSP) and the Imaging Science Subsystem (ISS) show an abundance of intrinsic small-scale structures (or clumping) seen across the entire ring system. These include self-gravity wakes (50-100m), sub-km structure at the A and B ring edges, and "straw"/"ropy" structures (1-3km).

  7. Large-scale Fractal Motion of Clouds

    NASA Image and Video Library

    2011-04-20

    waters surrounding the island.) The “swallowed” gulps of clear island air get carried along within the vortices, but these are soon mixed into the surrounding clouds. Landsat is unique in its ability to image both the small-scale eddies that mix clear and cloudy air, down to the 30 meter pixel size of Landsat, but also having a wide enough field-of-view, 180 km, to reveal the connection of the turbulence to large-scale flows such as the subtropical oceanic gyres. Landsat 7, with its new onboard digital recorder, has extended this capability away from the few Landsat ground stations to remote areas such as Alejandro Island, and thus is gradually providing a global dynamic picture of evolving human-scale phenomena. For more details on von Karman vortices, refer to climate.gsfc.nasa.gov/~cahalan. Image and caption courtesy Bob Cahalan, NASA GSFC Instrument: Landsat 7 - ETM+ Credit: NASA/GSFC/Landsat NASA Goddard Space Flight Center enables NASA’s mission through four scientific endeavors: Earth Science, Heliophysics, Solar System Exploration, and Astrophysics. Goddard plays a leading role in NASA’s accomplishments by contributing compelling scientific knowledge to advance the Agency’s mission. Follow us on Twitter Join us on Facebook

  8. Instantaneous variance scaling of AIRS thermodynamic profiles using a circular area Monte Carlo approach

    NASA Astrophysics Data System (ADS)

    Dorrestijn, Jesse; Kahn, Brian H.; Teixeira, João; Irion, Fredrick W.

    2018-05-01

    Satellite observations are used to obtain vertical profiles of variance scaling of temperature (T) and specific humidity (q) in the atmosphere. A higher spatial resolution nadir retrieval at 13.5 km complements previous Atmospheric Infrared Sounder (AIRS) investigations with 45 km resolution retrievals and enables the derivation of power law scaling exponents to length scales as small as 55 km. We introduce a variable-sized circular-area Monte Carlo methodology to compute exponents instantaneously within the swath of AIRS that yields additional insight into scaling behavior. While this method is approximate and some biases are likely to exist within non-Gaussian portions of the satellite observational swaths of T and q, this method enables the estimation of scale-dependent behavior within instantaneous swaths for individual tropical and extratropical systems of interest. Scaling exponents are shown to fluctuate between β = -1 and -3 at scales ≥ 500 km, while at scales ≤ 500 km they are typically near β ≈ -2, with q slightly lower than T at the smallest scales observed. In the extratropics, the large-scale β is near -3. Within the tropics, however, the large-scale β for T is closer to -1 as small-scale moist convective processes dominate. In the tropics, q exhibits large-scale β between -2 and -3. The values of β are generally consistent with previous works of either time-averaged spatial variance estimates, or aircraft observations that require averaging over numerous flight observational segments. The instantaneous variance scaling methodology is relevant for cloud parameterization development and the assessment of time variability of scaling exponents.

  9. Microphysical growth state of ice particles and large-scale electrical structure of clouds

    NASA Technical Reports Server (NTRS)

    Williams, Earle; Zhang, Renyi; Boccippio, Dennis

    1994-01-01

    Cloud temperature, liquid water content, and vertical air velocity are all considered in evaluating the microphysical growth state of ice phase precipitation particles in the atmosphere. The large-scale observations taken together with in situ measurements indicated that the most prevalent growth condition for large ice particles in active convection is sublimation during riming, whereas the most prevalent growth condition in stratiform precipitation is vapor deposition. The large-scale electrical observations lend further support to the idea that particles warmed by riming into sublimation charge negatively and particles in vapor deposition charge positively in collisions with small ice particles.

  10. Efficient stochastic approaches for sensitivity studies of an Eulerian large-scale air pollution model

    NASA Astrophysics Data System (ADS)

    Dimov, I.; Georgieva, R.; Todorov, V.; Ostromsky, Tz.

    2017-10-01

    Reliability of large-scale mathematical models is an important issue when such models are used to support decision makers. Sensitivity analysis of model outputs to variation or natural uncertainties of model inputs is crucial for improving the reliability of mathematical models. A comprehensive experimental study of Monte Carlo algorithms based on Sobol sequences for multidimensional numerical integration has been done. A comparison with Latin hypercube sampling and a particular quasi-Monte Carlo lattice rule based on generalized Fibonacci numbers has been presented. The algorithms have been successfully applied to compute global Sobol sensitivity measures corresponding to the influence of several input parameters (six chemical reactions rates and four different groups of pollutants) on the concentrations of important air pollutants. The concentration values have been generated by the Unified Danish Eulerian Model. The sensitivity study has been done for the areas of several European cities with different geographical locations. The numerical tests show that the stochastic algorithms under consideration are efficient for multidimensional integration and especially for computing small by value sensitivity indices. It is a crucial element since even small indices may be important to be estimated in order to achieve a more accurate distribution of inputs influence and a more reliable interpretation of the mathematical model results.

  11. Robust Control of Multivariable and Large Scale Systems.

    DTIC Science & Technology

    1986-03-14

    AD-A175 $5B ROBUST CONTROL OF MULTIVRRIALE AND LARG SCALE SYSTEMS V2 R75 (U) HONEYWELL SYSTEMS AND RESEARCH CENTER MINNEAPOLIS MN J C DOYLE ET AL...ONIJQ 86 R alFS ja ,.AMIECFOEPF:ORMING ORGANIZATION So OFFICE SYMBOL 7a NAME OF MONITORING ORGANIZATI ON jonevwell Systems & Research If 4000c" Air...Force Office of Scientific Research .~ C :AE S C.rv. Stare arma ZIP Code) 7C ADDRESS (Crty. Stare. am ZIP Code, *3660 Marshall Street NE Building 410

  12. Energy transfers in large-scale and small-scale dynamos

    NASA Astrophysics Data System (ADS)

    Samtaney, Ravi; Kumar, Rohit; Verma, Mahendra

    2015-11-01

    We present the energy transfers, mainly energy fluxes and shell-to-shell energy transfers in small-scale dynamo (SSD) and large-scale dynamo (LSD) using numerical simulations of MHD turbulence for Pm = 20 (SSD) and for Pm = 0.2 on 10243 grid. For SSD, we demonstrate that the magnetic energy growth is caused by nonlocal energy transfers from the large-scale or forcing-scale velocity field to small-scale magnetic field. The peak of these energy transfers move towards lower wavenumbers as dynamo evolves, which is the reason for the growth of the magnetic fields at the large scales. The energy transfers U2U (velocity to velocity) and B2B (magnetic to magnetic) are forward and local. For LSD, we show that the magnetic energy growth takes place via energy transfers from large-scale velocity field to large-scale magnetic field. We observe forward U2U and B2B energy flux, similar to SSD.

  13. The micro-environmental impact of volatile organic compound emissions from large-scale assemblies of people in a confined space

    USDA-ARS?s Scientific Manuscript database

    Large-scale assemblies of people in a con'ned space can exert signi'cant impacts on the local air chemistry due to human emissions of volatile organics. Variations of air-quality in such small scale can be studied by quantifying 'ngerprint volatile organic compounds (VOCs) such as acetone, toluene, ...

  14. Large-scale recrystallization of the S-layer of Bacillus coagulans E38-66 at the air/water interface and on lipid films.

    PubMed Central

    Pum, D; Weinhandl, M; Hödl, C; Sleytr, U B

    1993-01-01

    S-layer protein isolated from Bacillus coagulans E38-66 could be recrystallized into large-scale coherent monolayers at an air/water interface and on phospholipid films spread on a Langmuir-Blodgett trough. Because of the asymmetry in the physiochemical surface properties of the S-layer protein, the subunits were associated with their more hydrophobic outer face with the air/water interface and oriented with their negatively charged inner face to the zwitterionic head groups of the dipalmitoylphosphatidylcholine and dipalmitoylphosphatidylethanolamine (DPPE) monolayer films. The dynamic crystal growth at both types of interfaces was first initiated at several distant nucleation points. The individual monocrystalline areas grew isotropically in all directions until the front edge of neighboring crystals was met. The recrystallized S-layer protein and the S-layer-DPPE layer could be chemically cross-linked from the subphase with glutaraldehyde. Images PMID:8478338

  15. Variability of cold season surface air temperature over northeastern China and its linkage with large-scale atmospheric circulations

    NASA Astrophysics Data System (ADS)

    Zhuang, Yuanhuang; Zhang, Jingyong; Wang, Lin

    2018-05-01

    Cold temperature anomalies and extremes have profound effects on the society, the economy, and the environment of northeastern China (NEC). In this study, we define the cold season as the months from October to April, and investigate the variability of cold season surface air temperature (CSAT) over NEC and its relationships with large-scale atmospheric circulation patterns for the period 1981-2014. The empirical orthogonal function (EOF) analysis shows that the first EOF mode of the CSAT over NEC is characterized by a homogeneous structure that describes 92.2% of the total variance. The regionally averaged CSAT over NEC is closely linked with the Arctic Oscillation ( r = 0.62, 99% confidence level) and also has a statistically significant relation with the Polar/Eurasian pattern in the cold season. The positive phases of the Arctic Oscillation and the Polar/Eurasian pattern tend to result in a positive geopotential height anomaly over NEC and a weakened East Asian winter monsoon, which subsequently increase the CSAT over NEC by enhancing the downward solar radiation, strengthening the subsidence warming and warm air advection. Conversely, the negative phases of these two climate indices result in opposite regional atmospheric circulation anomalies and decrease the CSAT over NEC.

  16. Hydrometeorological variability on a large french catchment and its relation to large-scale circulation across temporal scales

    NASA Astrophysics Data System (ADS)

    Massei, Nicolas; Dieppois, Bastien; Fritier, Nicolas; Laignel, Benoit; Debret, Maxime; Lavers, David; Hannah, David

    2015-04-01

    basically consisted in 1- decomposing both signals (SLP field and precipitation or streamflow) using discrete wavelet multiresolution analysis and synthesis, 2- generating one statistical downscaling model per time-scale, 3- summing up all scale-dependent models in order to obtain a final reconstruction of the predictand. The results obtained revealed a significant improvement of the reconstructions for both precipitation and streamflow when using the multiresolution ESD model instead of basic ESD ; in addition, the scale-dependent spatial patterns associated to the model matched quite well those obtained from scale-dependent composite analysis. In particular, the multiresolution ESD model handled very well the significant changes in variance through time observed in either prepciptation or streamflow. For instance, the post-1980 period, which had been characterized by particularly high amplitudes in interannual-to-interdecadal variability associated with flood and extremely low-flow/drought periods (e.g., winter 2001, summer 2003), could not be reconstructed without integrating wavelet multiresolution analysis into the model. Further investigations would be required to address the issue of the stationarity of the large-scale/local-scale relationships and to test the capability of the multiresolution ESD model for interannual-to-interdecadal forecasting. In terms of methodological approach, further investigations may concern a fully comprehensive sensitivity analysis of the modeling to the parameter of the multiresolution approach (different families of scaling and wavelet functions used, number of coefficients/degree of smoothness, etc.).

  17. An air-liquid contactor for large-scale capture of CO2 from air.

    PubMed

    Holmes, Geoffrey; Keith, David W

    2012-09-13

    We present a conceptually simple method for optimizing the design of a gas-liquid contactor for capture of carbon dioxide from ambient air, or 'air capture'. We apply the method to a slab geometry contactor that uses components, design and fabrication methods derived from cooling towers. We use mass transfer data appropriate for capture using a strong NaOH solution, combined with engineering and cost data derived from engineering studies performed by Carbon Engineering Ltd, and find that the total costs for air contacting alone-no regeneration-can be of the order of $60 per tonne CO(2). We analyse the reasons why our cost estimate diverges from that of other recent reports and conclude that the divergence arises from fundamental design choices rather than from differences in costing methodology. Finally, we review the technology risks and conclude that they can be readily addressed by prototype testing.

  18. Large scale Tesla coil guided discharges initiated by femtosecond laser filamentation in air

    NASA Astrophysics Data System (ADS)

    Arantchouk, L.; Point, G.; Brelet, Y.; Prade, B.; Carbonnel, J.; André, Y.-B.; Mysyrowicz, A.; Houard, A.

    2014-07-01

    The guiding of meter scale electric discharges produced in air by a Tesla coil is realized in laboratory using a focused terawatt laser pulse undergoing filamentation. The influence of the focus position, the laser arrival time, or the gap length is studied to determine the best conditions for efficient laser guiding. Discharge parameters such as delay, jitter, and resistance are characterized. An increase of the discharge length by a factor 5 has been achieved with the laser filaments, corresponding to a mean breakdown field of 2 kV/cm for a 1.8 m gap length. Consecutive guided discharges at a repetition rate of 10 Hz are also reported.

  19. A large-scale perspective on stress-induced alterations in resting-state networks

    NASA Astrophysics Data System (ADS)

    Maron-Katz, Adi; Vaisvaser, Sharon; Lin, Tamar; Hendler, Talma; Shamir, Ron

    2016-02-01

    Stress is known to induce large-scale neural modulations. However, its neural effect once the stressor is removed and how it relates to subjective experience are not fully understood. Here we used a statistically sound data-driven approach to investigate alterations in large-scale resting-state functional connectivity (rsFC) induced by acute social stress. We compared rsfMRI profiles of 57 healthy male subjects before and after stress induction. Using a parcellation-based univariate statistical analysis, we identified a large-scale rsFC change, involving 490 parcel-pairs. Aiming to characterize this change, we employed statistical enrichment analysis, identifying anatomic structures that were significantly interconnected by these pairs. This analysis revealed strengthening of thalamo-cortical connectivity and weakening of cross-hemispheral parieto-temporal connectivity. These alterations were further found to be associated with change in subjective stress reports. Integrating report-based information on stress sustainment 20 minutes post induction, revealed a single significant rsFC change between the right amygdala and the precuneus, which inversely correlated with the level of subjective recovery. Our study demonstrates the value of enrichment analysis for exploring large-scale network reorganization patterns, and provides new insight on stress-induced neural modulations and their relation to subjective experience.

  20. Climate variability rather than overstocking causes recent large scale cover changes of Tibetan pastures.

    PubMed

    Lehnert, L W; Wesche, K; Trachte, K; Reudenbach, C; Bendix, J

    2016-04-13

    The Tibetan Plateau (TP) is a globally important "water tower" that provides water for nearly 40% of the world's population. This supply function is claimed to be threatened by pasture degradation on the TP and the associated loss of water regulation functions. However, neither potential large scale degradation changes nor their drivers are known. Here, we analyse trends in a high-resolution dataset of grassland cover to determine the interactions among vegetation dynamics, climate change and human impacts on the TP. The results reveal that vegetation changes have regionally different triggers: While the vegetation cover has increased since the year 2000 in the north-eastern part of the TP due to an increase in precipitation, it has declined in the central and western parts of the TP due to rising air temperature and declining precipitation. Increasing livestock numbers as a result of land use changes exacerbated the negative trends but were not their exclusive driver. Thus, we conclude that climate variability instead of overgrazing has been the primary cause for large scale vegetation cover changes on the TP since the new millennium. Since areas of positive and negative changes are almost equal in extent, pasture degradation is not generally proceeding.

  1. Climate variability rather than overstocking causes recent large scale cover changes of Tibetan pastures

    PubMed Central

    Lehnert, L. W.; Wesche, K.; Trachte, K.; Reudenbach, C.; Bendix, J.

    2016-01-01

    The Tibetan Plateau (TP) is a globally important “water tower” that provides water for nearly 40% of the world’s population. This supply function is claimed to be threatened by pasture degradation on the TP and the associated loss of water regulation functions. However, neither potential large scale degradation changes nor their drivers are known. Here, we analyse trends in a high-resolution dataset of grassland cover to determine the interactions among vegetation dynamics, climate change and human impacts on the TP. The results reveal that vegetation changes have regionally different triggers: While the vegetation cover has increased since the year 2000 in the north-eastern part of the TP due to an increase in precipitation, it has declined in the central and western parts of the TP due to rising air temperature and declining precipitation. Increasing livestock numbers as a result of land use changes exacerbated the negative trends but were not their exclusive driver. Thus, we conclude that climate variability instead of overgrazing has been the primary cause for large scale vegetation cover changes on the TP since the new millennium. Since areas of positive and negative changes are almost equal in extent, pasture degradation is not generally proceeding. PMID:27073126

  2. Climate variability rather than overstocking causes recent large scale cover changes of Tibetan pastures

    NASA Astrophysics Data System (ADS)

    Lehnert, L. W.; Wesche, K.; Trachte, K.; Reudenbach, C.; Bendix, J.

    2016-04-01

    The Tibetan Plateau (TP) is a globally important “water tower” that provides water for nearly 40% of the world’s population. This supply function is claimed to be threatened by pasture degradation on the TP and the associated loss of water regulation functions. However, neither potential large scale degradation changes nor their drivers are known. Here, we analyse trends in a high-resolution dataset of grassland cover to determine the interactions among vegetation dynamics, climate change and human impacts on the TP. The results reveal that vegetation changes have regionally different triggers: While the vegetation cover has increased since the year 2000 in the north-eastern part of the TP due to an increase in precipitation, it has declined in the central and western parts of the TP due to rising air temperature and declining precipitation. Increasing livestock numbers as a result of land use changes exacerbated the negative trends but were not their exclusive driver. Thus, we conclude that climate variability instead of overgrazing has been the primary cause for large scale vegetation cover changes on the TP since the new millennium. Since areas of positive and negative changes are almost equal in extent, pasture degradation is not generally proceeding.

  3. Characterization of laser-induced plasmas as a complement to high-explosive large-scale detonations

    DOE PAGES

    Kimblin, Clare; Trainham, Rusty; Capelle, Gene A.; ...

    2017-09-12

    Experimental investigations into the characteristics of laser-induced plasmas indicate that LIBS provides a relatively inexpensive and easily replicable laboratory technique to isolate and measure reactions germane to understanding aspects of high-explosive detonations under controlled conditions. Furthermore, we examine spectral signatures and derived physical parameters following laser ablation of aluminum, graphite and laser-sparked air as they relate to those observed following detonation of high explosives and as they relate to shocked air. Laser-induced breakdown spectroscopy (LIBS) reliably correlates reactions involving atomic Al and aluminum monoxide (AlO) with respect to both emission spectra and temperatures, as compared to small- and large-scale high-explosivemore » detonations. Atomic Al and AlO resulting from laser ablation and a cited small-scale study, decay within ~10 -5 s, roughly 100 times faster than the Al and AlO decay rates (~10 -3 s) observed following the large-scale detonation of an Al-encased explosive. Temperatures and species produced in laser-sparked air are compared to those produced with laser ablated graphite in air. With graphite present, CN is dominant relative to N 2 + . Thus, in studies where the height of the ablating laser's focus was altered relative to the surface of the graphite substrate, CN concentration was found to decrease with laser focus below the graphite surface, indicating that laser intensity is a critical factor in the production of CN, via reactive nitrogen.« less

  4. Characterization of laser-induced plasmas as a complement to high-explosive large-scale detonations

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

    Kimblin, Clare; Trainham, Rusty; Capelle, Gene A.

    Experimental investigations into the characteristics of laser-induced plasmas indicate that LIBS provides a relatively inexpensive and easily replicable laboratory technique to isolate and measure reactions germane to understanding aspects of high-explosive detonations under controlled conditions. Furthermore, we examine spectral signatures and derived physical parameters following laser ablation of aluminum, graphite and laser-sparked air as they relate to those observed following detonation of high explosives and as they relate to shocked air. Laser-induced breakdown spectroscopy (LIBS) reliably correlates reactions involving atomic Al and aluminum monoxide (AlO) with respect to both emission spectra and temperatures, as compared to small- and large-scale high-explosivemore » detonations. Atomic Al and AlO resulting from laser ablation and a cited small-scale study, decay within ~10 -5 s, roughly 100 times faster than the Al and AlO decay rates (~10 -3 s) observed following the large-scale detonation of an Al-encased explosive. Temperatures and species produced in laser-sparked air are compared to those produced with laser ablated graphite in air. With graphite present, CN is dominant relative to N 2 + . Thus, in studies where the height of the ablating laser's focus was altered relative to the surface of the graphite substrate, CN concentration was found to decrease with laser focus below the graphite surface, indicating that laser intensity is a critical factor in the production of CN, via reactive nitrogen.« less

  5. Small-scale open ocean currents have large effects on wind wave heights

    NASA Astrophysics Data System (ADS)

    Ardhuin, Fabrice; Gille, Sarah T.; Menemenlis, Dimitris; Rocha, Cesar B.; Rascle, Nicolas; Chapron, Bertrand; Gula, Jonathan; Molemaker, Jeroen

    2017-06-01

    Tidal currents and large-scale oceanic currents are known to modify ocean wave properties, causing extreme sea states that are a hazard to navigation. Recent advances in the understanding and modeling capability of open ocean currents have revealed the ubiquitous presence of eddies, fronts, and filaments at scales 10-100 km. Based on realistic numerical models, we show that these structures can be the main source of variability in significant wave heights at scales less than 200 km, including important variations down to 10 km. Model results are consistent with wave height variations along satellite altimeter tracks, resolved at scales larger than 50 km. The spectrum of significant wave heights is found to be of the order of 70>>2/>(g2>>2>) times the current spectrum, where >> is the spatially averaged significant wave height, >> is the energy-averaged period, and g is the gravity acceleration. This variability induced by currents has been largely overlooked in spite of its relevance for extreme wave heights and remote sensing.Plain Language SummaryWe show that the variations in currents at <span class="hlt">scales</span> 10 to 100 km are the main source of variations in wave heights at the same <span class="hlt">scales</span>. Our work uses a combination of realistic numerical models for currents and waves and data from the Jason-3 and SARAL/AltiKa satellites. This finding will be of interest for the investigation of extreme wave heights, remote sensing, and <span class="hlt">air</span>-sea interactions. As an immediate application, the present results will help constrain the error budget of the up-coming satellite missions, in particular the Surface Water and Ocean Topography (SWOT) mission, and decide how the data will have to be processed to arrive at accurate sea level and wave measurements. It will also help in the analysis of wave measurements by the CFOSAT satellite.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016IAUS..319..109U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016IAUS..319..109U"><span>Dusty Starbursts within a z=3 <span class="hlt">Large</span> <span class="hlt">Scale</span> Structure <span class="hlt">revealed</span> by ALMA</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Umehata, Hideki</p> <p></p> <p>The role of the <span class="hlt">large-scale</span> structure is one of the most important theme in studying galaxy formation and evolution. However, it has been still mystery especially at z>2. On the basis of our ALMA 1.1 mm observations in a z ~ 3 protocluster field, it is suggested that submillimeter galaxies (SMGs) preferentially reside in the densest environment at z ~ 3. Furthermore we find a rich cluster of AGN-host SMGs at the core of the protocluster, combining with Chandra X-ray data. Our results indicate the vigorous star-formation and accelerated super massive black hole (SMBH) growth in the node of the cosmic web.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25679511','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25679511"><span><span class="hlt">Large</span> <span class="hlt">scale</span> aggregate microarray analysis <span class="hlt">reveals</span> three distinct molecular subclasses of human preeclampsia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Leavey, Katherine; Bainbridge, Shannon A; Cox, Brian J</p> <p>2015-01-01</p> <p>Preeclampsia (PE) is a life-threatening hypertensive pathology of pregnancy affecting 3-5% of all pregnancies. To date, PE has no cure, early detection markers, or effective treatments short of the removal of what is thought to be the causative organ, the placenta, which may necessitate a preterm delivery. Additionally, numerous small placental microarray studies attempting to identify "PE-specific" genes have yielded inconsistent results. We therefore hypothesize that preeclampsia is a multifactorial disease encompassing several pathology subclasses, and that <span class="hlt">large</span> cohort placental gene expression analysis will <span class="hlt">reveal</span> these groups. To address our hypothesis, we utilized known bioinformatic methods to aggregate 7 microarray data sets across multiple platforms in order to generate a <span class="hlt">large</span> data set of 173 patient samples, including 77 with preeclampsia. Unsupervised clustering of these patient samples <span class="hlt">revealed</span> three distinct molecular subclasses of PE. This included a "canonical" PE subclass demonstrating elevated expression of known PE markers and genes associated with poor oxygenation and increased secretion, as well as two other subclasses potentially representing a poor maternal response to pregnancy and an immunological presentation of preeclampsia. Our analysis sheds new light on the heterogeneity of PE patients, and offers up additional avenues for future investigation. Hopefully, our subclassification of preeclampsia based on molecular diversity will finally lead to the development of robust diagnostics and patient-based treatments for this disorder.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930035198&hterms=pnl&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpnl','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930035198&hterms=pnl&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpnl"><span>On the <span class="hlt">scaling</span> of small-<span class="hlt">scale</span> jet noise to <span class="hlt">large</span> <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Soderman, Paul T.; Allen, Christopher S.</p> <p>1992-01-01</p> <p>An examination was made of several published jet noise studies for the purpose of evaluating <span class="hlt">scale</span> effects important to the simulation of jet aeroacoustics. Several studies confirmed that small conical jets, one as small as 59 mm diameter, could be used to correctly simulate the overall or PNL noise of <span class="hlt">large</span> jets dominated by mixing noise. However, the detailed acoustic spectra of <span class="hlt">large</span> jets are more difficult to simulate because of the lack of broad-band turbulence spectra in small jets. One study indicated that a jet Reynolds number of 5 x 10 exp 6 based on exhaust diameter enabled the generation of broad-band noise representative of <span class="hlt">large</span> jet mixing noise. Jet suppressor aeroacoustics is even more difficult to simulate at small <span class="hlt">scale</span> because of the small mixer nozzles with flows sensitive to Reynolds number. Likewise, one study showed incorrect ejector mixing and entrainment using small-<span class="hlt">scale</span>, short ejector that led to poor acoustic <span class="hlt">scaling</span>. Conversely, fairly good results were found with a longer ejector and, in a different study, with a 32-chute suppressor nozzle. Finally, it was found that small-<span class="hlt">scale</span> aeroacoustic resonance produced by jets impacting ground boards does not reproduce at <span class="hlt">large</span> <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ACP....18.3839H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ACP....18.3839H"><span>Impacts of different characterizations of <span class="hlt">large-scale</span> background on simulated regional-<span class="hlt">scale</span> ozone over the continental United States</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hogrefe, Christian; Liu, Peng; Pouliot, George; Mathur, Rohit; Roselle, Shawn; Flemming, Johannes; Lin, Meiyun; Park, Rokjin J.</p> <p>2018-03-01</p> <p> from the global models along the CMAQ boundaries. Using boundary conditions from AM3 yielded higher springtime ozone columns burdens in the middle and lower troposphere compared to boundary conditions from the other models. For surface ozone, the differences between the AM3-driven CMAQ simulations and the CMAQ simulations driven by other <span class="hlt">large-scale</span> models are especially pronounced during spring and winter where they can reach more than 10 ppb for seasonal mean ozone mixing ratios and as much as 15 ppb for domain-averaged daily maximum 8 h average ozone on individual days. In contrast, the differences between the C-IFS-, GEOS-Chem-, and H-CMAQ-driven regional-<span class="hlt">scale</span> CMAQ simulations are typically smaller. Comparing simulated surface ozone mixing ratios to observations and computing seasonal and regional model performance statistics <span class="hlt">revealed</span> that boundary conditions can have a substantial impact on model performance. Further analysis showed that boundary conditions can affect model performance across the entire range of the observed distribution, although the impacts tend to be lower during summer and for the very highest observed percentiles. The results are discussed in the context of future model development and analysis opportunities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013ClDy...40.1903B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013ClDy...40.1903B"><span>Simulating the impact of the <span class="hlt">large-scale</span> circulation on the 2-m temperature and precipitation climatology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bowden, Jared H.; Nolte, Christopher G.; Otte, Tanya L.</p> <p>2013-04-01</p> <p>The impact of the simulated <span class="hlt">large-scale</span> atmospheric circulation on the regional climate is examined using the Weather Research and Forecasting (WRF) model as a regional climate model. The purpose is to understand the potential need for interior grid nudging for dynamical downscaling of global climate model (GCM) output for <span class="hlt">air</span> quality applications under a changing climate. In this study we downscale the NCEP-Department of Energy Atmospheric Model Intercomparison Project (AMIP-II) Reanalysis using three continuous 20-year WRF simulations: one simulation without interior grid nudging and two using different interior grid nudging methods. The biases in 2-m temperature and precipitation for the simulation without interior grid nudging are unreasonably <span class="hlt">large</span> with respect to the North American Regional Reanalysis (NARR) over the eastern half of the contiguous United States (CONUS) during the summer when <span class="hlt">air</span> quality concerns are most relevant. This study examines how these differences arise from errors in predicting the <span class="hlt">large-scale</span> atmospheric circulation. It is demonstrated that the Bermuda high, which strongly influences the regional climate for much of the eastern half of the CONUS during the summer, is poorly simulated without interior grid nudging. In particular, two summers when the Bermuda high was west (1993) and east (2003) of its climatological position are chosen to illustrate problems in the <span class="hlt">large-scale</span> atmospheric circulation anomalies. For both summers, WRF without interior grid nudging fails to simulate the placement of the upper-level anticyclonic (1993) and cyclonic (2003) circulation anomalies. The displacement of the <span class="hlt">large-scale</span> circulation impacts the lower atmosphere moisture transport and precipitable water, affecting the convective environment and precipitation. Using interior grid nudging improves the <span class="hlt">large-scale</span> circulation aloft and moisture transport/precipitable water anomalies, thereby improving the simulated 2-m temperature and precipitation</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20373136','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20373136"><span>Unique risk and protective factors for partner aggression in a <span class="hlt">large</span> <span class="hlt">scale</span> <span class="hlt">air</span> force survey.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Slep, Amy M Smith; Foran, Heather M; Heyman, Richard E; Snarr, Jeffery D</p> <p>2010-08-01</p> <p>The objective of this study is to examine risk factors of physical aggression against a partner in a <span class="hlt">large</span> representative Active Duty <span class="hlt">Air</span> Force sample. A stratified sample of 128,950 United States Active Duty members were invited to participate in an <span class="hlt">Air</span> Force-wide anonymous online survey across 82 bases. The final sample (N = 52,780) was weighted to be representative of the United States <span class="hlt">Air</span> Force. Backward stepwise regression analyses were conducted to identify unique predictors of partner physical aggression perpetration within and across different ecological levels (individual, family, organization, and community levels). Relationship satisfaction, alcohol problems, financial stress, and number of years in the military were identified as unique predictors of men's and women's perpetration of violence against their partner across ecological levels. Parental status, support from neighbors, personal coping, and support from formal agencies also uniquely predicted men's but not women's perpetration of violence across ecological levels. This study identified specific risk factors of partner violence that may be targeted by prevention and intervention efforts aimed at different levels of impact (e.g., family interventions, community-wide programs).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=73535&keyword=greenhouse&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=73535&keyword=greenhouse&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>National-<span class="hlt">scale</span> Assessment of <span class="hlt">Air</span> Toxics Risks</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>The national-<span class="hlt">scale</span> assessment of <span class="hlt">air</span> toxics risks is a modeling assessment which combines emission inventory development, atmospheric fate and transport modeling, exposure modeling, and risk assessment to characterize the risk associated with inhaling <span class="hlt">air</span> toxics from outdoor sour...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21518392-cold-atmospheric-pressure-air-surface-barrier-discharge-plasma-large-area-sterilization-applications','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21518392-cold-atmospheric-pressure-air-surface-barrier-discharge-plasma-large-area-sterilization-applications"><span>The cold and atmospheric-pressure <span class="hlt">air</span> surface barrier discharge plasma for <span class="hlt">large</span>-area sterilization applications</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 Dacheng; Department of Aeronautics, Fujian Key Laboratory for Plasma and Magnetic Resonance, School of Physics and Mechanical and Electrical Engineering, Xiamen University, Xiamen, Fujian 361005; Zhao Di</p> <p>2011-04-18</p> <p>This letter reports a stable <span class="hlt">air</span> surface barrier discharge device for <span class="hlt">large</span>-area sterilization applications at room temperature. This design may result in visually uniform plasmas with the electrode area <span class="hlt">scaled</span> up (or down) to the required size. A comparison for the survival rates of Escherichia coli from <span class="hlt">air</span>, N{sub 2} and O{sub 2} surface barrier discharge plasmas is presented, and the <span class="hlt">air</span> surface plasma consisting of strong filamentary discharges can efficiently kill Escherichia coli. Optical emission measurements indicate that reactive species such as O and OH generated in the room temperature <span class="hlt">air</span> plasmas play a significant role in the sterilizationmore » process.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27009229','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27009229"><span>Millennial-<span class="hlt">scale</span> faunal record <span class="hlt">reveals</span> differential resilience of European <span class="hlt">large</span> mammals to human impacts across the Holocene.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Crees, Jennifer J; Carbone, Chris; Sommer, Robert S; Benecke, Norbert; Turvey, Samuel T</p> <p>2016-03-30</p> <p>The use of short-term indicators for understanding patterns and processes of biodiversity loss can mask longer-term faunal responses to human pressures. We use an extensive database of approximately 18,700 mammalian zooarchaeological records for the last 11,700 years across Europe to reconstruct spatio-temporal dynamics of Holocene range change for 15 <span class="hlt">large</span>-bodied mammal species. European mammals experienced protracted, non-congruent range losses, with significant declines starting in some species approximately 3000 years ago and continuing to the present, and with the timing, duration and magnitude of declines varying individually between species. Some European mammals became globally extinct during the Holocene, whereas others experienced limited or no significant range change. These findings demonstrate the relatively early onset of prehistoric human impacts on postglacial biodiversity, and mirror species-specific patterns of mammalian extinction during the Late Pleistocene. Herbivores experienced significantly greater declines than carnivores, <span class="hlt">revealing</span> an important historical extinction filter that informs our understanding of relative resilience and vulnerability to human pressures for different taxa. We highlight the importance of <span class="hlt">large-scale</span>, long-term datasets for understanding complex protracted extinction processes, although the dynamic pattern of progressive faunal depletion of European mammal assemblages across the Holocene challenges easy identification of 'static' past baselines to inform current-day environmental management and restoration. © 2016 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950028567&hterms=pnl&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpnl','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950028567&hterms=pnl&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpnl"><span>On the <span class="hlt">scaling</span> of small-<span class="hlt">scale</span> jet noise to <span class="hlt">large</span> <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Soderman, Paul T.; Allen, Christopher S.</p> <p>1992-01-01</p> <p>An examination was made of several published jet noise studies for the purpose of evaluating <span class="hlt">scale</span> effects important to the simulation of jet aeroacoustics. Several studies confirmed that small conical jets, one as small as 59 mm diameter, could be used to correctly simulate the overall or perceived noise level (PNL) noise of <span class="hlt">large</span> jets dominated by mixing noise. However, the detailed acoustic spectra of <span class="hlt">large</span> jets are more difficult to simulate because of the lack of broad-band turbulence spectra in small jets. One study indicated that a jet Reynolds number of 5 x 10(exp 6) based on exhaust diameter enabled the generation of broad-band noise representative of <span class="hlt">large</span> jet mixing noise. Jet suppressor aeroacoustics is even more difficult to simulate at small <span class="hlt">scale</span> because of the small mixer nozzles with flows sensitive to Reynolds number. Likewise, one study showed incorrect ejector mixing and entrainment using a small-<span class="hlt">scale</span>, short ejector that led to poor acoustic <span class="hlt">scaling</span>. Conversely, fairly good results were found with a longer ejector and, in a different study, with a 32-chute suppressor nozzle. Finally, it was found that small-<span class="hlt">scale</span> aeroacoustic resonance produced by jets impacting ground boards does not reproduce at <span class="hlt">large</span> <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840066337&hterms=reserach+methodologies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dreserach%2Bmethodologies','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840066337&hterms=reserach+methodologies&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dreserach%2Bmethodologies"><span><span class="hlt">Large-scale</span> structural optimization</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Sobieszczanski-Sobieski, J.</p> <p>1983-01-01</p> <p>Problems encountered by aerospace designers in attempting to optimize whole aircraft are discussed, along with possible solutions. <span class="hlt">Large</span> <span class="hlt">scale</span> optimization, as opposed to component-by-component optimization, is hindered by computational costs, software inflexibility, concentration on a single, rather than trade-off, design methodology and the incompatibility of <span class="hlt">large-scale</span> optimization with single program, single computer methods. The software problem can be approached by placing the full analysis outside of the optimization loop. Full analysis is then performed only periodically. Problem-dependent software can be removed from the generic code using a systems programming technique, and then embody the definitions of design variables, objective function and design constraints. Trade-off algorithms can be used at the design points to obtain quantitative answers. Finally, decomposing the <span class="hlt">large-scale</span> problem into independent subproblems allows systematic optimization of the problems by an organization of people and machines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFMIN23B1501W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFMIN23B1501W"><span><span class="hlt">Large-Scale</span>, Parallel, Multi-Sensor Data Fusion in the Cloud</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, B. D.; Manipon, G.; Hua, H.</p> <p>2012-12-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the "A-Train" platforms (<span class="hlt">AIRS</span>, AMSR-E, MODIS, MISR, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over periods of years to decades. However, moving from predominantly single-instrument studies to a multi-sensor, measurement-based model for long-duration analysis of important climate variables presents serious challenges for <span class="hlt">large-scale</span> data mining and data fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another instrument (MODIS), and to a model (ECMWF), stratify the comparisons using a classification of the "cloud scenes" from CloudSat, and repeat the entire analysis over years of <span class="hlt">AIRS</span> data. To perform such an analysis, one must discover & access multiple datasets from remote sites, find the space/time "matchups" between instruments swaths and model grids, understand the quality flags and uncertainties for retrieved physical variables, assemble merged datasets, and compute fused products for further scientific and statistical analysis. To efficiently assemble such decade-<span class="hlt">scale</span> datasets in a timely manner, we are utilizing Elastic Computing in the Cloud and parallel map/reduce-based algorithms. "SciReduce" is a Hadoop-like parallel analysis system, programmed in parallel python, that is designed from the ground up for Earth science. SciReduce executes inside VMWare images and <span class="hlt">scales</span> to any number of nodes in the Cloud. Unlike Hadoop, in which simple tuples (keys & values) are passed between the map and reduce functions, SciReduce operates on bundles of named numeric arrays, which can be passed in memory or serialized to disk in netCDF4 or HDF5. Thus, SciReduce uses the native datatypes (geolocated grids, swaths, and points) that geo-scientists are familiar with. We are deploying within Sci</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413008W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413008W"><span><span class="hlt">Large-Scale</span>, Parallel, Multi-Sensor Data Fusion in the Cloud</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, B.; Manipon, G.; Hua, H.</p> <p>2012-04-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the "A-Train" platforms (<span class="hlt">AIRS</span>, AMSR-E, MODIS, MISR, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over periods of years to decades. However, moving from predominantly single-instrument studies to a multi-sensor, measurement-based model for long-duration analysis of important climate variables presents serious challenges for <span class="hlt">large-scale</span> data mining and data fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another instrument (MODIS), and to a model (ECMWF), stratify the comparisons using a classification of the "cloud scenes" from CloudSat, and repeat the entire analysis over years of <span class="hlt">AIRS</span> data. To perform such an analysis, one must discover & access multiple datasets from remote sites, find the space/time "matchups" between instruments swaths and model grids, understand the quality flags and uncertainties for retrieved physical variables, assemble merged datasets, and compute fused products for further scientific and statistical analysis. To efficiently assemble such decade-<span class="hlt">scale</span> datasets in a timely manner, we are utilizing Elastic Computing in the Cloud and parallel map/reduce-based algorithms. "SciReduce" is a Hadoop-like parallel analysis system, programmed in parallel python, that is designed from the ground up for Earth science. SciReduce executes inside VMWare images and <span class="hlt">scales</span> to any number of nodes in the Cloud. Unlike Hadoop, in which simple tuples (keys & values) are passed between the map and reduce functions, SciReduce operates on bundles of named numeric arrays, which can be passed in memory or serialized to disk in netCDF4 or HDF5. Thus, SciReduce uses the native datatypes (geolocated grids, swaths, and points) that geo-scientists are familiar with. We are deploying within Sci</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15114356','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15114356"><span><span class="hlt">Large-scale</span> recording of neuronal ensembles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Buzsáki, György</p> <p>2004-05-01</p> <p>How does the brain orchestrate perceptions, thoughts and actions from the spiking activity of its neurons? Early single-neuron recording research treated spike pattern variability as noise that needed to be averaged out to <span class="hlt">reveal</span> the brain's representation of invariant input. Another view is that variability of spikes is centrally coordinated and that this brain-generated ensemble pattern in cortical structures is itself a potential source of cognition. <span class="hlt">Large-scale</span> recordings from neuronal ensembles now offer the opportunity to test these competing theoretical frameworks. Currently, wire and micro-machined silicon electrode arrays can record from <span class="hlt">large</span> numbers of neurons and monitor local neural circuits at work. Achieving the full potential of massively parallel neuronal recordings, however, will require further development of the neuron-electrode interface, automated and efficient spike-sorting algorithms for effective isolation and identification of single neurons, and new mathematical insights for the analysis of network properties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/15242150','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/15242150"><span>Simulating urban-<span class="hlt">scale</span> <span class="hlt">air</span> pollutants and their predicting capabilities over the Seoul metropolitan area.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Park, Il-Soo; Lee, Suk-Jo; Kim, Cheol-Hee; Yoo, Chul; Lee, Yong-Hee</p> <p>2004-06-01</p> <p>Urban-<span class="hlt">scale</span> <span class="hlt">air</span> pollutants for sulfur dioxide, nitrogen dioxide, particulate matter with aerodynamic diameter > or = 10 microm, and ozone (O3) were simulated over the Seoul metropolitan area, Korea, during the period of July 2-11, 2002, and their predicting capabilities were discussed. The <span class="hlt">Air</span> Pollution Model (TAPM) and the highly disaggregated anthropogenic and the biogenic gridded emissions (1 km x 1 km) recently prepared by the Korean Ministry of Environment were applied. Wind fields with observational nudging in the prognostic meteorological model TAPM are optionally adopted to comparatively examine the meteorological impact on the prediction capabilities of urban-<span class="hlt">scale</span> <span class="hlt">air</span> pollutants. The result shows that the simulated concentrations of secondary <span class="hlt">air</span> pollutant <span class="hlt">largely</span> agree with observed levels with an index of agreement (IOA) of >0.6, whereas IOAs of approximately 0.4 are found for most primary pollutants in the major cities, reflecting the quality of emission data in the urban area. The observationally nudged wind fields with higher IOAs have little effect on the prediction for both primary and secondary <span class="hlt">air</span> pollutants, implying that the detailed wind field does not consistently improve the urban <span class="hlt">air</span> pollution model performance if emissions are not well specified. However, the robust highest concentrations are better described toward observations by imposing observational nudging, suggesting the importance of wind fields for the predictions of extreme concentrations such as robust highest concentrations, maximum levels, and >90th percentiles of concentrations for both primary and secondary urban-<span class="hlt">scale</span> <span class="hlt">air</span> pollutants.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_3");'>3</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li class="active"><span>5</span></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_5 --> <div id="page_6" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_4");'>4</a></li> <li><a href="#" onclick='return showDiv("page_5");'>5</a></li> <li class="active"><span>6</span></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="101"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1348324-large-scale-metal-additive-techniques-review','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1348324-large-scale-metal-additive-techniques-review"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Metal Additive Techniques Review</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>Nycz, Andrzej; Adediran, Adeola I; Noakes, Mark W</p> <p>2016-01-01</p> <p>In recent years additive manufacturing made long strides toward becoming a main stream production technology. Particularly strong progress has been made in <span class="hlt">large-scale</span> polymer deposition. However, <span class="hlt">large</span> <span class="hlt">scale</span> metal additive has not yet reached parity with <span class="hlt">large</span> <span class="hlt">scale</span> polymer. This paper is a review study of the metal additive techniques in the context of building <span class="hlt">large</span> structures. Current commercial devices are capable of printing metal parts on the order of several cubic feet compared to hundreds of cubic feet for the polymer side. In order to follow the polymer progress path several factors are considered: potential to <span class="hlt">scale</span>, economy, environmentmore » friendliness, material properties, feedstock availability, robustness of the process, quality and accuracy, potential for defects, and post processing as well as potential applications. This paper focuses on current state of art of <span class="hlt">large</span> <span class="hlt">scale</span> metal additive technology with a focus on expanding the geometric limits.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27859842','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27859842"><span>Movement <span class="hlt">reveals</span> <span class="hlt">scale</span> dependence in habitat selection of a <span class="hlt">large</span> ungulate.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Northrup, Joseph M; Anderson, Charles R; Hooten, Mevin B; Wittemyer, George</p> <p>2016-12-01</p> <p>Ecological processes operate across temporal and spatial <span class="hlt">scales</span>. Anthropogenic disturbances impact these processes, but examinations of <span class="hlt">scale</span> dependence in impacts are infrequent. Such examinations can provide important insight to wildlife-human interactions and guide management efforts to reduce impacts. We assessed spatiotemporal <span class="hlt">scale</span> dependence in habitat selection of mule deer (Odocoileus hemionus) in the Piceance Basin of Colorado, USA, an area of ongoing natural gas development. We employed a newly developed animal movement method to assess habitat selection across <span class="hlt">scales</span> defined using animal-centric spatiotemporal definitions ranging from the local (defined from five hour movements) to the broad (defined from weekly movements). We extended our analysis to examine variation in <span class="hlt">scale</span> dependence between night and day and assess functional responses in habitat selection patterns relative to the density of anthropogenic features. Mule deer displayed <span class="hlt">scale</span> invariance in the direction of their response to energy development features, avoiding well pads and the areas closest to roads at all <span class="hlt">scales</span>, though with increasing strength of avoidance at coarser <span class="hlt">scales</span>. Deer displayed <span class="hlt">scale</span>-dependent responses to most other habitat features, including land cover type and habitat edges. Selection differed between night and day at the finest <span class="hlt">scales</span>, but homogenized as <span class="hlt">scale</span> increased. Deer displayed functional responses to development, with deer inhabiting the least developed ranges more strongly avoiding development relative to those with more development in their ranges. Energy development was a primary driver of habitat selection patterns in mule deer, structuring their behaviors across all <span class="hlt">scales</span> examined. Stronger avoidance at coarser <span class="hlt">scales</span> suggests that deer behaviorally mediated their interaction with development, but only to a degree. At higher development densities than seen in this area, such mediation may not be possible and thus maintenance of sufficient habitat</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70192619','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70192619"><span>Movement <span class="hlt">reveals</span> <span class="hlt">scale</span> dependence in habitat selection of a <span class="hlt">large</span> ungulate</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Northrup, Joseph; Anderson, Charles R.; Hooten, Mevin B.; Wittemyer, George</p> <p>2016-01-01</p> <p>Ecological processes operate across temporal and spatial <span class="hlt">scales</span>. Anthropogenic disturbances impact these processes, but examinations of <span class="hlt">scale</span> dependence in impacts are infrequent. Such examinations can provide important insight to wildlife–human interactions and guide management efforts to reduce impacts. We assessed spatiotemporal <span class="hlt">scale</span> dependence in habitat selection of mule deer (Odocoileus hemionus) in the Piceance Basin of Colorado, USA, an area of ongoing natural gas development. We employed a newly developed animal movement method to assess habitat selection across <span class="hlt">scales</span> defined using animal-centric spatiotemporal definitions ranging from the local (defined from five hour movements) to the broad (defined from weekly movements). We extended our analysis to examine variation in <span class="hlt">scale</span> dependence between night and day and assess functional responses in habitat selection patterns relative to the density of anthropogenic features. Mule deer displayed <span class="hlt">scale</span> invariance in the direction of their response to energy development features, avoiding well pads and the areas closest to roads at all <span class="hlt">scales</span>, though with increasing strength of avoidance at coarser <span class="hlt">scales</span>. Deer displayed <span class="hlt">scale</span>-dependent responses to most other habitat features, including land cover type and habitat edges. Selection differed between night and day at the finest <span class="hlt">scales</span>, but homogenized as <span class="hlt">scale</span> increased. Deer displayed functional responses to development, with deer inhabiting the least developed ranges more strongly avoiding development relative to those with more development in their ranges. Energy development was a primary driver of habitat selection patterns in mule deer, structuring their behaviors across all <span class="hlt">scales</span> examined. Stronger avoidance at coarser <span class="hlt">scales</span> suggests that deer behaviorally mediated their interaction with development, but only to a degree. At higher development densities than seen in this area, such mediation may not be possible and thus maintenance of sufficient</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A51H0157X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A51H0157X"><span>Extreme Temperature Regimes during the Cool Season and their Associated <span class="hlt">Large-Scale</span> Circulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xie, Z.</p> <p>2015-12-01</p> <p>In the cool season (November-March), extreme temperature events (ETEs) always hit the continental United States (US) and provide significant societal impacts. According to the anomalous amplitudes of the surface <span class="hlt">air</span> temperature (SAT), there are two typical types of ETEs, e.g. cold waves (CWs) and warm waves (WWs). This study used cluster analysis to categorize both CWs and WWs into four distinct regimes respectively and investigated their associated <span class="hlt">large-scale</span> circulations on intra-seasonal time <span class="hlt">scale</span>. Most of the CW regimes have <span class="hlt">large</span> areal impact over the continental US. However, the distribution of cold SAT anomalies varies apparently in four regimes. In the sea level, the four CW regimes are characterized by anomalous high pressure over North America (near and to west of cold anomaly) with different extension and orientation. As a result, anomalous northerlies along east flank of anomalous high pressure convey cold <span class="hlt">air</span> into the continental US. To the middle troposphere, the leading two groups feature <span class="hlt">large-scale</span> and zonally-elongated circulation anomaly pattern, while the other two regimes exhibit synoptic wavetrain pattern with meridionally elongated features. As for the WW regimes, there are some patterns symmetry and anti-symmetry with respect to CW regimes. The WW regimes are characterized by anomalous low pressure and southerlies wind over North America. The first and fourth groups are affected by remote forcing emanating from North Pacific, while the others appear mainly locally forced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1130708-first-large-scale-flood-inundation-forecasting-model','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1130708-first-large-scale-flood-inundation-forecasting-model"><span>A first <span class="hlt">large-scale</span> flood inundation forecasting model</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>Schumann, Guy J-P; Neal, Jeffrey C.; Voisin, Nathalie</p> <p>2013-11-04</p> <p>At present continental to global <span class="hlt">scale</span> flood forecasting focusses on predicting at a point discharge, with little attention to the detail and accuracy of local <span class="hlt">scale</span> inundation predictions. Yet, inundation is actually the variable of interest and all flood impacts are inherently local in nature. This paper proposes a first <span class="hlt">large</span> <span class="hlt">scale</span> flood inundation ensemble forecasting model that uses best available data and modeling approaches in data scarce areas and at continental <span class="hlt">scales</span>. The model was built for the Lower Zambezi River in southeast Africa to demonstrate current flood inundation forecasting capabilities in <span class="hlt">large</span> data-scarce regions. The inundation model domainmore » has a surface area of approximately 170k km2. ECMWF meteorological data were used to force the VIC (Variable Infiltration Capacity) macro-<span class="hlt">scale</span> hydrological model which simulated and routed daily flows to the input boundary locations of the 2-D hydrodynamic model. Efficient hydrodynamic modeling over <span class="hlt">large</span> areas still requires model grid resolutions that are typically larger than the width of many river channels that play a key a role in flood wave propagation. We therefore employed a novel sub-grid channel scheme to describe the river network in detail whilst at the same time representing the floodplain at an appropriate and efficient <span class="hlt">scale</span>. The modeling system was first calibrated using water levels on the main channel from the ICESat (Ice, Cloud, and land Elevation Satellite) laser altimeter and then applied to predict the February 2007 Mozambique floods. Model evaluation showed that simulated flood edge cells were within a distance of about 1 km (one model resolution) compared to an observed flood edge of the event. Our study highlights that physically plausible parameter values and satisfactory performance can be achieved at spatial <span class="hlt">scales</span> ranging from tens to several hundreds of thousands of km2 and at model grid resolutions up to several km2. However, initial model test runs in forecast</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28793326','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28793326"><span>Thermal oxidation of nuclear graphite: A <span class="hlt">large</span> <span class="hlt">scale</span> waste treatment option.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Theodosiou, Alex; Jones, Abbie N; Marsden, Barry J</p> <p>2017-01-01</p> <p>This study has investigated the laboratory <span class="hlt">scale</span> thermal oxidation of nuclear graphite, as a proof-of-concept for the treatment and decommissioning of reactor cores on a larger industrial <span class="hlt">scale</span>. If showed to be effective, this technology could have promising international significance with a considerable impact on the nuclear waste management problem currently facing many countries worldwide. The use of thermal treatment of such graphite waste is seen as advantageous since it will decouple the need for an operational Geological Disposal Facility (GDF). Particulate samples of Magnox Reactor Pile Grade-A (PGA) graphite, were oxidised in both <span class="hlt">air</span> and 60% O2, over the temperature range 400-1200°C. Oxidation rates were found to increase with temperature, with a particular rise between 700-800°C, suggesting a change in oxidation mechanism. A second increase in oxidation rate was observed between 1000-1200°C and was found to correspond to a <span class="hlt">large</span> increase in the CO/CO2 ratio, as confirmed through gas analysis. Increasing the oxidant flow rate gave a linear increase in oxidation rate, up to a certain point, and maximum rates of 23.3 and 69.6 mg / min for <span class="hlt">air</span> and 60% O2 respectively were achieved at a flow of 250 ml / min and temperature of 1000°C. These promising results show that <span class="hlt">large-scale</span> thermal treatment could be a potential option for the decommissioning of graphite cores, although the design of the plant would need careful consideration in order to achieve optimum efficiency and throughput.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5549958','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5549958"><span>Thermal oxidation of nuclear graphite: A <span class="hlt">large</span> <span class="hlt">scale</span> waste treatment option</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jones, Abbie N.; Marsden, Barry J.</p> <p>2017-01-01</p> <p>This study has investigated the laboratory <span class="hlt">scale</span> thermal oxidation of nuclear graphite, as a proof-of-concept for the treatment and decommissioning of reactor cores on a larger industrial <span class="hlt">scale</span>. If showed to be effective, this technology could have promising international significance with a considerable impact on the nuclear waste management problem currently facing many countries worldwide. The use of thermal treatment of such graphite waste is seen as advantageous since it will decouple the need for an operational Geological Disposal Facility (GDF). Particulate samples of Magnox Reactor Pile Grade-A (PGA) graphite, were oxidised in both <span class="hlt">air</span> and 60% O2, over the temperature range 400–1200°C. Oxidation rates were found to increase with temperature, with a particular rise between 700–800°C, suggesting a change in oxidation mechanism. A second increase in oxidation rate was observed between 1000–1200°C and was found to correspond to a <span class="hlt">large</span> increase in the CO/CO2 ratio, as confirmed through gas analysis. Increasing the oxidant flow rate gave a linear increase in oxidation rate, up to a certain point, and maximum rates of 23.3 and 69.6 mg / min for <span class="hlt">air</span> and 60% O2 respectively were achieved at a flow of 250 ml / min and temperature of 1000°C. These promising results show that <span class="hlt">large-scale</span> thermal treatment could be a potential option for the decommissioning of graphite cores, although the design of the plant would need careful consideration in order to achieve optimum efficiency and throughput. PMID:28793326</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JNEng..13e1001F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JNEng..13e1001F"><span><span class="hlt">Large-scale</span> neuromorphic computing systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Furber, Steve</p> <p>2016-10-01</p> <p>Neuromorphic computing covers a diverse range of approaches to information processing all of which demonstrate some degree of neurobiological inspiration that differentiates them from mainstream conventional computing systems. The philosophy behind neuromorphic computing has its origins in the seminal work carried out by Carver Mead at Caltech in the late 1980s. This early work influenced others to carry developments forward, and advances in VLSI technology supported steady growth in the <span class="hlt">scale</span> and capability of neuromorphic devices. Recently, a number of <span class="hlt">large-scale</span> neuromorphic projects have emerged, taking the approach to unprecedented <span class="hlt">scales</span> and capabilities. These <span class="hlt">large-scale</span> projects are associated with major new funding initiatives for brain-related research, creating a sense that the time and circumstances are right for progress in our understanding of information processing in the brain. In this review we present a brief history of neuromorphic engineering then focus on some of the principal current <span class="hlt">large-scale</span> projects, their main features, how their approaches are complementary and distinct, their advantages and drawbacks, and highlight the sorts of capabilities that each can deliver to neural modellers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28540497','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28540497"><span><span class="hlt">Large-scale</span> transcriptome analysis <span class="hlt">reveals</span> arabidopsis metabolic pathways are frequently influenced by different pathogens.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jiang, Zhenhong; He, Fei; Zhang, Ziding</p> <p>2017-07-01</p> <p>Through <span class="hlt">large-scale</span> transcriptional data analyses, we highlighted the importance of plant metabolism in plant immunity and identified 26 metabolic pathways that were frequently influenced by the infection of 14 different pathogens. Reprogramming of plant metabolism is a common phenomenon in plant defense responses. Currently, a <span class="hlt">large</span> number of transcriptional profiles of infected tissues in Arabidopsis (Arabidopsis thaliana) have been deposited in public databases, which provides a great opportunity to understand the expression patterns of metabolic pathways during plant defense responses at the systems level. Here, we performed a <span class="hlt">large-scale</span> transcriptome analysis based on 135 previously published expression samples, including 14 different pathogens, to explore the expression pattern of Arabidopsis metabolic pathways. Overall, metabolic genes are significantly changed in expression during plant defense responses. Upregulated metabolic genes are enriched on defense responses, and downregulated genes are enriched on photosynthesis, fatty acid and lipid metabolic processes. Gene set enrichment analysis (GSEA) identifies 26 frequently differentially expressed metabolic pathways (FreDE_Paths) that are differentially expressed in more than 60% of infected samples. These pathways are involved in the generation of energy, fatty acid and lipid metabolism as well as secondary metabolite biosynthesis. Clustering analysis based on the expression levels of these 26 metabolic pathways clearly distinguishes infected and control samples, further suggesting the importance of these metabolic pathways in plant defense responses. By comparing with FreDE_Paths from abiotic stresses, we find that the expression patterns of 26 FreDE_Paths from biotic stresses are more consistent across different infected samples. By investigating the expression correlation between transcriptional factors (TFs) and FreDE_Paths, we identify several notable relationships. Collectively, the current study</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29875410','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29875410"><span>Environment and host as <span class="hlt">large-scale</span> controls of ectomycorrhizal fungi.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>van der Linde, Sietse; Suz, Laura M; Orme, C David L; Cox, Filipa; Andreae, Henning; Asi, Endla; Atkinson, Bonnie; Benham, Sue; Carroll, Christopher; Cools, Nathalie; De Vos, Bruno; Dietrich, Hans-Peter; Eichhorn, Johannes; Gehrmann, Joachim; Grebenc, Tine; Gweon, Hyun S; Hansen, Karin; Jacob, Frank; Kristöfel, Ferdinand; Lech, Paweł; Manninger, Miklós; Martin, Jan; Meesenburg, Henning; Merilä, Päivi; Nicolas, Manuel; Pavlenda, Pavel; Rautio, Pasi; Schaub, Marcus; Schröck, Hans-Werner; Seidling, Walter; Šrámek, Vít; Thimonier, Anne; Thomsen, Iben Margrete; Titeux, Hugues; Vanguelova, Elena; Verstraeten, Arne; Vesterdal, Lars; Waldner, Peter; Wijk, Sture; Zhang, Yuxin; Žlindra, Daniel; Bidartondo, Martin I</p> <p>2018-06-06</p> <p>Explaining the <span class="hlt">large-scale</span> diversity of soil organisms that drive biogeochemical processes-and their responses to environmental change-is critical. However, identifying consistent drivers of belowground diversity and abundance for some soil organisms at <span class="hlt">large</span> spatial <span class="hlt">scales</span> remains problematic. Here we investigate a major guild, the ectomycorrhizal fungi, across European forests at a spatial <span class="hlt">scale</span> and resolution that is-to our knowledge-unprecedented, to explore key biotic and abiotic predictors of ectomycorrhizal diversity and to identify dominant responses and thresholds for change across complex environmental gradients. We show the effect of 38 host, environment, climate and geographical variables on ectomycorrhizal diversity, and define thresholds of community change for key variables. We quantify host specificity and <span class="hlt">reveal</span> plasticity in functional traits involved in soil foraging across gradients. We conclude that environmental and host factors explain most of the variation in ectomycorrhizal diversity, that the environmental thresholds used as major ecosystem assessment tools need adjustment and that the importance of belowground specificity and plasticity has previously been underappreciated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23211601C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23211601C"><span>The Relationship Between Galaxies and the <span class="hlt">Large-Scale</span> Structure of the Universe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Coil, Alison L.</p> <p>2018-06-01</p> <p>I will describe our current understanding of the relationship between galaxies and the <span class="hlt">large-scale</span> structure of the Universe, often called the galaxy-halo connection. Galaxies are thought to form and evolve in the centers of dark matter halos, which grow along with the galaxies they host. <span class="hlt">Large</span> galaxy redshift surveys have <span class="hlt">revealed</span> clear observational signatures of connections between galaxy properties and their clustering properties on <span class="hlt">large</span> <span class="hlt">scales</span>. For example, older, quiescent galaxies are known to cluster more strongly than younger, star-forming galaxies, which are more likely to be found in galactic voids and filaments rather than the centers of galaxy clusters. I will show how cosmological numerical simulations have aided our understanding of this galaxy-halo connection and what is known from a statistical point of view about how galaxies populate dark matter halos. This knowledge both helps us learn about galaxy evolution and is fundamental to our ability to use galaxy surveys to <span class="hlt">reveal</span> cosmological information. I will talk briefly about some of the current open questions in the field, including galactic conformity and assembly bias.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=air+AND+transportation&pg=3&id=EJ734375','ERIC'); return false;" href="https://eric.ed.gov/?q=air+AND+transportation&pg=3&id=EJ734375"><span>Development and Evaluation of the <span class="hlt">Air</span> Travel Stress <span class="hlt">Scale</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>Bricker, Jonathan B.</p> <p>2005-01-01</p> <p>Despite anecdotal evidence suggesting that <span class="hlt">air</span> travel is personally demanding, little research has examined <span class="hlt">air</span> travel stress. To address these issues, the author developed and evaluated the 1st known measure of <span class="hlt">air</span> travel stress-the <span class="hlt">Air</span> Travel Stress <span class="hlt">Scale</span>-in 3 studies. Exploratory and confirmatory factor analysis indicated 3 components: (a)…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1995761','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1995761"><span><span class="hlt">Large-Scale</span> Mitochondrial DNA Analysis of the Domestic Goat <span class="hlt">Reveals</span> Six Haplogroups with High Diversity</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Naderi, Saeid; Rezaei, Hamid-Reza; Taberlet, Pierre; Zundel, Stéphanie; Rafat, Seyed-Abbas; Naghash, Hamid-Reza; El-Barody, Mohamed A. A.; Ertugrul, Okan; Pompanon, François</p> <p>2007-01-01</p> <p>Background From the beginning of domestication, the transportation of domestic animals resulted in genetic and demographic processes that explain their present distribution and genetic structure. Thus studying the present genetic diversity helps to better understand the history of domestic species. Methodology/Principal Findings The genetic diversity of domestic goats has been characterized with 2430 individuals from all over the old world, including 946 new individuals from regions poorly studied until now (mainly the Fertile Crescent). These individuals represented 1540 haplotypes for the HVI segment of the mitochondrial DNA (mtDNA) control region. This <span class="hlt">large-scale</span> study allowed the establishment of a clear nomenclature of the goat maternal haplogroups. Only five of the six previously defined groups of haplotypes were divergent enough to be considered as different haplogroups. Moreover a new mitochondrial group has been localized around the Fertile Crescent. All groups showed very high haplotype diversity. Most of this diversity was distributed among groups and within geographic regions. The weak geographic structure may result from the worldwide distribution of the dominant A haplogroup (more than 90% of the individuals). The <span class="hlt">large-scale</span> distribution of other haplogroups (except one), may be related to human migration. The recent fragmentation of local goat populations into discrete breeds is not detectable with mitochondrial markers. The estimation of demographic parameters from mismatch analyses showed that all groups had a recent demographic expansion corresponding roughly to the period when domestication took place. But even with a <span class="hlt">large</span> data set it remains difficult to give relative dates of expansion for different haplogroups because of <span class="hlt">large</span> confidence intervals. Conclusions/Significance We propose standard criteria for the definition of the different haplogroups based on the result of mismatch analysis and on the use of sequences of reference. Such a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1995AAS...187.2403C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1995AAS...187.2403C"><span><span class="hlt">Large-Scale</span> Outflows in Seyfert Galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colbert, E. J. M.; Baum, S. A.</p> <p>1995-12-01</p> <p>\\catcode`\\@=11 \\ialign{m @th#1hfil ##hfil \\crcr#2\\crcr\\sim\\crcr}}} \\catcode`\\@=12 Highly collimated outflows extend out to Mpc <span class="hlt">scales</span> in many radio-loud active galaxies. In Seyfert galaxies, which are radio-quiet, the outflows extend out to kpc <span class="hlt">scales</span> and do not appear to be as highly collimated. In order to study the nature of <span class="hlt">large-scale</span> (>~1 kpc) outflows in Seyferts, we have conducted optical, radio and X-ray surveys of a distance-limited sample of 22 edge-on Seyfert galaxies. Results of the optical emission-line imaging and spectroscopic survey imply that <span class="hlt">large-scale</span> outflows are present in >~{{1} /{4}} of all Seyferts. The radio (VLA) and X-ray (ROSAT) surveys show that <span class="hlt">large-scale</span> radio and X-ray emission is present at about the same frequency. Kinetic luminosities of the outflows in Seyferts are comparable to those in starburst-driven superwinds. <span class="hlt">Large-scale</span> radio sources in Seyferts appear diffuse, but do not resemble radio halos found in some edge-on starburst galaxies (e.g. M82). We discuss the feasibility of the outflows being powered by the active nucleus (e.g. a jet) or a circumnuclear starburst.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/10769384','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/10769384"><span><span class="hlt">Large-scale</span> oscillatory calcium waves in the immature cortex.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Garaschuk, O; Linn, J; Eilers, J; Konnerth, A</p> <p>2000-05-01</p> <p>Two-photon imaging of <span class="hlt">large</span> neuronal networks in cortical slices of newborn rats <span class="hlt">revealed</span> synchronized oscillations in intracellular Ca2+ concentration. These spontaneous Ca2+ waves usually started in the posterior cortex and propagated slowly (2.1 mm per second) toward its anterior end. Ca2+ waves were associated with field-potential changes and required activation of AMPA and NMDA receptors. Although GABAA receptors were not involved in wave initiation, the developmental transition of GABAergic transmission from depolarizing to hyperpolarizing (around postnatal day 7) stopped the oscillatory activity. Thus we identified a type of <span class="hlt">large-scale</span> Ca2+ wave that may regulate long-distance wiring in the immature cortex.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..MARX44007H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..MARX44007H"><span>A novel computational approach towards the certification of <span class="hlt">large-scale</span> boson sampling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huh, Joonsuk</p> <p></p> <p>Recent proposals of boson sampling and the corresponding experiments exhibit the possible disproof of extended Church-Turning Thesis. Furthermore, the application of boson sampling to molecular computation has been suggested theoretically. Till now, however, only small-<span class="hlt">scale</span> experiments with a few photons have been successfully performed. The boson sampling experiments of 20-30 photons are expected to <span class="hlt">reveal</span> the computational superiority of the quantum device. A novel theoretical proposal for the <span class="hlt">large-scale</span> boson sampling using microwave photons is highly promising due to the deterministic photon sources and the scalability. Therefore, the certification protocol of <span class="hlt">large-scale</span> boson sampling experiments should be presented to complete the exciting story. We propose, in this presentation, a computational protocol towards the certification of <span class="hlt">large-scale</span> boson sampling. The correlations of paired photon modes and the time-dependent characteristic functional with its Fourier component can show the fingerprint of <span class="hlt">large-scale</span> boson sampling. This work was supported by Basic Science Research Program through the National Research Foundation of Korea(NRF) funded by the Ministry of Education, Science and Technology(NRF-2015R1A6A3A04059773), the ICT R&D program of MSIP/IITP [2015-019, Fundamental Research Toward Secure Quantum Communication] and Mueunjae Institute for Chemistry (MIC) postdoctoral fellowship.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22251573-synchronization-coupled-large-scale-boolean-networks','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22251573-synchronization-coupled-large-scale-boolean-networks"><span>Synchronization of coupled <span class="hlt">large-scale</span> Boolean networks</span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Li, Fangfei, E-mail: li-fangfei@163.com</p> <p>2014-03-15</p> <p>This paper investigates the complete synchronization and partial synchronization of two <span class="hlt">large-scale</span> Boolean networks. First, the aggregation algorithm towards <span class="hlt">large-scale</span> Boolean network is reviewed. Second, the aggregation algorithm is applied to study the complete synchronization and partial synchronization of <span class="hlt">large-scale</span> Boolean networks. Finally, an illustrative example is presented to show the efficiency of the proposed results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA595017','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA595017"><span>Global Behavior in <span class="hlt">Large</span> <span class="hlt">Scale</span> Systems</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2013-12-05</p> <p>release. <span class="hlt">AIR</span> FORCE RESEARCH LABORATORY AF OFFICE OF SCIENTIFIC RESEARCH (AFOSR)/RSL ARLINGTON, VIRGINIA 22203 <span class="hlt">AIR</span> FORCE MATERIEL COMMAND AFRL-OSR-VA...and Research 875 Randolph Street, Suite 325 Room 3112, Arlington, VA 22203 December 3, 2013 1 Abstract This research attained two main achievements: 1...microscopic random interactions among the agents. 2 1 Introduction In this research we considered two main problems: 1) <span class="hlt">large</span> deviation error performance in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1092307-genome-resequencing-populus-revealing-large-scale-genome-variation-implications-specialized-trait-genomics','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1092307-genome-resequencing-populus-revealing-large-scale-genome-variation-implications-specialized-trait-genomics"><span>Genome resequencing in Populus: <span class="hlt">Revealing</span> <span class="hlt">large-scale</span> genome variation and implications on specialized-trait genomics</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>Muchero, Wellington; Labbe, Jessy L; Priya, Ranjan</p> <p>2014-01-01</p> <p>To date, Populus ranks among a few plant species with a complete genome sequence and other highly developed genomic resources. With the first genome sequence among all tree species, Populus has been adopted as a suitable model organism for genomic studies in trees. However, far from being just a model species, Populus is a key renewable economic resource that plays a significant role in providing raw materials for the biofuel and pulp and paper industries. Therefore, aside from leading frontiers of basic tree molecular biology and ecological research, Populus leads frontiers in addressing global economic challenges related to fuel andmore » fiber production. The latter fact suggests that research aimed at improving quality and quantity of Populus as a raw material will likely drive the pursuit of more targeted and deeper research in order to unlock the economic potential tied in molecular biology processes that drive this tree species. Advances in genome sequence-driven technologies, such as resequencing individual genotypes, which in turn facilitates <span class="hlt">large</span> <span class="hlt">scale</span> SNP discovery and identification of <span class="hlt">large</span> <span class="hlt">scale</span> polymorphisms are key determinants of future success in these initiatives. In this treatise we discuss implications of genome sequence-enable technologies on Populus genomic and genetic studies of complex and specialized-traits.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AAS...23145411S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AAS...23145411S"><span>Dissecting the <span class="hlt">large-scale</span> galactic conformity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seo, Seongu</p> <p>2018-01-01</p> <p>Galactic conformity is an observed phenomenon that galaxies located in the same region have similar properties such as star formation rate, color, gas fraction, and so on. The conformity was first observed among galaxies within in the same halos (“one-halo conformity”). The one-halo conformity can be readily explained by mutual interactions among galaxies within a halo. Recent observations however further witnessed a puzzling connection among galaxies with no direct interaction. In particular, galaxies located within a sphere of ~5 Mpc radius tend to show similarities, even though the galaxies do not share common halos with each other ("two-halo conformity" or “<span class="hlt">large-scale</span> conformity”). Using a cosmological hydrodynamic simulation, Illustris, we investigate the physical origin of the two-halo conformity and put forward two scenarios. First, back-splash galaxies are likely responsible for the <span class="hlt">large-scale</span> conformity. They have evolved into red galaxies due to ram-pressure stripping in a given galaxy cluster and happen to reside now within a ~5 Mpc sphere. Second, galaxies in strong tidal field induced by <span class="hlt">large-scale</span> structure also seem to give rise to the <span class="hlt">large-scale</span> conformity. The strong tides suppress star formation in the galaxies. We discuss the importance of the <span class="hlt">large-scale</span> conformity in the context of galaxy evolution.</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/2017APS..DFDA26003H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..DFDA26003H"><span>A spatial picture of the synthetic <span class="hlt">large-scale</span> motion from dynamic roughness</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huynh, David; McKeon, Beverley</p> <p>2017-11-01</p> <p>Jacobi and McKeon (2011) set up a dynamic roughness apparatus to excite a synthetic, travelling wave-like disturbance in a wind tunnel, boundary layer study. In the present work, this dynamic roughness has been adapted for a flat-plate, turbulent boundary layer experiment in a water tunnel. A key advantage of operating in water as opposed to <span class="hlt">air</span> is the longer flow timescales. This makes accessible higher non-dimensional actuation frequencies and correspondingly shorter synthetic length <span class="hlt">scales</span>, and is thus more amenable to particle image velocimetry. As a result, this experiment provides a novel spatial picture of the synthetic mode, the coupled small <span class="hlt">scales</span>, and their streamwise development. It is demonstrated that varying the roughness actuation frequency allows for significant tuning of the streamwise wavelength of the synthetic mode, with a range of 3 δ-13 δ being achieved. Employing a phase-locked decomposition, spatial snapshots are constructed of the synthetic <span class="hlt">large</span> <span class="hlt">scale</span> and used to analyze its streamwise behavior. Direct spatial filtering is used to separate the synthetic <span class="hlt">large</span> <span class="hlt">scale</span> and the related small <span class="hlt">scales</span>, and the results are compared to those obtained by temporal filtering that invokes Taylor's hypothesis. The support of AFOSR (Grant # FA9550-16-1-0361) is gratefully acknowledged.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvD..97f3504C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvD..97f3504C"><span>Closing in on the <span class="hlt">large-scale</span> CMB power asymmetry</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Contreras, D.; Hutchinson, J.; Moss, A.; Scott, D.; Zibin, J. P.</p> <p>2018-03-01</p> <p>Measurements of the cosmic microwave background (CMB) temperature anisotropies have <span class="hlt">revealed</span> a dipolar asymmetry in power at the largest <span class="hlt">scales</span>, in apparent contradiction with the statistical isotropy of standard cosmological models. The significance of the effect is not very high, and is dependent on a posteriori choices. Nevertheless, a number of models have been proposed that produce a <span class="hlt">scale</span>-dependent asymmetry. We confront several such models for a physical, position-space modulation with CMB temperature observations. We find that, while some models that maintain the standard isotropic power spectrum are allowed, others, such as those with modulated tensor or uncorrelated isocurvature modes, can be ruled out on the basis of the overproduction of isotropic power. This remains the case even when an extra isocurvature mode fully anticorrelated with the adiabatic perturbations is added to suppress power on <span class="hlt">large</span> <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4750464','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4750464"><span>Systems Perturbation Analysis of a <span class="hlt">Large-Scale</span> Signal Transduction Model <span class="hlt">Reveals</span> Potentially Influential Candidates for Cancer Therapeutics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Puniya, Bhanwar Lal; Allen, Laura; Hochfelder, Colleen; Majumder, Mahbubul; Helikar, Tomáš</p> <p>2016-01-01</p> <p>Dysregulation in signal transduction pathways can lead to a variety of complex disorders, including cancer. Computational approaches such as network analysis are important tools to understand system dynamics as well as to identify critical components that could be further explored as therapeutic targets. Here, we performed perturbation analysis of a <span class="hlt">large-scale</span> signal transduction model in extracellular environments that stimulate cell death, growth, motility, and quiescence. Each of the model’s components was perturbed under both loss-of-function and gain-of-function mutations. Using 1,300 simulations under both types of perturbations across various extracellular conditions, we identified the most and least influential components based on the magnitude of their influence on the rest of the system. Based on the premise that the most influential components might serve as better drug targets, we characterized them for biological functions, housekeeping genes, essential genes, and druggable proteins. The most influential components under all environmental conditions were enriched with several biological processes. The inositol pathway was found as most influential under inactivating perturbations, whereas the kinase and small lung cancer pathways were identified as the most influential under activating perturbations. The most influential components were enriched with essential genes and druggable proteins. Moreover, known cancer drug targets were also classified in influential components based on the affected components in the network. Additionally, the systemic perturbation analysis of the model <span class="hlt">revealed</span> a network motif of most influential components which affect each other. Furthermore, our analysis predicted novel combinations of cancer drug targets with various effects on other most influential components. We found that the combinatorial perturbation consisting of PI3K inactivation and overactivation of IP3R1 can lead to increased activity levels of apoptosis</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28959632','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28959632"><span>Diacetyl and 2,3-pentanedione in breathing zone and area <span class="hlt">air</span> during <span class="hlt">large-scale</span> commercial coffee roasting, blending and grinding processes.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McCoy, Michael J; Hoppe Parr, Kimberly A; Anderson, Kim E; Cornish, Jim; Haapala, Matti; Greivell, John</p> <p>2017-01-01</p> <p>Recently described scientific literature has identified the airborne presence of 2,3-butanedione (diacetyl) and 2,3-pentanedione at concentrations approaching or potentially exceeding the current American Conference of Industrial Hygienists' (ACGIH) Threshold Limit Values (TLVs) at commercial coffee roasting and production facilities. Newly established National Institutes of Occupational Safety and Health (NIOSH) Recommended Exposure Limits for diacetyl and 2,3-pentanedione are even more conservative. Chronic exposure to these alpha-diketones at elevated airborne concentrations has been associated with lung damage, specifically bronchiolitis obliterans, most notably in industrial food processing facilities. Workers at a <span class="hlt">large</span> commercial coffee roaster were monitored for both eight-hour and task-based, short-term, 15-min sample durations for airborne concentrations of these alpha-diketones during specific work processes, including the coffee bean roasting, blending and grinding processes, during two separate 8-h work periods. Additionally, the authors performed real-time Fourier transform infrared spectroscopy (FTIR) analysis of the workers' breathing zone as well as the area workplace <span class="hlt">air</span> for the presence of organic compounds to determine the sources, as well as quantitate and identify various organic compounds proximal to the roasting and grinding processes. Real-time FTIR measurements provided both the identification and quantitation of diacetyl and 2,3-pentanedione, as well as other organic compounds generated during coffee bean roasting and grinding operations. Airborne concentrations of diacetyl in the workers' breathing zone, as eight-hour time-weighted averages were less than the ACGIH TLVs for diacetyl, while concentrations of 2,3-pentanedione were below the limit of detection in all samples. Short-term breathing zone samples <span class="hlt">revealed</span> airborne concentrations for diacetyl that exceeded the ACGIH short-term exposure limit of 0.02 parts per million (ppm) in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29388242','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29388242"><span><span class="hlt">Large</span> <span class="hlt">scale</span> ab initio modeling of structurally uncharacterized antimicrobial peptides <span class="hlt">reveals</span> known and novel folds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kozic, Mara; Fox, Stephen J; Thomas, Jens M; Verma, Chandra S; Rigden, Daniel J</p> <p>2018-05-01</p> <p>Antimicrobial resistance within a wide range of infectious agents is a severe and growing public health threat. Antimicrobial peptides (AMPs) are among the leading alternatives to current antibiotics, exhibiting broad spectrum activity. Their activity is determined by numerous properties such as cationic charge, amphipathicity, size, and amino acid composition. Currently, only around 10% of known AMP sequences have experimentally solved structures. To improve our understanding of the AMP structural universe we have carried out <span class="hlt">large</span> <span class="hlt">scale</span> ab initio 3D modeling of structurally uncharacterized AMPs that <span class="hlt">revealed</span> similarities between predicted folds of the modeled sequences and structures of characterized AMPs. Two of the peptides whose models matched known folds are Lebocin Peptide 1A (LP1A) and Odorranain M, predicted to form β-hairpins but, interestingly, to lack the intramolecular disulfide bonds, cation-π or aromatic interactions that generally stabilize such AMP structures. Other examples include Ponericin Q42, Latarcin 4a, Kassinatuerin 1, Ceratotoxin D, and CPF-B1 peptide, which have α-helical folds, as well as mixed αβ folds of human Histatin 2 peptide and Garvicin A which are, to the best of our knowledge, the first linear αββ fold AMPs lacking intramolecular disulfide bonds. In addition to fold matches to experimentally derived structures, unique folds were also obtained, namely for Microcin M and Ipomicin. These results help in understanding the range of protein scaffolds that naturally bear antimicrobial activity and may facilitate protein design efforts towards better AMPs. © 2018 The Authors Proteins: Structure, Function, and Bioinformatics Published by Wiley Periodicals, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1188620-scaling-design-analyses-scaled-down-high-temperature-test-facility-experimental-investigation-initial-stages-vhtr-air-ingress-accident','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1188620-scaling-design-analyses-scaled-down-high-temperature-test-facility-experimental-investigation-initial-stages-vhtr-air-ingress-accident"><span><span class="hlt">Scaling</span> and design analyses of a <span class="hlt">scaled</span>-down, high-temperature test facility for experimental investigation of the initial stages of a VHTR <span class="hlt">air</span>-ingress accident</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>Arcilesi, David J.; Ham, Tae Kyu; Kim, In Hun</p> <p>2015-07-01</p> <p>A critical event in the safety analysis of the very high-temperature gas-cooled reactor (VHTR) is an <span class="hlt">air</span>-ingress accident. This accident is initiated, in its worst case scenario, by a double-ended guillotine break of the coaxial cross vessel, which leads to a rapid reactor vessel depressurization. In a VHTR, the reactor vessel is located within a reactor cavity that is filled with <span class="hlt">air</span> during normal operating conditions. Following the vessel depressurization, the dominant mode of ingress of an air–helium mixture into the reactor vessel will either be molecular diffusion or density-driven stratified flow. The mode of ingress is hypothesized to dependmore » <span class="hlt">largely</span> on the break conditions of the cross vessel. Since the time <span class="hlt">scales</span> of these two ingress phenomena differ by orders of magnitude, it is imperative to understand under which conditions each of these mechanisms will dominate in the <span class="hlt">air</span> ingress process. Computer models have been developed to analyze this type of accident scenario. There are, however, limited experimental data available to understand the phenomenology of the <span class="hlt">air</span>-ingress accident and to validate these models. Therefore, there is a need to design and construct a <span class="hlt">scaled</span>-down experimental test facility to simulate the <span class="hlt">air</span>-ingress accident scenarios and to collect experimental data. The current paper focuses on the analyses performed for the design and operation of a 1/8th geometric <span class="hlt">scale</span> (by height and diameter), high-temperature test facility. A geometric <span class="hlt">scaling</span> analysis for the VHTR, a time <span class="hlt">scale</span> analysis of the <span class="hlt">air</span>-ingress phenomenon, a transient depressurization analysis of the reactor vessel, a hydraulic similarity analysis of the test facility, a heat transfer characterization of the hot plenum, a power <span class="hlt">scaling</span> analysis for the reactor system, and a design analysis of the containment vessel are discussed.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998myco.conf..234F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998myco.conf..234F"><span>The <span class="hlt">Large</span> -<span class="hlt">scale</span> Distribution of Galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flin, Piotr</p> <p></p> <p>A review of the <span class="hlt">Large-scale</span> structure of the Universe is given. A connection is made with the titanic work by Johannes Kepler in many areas of astronomy and cosmology. A special concern is made to spatial distribution of Galaxies, voids and walls (cellular structure of the Universe). Finaly, the author is concluding that the <span class="hlt">large</span> <span class="hlt">scale</span> structure of the Universe can be observed in much greater <span class="hlt">scale</span> that it was thought twenty years ago.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880042598&hterms=attention+pictures&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dattention%2Bpictures','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880042598&hterms=attention+pictures&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dattention%2Bpictures"><span>Rossby waves and two-dimensional turbulence in a <span class="hlt">large-scale</span> zonal jet</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Shepherd, Theodor G.</p> <p>1987-01-01</p> <p>Homogeneous barotropic beta-plane turbulence is investigated, taking into account the effects of spatial inhomogeneity in the form of a zonal shear flows. Attention is given to the case of zonal flows that are barotropically stable and of larger <span class="hlt">scale</span> than the resulting transient eddy field. Numerical simulations <span class="hlt">reveal</span> that <span class="hlt">large-scale</span> zonal flows alter the picture of classical beta-plane turbulence. It is found that the disturbance field penetrates to the largest <span class="hlt">scales</span> of motion, that the larger disturbance <span class="hlt">scales</span> show a tendency to meridional rather than zonal anisotropy, and that the initial spectral transfer rate away from an isotropic intermediate-<span class="hlt">scale</span> source is enhanced by the shear-induced transfer associated with straining by the zonal flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170008805','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170008805"><span>Results of <span class="hlt">Large-Scale</span> Spacecraft Flammability Tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ferkul, Paul; Olson, Sandra; Urban, David L.; Ruff, Gary A.; Easton, John; T'ien, James S.; Liao, Ta-Ting T.; Fernandez-Pello, A. Carlos; Torero, Jose L.; Eigenbrand, Christian; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170008805'); toggleEditAbsImage('author_20170008805_show'); toggleEditAbsImage('author_20170008805_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170008805_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170008805_hide"></p> <p>2017-01-01</p> <p>For the first time, a <span class="hlt">large-scale</span> fire was intentionally set inside a spacecraft while in orbit. Testing in low gravity aboard spacecraft had been limited to samples of modest size: for thin fuels the longest samples burned were around 15 cm in length and thick fuel samples have been even smaller. This is despite the fact that fire is a catastrophic hazard for spaceflight and the spread and growth of a fire, combined with its interactions with the vehicle cannot be expected to <span class="hlt">scale</span> linearly. While every type of occupied structure on earth has been the subject of full <span class="hlt">scale</span> fire testing, this had never been attempted in space owing to the complexity, cost, risk and absence of a safe location. Thus, there is a gap in knowledge of fire behavior in spacecraft. The recent utilization of <span class="hlt">large</span>, unmanned, resupply craft has provided the needed capability: a habitable but unoccupied spacecraft in low earth orbit. One such vehicle was used to study the flame spread over a 94 x 40.6 cm thin charring solid (fiberglasscotton fabric). The sample was an order of magnitude larger than anything studied to date in microgravity and was of sufficient <span class="hlt">scale</span> that it consumed 1.5 of the available oxygen. The experiment which is called Saffire consisted of two tests, forward or concurrent flame spread (with the direction of flow) and opposed flame spread (against the direction of flow). The average forced <span class="hlt">air</span> speed was 20 cms. For the concurrent flame spread test, the flame size remained constrained after the ignition transient, which is not the case in 1-g. These results were qualitatively different from those on earth where an upward-spreading flame on a sample of this size accelerates and grows. In addition, a curious effect of the chamber size is noted. Compared to previous microgravity work in smaller tunnels, the flame in the larger tunnel spread more slowly, even for a wider sample. This is attributed to the effect of flow acceleration in the smaller tunnels as a result of hot</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/978329','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/978329"><span><span class="hlt">Large-scale</span> functional models of visual cortex for remote sensing</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>Brumby, Steven P; Kenyon, Garrett; Rasmussen, Craig E</p> <p></p> <p>Neuroscience has <span class="hlt">revealed</span> many properties of neurons and of the functional organization of visual cortex that are believed to be essential to human vision, but are missing in standard artificial neural networks. Equally important may be the sheer <span class="hlt">scale</span> of visual cortex requiring {approx}1 petaflop of computation. In a year, the retina delivers {approx}1 petapixel to the brain, leading to massively <span class="hlt">large</span> opportunities for learning at many levels of the cortical system. We describe work at Los Alamos National Laboratory (LANL) to develop <span class="hlt">large-scale</span> functional models of visual cortex on LANL's Roadrunner petaflop supercomputer. An initial run of a simplemore » region VI code achieved 1.144 petaflops during trials at the IBM facility in Poughkeepsie, NY (June 2008). Here, we present criteria for assessing when a set of learned local representations is 'complete' along with general criteria for assessing computer vision models based on their projected <span class="hlt">scaling</span> behavior. Finally, we extend one class of biologically-inspired learning models to problems of remote sensing imagery.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1913162L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1913162L"><span>Super Clausius-Clapeyron <span class="hlt">scaling</span> of extreme hourly precipitation and its relation to <span class="hlt">large-scale</span> atmospheric conditions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenderink, Geert; Barbero, Renaud; Loriaux, Jessica; Fowler, Hayley</p> <p>2017-04-01</p> <p>Present-day precipitation-temperature <span class="hlt">scaling</span> relations indicate that hourly precipitation extremes may have a response to warming exceeding the Clausius-Clapeyron (CC) relation; for The Netherlands the dependency on surface dew point temperature follows two times the CC relation corresponding to 14 % per degree. Our hypothesis - as supported by a simple physical argument presented here - is that this 2CC behaviour arises from the physics of convective clouds. So, we think that this response is due to local feedbacks related to the convective activity, while other <span class="hlt">large</span> <span class="hlt">scale</span> atmospheric forcing conditions remain similar except for the higher temperature (approximately uniform warming with height) and absolute humidity (corresponding to the assumption of unchanged relative humidity). To test this hypothesis, we analysed the <span class="hlt">large-scale</span> atmospheric conditions accompanying summertime afternoon precipitation events using surface observations combined with a regional re-analysis for the data in The Netherlands. Events are precipitation measurements clustered in time and space derived from approximately 30 automatic weather stations. The hourly peak intensities of these events again <span class="hlt">reveal</span> a 2CC <span class="hlt">scaling</span> with the surface dew point temperature. The temperature excess of moist updrafts initialized at the surface and the maximum cloud depth are clear functions of surface dew point temperature, confirming the key role of surface humidity on convective activity. Almost no differences in relative humidity and the dry temperature lapse rate were found across the dew point temperature range, supporting our theory that 2CC <span class="hlt">scaling</span> is mainly due to the response of convection to increases in near surface humidity, while other atmospheric conditions remain similar. Additionally, hourly precipitation extremes are on average accompanied by substantial <span class="hlt">large-scale</span> upward motions and therefore <span class="hlt">large-scale</span> moisture convergence, which appears to accelerate with surface dew point. This</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750021772','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750021772"><span><span class="hlt">Large</span> <span class="hlt">scale</span> dynamic systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Doolin, B. F.</p> <p>1975-01-01</p> <p>Classes of <span class="hlt">large</span> <span class="hlt">scale</span> dynamic systems were discussed in the context of modern control theory. Specific examples discussed were in the technical fields of aeronautics, water resources and electric power.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/44861','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/44861"><span><span class="hlt">Large-scale</span> monitoring of <span class="hlt">air</span> pollution in remote and ecologically important areas</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Andrzej Bytnerowicz; Witold Fraczek</p> <p>2013-01-01</p> <p>New advances in <span class="hlt">air</span> quality monitoring techniques, such as passive samplers for nitrogenous (N) or sulphurous (S) pollutants and ozone (O3), have allowed for an improved understanding of concentrations of these pollutants in remote areas. Mountains create special problems with regard to the feasibility of establishing and maintaining <span class="hlt">air</span> pollution monitoring networks,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4380490','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4380490"><span>Computational Models of Consumer Confidence from <span class="hlt">Large-Scale</span> Online Attention Data: Crowd-Sourcing Econometrics</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>2015-01-01</p> <p>Economies are instances of complex socio-technical systems that are shaped by the interactions of <span class="hlt">large</span> numbers of individuals. The individual behavior and decision-making of consumer agents is determined by complex psychological dynamics that include their own assessment of present and future economic conditions as well as those of others, potentially leading to feedback loops that affect the macroscopic state of the economic system. We propose that the <span class="hlt">large-scale</span> interactions of a nation's citizens with its online resources can <span class="hlt">reveal</span> the complex dynamics of their collective psychology, including their assessment of future system states. Here we introduce a behavioral index of Chinese Consumer Confidence (C3I) that computationally relates <span class="hlt">large-scale</span> online search behavior recorded by Google Trends data to the macroscopic variable of consumer confidence. Our results indicate that such computational indices may <span class="hlt">reveal</span> the components and complex dynamics of consumer psychology as a collective socio-economic phenomenon, potentially leading to improved and more refined economic forecasting. PMID:25826692</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25826692','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25826692"><span>Computational models of consumer confidence from <span class="hlt">large-scale</span> online attention data: crowd-sourcing econometrics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dong, Xianlei; Bollen, Johan</p> <p>2015-01-01</p> <p>Economies are instances of complex socio-technical systems that are shaped by the interactions of <span class="hlt">large</span> numbers of individuals. The individual behavior and decision-making of consumer agents is determined by complex psychological dynamics that include their own assessment of present and future economic conditions as well as those of others, potentially leading to feedback loops that affect the macroscopic state of the economic system. We propose that the <span class="hlt">large-scale</span> interactions of a nation's citizens with its online resources can <span class="hlt">reveal</span> the complex dynamics of their collective psychology, including their assessment of future system states. Here we introduce a behavioral index of Chinese Consumer Confidence (C3I) that computationally relates <span class="hlt">large-scale</span> online search behavior recorded by Google Trends data to the macroscopic variable of consumer confidence. Our results indicate that such computational indices may <span class="hlt">reveal</span> the components and complex dynamics of consumer psychology as a collective socio-economic phenomenon, potentially leading to improved and more refined economic forecasting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://lofe.dukejournals.org/content/2/1.abstract','USGSPUBS'); return false;" href="http://lofe.dukejournals.org/content/2/1.abstract"><span><span class="hlt">Air</span>-water oxygen exchange in a <span class="hlt">large</span> whitewater river</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Hall, Robert O.; Kennedy, Theodore A.; Rosi-Marshall, Emma J.</p> <p>2012-01-01</p> <p><span class="hlt">Air</span>-water gas exchange governs fluxes of gas into and out of aquatic ecosystems. Knowing this flux is necessary to calculate gas budgets (i.e., O2) to estimate whole-ecosystem metabolism and basin-<span class="hlt">scale</span> carbon budgets. Empirical data on rates of gas exchange for streams, estuaries, and oceans are readily available. However, there are few data from <span class="hlt">large</span> rivers and no data from whitewater rapids. We measured gas transfer velocity in the Colorado River, Grand Canyon, as decline in O2 saturation deficit, 7 times in a 28-km segment spanning 7 rapids. The O2 saturation deficit exists because of hypolimnetic discharge from Glen Canyon Dam, located 25 km upriver from Lees Ferry. Gas transfer velocity (k600) increased with slope of the immediate reach. k600 was -1 in flat reaches, while k600 for the steepest rapid ranged 3600-7700 cm h-1, an extremely high value of k600. Using the rate of gas exchange per unit length of water surface elevation (Kdrop, m-1), segment-integrated k600 varied between 74 and 101 cm h-1. Using Kdrop we <span class="hlt">scaled</span> k600 to the remainder of the Colorado River in Grand Canyon. At the <span class="hlt">scale</span> corresponding to the segment length where 80% of the O2 exchanged with the atmosphere (mean length = 26.1 km), k600 varied 4.5-fold between 56 and 272 cm h-1 with a mean of 113 cm h-1. Gas transfer velocity for the Colorado River was higher than those from other aquatic ecosystems because of <span class="hlt">large</span> rapids. Our approach of <span class="hlt">scaling</span> k600 based on Kdrop allows comparing gas transfer velocity across rivers with spatially heterogeneous morphology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20060026026','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20060026026"><span>Aft-End Flow of a <span class="hlt">Large-Scale</span> Lifting Body During Free-Flight Tests</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Banks, Daniel W.; Fisher, David F.</p> <p>2006-01-01</p> <p>Free-flight tests of a <span class="hlt">large-scale</span> lifting-body configuration, the X-38 aircraft, were conducted using tufts to characterize the flow on the aft end, specifically in the inboard region of the vertical fins. Pressure data was collected on the fins and base. Flow direction and movement were correlated with surface pressure and flight condition. The X-38 was conceived to be a rescue vehicle for the International Space Station. The vehicle shape was derived from the U.S. <span class="hlt">Air</span> Force X-24 lifting body. Free-flight tests of the X-38 configuration were conducted at the NASA Dryden Flight Research Center at Edwards <span class="hlt">Air</span> Force Base, California from 1997 to 2001.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21568564','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21568564"><span>Transition from <span class="hlt">large-scale</span> to small-<span class="hlt">scale</span> dynamo.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ponty, Y; Plunian, F</p> <p>2011-04-15</p> <p>The dynamo equations are solved numerically with a helical forcing corresponding to the Roberts flow. In the fully turbulent regime the flow behaves as a Roberts flow on long time <span class="hlt">scales</span>, plus turbulent fluctuations at short time <span class="hlt">scales</span>. The dynamo onset is controlled by the long time <span class="hlt">scales</span> of the flow, in agreement with the former Karlsruhe experimental results. The dynamo mechanism is governed by a generalized α effect, which includes both the usual α effect and turbulent diffusion, plus all higher order effects. Beyond the onset we find that this generalized α effect <span class="hlt">scales</span> as O(Rm(-1)), suggesting the takeover of small-<span class="hlt">scale</span> dynamo action. This is confirmed by simulations in which dynamo occurs even if the <span class="hlt">large-scale</span> field is artificially suppressed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AtmEn..96..405P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AtmEn..96..405P"><span>Physicochemical characterization of smoke aerosol during <span class="hlt">large-scale</span> wildfires: Extreme event of August 2010 in Moscow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Popovicheva, O.; Kistler, M.; Kireeva, E.; Persiantseva, N.; Timofeev, M.; Kopeikin, V.; Kasper-Giebl, A.</p> <p>2014-10-01</p> <p> secondary inorganic species associated with wildfire gaseous emissions and their transformation in aged smoke. Accumulation of carbonyl compounds during extreme smoke event in Moscow resulted from photochemical aging and secondary organic aerosol (SOA) formation in the urban atmosphere. The mixture of carbonaceous particles and dust <span class="hlt">revealed</span> multicomponent structure of Moscow smoke aerosols, pointing the difference with non-smoke ambient aerosols. The abundance of group containing soot and tar balls approached at least a half of total aerosol concentration during extreme event, relating to elevated OC, EC and SOA. Fly ash groups contained calcium sulfates and carbonates from soil entrainment by hot <span class="hlt">air</span> convection. Small-<span class="hlt">scale</span> open fire experiments support the identification of specific chemical features of regional biomass burning and demonstrate the strong impact of <span class="hlt">large-scale</span> wildfires on aerosol chemistry and <span class="hlt">air</span> quality in highly polluted megacity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5214098','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5214098"><span>Tree Age Distributions <span class="hlt">Reveal</span> <span class="hlt">Large-Scale</span> Disturbance-Recovery Cycles in Three Tropical Forests</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Vlam, Mart; van der Sleen, Peter; Groenendijk, Peter; Zuidema, Pieter A.</p> <p>2017-01-01</p> <p>Over the past few decades there has been a growing realization that a <span class="hlt">large</span> share of apparently ‘virgin’ or ‘old-growth’ tropical forests carries a legacy of past natural or anthropogenic disturbances that have a substantial effect on present-day forest composition, structure and dynamics. Yet, direct evidence of such disturbances is scarce and comparisons of disturbance dynamics across regions even more so. Here we present a tree-ring based reconstruction of disturbance histories from three tropical forest sites in Bolivia, Cameroon, and Thailand. We studied temporal patterns in tree regeneration of shade-intolerant tree species, because establishment of these trees is indicative for canopy disturbance. In three <span class="hlt">large</span> areas (140–300 ha), stem disks and increment cores were collected for a total of 1154 trees (>5 cm diameter) from 12 tree species to estimate the age of every tree. Using these age estimates we produced population age distributions, which were analyzed for evidence of past disturbance. Our approach allowed us to reconstruct patterns of tree establishment over a period of around 250 years. In Bolivia, we found continuous regeneration rates of three species and a peaked age distribution of a long-lived pioneer species. In both Cameroon and Thailand we found irregular age distributions, indicating strongly reduced regeneration rates over a period of 10–60 years. Past fires, windthrow events or anthropogenic disturbances all provide plausible explanations for the reported variation in tree age across the three sites. Our results support the recent idea that the long-term dynamics of tropical forests are impacted by <span class="hlt">large-scale</span> disturbance-recovery cycles, similar to those driving temperate forest dynamics. PMID:28105034</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/28105034','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28105034"><span>Tree Age Distributions <span class="hlt">Reveal</span> <span class="hlt">Large-Scale</span> Disturbance-Recovery Cycles in Three Tropical Forests.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vlam, Mart; van der Sleen, Peter; Groenendijk, Peter; Zuidema, Pieter A</p> <p>2016-01-01</p> <p>Over the past few decades there has been a growing realization that a <span class="hlt">large</span> share of apparently 'virgin' or 'old-growth' tropical forests carries a legacy of past natural or anthropogenic disturbances that have a substantial effect on present-day forest composition, structure and dynamics. Yet, direct evidence of such disturbances is scarce and comparisons of disturbance dynamics across regions even more so. Here we present a tree-ring based reconstruction of disturbance histories from three tropical forest sites in Bolivia, Cameroon, and Thailand. We studied temporal patterns in tree regeneration of shade-intolerant tree species, because establishment of these trees is indicative for canopy disturbance. In three <span class="hlt">large</span> areas (140-300 ha), stem disks and increment cores were collected for a total of 1154 trees (>5 cm diameter) from 12 tree species to estimate the age of every tree. Using these age estimates we produced population age distributions, which were analyzed for evidence of past disturbance. Our approach allowed us to reconstruct patterns of tree establishment over a period of around 250 years. In Bolivia, we found continuous regeneration rates of three species and a peaked age distribution of a long-lived pioneer species. In both Cameroon and Thailand we found irregular age distributions, indicating strongly reduced regeneration rates over a period of 10-60 years. Past fires, windthrow events or anthropogenic disturbances all provide plausible explanations for the reported variation in tree age across the three sites. Our results support the recent idea that the long-term dynamics of tropical forests are impacted by <span class="hlt">large-scale</span> disturbance-recovery cycles, similar to those driving temperate forest dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25835386','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25835386"><span>Bio-inspired wooden actuators for <span class="hlt">large</span> <span class="hlt">scale</span> applications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rüggeberg, Markus; Burgert, Ingo</p> <p>2015-01-01</p> <p>Implementing programmable actuation into materials and structures is a major topic in the field of smart materials. In particular the bilayer principle has been employed to develop actuators that respond to various kinds of stimuli. A multitude of small <span class="hlt">scale</span> applications down to micrometer size have been developed, but up-<span class="hlt">scaling</span> remains challenging due to either limitations in mechanical stiffness of the material or in the manufacturing processes. Here, we demonstrate the actuation of wooden bilayers in response to changes in relative humidity, making use of the high material stiffness and a good machinability to reach <span class="hlt">large</span> <span class="hlt">scale</span> actuation and application. Amplitude and response time of the actuation were measured and can be predicted and controlled by adapting the geometry and the constitution of the bilayers. Field tests in full weathering conditions <span class="hlt">revealed</span> long-term stability of the actuation. The potential of the concept is shown by a first demonstrator. With the sensor and actuator intrinsically incorporated in the wooden bilayers, the daily change in relative humidity is exploited for an autonomous and solar powered movement of a tracker for solar modules.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A23D0348W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A23D0348W"><span>Modeling the MJO rain rates using parameterized <span class="hlt">large</span> <span class="hlt">scale</span> dynamics: vertical structure, radiation, and horizontal advection of dry <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, S.; Sobel, A. H.; Nie, J.</p> <p>2015-12-01</p> <p>Two Madden Julian Oscillation (MJO) events were observed during October and November 2011 in the equatorial Indian Ocean during the DYNAMO field campaign. Precipitation rates and <span class="hlt">large-scale</span> vertical motion profiles derived from the DYNAMO northern sounding array are simulated in a small-domain cloud-resolving model using parameterized <span class="hlt">large-scale</span> dynamics. Three parameterizations of <span class="hlt">large-scale</span> dynamics --- the conventional weak temperature gradient (WTG) approximation, vertical mode based spectral WTG (SWTG), and damped gravity wave coupling (DGW) --- are employed. The target temperature profiles and radiative heating rates are taken from a control simulation in which the <span class="hlt">large-scale</span> vertical motion is imposed (rather than directly from observations), and the model itself is significantly modified from that used in previous work. These methodological changes lead to significant improvement in the results.Simulations using all three methods, with imposed time -dependent radiation and horizontal moisture advection, capture the time variations in precipitation associated with the two MJO events well. The three methods produce significant differences in the <span class="hlt">large-scale</span> vertical motion profile, however. WTG produces the most top-heavy and noisy profiles, while DGW's is smoother with a peak in midlevels. SWTG produces a smooth profile, somewhere between WTG and DGW, and in better agreement with observations than either of the others. Numerical experiments without horizontal advection of moisture suggest that that process significantly reduces the precipitation and suppresses the top-heaviness of <span class="hlt">large-scale</span> vertical motion during the MJO active phases, while experiments in which the effect of cloud on radiation are disabled indicate that cloud-radiative interaction significantly amplifies the MJO. Experiments in which interactive radiation is used produce poorer agreement with observation than those with imposed time-varying radiative heating. Our results highlight the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23036648','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23036648"><span>Why small-<span class="hlt">scale</span> cannabis growers stay small: five mechanisms that prevent small-<span class="hlt">scale</span> growers from going <span class="hlt">large</span> <span class="hlt">scale</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hammersvik, Eirik; Sandberg, Sveinung; Pedersen, Willy</p> <p>2012-11-01</p> <p>Over the past 15-20 years, domestic cultivation of cannabis has been established in a number of European countries. New techniques have made such cultivation easier; however, the bulk of growers remain small-<span class="hlt">scale</span>. In this study, we explore the factors that prevent small-<span class="hlt">scale</span> growers from increasing their production. The study is based on 1 year of ethnographic fieldwork and qualitative interviews conducted with 45 Norwegian cannabis growers, 10 of whom were growing on a <span class="hlt">large-scale</span> and 35 on a small-<span class="hlt">scale</span>. The study identifies five mechanisms that prevent small-<span class="hlt">scale</span> indoor growers from going <span class="hlt">large-scale</span>. First, <span class="hlt">large-scale</span> operations involve a number of people, <span class="hlt">large</span> sums of money, a high work-load and a high risk of detection, and thus demand a higher level of organizational skills than for small growing operations. Second, financial assets are needed to start a <span class="hlt">large</span> 'grow-site'. Housing rent, electricity, equipment and nutrients are expensive. Third, to be able to sell <span class="hlt">large</span> quantities of cannabis, growers need access to an illegal distribution network and knowledge of how to act according to black market norms and structures. Fourth, <span class="hlt">large-scale</span> operations require advanced horticultural skills to maximize yield and quality, which demands greater skills and knowledge than does small-<span class="hlt">scale</span> cultivation. Fifth, small-<span class="hlt">scale</span> growers are often embedded in the 'cannabis culture', which emphasizes anti-commercialism, anti-violence and ecological and community values. Hence, starting up <span class="hlt">large-scale</span> production will imply having to renegotiate or abandon these values. Going from small- to <span class="hlt">large-scale</span> cannabis production is a demanding task-ideologically, technically, economically and personally. The many obstacles that small-<span class="hlt">scale</span> growers face and the lack of interest and motivation for going <span class="hlt">large-scale</span> suggest that the risk of a 'slippery slope' from small-<span class="hlt">scale</span> to <span class="hlt">large-scale</span> growing is limited. Possible political implications of the findings are discussed. Copyright</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19621066','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19621066"><span>Development of <span class="hlt">large-scale</span> functional brain networks in children.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Supekar, Kaustubh; Musen, Mark; Menon, Vinod</p> <p>2009-07-01</p> <p>The ontogeny of <span class="hlt">large-scale</span> functional organization of the human brain is not well understood. Here we use network analysis of intrinsic functional connectivity to characterize the organization of brain networks in 23 children (ages 7-9 y) and 22 young-adults (ages 19-22 y). Comparison of network properties, including path-length, clustering-coefficient, hierarchy, and regional connectivity, <span class="hlt">revealed</span> that although children and young-adults' brains have similar "small-world" organization at the global level, they differ significantly in hierarchical organization and interregional connectivity. We found that subcortical areas were more strongly connected with primary sensory, association, and paralimbic areas in children, whereas young-adults showed stronger cortico-cortical connectivity between paralimbic, limbic, and association areas. Further, combined analysis of functional connectivity with wiring distance measures derived from white-matter fiber tracking <span class="hlt">revealed</span> that the development of <span class="hlt">large-scale</span> brain networks is characterized by weakening of short-range functional connectivity and strengthening of long-range functional connectivity. Importantly, our findings show that the dynamic process of over-connectivity followed by pruning, which rewires connectivity at the neuronal level, also operates at the systems level, helping to reconfigure and rebalance subcortical and paralimbic connectivity in the developing brain. Our study demonstrates the usefulness of network analysis of brain connectivity to elucidate key principles underlying functional brain maturation, paving the way for novel studies of disrupted brain connectivity in neurodevelopmental disorders such as autism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2705656','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2705656"><span>Development of <span class="hlt">Large-Scale</span> Functional Brain Networks in Children</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Supekar, Kaustubh; Musen, Mark; Menon, Vinod</p> <p>2009-01-01</p> <p>The ontogeny of <span class="hlt">large-scale</span> functional organization of the human brain is not well understood. Here we use network analysis of intrinsic functional connectivity to characterize the organization of brain networks in 23 children (ages 7–9 y) and 22 young-adults (ages 19–22 y). Comparison of network properties, including path-length, clustering-coefficient, hierarchy, and regional connectivity, <span class="hlt">revealed</span> that although children and young-adults' brains have similar “small-world” organization at the global level, they differ significantly in hierarchical organization and interregional connectivity. We found that subcortical areas were more strongly connected with primary sensory, association, and paralimbic areas in children, whereas young-adults showed stronger cortico-cortical connectivity between paralimbic, limbic, and association areas. Further, combined analysis of functional connectivity with wiring distance measures derived from white-matter fiber tracking <span class="hlt">revealed</span> that the development of <span class="hlt">large-scale</span> brain networks is characterized by weakening of short-range functional connectivity and strengthening of long-range functional connectivity. Importantly, our findings show that the dynamic process of over-connectivity followed by pruning, which rewires connectivity at the neuronal level, also operates at the systems level, helping to reconfigure and rebalance subcortical and paralimbic connectivity in the developing brain. Our study demonstrates the usefulness of network analysis of brain connectivity to elucidate key principles underlying functional brain maturation, paving the way for novel studies of disrupted brain connectivity in neurodevelopmental disorders such as autism. PMID:19621066</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26551120','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26551120"><span>Generation of <span class="hlt">Large-Scale</span> Magnetic Fields by Small-<span class="hlt">Scale</span> Dynamo in Shear Flows.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Squire, J; Bhattacharjee, A</p> <p>2015-10-23</p> <p>We propose a new mechanism for a turbulent mean-field dynamo in which the magnetic fluctuations resulting from a small-<span class="hlt">scale</span> dynamo drive the generation of <span class="hlt">large-scale</span> magnetic fields. This is in stark contrast to the common idea that small-<span class="hlt">scale</span> magnetic fields should be harmful to <span class="hlt">large-scale</span> dynamo action. These dynamos occur in the presence of a <span class="hlt">large-scale</span> velocity shear and do not require net helicity, resulting from off-diagonal components of the turbulent resistivity tensor as the magnetic analogue of the "shear-current" effect. Given the inevitable existence of nonhelical small-<span class="hlt">scale</span> magnetic fields in turbulent plasmas, as well as the generic nature of velocity shear, the suggested mechanism may help explain the generation of <span class="hlt">large-scale</span> magnetic fields across a wide range of astrophysical objects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4675713','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4675713"><span>Captured metagenomics: <span class="hlt">large-scale</span> targeting of genes based on ‘sequence capture’ <span class="hlt">reveals</span> functional diversity in soils</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Manoharan, Lokeshwaran; Kushwaha, Sandeep K.; Hedlund, Katarina; Ahrén, Dag</p> <p>2015-01-01</p> <p>Microbial enzyme diversity is a key to understand many ecosystem processes. Whole metagenome sequencing (WMG) obtains information on functional genes, but it is costly and inefficient due to <span class="hlt">large</span> amount of sequencing that is required. In this study, we have applied a captured metagenomics technique for functional genes in soil microorganisms, as an alternative to WMG. <span class="hlt">Large-scale</span> targeting of functional genes, coding for enzymes related to organic matter degradation, was applied to two agricultural soil communities through captured metagenomics. Captured metagenomics uses custom-designed, hybridization-based oligonucleotide probes that enrich functional genes of interest in metagenomic libraries where only probe-bound DNA fragments are sequenced. The captured metagenomes were highly enriched with targeted genes while maintaining their target diversity and their taxonomic distribution correlated well with the traditional ribosomal sequencing. The captured metagenomes were highly enriched with genes related to organic matter degradation; at least five times more than similar, publicly available soil WMG projects. This target enrichment technique also preserves the functional representation of the soils, thereby facilitating comparative metagenomics projects. Here, we present the first study that applies the captured metagenomics approach in <span class="hlt">large</span> <span class="hlt">scale</span>, and this novel method allows deep investigations of central ecosystem processes by studying functional gene abundances. PMID:26490729</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1815055L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1815055L"><span>Climate variability rather than overstocking causes recent <span class="hlt">large</span> <span class="hlt">scale</span> cover changes of Tibetan pastures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lehnert, Lukas; Wesche, Karsten; Trachte, Katja; Reudenbach, Christoph; Miehe, Georg; Bendix, Jörg</p> <p>2016-04-01</p> <p>The Tibetan Plateau has been entitled "Third-Pole-Environment" because of its outstanding importance for the climate and the hydrology in East and South-east Asia. Its climatological and hydrological influences are strongly affected by the local grassland vegetation which is supposed to be subject to ongoing degradation. On a local <span class="hlt">scale</span>, numerous studies focused on grassland degradation of the Tibetan pastures. However, because methods and <span class="hlt">scales</span> substantially differed among previous studies, the overall pattern of the degradation in the Tibetan Plateau is unknown. Consequently, a satellite based approach was selected to cope with the spatial limitations. Therefore, a MODIS-based vegetation cover product was developed which is fully validated against 600 in situ measurements covering a wide extent of the Tibetan Plateau. The vegetation cover as a proxy for grassland degradation is modelled with low error rates using support vector machine regressions. To identify the changes in the vegetation cover, the trends seen in the new vegetation cover product since the beginning of the new millennium were analysed. The drivers of the vegetation changes were identified by the analysis of trends of climatic variables (precipitation and 2 m <span class="hlt">air</span> temperature) and land-use (livestock numbers) over the same time. The results <span class="hlt">reveal</span> that - in contrast to the prevailing opinion - pasture degradation on the Tibetan Plateau is not a generally proceeding process because areas of positive and negative changes are almost equal in extent. The positive and negative vegetation changes have regionally different triggers: While, from 2000 on, the vegetation cover has increased in the north-eastern part of the Tibetan Plateau due to increasing precipitation, it has declined in the central and western parts due to rising <span class="hlt">air</span> temperature and declining precipitation. Increasing livestock numbers as a result of land use changes exacerbated the negative trends but, contrarily to the assumptions of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/13843','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/13843"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Traffic Simulations</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1997-01-01</p> <p><span class="hlt">Large</span> <span class="hlt">scale</span> microscopic (i.e. vehicle-based) traffic simulations pose high demands on computation speed in at least two application areas: (i) real-time traffic forecasting, and (ii) long-term planning applications (where repeated "looping" between t...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998PhDT........58C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998PhDT........58C"><span>Downscaling <span class="hlt">large-scale</span> circulation to local winter climate using neural network techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cavazos Perez, Maria Tereza</p> <p>1998-12-01</p> <p>The severe impacts of climate variability on society <span class="hlt">reveal</span> the increasing need for improving regional-<span class="hlt">scale</span> climate diagnosis. A new downscaling approach for climate diagnosis is developed here. It is based on neural network techniques that derive transfer functions from the <span class="hlt">large-scale</span> atmospheric controls to the local winter climate in northeastern Mexico and southeastern Texas during the 1985-93 period. A first neural network (NN) model employs time-lagged component scores from a rotated principal component analysis of SLP, 500-hPa heights, and 1000-500 hPa thickness as predictors of daily precipitation. The model is able to reproduce the phase and, to some decree, the amplitude of <span class="hlt">large</span> rainfall events, reflecting the influence of the <span class="hlt">large-scale</span> circulation. <span class="hlt">Large</span> errors are found over the Sierra Madre, over the Gulf of Mexico, and during El Nino events, suggesting an increase in the importance of meso-<span class="hlt">scale</span> rainfall processes. However, errors are also due to the lack of randomization of the input data and the absence of local atmospheric predictors such as moisture. Thus, a second NN model uses time-lagged specific humidity at the Earth's surface and at the 700 hPa level, SLP tendency, and 700-500 hPa thickness as input to a self-organizing map (SOM) that pre-classifies the atmospheric fields into different patterns. The results from the SOM classification document that negative (positive) anomalies of winter precipitation over the region are associated with: (1) weaker (stronger) Aleutian low; (2) stronger (weaker) North Pacific high; (3) negative (positive) phase of the Pacific North American pattern; and (4) La Nina (El Nino) events. The SOM atmospheric patterns are then used as input to a feed-forward NN that captures over 60% of the daily rainfall variance and 94% of the daily minimum temperature variance over the region. This demonstrates the ability of artificial neural network models to simulate realistic relationships on daily time <span class="hlt">scales</span>. The</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.B43C2133H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.B43C2133H"><span><span class="hlt">Large-scale</span> modeling on the fate and transport of polycyclic aromatic hydrocarbons (PAHs) in multimedia over China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Huang, Y.; Liu, M.; Wada, Y.; He, X.; Sun, X.</p> <p>2017-12-01</p> <p>In recent decades, with rapid economic growth, industrial development and urbanization, expanding pollution of polycyclic aromatic hydrocarbons (PAHs) has become a diversified and complicated phenomenon in China. However, the availability of sufficient monitoring activities for PAHs in multi-compartment and the corresponding multi-interface migration processes are still limited, especially at a <span class="hlt">large</span> geographic area. In this study, we couple the Multimedia Fate Model (MFM) to the Community Multi-<span class="hlt">Scale</span> <span class="hlt">Air</span> Quality (CMAQ) model in order to consider the fugacity and the transient contamination processes. This coupled dynamic contaminant model can evaluate the detailed local variations and mass fluxes of PAHs in different environmental media (e.g., <span class="hlt">air</span>, surface film, soil, sediment, water and vegetation) across different spatial (a county to country) and temporal (days to years) <span class="hlt">scales</span>. This model has been applied to a <span class="hlt">large</span> geographical domain of China at a 36 km by 36 km grid resolution. The model considers response characteristics of typical environmental medium to complex underlying surface. Results suggest that direct emission is the main input pathway of PAHs entering the atmosphere, while advection is the main outward flow of pollutants from the environment. In addition, both soil and sediment act as the main sink of PAHs and have the longest retention time. Importantly, the highest PAHs loadings are found in urbanized and densely populated regions of China, such as Yangtze River Delta and Pearl River Delta. This model can provide a good scientific basis towards a better understanding of the <span class="hlt">large-scale</span> dynamics of environmental pollutants for land conservation and sustainable development. In a next step, the dynamic contaminant model will be integrated with the continental-<span class="hlt">scale</span> hydrological and water resources model (i.e., Community Water Model, CWatM) to quantify a more accurate representation and feedbacks between the hydrological cycle and water quality at</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1259593-generation-large-scale-magnetic-fields-small-scale-dynamo-shear-flows','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1259593-generation-large-scale-magnetic-fields-small-scale-dynamo-shear-flows"><span>Generation of <span class="hlt">large-scale</span> magnetic fields by small-<span class="hlt">scale</span> dynamo in shear flows</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Squire, J.; Bhattacharjee, A.</p> <p>2015-10-20</p> <p>We propose a new mechanism for a turbulent mean-field dynamo in which the magnetic fluctuations resulting from a small-<span class="hlt">scale</span> dynamo drive the generation of <span class="hlt">large-scale</span> magnetic fields. This is in stark contrast to the common idea that small-<span class="hlt">scale</span> magnetic fields should be harmful to <span class="hlt">large-scale</span> dynamo action. These dynamos occur in the presence of a <span class="hlt">large-scale</span> velocity shear and do not require net helicity, resulting from off-diagonal components of the turbulent resistivity tensor as the magnetic analogue of the "shear-current" effect. Furthermore, given the inevitable existence of nonhelical small-<span class="hlt">scale</span> magnetic fields in turbulent plasmas, as well as the generic naturemore » of velocity shear, the suggested mechanism may help explain the generation of <span class="hlt">large-scale</span> magnetic fields across a wide range of astrophysical objects.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhDT........31Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhDT........31Y"><span><span class="hlt">Large-scale</span> assembly of colloidal particles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Hongta</p> <p></p> <p>This study reports a simple, roll-to-roll compatible coating technology for producing three-dimensional highly ordered colloidal crystal-polymer composites, colloidal crystals, and macroporous polymer membranes. A vertically beveled doctor blade is utilized to shear align silica microsphere-monomer suspensions to form <span class="hlt">large</span>-area composites in a single step. The polymer matrix and the silica microspheres can be selectively removed to create colloidal crystals and self-standing macroporous polymer membranes. The thickness of the shear-aligned crystal is correlated with the viscosity of the colloidal suspension and the coating speed, and the correlations can be qualitatively explained by adapting the mechanisms developed for conventional doctor blade coating. Five important research topics related to the application of <span class="hlt">large-scale</span> three-dimensional highly ordered macroporous films by doctor blade coating are covered in this study. The first topic describes the invention in <span class="hlt">large</span> area and low cost color reflective displays. This invention is inspired by the heat pipe technology. The self-standing macroporous polymer films exhibit brilliant colors which originate from the Bragg diffractive of visible light form the three-dimensional highly ordered <span class="hlt">air</span> cavities. The colors can be easily changed by tuning the size of the <span class="hlt">air</span> cavities to cover the whole visible spectrum. When the <span class="hlt">air</span> cavities are filled with a solvent which has the same refractive index as that of the polymer, the macroporous polymer films become completely transparent due to the index matching. When the solvent trapped in the cavities is evaporated by in-situ heating, the sample color changes back to brilliant color. This process is highly reversible and reproducible for thousands of cycles. The second topic reports the achievement of rapid and reversible vapor detection by using 3-D macroporous photonic crystals. Capillary condensation of a condensable vapor in the interconnected macropores leads to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..MAR.A4009S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..MAR.A4009S"><span>Topological Properties of Some Integrated Circuits for Very <span class="hlt">Large</span> <span class="hlt">Scale</span> Integration Chip Designs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Swanson, S.; Lanzerotti, M.; Vernizzi, G.; Kujawski, J.; Weatherwax, A.</p> <p>2015-03-01</p> <p>This talk presents topological properties of integrated circuits for Very <span class="hlt">Large</span> <span class="hlt">Scale</span> Integration chip designs. These circuits can be implemented in very <span class="hlt">large</span> <span class="hlt">scale</span> integrated circuits, such as those in high performance microprocessors. Prior work considered basic combinational logic functions and produced a mathematical framework based on algebraic topology for integrated circuits composed of logic gates. Prior work also produced an historically-equivalent interpretation of Mr. E. F. Rent's work for today's complex circuitry in modern high performance microprocessors, where a heuristic linear relationship was observed between the number of connections and number of logic gates. This talk will examine topological properties and connectivity of more complex functionally-equivalent integrated circuits. The views expressed in this article are those of the author and do not reflect the official policy or position of the United States <span class="hlt">Air</span> Force, Department of Defense or the U.S. Government.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=scale&pg=3&id=EJ1025453','ERIC'); return false;" href="https://eric.ed.gov/?q=scale&pg=3&id=EJ1025453"><span>Toward Increasing Fairness in Score <span class="hlt">Scale</span> Calibrations Employed in International <span class="hlt">Large-Scale</span> Assessments</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>Oliveri, Maria Elena; von Davier, Matthias</p> <p>2014-01-01</p> <p>In this article, we investigate the creation of comparable score <span class="hlt">scales</span> across countries in international assessments. We examine potential improvements to current score <span class="hlt">scale</span> calibration procedures used in international <span class="hlt">large-scale</span> assessments. Our approach seeks to improve fairness in scoring international <span class="hlt">large-scale</span> assessments, which often…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19330099','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19330099"><span><span class="hlt">Large-scale</span> models <span class="hlt">reveal</span> the two-component mechanics of striated muscle.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jarosch, Robert</p> <p>2008-12-01</p> <p>This paper provides a comprehensive explanation of striated muscle mechanics and contraction on the basis of filament rotations. Helical proteins, particularly the coiled-coils of tropomyosin, myosin and alpha-actinin, shorten their H-bonds cooperatively and produce torque and filament rotations when the Coulombic net-charge repulsion of their highly charged side-chains is diminished by interaction with ions. The classical "two-component model" of active muscle differentiated a "contractile component" which stretches the "series elastic component" during force production. The contractile components are the helically shaped thin filaments of muscle that shorten the sarcomeres by clockwise drilling into the myosin cross-bridges with torque decrease (= force-deficit). Muscle stretch means drawing out the thin filament helices off the cross-bridges under passive counterclockwise rotation with torque increase (= stretch activation). Since each thin filament is anchored by four elastic alpha-actinin Z-filaments (provided with force-regulating sites for Ca(2+) binding), the thin filament rotations change the torsional twist of the four Z-filaments as the "series elastic components". <span class="hlt">Large</span> <span class="hlt">scale</span> models simulate the changes of structure and force in the Z-band by the different Z-filament twisting stages A, B, C, D, E, F and G. Stage D corresponds to the isometric state. The basic phenomena of muscle physiology, i. e. latency relaxation, Fenn-effect, the force-velocity relation, the length-tension relation, unexplained energy, shortening heat, the Huxley-Simmons phases, etc. are explained and interpreted with the help of the model experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..4412218Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..4412218Y"><span>High-Frequency Observations of Temperature and Dissolved Oxygen <span class="hlt">Reveal</span> Under-Ice Convection in a <span class="hlt">Large</span> Lake</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Bernard; Young, Joelle; Brown, Laura; Wells, Mathew</p> <p>2017-12-01</p> <p>Detailed observations of thermal structure over an entire winter in a <span class="hlt">large</span> lake <span class="hlt">reveal</span> the presence of <span class="hlt">large</span> (10-20 m) overturns under the ice, driven by diurnal solar heating. Convection can occur in the early winter, but the most vigorous convection occurred near the end of winter. Both periods are when our lake ice model suggest thinner ice that would have been transparent. This under-ice convection led to a deepening of the mixed layer over time, consistent with previous short-term studies. During periods of vigorous convection under the ice at the end of winter, the dissolved oxygen had become supersaturated from the surface to 23 m below the surface, suggesting abundant algal growth. Analysis of our high-frequency observations over the entire winter of 2015 using the Thorpe-<span class="hlt">scale</span> method quantified the <span class="hlt">scale</span> of mixing. Furthermore, it <span class="hlt">revealed</span> that changes in oxygen concentrations are closely related to the intensity of mixing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=electric+AND+machines&pg=6&id=ED265841','ERIC'); return false;" href="https://eric.ed.gov/?q=electric+AND+machines&pg=6&id=ED265841"><span>Very <span class="hlt">Large</span> <span class="hlt">Scale</span> Integration (VLSI).</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>Yeaman, Andrew R. J.</p> <p></p> <p>Very <span class="hlt">Large</span> <span class="hlt">Scale</span> Integration (VLSI), the state-of-the-art production techniques for computer chips, promises such powerful, inexpensive computing that, in the future, people will be able to communicate with computer devices in natural language or even speech. However, before full-<span class="hlt">scale</span> VLSI implementation can occur, certain salient factors must be…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3893195','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3893195"><span>Inverse Association between <span class="hlt">Air</span> Pressure and Rheumatoid Arthritis Synovitis</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Furu, Moritoshi; Nakabo, Shuichiro; Ohmura, Koichiro; Nakashima, Ran; Imura, Yoshitaka; Yukawa, Naoichiro; Yoshifuji, Hajime; Matsuda, Fumihiko; Ito, Hiromu; Fujii, Takao; Mimori, Tsuneyo</p> <p>2014-01-01</p> <p>Rheumatoid arthritis (RA) is a bone destructive autoimmune disease. Many patients with RA recognize fluctuations of their joint synovitis according to changes of <span class="hlt">air</span> pressure, but the correlations between them have never been addressed in <span class="hlt">large-scale</span> association studies. To address this point we recruited <span class="hlt">large-scale</span> assessments of RA activity in a Japanese population, and performed an association analysis. Here, a total of 23,064 assessments of RA activity from 2,131 patients were obtained from the KURAMA (Kyoto University Rheumatoid Arthritis Management Alliance) database. Detailed correlations between <span class="hlt">air</span> pressure and joint swelling or tenderness were analyzed separately for each of the 326 patients with more than 20 assessments to regulate intra-patient correlations. Association studies were also performed for seven consecutive days to identify the strongest correlations. Standardized multiple linear regression analysis was performed to evaluate independent influences from other meteorological factors. As a result, components of composite measures for RA disease activity <span class="hlt">revealed</span> suggestive negative associations with <span class="hlt">air</span> pressure. The 326 patients displayed significant negative mean correlations between <span class="hlt">air</span> pressure and swellings or the sum of swellings and tenderness (p = 0.00068 and 0.00011, respectively). Among the seven consecutive days, the most significant mean negative correlations were observed for <span class="hlt">air</span> pressure three days before evaluations of RA synovitis (p = 1.7×10−7, 0.00027, and 8.3×10−8, for swellings, tenderness and the sum of them, respectively). Standardized multiple linear regression analysis <span class="hlt">revealed</span> these associations were independent from humidity and temperature. Our findings suggest that <span class="hlt">air</span> pressure is inversely associated with synovitis in patients with RA. PMID:24454853</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1213747B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1213747B"><span>Methodology for <span class="hlt">Air</span> Quality Forecast Downscaling from Regional- to Street-<span class="hlt">Scale</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baklanov, Alexander; Nuterman, Roman; Mahura, Alexander; Amstrup, Bjarne; Hansen Saas, Bent; Havskov Sørensen, Jens; Lorenzen, Thomas; Weismann, Jakob</p> <p>2010-05-01</p> <p>The most serious <span class="hlt">air</span> pollution events occur in cities where there is a combination of high population density and <span class="hlt">air</span> pollution, e.g. from vehicles. The pollutants can lead to serious human health problems, including asthma, irritation of the lungs, bronchitis, pneumonia, decreased resistance to respiratory infections, and premature death. In particular <span class="hlt">air</span> pollution is associated with increase in cardiovascular disease and lung cancer. In 2000 WHO estimated that between 2.5 % and 11 % of total annual deaths are caused by exposure to <span class="hlt">air</span> pollution. However, European-<span class="hlt">scale</span> <span class="hlt">air</span> quality models are not suited for local forecasts, as their grid-cell is typically of the order of 5 to 10km and they generally lack detailed representation of urban effects. Two suites are used in the framework of the EC FP7 project MACC (Monitoring of Atmosphere Composition and Climate) to demonstrate how downscaling from the European MACC ensemble to local-<span class="hlt">scale</span> <span class="hlt">air</span> quality forecast will be carried out: one will illustrate capabilities for the city of Copenhagen (Denmark); the second will focus on the city of Bucharest (Romania). This work is devoted to the first suite, where methodological aspects of downscaling from regional (European/ Denmark) to urban <span class="hlt">scale</span> (Copenhagen), and from the urban down to street <span class="hlt">scale</span>. The first results of downscaling according to the proposed methodology are presented. The potential for downscaling of European <span class="hlt">air</span> quality forecasts by operating urban and street-level forecast models is evaluated. This will bring a strong support for continuous improvement of the regional forecast modelling systems for <span class="hlt">air</span> quality in Europe, and underline clear perspectives for the future regional <span class="hlt">air</span> quality core and downstream services for end-users. At the end of the MACC project, requirements on "how-to-do" downscaling of European <span class="hlt">air</span>-quality forecasts to the city and street levels with different approaches will be formulated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2382T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2382T"><span>Impact of <span class="hlt">air</span>-sea drag coefficient for latent heat flux on <span class="hlt">large</span> <span class="hlt">scale</span> climate in coupled and atmosphere stand-alone simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torres, Olivier; Braconnot, Pascale; Marti, Olivier; Gential, Luc</p> <p>2018-05-01</p> <p>The turbulent fluxes across the ocean/atmosphere interface represent one of the principal driving forces of the global atmospheric and oceanic circulation. Despite decades of effort and improvements, representation of these fluxes still presents a challenge due to the small-<span class="hlt">scale</span> acting turbulent processes compared to the resolved <span class="hlt">scales</span> of the models. Beyond this subgrid parameterization issue, a comprehensive understanding of the impact of <span class="hlt">air</span>-sea interactions on the climate system is still lacking. In this paper we investigates the <span class="hlt">large-scale</span> impacts of the transfer coefficient used to compute turbulent heat fluxes with the IPSL-CM4 climate model in which the surface bulk formula is modified. Analyzing both atmosphere and coupled ocean-atmosphere general circulation model (AGCM, OAGCM) simulations allows us to study the direct effect and the mechanisms of adjustment to this modification. We focus on the representation of latent heat flux in the tropics. We show that the heat transfer coefficients are highly similar for a given parameterization between AGCM and OAGCM simulations. Although the same areas are impacted in both kind of simulations, the differences in surface heat fluxes are substantial. A regional modification of heat transfer coefficient has more impact than uniform modification in AGCM simulations while in OAGCM simulations, the opposite is observed. By studying the global energetics and the atmospheric circulation response to the modification, we highlight the role of the ocean in dampening a <span class="hlt">large</span> part of the disturbance. Modification of the heat exchange coefficient modifies the way the coupled system works due to the link between atmospheric circulation and SST, and the different feedbacks between ocean and atmosphere. The adjustment that takes place implies a balance of net incoming solar radiation that is the same in all simulations. As there is no change in model physics other than drag coefficient, we obtain similar latent heat flux</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160000353','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160000353"><span><span class="hlt">Air</span> Mass Origin in the Arctic and its Response to Future Warming</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Orbe, Clara; Newman, Paul A.; Waugh, Darryn W.; Holzer, Mark; Oman, Luke; Polvani, Lorenzo M.; Li, Feng</p> <p>2014-01-01</p> <p>We present the first climatology of <span class="hlt">air</span> mass origin in the Arctic in terms of rigorously defined <span class="hlt">air</span> mass fractions that partition <span class="hlt">air</span> according to where it last contacted the planetary boundary layer (PBL). Results from a present-day climate integration of the GEOSCCM general circulation model <span class="hlt">reveal</span> that the Arctic lower troposphere below 700 mb is dominated year round by <span class="hlt">air</span> whose last PBL contact occurred poleward of 60degN, (Arctic <span class="hlt">air</span>, or <span class="hlt">air</span> of Arctic origin). By comparison, approx. 63% of the Arctic troposphere above 700 mb originates in the NH midlatitude PBL, (midlatitude <span class="hlt">air</span>). Although seasonal changes in the total fraction of midlatitude <span class="hlt">air</span> are small, there are dramatic changes in where that <span class="hlt">air</span> last contacted the PBL, especially above 700 mb. Specifically, during winter <span class="hlt">air</span> in the Arctic originates preferentially over the oceans, approx. 26% in the East Pacific, and approx. 20% in the Atlantic PBL. By comparison, during summer <span class="hlt">air</span> in the Arctic last contacted the midlatitude PBL primarily over land, overwhelmingly so in Asia (approx. 40 %) and, to a lesser extent, in North America (approx. 24%). Seasonal changes in <span class="hlt">air</span>-mass origin are interpreted in terms of seasonal variations in the <span class="hlt">large-scale</span> ventilation of the midlatitude boundary layer and lower troposphere, namely changes in the midlatitude tropospheric jet and associated transient eddies during winter and <span class="hlt">large</span> <span class="hlt">scale</span> convective motions over midlatitudes during summer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880003992','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880003992"><span>Survey on <span class="hlt">large</span> <span class="hlt">scale</span> system control methods</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mercadal, Mathieu</p> <p>1987-01-01</p> <p>The problem inherent to <span class="hlt">large</span> <span class="hlt">scale</span> systems such as power network, communication network and economic or ecological systems were studied. The increase in size and flexibility of future spacecraft has put those dynamical systems into the category of <span class="hlt">large</span> <span class="hlt">scale</span> systems, and tools specific to the class of <span class="hlt">large</span> systems are being sought to design control systems that can guarantee more stability and better performance. Among several survey papers, reference was found to a thorough investigation on decentralized control methods. Especially helpful was the classification made of the different existing approaches to deal with <span class="hlt">large</span> <span class="hlt">scale</span> systems. A very similar classification is used, even though the papers surveyed are somehow different from the ones reviewed in other papers. Special attention is brought to the applicability of the existing methods to controlling <span class="hlt">large</span> mechanical systems like <span class="hlt">large</span> space structures. Some recent developments are added to this survey.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10374E..0BK','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10374E..0BK"><span>A fiber-optic ice detection system for <span class="hlt">large-scale</span> wind turbine blades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Dae-gil; Sampath, Umesh; Kim, Hyunjin; Song, Minho</p> <p>2017-09-01</p> <p>Icing causes substantial problems in the integrity of <span class="hlt">large-scale</span> wind turbines. In this work, a fiber-optic sensor system for detection of icing with an arrayed waveguide grating is presented. The sensor system detects Fresnel reflections from the ends of the fibers. The transition in Fresnel reflection due to icing gives peculiar intensity variations, which categorizes the ice, the water, and the <span class="hlt">air</span> medium on the wind turbine blades. From the experimental results, with the proposed sensor system, the formation of icing conditions and thickness of ice were identified successfully in real time.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..324a2088J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..324a2088J"><span><span class="hlt">Large-Scale</span> 3D Printing: The Way Forward</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jassmi, Hamad Al; Najjar, Fady Al; Ismail Mourad, Abdel-Hamid</p> <p>2018-03-01</p> <p>Research on small-<span class="hlt">scale</span> 3D printing has rapidly evolved, where numerous industrial products have been tested and successfully applied. Nonetheless, research on <span class="hlt">large-scale</span> 3D printing, directed to <span class="hlt">large-scale</span> applications such as construction and automotive manufacturing, yet demands a great a great deal of efforts. <span class="hlt">Large-scale</span> 3D printing is considered an interdisciplinary topic and requires establishing a blended knowledge base from numerous research fields including structural engineering, materials science, mechatronics, software engineering, artificial intelligence and architectural engineering. This review article summarizes key topics of relevance to new research trends on <span class="hlt">large-scale</span> 3D printing, particularly pertaining (1) technological solutions of additive construction (i.e. the 3D printers themselves), (2) materials science challenges, and (3) new design opportunities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22356256','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22356256"><span>Novel method to construct <span class="hlt">large-scale</span> design space in lubrication process utilizing Bayesian estimation based on a small-<span class="hlt">scale</span> design-of-experiment and small sets of <span class="hlt">large-scale</span> manufacturing data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Maeda, Jin; Suzuki, Tatsuya; Takayama, Kozo</p> <p>2012-12-01</p> <p>A <span class="hlt">large-scale</span> design space was constructed using a Bayesian estimation method with a small-<span class="hlt">scale</span> design of experiments (DoE) and small sets of <span class="hlt">large-scale</span> manufacturing data without enforcing a <span class="hlt">large-scale</span> DoE. The small-<span class="hlt">scale</span> DoE was conducted using various Froude numbers (X(1)) and blending times (X(2)) in the lubricant blending process for theophylline tablets. The response surfaces, design space, and their reliability of the compression rate of the powder mixture (Y(1)), tablet hardness (Y(2)), and dissolution rate (Y(3)) on a small <span class="hlt">scale</span> were calculated using multivariate spline interpolation, a bootstrap resampling technique, and self-organizing map clustering. The constant Froude number was applied as a <span class="hlt">scale</span>-up rule. Three experiments under an optimal condition and two experiments under other conditions were performed on a <span class="hlt">large</span> <span class="hlt">scale</span>. The response surfaces on the small <span class="hlt">scale</span> were corrected to those on a <span class="hlt">large</span> <span class="hlt">scale</span> by Bayesian estimation using the <span class="hlt">large-scale</span> results. <span class="hlt">Large-scale</span> experiments under three additional sets of conditions showed that the corrected design space was more reliable than that on the small <span class="hlt">scale</span>, even if there was some discrepancy in the pharmaceutical quality between the manufacturing <span class="hlt">scales</span>. This approach is useful for setting up a design space in pharmaceutical development when a DoE cannot be performed at a commercial <span class="hlt">large</span> manufacturing <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27382163','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27382163"><span><span class="hlt">Large</span> <span class="hlt">scale</span>, synchronous variability of marine fish populations driven by commercial exploitation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Frank, Kenneth T; Petrie, Brian; Leggett, William C; Boyce, Daniel G</p> <p>2016-07-19</p> <p>Synchronous variations in the abundance of geographically distinct marine fish populations are known to occur across spatial <span class="hlt">scales</span> on the order of 1,000 km and greater. The prevailing assumption is that this <span class="hlt">large-scale</span> coherent variability is a response to coupled atmosphere-ocean dynamics, commonly represented by climate indexes, such as the Atlantic Multidecadal Oscillation and North Atlantic Oscillation. On the other hand, it has been suggested that exploitation might contribute to this coherent variability. This possibility has been generally ignored or dismissed on the grounds that exploitation is unlikely to operate synchronously at such <span class="hlt">large</span> spatial <span class="hlt">scales</span>. Our analysis of adult fishing mortality and spawning stock biomass of 22 North Atlantic cod (Gadus morhua) stocks <span class="hlt">revealed</span> that both the temporal and spatial <span class="hlt">scales</span> in fishing mortality and spawning stock biomass were equivalent to those of the climate drivers. From these results, we conclude that greater consideration must be given to the potential of exploitation as a driving force behind broad, coherent variability of heavily exploited fish species.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/grants/community-scale-air-toxics-ambient-monitoring-grant-closed-announcement-fy-2015','PESTICIDES'); return false;" href="https://www.epa.gov/grants/community-scale-air-toxics-ambient-monitoring-grant-closed-announcement-fy-2015"><span>Community-<span class="hlt">Scale</span> <span class="hlt">Air</span> Toxics Ambient Monitoring Grant - Closed Announcement FY 2015</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>Grant to fund projects designed to assist state, local and tribal communities in identifying <span class="hlt">air</span> toxics sources, characterizing the degree and extent of local-<span class="hlt">scale</span> <span class="hlt">air</span> toxics problems, tracking progress of <span class="hlt">air</span> toxics reduction activities, etc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..245b2046M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..245b2046M"><span>Resistance to Internal Damage and <span class="hlt">Scaling</span> of Concrete <span class="hlt">Air</span> Entrained By Microspheres</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Molendowska, Agnieszka; Wawrzenczyk, Jerzy</p> <p>2017-10-01</p> <p>This paper report the test results of high strength concrete produced with slag cement and <span class="hlt">air</span> entrained with polymer microspheres in three diameters. The study focused on determining the effects of the microsphere size and quantity on the <span class="hlt">air</span> void structure and resistance to internal cracking and <span class="hlt">scaling</span> of the concrete. The resistance to internal cracking was determined in compliance with the requirements of the modified ASTM C666 A method on beam specimens. The <span class="hlt">scaling</span> resistance in a 3% NaCl solution was determined using the slab test in accordance with PKN-CEN/TS 12390-9:2007. The <span class="hlt">air</span> void structure parameters were determined to PN-EN 480-11:1998. The study results indicate that the use of microspheres is an effective <span class="hlt">air</span> entrainment method providing very good <span class="hlt">air</span> void structure parameters. The results show high freeze-thaw durability of polymer microsphere-based concrete in exposure class XF3. The <span class="hlt">scaling</span> resistance test confirms that it is substantially more difficult to protect concrete against <span class="hlt">scaling</span> in the presence of the 3% NaCl solution (exposure class XF4). Concrete <span class="hlt">scaling</span> is a complex phenomenon controlled by a number of independent factors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4383548','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4383548"><span>Bio-Inspired Wooden Actuators for <span class="hlt">Large</span> <span class="hlt">Scale</span> Applications</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Rüggeberg, Markus; Burgert, Ingo</p> <p>2015-01-01</p> <p>Implementing programmable actuation into materials and structures is a major topic in the field of smart materials. In particular the bilayer principle has been employed to develop actuators that respond to various kinds of stimuli. A multitude of small <span class="hlt">scale</span> applications down to micrometer size have been developed, but up-<span class="hlt">scaling</span> remains challenging due to either limitations in mechanical stiffness of the material or in the manufacturing processes. Here, we demonstrate the actuation of wooden bilayers in response to changes in relative humidity, making use of the high material stiffness and a good machinability to reach <span class="hlt">large</span> <span class="hlt">scale</span> actuation and application. Amplitude and response time of the actuation were measured and can be predicted and controlled by adapting the geometry and the constitution of the bilayers. Field tests in full weathering conditions <span class="hlt">revealed</span> long-term stability of the actuation. The potential of the concept is shown by a first demonstrator. With the sensor and actuator intrinsically incorporated in the wooden bilayers, the daily change in relative humidity is exploited for an autonomous and solar powered movement of a tracker for solar modules. PMID:25835386</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2635638','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2635638"><span><span class="hlt">Large-scale</span> Models <span class="hlt">Reveal</span> the Two-component Mechanics of Striated Muscle</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jarosch, Robert</p> <p>2008-01-01</p> <p>This paper provides a comprehensive explanation of striated muscle mechanics and contraction on the basis of filament rotations. Helical proteins, particularly the coiled-coils of tropomyosin, myosin and α-actinin, shorten their H-bonds cooperatively and produce torque and filament rotations when the Coulombic net-charge repulsion of their highly charged side-chains is diminished by interaction with ions. The classical “two-component model” of active muscle differentiated a “contractile component” which stretches the “series elastic component” during force production. The contractile components are the helically shaped thin filaments of muscle that shorten the sarcomeres by clockwise drilling into the myosin cross-bridges with torque decrease (= force-deficit). Muscle stretch means drawing out the thin filament helices off the cross-bridges under passive counterclockwise rotation with torque increase (= stretch activation). Since each thin filament is anchored by four elastic α-actinin Z-filaments (provided with force-regulating sites for Ca2+ binding), the thin filament rotations change the torsional twist of the four Z-filaments as the “series elastic components”. <span class="hlt">Large</span> <span class="hlt">scale</span> models simulate the changes of structure and force in the Z-band by the different Z-filament twisting stages A, B, C, D, E, F and G. Stage D corresponds to the isometric state. The basic phenomena of muscle physiology, i. e. latency relaxation, Fenn-effect, the force-velocity relation, the length-tension relation, unexplained energy, shortening heat, the Huxley-Simmons phases, etc. are explained and interpreted with the help of the model experiments. PMID:19330099</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..15.4309M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..15.4309M"><span>The influence of Seychelles Dome on the <span class="hlt">large</span> <span class="hlt">scale</span> Tropical Variability</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Manola, Iris; Selten, Frank; Hazeleger, Wilco</p> <p>2013-04-01</p> <p>The Seychelles Dome (SD) is the thermocline ridge just South of the equator in the Western Indian Ocean basin. It is characterized by strong atmospheric convection and a shallow thermocline and is associated with <span class="hlt">large</span> intraseasonal convection and SST variability (Harrison and Vecchi 2001). The SD is influenced by surface and subsurface processes, such as <span class="hlt">air</span>-sea fluxes, Ekman upwelling from wind stress curl, ocean dynamics (vertical mixing) and oceanic Rossby waves from southeastern Indian Ocean. The favoring season for a strong SD is the boreal winter, where the thermocline is most shallow. Then the southeasterly trade winds converge with the northwesterly monsoonal winds over the intertropical convergence zone and cause cyclonic wind stress curl that drives Ekman divergence and a ridging of the thermocline. It is found that the subseasonal and interranual variability of the SD is influenced by <span class="hlt">large</span> <span class="hlt">scale</span> events, such as the Indian Ocean Dipole (IOD), the ENSO and the Madden-Julian Oscillation (MJO) (Tozuka et al., 2010, Lloyd and Vecchi, 2010). The SD is enhanced by cooling events in the Western Indian Ocean and easterly winds that raise the thermocline and increase the upwelling. This can be associated with a strong Walker circulation, like negative IOD conditions or La Nina-like conditions. So far the studies focus on the origins of the SD variability, but the influence of the SD itself on regional or <span class="hlt">large</span> <span class="hlt">scale</span> climate is <span class="hlt">largely</span> unknown. In this study we focus on the influence of the SD variations on the <span class="hlt">large</span> <span class="hlt">scale</span> tropical circulation. We analyze the covariance of the SD variations and the tropical circulation in a 200 year control imulation of the climate model EC-EARTH and perform idealized SST forced simulations to study the character of the atmospheric response and its relation to ENSO, IOD and MJO. References -Harrison, D. E. and G. A. Vecchi, 2001: January 1999 Indian Ocean cooling event. Geophys. Res. Lett., 28, 3717-3720. -Lloyd, I. D., and G. A</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PDU....13...30B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PDU....13...30B"><span>A relativistic signature in <span class="hlt">large-scale</span> structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bartolo, Nicola; Bertacca, Daniele; Bruni, Marco; Koyama, Kazuya; Maartens, Roy; Matarrese, Sabino; Sasaki, Misao; Verde, Licia; Wands, David</p> <p>2016-09-01</p> <p>In General Relativity, the constraint equation relating metric and density perturbations is inherently nonlinear, leading to an effective non-Gaussianity in the dark matter density field on <span class="hlt">large</span> <span class="hlt">scales</span>-even if the primordial metric perturbation is Gaussian. Intrinsic non-Gaussianity in the <span class="hlt">large-scale</span> dark matter overdensity in GR is real and physical. However, the variance smoothed on a local physical <span class="hlt">scale</span> is not correlated with the <span class="hlt">large-scale</span> curvature perturbation, so that there is no relativistic signature in the galaxy bias when using the simplest model of bias. It is an open question whether the observable mass proxies such as luminosity or weak lensing correspond directly to the physical mass in the simple halo bias model. If not, there may be observables that encode this relativistic signature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040087488&hterms=functions+proteins&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfunctions%2Bproteins','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040087488&hterms=functions+proteins&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dfunctions%2Bproteins"><span>Predicting protein functions from redundancies in <span class="hlt">large-scale</span> protein interaction networks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Samanta, Manoj Pratim; Liang, Shoudan</p> <p>2003-01-01</p> <p>Interpreting data from <span class="hlt">large-scale</span> protein interaction experiments has been a challenging task because of the widespread presence of random false positives. Here, we present a network-based statistical algorithm that overcomes this difficulty and allows us to derive functions of unannotated proteins from <span class="hlt">large-scale</span> interaction data. Our algorithm uses the insight that if two proteins share significantly larger number of common interaction partners than random, they have close functional associations. Analysis of publicly available data from Saccharomyces cerevisiae <span class="hlt">reveals</span> >2,800 reliable functional associations, 29% of which involve at least one unannotated protein. By further analyzing these associations, we derive tentative functions for 81 unannotated proteins with high certainty. Our method is not overly sensitive to the false positives present in the data. Even after adding 50% randomly generated interactions to the measured data set, we are able to recover almost all (approximately 89%) of the original associations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=148683&keyword=TENS&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=148683&keyword=TENS&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>RESOLVING NEIGHBORHOOD-<span class="hlt">SCALE</span> <span class="hlt">AIR</span> TOXICS MODELING: A CASE STUDY IN WILMINGTON, CALIFORNIA</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p><span class="hlt">Air</span> quality modeling is useful for characterizing exposures to <span class="hlt">air</span> pollutants. While models typically provide results on regional <span class="hlt">scales</span>, there is a need for refined modeling approaches capable of resolving concentrations on the <span class="hlt">scale</span> of tens of meters, across modeling domains 1...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=88218&Lab=NERL&keyword=dependency&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=88218&Lab=NERL&keyword=dependency&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>CMAQ MODELING FOR <span class="hlt">AIR</span> TOXICS AT FINE <span class="hlt">SCALES</span>: A PROTOTYPE STUDY</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>Toxic <span class="hlt">air</span> pollutants (TAPs) or hazardous <span class="hlt">air</span> pollutants (HAPs) exhibit considerable spatial and temporal variability across urban areas. Therefore, the ability of chemical transport models (CTMs), e.g. Community Multi-<span class="hlt">scale</span> <span class="hlt">Air</span> Quality (CMAQ), to reproduce the spatial and tempor...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790054108&hterms=sound+amplitude&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsound%2Bamplitude','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790054108&hterms=sound+amplitude&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dsound%2Bamplitude"><span>Sound production due to <span class="hlt">large-scale</span> coherent structures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gatski, T. B.</p> <p>1979-01-01</p> <p>The acoustic pressure fluctuations due to <span class="hlt">large-scale</span> finite amplitude disturbances in a free turbulent shear flow are calculated. The flow is decomposed into three component <span class="hlt">scales</span>; the mean motion, the <span class="hlt">large-scale</span> wave-like disturbance, and the small-<span class="hlt">scale</span> random turbulence. The effect of the <span class="hlt">large-scale</span> structure on the flow is isolated by applying both a spatial and phase average on the governing differential equations and by initially taking the small-<span class="hlt">scale</span> turbulence to be in energetic equilibrium with the mean flow. The subsequent temporal evolution of the flow is computed from global energetic rate equations for the different component <span class="hlt">scales</span>. Lighthill's theory is then applied to the region with the flowfield as the source and an observer located outside the flowfield in a region of uniform velocity. Since the time history of all flow variables is known, a minimum of simplifying assumptions for the Lighthill stress tensor is required, including no far-field approximations. A phase average is used to isolate the pressure fluctuations due to the <span class="hlt">large-scale</span> structure, and also to isolate the dynamic process responsible. Variation of mean square pressure with distance from the source is computed to determine the acoustic far-field location and decay rate, and, in addition, spectra at various acoustic field locations are computed and analyzed. Also included are the effects of varying the growth and decay of the <span class="hlt">large-scale</span> disturbance on the sound produced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28157285','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28157285"><span>Boreal Forests Sequester <span class="hlt">Large</span> Amounts of Mercury over Millennial Time <span class="hlt">Scales</span> in the Absence of Wildfire.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Giesler, Reiner; Clemmensen, Karina E; Wardle, David A; Klaminder, Jonatan; Bindler, Richard</p> <p>2017-03-07</p> <p>Alterations in fire activity due to climate change and fire suppression may have profound effects on the balance between storage and release of carbon (C) and associated volatile elements. Stored soil mercury (Hg) is known to volatilize due to wildfires and this could substantially affect the land-<span class="hlt">air</span> exchange of Hg; conversely the absence of fires and human disturbance may increase the time period over which Hg is sequestered. Here we show for a wildfire chronosequence spanning over more than 5000 years in boreal forest in northern Sweden that belowground inventories of total Hg are strongly related to soil humus C accumulation (R 2 = 0.94, p < 0.001). Our data clearly show that northern boreal forest soils have a strong sink capacity for Hg, and indicate that the sequestered Hg is bound in soil organic matter pools accumulating over millennia. Our results also suggest that more than half of the Hg stock in the sites with the longest time since fire originates from deposition predating the onset of <span class="hlt">large-scale</span> anthropogenic emissions. This study emphasizes the importance of boreal forest humus soils for Hg storage and <span class="hlt">reveals</span> that this pool is likely to persist over millennial time <span class="hlt">scales</span> in the prolonged absence of fire.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=galvanizing&id=EJ910751','ERIC'); return false;" href="https://eric.ed.gov/?q=galvanizing&id=EJ910751"><span>The Challenge of <span class="hlt">Large-Scale</span> Literacy Improvement</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>Levin, Ben</p> <p>2010-01-01</p> <p>This paper discusses the challenge of making <span class="hlt">large-scale</span> improvements in literacy in schools across an entire education system. Despite growing interest and rhetoric, there are very few examples of sustained, <span class="hlt">large-scale</span> change efforts around school-age literacy. The paper reviews 2 instances of such efforts, in England and Ontario. After…</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('https://www.ncbi.nlm.nih.gov/pubmed/17244584','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17244584"><span><span class="hlt">Large-scale</span> influences in near-wall turbulence.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hutchins, Nicholas; Marusic, Ivan</p> <p>2007-03-15</p> <p>Hot-wire data acquired in a high Reynolds number facility are used to illustrate the need for adequate <span class="hlt">scale</span> separation when considering the coherent structure in wall-bounded turbulence. It is found that a <span class="hlt">large-scale</span> motion in the log region becomes increasingly comparable in energy to the near-wall cycle as the Reynolds number increases. Through decomposition of fluctuating velocity signals, it is shown that this <span class="hlt">large-scale</span> motion has a distinct modulating influence on the small-<span class="hlt">scale</span> energy (akin to amplitude modulation). Reassessment of DNS data, in light of these results, shows similar trends, with the rate and intensity of production due to the near-wall cycle subject to a modulating influence from the largest-<span class="hlt">scale</span> motions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DPPN12126S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DPPN12126S"><span>Generation of <span class="hlt">large-scale</span> magnetic fields by small-<span class="hlt">scale</span> dynamo in shear flows</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Squire, Jonathan; Bhattacharjee, Amitava</p> <p>2015-11-01</p> <p>A new mechanism for turbulent mean-field dynamo is proposed, in which the magnetic fluctuations resulting from a small-<span class="hlt">scale</span> dynamo drive the generation of <span class="hlt">large-scale</span> magnetic fields. This is in stark contrast to the common idea that small-<span class="hlt">scale</span> magnetic fields should be harmful to <span class="hlt">large-scale</span> dynamo action. These dynamos occur in the presence of <span class="hlt">large-scale</span> velocity shear and do not require net helicity, resulting from off-diagonal components of the turbulent resistivity tensor as the magnetic analogue of the ``shear-current'' effect. The dynamo is studied using a variety of computational and analytic techniques, both when the magnetic fluctuations arise self-consistently through the small-<span class="hlt">scale</span> dynamo and in lower Reynolds number regimes. Given the inevitable existence of non-helical small-<span class="hlt">scale</span> magnetic fields in turbulent plasmas, as well as the generic nature of velocity shear, the suggested mechanism may help to explain generation of <span class="hlt">large-scale</span> magnetic fields across a wide range of astrophysical objects. This work was supported by a Procter Fellowship at Princeton University, and the US Department of Energy Grant DE-AC02-09-CH11466.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2650504','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2650504"><span><span class="hlt">Large-scale</span> impacts of herbivores on the structural diversity of African savannas</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Asner, Gregory P.; Levick, Shaun R.; Kennedy-Bowdoin, Ty; Knapp, David E.; Emerson, Ruth; Jacobson, James; Colgan, Matthew S.; Martin, Roberta E.</p> <p>2009-01-01</p> <p>African savannas are undergoing management intensification, and decision makers are increasingly challenged to balance the needs of <span class="hlt">large</span> herbivore populations with the maintenance of vegetation and ecosystem diversity. Ensuring the sustainability of Africa's natural protected areas requires information on the efficacy of management decisions at <span class="hlt">large</span> spatial <span class="hlt">scales</span>, but often neither experimental treatments nor <span class="hlt">large-scale</span> responses are available for analysis. Using a new airborne remote sensing system, we mapped the three-dimensional (3-D) structure of vegetation at a spatial resolution of 56 cm throughout 1640 ha of savanna after 6-, 22-, 35-, and 41-year exclusions of herbivores, as well as in unprotected areas, across Kruger National Park in South Africa. Areas in which herbivores were excluded over the short term (6 years) contained 38%–80% less bare ground compared with those that were exposed to mammalian herbivory. In the longer-term (> 22 years), the 3-D structure of woody vegetation differed significantly between protected and accessible landscapes, with up to 11-fold greater woody canopy cover in the areas without herbivores. Our maps <span class="hlt">revealed</span> 2 <span class="hlt">scales</span> of ecosystem response to herbivore consumption, one broadly mediated by geologic substrate and the other mediated by hillslope-<span class="hlt">scale</span> variation in soil nutrient availability and moisture conditions. Our results are the first to quantitatively illustrate the extent to which herbivores can affect the 3-D structural diversity of vegetation across <span class="hlt">large</span> savanna landscapes. PMID:19258457</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24960397','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24960397"><span>Natural snowfall <span class="hlt">reveals</span> <span class="hlt">large-scale</span> flow structures in the wake of a 2.5-MW wind turbine.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hong, Jiarong; Toloui, Mostafa; Chamorro, Leonardo P; Guala, Michele; Howard, Kevin; Riley, Sean; Tucker, James; Sotiropoulos, Fotis</p> <p>2014-06-24</p> <p>To improve power production and structural reliability of wind turbines, there is a pressing need to understand how turbines interact with the atmospheric boundary layer. However, experimental techniques capable of quantifying or even qualitatively visualizing the <span class="hlt">large-scale</span> turbulent flow structures around full-<span class="hlt">scale</span> turbines do not exist today. Here we use snowflakes from a winter snowstorm as flow tracers to obtain velocity fields downwind of a 2.5-MW wind turbine in a sampling area of ~36 × 36 m(2). The spatial and temporal resolutions of the measurements are sufficiently high to quantify the evolution of blade-generated coherent motions, such as the tip and trailing sheet vortices, identify their instability mechanisms and correlate them with turbine operation, control and performance. Our experiment provides an unprecedented in situ characterization of flow structures around utility-<span class="hlt">scale</span> turbines, and yields significant insights into the Reynolds number similarity issues presented in wind energy applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20827570','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20827570"><span>PKI security in <span class="hlt">large-scale</span> healthcare networks.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Mantas, Georgios; Lymberopoulos, Dimitrios; Komninos, Nikos</p> <p>2012-06-01</p> <p>During the past few years a lot of PKI (Public Key Infrastructures) infrastructures have been proposed for healthcare networks in order to ensure secure communication services and exchange of data among healthcare professionals. However, there is a plethora of challenges in these healthcare PKI infrastructures. Especially, there are a lot of challenges for PKI infrastructures deployed over <span class="hlt">large-scale</span> healthcare networks. In this paper, we propose a PKI infrastructure to ensure security in a <span class="hlt">large-scale</span> Internet-based healthcare network connecting a wide spectrum of healthcare units geographically distributed within a wide region. Furthermore, the proposed PKI infrastructure facilitates the trust issues that arise in a <span class="hlt">large-scale</span> healthcare network including multi-domain PKI infrastructures.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUSMCG11B..03M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUSMCG11B..03M"><span>Wildfires, mountain pine beetle and <span class="hlt">large-scale</span> climate in Northern North America.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Macias Fauria, M.; Johnson, E. A.</p> <p>2009-05-01</p> <p>Research on the interactions between biosphere and atmosphere and ocean/atmosphere dynamics, concretely on the coupling between ecological processes and <span class="hlt">large-scale</span> climate, is presented in two studies in Northern North America: the occurrence of <span class="hlt">large</span> lightning wildfires and the forest area affected by mountain pine beetle (Dendroctonus ponderosae, MPB). In both cases, <span class="hlt">large-scale</span> climatic patterns such as the Pacific Decadal Oscillation (PDO) and the Arctic Oscillation (AO) operate as low and low and high frequency frameworks, respectively, that control the occurrence, duration and spatial correlation over <span class="hlt">large</span> areas of key local weather variables which affect specific ecological processes. Warm PDO phases tend to produce persistent (more than 10 days long) positive mid-troposphere anomalies (blocking highs) over western Canada and Alaska. Likewise, positive (negative) AO configurations increase the frequency of blocking highs at mid (high) latitudes of the Northern Hemisphere. Under these conditions, lack of precipitation and prevailing warm <span class="hlt">air</span> meridional flow rapidly dry fuel over <span class="hlt">large</span> areas and increase fire hazard. The spatiotemporal patterns of occurrence of <span class="hlt">large</span> lightning wildfire in Canada and Alaska for 1959-1999 were <span class="hlt">largely</span> explained by the action and possible interaction of AO and PDO, the AO being more influential over Eastern Canada, the PDO over Western Canada and Alaska. Changes in the dynamics of the PDO are linked to the occurrence of cold winter temperatures in British Columbia (BC), Western Canada. Reduced frequency of cold events during warm PDO winters is consistent with a northward-displaced polar jet stream inhibiting the outflow of cold Arctic <span class="hlt">air</span> over BC. Likewise, the AO influences the occurrence of winter cold spells in the area. PDO, and to a lesser degree AO, were strongly related to MPB synchrony in BC during 1959-2002, operating through the control of the frequency of extreme cold winter temperatures that affect MPB larvae</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=336515&Lab=NERL&keyword=soil&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=336515&Lab=NERL&keyword=soil&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>Persistence of initial conditions in continental <span class="hlt">scale</span> <span class="hlt">air</span> quality simulations</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 investigates the effect of initial conditions (IC) for pollutant concentrations in the atmosphere and soil on simulated <span class="hlt">air</span> quality for two continental-<span class="hlt">scale</span> Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model applications. One of these applications was performed for springt...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21421102-large-scale-velocities-primordial-non-gaussianity','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21421102-large-scale-velocities-primordial-non-gaussianity"><span><span class="hlt">Large-scale</span> velocities and primordial non-Gaussianity</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>Schmidt, Fabian</p> <p>2010-09-15</p> <p>We study the peculiar velocities of density peaks in the presence of primordial non-Gaussianity. Rare, high-density peaks in the initial density field can be identified with tracers such as galaxies and clusters in the evolved matter distribution. The distribution of relative velocities of peaks is derived in the <span class="hlt">large-scale</span> limit using two different approaches based on a local biasing scheme. Both approaches agree, and show that halos still stream with the dark matter locally as well as statistically, i.e. they do not acquire a velocity bias. Nonetheless, even a moderate degree of (not necessarily local) non-Gaussianity induces a significant skewnessmore » ({approx}0.1-0.2) in the relative velocity distribution, making it a potentially interesting probe of non-Gaussianity on intermediate to <span class="hlt">large</span> <span class="hlt">scales</span>. We also study two-point correlations in redshift space. The well-known Kaiser formula is still a good approximation on <span class="hlt">large</span> <span class="hlt">scales</span>, if the Gaussian halo bias is replaced with its (<span class="hlt">scale</span>-dependent) non-Gaussian generalization. However, there are additional terms not encompassed by this simple formula which become relevant on smaller <span class="hlt">scales</span> (k > or approx. 0.01h/Mpc). Depending on the allowed level of non-Gaussianity, these could be of relevance for future <span class="hlt">large</span> spectroscopic surveys.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43F..07J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43F..07J"><span>The <span class="hlt">Large</span> <span class="hlt">Scale</span> Distribution of Water Ice in the Polar Regions of the Moon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jordan, A.; Wilson, J. K.; Schwadron, N.; Spence, H. E.</p> <p>2017-12-01</p> <p>For in situ resource utilization, one must know where water ice is on the Moon. Many datasets have <span class="hlt">revealed</span> both surface deposits of water ice and subsurface deposits of hydrogen near the lunar poles, but it has proved difficult to resolve the differences among the locations of these deposits. Despite these datasets disagreeing on how deposits are distributed on small <span class="hlt">scales</span>, we show that most of these datasets do agree on the <span class="hlt">large</span> <span class="hlt">scale</span> distribution of water ice. We present data from the Cosmic Ray Telescope for the Effects of Radiation (CRaTER) on the Lunar Reconnaissance Orbiter (LRO), LRO's Lunar Exploration Neutron Detector (LEND), the Neutron Spectrometer on Lunar Prospector (LPNS), LRO's Lyman Alpha Mapping Project (LAMP), LRO's Lunar Orbiter Laser Altimeter (LOLA), and Chandrayaan-1's Moon Mineralogy Mapper (M3). All, including those that show clear evidence for water ice, <span class="hlt">reveal</span> surprisingly similar trends with latitude, suggesting that both surface and subsurface datasets are measuring ice. All show that water ice increases towards the poles, and most demonstrate that its signature appears at about ±70° latitude and increases poleward. This is consistent with simulations of how surface and subsurface cold traps are distributed with latitude. This <span class="hlt">large</span> <span class="hlt">scale</span> agreement constrains the origin of the ice, suggesting that an ancient cometary impact (or impacts) created a <span class="hlt">large</span> <span class="hlt">scale</span> deposit that has been rendered locally heterogeneous by subsequent impacts. Furthermore, it also shows that water ice may be available down to ±70°—latitudes that are more accessible than the poles for landing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22472178-large-scale-regions-antimatter','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22472178-large-scale-regions-antimatter"><span><span class="hlt">Large-scale</span> regions of antimatter</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>Grobov, A. V., E-mail: alexey.grobov@gmail.com; Rubin, S. G., E-mail: sgrubin@mephi.ru</p> <p>2015-07-15</p> <p>Amodified mechanism of the formation of <span class="hlt">large-scale</span> antimatter regions is proposed. Antimatter appears owing to fluctuations of a complex scalar field that carries a baryon charge in the inflation era.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5566788','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5566788"><span><span class="hlt">Large-Scale</span> Phylogenomics of the Lactobacillus casei Group Highlights Taxonomic Inconsistencies and <span class="hlt">Reveals</span> Novel Clade-Associated Features</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wuyts, Sander; Wittouck, Stijn; De Boeck, Ilke; Allonsius, Camille N.; Pasolli, Edoardo</p> <p>2017-01-01</p> <p>ABSTRACT Although the genotypic and phenotypic properties of the Lactobacillus casei group have been studied extensively, the taxonomic structure has been the subject of debate for a long time. Here, we performed a <span class="hlt">large-scale</span> comparative analysis by using 183 publicly available genomes supplemented with a Lactobacillus strain isolated from the human upper respiratory tract. On the basis of this analysis, we identified inconsistencies in the taxonomy and reclassified all of the genomes according to their most closely related type strains. This led to the identification of a catalase-encoding gene in all 10 L. casei sensu stricto strains, making it the first described catalase-positive species in the Lactobacillus genus. Moreover, we found that 6 of 10 L. casei genomes contained a SecA2/SecY2 gene cluster with two putative glycosylated surface adhesin proteins. Altogether, our results highlight current inconsistencies in the taxonomy of the L. casei group and <span class="hlt">reveal</span> new clade-associated functional features. IMPORTANCE The closely related species of the Lactobacillus casei group are extensively studied because of their applications in food fermentations and as probiotics. Our results show that many strains in this group are incorrectly classified and that reclassifying them to their most closely related species type strain improves the functional predictive power of their taxonomy. In addition, our findings may spark increased interest in the L. casei species. We find that after reclassification, only 10 genomes remain classified as L. casei. These strains show some interesting properties. First, they all appear to be catalase positive. This suggests that they have increased oxidative stress resistance. Second, we isolated an L. casei strain from the human upper respiratory tract and discovered that it and multiple other L. casei strains harbor one or even two <span class="hlt">large</span>, glycosylated putative surface adhesins. This might inspire further exploration of this species</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014SPIE.9085E..0WV','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014SPIE.9085E..0WV"><span>Towards <span class="hlt">large</span> <span class="hlt">scale</span> multi-target tracking</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vo, Ba-Ngu; Vo, Ba-Tuong; Reuter, Stephan; Lam, Quang; Dietmayer, Klaus</p> <p>2014-06-01</p> <p>Multi-target tracking is intrinsically an NP-hard problem and the complexity of multi-target tracking solutions usually do not <span class="hlt">scale</span> gracefully with problem size. Multi-target tracking for on-line applications involving a <span class="hlt">large</span> number of targets is extremely challenging. This article demonstrates the capability of the random finite set approach to provide <span class="hlt">large</span> <span class="hlt">scale</span> multi-target tracking algorithms. In particular it is shown that an approximate filter known as the labeled multi-Bernoulli filter can simultaneously track one thousand five hundred targets in clutter on a standard laptop computer.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA179406','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA179406"><span>The Expanded <span class="hlt">Large</span> <span class="hlt">Scale</span> Gap Test</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1987-03-01</p> <p>NSWC TR 86-32 DTIC THE EXPANDED <span class="hlt">LARGE</span> <span class="hlt">SCALE</span> GAP TEST BY T. P. LIDDIARD D. PRICE RESEARCH AND TECHNOLOGY DEPARTMENT ’ ~MARCH 1987 Ap~proved for public...arises, to reduce the spread in the LSGT 50% gap value.) The worst charges, such as those with the highest or lowest densities, the largest re-pressed...Arlington, VA 22217 PE 62314N INS3A 1 RJ14E31 7R4TBK 11 TITLE (Include Security CIlmsilficatiorn The Expanded <span class="hlt">Large</span> <span class="hlt">Scale</span> Gap Test . 12. PEIRSONAL AUTHOR() T</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750021775','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750021775"><span>An informal paper on <span class="hlt">large-scale</span> dynamic systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ho, Y. C.</p> <p>1975-01-01</p> <p><span class="hlt">Large</span> <span class="hlt">scale</span> systems are defined as systems requiring more than one decision maker to control the system. Decentralized control and decomposition are discussed for <span class="hlt">large</span> <span class="hlt">scale</span> dynamic systems. Information and many-person decision problems are analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhFl...30d6601Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhFl...30d6601Z"><span><span class="hlt">Large-scale</span> coherent structures of suspended dust concentration in the neutral atmospheric surface layer: A <span class="hlt">large</span>-eddy simulation study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Yangyue; Hu, Ruifeng; Zheng, Xiaojing</p> <p>2018-04-01</p> <p>Dust particles can remain suspended in the atmospheric boundary layer, motions of which are primarily determined by turbulent diffusion and gravitational settling. Little is known about the spatial organizations of suspended dust concentration and how turbulent coherent motions contribute to the vertical transport of dust particles. Numerous studies in recent years have <span class="hlt">revealed</span> that <span class="hlt">large</span>- and very-<span class="hlt">large-scale</span> motions in the logarithmic region of laboratory-<span class="hlt">scale</span> turbulent boundary layers also exist in the high Reynolds number atmospheric boundary layer, but their influence on dust transport is still unclear. In this study, numerical simulations of dust transport in a neutral atmospheric boundary layer based on an Eulerian modeling approach and <span class="hlt">large</span>-eddy simulation technique are performed to investigate the coherent structures of dust concentration. The instantaneous fields confirm the existence of very long meandering streaks of dust concentration, with alternating high- and low-concentration regions. A strong negative correlation between the streamwise velocity and concentration and a mild positive correlation between the vertical velocity and concentration are observed. The spatial length <span class="hlt">scales</span> and inclination angles of concentration structures are determined, compared with their flow counterparts. The conditionally averaged fields vividly depict that high- and low-concentration events are accompanied by a pair of counter-rotating quasi-streamwise vortices, with a downwash inside the low-concentration region and an upwash inside the high-concentration region. Through the quadrant analysis, it is indicated that the vertical dust transport is closely related to the <span class="hlt">large-scale</span> roll modes, and ejections in high-concentration regions are the major mechanisms for the upward motions of dust particles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22356448-large-scale-dynamo-action-high-magnetic-reynolds-number','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22356448-large-scale-dynamo-action-high-magnetic-reynolds-number"><span>On <span class="hlt">large-scale</span> dynamo action at high magnetic Reynolds number</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>Cattaneo, F.; Tobias, S. M., E-mail: smt@maths.leeds.ac.uk</p> <p>2014-07-01</p> <p>We consider the generation of magnetic activity—dynamo waves—in the astrophysical limit of very <span class="hlt">large</span> magnetic Reynolds number. We consider kinematic dynamo action for a system consisting of helical flow and <span class="hlt">large-scale</span> shear. We demonstrate that <span class="hlt">large-scale</span> dynamo waves persist at high Rm if the helical flow is characterized by a narrow band of spatial <span class="hlt">scales</span> and the shear is <span class="hlt">large</span> enough. However, for a wide band of <span class="hlt">scales</span> the dynamo becomes small <span class="hlt">scale</span> with a further increase of Rm, with dynamo waves re-emerging only if the shear is then increased. We show that at high Rm, the key effect ofmore » the shear is to suppress small-<span class="hlt">scale</span> dynamo action, allowing <span class="hlt">large-scale</span> dynamo action to be observed. We conjecture that this supports a general 'suppression principle'—<span class="hlt">large-scale</span> dynamo action can only be observed if there is a mechanism that suppresses the small-<span class="hlt">scale</span> fluctuations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018A%26A...612A..97B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018A%26A...612A..97B"><span><span class="hlt">Large-scale</span> dynamos in rapidly rotating plane layer convection</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bushby, P. J.; Käpylä, P. J.; Masada, Y.; Brandenburg, A.; Favier, B.; Guervilly, C.; Käpylä, M. J.</p> <p>2018-05-01</p> <p>Context. Convectively driven flows play a crucial role in the dynamo processes that are responsible for producing magnetic activity in stars and planets. It is still not fully understood why many astrophysical magnetic fields have a significant <span class="hlt">large-scale</span> component. Aims: Our aim is to investigate the dynamo properties of compressible convection in a rapidly rotating Cartesian domain, focusing upon a parameter regime in which the underlying hydrodynamic flow is known to be unstable to a <span class="hlt">large-scale</span> vortex instability. Methods: The governing equations of three-dimensional non-linear magnetohydrodynamics (MHD) are solved numerically. Different numerical schemes are compared and we propose a possible benchmark case for other similar codes. Results: In keeping with previous related studies, we find that convection in this parameter regime can drive a <span class="hlt">large-scale</span> dynamo. The components of the mean horizontal magnetic field oscillate, leading to a continuous overall rotation of the mean field. Whilst the <span class="hlt">large-scale</span> vortex instability dominates the early evolution of the system, the <span class="hlt">large-scale</span> vortex is suppressed by the magnetic field and makes a negligible contribution to the mean electromotive force that is responsible for driving the <span class="hlt">large-scale</span> dynamo. The cycle period of the dynamo is comparable to the ohmic decay time, with longer cycles for dynamos in convective systems that are closer to onset. In these particular simulations, <span class="hlt">large-scale</span> dynamo action is found only when vertical magnetic field boundary conditions are adopted at the upper and lower boundaries. Strongly modulated <span class="hlt">large-scale</span> dynamos are found at higher Rayleigh numbers, with periods of reduced activity (grand minima-like events) occurring during transient phases in which the <span class="hlt">large-scale</span> vortex temporarily re-establishes itself, before being suppressed again by the magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EPJWC.15900032M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EPJWC.15900032M"><span>Experimental study of <span class="hlt">air</span> delivery into water-conveyance system of the radial-axial turbine</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maslennikova, Alexandra; Platonov, Dmitry; Minakov, Andrey; Dekterev, Dmitry</p> <p>2017-10-01</p> <p>The paper presents an experimental study of oscillatory response in the Francis turbine of hydraulic unit. The experiment was performed on <span class="hlt">large-scale</span> hydrodynamic test-bench with impeller diameter of 0.3 m. The effect of <span class="hlt">air</span> injection on the intensity of pressure pulsations was studied at the maximum pressure pulsations in the hydraulic unit. It was <span class="hlt">revealed</span> that <span class="hlt">air</span> delivery into the water-conveyance system of the turbine results in almost two-fold reduction of pressure pulsations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810046679&hterms=L37&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DL37','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810046679&hterms=L37&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DL37"><span><span class="hlt">Large-scale</span> anisotropy of the cosmic microwave background radiation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Silk, J.; Wilson, M. L.</p> <p>1981-01-01</p> <p>Inhomogeneities in the <span class="hlt">large-scale</span> distribution of matter inevitably lead to the generation of <span class="hlt">large-scale</span> anisotropy in the cosmic background radiation. The dipole, quadrupole, and higher order fluctuations expected in an Einstein-de Sitter cosmological model have been computed. The dipole and quadrupole anisotropies are comparable to the measured values, and impose important constraints on the allowable spectrum of <span class="hlt">large-scale</span> matter density fluctuations. A significant dipole anisotropy is generated by the matter distribution on <span class="hlt">scales</span> greater than approximately 100 Mpc. The <span class="hlt">large-scale</span> anisotropy is insensitive to the ionization history of the universe since decoupling, and cannot easily be reconciled with a galaxy formation theory that is based on primordial adiabatic density fluctuations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950039640&hterms=affect+heuristics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Daffect%2Bheuristics','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950039640&hterms=affect+heuristics&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Daffect%2Bheuristics"><span><span class="hlt">Large-scale</span> effects on the regulation of tropical sea surface temperature</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hartmann, Dennis L.; Michelsen, Marc L.</p> <p>1993-01-01</p> <p>The dominant terms in the surface energy budget of the tropical oceans are absorption of solar radiation and evaporative cooling. If it is assumed that relative humidity in the boundary layer remains constant, evaporative cooling will increase rapidly with sea surface temperature (SST) because of the strong temperature dependence of saturation water vapor pressure. The resulting stabilization of SST provided by evaporative cooling is sufficient to overcome positive feedback contributed by the decrease of surface net longwave cooling with increasing SST. Evaporative cooling is sensitive to small changes in boundary-layer relative humidity. <span class="hlt">Large</span> and negative shortwave cloud forcing in the regions of highest SST are supported by the moisture convergence associated with largescale circulations. In the descending portions of these circulations the shortwave cloud forcing is suppressed. When the effect of these circulations is taken into account by spatial averaging, the area-averaged cloud forcing shows no sensitivity to area-averaged SST changes associated with the 1987 warming event in the tropical Pacific. While the shortwave cloud forcing is <span class="hlt">large</span> and important in the convective regions, the importance of its role in regulating the average temperature of the tropics and in modulating temperature gradients within the tropics is less clear. A heuristic model of SST is used to illustrate the possible role of <span class="hlt">large-scale</span> atmospheric circulations on SST in the tropics and the coupling between SST gradients and mean tropical SST. The intensity of <span class="hlt">large-scale</span> circulations responds sensitivity to SST gradients and affects the mean tropical SST by supplying dry <span class="hlt">air</span> to the planetary boundary layer. <span class="hlt">Large</span> SST gradients generate vigorous circulations that increase evaporation and reduce the mean SST.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li class="active"><span>10</span></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_10 --> <div id="page_11" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="201"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AMT.....6..817W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AMT.....6..817W"><span>Jena Reference <span class="hlt">Air</span> Set (JRAS): a multi-point <span class="hlt">scale</span> anchor for isotope measurements of CO2 in <span class="hlt">air</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wendeberg, M.; Richter, J. M.; Rothe, M.; Brand, W. A.</p> <p>2013-03-01</p> <p>The need for a unifying <span class="hlt">scale</span> anchor for isotopes of CO2 in <span class="hlt">air</span> was brought to light at the 11th WMO/IAEA Meeting of Experts on Carbon Dioxide in Tokyo 2001. During discussions about persistent discrepancies in isotope measurements between the worlds leading laboratories, it was concluded that a unifying <span class="hlt">scale</span> anchor for Vienna Pee Dee Belemnite (VPDB) of CO2 in <span class="hlt">air</span> was desperately needed. Ten years later, at the 2011 Meeting of Experts on Carbon Dioxide in Wellington, it was recommended that the Jena Reference <span class="hlt">Air</span> Set (JRAS) become the official <span class="hlt">scale</span> anchor for isotope measurements of CO2 in <span class="hlt">air</span> (Brailsford, 2012). The source of CO2 used for JRAS is two calcites. After releasing CO2 by reaction with phosphoric acid, the gases are mixed into CO2-free <span class="hlt">air</span>. This procedure ensures both isotopic stability and longevity of the CO2. That the reference CO2 is generated from calcites and supplied as an <span class="hlt">air</span> mixture is unique to JRAS. This is made to ensure that any measurement bias arising from the extraction procedure is eliminated. As every laboratory has its own procedure for extracting the CO2, this is of paramount importance if the local <span class="hlt">scales</span> are to be unified with a common anchor. For a period of four years, JRAS has been evaluated through the IMECC1 program, which made it possible to distribute sets of JRAS gases to 13 laboratories worldwide. A summary of data from the six laboratories that have reported the full set of results is given here along with a description of the production and maintenance of the JRAS <span class="hlt">scale</span> anchors. 1 IMECC refers to the EU project "Infrastructure for Measurements of the European Carbon Cycle" (<a href="http://imecc.ipsl.jussieu.fr/"target="_blank">http://imecc.ipsl.jussieu.fr/</a>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..171a2013C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..171a2013C"><span>Economically viable <span class="hlt">large-scale</span> hydrogen liquefaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cardella, U.; Decker, L.; Klein, H.</p> <p>2017-02-01</p> <p>The liquid hydrogen demand, particularly driven by clean energy applications, will rise in the near future. As industrial <span class="hlt">large</span> <span class="hlt">scale</span> liquefiers will play a major role within the hydrogen supply chain, production capacity will have to increase by a multiple of today’s typical sizes. The main goal is to reduce the total cost of ownership for these plants by increasing energy efficiency with innovative and simple process designs, optimized in capital expenditure. New concepts must ensure a manageable plant complexity and flexible operability. In the phase of process development and selection, a dimensioning of key equipment for <span class="hlt">large</span> <span class="hlt">scale</span> liquefiers, such as turbines and compressors as well as heat exchangers, must be performed iteratively to ensure technological feasibility and maturity. Further critical aspects related to hydrogen liquefaction, e.g. fluid properties, ortho-para hydrogen conversion, and coldbox configuration, must be analysed in detail. This paper provides an overview on the approach, challenges and preliminary results in the development of efficient as well as economically viable concepts for <span class="hlt">large-scale</span> hydrogen liquefaction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990109131&hterms=Jason+Moore&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DJason%2BMoore','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990109131&hterms=Jason+Moore&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DJason%2BMoore"><span><span class="hlt">Large-Scale</span> Coronal Heating from the Solar Magnetic Network</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Falconer, David A.; Moore, Ronald L.; Porter, Jason G.; Hathaway, David H.</p> <p>1999-01-01</p> <p>In Fe 12 images from SOHO/EIT, the quiet solar corona shows structure on <span class="hlt">scales</span> ranging from sub-supergranular (i.e., bright points and coronal network) to multi- supergranular. In Falconer et al 1998 (Ap.J., 501, 386) we suppressed the <span class="hlt">large-scale</span> background and found that the network-<span class="hlt">scale</span> features are predominantly rooted in the magnetic network lanes at the boundaries of the supergranules. The emission of the coronal network and bright points contribute only about 5% of the entire quiet solar coronal Fe MI emission. Here we investigate the <span class="hlt">large-scale</span> corona, the supergranular and larger-<span class="hlt">scale</span> structure that we had previously treated as a background, and that emits 95% of the total Fe XII emission. We compare the dim and bright halves of the <span class="hlt">large</span>- <span class="hlt">scale</span> corona and find that the bright half is 1.5 times brighter than the dim half, has an order of magnitude greater area of bright point coverage, has three times brighter coronal network, and has about 1.5 times more magnetic flux than the dim half These results suggest that the brightness of the <span class="hlt">large-scale</span> corona is more closely related to the <span class="hlt">large</span>- <span class="hlt">scale</span> total magnetic flux than to bright point activity. We conclude that in the quiet sun: (1) Magnetic flux is modulated (concentrated/diluted) on size <span class="hlt">scales</span> larger than supergranules. (2) The <span class="hlt">large-scale</span> enhanced magnetic flux gives an enhanced, more active, magnetic network and an increased incidence of network bright point formation. (3) The heating of the <span class="hlt">large-scale</span> corona is dominated by more widespread, but weaker, network activity than that which heats the bright points. This work was funded by the Solar Physics Branch of NASA's office of Space Science through the SR&T Program and the SEC Guest Investigator Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015APS..DFDL32003S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDL32003S"><span><span class="hlt">Large</span> Field of View PIV Measurements of <span class="hlt">Air</span> Entrainment by SLS SMAT Water Sound Suppression System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stegmeir, Matthew; Pothos, Stamatios; Bissell, Dan</p> <p>2015-11-01</p> <p>Water-based sound suppressions systems have been used to reduce the acoustic impact of space vehicle launches. Water flows at a high rate during launch in order to suppress Engine Generated Acoustics and other potentially damaging sources of noise. For the Space Shuttle, peak flow rates exceeded 900,000 gallons per minute. Such <span class="hlt">large</span> water flow rates have the potential to induce substantial entrainment of the surrounding <span class="hlt">air</span>, affecting the launch conditions and generating airflow around the launch vehicle. Validation testing is necessary to quantify this impact for future space launch systems. In this study, PIV measurements were performed to map the flow field above the SMAT sub-<span class="hlt">scale</span> launch vehicle <span class="hlt">scaled</span> launch stand. <span class="hlt">Air</span> entrainment effects generated by a water-based sound suppression system were studied. Mean and fluctuating fluid velocities were mapped up to 1m above the test stand deck and compared to simulation results. Measurements performed with NASA MSFC.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A21I..03G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A21I..03G"><span><span class="hlt">Large</span>- and Very-<span class="hlt">Large-Scale</span> Motions in Katabatic Flows Over Steep Slopes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Giometto, M. G.; Fang, J.; Salesky, S.; Parlange, M. B.</p> <p>2016-12-01</p> <p>Evidence of <span class="hlt">large</span>- and very-<span class="hlt">large-scale</span> motions populating the boundary layer in katabatic flows over steep slopes is presented via direct numerical simulations (DNSs). DNSs are performed at a modified Reynolds number (Rem = 967), considering four sloping angles (α = 60°, 70°, 80° and 90°). <span class="hlt">Large</span> coherent structures prove to be strongly dependent on the inclination of the underlying surface. Spectra and co-spectra consistently show signatures of <span class="hlt">large-scale</span> motions (LSMs), with streamwise extension on the order of the boundary layer thickness. A second low-wavenumber mode characterizes pre-multiplied spectra and co-spectra when the slope angle is below 70°, indicative of very-<span class="hlt">large-scale</span> motions (VLSMs). In addition, conditional sampling and averaging shows how LSMs and VLSMs are induced by counter-rotating roll modes, in agreement with findings from canonical wall-bounded flows. VLSMs contribute to the stream-wise velocity variance and shear stress in the above-jet regions up to 30% and 45% respectively, whereas both LSMs and VLSMs are inactive in the near-wall regions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012JPhCS.340a2094Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012JPhCS.340a2094Y"><span>Correlated motion of protein subdomains and <span class="hlt">large-scale</span> conformational flexibility of RecA protein filament</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yu, Garmay; A, Shvetsov; D, Karelov; D, Lebedev; A, Radulescu; M, Petukhov; V, Isaev-Ivanov</p> <p>2012-02-01</p> <p>Based on X-ray crystallographic data available at Protein Data Bank, we have built molecular dynamics (MD) models of homologous recombinases RecA from E. coli and D. radiodurans. Functional form of RecA enzyme, which is known to be a long helical filament, was approximated by a trimer, simulated in periodic water box. The MD trajectories were analyzed in terms of <span class="hlt">large-scale</span> conformational motions that could be detectable by neutron and X-ray scattering techniques. The analysis <span class="hlt">revealed</span> that <span class="hlt">large-scale</span> RecA monomer dynamics can be described in terms of relative motions of 7 subdomains. Motion of C-terminal domain was the major contributor to the overall dynamics of protein. Principal component analysis (PCA) of the MD trajectories in the atom coordinate space showed that rotation of C-domain is correlated with the conformational changes in the central domain and N-terminal domain, that forms the monomer-monomer interface. Thus, even though C-terminal domain is relatively far from the interface, its orientation is correlated with <span class="hlt">large-scale</span> filament conformation. PCA of the trajectories in the main chain dihedral angle coordinate space implicates a co-existence of a several different <span class="hlt">large-scale</span> conformations of the modeled trimer. In order to clarify the relationship of independent domain orientation with <span class="hlt">large-scale</span> filament conformation, we have performed analysis of independent domain motion and its implications on the filament geometry.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H21A1366R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H21A1366R"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Processes and Extreme Floods in Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ribeiro Lima, C. H.; AghaKouchak, A.; Lall, U.</p> <p>2016-12-01</p> <p>Persistent <span class="hlt">large</span> <span class="hlt">scale</span> anomalies in the atmospheric circulation and ocean state have been associated with heavy rainfall and extreme floods in water basins of different sizes across the world. Such studies have emerged in the last years as a new tool to improve the traditional, stationary based approach in flood frequency analysis and flood prediction. Here we seek to advance previous studies by evaluating the dominance of <span class="hlt">large</span> <span class="hlt">scale</span> processes (e.g. atmospheric rivers/moisture transport) over local processes (e.g. local convection) in producing floods. We consider flood-prone regions in Brazil as case studies and the role of <span class="hlt">large</span> <span class="hlt">scale</span> climate processes in generating extreme floods in such regions is explored by means of observed streamflow, reanalysis data and machine learning methods. The dynamics of the <span class="hlt">large</span> <span class="hlt">scale</span> atmospheric circulation in the days prior to the flood events are evaluated based on the vertically integrated moisture flux and its divergence field, which are interpreted in a low-dimensional space as obtained by machine learning techniques, particularly supervised kernel principal component analysis. In such reduced dimensional space, clusters are obtained in order to better understand the role of regional moisture recycling or teleconnected moisture in producing floods of a given magnitude. The convective available potential energy (CAPE) is also used as a measure of local convection activities. We investigate for individual sites the exceedance probability in which <span class="hlt">large</span> <span class="hlt">scale</span> atmospheric fluxes dominate the flood process. Finally, we analyze regional patterns of floods and how the <span class="hlt">scaling</span> law of floods with drainage area responds to changes in the climate forcing mechanisms (e.g. local vs <span class="hlt">large</span> <span class="hlt">scale</span>).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920021427&hterms=density+buoyancy&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddensity%2Bbuoyancy','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920021427&hterms=density+buoyancy&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Ddensity%2Bbuoyancy"><span>Generation of <span class="hlt">large-scale</span> density fluctuations by buoyancy</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chasnov, J. R.; Rogallo, R. S.</p> <p>1990-01-01</p> <p>The generation of fluid motion from a state of rest by buoyancy forces acting on a homogeneous isotropic small-<span class="hlt">scale</span> density field is considered. Nonlinear interactions between the generated fluid motion and the initial isotropic small-<span class="hlt">scale</span> density field are found to create an anisotropic <span class="hlt">large-scale</span> density field with spectrum proportional to kappa(exp 4). This <span class="hlt">large-scale</span> density field is observed to result in an increasing Reynolds number of the fluid turbulence in its final period of decay.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AtmEn..45.4481R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AtmEn..45.4481R"><span>A cellphone based system for <span class="hlt">large-scale</span> monitoring of black carbon</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ramanathan, N.; Lukac, M.; Ahmed, T.; Kar, A.; Praveen, P. S.; Honles, T.; Leong, I.; Rehman, I. H.; Schauer, J. J.; Ramanathan, V.</p> <p>2011-08-01</p> <p>Black carbon aerosols are a major component of soot and are also a major contributor to global and regional climate change. Reliable and cost-effective systems to measure near-surface black carbon (BC) mass concentrations (hereafter denoted as [BC]) globally are necessary to validate <span class="hlt">air</span> pollution and climate models and to evaluate the effectiveness of BC mitigation actions. Toward this goal we describe a new wireless, low-cost, ultra low-power, BC cellphone based monitoring system (BC_CBM). BC_CBM integrates a Miniaturized Aerosol filter Sampler (MAS) with a cellphone for filter image collection, transmission and image analysis for determining [BC] in real time. The BC aerosols in the <span class="hlt">air</span> accumulate on the MAS quartz filter, resulting in a coloration of the filter. A photograph of the filter is captured by the cellphone camera and transmitted by the cellphone to the analytics component of BC_CBM. The analytics component compares the image with a calibrated reference <span class="hlt">scale</span> (also included in the photograph) to estimate [BC]. We demonstrate with field data collected from vastly differing environments, ranging from southern California to rural regions in the Indo-Gangetic plains of Northern India, that the total BC deposited on the filter is directly and uniquely related to the reflectance of the filter in the red wavelength, irrespective of its source or how the particles were deposited. [BC] varied from 0.1 to 1 μg m -3 in Southern California and from 10 to 200 μg m -3 in rural India in our field studies. In spite of the 3 orders of magnitude variation in [BC], the BC_CBM system was able to determine the [BC] well within the experimental error of two independent reference instruments for both indoor <span class="hlt">air</span> and outdoor ambient <span class="hlt">air</span>. Accurate, global-<span class="hlt">scale</span> measurements of [BC] in urban and remote rural locations, enabled by the wireless, low-cost, ultra low-power operation of BC_CBM, will make it possible to better capture the <span class="hlt">large</span> spatial and temporal variations in</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2950238','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2950238"><span>Development of a <span class="hlt">large-scale</span> isolation chamber system for the safe and humane care of medium-sized laboratory animals harboring infectious diseases*</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Pan, Xin; Qi, Jian-cheng; Long, Ming; Liang, Hao; Chen, Xiao; Li, Han; Li, Guang-bo; Zheng, Hao</p> <p>2010-01-01</p> <p>The close phylogenetic relationship between humans and non-human primates makes non-human primates an irreplaceable model for the study of human infectious diseases. In this study, we describe the development of a <span class="hlt">large-scale</span> automatic multi-functional isolation chamber for use with medium-sized laboratory animals carrying infectious diseases. The isolation chamber, including the transfer chain, disinfection chain, negative <span class="hlt">air</span> pressure isolation system, animal welfare system, and the automated system, is designed to meet all biological safety standards. To create an internal chamber environment that is completely isolated from the exterior, variable frequency drive blowers are used in the <span class="hlt">air</span>-intake and <span class="hlt">air</span>-exhaust system, precisely controlling the filtered <span class="hlt">air</span> flow and providing an <span class="hlt">air</span>-barrier protection. A double door transfer port is used to transfer material between the interior of the isolation chamber and the outside. A peracetic acid sterilizer and its associated pipeline allow for complete disinfection of the isolation chamber. All of the isolation chamber parameters can be automatically controlled by a programmable computerized menu, allowing for work with different animals in different-sized cages depending on the research project. The <span class="hlt">large-scale</span> multi-functional isolation chamber provides a useful and safe system for working with infectious medium-sized laboratory animals in high-level bio-safety laboratories. PMID:20872984</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA531338','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA531338"><span><span class="hlt">Large-Scale</span> Aerosol Modeling and Analysis</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2009-09-30</p> <p>Modeling of Burning Emissions ( FLAMBE ) project, and other related parameters. Our plans to embed NAAPS inside NOGAPS may need to be put on hold...AOD, FLAMBE and FAROP at FNMOC are supported by 6.4 funding from PMW-120 for “<span class="hlt">Large-scale</span> Atmospheric Models”, “Small-<span class="hlt">scale</span> Atmospheric Models</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1011080','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1011080"><span>Information Tailoring Enhancements for <span class="hlt">Large-Scale</span> Social Data</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-06-15</p> <p>Intelligent Automation Incorporated Information Tailoring Enhancements for <span class="hlt">Large-Scale</span>... Automation Incorporated Progress Report No. 3 Information Tailoring Enhancements for <span class="hlt">Large-Scale</span> Social Data Submitted in accordance with...1 Work Performed within This Reporting Period .................................................... 2 1.1 Enhanced Named Entity Recognition (NER</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.H53F1516N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.H53F1516N"><span>Temporal sequencing of throughfall drop generation as <span class="hlt">revealed</span> by use of a <span class="hlt">large-scale</span> rainfall simulator</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nanko, K.; Levia, D. F., Jr.; Iida, S.; SUN, X.; Shinohara, Y.; Sakai, N.</p> <p>2017-12-01</p> <p>Scientists have been interested in throughfall drop size and its distribution because of its importance to soil erosion and the forest water balance. An indoor experiment was employed to deepen our understanding of throughfall drop generation processes to promote better management of forested ecosystems. The indoor experiment provides a unique opportunity to examine an array of constant rainfall intensities that are ideal conditions to pick up the effect of changing intensities and not found in the fields. Throughfall drop generation was examined for three species- Cryptomeria japonica D. Don (Japanese cedar), Chamaecyparis obtusa (Siebold & Zucc.) Endl. (Japanese cypress), and Zelkova serrata Thunb. (Japanese zelkova)- under both leafed and leafless conditions in the <span class="hlt">large-scale</span> rainfall simulator in the National Research Institute for Earth Science and Disaster Resilience (Tsukuba, Japan) at varying rainfall intensities ranging from15 to 100 mm h-1. Drop size distributions of the applied rainfall and throughfall were measured simultaneously by 20 laser disdrometers. Utilizing the drop size dataset, throughfall was separated into three components: free throughfall, canopy drip, and splash throughfall. The temporal sequencing of the throughfall components were analyzed on a 1-min interval during each experimental run. The throughfall component percentage and drop size of canopy drip differed among tree species and rainfall intensities and by elapsed time from the beginning of the rainfall event. Preliminary analysis <span class="hlt">revealed</span> that the time differences to produce branch drip as compared to leaf (or needle) drip was partly due to differential canopy wet-up processes and the disappearance of branch drips due to canopy saturation, leading to dissimilar throughfall drop size distributions beneath the various tree species examined. This research was supported by JSPS Invitation Fellowship for Research in Japan (Grant No.: S16088) and JSPS KAKENHI (Grant No.: JP15H05626).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014QSRv...90..106Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014QSRv...90..106Z"><span>Mid-Holocene cluster of <span class="hlt">large-scale</span> landslides <span class="hlt">revealed</span> in the Southwestern Alps by 36Cl dating. Insight on an Alpine-<span class="hlt">scale</span> landslide activity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zerathe, Swann; Lebourg, Thomas; Braucher, Régis; Bourlès, Didier</p> <p>2014-04-01</p> <p>Although it is generally assumed that the internal structure of a slope (e.g. lithology and rock mass properties, inherited faults and heterogeneities, etc.) is preponderant for the progressive development of <span class="hlt">large-scale</span> landslides, the ability to identify triggering factors responsible for final slope failures such as glacial debuttressing, seismic activities or climatic changes, especially when considering landslide cluster at an orogen-<span class="hlt">scale</span>, is still debated. Highlighting in this study the spatial and temporal concordant clustering of deep-seated slope failures in the external Southwestern Alps, we discuss and review the possible causes for such wide-spread slope instabilities at both local and larger (Alpine) <span class="hlt">scale</span>. High resolution field mapping coupled with electrical resistivity tomography first allows establishing an inventory of <span class="hlt">large</span> landslides in the Southwestern Alps, determining their structural model, precising their depth limit (100-200 m) as well as the involved rock volumes (>107 m3). We show that they developed in the same geostructural context of thick mudstone layers overlain by faulted limestone and followed a block-spread model of deformation that could evolve in rock-collapse events. Cosmic ray exposure dating (CRE), using both 36Cl and 10Be in coexisting limestone and chert, respectively, has been carried out from the main scarps of six Deep Seated Landslides (DSL) and leads to landslide-failure CRE ages ranging from 3.7 to 4.7 ka. They highlighted: (i) mainly single and fast ruptures and (ii) a possible concomitant initiation with a main peak of activity between 3.3 and 5.1 ka, centered at ca 4.2 ka. Because this region was not affected by historical glaciations events, landslide triggering by glacial unloading can be excluded. The presented data combined with field observations preferentially suggest that these failures were climatically driven and were most likely controlled by high pressure changes in the karstic medium. In effect, the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720016558','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720016558"><span>A bibliographical surveys of <span class="hlt">large-scale</span> systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Corliss, W. R.</p> <p>1970-01-01</p> <p>A limited, partly annotated bibliography was prepared on the subject of <span class="hlt">large-scale</span> system control. Approximately 400 references are divided into thirteen application areas, such as <span class="hlt">large</span> societal systems and <span class="hlt">large</span> communication systems. A first-author index is provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AtmEn..45.3352Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AtmEn..45.3352Z"><span>Effect of real-time boundary wind conditions on the <span class="hlt">air</span> flow and pollutant dispersion in an urban street canyon—<span class="hlt">Large</span> eddy simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Yun-Wei; Gu, Zhao-Lin; Cheng, Yan; Lee, Shun-Cheng</p> <p>2011-07-01</p> <p><span class="hlt">Air</span> flow and pollutant dispersion characteristics in an urban street canyon are studied under the real-time boundary conditions. A new scheme for realizing real-time boundary conditions in simulations is proposed, to keep the upper boundary wind conditions consistent with the measured time series of wind data. The <span class="hlt">air</span> flow structure and its evolution under real-time boundary wind conditions are simulated by using this new scheme. The induced effect of time series of ambient wind conditions on the flow structures inside and above the street canyon is investigated. The flow shows an obvious intermittent feature in the street canyon and the flapping of the shear layer forms near the roof layer under real-time wind conditions, resulting in the expansion or compression of the <span class="hlt">air</span> mass in the canyon. The simulations of pollutant dispersion show that the pollutants inside and above the street canyon are transported by different dispersion mechanisms, relying on the time series of <span class="hlt">air</span> flow structures. <span class="hlt">Large</span> <span class="hlt">scale</span> <span class="hlt">air</span> movements in the processes of the <span class="hlt">air</span> mass expansion or compression in the canyon exhibit obvious effects on pollutant dispersion. The simulations of pollutant dispersion also show that the transport of pollutants from the canyon to the upper <span class="hlt">air</span> flow is dominated by the shear layer turbulence near the roof level and the expansion or compression of the <span class="hlt">air</span> mass in street canyon under real-time boundary wind conditions. Especially, the expansion of the <span class="hlt">air</span> mass, which features the <span class="hlt">large</span> <span class="hlt">scale</span> <span class="hlt">air</span> movement of the <span class="hlt">air</span> mass, makes more contribution to the pollutant dispersion in this study. Comparisons of simulated results under different boundary wind conditions indicate that real-time boundary wind conditions produces better condition for pollutant dispersion than the artificially-designed steady boundary wind conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080040697','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080040697"><span>A Revised Method of Presenting Wavenumber-Frequency Power Spectrum Diagrams That <span class="hlt">Reveals</span> the Asymmetric Nature of Tropical <span class="hlt">Large-scale</span> Waves</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chao, Winston C.; Yang, Bo; Fu, Xiouhua</p> <p>2007-01-01</p> <p>The popular method of presenting wavenumber-frequency power spectrum diagrams for studying tropical <span class="hlt">large-scale</span> waves in the literature is shown to give an incomplete presentation of these waves. The so-called "convectively-coupled Kelvin (mixed Rossby-gravity) waves" are presented as existing only in the symmetric (antisymmetric) component of the diagrams. This is obviously not consistent with the published composite/regression studies of "convectively-coupled Kelvin waves," which illustrate the asymmetric nature of these waves. The cause of this inconsistency is <span class="hlt">revealed</span> in this note and a revised method of presenting the power spectrum diagrams is proposed. When this revised method is used, "convectively-coupled Kelvin waves" do show anti-symmetric components, and "convectively-coupled mixed Rossby-gravity waves (also known as Yanai waves)" do show a hint of symmetric components. These results bolster a published proposal that these waves be called "chimeric Kelvin waves," "chimeric mixed Rossby-gravity waves," etc. This revised method of presenting power spectrum diagrams offers a more rigorous means of comparing the General Circulation Models (GCM) output with observations by calling attention to the capability of GCMs in correctly simulating the asymmetric characteristics of the equatorial waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22006969','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22006969"><span>A <span class="hlt">large-scale</span> forest fragmentation experiment: the Stability of Altered Forest Ecosystems Project.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ewers, Robert M; Didham, Raphael K; Fahrig, Lenore; Ferraz, Gonçalo; Hector, Andy; Holt, Robert D; Kapos, Valerie; Reynolds, Glen; Sinun, Waidi; Snaddon, Jake L; Turner, Edgar C</p> <p>2011-11-27</p> <p>Opportunities to conduct <span class="hlt">large-scale</span> field experiments are rare, but provide a unique opportunity to <span class="hlt">reveal</span> the complex processes that operate within natural ecosystems. Here, we review the design of existing, <span class="hlt">large-scale</span> forest fragmentation experiments. Based on this review, we develop a design for the Stability of Altered Forest Ecosystems (SAFE) Project, a new forest fragmentation experiment to be located in the lowland tropical forests of Borneo (Sabah, Malaysia). The SAFE Project represents an advance on existing experiments in that it: (i) allows discrimination of the effects of landscape-level forest cover from patch-level processes; (ii) is designed to facilitate the unification of a wide range of data types on ecological patterns and processes that operate over a wide range of spatial <span class="hlt">scales</span>; (iii) has greater replication than existing experiments; (iv) incorporates an experimental manipulation of riparian corridors; and (v) embeds the experimentally fragmented landscape within a wider gradient of land-use intensity than do existing projects. The SAFE Project represents an opportunity for ecologists across disciplines to participate in a <span class="hlt">large</span> initiative designed to generate a broad understanding of the ecological impacts of tropical forest modification.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3179633','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3179633"><span>A <span class="hlt">large-scale</span> forest fragmentation experiment: the Stability of Altered Forest Ecosystems Project</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ewers, Robert M.; Didham, Raphael K.; Fahrig, Lenore; Ferraz, Gonçalo; Hector, Andy; Holt, Robert D.; Kapos, Valerie; Reynolds, Glen; Sinun, Waidi; Snaddon, Jake L.; Turner, Edgar C.</p> <p>2011-01-01</p> <p>Opportunities to conduct <span class="hlt">large-scale</span> field experiments are rare, but provide a unique opportunity to <span class="hlt">reveal</span> the complex processes that operate within natural ecosystems. Here, we review the design of existing, <span class="hlt">large-scale</span> forest fragmentation experiments. Based on this review, we develop a design for the Stability of Altered Forest Ecosystems (SAFE) Project, a new forest fragmentation experiment to be located in the lowland tropical forests of Borneo (Sabah, Malaysia). The SAFE Project represents an advance on existing experiments in that it: (i) allows discrimination of the effects of landscape-level forest cover from patch-level processes; (ii) is designed to facilitate the unification of a wide range of data types on ecological patterns and processes that operate over a wide range of spatial <span class="hlt">scales</span>; (iii) has greater replication than existing experiments; (iv) incorporates an experimental manipulation of riparian corridors; and (v) embeds the experimentally fragmented landscape within a wider gradient of land-use intensity than do existing projects. The SAFE Project represents an opportunity for ecologists across disciplines to participate in a <span class="hlt">large</span> initiative designed to generate a broad understanding of the ecological impacts of tropical forest modification. PMID:22006969</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016cosp...41E.765G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016cosp...41E.765G"><span>Moon-based Earth Observation for <span class="hlt">Large</span> <span class="hlt">Scale</span> Geoscience Phenomena</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Guo, Huadong; Liu, Guang; Ding, Yixing</p> <p>2016-07-01</p> <p>The capability of Earth observation for <span class="hlt">large-global-scale</span> natural phenomena needs to be improved and new observing platform are expected. We have studied the concept of Moon as an Earth observation in these years. Comparing with manmade satellite platform, Moon-based Earth observation can obtain multi-spherical, full-band, active and passive information,which is of following advantages: <span class="hlt">large</span> observation range, variable view angle, long-term continuous observation, extra-long life cycle, with the characteristics of longevity ,consistency, integrity, stability and uniqueness. Moon-based Earth observation is suitable for monitoring the <span class="hlt">large</span> <span class="hlt">scale</span> geoscience phenomena including <span class="hlt">large</span> <span class="hlt">scale</span> atmosphere change, <span class="hlt">large</span> <span class="hlt">scale</span> ocean change,<span class="hlt">large</span> <span class="hlt">scale</span> land surface dynamic change,solid earth dynamic change,etc. For the purpose of establishing a Moon-based Earth observation platform, we already have a plan to study the five aspects as follows: mechanism and models of moon-based observing earth sciences macroscopic phenomena; sensors' parameters optimization and methods of moon-based Earth observation; site selection and environment of moon-based Earth observation; Moon-based Earth observation platform; and Moon-based Earth observation fundamental scientific 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_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhRvL.119m6002M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhRvL.119m6002M"><span><span class="hlt">Large-Scale</span> Structure and Hyperuniformity of Amorphous Ices</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Martelli, Fausto; Torquato, Salvatore; Giovambattista, Nicolas; Car, Roberto</p> <p>2017-09-01</p> <p>We investigate the <span class="hlt">large-scale</span> structure of amorphous ices and transitions between their different forms by quantifying their <span class="hlt">large-scale</span> density fluctuations. Specifically, we simulate the isothermal compression of low-density amorphous ice (LDA) and hexagonal ice to produce high-density amorphous ice (HDA). Both HDA and LDA are nearly hyperuniform; i.e., they are characterized by an anomalous suppression of <span class="hlt">large-scale</span> density fluctuations. By contrast, in correspondence with the nonequilibrium phase transitions to HDA, the presence of structural heterogeneities strongly suppresses the hyperuniformity and the system becomes hyposurficial (devoid of "surface-area fluctuations"). Our investigation challenges the <span class="hlt">largely</span> accepted "frozen-liquid" picture, which views glasses as structurally arrested liquids. Beyond implications for water, our findings enrich our understanding of pressure-induced structural transformations in glasses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.A13B3157Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.A13B3157Q"><span>Improving the City-<span class="hlt">scale</span> Emission Inventory of Anthropogenic <span class="hlt">Air</span> Pollutants: A Case Study of Nanjing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qiu, L.; Zhao, Y.; Xu, R.; Xie, F.; Wang, H.; Qin, H.; Wu, X.; Zhang, J.</p> <p>2014-12-01</p> <p> inventory on industrial and transportation sources other than big power plants. Through the inventory evaluation, the necessity to develop high-resolution emission inventory with comprehensive emission source information is <span class="hlt">revealed</span> for atmospheric science studies and <span class="hlt">air</span> quality improvement at local <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1027672','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1027672"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Cross Drive Correlation Of Digital Media</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2016-03-01</p> <p>NAVAL POSTGRADUATE SCHOOL MONTEREY, CALIFORNIA THESIS <span class="hlt">LARGE</span> <span class="hlt">SCALE</span> CROSS-DRIVE CORRELATION OF DIGITAL MEDIA by Joseph Van Bruaene March 2016 Thesis Co...CROSS-DRIVE CORRELATION OF DIGITAL MEDIA 5. FUNDING NUMBERS 6. AUTHOR(S) Joseph Van Bruaene 7. PERFORMING ORGANIZATION NAME(S) AND ADDRESS(ES) Naval...the ability to make <span class="hlt">large</span> <span class="hlt">scale</span> cross-drive correlations among a <span class="hlt">large</span> corpus of digital media becomes increasingly important. We propose a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900057028&hterms=sampling+distribution&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsampling%2Bdistribution','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900057028&hterms=sampling+distribution&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dsampling%2Bdistribution"><span>The <span class="hlt">large-scale</span> distribution of galaxies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Geller, Margaret J.</p> <p>1989-01-01</p> <p>The spatial distribution of galaxies in the universe is characterized on the basis of the six completed strips of the Harvard-Smithsonian Center for Astrophysics redshift-survey extension. The design of the survey is briefly reviewed, and the results are presented graphically. Vast low-density voids similar to the void in Bootes are found, almost completely surrounded by thin sheets of galaxies. Also discussed are the implications of the results for the survey sampling problem, the two-point correlation function of the galaxy distribution, the possibility of detecting <span class="hlt">large-scale</span> coherent flows, theoretical models of <span class="hlt">large-scale</span> structure, and the identification of groups and clusters of galaxies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29546546','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29546546"><span>A guide to <span class="hlt">large-scale</span> RNA sample preparation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baronti, Lorenzo; Karlsson, Hampus; Marušič, Maja; Petzold, Katja</p> <p>2018-05-01</p> <p>RNA is becoming more important as an increasing number of functions, both regulatory and enzymatic, are being discovered on a daily basis. As the RNA boom has just begun, most techniques are still in development and changes occur frequently. To understand RNA functions, <span class="hlt">revealing</span> the structure of RNA is of utmost importance, which requires sample preparation. We review the latest methods to produce and purify a variation of RNA molecules for different purposes with the main focus on structural biology and biophysics. We present a guide aimed at identifying the most suitable method for your RNA and your biological question and highlighting the advantages of different methods. Graphical abstract In this review we present different methods for <span class="hlt">large-scale</span> production and purification of RNAs for structural and biophysical studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017A%26A...606A...9J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017A%26A...606A...9J"><span><span class="hlt">Large-scale</span> environments of narrow-line Seyfert 1 galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Järvelä, E.; Lähteenmäki, A.; Lietzen, H.; Poudel, A.; Heinämäki, P.; Einasto, M.</p> <p>2017-09-01</p> <p>Studying <span class="hlt">large-scale</span> environments of narrow-line Seyfert 1 (NLS1) galaxies gives a new perspective on their properties, particularly their radio loudness. The <span class="hlt">large-scale</span> environment is believed to have an impact on the evolution and intrinsic properties of galaxies, however, NLS1 sources have not been studied in this context before. We have a <span class="hlt">large</span> and diverse sample of 1341 NLS1 galaxies and three separate environment data sets constructed using Sloan Digital Sky Survey. We use various statistical methods to investigate how the properties of NLS1 galaxies are connected to the <span class="hlt">large-scale</span> environment, and compare the <span class="hlt">large-scale</span> environments of NLS1 galaxies with other active galactic nuclei (AGN) classes, for example, other jetted AGN and broad-line Seyfert 1 (BLS1) galaxies, to study how they are related. NLS1 galaxies reside in less dense environments than any of the comparison samples, thus confirming their young age. The average <span class="hlt">large-scale</span> environment density and environmental distribution of NLS1 sources is clearly different compared to BLS1 galaxies, thus it is improbable that they could be the parent population of NLS1 galaxies and unified by orientation. Within the NLS1 class there is a trend of increasing radio loudness with increasing <span class="hlt">large-scale</span> environment density, indicating that the <span class="hlt">large-scale</span> environment affects their intrinsic properties. Our results suggest that the NLS1 class of sources is not homogeneous, and furthermore, that a considerable fraction of them are misclassified. We further support a published proposal to replace the traditional classification to radio-loud, and radio-quiet or radio-silent sources with a division into jetted and non-jetted sources.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880036349&hterms=inflation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dinflation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880036349&hterms=inflation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dinflation"><span>Double inflation - A possible resolution of the <span class="hlt">large-scale</span> structure problem</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Turner, Michael S.; Villumsen, Jens V.; Vittorio, Nicola; Silk, Joseph; Juszkiewicz, Roman</p> <p>1987-01-01</p> <p>A model is presented for the <span class="hlt">large-scale</span> structure of the universe in which two successive inflationary phases resulted in <span class="hlt">large</span> small-<span class="hlt">scale</span> and small <span class="hlt">large-scale</span> density fluctuations. This bimodal density fluctuation spectrum in an Omega = 1 universe dominated by hot dark matter leads to <span class="hlt">large-scale</span> structure of the galaxy distribution that is consistent with recent observational results. In particular, <span class="hlt">large</span>, nearly empty voids and significant <span class="hlt">large-scale</span> peculiar velocity fields are produced over <span class="hlt">scales</span> of about 100 Mpc, while the small-<span class="hlt">scale</span> structure over less than about 10 Mpc resembles that in a low-density universe, as observed. Detailed analytical calculations and numerical simulations are given of the spatial and velocity correlations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH51C2497H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH51C2497H"><span>Measuring the <span class="hlt">Large-scale</span> Solar Magnetic Field</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hoeksema, J. T.; Scherrer, P. H.; Peterson, E.; Svalgaard, L.</p> <p>2017-12-01</p> <p>The Sun's <span class="hlt">large-scale</span> magnetic field is important for determining global structure of the corona and for quantifying the evolution of the polar field, which is sometimes used for predicting the strength of the next solar cycle. Having confidence in the determination of the <span class="hlt">large-scale</span> magnetic field of the Sun is difficult because the field is often near the detection limit, various observing methods all measure something a little different, and various systematic effects can be very important. We compare resolved and unresolved observations of the <span class="hlt">large-scale</span> magnetic field from the Wilcox Solar Observatory, Heliseismic and Magnetic Imager (HMI), Michelson Doppler Imager (MDI), and Solis. Cross comparison does not enable us to establish an absolute calibration, but it does allow us to discover and compensate for instrument problems, such as the sensitivity decrease seen in the WSO measurements in late 2016 and early 2017.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22233726','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22233726"><span>Spectral fingerprints of <span class="hlt">large-scale</span> neuronal interactions.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siegel, Markus; Donner, Tobias H; Engel, Andreas K</p> <p>2012-01-11</p> <p>Cognition results from interactions among functionally specialized but widely distributed brain regions; however, neuroscience has so far <span class="hlt">largely</span> focused on characterizing the function of individual brain regions and neurons therein. Here we discuss recent studies that have instead investigated the interactions between brain regions during cognitive processes by assessing correlations between neuronal oscillations in different regions of the primate cerebral cortex. These studies have opened a new window onto the <span class="hlt">large-scale</span> circuit mechanisms underlying sensorimotor decision-making and top-down attention. We propose that frequency-specific neuronal correlations in <span class="hlt">large-scale</span> cortical networks may be 'fingerprints' of canonical neuronal computations underlying cognitive processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016MNRAS.461..240B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016MNRAS.461..240B"><span>A unified <span class="hlt">large/small-scale</span> dynamo in helical turbulence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bhat, Pallavi; Subramanian, Kandaswamy; Brandenburg, Axel</p> <p>2016-09-01</p> <p>We use high resolution direct numerical simulations (DNS) to show that helical turbulence can generate significant <span class="hlt">large-scale</span> fields even in the presence of strong small-<span class="hlt">scale</span> dynamo action. During the kinematic stage, the unified <span class="hlt">large/small-scale</span> dynamo grows fields with a shape-invariant eigenfunction, with most power peaked at small <span class="hlt">scales</span> or <span class="hlt">large</span> k, as in Subramanian & Brandenburg. Nevertheless, the <span class="hlt">large-scale</span> field can be clearly detected as an excess power at small k in the negatively polarized component of the energy spectrum for a forcing with positively polarized waves. Its strength overline{B}, relative to the total rms field Brms, decreases with increasing magnetic Reynolds number, ReM. However, as the Lorentz force becomes important, the field generated by the unified dynamo orders itself by saturating on successively larger <span class="hlt">scales</span>. The magnetic integral <span class="hlt">scale</span> for the positively polarized waves, characterizing the small-<span class="hlt">scale</span> field, increases significantly from the kinematic stage to saturation. This implies that the small-<span class="hlt">scale</span> field becomes as coherent as possible for a given forcing <span class="hlt">scale</span>, which averts the ReM-dependent quenching of overline{B}/B_rms. These results are obtained for 10243 DNS with magnetic Prandtl numbers of PrM = 0.1 and 10. For PrM = 0.1, overline{B}/B_rms grows from about 0.04 to about 0.4 at saturation, aided in the final stages by helicity dissipation. For PrM = 10, overline{B}/B_rms grows from much less than 0.01 to values of the order the 0.2. Our results confirm that there is a unified <span class="hlt">large/small-scale</span> dynamo in helical turbulence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1996APS..DFD..EK06B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1996APS..DFD..EK06B"><span>Modulation of Small-<span class="hlt">scale</span> Turbulence Structure by <span class="hlt">Large-scale</span> Motions in the Absence of Direct Energy Transfer.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brasseur, James G.; Juneja, Anurag</p> <p>1996-11-01</p> <p>Previous DNS studies indicate that small-<span class="hlt">scale</span> structure can be directly altered through ``distant'' dynamical interactions by energetic forcing of the <span class="hlt">large</span> <span class="hlt">scales</span>. To remove the possibility of stimulating energy transfer between the <span class="hlt">large</span>- and small-<span class="hlt">scale</span> motions in these long-range interactions, we here perturb the <span class="hlt">large</span> <span class="hlt">scale</span> structure without altering its energy content by suddenly altering only the phases of <span class="hlt">large-scale</span> Fourier modes. <span class="hlt">Scale</span>-dependent changes in turbulence structure appear as a non zero difference field between two simulations from identical initial conditions of isotropic decaying turbulence, one perturbed and one unperturbed. We find that the <span class="hlt">large-scale</span> phase perturbations leave the evolution of the energy spectrum virtually unchanged relative to the unperturbed turbulence. The difference field, on the other hand, is strongly affected by the perturbation. Most importantly, the time <span class="hlt">scale</span> τ characterizing the change in in turbulence structure at spatial <span class="hlt">scale</span> r shortly after initiating a change in <span class="hlt">large-scale</span> structure decreases with decreasing turbulence <span class="hlt">scale</span> r. Thus, structural information is transferred directly from the <span class="hlt">large</span>- to the smallest-<span class="hlt">scale</span> motions in the absence of direct energy transfer---a long-range effect which cannot be explained by a linear mechanism such as rapid distortion theory. * Supported by ARO grant DAAL03-92-G-0117</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28798849','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28798849"><span>A small-<span class="hlt">scale</span>, rolled-membrane microfluidic artificial lung designed towards future <span class="hlt">large</span> area manufacturing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Thompson, A J; Marks, L H; Goudie, M J; Rojas-Pena, A; Handa, H; Potkay, J A</p> <p>2017-03-01</p> <p>Artificial lungs have been used in the clinic for multiple decades to supplement patient pulmonary function. Recently, small-<span class="hlt">scale</span> microfluidic artificial lungs (μAL) have been demonstrated with <span class="hlt">large</span> surface area to blood volume ratios, biomimetic blood flow paths, and pressure drops compatible with pumpless operation. Initial small-<span class="hlt">scale</span> microfluidic devices with blood flow rates in the μ l/min to ml/min range have exhibited excellent gas transfer efficiencies; however, current manufacturing techniques may not be suitable for <span class="hlt">scaling</span> up to human applications. Here, we present a new manufacturing technology for a microfluidic artificial lung in which the structure is assembled via a continuous "rolling" and bonding procedure from a single, patterned layer of polydimethyl siloxane (PDMS). This method is demonstrated in a small-<span class="hlt">scale</span> four-layer device, but is expected to easily <span class="hlt">scale</span> to larger area devices. The presented devices have a biomimetic branching blood flow network, 10  μ m tall artificial capillaries, and a 66  μ m thick gas transfer membrane. Gas transfer efficiency in blood was evaluated over a range of blood flow rates (0.1-1.25 ml/min) for two different sweep gases (pure O 2 , atmospheric <span class="hlt">air</span>). The achieved gas transfer data closely follow predicted theoretical values for oxygenation and CO 2 removal, while pressure drop is marginally higher than predicted. This work is the first step in developing a scalable method for creating <span class="hlt">large</span> area microfluidic artificial lungs. Although designed for microfluidic artificial lungs, the presented technique is expected to result in the first manufacturing method capable of simply and easily creating <span class="hlt">large</span> area microfluidic devices from PDMS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED214303.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED214303.pdf"><span>A Functional Model for Management of <span class="hlt">Large</span> <span class="hlt">Scale</span> Assessments.</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>Banta, Trudy W.; And Others</p> <p></p> <p>This functional model for managing <span class="hlt">large-scale</span> program evaluations was developed and validated in connection with the assessment of Tennessee's Nutrition Education and Training Program. Management of such a <span class="hlt">large-scale</span> assessment requires the development of a structure for the organization; distribution and recovery of <span class="hlt">large</span> quantities of…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19860014611','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19860014611"><span>Current Scientific Issues in <span class="hlt">Large</span> <span class="hlt">Scale</span> Atmospheric Dynamics</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, T. L. (Compiler)</p> <p>1986-01-01</p> <p>Topics in <span class="hlt">large</span> <span class="hlt">scale</span> atmospheric dynamics are discussed. Aspects of atmospheric blocking, the influence of transient baroclinic eddies on planetary-<span class="hlt">scale</span> waves, cyclogenesis, the effects of orography on planetary <span class="hlt">scale</span> flow, small <span class="hlt">scale</span> frontal structure, and simulations of gravity waves in frontal zones are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/54999','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/54999"><span>Lichen elemental content bioindicators for <span class="hlt">air</span> quality in upper Midwest, USA: A model for <span class="hlt">large-scale</span> monitoring</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Susan Will-Wolf; Sarah Jovan; Michael C. Amacher</p> <p>2017-01-01</p> <p>Our development of lichen elemental bioindicators for a United States of America (USA) national monitoring program is a useful model for other <span class="hlt">large-scale</span> programs. Concentrations of 20 elements were measured, validated, and analyzed for 203 samples of five common lichen species. Collections were made by trained non-specialists near 75 permanent plots and an expert...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5187734','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5187734"><span>Unfolding <span class="hlt">large-scale</span> online collaborative human dynamics</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Zha, Yilong; Zhou, Tao; Zhou, Changsong</p> <p>2016-01-01</p> <p><span class="hlt">Large-scale</span> interacting human activities underlie all social and economic phenomena, but quantitative understanding of regular patterns and mechanism is very challenging and still rare. Self-organized online collaborative activities with a precise record of event timing provide unprecedented opportunity. Our empirical analysis of the history of millions of updates in Wikipedia shows a universal double–power-law distribution of time intervals between consecutive updates of an article. We then propose a generic model to unfold collaborative human activities into three modules: (i) individual behavior characterized by Poissonian initiation of an action, (ii) human interaction captured by a cascading response to previous actions with a power-law waiting time, and (iii) population growth due to the increasing number of interacting individuals. This unfolding allows us to obtain an analytical formula that is fully supported by the universal patterns in empirical data. Our modeling approaches <span class="hlt">reveal</span> “simplicity” beyond complex interacting human activities. PMID:27911766</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1997PhDT........66L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1997PhDT........66L"><span>Climate dynamics of South America during summer: Connections between the <span class="hlt">large-scale</span> circulation and regional precipitation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lenters, Johh Derick</p> <p>1997-05-01</p> <p>Relationships between the <span class="hlt">large-scale</span> circulation and regional precipitation over South America during austral summer are examined using a GCM, linear model, and observational analyses. Emphasis is placed on understanding the origin of upper-tropospheric circulation features such as the Bolivian high and its effects on South American precipitation variability, particularly on the Central Andean Altiplano. Results from the linear model indicate that the Bolivian high and 'Nordeste low' are generated in response to precipitation over the Amazon basin, Central Andes, and South Atlantic convergence zone (SACZ), with African precipitation also playing a crucial role in the formation of the low. The direct mechanical and sensible heating effects of the Andes are minimal, acting only to induce a weak lee trough in midlatitudes and a shallow monsoonal circulation over the Central Andes. In the GCM the effects of the Andes include a strengthening of the Bolivian high and northward shift of the Nordeste low, primarily through changes in the precipitation field. The position of the Bolivian high is primarily determined by Amazonian precipitation and is little affected by the removal of the Andes. Strong subsidence to the west of the high is found to be important for the maintenance of the high's warm core, while <span class="hlt">large-scale</span> convective overshooting to the east is responsible for a layer of cold <span class="hlt">air</span> above the high. Observations from eight summer seasons <span class="hlt">reveal</span> a close relationship between precipitation variability in the Central Andes and the position and intensity of the Bolivian high. The physical mechanisms of this connection are explored using composite, EOF, and correlation techniques. On intraseasonal to interannual timescales, rainy episodes on the Altiplano are found to be associated with warm, moist, poleward flow along the eastern flank of the Andes, often in conjunction with extratropical disturbances and a westward displacement of the SACZ. Corresponding to this</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=149943&keyword=space+AND+weather&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=149943&keyword=space+AND+weather&actType=&TIMSType=+&TIMSSubTypeID=&DEID=&epaNumber=&ntisID=&archiveStatus=Both&ombCat=Any&dateBeginCreated=&dateEndCreated=&dateBeginPublishedPresented=&dateEndPublishedPresented=&dateBeginUpdated=&dateEndUpdated=&dateBeginCompleted=&dateEndCompleted=&personID=&role=Any&journalID=&publisherID=&sortBy=revisionDate&count=50"><span>USE OF REMOTE SENSING <span class="hlt">AIR</span> QUALITY INFORMATION IN REGIONAL <span class="hlt">SCALE</span> <span class="hlt">AIR</span> POLLUTION MODELING: CURRENT USE AND REQUIREMENTS</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>In recent years the applications of regional <span class="hlt">air</span> quality models are continuously being extended to address atmospheric pollution phenomenon from local to hemispheric spatial <span class="hlt">scales</span> over time <span class="hlt">scales</span> ranging from episodic to annual. The need to represent interactions between physic...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19990051020','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19990051020"><span>Condition Monitoring of <span class="hlt">Large-Scale</span> Facilities</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hall, David L.</p> <p>1999-01-01</p> <p>This document provides a summary of the research conducted for the NASA Ames Research Center under grant NAG2-1182 (Condition-Based Monitoring of <span class="hlt">Large-Scale</span> Facilities). The information includes copies of view graphs presented at NASA Ames in the final Workshop (held during December of 1998), as well as a copy of a technical report provided to the COTR (Dr. Anne Patterson-Hine) subsequent to the workshop. The material describes the experimental design, collection of data, and analysis results associated with monitoring the health of <span class="hlt">large-scale</span> facilities. In addition to this material, a copy of the Pennsylvania State University Applied Research Laboratory data fusion visual programming tool kit was also provided to NASA Ames researchers.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E%26ES...84a2042M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E%26ES...84a2042M"><span>Seismic safety in conducting <span class="hlt">large-scale</span> blasts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mashukov, I. V.; Chaplygin, V. V.; Domanov, V. P.; Semin, A. A.; Klimkin, M. A.</p> <p>2017-09-01</p> <p>In mining enterprises to prepare hard rocks for excavation a drilling and blasting method is used. With the approach of mining operations to settlements the negative effect of <span class="hlt">large-scale</span> blasts increases. To assess the level of seismic impact of <span class="hlt">large-scale</span> blasts the scientific staff of Siberian State Industrial University carried out expertise for coal mines and iron ore enterprises. Determination of the magnitude of surface seismic vibrations caused by mass explosions was performed using seismic receivers, an analog-digital converter with recording on a laptop. The registration results of surface seismic vibrations during production of more than 280 <span class="hlt">large-scale</span> blasts at 17 mining enterprises in 22 settlements are presented. The maximum velocity values of the Earth’s surface vibrations are determined. The safety evaluation of seismic effect was carried out according to the permissible value of vibration velocity. For cases with exceedance of permissible values recommendations were developed to reduce the level of seismic impact.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22689510-micro-environmental-impact-volatile-organic-compound-emissions-from-large-scale-assemblies-people-confined-space','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22689510-micro-environmental-impact-volatile-organic-compound-emissions-from-large-scale-assemblies-people-confined-space"><span>The micro-environmental impact of volatile organic compound emissions from <span class="hlt">large-scale</span> assemblies of people in a confined space</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>Dutta, Tanushree</p> <p></p> <p><span class="hlt">Large-scale</span> assemblies of people in a confined space can exert significant impacts on the local <span class="hlt">air</span> chemistry due to human emissions of volatile organics. Variations of <span class="hlt">air</span>-quality in such small <span class="hlt">scale</span> can be studied by quantifying fingerprint volatile organic compounds (VOCs) such as acetone, toluene, and isoprene produced during concerts, movie screenings, and sport events (like the Olympics and the World Cup). This review summarizes the extent of VOC accumulation resulting from a <span class="hlt">large</span> population in a confined area or in a small open area during sporting and other recreational activities. Apart from VOCs emitted directly from human bodies (e.g.,more » perspiration and exhaled breath), those released indirectly from other related sources (e.g., smoking, waste disposal, discharge of food-waste, and use of personal-care products) are also discussed. Although direct and indirect emissions of VOCs from human may constitute <1% of the global atmospheric VOCs budget, unique spatiotemporal variations in VOCs species within a confined space can have unforeseen impacts on the local atmosphere to lead to acute human exposure to harmful pollutants.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014E%26ES...22e2024R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014E%26ES...22e2024R"><span>Mitigation of tip vortex cavitation by means of <span class="hlt">air</span> injection on a Kaplan turbine <span class="hlt">scale</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>Rivetti, A.; Angulo, M.; Lucino, C.; Liscia, S.</p> <p>2014-03-01</p> <p>Kaplan turbines operating at full-load conditions may undergo excessive vibration, noise and cavitation. In such cases, damage by erosion associated to tip vortex cavitation can be observed at the discharge ring. This phenomenon involves design features such as (1) overhang of guide vanes; (2) blade profile; (3) gap increasing size with blade opening; (4) suction head; (5) operation point; and (6) discharge ring stiffness, among others. Tip vortex cavitation may cause erosion at the discharge ring and draft tube inlet following a wavy pattern, in which the number of vanes can be clearly identified. Injection of pressurized <span class="hlt">air</span> above the runner blade centerline was tested as a mean to mitigate discharge ring cavitation damage on a <span class="hlt">scale</span> model. <span class="hlt">Air</span> entrance was observed by means of a high-speed camera in order to track the <span class="hlt">air</span> trajectory toward its mergence with the tip vortex cavitation core. Post-processing of acceleration signals shows that the level of vibration and the RSI frequency amplitude decrease proportionally with <span class="hlt">air</span> flow rate injected. These findings <span class="hlt">reveal</span> the potential mitigating effect of <span class="hlt">air</span> injection in preventing cavitation damage and will be useful in further tests to be performed on prototype, aiming at determining the optimum <span class="hlt">air</span> flow rate, size and distribution of the injectors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ems..confE.819N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ems..confE.819N"><span>Downscaling modelling system for multi-<span class="hlt">scale</span> <span class="hlt">air</span> quality forecasting</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nuterman, R.; Baklanov, A.; Mahura, A.; Amstrup, B.; Weismann, J.</p> <p>2010-09-01</p> <p>Urban modelling for real meteorological situations, in general, considers only a small part of the urban area in a micro-meteorological model, and urban heterogeneities outside a modelling domain affect micro-<span class="hlt">scale</span> processes. Therefore, it is important to build a chain of models of different <span class="hlt">scales</span> with nesting of higher resolution models into larger <span class="hlt">scale</span> lower resolution models. Usually, the up-<span class="hlt">scaled</span> city- or meso-<span class="hlt">scale</span> models consider parameterisations of urban effects or statistical descriptions of the urban morphology, whereas the micro-<span class="hlt">scale</span> (street canyon) models are obstacle-resolved and they consider a detailed geometry of the buildings and the urban canopy. The developed system consists of the meso-, urban- and street-<span class="hlt">scale</span> models. First, it is the Numerical Weather Prediction (HIgh Resolution Limited Area Model) model combined with Atmospheric Chemistry Transport (the Comprehensive <span class="hlt">Air</span> quality Model with extensions) model. Several levels of urban parameterisation are considered. They are chosen depending on selected <span class="hlt">scales</span> and resolutions. For regional <span class="hlt">scale</span>, the urban parameterisation is based on the roughness and flux corrections approach; for urban <span class="hlt">scale</span> - building effects parameterisation. Modern methods of computational fluid dynamics allow solving environmental problems connected with atmospheric transport of pollutants within urban canopy in a presence of penetrable (vegetation) and impenetrable (buildings) obstacles. For local- and micro-<span class="hlt">scales</span> nesting the Micro-<span class="hlt">scale</span> Model for Urban Environment is applied. This is a comprehensive obstacle-resolved urban wind-flow and dispersion model based on the Reynolds averaged Navier-Stokes approach and several turbulent closures, i.e. k -ɛ linear eddy-viscosity model, k - ɛ non-linear eddy-viscosity model and Reynolds stress model. Boundary and initial conditions for the micro-<span class="hlt">scale</span> model are used from the up-<span class="hlt">scaled</span> models with corresponding interpolation conserving the mass. For the boundaries a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70012121','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70012121"><span>Potential for geophysical experiments in <span class="hlt">large</span> <span class="hlt">scale</span> tests.</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Dieterich, J.H.</p> <p>1981-01-01</p> <p>Potential research applications for <span class="hlt">large</span>-specimen geophysical experiments include measurements of <span class="hlt">scale</span> dependence of physical parameters and examination of interactions with heterogeneities, especially flaws such as cracks. In addition, increased specimen size provides opportunities for improved recording resolution and greater control of experimental variables. <span class="hlt">Large-scale</span> experiments using a special purpose low stress (100MPa).-Author</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1171U','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1171U"><span>Disruption of circumstellar discs by <span class="hlt">large-scale</span> stellar magnetic fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>ud-Doula, Asif; Owocki, Stanley P.; Kee, Nathaniel Dylan</p> <p>2018-05-01</p> <p>Spectropolarimetric surveys <span class="hlt">reveal</span> that 8-10% of OBA stars harbor <span class="hlt">large-scale</span> magnetic fields, but thus far no such fields have been detected in any classical Be stars. Motivated by this, we present here MHD simulations for how a pre-existing Keplerian disc - like that inferred to form from decretion of material from rapidly rotating Be stars - can be disrupted by a rotation-aligned stellar dipole field. For characteristic stellar and disc parameters of a near-critically rotating B2e star, we find that a polar surface field strength of just 10 G can significantly disrupt the disc, while a field of 100 G, near the observational upper limit inferred for most Be stars, completely destroys the disc over just a few days. Our parameter study shows that the efficacy of this magnetic disruption of a disc <span class="hlt">scales</span> with the characteristic plasma beta (defined as the ratio between thermal and magnetic pressure) in the disc, but is surprisingly insensitive to other variations, e.g. in stellar rotation speed, or the mass loss rate of the star's radiatively driven wind. The disc disruption seen here for even a modest field strength suggests that the presumed formation of such Be discs by decretion of material from the star would likely be strongly inhibited by such fields; this provides an attractive explanation for why no <span class="hlt">large-scale</span> fields are detected from such Be stars.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5362049','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5362049"><span>Multimodal MR-imaging <span class="hlt">reveals</span> <span class="hlt">large-scale</span> structural and functional connectivity changes in profound early blindness</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Bauer, Corinna M.; Hirsch, Gabriella V.; Zajac, Lauren; Koo, Bang-Bon; Collignon, Olivier</p> <p>2017-01-01</p> <p> between occipital and frontal and somatosensory-motor areas and between temporal (mainly fusiform and parahippocampus) and parietal, frontal, and other temporal areas. Correlations in white matter connectivity and functional connectivity observed between early blind and sighted controls showed an overall high degree of association. However, comparing the relative changes in white matter and functional connectivity between early blind and sighted controls did not show a significant correlation. In summary, these findings provide complimentary evidence, as well as highlight potential contradictions, regarding the nature of regional and <span class="hlt">large</span> <span class="hlt">scale</span> neuroplastic reorganization resulting from early onset blindness. PMID:28328939</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70034432','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70034432"><span>Homogenization of <span class="hlt">Large-Scale</span> Movement Models in Ecology</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Garlick, M.J.; Powell, J.A.; Hooten, M.B.; McFarlane, L.R.</p> <p>2011-01-01</p> <p>A difficulty in using diffusion models to predict <span class="hlt">large</span> <span class="hlt">scale</span> animal population dispersal is that individuals move differently based on local information (as opposed to gradients) in differing habitat types. This can be accommodated by using ecological diffusion. However, real environments are often spatially complex, limiting application of a direct approach. Homogenization for partial differential equations has long been applied to Fickian diffusion (in which average individual movement is organized along gradients of habitat and population density). We derive a homogenization procedure for ecological diffusion and apply it to a simple model for chronic wasting disease in mule deer. Homogenization allows us to determine the impact of small <span class="hlt">scale</span> (10-100 m) habitat variability on <span class="hlt">large</span> <span class="hlt">scale</span> (10-100 km) movement. The procedure generates asymptotic equations for solutions on the <span class="hlt">large</span> <span class="hlt">scale</span> with parameters defined by small-<span class="hlt">scale</span> variation. The simplicity of this homogenization procedure is striking when compared to the multi-dimensional homogenization procedure for Fickian diffusion,and the method will be equally straightforward for more complex models. ?? 2010 Society for Mathematical Biology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26741542','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26741542"><span>Ceramic membrane defouling (cleaning) by <span class="hlt">air</span> Nano Bubbles.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ghadimkhani, Aliasghar; Zhang, Wen; Marhaba, Taha</p> <p>2016-03-01</p> <p>Ceramic membranes are among the most promising technologies for membrane applications, owing to their excellent resistance to mechanical, chemical, and thermal stresses. However, membrane fouling is still an issue that hampers the applications at <span class="hlt">large</span> <span class="hlt">scales</span>. <span class="hlt">Air</span> Nano Bubbles (NBs), due to high mass transfer efficiency, could potentially prevent fouling of ceramic membrane filtration processes. In this study, bench and pilot <span class="hlt">scale</span> ceramic membrane filtration was performed with <span class="hlt">air</span> NBs to resist fouling. To simulate fouling, humic acid, as an organic foulant, was applied to the membrane flat sheet surface. Complete membrane clogging was achieved in less than 6 h. Membrane defouling (cleaning) was performed by directly feeding of <span class="hlt">air</span> NBs to the membrane cells. The surface of the ceramic membrane was superbly cleaned by <span class="hlt">air</span> NBs, as <span class="hlt">revealed</span> by atomic force microscope (AFM) images before and after the treatment. The permeate flux recovered to its initial level (e.g., 26.7 × 10(-9) m(3)/m(2)/s at applied pressure of 275.8 kPa), which indicated that NBs successfully unclogged the pores of the membrane. The integrated ceramic membrane and <span class="hlt">air</span> NBs system holds potential as an innovative sustainable technology. Copyright © 2015 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2000Natur.407..651J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2000Natur.407..651J"><span>The <span class="hlt">large-scale</span> organization of metabolic networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jeong, H.; Tombor, B.; Albert, R.; Oltvai, Z. N.; Barabási, A.-L.</p> <p>2000-10-01</p> <p>In a cell or microorganism, the processes that generate mass, energy, information transfer and cell-fate specification are seamlessly integrated through a complex network of cellular constituents and reactions. However, despite the key role of these networks in sustaining cellular functions, their <span class="hlt">large-scale</span> structure is essentially unknown. Here we present a systematic comparative mathematical analysis of the metabolic networks of 43 organisms representing all three domains of life. We show that, despite significant variation in their individual constituents and pathways, these metabolic networks have the same topological <span class="hlt">scaling</span> properties and show striking similarities to the inherent organization of complex non-biological systems. This may indicate that metabolic organization is not only identical for all living organisms, but also complies with the design principles of robust and error-tolerant <span class="hlt">scale</span>-free networks, and may represent a common blueprint for the <span class="hlt">large-scale</span> organization of interactions among all cellular constituents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JAP...122e4901S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JAP...122e4901S"><span><span class="hlt">Scaling</span> beta-delayed neutron measurements to <span class="hlt">large</span> detector areas</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sutanto, F.; Nattress, J.; Jovanovic, I.</p> <p>2017-08-01</p> <p>We explore the performance of a cargo screening system that consists of two <span class="hlt">large</span>-sized composite scintillation detectors and a high-energy neutron interrogation source by modeling and simulation. The goal of the system is to measure β-delayed neutron emission from an illicit special nuclear material by use of active interrogation. This task is challenging because the β-delayed neutron yield is small in comparison with the yield of the prompt fission secondary products, β-delayed neutrons are emitted with relatively low energies, and high neutron and gamma backgrounds are typically present. Detectors used to measure delayed neutron emission must exhibit high intrinsic efficiency and cover a <span class="hlt">large</span> solid angle, which also makes them sensitive to background neutron radiation. We present a case study where we attempt to detect the presence of 5 kg-<span class="hlt">scale</span> quantities of 235U in a standard <span class="hlt">air</span>-filled cargo container using 14 MeV neutrons as a probe. We find that by using a total measurement time of ˜11.6 s and a dose equivalent of ˜1.7 mrem, the presence of 235U can be detected with false positive and false negative probabilities that are both no larger than 0.1%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25643405','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25643405"><span><span class="hlt">Large-scale</span> weakly supervised object localization via latent category learning.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chong Wang; Kaiqi Huang; Weiqiang Ren; Junge Zhang; Maybank, Steve</p> <p>2015-04-01</p> <p>Localizing objects in cluttered backgrounds is challenging under <span class="hlt">large-scale</span> weakly supervised conditions. Due to the cluttered image condition, objects usually have <span class="hlt">large</span> ambiguity with backgrounds. Besides, there is also a lack of effective algorithm for <span class="hlt">large-scale</span> weakly supervised localization in cluttered backgrounds. However, backgrounds contain useful latent information, e.g., the sky in the aeroplane class. If this latent information can be learned, object-background ambiguity can be <span class="hlt">largely</span> reduced and background can be suppressed effectively. In this paper, we propose the latent category learning (LCL) in <span class="hlt">large-scale</span> cluttered conditions. LCL is an unsupervised learning method which requires only image-level class labels. First, we use the latent semantic analysis with semantic object representation to learn the latent categories, which represent objects, object parts or backgrounds. Second, to determine which category contains the target object, we propose a category selection strategy by evaluating each category's discrimination. Finally, we propose the online LCL for use in <span class="hlt">large-scale</span> conditions. Evaluation on the challenging PASCAL Visual Object Class (VOC) 2007 and the <span class="hlt">large-scale</span> imagenet <span class="hlt">large-scale</span> visual recognition challenge 2013 detection data sets shows that the method can improve the annotation precision by 10% over previous methods. More importantly, we achieve the detection precision which outperforms previous results by a <span class="hlt">large</span> margin and can be competitive to the supervised deformable part model 5.0 baseline on both data sets.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009ClDy...33..843C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009ClDy...33..843C"><span>A revised method of presenting wavenumber-frequency power spectrum diagrams that <span class="hlt">reveals</span> the asymmetric nature of tropical <span class="hlt">large-scale</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>Chao, Winston C.; Yang, Bo; Fu, Xiouhua</p> <p>2009-11-01</p> <p>The popular method of presenting wavenumber-frequency power spectrum diagrams for studying tropical <span class="hlt">large-scale</span> waves in the literature is shown to give an incomplete presentation of these waves. The so-called “convectively coupled Kelvin (mixed Rossby-gravity) waves” are presented as existing only in the symmetric (anti-symmetric) component of the diagrams. This is obviously not consistent with the published composite/regression studies of “convectively coupled Kelvin waves,” which illustrate the asymmetric nature of these waves. The cause of this inconsistency is <span class="hlt">revealed</span> in this note and a revised method of presenting the power spectrum diagrams is proposed. When this revised method is used, “convectively coupled Kelvin waves” do show anti-symmetric components, and “convectively coupled mixed Rossby-gravity waves (also known as Yanai waves)” do show a hint of symmetric components. These results bolster a published proposal that these waves should be called “chimeric Kelvin waves,” “chimeric mixed Rossby-gravity waves,” etc. This revised method of presenting power spectrum diagrams offers an additional means of comparing the GCM output with observations by calling attention to the capability of GCMs to correctly simulate the asymmetric characteristics of equatorial waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........38H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........38H"><span>Composite and case study analyses of the <span class="hlt">large-scale</span> environments associated with West Pacific Polar and subtropical vertical jet superposition events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Handlos, Zachary J.</p> <p></p> <p>Though considerable research attention has been devoted to examination of the Northern Hemispheric polar and subtropical jet streams, relatively little has been directed toward understanding the circumstances that conspire to produce the relatively rare vertical superposition of these usually separate features. This dissertation investigates the structure and evolution of <span class="hlt">large-scale</span> environments associated with jet superposition events in the northwest Pacific. An objective identification scheme, using NCEP/NCAR Reanalysis 1 data, is employed to identify all jet superpositions in the west Pacific (30-40°N, 135-175°E) for boreal winters (DJF) between 1979/80 - 2009/10. The analysis <span class="hlt">reveals</span> that environments conducive to west Pacific jet superposition share several <span class="hlt">large-scale</span> features usually associated with East Asian Winter Monsoon (EAWM) northerly cold surges, including the presence of an enhanced Hadley Cell-like circulation within the jet entrance region. It is further demonstrated that several EAWM indices are statistically significantly correlated with jet superposition frequency in the west Pacific. The life cycle of EAWM cold surges promotes interaction between tropical convection and internal jet dynamics. Low potential vorticity (PV), high theta e tropical boundary layer <span class="hlt">air</span>, exhausted by anomalous convection in the west Pacific lower latitudes, is advected poleward towards the equatorward side of the jet in upper tropospheric isentropic layers resulting in anomalous anticyclonic wind shear that accelerates the jet. This, along with geostrophic cold <span class="hlt">air</span> advection in the left jet entrance region that drives the polar tropopause downward through the jet core, promotes the development of the deep, vertical PV wall characteristic of superposed jets. West Pacific jet superpositions preferentially form within an environment favoring the aforementioned characteristics regardless of EAWM seasonal strength. Post-superposition, it is shown that the west Pacific</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MS%26E..322e2057M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MS%26E..322e2057M"><span>An Novel Architecture of <span class="hlt">Large-scale</span> Communication in IOT</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ma, Wubin; Deng, Su; Huang, Hongbin</p> <p>2018-03-01</p> <p>In recent years, many scholars have done a great deal of research on the development of Internet of Things and networked physical systems. However, few people have made the detailed visualization of the <span class="hlt">large-scale</span> communications architecture in the IOT. In fact, the non-uniform technology between IPv6 and access points has led to a lack of broad principles of <span class="hlt">large-scale</span> communications architectures. Therefore, this paper presents the Uni-IPv6 Access and Information Exchange Method (UAIEM), a new architecture and algorithm that addresses <span class="hlt">large-scale</span> communications in the IOT.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10491E..0CH','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10491E..0CH"><span>1 million-Q optomechanical microdisk resonators for sensing with very <span class="hlt">large</span> <span class="hlt">scale</span> integration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hermouet, M.; Sansa, M.; Banniard, L.; Fafin, A.; Gely, M.; Allain, P. E.; Santos, E. Gil; Favero, I.; Alava, T.; Jourdan, G.; Hentz, S.</p> <p>2018-02-01</p> <p>Cavity optomechanics have become a promising route towards the development of ultrasensitive sensors for a wide range of applications including mass, chemical and biological sensing. In this study, we demonstrate the potential of Very <span class="hlt">Large</span> <span class="hlt">Scale</span> Integration (VLSI) with state-of-the-art low-loss performance silicon optomechanical microdisks for sensing applications. We report microdisks exhibiting optical Whispering Gallery Modes (WGM) with 1 million quality factors, yielding high displacement sensitivity and strong coupling between optical WGMs and in-plane mechanical Radial Breathing Modes (RBM). Such high-Q microdisks with mechanical resonance frequencies in the 102 MHz range were fabricated on 200 mm wafers with Variable Shape Electron Beam lithography. Benefiting from ultrasensitive readout, their Brownian motion could be resolved with good Signal-to-Noise ratio at ambient pressure, as well as in liquid, despite high frequency operation and <span class="hlt">large</span> fluidic damping: the mechanical quality factor reduced from few 103 in <span class="hlt">air</span> to 10's in liquid, and the mechanical resonance frequency shifted down by a few percent. Proceeding one step further, we performed an all-optical operation of the resonators in <span class="hlt">air</span> using a pump-probe scheme. Our results show our VLSI process is a viable approach for the next generation of sensors operating in vacuum, gas or liquid phase.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19880062376&hterms=gravitational+lensing&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dgravitational%2Blensing','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19880062376&hterms=gravitational+lensing&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dgravitational%2Blensing"><span>Gravitational lenses and <span class="hlt">large</span> <span class="hlt">scale</span> structure</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Turner, Edwin L.</p> <p>1987-01-01</p> <p>Four possible statistical tests of the <span class="hlt">large</span> <span class="hlt">scale</span> distribution of cosmic material are described. Each is based on gravitational lensing effects. The current observational status of these tests is also summarized.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/EJ1071344.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/EJ1071344.pdf"><span><span class="hlt">Large-Scale</span> 1:1 Computing Initiatives: An Open Access Database</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>Richardson, Jayson W.; McLeod, Scott; Flora, Kevin; Sauers, Nick J.; Kannan, Sathiamoorthy; Sincar, Mehmet</p> <p>2013-01-01</p> <p>This article details the spread and scope of <span class="hlt">large-scale</span> 1:1 computing initiatives around the world. What follows is a review of the existing literature around 1:1 programs followed by a description of the <span class="hlt">large-scale</span> 1:1 database. Main findings include: 1) the XO and the Classmate PC dominate <span class="hlt">large-scale</span> 1:1 initiatives; 2) if professional…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhyA..495...40Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhyA..495...40Z"><span>Spatiotemporal property and predictability of <span class="hlt">large-scale</span> human mobility</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Hai-Tao; Zhu, Tao; Fu, Dongfei; Xu, Bowen; Han, Xiao-Pu; Chen, Duxin</p> <p>2018-04-01</p> <p>Spatiotemporal characteristics of human mobility emerging from complexity on individual <span class="hlt">scale</span> have been extensively studied due to the application potential on human behavior prediction and recommendation, and control of epidemic spreading. We collect and investigate a comprehensive data set of human activities on <span class="hlt">large</span> geographical <span class="hlt">scales</span>, including both websites browse and mobile towers visit. Numerical results show that the degree of activity decays as a power law, indicating that human behaviors are reminiscent of <span class="hlt">scale</span>-free random walks known as Lévy flight. More significantly, this study suggests that human activities on <span class="hlt">large</span> geographical <span class="hlt">scales</span> have specific non-Markovian characteristics, such as a two-segment power-law distribution of dwelling time and a high possibility for prediction. Furthermore, a <span class="hlt">scale</span>-free featured mobility model with two essential ingredients, i.e., preferential return and exploration, and a Gaussian distribution assumption on the exploration tendency parameter is proposed, which outperforms existing human mobility models under scenarios of <span class="hlt">large</span> geographical <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/37997','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/37997"><span>Wedge measures parallax separations...on <span class="hlt">large-scale</span> 70-mm</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Steven L. Wert; Richard J. Myhre</p> <p>1967-01-01</p> <p>A new parallax wedge (range: 1.5 to 2 inches) has been designed for use with <span class="hlt">large-scaled</span> 70-mm. aerial photographs. The narrow separation of the wedge allows the user to measure small parallax separations that are characteristic of <span class="hlt">large-scale</span> photographs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160007964','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160007964"><span>Semantic Representation and <span class="hlt">Scale</span>-Up of Integrated <span class="hlt">Air</span> Traffic Management Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Keller, Richard M.; Ranjan, Shubha; Wei, Mei Y.; Eshow, Michelle M.</p> <p>2016-01-01</p> <p>Each day, the global <span class="hlt">air</span> transportation industry generates a vast amount of heterogeneous data from <span class="hlt">air</span> carriers, <span class="hlt">air</span> traffic control providers, and secondary aviation entities handling baggage, ticketing, catering, fuel delivery, and other services. Generally, these data are stored in isolated data systems, separated from each other by significant political, regulatory, economic, and technological divides. These realities aside, integrating aviation data into a single, queryable, big data store could enable insights leading to major efficiency, safety, and cost advantages. In this paper, we describe an implemented system for combining heterogeneous <span class="hlt">air</span> traffic management data using semantic integration techniques. The system transforms data from its original disparate source formats into a unified semantic representation within an ontology-based triple store. Our initial prototype stores only a small sliver of <span class="hlt">air</span> traffic data covering one day of operations at a major airport. The paper also describes our analysis of difficulties ahead as we prepare to <span class="hlt">scale</span> up data storage to accommodate successively larger quantities of data -- eventually covering all US commercial domestic flights over an extended multi-year timeframe. We review several approaches to mitigating <span class="hlt">scale</span>-up related query performance concerns.</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.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5318284','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5318284"><span>Retinotopic patterns of functional connectivity between V1 and <span class="hlt">large-scale</span> brain networks during resting fixation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Griffis, Joseph C.; Elkhetali, Abdurahman S.; Burge, Wesley K.; Chen, Richard H.; Bowman, Anthony D.; Szaflarski, Jerzy P.; Visscher, Kristina M.</p> <p>2016-01-01</p> <p>Psychophysical and neurobiological evidence suggests that central and peripheral vision are specialized for different functions. This specialization of function might be expected to lead to differences in the <span class="hlt">large-scale</span> functional interactions of early cortical areas that represent central and peripheral visual space. Here, we characterize differences in whole-brain functional connectivity among sectors in primary visual cortex (V1) corresponding to central, near-peripheral, and far-peripheral vision during resting fixation. Importantly, our analyses <span class="hlt">reveal</span> that eccentricity sectors in V1 have different functional connectivity with non-visual areas associated with <span class="hlt">large-scale</span> brain networks. Regions associated with the fronto-parietal control network are most strongly connected with central sectors of V1, regions associated with the cingulo-opercular control network are most strongly connected with near-peripheral sectors of V1, and regions associated with the default mode and auditory networks are most strongly connected with far-peripheral sectors of V1. Additional analyses suggest that similar patterns are present during eyes-closed rest. These results suggest that different types of visual information may be prioritized by <span class="hlt">large-scale</span> brain networks with distinct functional profiles, and provide insights into how the small-<span class="hlt">scale</span> functional specialization within early visual regions such as V1 relates to the <span class="hlt">large-scale</span> organization of functionally distinct whole-brain networks. PMID:27554527</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008HESSD...5.2791V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008HESSD...5.2791V"><span>On the relationship between <span class="hlt">large-scale</span> climate modes and regional synoptic patterns that drive Victorian rainfall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Verdon-Kidd, D.; Kiem, A. S.</p> <p>2008-10-01</p> <p>In this paper regional (synoptic) and <span class="hlt">large-scale</span> climate drivers of rainfall are investigated for Victoria, Australia. A non-linear classification methodology known as self-organizing maps (SOM) is used to identify 20 key regional synoptic patterns, which are shown to capture a range of significant synoptic features known to influence the climate of the region. Rainfall distributions are assigned to each of the 20 patterns for nine rainfall stations located across Victoria, resulting in a clear distinction between wet and dry synoptic types at each station. The influence of <span class="hlt">large-scale</span> climate modes on the frequency and timing of the regional synoptic patterns is also investigated. This analysis <span class="hlt">revealed</span> that phase changes in the El Niño Southern Oscillation (ENSO), the Southern Annular Mode (SAM) and/or Indian Ocean Dipole (IOD) are associated with a shift in the relative frequency of wet and dry synoptic types. Importantly, these results highlight the potential to utilise the link between the regional synoptic patterns derived in this study and <span class="hlt">large-scale</span> climate modes to improve rainfall forecasting for Victoria, both in the short- (i.e. seasonal) and long-term (i.e. decadal/multi-decadal <span class="hlt">scale</span>). In addition, the regional and <span class="hlt">large-scale</span> climate drivers identified in this study provide a benchmark by which the performance of Global Climate Models (GCMs) may be assessed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=326152&Lab=NRMRL&keyword=interest+AND+simple&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=326152&Lab=NRMRL&keyword=interest+AND+simple&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>Deriving spatial trends of <span class="hlt">air</span> pollution at a neighborhood-<span class="hlt">scale</span> through mobile monitoring</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>Abstract: Measuring <span class="hlt">air</span> pollution in real-time using an instrumented vehicle platform has been an emerging strategy to resolve <span class="hlt">air</span> pollution trends at a very fine spatial <span class="hlt">scale</span> (10s of meters). Achieving second-by-second data representative of urban <span class="hlt">air</span> quality trends requires a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H53K..01F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H53K..01F"><span>Parameterizing a <span class="hlt">Large-scale</span> Water Balance Model in Regions with Sparse Data: The Tigris-Euphrates River Basins as an Example</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Flint, A. L.; Flint, L. E.</p> <p>2010-12-01</p> <p>The characterization of hydrologic response to current and future climates is of increasing importance to many countries around the world that rely heavily on changing and uncertain water supplies. <span class="hlt">Large-scale</span> models that can calculate a spatially distributed water balance and elucidate groundwater recharge and surface water flows for <span class="hlt">large</span> river basins provide a basis of estimates of changes due to future climate projections. Unfortunately many regions in the world have very sparse data for parameterization or calibration of hydrologic models. For this study, the Tigris and Euphrates River basins were used for the development of a regional water balance model at 180-m spatial <span class="hlt">scale</span>, using the Basin Characterization Model, to estimate historical changes in groundwater recharge and surface water flows in the countries of Turkey, Syria, Iraq, Iran, and Saudi Arabia. Necessary input parameters include precipitation, <span class="hlt">air</span> temperature, potential evapotranspiration (PET), soil properties and thickness, and estimates of bulk permeability from geologic units. Data necessary for calibration includes snow cover, reservoir volumes (from satellite data and historic, pre-reservoir elevation data) and streamflow measurements. Global datasets for precipitation, <span class="hlt">air</span> temperature, and PET were available at very <span class="hlt">large</span> spatial <span class="hlt">scales</span> (50 km) through the world <span class="hlt">scale</span> databases, finer <span class="hlt">scale</span> WorldClim climate data, and required downscaling to fine <span class="hlt">scales</span> for model input. Soils data were available through world <span class="hlt">scale</span> soil maps but required parameterization on the basis of textural data to estimate soil hydrologic properties. Soil depth was interpreted from geomorphologic interpretation and maps of quaternary deposits, and geologic materials were categorized from generalized geologic maps of each country. Estimates of bedrock permeability were made on the basis of literature and data on driller’s logs and adjusted during calibration of the model to streamflow measurements where available</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29507254','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29507254"><span>Protein homology model refinement by <span class="hlt">large-scale</span> energy optimization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Park, Hahnbeom; Ovchinnikov, Sergey; Kim, David E; DiMaio, Frank; Baker, David</p> <p>2018-03-20</p> <p>Proteins fold to their lowest free-energy structures, and hence the most straightforward way to increase the accuracy of a partially incorrect protein structure model is to search for the lowest-energy nearby structure. This direct approach has met with little success for two reasons: first, energy function inaccuracies can lead to false energy minima, resulting in model degradation rather than improvement; and second, even with an accurate energy function, the search problem is formidable because the energy only drops considerably in the immediate vicinity of the global minimum, and there are a very <span class="hlt">large</span> number of degrees of freedom. Here we describe a <span class="hlt">large-scale</span> energy optimization-based refinement method that incorporates advances in both search and energy function accuracy that can substantially improve the accuracy of low-resolution homology models. The method refined low-resolution homology models into correct folds for 50 of 84 diverse protein families and generated improved models in recent blind structure prediction experiments. Analyses of the basis for these improvements <span class="hlt">reveal</span> contributions from both the improvements in conformational sampling techniques and the energy function.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EMS....46..271S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EMS....46..271S"><span>Bridging the <span class="hlt">scales</span> in a eulerian <span class="hlt">air</span> quality model to assess megacity export of pollution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Siour, G.; Colette, A.; Menut, L.; Bessagnet, B.; Coll, I.; Meleux, F.</p> <p>2013-08-01</p> <p>In Chemistry Transport Models (CTMs), spatial <span class="hlt">scale</span> interactions are often represented through off-line coupling between <span class="hlt">large</span> and small <span class="hlt">scale</span> models. However, those nested configurations cannot give account of the impact of the local <span class="hlt">scale</span> on its surroundings. This issue can be critical in areas exposed to <span class="hlt">air</span> mass recirculation (sea breeze cells) or around regions with sharp pollutant emission gradients (<span class="hlt">large</span> cities). Such phenomena can still be captured by the mean of adaptive gridding, two-way nesting or using model nudging, but these approaches remain relatively costly. We present here the development and the results of a simple alternative multi-<span class="hlt">scale</span> approach making use of a horizontal stretched grid, in the Eulerian CTM CHIMERE. This method, called "stretching" or "zooming", consists in the introduction of local zooms in a single chemistry-transport simulation. It allows bridging online the spatial <span class="hlt">scales</span> from the city (∼1 km resolution) to the continental area (∼50 km resolution). The CHIMERE model was run over a continental European domain, zoomed over the BeNeLux (Belgium, Netherlands and Luxembourg) area. We demonstrate that, compared with one-way nesting, the zooming method allows the expression of a significant feedback of the refined domain towards the <span class="hlt">large</span> <span class="hlt">scale</span>: around the city cluster of BeNeLuX, NO2 and O3 scores are improved. NO2 variability around BeNeLux is also better accounted for, and the net primary pollutant flux transported back towards BeNeLux is reduced. Although the results could not be validated for ozone over BeNeLux, we show that the zooming approach provides a simple and immediate way to better represent <span class="hlt">scale</span> interactions within a CTM, and constitutes a useful tool for apprehending the hot topic of megacities within their continental environment.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GeoRL..44.1892K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GeoRL..44.1892K"><span>Multiple mechanisms generate a universal <span class="hlt">scaling</span> with dissipation for the <span class="hlt">air</span>-water gas transfer velocity</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katul, Gabriel; Liu, Heping</p> <p>2017-02-01</p> <p>A <span class="hlt">large</span> corpus of field and laboratory experiments support the finding that the water side transfer velocity kL of sparingly soluble gases near <span class="hlt">air</span>-water interfaces <span class="hlt">scales</span> as kL˜(νɛ)1/4, where ν is the kinematic water viscosity and ɛ is the mean turbulent kinetic energy dissipation rate. Originally predicted from surface renewal theory, this <span class="hlt">scaling</span> appears to hold for marine and coastal systems and across many environmental conditions. It is shown that multiple approaches to representing the effects of turbulence on kL lead to this expression when the Kolmogorov microscale is assumed to be the most efficient transporting eddy near the interface. The approaches considered range from simplified surface renewal schemes with distinct models for renewal durations, <span class="hlt">scaling</span> and dimensional considerations, and a new structure function approach derived using analogies between scalar and momentum transfer. The work offers a new perspective as to why the aforementioned 1/4 <span class="hlt">scaling</span> is robust.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp.2351D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp.2351D"><span>On unravelling mechanism of interplay between cloud and <span class="hlt">large</span> <span class="hlt">scale</span> circulation: a grey area in climate science</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>De, S.; Agarwal, N. K.; Hazra, Anupam; Chaudhari, Hemantkumar S.; Sahai, A. K.</p> <p>2018-04-01</p> <p>The interaction between cloud and <span class="hlt">large</span> <span class="hlt">scale</span> circulation is much less explored area in climate science. Unfolding the mechanism of coupling between these two parameters is imperative for improved simulation of Indian summer monsoon (ISM) and to reduce imprecision in climate sensitivity of global climate model. This work has made an effort to explore this mechanism with CFSv2 climate model experiments whose cloud has been modified by changing the critical relative humidity (CRH) profile of model during ISM. Study <span class="hlt">reveals</span> that the variable CRH in CFSv2 has improved the nonlinear interactions between high and low frequency oscillations in wind field (<span class="hlt">revealed</span> as internal dynamics of monsoon) and modulates realistically the spatial distribution of interactions over Indian landmass during the contrasting monsoon season compared to the existing CRH profile of CFSv2. The lower tropospheric wind error energy in the variable CRH simulation of CFSv2 appears to be minimum due to the reduced nonlinear convergence of error to the planetary <span class="hlt">scale</span> range from long and synoptic <span class="hlt">scales</span> (another facet of internal dynamics) compared to as observed from other CRH experiments in normal and deficient monsoons. Hence, the interplay between cloud and <span class="hlt">large</span> <span class="hlt">scale</span> circulation through CRH may be manifested as a change in internal dynamics of ISM <span class="hlt">revealed</span> from <span class="hlt">scale</span> interactive quasi-linear and nonlinear kinetic energy exchanges in frequency as well as in wavenumber domain during the monsoon period that eventually modify the internal variance of CFSv2 model. Conversely, the reduced wind bias and proper modulation of spatial distribution of <span class="hlt">scale</span> interaction between the synoptic and low frequency oscillations improve the eastward and northward extent of water vapour flux over Indian landmass that in turn give feedback to the realistic simulation of cloud condensates attributing improved ISM rainfall in CFSv2.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70024964','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70024964"><span>Relationship of epithermal gold deposits to <span class="hlt">large-scale</span> fractures in northern Nevada</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Ponce, D.A.; Glen, J.M.G.</p> <p>2002-01-01</p> <p>Geophysical maps of northern Nevada <span class="hlt">reveal</span> at least three and possibly six <span class="hlt">large-scale</span> arcuate features, one of which corresponds to the northern Nevada rift that possibly extends more than 1,000 km from the Oregon- Idaho border to southern Nevada. These features may reflect deep discontinuities within the earth's crust, possibly related to the impact of the Yellowstone hot spot. Because mid-Miocene epithermal gold deposits have been shown to correlate with the northern Nevada rift, we investigate the association of other epithermal gold deposits to other similar arcuate features in northern Nevada. Mid-Miocene and younger epithermal gold- silver deposits also occur along two prominent aeromagnetic anomalies west of the northern Nevada rift. Here, we speculate that mid-Miocene deposits formed along deep fractures in association with mid-Miocene rift- related magmatism and that younger deposits preferentially followed these preexisting features. Statistical analysis of the proximity of epithermal gold deposits to these features suggests that epithermal gold deposits in northern Nevada are spatially associated with <span class="hlt">large-scale</span> crustal features interpreted from geophysical data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19850026832','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19850026832"><span>Management of <span class="hlt">large-scale</span> technology</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Levine, A.</p> <p>1985-01-01</p> <p>Two major themes are addressed in this assessment of the management of <span class="hlt">large-scale</span> NASA programs: (1) how a high technology agency was a decade marked by a rapid expansion of funds and manpower in the first half and almost as rapid contraction in the second; and (2) how NASA combined central planning and control with decentralized project execution.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JTurb..19..274F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JTurb..19..274F"><span>Computational domain length and Reynolds number effects on <span class="hlt">large-scale</span> coherent motions in turbulent pipe flow</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feldmann, Daniel; Bauer, Christian; Wagner, Claus</p> <p>2018-03-01</p> <p>We present results from direct numerical simulations (DNS) of turbulent pipe flow at shear Reynolds numbers up to Reτ = 1500 using different computational domains with lengths up to ?. The objectives are to analyse the effect of the finite size of the periodic pipe domain on <span class="hlt">large</span> flow structures in dependency of Reτ and to assess a minimum ? required for relevant turbulent <span class="hlt">scales</span> to be captured and a minimum Reτ for very <span class="hlt">large-scale</span> motions (VLSM) to be analysed. Analysing one-point statistics <span class="hlt">revealed</span> that the mean velocity profile is invariant for ?. The wall-normal location at which deviations occur in shorter domains changes strongly with increasing Reτ from the near-wall region to the outer layer, where VLSM are believed to live. The root mean square velocity profiles exhibit domain length dependencies for pipes shorter than 14R and 7R depending on Reτ. For all Reτ, the higher-order statistical moments show only weak dependencies and only for the shortest domain considered here. However, the analysis of one- and two-dimensional pre-multiplied energy spectra <span class="hlt">revealed</span> that even for larger ?, not all physically relevant <span class="hlt">scales</span> are fully captured, even though the aforementioned statistics are in good agreement with the literature. We found ? to be sufficiently <span class="hlt">large</span> to capture VLSM-relevant turbulent <span class="hlt">scales</span> in the considered range of Reτ based on our definition of an integral energy threshold of 10%. The requirement to capture at least 1/10 of the global maximum energy level is justified by a 14% increase of the streamwise turbulence intensity in the outer region between Reτ = 720 and 1500, which can be related to VLSM-relevant length <span class="hlt">scales</span>. Based on this <span class="hlt">scaling</span> anomaly, we found Reτ⪆1500 to be a necessary minimum requirement to investigate VLSM-related effects in pipe flow, even though the streamwise energy spectra does not yet indicate sufficient <span class="hlt">scale</span> separation between the most energetic and the very long motions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1992P%26SS...40..829B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1992P%26SS...40..829B"><span>Some aspects of <span class="hlt">large-scale</span> travelling ionospheric disturbances</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bowman, G. G.</p> <p>1992-06-01</p> <p>On two occasions the speeds and directions of travel of <span class="hlt">large-scale</span> traveling ionospheric disturbances (LS-TIDs) following geomagnetic substorm onsets, have been calculated for the propagation of these disturbances in both hemispheres of the earth. N(h) analyses have been used to produce height change profiles at a fixed frequency from which time shifts between stations (used for the speed and direction-of-travel values) have been calculated. Fixed-frequency phase path measurements at Bribie Island for two events <span class="hlt">reveal</span> wavetrains with periodicities around 17 min associated with these disturbances. Another event recorded a periodicity of 19 min. Also, for two of the events additional periodicities around 30 min were found. These wavetrains along with the macroscale height changes and electron density depletions associated with these LS-TIDs are essentially the same as the ionospheric structure changes observed during the passage of night-time medium-<span class="hlt">scale</span> traveling ionospheric disturbances (MS-TIDs). However, unlike these MS-TIDs, the LS-TIDs are generally not associated with the recording of spread-F on ionograms. Possible reasons for this difference are discussed as well as the special conditions which probably prevail on the few occasions when spread-F is associated with LS-TIDs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4325324','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4325324"><span>Energetics and Structural Characterization of the <span class="hlt">large-scale</span> Functional Motion of Adenylate Kinase</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Formoso, Elena; Limongelli, Vittorio; Parrinello, Michele</p> <p>2015-01-01</p> <p>Adenylate Kinase (AK) is a signal transducing protein that regulates cellular energy homeostasis balancing between different conformations. An alteration of its activity can lead to severe pathologies such as heart failure, cancer and neurodegenerative diseases. A comprehensive elucidation of the <span class="hlt">large-scale</span> conformational motions that rule the functional mechanism of this enzyme is of great value to guide rationally the development of new medications. Here using a metadynamics-based computational protocol we elucidate the thermodynamics and structural properties underlying the AK functional transitions. The free energy estimation of the conformational motions of the enzyme allows characterizing the sequence of events that regulate its action. We <span class="hlt">reveal</span> the atomistic details of the most relevant enzyme states, identifying residues such as Arg119 and Lys13, which play a key role during the conformational transitions and represent druggable spots to design enzyme inhibitors. Our study offers tools that open new areas of investigation on <span class="hlt">large-scale</span> motion in proteins. PMID:25672826</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015NatSR...5E8425F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015NatSR...5E8425F"><span>Energetics and Structural Characterization of the <span class="hlt">large-scale</span> Functional Motion of Adenylate Kinase</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Formoso, Elena; Limongelli, Vittorio; Parrinello, Michele</p> <p>2015-02-01</p> <p>Adenylate Kinase (AK) is a signal transducing protein that regulates cellular energy homeostasis balancing between different conformations. An alteration of its activity can lead to severe pathologies such as heart failure, cancer and neurodegenerative diseases. A comprehensive elucidation of the <span class="hlt">large-scale</span> conformational motions that rule the functional mechanism of this enzyme is of great value to guide rationally the development of new medications. Here using a metadynamics-based computational protocol we elucidate the thermodynamics and structural properties underlying the AK functional transitions. The free energy estimation of the conformational motions of the enzyme allows characterizing the sequence of events that regulate its action. We <span class="hlt">reveal</span> the atomistic details of the most relevant enzyme states, identifying residues such as Arg119 and Lys13, which play a key role during the conformational transitions and represent druggable spots to design enzyme inhibitors. Our study offers tools that open new areas of investigation on <span class="hlt">large-scale</span> motion in proteins.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025287','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025287"><span>US National <span class="hlt">Large-scale</span> City Orthoimage Standard Initiative</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Zhou, G.; Song, C.; Benjamin, S.; Schickler, W.</p> <p>2003-01-01</p> <p>The early procedures and algorithms for National digital orthophoto generation in National Digital Orthophoto Program (NDOP) were based on earlier USGS mapping operations, such as field control, aerotriangulation (derived in the early 1920's), the quarter-quadrangle-centered (3.75 minutes of longitude and latitude in geographic extent), 1:40,000 aerial photographs, and 2.5 D digital elevation models. However, <span class="hlt">large-scale</span> city orthophotos using early procedures have disclosed many shortcomings, e.g., ghost image, occlusion, shadow. Thus, to provide the technical base (algorithms, procedure) and experience needed for city <span class="hlt">large-scale</span> digital orthophoto creation is essential for the near future national <span class="hlt">large-scale</span> digital orthophoto deployment and the revision of the Standards for National <span class="hlt">Large-scale</span> City Digital Orthophoto in National Digital Orthophoto Program (NDOP). This paper will report our initial research results as follows: (1) High-precision 3D city DSM generation through LIDAR data processing, (2) Spatial objects/features extraction through surface material information and high-accuracy 3D DSM data, (3) 3D city model development, (4) Algorithm development for generation of DTM-based orthophoto, and DBM-based orthophoto, (5) True orthophoto generation by merging DBM-based orthophoto and DTM-based orthophoto, and (6) Automatic mosaic by optimizing and combining imagery from many perspectives.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011ExFl...50..929K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011ExFl...50..929K"><span><span class="hlt">Large-scale</span> tomographic particle image velocimetry using helium-filled soap bubbles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kühn, Matthias; Ehrenfried, Klaus; Bosbach, Johannes; Wagner, Claus</p> <p>2011-04-01</p> <p>To measure <span class="hlt">large-scale</span> flow structures in <span class="hlt">air</span>, a tomographic particle image velocimetry (tomographic PIV) system for measurement volumes of the order of one cubic metre is developed, which employs helium-filled soap bubbles (HFSBs) as tracer particles. The technique has several specific characteristics compared to most conventional tomographic PIV systems, which are usually applied to small measurement volumes. One of them is spot lights on the HFSB tracers, which slightly change their position, when the direction of observation is altered. Further issues are the <span class="hlt">large</span> particle to voxel ratio and the short focal length of the used camera lenses, which result in a noticeable variation of the magnification factor in volume depth direction. Taking the specific characteristics of the HFSBs into account, the feasibility of our <span class="hlt">large-scale</span> tomographic PIV system is demonstrated by showing that the calibration errors can be reduced down to 0.1 pixels as required. Further, an accurate and fast implementation of the multiplicative algebraic reconstruction technique, which calculates the weighting coefficients when needed instead of storing them, is discussed. The tomographic PIV system is applied to measure forced convection in a convection cell at a Reynolds number of 530 based on the inlet channel height and the mean inlet velocity. The size of the measurement volume and the interrogation volumes amount to 750 mm × 450 mm × 165 mm and 48 mm × 48 mm × 24 mm, respectively. Validation of the tomographic PIV technique employing HFSBs is further provided by comparing profiles of the mean velocity and of the root mean square velocity fluctuations to respective planar PIV data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhRvD..89f3014Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhRvD..89f3014Y"><span><span class="hlt">Large-scale</span> structure in superfluid Chaplygin gas cosmology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Rongjia</p> <p>2014-03-01</p> <p>We investigate the growth of the <span class="hlt">large-scale</span> structure in the superfluid Chaplygin gas (SCG) model. Both linear and nonlinear growth, such as σ8 and the skewness S3, are discussed. We find the growth factor of SCG reduces to the Einstein-de Sitter case at early times while it differs from the cosmological constant model (ΛCDM) case in the <span class="hlt">large</span> a limit. We also find there will be more stricture growth on <span class="hlt">large</span> <span class="hlt">scales</span> in the SCG scenario than in ΛCDM and the variations of σ8 and S3 between SCG and ΛCDM cannot be discriminated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1126849','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1126849"><span>Geospatial Optimization of Siting <span class="hlt">Large-Scale</span> Solar Projects</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>Macknick, Jordan; Quinby, Ted; Caulfield, Emmet</p> <p>2014-03-01</p> <p>Recent policy and economic conditions have encouraged a renewed interest in developing <span class="hlt">large-scale</span> solar projects in the U.S. Southwest. However, siting <span class="hlt">large-scale</span> solar projects is complex. In addition to the quality of the solar resource, solar developers must take into consideration many environmental, social, and economic factors when evaluating a potential site. This report describes a proof-of-concept, Web-based Geographical Information Systems (GIS) tool that evaluates multiple user-defined criteria in an optimization algorithm to inform discussions and decisions regarding the locations of utility-<span class="hlt">scale</span> solar projects. Existing siting recommendations for <span class="hlt">large-scale</span> solar projects from governmental and non-governmental organizations are not consistent withmore » each other, are often not transparent in methods, and do not take into consideration the differing priorities of stakeholders. The siting assistance GIS tool we have developed improves upon the existing siting guidelines by being user-driven, transparent, interactive, capable of incorporating multiple criteria, and flexible. This work provides the foundation for a dynamic siting assistance tool that can greatly facilitate siting decisions among multiple stakeholders.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=System+AND+1+AND+vs+AND+System+AND+2+AND+Decision+AND+Making&id=ED466499','ERIC'); return false;" href="https://eric.ed.gov/?q=System+AND+1+AND+vs+AND+System+AND+2+AND+Decision+AND+Making&id=ED466499"><span>Critical Issues in <span class="hlt">Large-Scale</span> Assessment: A Resource Guide.</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>Redfield, Doris</p> <p></p> <p>The purpose of this document is to provide practical guidance and support for the design, development, and implementation of <span class="hlt">large-scale</span> assessment systems that are grounded in research and best practice. Information is included about existing <span class="hlt">large-scale</span> testing efforts, including national testing programs, state testing programs, and…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.H23I..08H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.H23I..08H"><span>The Design of <span class="hlt">Large</span> Geothermally Powered <span class="hlt">Air</span>-Conditioning Systems Using an Optimal Control Approach</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Horowitz, F. G.; O'Bryan, L.</p> <p>2010-12-01</p> <p>The direct use of geothermal energy from Hot Sedimentary Aquifer (HSA) systems for <span class="hlt">large</span> <span class="hlt">scale</span> <span class="hlt">air</span>-conditioning projects involves many tradeoffs. Aspects contributing towards making design decisions for such systems include: the inadequately known permeability and thermal distributions underground; the combinatorial complexity of selecting pumping and chiller systems to match the underground conditions to the <span class="hlt">air</span>-conditioning requirements; the future price variations of the electricity market; any uncertainties in future Carbon pricing; and the applicable discount rate for evaluating the financial worth of the project. Expanding upon the previous work of Horowitz and Hornby (2007), we take an optimal control approach to the design of such systems. By building a model of the HSA system, the drilling process, the pumping process, and the chilling operations, along with a specified objective function, we can write a Hamiltonian for the system. Using the standard techniques of optimal control, we use gradients of the Hamiltonian to find the optimal design for any given set of permeabilities, thermal distributions, and the other engineering and financial parameters. By using this approach, optimal system designs could potentially evolve in response to the actual conditions encountered during drilling. Because the granularity of some current models is so coarse, we will be able to compare our optimal control approach to an exhaustive search of parameter space. We will present examples from the conditions appropriate for the Perth Basin of Western Australia, where the WA Geothermal Centre of Excellence is involved with two <span class="hlt">large</span> <span class="hlt">air</span>-conditioning projects using geothermal water from deep aquifers at 75 to 95 degrees C.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2015APS..DFDM14010X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015APS..DFDM14010X"><span>Rolling up of <span class="hlt">Large-scale</span> Laminar Vortex Ring from Synthetic Jet Impinging onto a Wall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Yang; Pan, Chong; Wang, Jinjun; Flow Control Lab Team</p> <p>2015-11-01</p> <p>Vortex ring impinging onto a wall exhibits a wide range of interesting behaviors. The present work devotes to an experimental investigation of a series of small-<span class="hlt">scale</span> vortex rings impinging onto a wall. These laminar vortex rings were generated by a piston-cylinder driven synthetic jet in a water tank. Laser Induced Fluorescence (LIF) and Particle Image Velocimetry (PIV) were used for flow visualization/quantification. A special scenario of vortical dynamic was found for the first time: a <span class="hlt">large-scale</span> laminar vortex ring is formed above the wall, on the outboard side of the jet. This <span class="hlt">large-scale</span> structure is stable in topology pattern, and continuously grows in strength and size along time, thus dominating dynamics of near wall flow. To quantify its spatial/temporal characteristics, Finite-Time Lyapunov Exponent (FTLE) fields were calculated from PIV velocity fields. It is shown that the flow pattern <span class="hlt">revealed</span> by FTLE fields is similar to the visualization. The size of this <span class="hlt">large-scale</span> vortex ring can be up to one-order larger than the jet vortices, and its rolling-up speed and entrainment strength was correlated to constant vorticity flux issued from the jet. This work was supported by the National Natural Science Foundation of China (Grants No.11202015 and 11327202).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.7378K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.7378K"><span>Storm generated <span class="hlt">large</span> <span class="hlt">scale</span> TIDs (LSTIDs): local, regional and global observations during solar cycles 23-24</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katamzi, Zama; Bosco Habarulema, John</p> <p>2017-04-01</p> <p><span class="hlt">Large</span> <span class="hlt">scale</span> traveling ionospheric disturbances (LSTIDs) are a key dynamic ionospheric process that transports energy and momentum vertically and horizontally during storms. These disturbances are observed as electron density irregularities in total electron content and other ionospheric parameters. This study reports on various explorations of LSTIDs characteristics, in particular horizontal and vertical propagation, during some major/severe storms of solar cycles 23-24. We have employed GNSS TEC to estimate horizontal propagation and radio occultation data from COSMIC/FORMOSAT-3 and SWARM satellites to estimate vertical motion. The work presented here <span class="hlt">reveals</span> the evolution of the characterisation efficiency from using sparsely populated stations, resulting in limited spatial resolution through rudimentary analysis to more densely populated GNSS network leading to more accurate temporal and spatial determinations. For example, early observations of LSTIDs <span class="hlt">largely</span> <span class="hlt">revealed</span> unidirectional propagation whereas later studies have showed that one storm can induce multi-directional propagation, e.g. Halloween 2003 storm induced equatorward LSTIDs on a local <span class="hlt">scale</span> whereas the 9 March 2012 storm induced simultaneous equatorward and poleward LSTIDs on a global <span class="hlt">scale</span>. This later study, i.e. 9 March 2012 storm, <span class="hlt">revealed</span> for the first time that ionospheric electrodynamics, specifically variations in ExB drift, is also an efficient generator of LSTIDs. Results from these studies also <span class="hlt">revealed</span> constructive and destructive interference pattern of storm induced LSTIDs. Constellations of LEO satellites such as COSMIC/FORMOSAT-3 and SWARM have given sufficient spatial and temporal resolution to study vertical propagation of LSTIDs in addition to the meridional propagation given by GNSS TEC; the former (i.e. vertical velocities) were found to fall below 100 m/s.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010OcMod..35..105S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010OcMod..35..105S"><span>Modeling quiescent phase transport of <span class="hlt">air</span> bubbles induced by breaking waves</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shi, Fengyan; Kirby, James T.; Ma, Gangfeng</p> <p></p> <p> production in the algorithm for initial bubble entrainment. The study demonstrates a potential use of an entrainment formula in simulations of <span class="hlt">air</span> bubble population in a surfzone-<span class="hlt">scale</span> domain. It also <span class="hlt">reveals</span> some difficulties in use of the two-fluid model for predicting <span class="hlt">large</span> <span class="hlt">air</span> pockets induced by wave breaking, and suggests that it may be necessary to use a gas-liquid two-phase model as the basic model framework for the mixture phase and to develop an algorithm to allow for transfer of discrete <span class="hlt">air</span> pockets to the continuum bubble phase. A more theoretically justifiable <span class="hlt">air</span> entrainment formulation should be developed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011279','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011279"><span>State of the Art in <span class="hlt">Large-Scale</span> Soil Moisture Monitoring</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ochsner, Tyson E.; Cosh, Michael Harold; Cuenca, Richard H.; Dorigo, Wouter; Draper, Clara S.; Hagimoto, Yutaka; Kerr, Yan H.; Larson, Kristine M.; Njoku, Eni Gerald; Small, Eric E.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140011279'); toggleEditAbsImage('author_20140011279_show'); toggleEditAbsImage('author_20140011279_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140011279_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140011279_hide"></p> <p>2013-01-01</p> <p>Soil moisture is an essential climate variable influencing land atmosphere interactions, an essential hydrologic variable impacting rainfall runoff processes, an essential ecological variable regulating net ecosystem exchange, and an essential agricultural variable constraining food security. <span class="hlt">Large-scale</span> soil moisture monitoring has advanced in recent years creating opportunities to transform scientific understanding of soil moisture and related processes. These advances are being driven by researchers from a broad range of disciplines, but this complicates collaboration and communication. For some applications, the science required to utilize <span class="hlt">large-scale</span> soil moisture data is poorly developed. In this review, we describe the state of the art in <span class="hlt">large-scale</span> soil moisture monitoring and identify some critical needs for research to optimize the use of increasingly available soil moisture data. We review representative examples of 1) emerging in situ and proximal sensing techniques, 2) dedicated soil moisture remote sensing missions, 3) soil moisture monitoring networks, and 4) applications of <span class="hlt">large-scale</span> soil moisture measurements. Significant near-term progress seems possible in the use of <span class="hlt">large-scale</span> soil moisture data for drought monitoring. Assimilation of soil moisture data for meteorological or hydrologic forecasting also shows promise, but significant challenges related to model structures and model errors remain. Little progress has been made yet in the use of <span class="hlt">large-scale</span> soil moisture observations within the context of ecological or agricultural modeling. Opportunities abound to advance the science and practice of <span class="hlt">large-scale</span> soil moisture monitoring for the sake of improved Earth system monitoring, modeling, and forecasting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16..438R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16..438R"><span>The influence of <span class="hlt">scales</span> of atmospheric motion on <span class="hlt">air</span> pollution over Portugal</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Russo, Ana; Trigo, Ricardo; Mendes, Manuel; Jerez, Sonia; Gouveia, Célia Marina</p> <p>2014-05-01</p> <p><span class="hlt">Air</span> pollution is determined by the combination of different factors, namely, emissions, physical constrains, meteorology and chemical processes [1,2,3]. The relative importance of such factors is influenced by their interaction on diverse <span class="hlt">scales</span> of atmospheric motion. Each <span class="hlt">scale</span> depicts different meteorological conditions, which, when combined with the different <span class="hlt">air</span> pollution sources and photochemistry, result in varying ambient concentrations [2]. Identifying the dominant <span class="hlt">scales</span> of atmospheric motion over a given airshed can be of great importance for many applications such as <span class="hlt">air</span> pollution and pollen dispersion or wind energy management [2]. Portugal has been affected by numerous <span class="hlt">air</span> pollution episodes during the last decade. These episodes are often related to peak emissions from local industry or transport, but can also be associated to regional transport from other urban areas or to exceptional emission events, such as forest fires. This research aims to identify the <span class="hlt">scales</span> of atmospheric motion which contribute to an increase of <span class="hlt">air</span> pollution. A method is proposed for differentiating between the <span class="hlt">scales</span> of atmospheric motion that can be applied on a daily basis from data collected at several wind-measuring sites in a given airshed and to reanalysis datasets. The method is based on the daily mean wind recirculation and the mean and standard deviation between sites. The determination of the thresholds between <span class="hlt">scales</span> is performed empirically following the approach of Levy et al. [2] and also through a automatic statistical approach computed taking into account the tails of the distributions (e.g. 95% and 99% percentile) of the different wind samples. A comparison is made with two objective approaches: 1) daily synoptic classification for the same period over the region [4] and 2) a 3-D backward trajectory approach [5,6] for specific episodes. Furthermore, the outcomes are expected to support the Portuguese authorities on the implementation of strategies for a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A31H2280G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A31H2280G"><span>Improving Prediction of <span class="hlt">Large-scale</span> Regime Transitions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gyakum, J. R.; Roebber, P.; Bosart, L. F.; Honor, A.; Bunker, E.; Low, Y.; Hart, J.; Bliankinshtein, N.; Kolly, A.; Atallah, E.; Huang, Y.</p> <p>2017-12-01</p> <p>Cool season atmospheric predictability over the CONUS on subseasonal times <span class="hlt">scales</span> (1-4 weeks) is critically dependent upon the structure, configuration, and evolution of the North Pacific jet stream (NPJ). The NPJ can be perturbed on its tropical side on synoptic time <span class="hlt">scales</span> by recurving and transitioning tropical cyclones (TCs) and on subseasonal time <span class="hlt">scales</span> by longitudinally varying convection associated with the Madden-Julian Oscillation (MJO). Likewise, the NPJ can be perturbed on its poleward side on synoptic time <span class="hlt">scales</span> by midlatitude and polar disturbances that originate over the Asian continent. These midlatitude and polar disturbances can often trigger downstream Rossby wave propagation across the North Pacific, North America, and the North Atlantic. The project team is investigating the following multiscale processes and features: the spatiotemporal distribution of cyclone clustering over the Northern Hemisphere; cyclone clustering as influenced by atmospheric blocking and the phases and amplitudes of the major teleconnection indices, ENSO and the MJO; composite and case study analyses of representative cyclone clustering events to establish the governing dynamics; regime change predictability horizons associated with cyclone clustering events; Arctic <span class="hlt">air</span> mass generation and modification; life cycles of the MJO; and poleward heat and moisture transports of subtropical <span class="hlt">air</span> masses. A critical component of the study is weather regime classification. These classifications are defined through: the spatiotemporal clustering of surface cyclogenesis; a general circulation metric combining data at 500-hPa and the dynamic tropopause; Self Organizing Maps (SOM), constructed from dynamic tropopause and 850 hPa equivalent potential temperature data. The resultant lattice of nodes is used to categorize synoptic classes and their predictability, as well as to determine the robustness of the CFSv2 model climate relative to observations. Transition pathways between these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19730011429','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19730011429"><span>Hierarchical hybrid control of manipulators: Artificial intelligence in <span class="hlt">large</span> <span class="hlt">scale</span> integrated circuits</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Greene, P. H.</p> <p>1972-01-01</p> <p>Both in practical engineering and in control of muscular systems, low level subsystems automatically provide crude approximations to the proper response. Through low level tuning of these approximations, the proper response variant can emerge from standardized high level commands. Such systems are expressly suited to emerging <span class="hlt">large</span> <span class="hlt">scale</span> integrated circuit technology. A computer, using symbolic descriptions of subsystem responses, can select and shape responses of low level digital or analog microcircuits. A mathematical theory that <span class="hlt">reveals</span> significant informational units in this style of control and software for realizing such information structures are formulated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920058377&hterms=microbiota&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmicrobiota','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920058377&hterms=microbiota&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmicrobiota"><span>Remote sensing of the biological dynamics of <span class="hlt">large-scale</span> salt evaporation ponds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Richardson, Laurie L.; Bachoon, Dave; Ingram-Willey, Vebbra; Chow, Colin C.; Weinstock, Kenneth</p> <p>1992-01-01</p> <p>Optical properties of salt evaporation ponds associated with Exportadora de Sal, a salt production company in Baja California Sur, Mexico, were analyzed using a combination of spectroradiometer and extracted pigment data, and Landsat-5 Thematic Mapper imagery. The optical characteristics of each pond are determined by the biota, which consists of dense populations of algae and photosynthetic bacteria containing a wide variety of photosynthetic and photoprotective pigments. Analysis has shown that spectral and image data can differentiate between taxonomic groups of the microbiota, detect changes in population distributions, and <span class="hlt">reveal</span> <span class="hlt">large-scale</span> seasonal dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009EGUGA..1113087A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009EGUGA..1113087A"><span>Nonlinear Generation of shear flows and <span class="hlt">large</span> <span class="hlt">scale</span> magnetic fields by small <span class="hlt">scale</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aburjania, G.</p> <p>2009-04-01</p> <p>EGU2009-233 Nonlinear Generation of shear flows and <span class="hlt">large</span> <span class="hlt">scale</span> magnetic fields by small <span class="hlt">scale</span> turbulence in the ionosphere by G. Aburjania Contact: George Aburjania, g.aburjania@gmail.com,aburj@mymail.ge</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3737197','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3737197"><span>Eyjafjallajökull and 9/11: The Impact of <span class="hlt">Large-Scale</span> Disasters on Worldwide Mobility</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Woolley-Meza, Olivia; Grady, Daniel; Thiemann, Christian; Bagrow, James P.; Brockmann, Dirk</p> <p>2013-01-01</p> <p><span class="hlt">Large-scale</span> disasters that interfere with globalized socio-technical infrastructure, such as mobility and transportation networks, trigger high socio-economic costs. Although the origin of such events is often geographically confined, their impact reverberates through entire networks in ways that are poorly understood, difficult to assess, and even more difficult to predict. We investigate how the eruption of volcano Eyjafjallajökull, the September 11th terrorist attacks, and geographical disruptions in general interfere with worldwide mobility. To do this we track changes in effective distance in the worldwide <span class="hlt">air</span> transportation network from the perspective of individual airports. We find that universal features exist across these events: airport susceptibilities to regional disruptions follow similar, strongly heterogeneous distributions that lack a <span class="hlt">scale</span>. On the other hand, airports are more uniformly susceptible to attacks that target the most important hubs in the network, exhibiting a well-defined <span class="hlt">scale</span>. The statistical behavior of susceptibility can be characterized by a single <span class="hlt">scaling</span> exponent. Using <span class="hlt">scaling</span> arguments that capture the interplay between individual airport characteristics and the structural properties of routes we can recover the exponent for all types of disruption. We find that the same mechanisms responsible for efficient passenger flow may also keep the system in a vulnerable state. Our approach can be applied to understand the impact of <span class="hlt">large</span>, correlated disruptions in financial systems, ecosystems and other systems with a complex interaction structure between heterogeneous components. PMID:23950904</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=88273&keyword=e+AND+commerce&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=88273&keyword=e+AND+commerce&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>APPLICATION OF FINE <span class="hlt">SCALE</span> <span class="hlt">AIR</span> TOXICS MODELING WITH CMAQ TO HAPEM5</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 paper provides a preliminary demonstration of the EPA neighborhood <span class="hlt">scale</span> modeling paradigm for <span class="hlt">air</span> toxics by linking concentration from the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) modeling system to the fifth version of the Hazardous Pollutant Exposure Model (HAPEM5). For t...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Geomo.151..164M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Geomo.151..164M"><span>The interaction between active normal faulting and <span class="hlt">large</span> <span class="hlt">scale</span> gravitational mass movements <span class="hlt">revealed</span> by paleoseismological techniques: A case study from central Italy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moro, M.; Saroli, M.; Gori, S.; Falcucci, E.; Galadini, F.; Messina, P.</p> <p>2012-05-01</p> <p>Paleoseismological techniques have been applied to characterize the kinematic behaviour of <span class="hlt">large-scale</span> gravitational phenomena located in proximity of the seismogenic fault responsible for the Mw 7.0, 1915 Avezzano earthquake and to identify evidence of a possible coseismic reactivation. The above mentioned techniques were applied to the surface expression of the main sliding planes of the Mt. Serrone gravitational deformation, located in the southeastern border of the Fucino basin (central Italy). The approach allows us to detect instantaneous events of deformation along the uphill-facing scarp. These events are testified by the presence of faulted deposits and colluvial wedges. The identified and chronologically-constrained episodes of rapid displacement can be probably correlated with seismic events determined by the activation of the Fucino seismogenic fault, affecting the toe of the gravitationally unstable rock mass. Indeed this fault can produce strong, short-term dynamic stresses able to trigger the release of local gravitational stress accumulated by Mt. Serrone's <span class="hlt">large-scale</span> gravitational phenomena. The applied methodology could allow us to better understand the geometric and kinematic relationships between active tectonic structures and <span class="hlt">large-scale</span> gravitational phenomena. It would be more important in seismically active regions, since deep-seated gravitational slope deformations can evolve into a catastrophic collapse and can strongly increase the level of earthquake-induced hazards.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN11E..04M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN11E..04M"><span><span class="hlt">Large-scale</span> Labeled Datasets to Fuel Earth Science Deep Learning Applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Maskey, M.; Ramachandran, R.; Miller, J.</p> <p>2017-12-01</p> <p>Deep learning has revolutionized computer vision and natural language processing with various algorithms <span class="hlt">scaled</span> using high-performance computing. However, generic <span class="hlt">large-scale</span> labeled datasets such as the ImageNet are the fuel that drives the impressive accuracy of deep learning results. <span class="hlt">Large-scale</span> labeled datasets already exist in domains such as medical science, but creating them in the Earth science domain is a challenge. While there are ways to apply deep learning using limited labeled datasets, there is a need in the Earth sciences for creating <span class="hlt">large-scale</span> labeled datasets for benchmarking and <span class="hlt">scaling</span> deep learning applications. At the NASA Marshall Space Flight Center, we are using deep learning for a variety of Earth science applications where we have encountered the need for <span class="hlt">large-scale</span> labeled datasets. We will discuss our approaches for creating such datasets and why these datasets are just as valuable as deep learning algorithms. We will also describe successful usage of these <span class="hlt">large-scale</span> labeled datasets with our deep learning based applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JETPL.107..157O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JETPL.107..157O"><span><span class="hlt">Large-Scale</span> Coherent Vortex Formation in Two-Dimensional Turbulence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Orlov, A. V.; Brazhnikov, M. Yu.; Levchenko, A. A.</p> <p>2018-04-01</p> <p>The evolution of a vortex flow excited by an electromagnetic technique in a thin layer of a conducting liquid was studied experimentally. Small-<span class="hlt">scale</span> vortices, excited at the pumping <span class="hlt">scale</span>, merge with time due to the nonlinear interaction and produce <span class="hlt">large-scale</span> structures—the inverse energy cascade is formed. The dependence of the energy spectrum in the developed inverse cascade is well described by the Kraichnan law k -5/3. At <span class="hlt">large</span> <span class="hlt">scales</span>, the inverse cascade is limited by cell sizes, and a <span class="hlt">large-scale</span> coherent vortex flow is formed, which occupies almost the entire area of the experimental cell. The radial profile of the azimuthal velocity of the coherent vortex immediately after the pumping was switched off has been established for the first time. Inside the vortex core, the azimuthal velocity grows linearly along a radius and reaches a constant value outside the core, which agrees well with the theoretical prediction.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25731989','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25731989"><span>Robust regression for <span class="hlt">large-scale</span> neuroimaging studies.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fritsch, Virgile; Da Mota, Benoit; Loth, Eva; Varoquaux, Gaël; Banaschewski, Tobias; Barker, Gareth J; Bokde, Arun L W; Brühl, Rüdiger; Butzek, Brigitte; Conrod, Patricia; Flor, Herta; Garavan, Hugh; Lemaitre, Hervé; Mann, Karl; Nees, Frauke; Paus, Tomas; Schad, Daniel J; Schümann, Gunter; Frouin, Vincent; Poline, Jean-Baptiste; Thirion, Bertrand</p> <p>2015-05-01</p> <p>Multi-subject datasets used in neuroimaging group studies have a complex structure, as they exhibit non-stationary statistical properties across regions and display various artifacts. While studies with small sample sizes can rarely be shown to deviate from standard hypotheses (such as the normality of the residuals) due to the poor sensitivity of normality tests with low degrees of freedom, <span class="hlt">large-scale</span> studies (e.g. >100 subjects) exhibit more obvious deviations from these hypotheses and call for more refined models for statistical inference. Here, we demonstrate the benefits of robust regression as a tool for analyzing <span class="hlt">large</span> neuroimaging cohorts. First, we use an analytic test based on robust parameter estimates; based on simulations, this procedure is shown to provide an accurate statistical control without resorting to permutations. Second, we show that robust regression yields more detections than standard algorithms using as an example an imaging genetics study with 392 subjects. Third, we show that robust regression can avoid false positives in a <span class="hlt">large-scale</span> analysis of brain-behavior relationships with over 1500 subjects. Finally we embed robust regression in the Randomized Parcellation Based Inference (RPBI) method and demonstrate that this combination further improves the sensitivity of tests carried out across the whole brain. Altogether, our results show that robust procedures provide important advantages in <span class="hlt">large-scale</span> neuroimaging group studies. Copyright © 2015 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22727063','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22727063"><span>Intensive agriculture erodes β-diversity at <span class="hlt">large</span> <span class="hlt">scales</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Karp, Daniel S; Rominger, Andrew J; Zook, Jim; Ranganathan, Jai; Ehrlich, Paul R; Daily, Gretchen C</p> <p>2012-09-01</p> <p>Biodiversity is declining from unprecedented land conversions that replace diverse, low-intensity agriculture with vast expanses under homogeneous, intensive production. Despite documented losses of species richness, consequences for β-diversity, changes in community composition between sites, are <span class="hlt">largely</span> unknown, especially in the tropics. Using a 10-year data set on Costa Rican birds, we find that low-intensity agriculture sustained β-diversity across <span class="hlt">large</span> <span class="hlt">scales</span> on a par with forest. In high-intensity agriculture, low local (α) diversity inflated β-diversity as a statistical artefact. Therefore, at small spatial <span class="hlt">scales</span>, intensive agriculture appeared to retain β-diversity. Unlike in forest or low-intensity systems, however, high-intensity agriculture also homogenised vegetation structure over <span class="hlt">large</span> distances, thereby decoupling the fundamental ecological pattern of bird communities changing with geographical distance. This ~40% decline in species turnover indicates a significant decline in β-diversity at <span class="hlt">large</span> spatial <span class="hlt">scales</span>. These findings point the way towards multi-functional agricultural systems that maintain agricultural productivity while simultaneously conserving biodiversity. © 2012 Blackwell Publishing Ltd/CNRS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/9190','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/9190"><span><span class="hlt">Large</span> <span class="hlt">scale</span> systems : a study of computer organizations for <span class="hlt">air</span> traffic control applications.</span></a></p> <p><a target="_blank" href="http://ntlsearch.bts.gov/tris/index.do">DOT National Transportation Integrated Search</a></p> <p></p> <p>1971-06-01</p> <p>Based on current sizing estimates and tracking algorithms, some computer organizations applicable to future <span class="hlt">air</span> traffic control computing systems are described and assessed. Hardware and software problem areas are defined and solutions are outlined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1177374-tools-large-scale-mobile-malware-analysis','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1177374-tools-large-scale-mobile-malware-analysis"><span>Tools for <span class="hlt">Large-Scale</span> Mobile Malware Analysis</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>Bierma, Michael</p> <p></p> <p>Analyzing mobile applications for malicious behavior is an important area of re- search, and is made di cult, in part, by the increasingly <span class="hlt">large</span> number of appli- cations available for the major operating systems. There are currently over 1.2 million apps available in both the Google Play and Apple App stores (the respec- tive o cial marketplaces for the Android and iOS operating systems)[1, 2]. Our research provides two <span class="hlt">large-scale</span> analysis tools to aid in the detection and analysis of mobile malware. The rst tool we present, Andlantis, is a scalable dynamic analysis system capa- ble of processing over 3000more » Android applications per hour. Traditionally, Android dynamic analysis techniques have been relatively limited in <span class="hlt">scale</span> due to the compu- tational resources required to emulate the full Android system to achieve accurate execution. Andlantis is the most scalable Android dynamic analysis framework to date, and is able to collect valuable forensic data, which helps reverse-engineers and malware researchers identify and understand anomalous application behavior. We discuss the results of running 1261 malware samples through the system, and provide examples of malware analysis performed with the resulting data. While techniques exist to perform static analysis on a <span class="hlt">large</span> number of appli- cations, <span class="hlt">large-scale</span> analysis of iOS applications has been relatively small <span class="hlt">scale</span> due to the closed nature of the iOS ecosystem, and the di culty of acquiring appli- cations for analysis. The second tool we present, iClone, addresses the challenges associated with iOS research in order to detect application clones within a dataset of over 20,000 iOS applications.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19730039237&hterms=principles+information+systems&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dprinciples%2Binformation%2Bsystems','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730039237&hterms=principles+information+systems&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dprinciples%2Binformation%2Bsystems"><span>Stability of <span class="hlt">large-scale</span> systems.</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Siljak, D. D.</p> <p>1972-01-01</p> <p>The purpose of this paper is to present the results obtained in stability study of <span class="hlt">large-scale</span> systems based upon the comparison principle and vector Liapunov functions. The exposition is essentially self-contained, with emphasis on recent innovations which utilize explicit information about the system structure. This provides a natural foundation for the stability theory of dynamic systems under structural perturbations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016E%26ES...39a2050L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016E%26ES...39a2050L"><span>Real-time simulation of <span class="hlt">large-scale</span> floods</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Q.; Qin, Y.; Li, G. D.; Liu, Z.; Cheng, D. J.; Zhao, Y. H.</p> <p>2016-08-01</p> <p>According to the complex real-time water situation, the real-time simulation of <span class="hlt">large-scale</span> floods is very important for flood prevention practice. Model robustness and running efficiency are two critical factors in successful real-time flood simulation. This paper proposed a robust, two-dimensional, shallow water model based on the unstructured Godunov- type finite volume method. A robust wet/dry front method is used to enhance the numerical stability. An adaptive method is proposed to improve the running efficiency. The proposed model is used for <span class="hlt">large-scale</span> flood simulation on real topography. Results compared to those of MIKE21 show the strong performance of the proposed model.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PrICA...1..124W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PrICA...1..124W"><span>Geospatial Augmented Reality for the interactive exploitation of <span class="hlt">large-scale</span> walkable orthoimage maps in museums</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wüest, Robert; Nebiker, Stephan</p> <p>2018-05-01</p> <p>In this paper we present an app framework for augmenting <span class="hlt">large-scale</span> walkable maps and orthoimages in museums or public spaces using standard smartphones and tablets. We first introduce a novel approach for using huge orthoimage mosaic floor prints covering several hundred square meters as natural Augmented Reality (AR) markers. We then present a new app architecture and subsequent tests in the Swissarena of the Swiss National Transport Museum in Lucerne demonstrating the capabilities of accurately tracking and augmenting different map topics, including dynamic 3d data such as live <span class="hlt">air</span> traffic. The resulting prototype was tested with everyday visitors of the museum to get feedback on the usability of the AR app and to identify pitfalls when using AR in the context of a potentially crowded museum. The prototype is to be rolled out to the public after successful testing and optimization of the app. We were able to show that AR apps on standard smartphone devices can dramatically enhance the interactive use of <span class="hlt">large-scale</span> maps for different purposes such as education or serious gaming in a museum context.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JaJAP..57d7001Q','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JaJAP..57d7001Q"><span>A novel bonding method for <span class="hlt">large</span> <span class="hlt">scale</span> poly(methyl methacrylate) micro- and nanofluidic chip fabrication</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Qu, Xingtian; Li, Jinlai; Yin, Zhifu</p> <p>2018-04-01</p> <p>Micro- and nanofluidic chips are becoming increasing significance for biological and medical applications. Future advances in micro- and nanofluidics and its utilization in commercial applications depend on the development and fabrication of low cost and high fidelity <span class="hlt">large</span> <span class="hlt">scale</span> plastic micro- and nanofluidic chips. However, the majority of the present fabrication methods suffer from a low bonding rate of the chip during thermal bonding process due to <span class="hlt">air</span> trapping between the substrate and the cover plate. In the present work, a novel bonding technique based on Ar plasma and water treatment was proposed to fully bond the <span class="hlt">large</span> <span class="hlt">scale</span> micro- and nanofluidic chips. The influence of Ar plasma parameters on the water contact angle and the effect of bonding conditions on the bonding rate and the bonding strength of the chip were studied. The fluorescence tests demonstrate that the 5 × 5 cm2 poly(methyl methacrylate) chip with 180 nm wide and 180 nm deep nanochannels can be fabricated without any block and leakage by our newly developed method.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040082087','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040082087"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Water Vapor Sources Relative to the October 2000 Piedmont Flood</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Turato, Barbara; Reale, Oreste; Siccardi, Franco</p> <p>2003-01-01</p> <p>Very intense mesoscale or synoptic-<span class="hlt">scale</span> rainfall events can occasionally be observed in the Mediterranean region without any deep cyclone developing over the areas affected by precipitation. In these perplexing cases the synoptic situation can superficially look similar to cases in which very little precipitation occurs. These situations could possibly baffle the operational weather forecasters. In this article, the major precipitation event that affected Piedmont (Italy) between 13 and 16 October 2000 is investigated. This is one of the cases in which no intense cyclone was observed within the Mediterranean region at any time, only a moderate system was present, and yet exceptional rainfall and flooding occurred. The emphasis of this study is on the moisture origin and transport. Moisture and energy balances are computed on different space- and time-<span class="hlt">scales</span>, <span class="hlt">revealing</span> that precipitation exceeds evaporation over an area inclusive of Piedmont and the northwestern Mediterranean region, on a time-<span class="hlt">scale</span> encompassing the event and about two weeks preceding it. This is suggestive of an important moisture contribution originating from outside the region. A synoptic and dynamic analysis is then performed to outline the potential mechanisms that could have contributed to the <span class="hlt">large-scale</span> moisture transport. The central part of the work uses a quasi-isentropic water-vapor back trajectory technique. The moisture sources obtained by this technique are compared with the results of the balances and with the synoptic situation, to unveil possible dynamic mechanisms and physical processes involved. It is found that moisture sources on a variety of atmospheric <span class="hlt">scales</span> contribute to this event. First, an important contribution is caused by the extratropical remnants of former tropical storm Leslie. The <span class="hlt">large-scale</span> environment related to this system allows a significant amount of moisture to be carried towards Europe. This happens on a time- <span class="hlt">scale</span> of about 5-15 days preceding the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24483788','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24483788"><span><span class="hlt">Large</span> <span class="hlt">scale</span> anomalies in the microwave background: causation and correlation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Aslanyan, Grigor; Easther, Richard</p> <p>2013-12-27</p> <p>Most treatments of <span class="hlt">large</span> <span class="hlt">scale</span> anomalies in the microwave sky are a posteriori, with unquantified look-elsewhere effects. We contrast these with physical models of specific inhomogeneities in the early Universe which can generate these apparent anomalies. Physical models predict correlations between candidate anomalies and the corresponding signals in polarization and <span class="hlt">large</span> <span class="hlt">scale</span> structure, reducing the impact of cosmic variance. We compute the apparent spatial curvature associated with <span class="hlt">large-scale</span> inhomogeneities and show that it is typically small, allowing for a self-consistent analysis. As an illustrative example we show that a single <span class="hlt">large</span> plane wave inhomogeneity can contribute to low-l mode alignment and odd-even asymmetry in the power spectra and the best-fit model accounts for a significant part of the claimed odd-even asymmetry. We argue that this approach can be generalized to provide a more quantitative assessment of potential <span class="hlt">large</span> <span class="hlt">scale</span> anomalies in the Universe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/21502552-effects-biasing-galaxy-power-spectrum-large-scales','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/21502552-effects-biasing-galaxy-power-spectrum-large-scales"><span>Effects of biasing on the galaxy power spectrum at <span class="hlt">large</span> <span class="hlt">scales</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>Beltran Jimenez, Jose; Departamento de Fisica Teorica, Universidad Complutense de Madrid, 28040, Madrid; Durrer, Ruth</p> <p>2011-05-15</p> <p>In this paper we study the effect of biasing on the power spectrum at <span class="hlt">large</span> <span class="hlt">scales</span>. We show that even though nonlinear biasing does introduce a white noise contribution on <span class="hlt">large</span> <span class="hlt">scales</span>, the P(k){proportional_to}k{sup n} behavior of the matter power spectrum on <span class="hlt">large</span> <span class="hlt">scales</span> may still be visible and above the white noise for about one decade. We show, that the Kaiser biasing scheme which leads to linear bias of the correlation function on <span class="hlt">large</span> <span class="hlt">scales</span>, also generates a linear bias of the power spectrum on rather small <span class="hlt">scales</span>. This is a consequence of the divergence on small <span class="hlt">scales</span> ofmore » the pure Harrison-Zeldovich spectrum. However, biasing becomes k dependent if we damp the underlying power spectrum on small <span class="hlt">scales</span>. We also discuss the effect of biasing on the baryon acoustic oscillations.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20180000566','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20180000566"><span><span class="hlt">Large-Scale</span> Transport Responses to Tropospheric Circulation Changes Using GEOS-5</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Orbe, Clara; Molod, Andrea; Arnold, Nathan; Waugh, Darryn W.; Yang, Huang</p> <p>2017-01-01</p> <p>The mean age since <span class="hlt">air</span> was last at the Northern Hemisphere midlatitude surface is a fundamental property of tropospheric transport. Recent comparisons among chemistry climate models, however, <span class="hlt">reveal</span> that there are <span class="hlt">large</span> differences in the mean age among models and that these differences are most likely related to differences in tropical (parameterized) convection. Here we use aquaplanet simulations of the Goddard Earth Observing System Model Version 5 (GEOS-5) to explore the sensitivity of the mean age to changes in the tropical circulation. Tropical circulation changes are forced by prescribed localized off-equatorial warm sea surface temperature anomalies that (qualitatively) reproduce the convection and circulation differences among the comprehensive models. Idealized chemical species subject to prescribed OH loss are also integrated in parallel in order to illustrate the impact of tropical transport changes on interhemispheric constituent transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27853445','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27853445"><span>Semantic Differential <span class="hlt">Scale</span> Method Can <span class="hlt">Reveal</span> Multi-Dimensional Aspects of Mind Perception.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Takahashi, Hideyuki; Ban, Midori; Asada, Minoru</p> <p>2016-01-01</p> <p>As humans, we tend to perceive minds in both living and non-living entities, such as robots. From a questionnaire developed in a previous mind perception study, authors found that perceived minds could be located on two dimensions "experience" and "agency." This questionnaire allowed the assessment of how we perceive minds of various entities from a multi-dimensional point of view. In this questionnaire, subjects had to evaluate explicit mental capacities of target characters (e.g., capacity to feel hunger). However, we sometimes perceive minds in non-living entities, even though we cannot attribute these evidently biological capacities to the entity. In this study, we performed a <span class="hlt">large-scale</span> web survey to assess mind perception by using the semantic differential <span class="hlt">scale</span> method. We <span class="hlt">revealed</span> that two mind dimensions "emotion" and "intelligence," respectively, corresponded to the two mind dimensions (experience and agency) proposed in a previous mind perception study. We did this without having to ask about specific mental capacities. We believe that the semantic differential <span class="hlt">scale</span> is a useful method to assess the dimensions of mind perception especially for non-living entities that are hard to be attributed to biological capacities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=336800','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=336800"><span>Reduced-form <span class="hlt">air</span> quality modeling for community-<span class="hlt">scale</span> ...</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>Transportation plays an important role in modern society, but its impact on <span class="hlt">air</span> quality has been shown to have significant adverse effects on public health. Numerous reviews (HEI, CDC, WHO) summarizing findings of hundreds of studies conducted mainly in the last decade, conclude that exposures to traffic emissions near roads are a public health concern. The Community LINE Source Model (C-LINE) is a web-based model designed to inform the community user of local <span class="hlt">air</span> quality impacts due to roadway vehicles in their region of interest using a simplified modeling approach. Reduced-form <span class="hlt">air</span> quality modeling is a useful tool for examining what-if scenarios of changes in emissions, such as those due to changes in traffic volume, fleet mix, or vehicle speed. Examining various scenarios of <span class="hlt">air</span> quality impacts in this way can identify potentially at-risk populations located near roadways, and the effects that a change in traffic activity may have on them. C-LINE computes dispersion of primary mobile source pollutants using meteorological conditions for the region of interest and computes <span class="hlt">air</span>-quality concentrations corresponding to these selected conditions. C-LINE functionality has been expanded to model emissions from port-related activities (e.g. ships, trucks, cranes, etc.) in a reduced-form modeling system for local-<span class="hlt">scale</span> near-port <span class="hlt">air</span> quality analysis. This presentation describes the Community modeling tools C-LINE and C-PORT that are intended to be used by local gove</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=338763&Lab=NERL&keyword=physics&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=338763&Lab=NERL&keyword=physics&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>Implementing subgrid-<span class="hlt">scale</span> cloudiness into the Model for Prediction Across <span class="hlt">Scales</span>-Atmosphere (MPAS-A) for next generation global <span class="hlt">air</span> quality modeling</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>A next generation <span class="hlt">air</span> quality modeling system is being developed at the U.S. EPA to enable seamless modeling of <span class="hlt">air</span> quality from global to regional to (eventually) local <span class="hlt">scales</span>. State of the science chemistry and aerosol modules from the Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) mo...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040028040','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040028040"><span>Optical Levitation of Micro-<span class="hlt">Scale</span> Particles in <span class="hlt">Air</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wrbanek, Susan Y.; Weiland, Kenneth E.</p> <p>2004-01-01</p> <p>Success has been achieved using a radiation pressure gradient to levitate microscale particles in <span class="hlt">air</span> for as long as four hours. This work is performed as a precursor to the development of a vacuum based optical tweezers interrogation tool for nanotechnology research. It was decided to first proceed with solving the problem of achieving optical levitation of a micro-<span class="hlt">scale</span> particle in <span class="hlt">air</span> before trying the same in a vacuum environment. This successful optical levitation in <span class="hlt">air</span> confirms the work of Ashkin and Dziedzic. Levitation of 10 and 13.8 microns diameter polystyrene spheres was achieved, as well as the levitation of 10 and 100 microns diameter glass spheres. Particles were raised and lowered. A modicum of success was achieved translating particles horizontally. Trapping of multiple particles in one laser beam has been photographed. Also, it has been observed that particles, that may be conglomerates or irregular in shape, can also be trapped by a focused laser beam. Levitated glass beads were photographed using laser light scattered from the beads. The fact that there is evidence of optical traps in <span class="hlt">air</span> containing irregular and conglomerate particles provides hope that future tool particles need not be perfect spheres.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993AAS...183.6702V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993AAS...183.6702V"><span>Statistical Measures of <span class="hlt">Large-Scale</span> Structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vogeley, Michael; Geller, Margaret; Huchra, John; Park, Changbom; Gott, J. Richard</p> <p>1993-12-01</p> <p>\\inv Mpc} To quantify clustering in the <span class="hlt">large-scale</span> distribution of galaxies and to test theories for the formation of structure in the universe, we apply statistical measures to the CfA Redshift Survey. This survey is complete to m_{B(0)}=15.5 over two contiguous regions which cover one-quarter of the sky and include ~ 11,000 galaxies. The salient features of these data are voids with diameter 30-50\\hmpc and coherent dense structures with a <span class="hlt">scale</span> ~ 100\\hmpc. Comparison with N-body simulations rules out the ``standard" CDM model (Omega =1, b=1.5, sigma_8 =1) at the 99% confidence level because this model has insufficient power on <span class="hlt">scales</span> lambda >30\\hmpc. An unbiased open universe CDM model (Omega h =0.2) and a biased CDM model with non-zero cosmological constant (Omega h =0.24, lambda_0 =0.6) match the observed power spectrum. The amplitude of the power spectrum depends on the luminosity of galaxies in the sample; bright (L>L(*) ) galaxies are more strongly clustered than faint galaxies. The paucity of bright galaxies in low-density regions may explain this dependence. To measure the topology of <span class="hlt">large-scale</span> structure, we compute the genus of isodensity surfaces of the smoothed density field. On <span class="hlt">scales</span> in the ``non-linear" regime, <= 10\\hmpc, the high- and low-density regions are multiply-connected over a broad range of density threshold, as in a filamentary net. On smoothing <span class="hlt">scales</span> >10\\hmpc, the topology is consistent with statistics of a Gaussian random field. Simulations of CDM models fail to produce the observed coherence of structure on non-linear <span class="hlt">scales</span> (>95% confidence level). The underdensity probability (the frequency of regions with density contrast delta rho //lineρ=-0.8) depends strongly on the luminosity of galaxies; underdense regions are significantly more common (>2sigma ) in bright (L>L(*) ) galaxy samples than in samples which include fainter galaxies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19890032233&hterms=string+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dstring%2Btheory','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19890032233&hterms=string+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dstring%2Btheory"><span>Cosmic strings and the <span class="hlt">large-scale</span> structure</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Stebbins, Albert</p> <p>1988-01-01</p> <p>A possible problem for cosmic string models of galaxy formation is presented. If very <span class="hlt">large</span> voids are common and if loop fragmentation is not much more efficient than presently believed, then it may be impossible for string scenarios to produce the observed <span class="hlt">large-scale</span> structure with Omega sub 0 = 1 and without strong environmental biasing.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19780047277&hterms=Krieger&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKrieger','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19780047277&hterms=Krieger&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DKrieger"><span>Coronal hole evolution by sudden <span class="hlt">large</span> <span class="hlt">scale</span> changes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nolte, J. T.; Gerassimenko, M.; Krieger, A. S.; Solodyna, C. V.</p> <p>1978-01-01</p> <p>Sudden shifts in coronal-hole boundaries observed by the S-054 X-ray telescope on Skylab between May and November, 1973, within 1 day of CMP of the holes, at latitudes not exceeding 40 deg, are compared with the long-term evolution of coronal-hole area. It is found that <span class="hlt">large-scale</span> shifts in boundary locations can account for most if not all of the evolution of coronal holes. The temporal and spatial <span class="hlt">scales</span> of these <span class="hlt">large-scale</span> changes imply that they are the results of a physical process occurring in the corona. It is concluded that coronal holes evolve by magnetic-field lines' opening when the holes are growing, and by fields' closing as the holes shrink.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT.......134A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT.......134A"><span>New probes of Cosmic Microwave Background <span class="hlt">large-scale</span> anomalies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Aiola, Simone</p> <p></p> <p>Fifty years of Cosmic Microwave Background (CMB) data played a crucial role in constraining the parameters of the LambdaCDM model, where Dark Energy, Dark Matter, and Inflation are the three most important pillars not yet understood. Inflation prescribes an isotropic universe on <span class="hlt">large</span> <span class="hlt">scales</span>, and it generates spatially-correlated density fluctuations over the whole Hubble volume. CMB temperature fluctuations on <span class="hlt">scales</span> bigger than a degree in the sky, affected by modes on super-horizon <span class="hlt">scale</span> at the time of recombination, are a clean snapshot of the universe after inflation. In addition, the accelerated expansion of the universe, driven by Dark Energy, leaves a hardly detectable imprint in the <span class="hlt">large-scale</span> temperature sky at late times. Such fundamental predictions have been tested with current CMB data and found to be in tension with what we expect from our simple LambdaCDM model. Is this tension just a random fluke or a fundamental issue with the present model? In this thesis, we present a new framework to probe the lack of <span class="hlt">large-scale</span> correlations in the temperature sky using CMB polarization data. Our analysis shows that if a suppression in the CMB polarization correlations is detected, it will provide compelling evidence for new physics on super-horizon <span class="hlt">scale</span>. To further analyze the statistical properties of the CMB temperature sky, we constrain the degree of statistical anisotropy of the CMB in the context of the observed <span class="hlt">large-scale</span> dipole power asymmetry. We find evidence for a <span class="hlt">scale</span>-dependent dipolar modulation at 2.5sigma. To isolate late-time signals from the primordial ones, we test the anomalously high Integrated Sachs-Wolfe effect signal generated by superstructures in the universe. We find that the detected signal is in tension with the expectations from LambdaCDM at the 2.5sigma level, which is somewhat smaller than what has been previously argued. To conclude, we describe the current status of CMB observations on small <span class="hlt">scales</span>, highlighting the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPhCS1001a2017O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPhCS1001a2017O"><span>Exploring the <span class="hlt">large-scale</span> structure of Taylor–Couette turbulence through <span class="hlt">Large</span>-Eddy Simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ostilla-Mónico, Rodolfo; Zhu, Xiaojue; Verzicco, Roberto</p> <p>2018-04-01</p> <p><span class="hlt">Large</span> eddy simulations (LES) of Taylor-Couette (TC) flow, the flow between two co-axial and independently rotating cylinders are performed in an attempt to explore the <span class="hlt">large-scale</span> axially-pinned structures seen in experiments and simulations. Both static and dynamic LES models are used. The Reynolds number is kept fixed at Re = 3.4 · 104, and the radius ratio η = ri /ro is set to η = 0.909, limiting the effects of curvature and resulting in frictional Reynolds numbers of around Re τ ≈ 500. Four rotation ratios from Rot = ‑0.0909 to Rot = 0.3 are simulated. First, the LES of TC is benchmarked for different rotation ratios. Both the Smagorinsky model with a constant of cs = 0.1 and the dynamic model are found to produce reasonable results for no mean rotation and cyclonic rotation, but deviations increase for increasing rotation. This is attributed to the increasing anisotropic character of the fluctuations. Second, “over-damped” LES, i.e. LES with a <span class="hlt">large</span> Smagorinsky constant is performed and is shown to reproduce some features of the <span class="hlt">large-scale</span> structures, even when the near-wall region is not adequately modeled. This shows the potential for using over-damped LES for fast explorations of the parameter space where <span class="hlt">large-scale</span> structures are found.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920074290&hterms=seeds&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dseeds','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920074290&hterms=seeds&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Dseeds"><span><span class="hlt">Large-scale</span> microwave anisotropy from gravitating seeds</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Veeraraghavan, Shoba; Stebbins, Albert</p> <p>1992-01-01</p> <p>Topological defects could have seeded primordial inhomogeneities in cosmological matter. We examine the horizon-<span class="hlt">scale</span> matter and geometry perturbations generated by such seeds in an expanding homogeneous and isotropic universe. Evolving particle horizons generally lead to perturbations around motionless seeds, even when there are compensating initial underdensities in the matter. We describe the pattern of the resulting <span class="hlt">large</span> angular <span class="hlt">scale</span> microwave anisotropy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3948790','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3948790"><span><span class="hlt">Large-Scale</span> Ichthyoplankton and Water Mass Distribution along the South Brazil Shelf</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>de Macedo-Soares, Luis Carlos Pinto; Garcia, Carlos Alberto Eiras; Freire, Andrea Santarosa; Muelbert, José Henrique</p> <p>2014-01-01</p> <p>Ichthyoplankton is an essential component of pelagic ecosystems, and environmental factors play an important role in determining its distribution. We have investigated simultaneous latitudinal and cross-shelf gradients in ichthyoplankton abundance to test the hypothesis that the <span class="hlt">large-scale</span> distribution of fish larvae in the South Brazil Shelf is associated with water mass composition. Vertical plankton tows were collected between 21°27′ and 34°51′S at 107 stations, in austral late spring and early summer seasons. Samples were taken with a conical-cylindrical plankton net from the depth of chlorophyll maxima to the surface in deep stations, or from 10 m from the bottom to the surface in shallow waters. Salinity and temperature were obtained with a CTD/rosette system, which provided seawater for chlorophyll-a and nutrient concentrations. The influence of water mass on larval fish species was studied using Indicator Species Analysis, whereas environmental effects on the distribution of larval fish species were analyzed by Distance-based Redundancy Analysis. Larval fish species were associated with specific water masses: in the north, Sardinella brasiliensis was found in Shelf Water; whereas in the south, Engraulis anchoita inhabited the Plata Plume Water. At the slope, Tropical Water was characterized by the bristlemouth Cyclothone acclinidens. The concurrent analysis showed the importance of both cross-shelf and latitudinal gradients on the <span class="hlt">large-scale</span> distribution of larval fish species. Our findings <span class="hlt">reveal</span> that ichthyoplankton composition and <span class="hlt">large-scale</span> spatial distribution are determined by water mass composition in both latitudinal and cross-shelf gradients. PMID:24614798</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24614798','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24614798"><span><span class="hlt">Large-scale</span> ichthyoplankton and water mass distribution along the South Brazil Shelf.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>de Macedo-Soares, Luis Carlos Pinto; Garcia, Carlos Alberto Eiras; Freire, Andrea Santarosa; Muelbert, José Henrique</p> <p>2014-01-01</p> <p>Ichthyoplankton is an essential component of pelagic ecosystems, and environmental factors play an important role in determining its distribution. We have investigated simultaneous latitudinal and cross-shelf gradients in ichthyoplankton abundance to test the hypothesis that the <span class="hlt">large-scale</span> distribution of fish larvae in the South Brazil Shelf is associated with water mass composition. Vertical plankton tows were collected between 21°27' and 34°51'S at 107 stations, in austral late spring and early summer seasons. Samples were taken with a conical-cylindrical plankton net from the depth of chlorophyll maxima to the surface in deep stations, or from 10 m from the bottom to the surface in shallow waters. Salinity and temperature were obtained with a CTD/rosette system, which provided seawater for chlorophyll-a and nutrient concentrations. The influence of water mass on larval fish species was studied using Indicator Species Analysis, whereas environmental effects on the distribution of larval fish species were analyzed by Distance-based Redundancy Analysis. Larval fish species were associated with specific water masses: in the north, Sardinella brasiliensis was found in Shelf Water; whereas in the south, Engraulis anchoita inhabited the Plata Plume Water. At the slope, Tropical Water was characterized by the bristlemouth Cyclothone acclinidens. The concurrent analysis showed the importance of both cross-shelf and latitudinal gradients on the <span class="hlt">large-scale</span> distribution of larval fish species. Our findings <span class="hlt">reveal</span> that ichthyoplankton composition and <span class="hlt">large-scale</span> spatial distribution are determined by water mass composition in both latitudinal and cross-shelf gradients.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...636333T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...636333T"><span>Dynamics of Disagreement: <span class="hlt">Large-Scale</span> Temporal Network Analysis <span class="hlt">Reveals</span> Negative Interactions in Online Collaboration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tsvetkova, Milena; García-Gavilanes, Ruth; Yasseri, Taha</p> <p>2016-11-01</p> <p>Disagreement and conflict are a fact of social life. However, negative interactions are rarely explicitly declared and recorded and this makes them hard for scientists to study. In an attempt to understand the structural and temporal features of negative interactions in the community, we use complex network methods to analyze patterns in the timing and configuration of reverts of article edits to Wikipedia. We investigate how often and how fast pairs of reverts occur compared to a null model in order to control for patterns that are natural to the content production or are due to the internal rules of Wikipedia. Our results suggest that Wikipedia editors systematically revert the same person, revert back their reverter, and come to defend a reverted editor. We further relate these interactions to the status of the involved editors. Even though the individual reverts might not necessarily be negative social interactions, our analysis points to the existence of certain patterns of negative social dynamics within the community of editors. Some of these patterns have not been previously explored and carry implications for the knowledge collection practice conducted on Wikipedia. Our method can be applied to other <span class="hlt">large-scale</span> temporal collaboration networks to identify the existence of negative social interactions and other social processes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3839459','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3839459"><span>Preventing <span class="hlt">Large-Scale</span> Controlled Substance Diversion From Within the Pharmacy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Martin, Emory S.; Dzierba, Steven H.; Jones, David M.</p> <p>2013-01-01</p> <p><span class="hlt">Large-scale</span> diversion of controlled substances (CS) from within a hospital or heath system pharmacy is a rare but growing problem. It is the responsibility of pharmacy leadership to scrutinize control processes to expose weaknesses. This article reviews examples of <span class="hlt">large-scale</span> diversion incidents and diversion techniques and provides practical strategies to stimulate enhanced CS security within the pharmacy staff. <span class="hlt">Large-scale</span> diversion from within a pharmacy department can be averted by a pharmacist-in-charge who is informed and proactive in taking effective countermeasures. PMID:24421497</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('https://pubs.er.usgs.gov/publication/70004055','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70004055"><span><span class="hlt">Large-scale</span> flow experiments for managing river systems</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Konrad, Christopher P.; Olden, Julian D.; Lytle, David A.; Melis, Theodore S.; Schmidt, John C.; Bray, Erin N.; Freeman, Mary C.; Gido, Keith B.; Hemphill, Nina P.; Kennard, Mark J.; McMullen, Laura E.; Mims, Meryl C.; Pyron, Mark; Robinson, Christopher T.; Williams, John G.</p> <p>2011-01-01</p> <p>Experimental manipulations of streamflow have been used globally in recent decades to mitigate the impacts of dam operations on river systems. Rivers are challenging subjects for experimentation, because they are open systems that cannot be isolated from their social context. We identify principles to address the challenges of conducting effective <span class="hlt">large-scale</span> flow experiments. Flow experiments have both scientific and social value when they help to resolve specific questions about the ecological action of flow with a clear nexus to water policies and decisions. Water managers must integrate new information into operating policies for <span class="hlt">large-scale</span> experiments to be effective. Modeling and monitoring can be integrated with experiments to analyze long-term ecological responses. Experimental design should include spatially extensive observations and well-defined, repeated treatments. <span class="hlt">Large-scale</span> flow manipulations are only a part of dam operations that affect river systems. Scientists can ensure that experimental manipulations continue to be a valuable approach for the scientifically based management of river systems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29697371','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29697371"><span><span class="hlt">Large-scale</span> two-photon imaging <span class="hlt">revealed</span> super-sparse population codes in the V1 superficial layer of awake monkeys.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tang, Shiming; Zhang, Yimeng; Li, Zhihao; Li, Ming; Liu, Fang; Jiang, Hongfei; Lee, Tai Sing</p> <p>2018-04-26</p> <p>One general principle of sensory information processing is that the brain must optimize efficiency by reducing the number of neurons that process the same information. The sparseness of the sensory representations in a population of neurons reflects the efficiency of the neural code. Here, we employ <span class="hlt">large-scale</span> two-photon calcium imaging to examine the responses of a <span class="hlt">large</span> population of neurons within the superficial layers of area V1 with single-cell resolution, while simultaneously presenting a <span class="hlt">large</span> set of natural visual stimuli, to provide the first direct measure of the population sparseness in awake primates. The results show that only 0.5% of neurons respond strongly to any given natural image - indicating a ten-fold increase in the inferred sparseness over previous measurements. These population activities are nevertheless necessary and sufficient to discriminate visual stimuli with high accuracy, suggesting that the neural code in the primary visual cortex is both super-sparse and highly efficient. © 2018, Tang et al.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AIPC.1770c0005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AIPC.1770c0005S"><span>Multi-hole pressure probes to <span class="hlt">air</span> data system for subsonic small-<span class="hlt">scale</span> <span class="hlt">air</span> vehicles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shevchenko, A. M.; Berezin, D. R.; Puzirev, L. N.; Tarasov, A. Z.; Kharitonov, A. M.; Shmakov, A. S.</p> <p>2016-10-01</p> <p>A brief review of research performed to develop multi-hole probes to measure of aerodynamic angles, dynamic head, and static pressure of a flying vehicle. The basis of these works is the application a well-known classical multi-hole pressure probe technique of measuring of a 3D flow to use in the <span class="hlt">air</span> data system. Two multi-hole pressure probes with spherical and hemispherical head to <span class="hlt">air</span>-data system for subsonic small-<span class="hlt">scale</span> vehicles have been developed. A simple analytical probe model with separation of variables is proposed. The probes were calibrated in the wind tunnel, one of them is in-flight tested.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020046818','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020046818"><span>Experimental Simulations of <span class="hlt">Large-Scale</span> Collisions</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Housen, Kevin R.</p> <p>2002-01-01</p> <p>This report summarizes research on the effects of target porosity on the mechanics of impact cratering. Impact experiments conducted on a centrifuge provide direct simulations of <span class="hlt">large-scale</span> cratering on porous asteroids. The experiments show that <span class="hlt">large</span> craters in porous materials form mostly by compaction, with essentially no deposition of material into the ejecta blanket that is a signature of cratering in less-porous materials. The ratio of ejecta mass to crater mass is shown to decrease with increasing crater size or target porosity. These results are consistent with the observation that <span class="hlt">large</span> closely-packed craters on asteroid Mathilde appear to have formed without degradation to earlier craters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27862509','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27862509"><span>Psychometric properties of the <span class="hlt">AIR</span> Self-Determination <span class="hlt">Scale</span>: the Chinese version (<span class="hlt">AIR</span> SDS-C) for Chinese people with intellectual disabilities.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wong, P K S; Wong, D F K; Zhuang, X Y; Liu, Y</p> <p>2017-03-01</p> <p>The construct of self-determination has received considerable attention in the international field of intellectual disabilities (ID). Recently, there has been a rapid development of this construct in Chinese societies including Hong Kong. However, there is no locally validated instrument to measure self-determination in people with ID. This article explains the validation process of the <span class="hlt">AIR</span> Self-Determination <span class="hlt">Scale</span> - Chinese version (<span class="hlt">AIR</span> SDS-C) adapted from the 24-item <span class="hlt">AIR</span> Self-Determination <span class="hlt">Scale</span>, developed by Wolman and his colleagues, which is used in school setting. People with mild/moderate ID aged 15 years or above were recruited from special schools and social services units in different regions of Hong Kong. Factor analysis and reliability tests were conducted. Data for a total of 356 participants were used for the analysis. A confirmatory factor analysis was performed to test the factorial construct, and Mplus 7.0 was used for the analysis. The factor structure proposed in the original English version was supported by the data, and all factor loadings were between 0.42 and 0.76. The whole <span class="hlt">scale</span> achieved good reliability (Cronbach's α = 0.88 and ω = 0.90). The <span class="hlt">AIR</span> SDS-C appears to be a valid and reliable <span class="hlt">scale</span>. This study examined adult groups as well as student groups. The application of the <span class="hlt">scale</span> can thus be extended to a wider population. The implications for theory building and practice are discussed. © 2016 MENCAP and International Association of the Scientific Study of Intellectual and Developmental Disabilities and John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006AcPPB..37.2115K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006AcPPB..37.2115K"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Underground Detectors in Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Katsanevas, S. K.</p> <p>2006-07-01</p> <p>The physics potential and the complementarity of the <span class="hlt">large</span> <span class="hlt">scale</span> underground European detectors: Water Cherenkov (MEMPHYS), Liquid Argon TPC (GLACIER) and Liquid Scintillator (LENA) is presented with emphasis on the major physics opportunities, namely proton decay, supernova detection and neutrino parameter determination using accelerator beams.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012Nanos...4.1636Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012Nanos...4.1636Y"><span>Production of <span class="hlt">large-scale</span>, freestanding vanadium pentoxide nanobelt porous structures</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yun, Yong Ju; Kim, Byung Hoon; Hong, Won G.; Kim, Chang Hee; Kim, Yark Yeon; Jeong, Eun-Ju; Jang, Won Ick; Yu, Han Young</p> <p>2012-02-01</p> <p><span class="hlt">Large-scale</span>, freestanding, porous structures of vanadium pentoxide nanobelts (VPNs) were successfully prepared using the template-free freeze-drying method. The porous and multi-layered VPN macrostructures are composed of randomly oriented long nanobelts (over 100 μm) and their side length can be controlled up to a few tens of centimetres. Also, the bulk density and surface area of these macrostructures are 3-5 mg cm-3 and 40-80 m2 g-1, respectively, which are similar to those of the excellent adsorbents. In addition, the removal efficiency measurements of ammonia molecules <span class="hlt">revealed</span> that the VPN porous structures can adsorb the ammonia molecules with the combinations of van der Waals forces and strong chemical bonding by functional groups on the VPN surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22293666','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22293666"><span>Production of <span class="hlt">large-scale</span>, freestanding vanadium pentoxide nanobelt porous structures.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yun, Yong Ju; Kim, Byung Hoon; Hong, Won G; Kim, Chang Hee; Kim, Yark Yeon; Jeong, Eun-ju; Jang, Won Ick; Yu, Han Young</p> <p>2012-03-07</p> <p><span class="hlt">Large-scale</span>, freestanding, porous structures of vanadium pentoxide nanobelts (VPNs) were successfully prepared using the template-free freeze-drying method. The porous and multi-layered VPN macrostructures are composed of randomly oriented long nanobelts (over 100 μm) and their side length can be controlled up to a few tens of centimetres. Also, the bulk density and surface area of these macrostructures are 3-5 mg cm(-3) and 40-80 m(2) g(-1), respectively, which are similar to those of the excellent adsorbents. In addition, the removal efficiency measurements of ammonia molecules <span class="hlt">revealed</span> that the VPN porous structures can adsorb the ammonia molecules with the combinations of van der Waals forces and strong chemical bonding by functional groups on the VPN surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29031831','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29031831"><span><span class="hlt">Large-scale</span> retrieval for medical image analytics: A comprehensive review.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Li, Zhongyu; Zhang, Xiaofan; Müller, Henning; Zhang, Shaoting</p> <p>2018-01-01</p> <p>Over the past decades, medical image analytics was greatly facilitated by the explosion of digital imaging techniques, where huge amounts of medical images were produced with ever-increasing quality and diversity. However, conventional methods for analyzing medical images have achieved limited success, as they are not capable to tackle the huge amount of image data. In this paper, we review state-of-the-art approaches for <span class="hlt">large-scale</span> medical image analysis, which are mainly based on recent advances in computer vision, machine learning and information retrieval. Specifically, we first present the general pipeline of <span class="hlt">large-scale</span> retrieval, summarize the challenges/opportunities of medical image analytics on a <span class="hlt">large-scale</span>. Then, we provide a comprehensive review of algorithms and techniques relevant to major processes in the pipeline, including feature representation, feature indexing, searching, etc. On the basis of existing work, we introduce the evaluation protocols and multiple applications of <span class="hlt">large-scale</span> medical image retrieval, with a variety of exploratory and diagnostic scenarios. Finally, we discuss future directions of <span class="hlt">large-scale</span> retrieval, which can further improve the performance of medical image analysis. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMSM41D2510C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMSM41D2510C"><span>Penetration of <span class="hlt">Large</span> <span class="hlt">Scale</span> Electric Field to Inner Magnetosphere</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, S. H.; Fok, M. C. H.; Sibeck, D. G.; Wygant, J. R.; Spence, H. E.; Larsen, B.; Reeves, G. D.; Funsten, H. O.</p> <p>2015-12-01</p> <p> simulations <span class="hlt">reveal</span> alternating penetration and shielding electric fields during the main phase of the geomagnetic storm, indicating an impulsive nature of the <span class="hlt">large</span> <span class="hlt">scale</span> penetrating electric field in regulating the gain and loss of radiation belt particles. We will present the statistical analysis and simulations results.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=suicidal+AND+ideation&pg=5&id=EJ966087','ERIC'); return false;" href="https://eric.ed.gov/?q=suicidal+AND+ideation&pg=5&id=EJ966087"><span>Recent Suicidal Ideation and Suicide Attempts in a <span class="hlt">Large-Scale</span> Survey of the U.S. <span class="hlt">Air</span> Force: Prevalences and Demographic Risk Factors</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>Snarr, Jeffery D.; Heyman, Richard E.; Slep, Amy M. Smith</p> <p>2010-01-01</p> <p>One-year prevalences of self-reported noteworthy suicidal ideation and nonfatal suicide attempts were assessed in a <span class="hlt">large</span> sample of U.S. <span class="hlt">Air</span> Force active duty members (N = 52,780). Participants completed the 2006 Community Assessment, which was conducted online. Over 3% of male and 5.5% of female participants reported having experienced noteworthy…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/air-research/kansas-city-transportation-and-local-scale-air-quality-study-kc-traqs-fact-sheet','PESTICIDES'); return false;" href="https://www.epa.gov/air-research/kansas-city-transportation-and-local-scale-air-quality-study-kc-traqs-fact-sheet"><span>Kansas City Transportation and Local-<span class="hlt">Scale</span> <span class="hlt">Air</span> Quality Study (KC-TRAQS) Fact Sheet</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>In fall 2017, the U.S. Environmental Protection Agency (EPA) launched the Kansas City Transportation Local-<span class="hlt">Scale</span> <span class="hlt">Air</span> Quality Study (KC-TRAQS) to learn more about local community <span class="hlt">air</span> quality in three neighborhoods in Kansas City, KS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.H21B1028M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.H21B1028M"><span>A high resolution method for soil moisture mapping at <span class="hlt">large</span> spatial and temporal <span class="hlt">scales</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>moreno, D.; Sayde, C.; Ochsner, T. E.; Sorin, C.; Selker, J. S.</p> <p>2013-12-01</p> <p>Soil moisture is a critical component of the planet's water budget, yet precise measurement of its dynamics across the critical <span class="hlt">scales</span> of 0.1-1,000 m continues to be an area of great uncertainty. Here we present the preliminary results for a <span class="hlt">large</span> <span class="hlt">scale</span> installation of soil moisture quantification based on the work of Sayde et al. (2010) using actively heated fiber optic with a DTS system capable of soil moisture measurements at high spatial (reporting every 0.125 m) and temporal resolution (read as frequently as each 15 min)). The fiber optic (FO) sensing cables were installed in 2 sections: 1) a highly resolved multi-<span class="hlt">scale</span> spiral 75m x 65m in size, 530 m total path length, and 2) a 770 m transect in the foot print of the cosmos cosmic ray probe installed at the site. In each of those 2 sections, the FO cables were deployed at 3 depths: 5, 10, and 15 cm. In this system the FO sensing system provides measurements of soil moisture at >39,000 locations simultaneously for each heat pulse. In addition, six soil monitoring stations along the fiber optic path were installed to provide additional validation and calibration of the DTS data. Finally, gravimetric soil moisture and soil thermal samplings were performed periodically to provide additional distributed validation and calibration of the DTS data. The ability of this DTS FO system to provide soil moisture measurements over four orders of magnitude in spatial <span class="hlt">scale</span> (0.1 - 1,000m) will allow better understanding of the spatio-temporal variability in soil moisture in the field, which is essential to develop protocols for calibration and validation of <span class="hlt">large</span> <span class="hlt">scale</span> soil moisture remote sensing data (such as NASA <span class="hlt">air</span>MOSS soil moisture <span class="hlt">air</span> flights). The material is based upon work supported by NASA under award NNX12AP58G, with equipment and assistance also provided by CTEMPs.org with support from the National Science Foundation under Grant Number 1129003. Any opinions, findings, and conclusions or recommendations expressed</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27013727','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27013727"><span><span class="hlt">Large-scale</span> magnetic fields at high Reynolds numbers in magnetohydrodynamic simulations.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hotta, H; Rempel, M; Yokoyama, T</p> <p>2016-03-25</p> <p>The 11-year solar magnetic cycle shows a high degree of coherence in spite of the turbulent nature of the solar convection zone. It has been found in recent high-resolution magnetohydrodynamics simulations that the maintenance of a <span class="hlt">large-scale</span> coherent magnetic field is difficult with small viscosity and magnetic diffusivity (≲10 (12) square centimenters per second). We reproduced previous findings that indicate a reduction of the energy in the <span class="hlt">large-scale</span> magnetic field for lower diffusivities and demonstrate the recovery of the global-<span class="hlt">scale</span> magnetic field using unprecedentedly high resolution. We found an efficient small-<span class="hlt">scale</span> dynamo that suppresses small-<span class="hlt">scale</span> flows, which mimics the properties of <span class="hlt">large</span> diffusivity. As a result, the global-<span class="hlt">scale</span> magnetic field is maintained even in the regime of small diffusivities-that is, <span class="hlt">large</span> Reynolds numbers. Copyright © 2016, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/960433','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/960433"><span>Prototype Vector Machine for <span class="hlt">Large</span> <span class="hlt">Scale</span> Semi-Supervised Learning</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>Zhang, Kai; Kwok, James T.; Parvin, Bahram</p> <p>2009-04-29</p> <p>Practicaldataminingrarelyfalls exactlyinto the supervisedlearning scenario. Rather, the growing amount of unlabeled data poses a big challenge to <span class="hlt">large-scale</span> semi-supervised learning (SSL). We note that the computationalintensivenessofgraph-based SSLarises <span class="hlt">largely</span> from the manifold or graph regularization, which in turn lead to <span class="hlt">large</span> models that are dificult to handle. To alleviate this, we proposed the prototype vector machine (PVM), a highlyscalable,graph-based algorithm for <span class="hlt">large-scale</span> SSL. Our key innovation is the use of"prototypes vectors" for effcient approximation on both the graph-based regularizer and model representation. The choice of prototypes are grounded upon two important criteria: they not only perform effective low-rank approximation of themore » kernel matrix, but also span a model suffering the minimum information loss compared with the complete model. We demonstrate encouraging performance and appealing <span class="hlt">scaling</span> properties of the PVM on a number of machine learning benchmark data sets.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MNRAS.466.3513S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MNRAS.466.3513S"><span><span class="hlt">Large</span>- to small-<span class="hlt">scale</span> dynamo in domains of <span class="hlt">large</span> aspect ratio: kinematic regime</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Shumaylova, Valeria; Teed, Robert J.; Proctor, Michael R. E.</p> <p>2017-04-01</p> <p>The Sun's magnetic field exhibits coherence in space and time on much larger <span class="hlt">scales</span> than the turbulent convection that ultimately powers the dynamo. In this work, we look for numerical evidence of a <span class="hlt">large-scale</span> magnetic field as the magnetic Reynolds number, Rm, is increased. The investigation is based on the simulations of the induction equation in elongated periodic boxes. The imposed flows considered are the standard ABC flow (named after Arnold, Beltrami & Childress) with wavenumber ku = 1 (small-<span class="hlt">scale</span>) and a modulated ABC flow with wavenumbers ku = m, 1, 1 ± m, where m is the wavenumber corresponding to the long-wavelength perturbation on the <span class="hlt">scale</span> of the box. The critical magnetic Reynolds number R_m^{crit} decreases as the permitted <span class="hlt">scale</span> separation in the system increases, such that R_m^{crit} ∝ [L_x/L_z]^{-1/2}. The results show that the α-effect derived from the mean-field theory ansatz is valid for a small range of Rm after which small <span class="hlt">scale</span> dynamo instability occurs and the mean-field approximation is no longer valid. The transition from <span class="hlt">large</span>- to small-<span class="hlt">scale</span> dynamo is smooth and takes place in two stages: a fast transition into a predominantly small-<span class="hlt">scale</span> magnetic energy state and a slower transition into even smaller <span class="hlt">scales</span>. In the range of Rm considered, the most energetic Fourier component corresponding to the structure in the long x-direction has twice the length-<span class="hlt">scale</span> of the forcing <span class="hlt">scale</span>. The long-wavelength perturbation imposed on the ABC flow in the modulated case is not preserved in the eigenmodes of the magnetic field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMIN51B1814W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMIN51B1814W"><span><span class="hlt">Large-Scale</span>, Multi-Sensor Atmospheric Data Fusion Using Hybrid Cloud Computing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, B. D.; Manipon, G.; Hua, H.; Fetzer, E. J.</p> <p>2015-12-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the "A-Train" platforms (<span class="hlt">AIRS</span>, MODIS, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over decades. Moving to multi-sensor, long-duration presents serious challenges for <span class="hlt">large-scale</span> data mining and fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another (MODIS), and to a model (ECMWF), stratify the comparisons using a classification of the "cloud scenes" from CloudSat, and repeat the entire analysis over 10 years of data. HySDS is a Hybrid-Cloud Science Data System that has been developed and applied under NASA AIST, MEaSUREs, and ACCESS grants. HySDS uses the SciFlow workflow engine to partition analysis workflows into parallel tasks (e.g. segmenting by time or space) that are pushed into a durable job queue. The tasks are "pulled" from the queue by worker Virtual Machines (VM's) and executed in an on-premise Cloud (Eucalyptus or OpenStack) or at Amazon in the public Cloud or govCloud. In this way, years of data (millions of files) can be processed in a massively parallel way. Input variables (arrays) are pulled on-demand into the Cloud using OPeNDAP URLs or other subsetting services, thereby minimizing the size of the transferred data. We are using HySDS to automate the production of multiple versions of a ten-year A-Train water vapor climatology under a MEASURES grant. We will present the architecture of HySDS, describe the achieved "clock time" speedups in fusing datasets on our own nodes and in the Amazon Cloud, and discuss the Cloud cost tradeoffs for storage, compute, and data transfer. Our system demonstrates how one can pull A-Train variables (Levels 2 & 3) on-demand into the Amazon Cloud, and cache only those variables that are heavily used, so that any number of compute jobs can be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..1214485S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..1214485S"><span>Analysis of the ability of <span class="hlt">large-scale</span> reanalysis data to define Siberian fire danger in preparation for future fire prediction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soja, Amber; Westberg, David; Stackhouse, Paul, Jr.; McRae, Douglas; Jin, Ji-Zhong; Sukhinin, Anatoly</p> <p>2010-05-01</p> <p>Fire is the dominant disturbance that precipitates ecosystem change in boreal regions, and fire is <span class="hlt">largely</span> under the control of weather and climate. Fire frequency, fire severity, area burned and fire season length are predicted to increase in boreal regions under current climate change scenarios. Therefore, changes in fire regimes have the potential to compel ecological change, moving ecosystems more quickly towards equilibrium with a new climate. The ultimate goal of this research is to assess the viability of <span class="hlt">large-scale</span> (1°) data to be used to define fire weather danger and fire regimes, so that <span class="hlt">large-scale</span> data can be confidently used to predict future fire regimes using <span class="hlt">large-scale</span> fire weather data, like that available from current Intergovernmental Panel on Climate Change (IPCC) climate change scenarios. In this talk, we intent to: (1) evaluate Fire Weather Indices (FWI) derived using reanalysis and interpolated station data; (2) discuss the advantages and disadvantages of using these distinct data sources; and (3) highlight established relationships between <span class="hlt">large-scale</span> fire weather data, area burned, active fires and ecosystems burned. Specifically, the Canadian Forestry Service (CFS) Fire Weather Index (FWI) will be derived using: (1) NASA Goddard Earth Observing System version 4 (GEOS-4) <span class="hlt">large-scale</span> reanalysis and NASA Global Precipitation Climatology Project (GPCP) data; and National Climatic Data Center (NCDC) surface station-interpolated data. Requirements of the FWI are local noon surface-level <span class="hlt">air</span> temperature, relative humidity, wind speed, and daily (noon-noon) rainfall. GEOS-4 reanalysis and NCDC station-interpolated fire weather indices are generally consistent spatially, temporally and quantitatively. Additionally, increased fire activity coincides with increased FWI ratings in both data products. Relationships have been established between <span class="hlt">large-scale</span> FWI to area burned, fire frequency, ecosystem types, and these can be use to estimate</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29564496','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29564496"><span>Understanding the Patterns and Drivers of <span class="hlt">Air</span> Pollution on Multiple Time <span class="hlt">Scales</span>: The Case of Northern China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Yupeng; Wu, Jianguo; Yu, Deyong; Hao, Ruifang</p> <p>2018-06-01</p> <p>China's rapid economic growth during the past three decades has resulted in a number of environmental problems, including the deterioration of <span class="hlt">air</span> quality. It is necessary to better understand how the spatial pattern of <span class="hlt">air</span> pollutants varies with time <span class="hlt">scales</span> and what drive these changes. To address these questions, this study focused on one of the most heavily <span class="hlt">air</span>-polluted areas in North China. We first quantified the spatial pattern of <span class="hlt">air</span> pollution, and then systematically examined the relationships of <span class="hlt">air</span> pollution to several socioeconomic and climatic factors using the constraint line method, correlation analysis, and stepwise regression on decadal, annual, and seasonal <span class="hlt">scales</span>. Our results indicate that PM 2.5 was the dominant <span class="hlt">air</span> pollutant in the Beijing-Tianjin-Hebei region, while PM 2.5 and PM 10 were both important pollutants in the Agro-pastoral Transitional Zone (APTZ) region. Our statistical analyses suggest that energy consumption and gross domestic product (GDP) in the industry were the most important factors for <span class="hlt">air</span> pollution on the decadal <span class="hlt">scale</span>, but the impacts of climatic factors could also be significant. On the annual and seasonal <span class="hlt">scales</span>, high wind speed, low relative humidity, and long sunshine duration constrained PM 2.5 accumulation; low wind speed and high relative humidity constrained PM 10 accumulation; and short sunshine duration and high wind speed constrained O 3 accumulation. Our study showed that analyses on multiple temporal <span class="hlt">scales</span> are not only necessary to determine key drivers of <span class="hlt">air</span> pollution, but also insightful for understanding the spatial patterns of <span class="hlt">air</span> pollution, which was important for urban planning and <span class="hlt">air</span> pollution control.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018EnMan..61.1048L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018EnMan..61.1048L"><span>Understanding the Patterns and Drivers of <span class="hlt">Air</span> Pollution on Multiple Time <span class="hlt">Scales</span>: The Case of Northern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Yupeng; Wu, Jianguo; Yu, Deyong; Hao, Ruifang</p> <p>2018-06-01</p> <p>China's rapid economic growth during the past three decades has resulted in a number of environmental problems, including the deterioration of <span class="hlt">air</span> quality. It is necessary to better understand how the spatial pattern of <span class="hlt">air</span> pollutants varies with time <span class="hlt">scales</span> and what drive these changes. To address these questions, this study focused on one of the most heavily <span class="hlt">air</span>-polluted areas in North China. We first quantified the spatial pattern of <span class="hlt">air</span> pollution, and then systematically examined the relationships of <span class="hlt">air</span> pollution to several socioeconomic and climatic factors using the constraint line method, correlation analysis, and stepwise regression on decadal, annual, and seasonal <span class="hlt">scales</span>. Our results indicate that PM2.5 was the dominant <span class="hlt">air</span> pollutant in the Beijing-Tianjin-Hebei region, while PM2.5 and PM10 were both important pollutants in the Agro-pastoral Transitional Zone (APTZ) region. Our statistical analyses suggest that energy consumption and gross domestic product (GDP) in the industry were the most important factors for <span class="hlt">air</span> pollution on the decadal <span class="hlt">scale</span>, but the impacts of climatic factors could also be significant. On the annual and seasonal <span class="hlt">scales</span>, high wind speed, low relative humidity, and long sunshine duration constrained PM2.5 accumulation; low wind speed and high relative humidity constrained PM10 accumulation; and short sunshine duration and high wind speed constrained O3 accumulation. Our study showed that analyses on multiple temporal <span class="hlt">scales</span> are not only necessary to determine key drivers of <span class="hlt">air</span> pollution, but also insightful for understanding the spatial patterns of <span class="hlt">air</span> pollution, which was important for urban planning and <span class="hlt">air</span> pollution control.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912955B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912955B"><span>Measuring <span class="hlt">large-scale</span> vertical motion in the atmosphere with dropsondes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bony, Sandrine; Stevens, Bjorn</p> <p>2017-04-01</p> <p><span class="hlt">Large-scale</span> vertical velocity modulates important processes in the atmosphere, including the formation of clouds, and constitutes a key component of the <span class="hlt">large-scale</span> forcing of Single-Column Model simulations and <span class="hlt">Large</span>-Eddy Simulations. Its measurement has also been a long-standing challenge for observationalists. We will show that it is possible to measure the vertical profile of <span class="hlt">large-scale</span> wind divergence and vertical velocity from aircraft by using dropsondes. This methodology was tested in August 2016 during the NARVAL2 campaign in the lower Atlantic trades. Results will be shown for several research flights, the robustness and the uncertainty of measurements will be assessed, ands observational estimates will be compared with data from high-resolution numerical forecasts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27295924','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27295924"><span>Biomass production of multipopulation microalgae in open <span class="hlt">air</span> pond for biofuel potential.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Selvakumar, P; Umadevi, K</p> <p>2016-04-01</p> <p>Biodiesel gains attention as it is made from renewable resources and has considerable environmental benefits. The present investigation has focused on <span class="hlt">large</span> <span class="hlt">scale</span> cultivation of multipopulation microalgae in open <span class="hlt">air</span> pond using natural sea water without any additional nutritive supplements for low cost biomass production as a possible source of biofuel in <span class="hlt">large</span> <span class="hlt">scale</span>. Open <span class="hlt">air</span> algal pond attained average chlorophyll concentration of 11.01 µg/L with the maximum of 43.65 µg/L as well as a higher lipid concentration of 18% (w/w) with lipid content 9.3 mg/L on the 10th day of the culture; and maximum biomass of 0.36 g/L on the 7th day of the culture. Composition analysis of fatty acid methyl ester (FAME) was performed by gas chromatography and mass spectrometry (GCMS). Multipopulation of algal biomass had 18% of total lipid content with 55% of total saturated fatty acids (SFA), 35.3% of monounsaturated fatty acids (MUFA) and 9.7% of polyunsaturated fatty acids (PUFA), <span class="hlt">revealing</span> a potential source of biofuel production at low cost.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18052776','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18052776"><span>Bayesian hierarchical model for <span class="hlt">large-scale</span> covariance matrix estimation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhu, Dongxiao; Hero, Alfred O</p> <p>2007-12-01</p> <p>Many bioinformatics problems implicitly depend on estimating <span class="hlt">large-scale</span> covariance matrix. The traditional approaches tend to give rise to high variance and low accuracy due to "overfitting." We cast the <span class="hlt">large-scale</span> covariance matrix estimation problem into the Bayesian hierarchical model framework, and introduce dependency between covariance parameters. We demonstrate the advantages of our approaches over the traditional approaches using simulations and OMICS data analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1029260-large-scale-experimental-landscapes-reveal-distinctive-effects-patch-shape-connectivity-arthropod-communities','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1029260-large-scale-experimental-landscapes-reveal-distinctive-effects-patch-shape-connectivity-arthropod-communities"><span><span class="hlt">Large-scale</span> experimental landscapes <span class="hlt">reveal</span> distinctive effects of patch shape and connectivity on arthropod communities.</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>Orrock, John, L.; Curler, Gregory, R.; Danielson, Brent, J.</p> <p>2011-09-14</p> <p>The size, shape, and isolation of habitat patches can affect organism behavior and population dynamics, but little is known about the relative role of shape and connectivity in affecting ecological communities at <span class="hlt">large</span> spatial <span class="hlt">scales</span>. Using six sampling sessions from July 2001 until August 2002, we collected 33,685 arthropods throughout seven 12-ha experimental landscapes consisting of clear-cut patches surrounded by a matrix of mature pine forest. Patches were explicitly designed to manipulate connectivity (via habitat corridors) independently of area and edge effects. We found that patch shape, rather than connectivity, affected ground-dwelling arthropod richness and beta diversity (i.e. turnover ofmore » genera among patches). Arthropod communities contained fewer genera and exhibited less turnover in high-edge connected and high-edge unconnected patches relative to low-edge unconnected patches of similar area. Connectivity, rather than patch shape, affected the evenness of ground-dwelling arthropod communities; regardless of patch shape, high-edge connected patches had lower evenness than low- or high-edge unconnected patches. Among the most abundant arthropod orders, increased richness in low-edge unconnected patches was <span class="hlt">largely</span> due to increased richness of Coleoptera, whereas Hymenoptera played an important role in the lower evenness in connected patches and patterns of turnover. These findings suggest that anthropogenic habitat alteration can have distinct effects on ground-dwelling arthropod communities that arise due to changes in shape and connectivity. Moreover, this work suggests that corridors, which are common conservation tools that change both patch shape and connectivity, can have multiple effects on arthropod communities via different mechanisms, and each effect may alter components of community structure.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70025488','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70025488"><span>New insights into Kilauea's volcano dynamics brought by <span class="hlt">large-scale</span> relative relocation of microearthquakes</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Got, J.-L.; Okubo, P.</p> <p>2003-01-01</p> <p>We investigated the microseismicity recorded in an active volcano to infer information concerning the volcano structure and long-term dynamics, by using relative relocations and focal mechanisms of microearthquakes. There were 32,000 earthquakes of the Mauna Loa and Kilauea volcanoes recorded by more than eight stations of the Hawaiian Volcano Observatory seismic network between 1988 and 1999. We studied 17,000 of these events and relocated more than 70%, with an accuracy ranging from 10 to 500 m. About 75% of these relocated events are located in the vicinity of subhorizontal decollement planes, at a depth of 8-11 km. However, the striking features <span class="hlt">revealed</span> by these relocation results are steep southeast dipping fault planes working as reverse faults, clearly located below the decollement plane and which intersect it. If this decollement plane coincides with the pre-Mauna Loa seafloor, as hypothesized by numerous authors, such reverse faults rupture the pre-Mauna Loa oceanic crust. The weight of the volcano and pressure in the magma storage system are possible causes of these ruptures, fully compatible with the local stress tensor computed by Gillard et al. [1996]. Reverse faults are suspected of producing scarps <span class="hlt">revealed</span> by kilometer-long horizontal slip-perpendicular lineations along the decollement surface and therefore <span class="hlt">large-scale</span> roughness, asperities, and normal stress variations. These are capable of generating stick-slip, <span class="hlt">large</span>-magnitude earthquakes, the spatial microseismic pattern observed in the south flank of Kilauea volcano, and Hilina-type instabilities. Rupture intersecting the decollement surface, causing its <span class="hlt">large-scale</span> roughness, may be an important parameter controlling the growth of Hawaiian volcanoes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020017755','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020017755"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Deformation of the Western US Cordillera</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bennett, Richard A.</p> <p>2001-01-01</p> <p>Destructive earthquakes occur throughout the western US Cordillera (WUSC), not just within the San Andreas fault zone. But because we do not understand the present-day <span class="hlt">large-scale</span> deformations of the crust throughout the WUSC, our ability to assess the potential for seismic hazards in this region remains severely limited. To address this problem, we are using a <span class="hlt">large</span> collection of Global Positioning System (GPS) networks which spans the WUSC to precisely quantify present-day <span class="hlt">large-scale</span> crustal deformations in a single uniform reference frame. Our work can roughly be divided into an analysis of the GPS observations to infer the deformation field across and within the entire plate boundary zone and an investigation of the implications of this deformation field regarding plate boundary dynamics.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=career+AND+review&pg=7&id=EJ806429','ERIC'); return false;" href="https://eric.ed.gov/?q=career+AND+review&pg=7&id=EJ806429"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Survey Data in Career Development Research</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>Diemer, Matthew A.</p> <p>2008-01-01</p> <p><span class="hlt">Large</span> <span class="hlt">scale</span> survey datasets have been underutilized but offer numerous advantages for career development scholars, as they contain numerous career development constructs with <span class="hlt">large</span> and diverse samples that are followed longitudinally. Constructs such as work salience, vocational expectations, educational expectations, work satisfaction, and…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015DPS....4741905H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015DPS....4741905H"><span><span class="hlt">Large-Scale</span> Weather Disturbances in Mars’ Southern Extratropics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hollingsworth, Jeffery L.; Kahre, Melinda A.</p> <p>2015-11-01</p> <p>Between late autumn and early spring, Mars’ middle and high latitudes within its atmosphere support strong mean thermal gradients between the tropics and poles. Observations from both the Mars Global Surveyor (MGS) and Mars Reconnaissance Orbiter (MRO) indicate that this strong baroclinicity supports intense, <span class="hlt">large-scale</span> eastward traveling weather systems (i.e., transient synoptic-period waves). These extratropical weather disturbances are key components of the global circulation. Such wave-like disturbances act as agents in the transport of heat and momentum, and generalized scalar/tracer quantities (e.g., atmospheric dust, water-vapor and ice clouds). The character of <span class="hlt">large-scale</span>, traveling extratropical synoptic-period disturbances in Mars' southern hemisphere during late winter through early spring is investigated using a moderately high-resolution Mars global climate model (Mars GCM). This Mars GCM imposes interactively lifted and radiatively active dust based on a threshold value of the surface stress. The model exhibits a reasonable "dust cycle" (i.e., globally averaged, a dustier atmosphere during southern spring and summer occurs). Compared to their northern-hemisphere counterparts, southern synoptic-period weather disturbances and accompanying frontal waves have smaller meridional and zonal <span class="hlt">scales</span>, and are far less intense. Influences of the zonally asymmetric (i.e., east-west varying) topography on southern <span class="hlt">large-scale</span> weather are examined. Simulations that adapt Mars’ full topography compared to simulations that utilize synthetic topographies emulating key <span class="hlt">large-scale</span> features of the southern middle latitudes indicate that Mars’ transient barotropic/baroclinic eddies are highly influenced by the great impact basins of this hemisphere (e.g., Argyre and Hellas). The occurrence of a southern storm zone in late winter and early spring appears to be anchored to the western hemisphere via orographic influences from the Tharsis highlands, and the Argyre</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009HESS...13..467V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009HESS...13..467V"><span>On the relationship between <span class="hlt">large-scale</span> climate modes and regional synoptic patterns that drive Victorian rainfall</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Verdon-Kidd, D. C.; Kiem, A. S.</p> <p>2009-04-01</p> <p>In this paper regional (synoptic) and <span class="hlt">large-scale</span> climate drivers of rainfall are investigated for Victoria, Australia. A non-linear classification methodology known as self-organizing maps (SOM) is used to identify 20 key regional synoptic patterns, which are shown to capture a range of significant synoptic features known to influence the climate of the region. Rainfall distributions are assigned to each of the 20 patterns for nine rainfall stations located across Victoria, resulting in a clear distinction between wet and dry synoptic types at each station. The influence of <span class="hlt">large-scale</span> climate modes on the frequency and timing of the regional synoptic patterns is also investigated. This analysis <span class="hlt">revealed</span> that phase changes in the El Niño Southern Oscillation (ENSO), the Indian Ocean Dipole (IOD) and/or the Southern Annular Mode (SAM) are associated with a shift in the relative frequency of wet and dry synoptic types on an annual to inter-annual timescale. In addition, the relative frequency of synoptic types is shown to vary on a multi-decadal timescale, associated with changes in the Inter-decadal Pacific Oscillation (IPO). Importantly, these results highlight the potential to utilise the link between the regional synoptic patterns derived in this study and <span class="hlt">large-scale</span> climate modes to improve rainfall forecasting for Victoria, both in the short- (i.e. seasonal) and long-term (i.e. decadal/multi-decadal <span class="hlt">scale</span>). In addition, the regional and <span class="hlt">large-scale</span> climate drivers identified in this study provide a benchmark by which the performance of Global Climate Models (GCMs) may be assessed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..1611259W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..1611259W"><span><span class="hlt">Large-Scale</span>, Multi-Sensor Atmospheric Data Fusion Using Hybrid Cloud Computing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, Brian; Manipon, Gerald; Hua, Hook; Fetzer, Eric</p> <p>2014-05-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the "A-Train" platforms (<span class="hlt">AIRS</span>, AMSR-E, MODIS, MISR, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over decades. Moving to multi-sensor, long-duration analyses of important climate variables presents serious challenges for <span class="hlt">large-scale</span> data mining and fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another (MODIS), and to a model (ECMWF), stratify the comparisons using a classification of the "cloud scenes" from CloudSat, and repeat the entire analysis over 10 years of data. To efficiently assemble such datasets, we are utilizing Elastic Computing in the Cloud and parallel map-reduce-based algorithms. However, these problems are Data Intensive computing so the data transfer times and storage costs (for caching) are key issues. SciReduce is a Hadoop-like parallel analysis system, programmed in parallel python, that is designed from the ground up for Earth science. SciReduce executes inside VMWare images and <span class="hlt">scales</span> to any number of nodes in a hybrid Cloud (private eucalyptus & public Amazon). Unlike Hadoop, SciReduce operates on bundles of named numeric arrays, which can be passed in memory or serialized to disk in netCDF4 or HDF5. Multi-year datasets are automatically "sharded" by time and space across a cluster of nodes so that years of data (millions of files) can be processed in a massively parallel way. Input variables (arrays) are pulled on-demand into the Cloud using OPeNDAP URLs or other subsetting services, thereby minimizing the size of the cached input and intermediate datasets. We are using SciReduce to automate the production of multiple versions of a ten-year A-Train water vapor climatology under a NASA MEASURES grant. We will present the architecture of SciReduce, describe the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUSMIN33B..04W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUSMIN33B..04W"><span><span class="hlt">Large-Scale</span>, Parallel, Multi-Sensor Atmospheric Data Fusion Using Cloud Computing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, B. D.; Manipon, G.; Hua, H.; Fetzer, E.</p> <p>2013-05-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the "A-Train" platforms (<span class="hlt">AIRS</span>, AMSR-E, MODIS, MISR, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over decades. Moving to multi-sensor, long-duration analyses of important climate variables presents serious challenges for <span class="hlt">large-scale</span> data mining and fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another (MODIS), and to a model (ECMWF), stratify the comparisons using a classification of the "cloud scenes" from CloudSat, and repeat the entire analysis over 10 years of data. To efficiently assemble such datasets, we are utilizing Elastic Computing in the Cloud and parallel map/reduce-based algorithms. However, these problems are Data Intensive computing so the data transfer times and storage costs (for caching) are key issues. SciReduce is a Hadoop-like parallel analysis system, programmed in parallel python, that is designed from the ground up for Earth science. SciReduce executes inside VMWare images and <span class="hlt">scales</span> to any number of nodes in the Cloud. Unlike Hadoop, SciReduce operates on bundles of named numeric arrays, which can be passed in memory or serialized to disk in netCDF4 or HDF5. Figure 1 shows the architecture of the full computational system, with SciReduce at the core. Multi-year datasets are automatically "sharded" by time and space across a cluster of nodes so that years of data (millions of files) can be processed in a massively parallel way. Input variables (arrays) are pulled on-demand into the Cloud using OPeNDAP URLs or other subsetting services, thereby minimizing the size of the cached input and intermediate datasets. We are using SciReduce to automate the production of multiple versions of a ten-year A-Train water vapor climatology under a NASA MEASURES grant. We will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMIN23A1419W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMIN23A1419W"><span><span class="hlt">Large-Scale</span>, Parallel, Multi-Sensor Atmospheric Data Fusion Using Cloud Computing</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilson, B. D.; Manipon, G.; Hua, H.; Fetzer, E. J.</p> <p>2013-12-01</p> <p>NASA's Earth Observing System (EOS) is an ambitious facility for studying global climate change. The mandate now is to combine measurements from the instruments on the 'A-Train' platforms (<span class="hlt">AIRS</span>, AMSR-E, MODIS, MISR, MLS, and CloudSat) and other Earth probes to enable <span class="hlt">large-scale</span> studies of climate change over decades. Moving to multi-sensor, long-duration analyses of important climate variables presents serious challenges for <span class="hlt">large-scale</span> data mining and fusion. For example, one might want to compare temperature and water vapor retrievals from one instrument (<span class="hlt">AIRS</span>) to another (MODIS), and to a model (MERRA), stratify the comparisons using a classification of the 'cloud scenes' from CloudSat, and repeat the entire analysis over 10 years of data. To efficiently assemble such datasets, we are utilizing Elastic Computing in the Cloud and parallel map/reduce-based algorithms. However, these problems are Data Intensive computing so the data transfer times and storage costs (for caching) are key issues. SciReduce is a Hadoop-like parallel analysis system, programmed in parallel python, that is designed from the ground up for Earth science. SciReduce executes inside VMWare images and <span class="hlt">scales</span> to any number of nodes in the Cloud. Unlike Hadoop, SciReduce operates on bundles of named numeric arrays, which can be passed in memory or serialized to disk in netCDF4 or HDF5. Figure 1 shows the architecture of the full computational system, with SciReduce at the core. Multi-year datasets are automatically 'sharded' by time and space across a cluster of nodes so that years of data (millions of files) can be processed in a massively parallel way. Input variables (arrays) are pulled on-demand into the Cloud using OPeNDAP URLs or other subsetting services, thereby minimizing the size of the cached input and intermediate datasets. We are using SciReduce to automate the production of multiple versions of a ten-year A-Train water vapor climatology under a NASA MEASURES grant. We will</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20050110150&hterms=Solar+still&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DSolar%2Bstill','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20050110150&hterms=Solar+still&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3DSolar%2Bstill"><span>How <span class="hlt">Large</span> <span class="hlt">Scales</span> Flows May Influence Solar Activity</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hathaway, D. H.</p> <p>2004-01-01</p> <p><span class="hlt">Large</span> <span class="hlt">scale</span> flows within the solar convection zone are the primary drivers of the Sun's magnetic activity cycle and play important roles in shaping the Sun's magnetic field. Differential rotation amplifies the magnetic field through its shearing action and converts poloidal field into toroidal field. Poleward meridional flow near the surface carries magnetic flux that reverses the magnetic poles at about the time of solar maximum. The deeper, equatorward meridional flow can carry magnetic flux back toward the lower latitudes where it erupts through the surface to form tilted active regions that convert toroidal fields into oppositely directed poloidal fields. These axisymmetric flows are themselves driven by <span class="hlt">large</span> <span class="hlt">scale</span> convective motions. The effects of the Sun's rotation on convection produce velocity correlations that can maintain both the differential rotation and the meridional circulation. These convective motions can also influence solar activity directly by shaping the magnetic field pattern. While considerable theoretical advances have been made toward understanding these <span class="hlt">large</span> <span class="hlt">scale</span> flows, outstanding problems in matching theory to observations still remain.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013SPIE.8630E..0MD','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013SPIE.8630E..0MD"><span>Optical interconnect for <span class="hlt">large-scale</span> systems</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dress, William</p> <p>2013-02-01</p> <p>This paper presents a switchless, optical interconnect module that serves as a node in a network of identical distribution modules for <span class="hlt">large-scale</span> systems. Thousands to millions of hosts or endpoints may be interconnected by a network of such modules, avoiding the need for multi-level switches. Several common network topologies are reviewed and their <span class="hlt">scaling</span> properties assessed. The concept of message-flow routing is discussed in conjunction with the unique properties enabled by the optical distribution module where it is shown how top-down software control (global routing tables, spanning-tree algorithms) may be avoided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950031802&hterms=structures+cellular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dstructures%2Bcellular','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950031802&hterms=structures+cellular&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dstructures%2Bcellular"><span>Contribution of peculiar shear motions to <span class="hlt">large-scale</span> structure</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mueler, Hans-Reinhard; Treumann, Rudolf A.</p> <p>1994-01-01</p> <p>Self-gravitating shear flow instability simulations in a cold dark matter-dominated expanding Einstein-de Sitter universe have been performed. When the shear flow speed exceeds a certain threshold, self-gravitating Kelvin-Helmoholtz instability occurs, forming density voids and excesses along the shear flow layer which serve as seeds for <span class="hlt">large-scale</span> structure formation. A possible mechanism for generating shear peculiar motions are velocity fluctuations induced by the density perturbations of the postinflation era. In this scenario, short <span class="hlt">scales</span> grow earlier than <span class="hlt">large</span> <span class="hlt">scales</span>. A model of this kind may contribute to the cellular structure of the luminous mass distribution in the universe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..248a2007C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..248a2007C"><span>Performance Study of Salt Cavern <span class="hlt">Air</span> Storage Based Non-Supplementary Fired Compressed <span class="hlt">Air</span> Energy Storage System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chen, Xiaotao; Song, Jie; Liang, Lixiao; Si, Yang; Wang, Le; Xue, Xiaodai</p> <p>2017-10-01</p> <p><span class="hlt">Large-scale</span> energy storage system (ESS) plays an important role in the planning and operation of smart grid and energy internet. Compressed <span class="hlt">air</span> energy storage (CAES) is one of promising <span class="hlt">large-scale</span> energy storage techniques. However, the high cost of the storage of compressed <span class="hlt">air</span> and the low capacity remain to be solved. This paper proposes a novel non-supplementary fired compressed <span class="hlt">air</span> energy storage system (NSF-CAES) based on salt cavern <span class="hlt">air</span> storage to address the issues of <span class="hlt">air</span> storage and the efficiency of CAES. Operating mechanisms of the proposed NSF-CAES are analysed based on thermodynamics principle. Key factors which has impact on the system storage efficiency are thoroughly explored. The energy storage efficiency of the proposed NSF-CAES system can be improved by reducing the maximum working pressure of the salt cavern and improving inlet <span class="hlt">air</span> pressure of the turbine. Simulation results show that the electric-to-electric conversion efficiency of the proposed NSF-CAES can reach 63.29% with a maximum salt cavern working pressure of 9.5 MPa and 9 MPa inlet <span class="hlt">air</span> pressure of the turbine, which is higher than the current commercial CAES plants.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.S33A0845C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.S33A0845C"><span>Numerical simulation of seismic wave propagation from land-excited <span class="hlt">large</span> volume <span class="hlt">air</span>-gun source</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cao, W.; Zhang, W.</p> <p>2017-12-01</p> <p>The land-excited <span class="hlt">large</span> volume <span class="hlt">air</span>-gun source can be used to study regional underground structures and to detect temporal velocity changes. The <span class="hlt">air</span>-gun source is characterized by rich low frequency energy (from bubble oscillation, 2-8Hz) and high repeatability. It can be excited in rivers, reservoirs or man-made pool. Numerical simulation of the seismic wave propagation from the <span class="hlt">air</span>-gun source helps to understand the energy partitioning and characteristics of the waveform records at stations. However, the effective energy recorded at a distance station is from the process of bubble oscillation, which can not be approximated by a single point source. We propose a method to simulate the seismic wave propagation from the land-excited <span class="hlt">large</span> volume <span class="hlt">air</span>-gun source by finite difference method. The process can be divided into three parts: bubble oscillation and source coupling, solid-fluid coupling and the propagation in the solid medium. For the first part, the wavelet of the bubble oscillation can be simulated by bubble model. We use wave injection method combining the bubble wavelet with elastic wave equation to achieve the source coupling. Then, the solid-fluid boundary condition is implemented along the water bottom. And the last part is the seismic wave propagation in the solid medium, which can be readily implemented by the finite difference method. Our method can get accuracy waveform of land-excited <span class="hlt">large</span> volume <span class="hlt">air</span>-gun source. Based on the above forward modeling technology, we analysis the effect of the excited P wave and the energy of converted S wave due to different water shapes. We study two land-excited <span class="hlt">large</span> volume <span class="hlt">air</span>-gun fields, one is Binchuan in Yunnan, and the other is Hutubi in Xinjiang. The station in Binchuan, Yunnan is located in a <span class="hlt">large</span> irregular reservoir, the waveform records have a clear S wave. Nevertheless, the station in Hutubi, Xinjiang is located in a small man-made pool, the waveform records have very weak S wave. Better understanding of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PPCF...55l4011F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PPCF...55l4011F"><span>Exploiting multi-<span class="hlt">scale</span> parallelism for <span class="hlt">large</span> <span class="hlt">scale</span> numerical modelling of laser wakefield accelerators</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fonseca, R. A.; Vieira, J.; Fiuza, F.; Davidson, A.; Tsung, F. S.; Mori, W. B.; Silva, L. O.</p> <p>2013-12-01</p> <p>A new generation of laser wakefield accelerators (LWFA), supported by the extreme accelerating fields generated in the interaction of PW-Class lasers and underdense targets, promises the production of high quality electron beams in short distances for multiple applications. Achieving this goal will rely heavily on numerical modelling to further understand the underlying physics and identify optimal regimes, but <span class="hlt">large</span> <span class="hlt">scale</span> modelling of these scenarios is computationally heavy and requires the efficient use of state-of-the-art petascale supercomputing systems. We discuss the main difficulties involved in running these simulations and the new developments implemented in the OSIRIS framework to address these issues, ranging from multi-dimensional dynamic load balancing and hybrid distributed/shared memory parallelism to the vectorization of the PIC algorithm. We present the results of the OASCR Joule Metric program on the issue of <span class="hlt">large</span> <span class="hlt">scale</span> modelling of LWFA, demonstrating speedups of over 1 order of magnitude on the same hardware. Finally, scalability to over ˜106 cores and sustained performance over ˜2 P Flops is demonstrated, opening the way for <span class="hlt">large</span> <span class="hlt">scale</span> modelling of LWFA scenarios.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25680509','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25680509"><span>[A <span class="hlt">large-scale</span> accident in Alpine terrain].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wildner, M; Paal, P</p> <p>2015-02-01</p> <p>Due to the geographical conditions, <span class="hlt">large-scale</span> accidents amounting to mass casualty incidents (MCI) in Alpine terrain regularly present rescue teams with huge challenges. Using an example incident, specific conditions and typical problems associated with such a situation are presented. The first rescue team members to arrive have the elementary tasks of qualified triage and communication to the control room, which is required to dispatch the necessary additional support. Only with a clear "concept", to which all have to adhere, can the subsequent chaos phase be limited. In this respect, a time factor confounded by adverse weather conditions or darkness represents enormous pressure. Additional hazards are frostbite and hypothermia. If priorities can be established in terms of urgency, then treatment and procedure algorithms have proven successful. For evacuation of causalities, a helicopter should be strived for. Due to the low density of hospitals in Alpine regions, it is often necessary to distribute the patients over a wide area. Rescue operations in Alpine terrain have to be performed according to the particular conditions and require rescue teams to have specific knowledge and expertise. The possibility of a <span class="hlt">large-scale</span> accident should be considered when planning events. With respect to optimization of rescue measures, regular training and exercises are rational, as is the analysis of previous <span class="hlt">large-scale</span> Alpine accidents.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmRe.193...10C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmRe.193...10C"><span><span class="hlt">Large</span>-eddy simulations of a Salt Lake Valley cold-<span class="hlt">air</span> pool</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Crosman, Erik T.; Horel, John D.</p> <p>2017-09-01</p> <p>Persistent cold-<span class="hlt">air</span> pools are often poorly forecast by mesoscale numerical weather prediction models, in part due to inadequate parameterization of planetary boundary-layer physics in stable atmospheric conditions, and also because of errors in the initialization and treatment of the model surface state. In this study, an improved numerical simulation of the 27-30 January 2011 cold-<span class="hlt">air</span> pool in Utah's Great Salt Lake Basin is obtained using a <span class="hlt">large</span>-eddy simulation with more realistic surface state characterization. Compared to a Weather Research and Forecasting model configuration run as a mesoscale model with a planetary boundary-layer scheme where turbulence is highly parameterized, the <span class="hlt">large</span>-eddy simulation more accurately captured turbulent interactions between the stable boundary-layer and flow aloft. The simulations were also found to be sensitive to variations in the Great Salt Lake temperature and Salt Lake Valley snow cover, illustrating the importance of land surface state in modelling cold-<span class="hlt">air</span> pools.</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/21714928','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21714928"><span>How Can the Evidence from Global <span class="hlt">Large-scale</span> Clinical Trials for Cardiovascular Diseases be Improved?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sawata, Hiroshi; Tsutani, Kiichiro</p> <p>2011-06-29</p> <p>Clinical investigations are important for obtaining evidence to improve medical treatment. <span class="hlt">Large-scale</span> clinical trials with thousands of participants are particularly important for this purpose in cardiovascular diseases. Conducting <span class="hlt">large-scale</span> clinical trials entails high research costs. This study sought to investigate global trends in <span class="hlt">large-scale</span> clinical trials in cardiovascular diseases. We searched for trials using clinicaltrials.gov (URL: http://www.clinicaltrials.gov/) using the key words 'cardio' and 'event' in all fields on 10 April, 2010. We then selected trials with 300 or more participants examining cardiovascular diseases. The search <span class="hlt">revealed</span> 344 trials that met our criteria. Of 344 trials, 71% were randomized controlled trials, 15% involved more than 10,000 participants, and 59% were funded by industry. In RCTs whose results were disclosed, 55% of industry-funded trials and 25% of non-industry funded trials reported statistically significant superiority over control (p = 0.012, 2-sided Fisher's exact test). Our findings highlighted concerns regarding potential bias related to funding sources, and that researchers should be aware of the importance of trial information disclosures and conflicts of interest. We should keep considering management and training regarding information disclosures and conflicts of interest for researchers. This could lead to better clinical evidence and further improvements in the development of medical treatment worldwide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1159997-large-scale-anisotropy-stably-stratified-rotating-flows','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1159997-large-scale-anisotropy-stably-stratified-rotating-flows"><span><span class="hlt">Large-scale</span> anisotropy in stably stratified rotating flows</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Marino, R.; Mininni, P. D.; Rosenberg, D. L.; ...</p> <p>2014-08-28</p> <p>We present results from direct numerical simulations of the Boussinesq equations in the presence of rotation and/or stratification, both in the vertical direction. The runs are forced isotropically and randomly at small <span class="hlt">scales</span> and have spatial resolutions of up tomore » $1024^3$ grid points and Reynolds numbers of $$\\approx 1000$$. We first show that solutions with negative energy flux and inverse cascades develop in rotating turbulence, whether or not stratification is present. However, the purely stratified case is characterized instead by an early-time, highly anisotropic transfer to <span class="hlt">large</span> <span class="hlt">scales</span> with almost zero net isotropic energy flux. This is consistent with previous studies that observed the development of vertically sheared horizontal winds, although only at substantially later times. However, and unlike previous works, when sufficient <span class="hlt">scale</span> separation is allowed between the forcing <span class="hlt">scale</span> and the domain size, the total energy displays a perpendicular (horizontal) spectrum with power law behavior compatible with $$\\sim k_\\perp^{-5/3}$$, including in the absence of rotation. In this latter purely stratified case, such a spectrum is the result of a direct cascade of the energy contained in the <span class="hlt">large-scale</span> horizontal wind, as is evidenced by a strong positive flux of energy in the parallel direction at all <span class="hlt">scales</span> including the largest resolved <span class="hlt">scales</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PDU....15...31G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PDU....15...31G"><span>Neutrino footprint in <span class="hlt">large</span> <span class="hlt">scale</span> structure</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garay, Carlos Peña; Verde, Licia; Jimenez, Raul</p> <p>2017-03-01</p> <p>Recent constrains on the sum of neutrino masses inferred by analyzing cosmological data, show that detecting a non-zero neutrino mass is within reach of forthcoming cosmological surveys. Such a measurement will imply a direct determination of the absolute neutrino mass <span class="hlt">scale</span>. Physically, the measurement relies on constraining the shape of the matter power spectrum below the neutrino free streaming <span class="hlt">scale</span>: massive neutrinos erase power at these <span class="hlt">scales</span>. However, detection of a lack of small-<span class="hlt">scale</span> power from cosmological data could also be due to a host of other effects. It is therefore of paramount importance to validate neutrinos as the source of power suppression at small <span class="hlt">scales</span>. We show that, independent on hierarchy, neutrinos always show a footprint on <span class="hlt">large</span>, linear <span class="hlt">scales</span>; the exact location and properties are fully specified by the measured power suppression (an astrophysical measurement) and atmospheric neutrinos mass splitting (a neutrino oscillation experiment measurement). This feature cannot be easily mimicked by systematic uncertainties in the cosmological data analysis or modifications in the cosmological model. Therefore the measurement of such a feature, up to 1% relative change in the power spectrum for extreme differences in the mass eigenstates mass ratios, is a smoking gun for confirming the determination of the absolute neutrino mass <span class="hlt">scale</span> from cosmological observations. It also demonstrates the synergy between astrophysics and particle physics experiments.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017HESS...21.4469A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017HESS...21.4469A"><span><span class="hlt">Large-scale</span> vegetation responses to terrestrial moisture storage changes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrew, Robert L.; Guan, Huade; Batelaan, Okke</p> <p>2017-09-01</p> <p>The normalised difference vegetation index (NDVI) is a useful tool for studying vegetation activity and ecosystem performance at a <span class="hlt">large</span> spatial <span class="hlt">scale</span>. In this study we use the Gravity Recovery and Climate Experiment (GRACE) total water storage (TWS) estimates to examine temporal variability of the NDVI across Australia. We aim to demonstrate a new method that <span class="hlt">reveals</span> the moisture dependence of vegetation cover at different temporal resolutions. Time series of monthly GRACE TWS anomalies are decomposed into different temporal frequencies using a discrete wavelet transform and analysed against time series of the NDVI anomalies in a stepwise regression. The results show that combinations of different frequencies of decomposed GRACE TWS data explain NDVI temporal variations better than raw GRACE TWS alone. Generally, the NDVI appears to be more sensitive to interannual changes in water storage than shorter changes, though grassland-dominated areas are sensitive to higher-frequencies of water-storage changes. Different types of vegetation, defined by areas of land use type, show distinct differences in how they respond to the changes in water storage, which is generally consistent with our physical understanding. This unique method provides useful insight into how the NDVI is affected by changes in water storage at different temporal <span class="hlt">scales</span> across land use types.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19870009445','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19870009445"><span>Sensitivity analysis for <span class="hlt">large-scale</span> problems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Noor, Ahmed K.; Whitworth, Sandra L.</p> <p>1987-01-01</p> <p>The development of efficient techniques for calculating sensitivity derivatives is studied. The objective is to present a computational procedure for calculating sensitivity derivatives as part of performing structural reanalysis for <span class="hlt">large-scale</span> problems. The scope is limited to framed type structures. Both linear static analysis and free-vibration eigenvalue problems are considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/890987-corridors-increase-plant-species-richness-large-scales','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/890987-corridors-increase-plant-species-richness-large-scales"><span>Corridors Increase Plant Species Richness at <span class="hlt">Large</span> <span class="hlt">Scales</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>Damschen, Ellen I.; Haddad, Nick M.; Orrock,John L.</p> <p>2006-09-01</p> <p>Habitat fragmentation is one of the largest threats to biodiversity. Landscape corridors, which are hypothesized to reduce the negative consequences of fragmentation, have become common features of ecological management plans worldwide. Despite their popularity, there is little evidence documenting the effectiveness of corridors in preserving biodiversity at <span class="hlt">large</span> <span class="hlt">scales</span>. Using a <span class="hlt">large-scale</span> replicated experiment, we showed that habitat patches connected by corridors retain more native plant species than do isolated patches, that this difference increases over time, and that corridors do not promote invasion by exotic species. Our results support the use of corridors in biodiversity conservation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16946070','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16946070"><span>Corridors increase plant species richness at <span class="hlt">large</span> <span class="hlt">scales</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Damschen, Ellen I; Haddad, Nick M; Orrock, John L; Tewksbury, Joshua J; Levey, Douglas J</p> <p>2006-09-01</p> <p>Habitat fragmentation is one of the largest threats to biodiversity. Landscape corridors, which are hypothesized to reduce the negative consequences of fragmentation, have become common features of ecological management plans worldwide. Despite their popularity, there is little evidence documenting the effectiveness of corridors in preserving biodiversity at <span class="hlt">large</span> <span class="hlt">scales</span>. Using a <span class="hlt">large-scale</span> replicated experiment, we showed that habitat patches connected by corridors retain more native plant species than do isolated patches, that this difference increases over time, and that corridors do not promote invasion by exotic species. Our results support the use of corridors in biodiversity conservation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10203E..0QE','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10203E..0QE"><span>Comparison of sub-<span class="hlt">scaled</span> to full-<span class="hlt">scaled</span> aircrafts in simulation environment for <span class="hlt">air</span> traffic management</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Elbakary, Mohamed I.; Iftekharuddin, Khan M.; Papelis, Yiannis; Newman, Brett</p> <p>2017-05-01</p> <p><span class="hlt">Air</span> Traffic Management (ATM) concepts are commonly tested in simulation to obtain preliminary results and validate the concepts before adoption. Recently, the researchers found that simulation is not enough because of complexity associated with ATM concepts. In other words, full-<span class="hlt">scale</span> tests must eventually take place to provide compelling performance evidence before adopting full implementation. Testing using full-<span class="hlt">scale</span> aircraft produces a high-cost approach that yields high-confidence results but simulation provides a low-risk/low-cost approach with reduced confidence on the results. One possible approach to increase the confidence of the results and simultaneously reduce the risk and the cost is using unmanned sub-<span class="hlt">scale</span> aircraft in testing new concepts for ATM. This paper presents the simulation results of using unmanned sub-<span class="hlt">scale</span> aircraft in implementing ATM concepts compared to the full <span class="hlt">scale</span> aircraft. The results of simulation show that the performance of sub-<span class="hlt">scale</span> is quite comparable to that of the full-<span class="hlt">scale</span> which validates use of the sub-<span class="hlt">scale</span> in testing new ATM concepts. Keywords: Unmanned</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170003328','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170003328"><span>The Cosmology <span class="hlt">Large</span> Angular <span class="hlt">Scale</span> Surveyor</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Harrington, Kathleen; Marriage, Tobias; Ali, Aamir; Appel, John; Bennett, Charles; Boone, Fletcher; Brewer, Michael; Chan, Manwei; Chuss, David T.; Colazo, Felipe; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170003328'); toggleEditAbsImage('author_20170003328_show'); toggleEditAbsImage('author_20170003328_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170003328_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170003328_hide"></p> <p>2016-01-01</p> <p>The Cosmology <span class="hlt">Large</span> Angular <span class="hlt">Scale</span> Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from inflation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular <span class="hlt">scales</span>. The frequencies of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower frequencies and dust emission at higher frequencies. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular <span class="hlt">scales</span>. Using this combination of a broad frequency range, <span class="hlt">large</span> sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016SPIE.9914E..1KH','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016SPIE.9914E..1KH"><span>The Cosmology <span class="hlt">Large</span> Angular <span class="hlt">Scale</span> Surveyor</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Harrington, Kathleen; Marriage, Tobias; Ali, Aamir; Appel, John W.; Bennett, Charles L.; Boone, Fletcher; Brewer, Michael; Chan, Manwei; Chuss, David T.; Colazo, Felipe; Dahal, Sumit; Denis, Kevin; Dünner, Rolando; Eimer, Joseph; Essinger-Hileman, Thomas; Fluxa, Pedro; Halpern, Mark; Hilton, Gene; Hinshaw, Gary F.; Hubmayr, Johannes; Iuliano, Jeffrey; Karakla, John; McMahon, Jeff; Miller, Nathan T.; Moseley, Samuel H.; Palma, Gonzalo; Parker, Lucas; Petroff, Matthew; Pradenas, Bastián.; Rostem, Karwan; Sagliocca, Marco; Valle, Deniz; Watts, Duncan; Wollack, Edward; Xu, Zhilei; Zeng, Lingzhen</p> <p>2016-07-01</p> <p>The Cosmology <span class="hlt">Large</span> Angular <span class="hlt">Scale</span> Surveyor (CLASS) is a four telescope array designed to characterize relic primordial gravitational waves from in ation and the optical depth to reionization through a measurement of the polarized cosmic microwave background (CMB) on the largest angular <span class="hlt">scales</span>. The frequencies of the four CLASS telescopes, one at 38 GHz, two at 93 GHz, and one dichroic system at 145/217 GHz, are chosen to avoid spectral regions of high atmospheric emission and span the minimum of the polarized Galactic foregrounds: synchrotron emission at lower frequencies and dust emission at higher frequencies. Low-noise transition edge sensor detectors and a rapid front-end polarization modulator provide a unique combination of high sensitivity, stability, and control of systematics. The CLASS site, at 5200 m in the Chilean Atacama desert, allows for daily mapping of up to 70% of the sky and enables the characterization of CMB polarization at the largest angular <span class="hlt">scales</span>. Using this combination of a broad frequency range, <span class="hlt">large</span> sky coverage, control over systematics, and high sensitivity, CLASS will observe the reionization and recombination peaks of the CMB E- and B-mode power spectra. CLASS will make a cosmic variance limited measurement of the optical depth to reionization and will measure or place upper limits on the tensor-to-scalar ratio, r, down to a level of 0.01 (95% C.L.).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27272487','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27272487"><span>Prehospital Acute Stroke Severity <span class="hlt">Scale</span> to Predict <span class="hlt">Large</span> Artery Occlusion: Design and Comparison With Other <span class="hlt">Scales</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hastrup, Sidsel; Damgaard, Dorte; Johnsen, Søren Paaske; Andersen, Grethe</p> <p>2016-07-01</p> <p>We designed and validated a simple prehospital stroke <span class="hlt">scale</span> to identify emergent <span class="hlt">large</span> vessel occlusion (ELVO) in patients with acute ischemic stroke and compared the <span class="hlt">scale</span> to other published <span class="hlt">scales</span> for prediction of ELVO. A national historical test cohort of 3127 patients with information on intracranial vessel status (angiography) before reperfusion therapy was identified. National Institutes of Health Stroke <span class="hlt">Scale</span> (NIHSS) items with the highest predictive value of occlusion of a <span class="hlt">large</span> intracranial artery were identified, and the most optimal combination meeting predefined criteria to ensure usefulness in the prehospital phase was determined. The predictive performance of Prehospital Acute Stroke Severity (PASS) <span class="hlt">scale</span> was compared with other published <span class="hlt">scales</span> for ELVO. The PASS <span class="hlt">scale</span> was composed of 3 NIHSS scores: level of consciousness (month/age), gaze palsy/deviation, and arm weakness. In derivation of PASS 2/3 of the test cohort was used and showed accuracy (area under the curve) of 0.76 for detecting <span class="hlt">large</span> arterial occlusion. Optimal cut point ≥2 abnormal scores showed: sensitivity=0.66 (95% CI, 0.62-0.69), specificity=0.83 (0.81-0.85), and area under the curve=0.74 (0.72-0.76). Validation on 1/3 of the test cohort showed similar performance. Patients with a <span class="hlt">large</span> artery occlusion on angiography with PASS ≥2 had a median NIHSS score of 17 (interquartile range=6) as opposed to PASS <2 with a median NIHSS score of 6 (interquartile range=5). The PASS <span class="hlt">scale</span> showed equal performance although more simple when compared with other <span class="hlt">scales</span> predicting ELVO. The PASS <span class="hlt">scale</span> is simple and has promising accuracy for prediction of ELVO in the field. © 2016 American Heart Association, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/21062654','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/21062654"><span>Facilitating <span class="hlt">large-scale</span> clinical trials: in Asia.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Choi, Han Yong; Ko, Jae-Wook</p> <p>2010-01-01</p> <p>The number of clinical trials conducted in Asian countries has started to increase as a result of expansion of the pharmaceutical market in this area. There is a growing opportunity for <span class="hlt">large-scale</span> clinical trials because of the <span class="hlt">large</span> number of patients, significant market potential, good quality of data, and the cost effective and qualified medical infrastructure. However, for carrying out <span class="hlt">large-scale</span> clinical trials in Asia, there are several major challenges, including the quality control of data, budget control, laboratory validation, monitoring capacity, authorship, staff training, and nonstandard treatment that need to be considered. There are also several difficulties in collaborating on international trials in Asia because Asia is an extremely diverse continent. The major challenges are language differences, diversity of patterns of disease, and current treatments, a <span class="hlt">large</span> gap in the experience with performing multinational trials, and regulatory differences among the Asian countries. In addition, there are also differences in the understanding of global clinical trials, medical facilities, indemnity assurance, and culture, including food and religion. To make regional and local data provide evidence for efficacy through the standardization of these differences, unlimited effort is required. At this time, there are no <span class="hlt">large</span> clinical trials led by urologists in Asia, but it is anticipated that the role of urologists in clinical trials will continue to increase. Copyright © 2010 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27275008','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27275008"><span>Rank Order Coding: a Retinal Information Decoding Strategy <span class="hlt">Revealed</span> by <span class="hlt">Large-Scale</span> Multielectrode Array Retinal Recordings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Portelli, Geoffrey; Barrett, John M; Hilgen, Gerrit; Masquelier, Timothée; Maccione, Alessandro; Di Marco, Stefano; Berdondini, Luca; Kornprobst, Pierre; Sernagor, Evelyne</p> <p>2016-01-01</p> <p>How a population of retinal ganglion cells (RGCs) encodes the visual scene remains an open question. Going beyond individual RGC coding strategies, results in salamander suggest that the relative latencies of a RGC pair encode spatial information. Thus, a population code based on this concerted spiking could be a powerful mechanism to transmit visual information rapidly and efficiently. Here, we tested this hypothesis in mouse by recording simultaneous light-evoked responses from hundreds of RGCs, at pan-retinal level, using a new generation of <span class="hlt">large-scale</span>, high-density multielectrode array consisting of 4096 electrodes. Interestingly, we did not find any RGCs exhibiting a clear latency tuning to the stimuli, suggesting that in mouse, individual RGC pairs may not provide sufficient information. We show that a significant amount of information is encoded synergistically in the concerted spiking of <span class="hlt">large</span> RGC populations. Thus, the RGC population response described with relative activities, or ranks, provides more relevant information than classical independent spike count- or latency- based codes. In particular, we report for the first time that when considering the relative activities across the whole population, the wave of first stimulus-evoked spikes is an accurate indicator of stimulus content. We show that this coding strategy coexists with classical neural codes, and that it is more efficient and faster. Overall, these novel observations suggest that already at the level of the retina, concerted spiking provides a reliable and fast strategy to rapidly transmit new visual scenes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4063973','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4063973"><span>Systematic Phenotyping of a <span class="hlt">Large-Scale</span> Candida glabrata Deletion Collection <span class="hlt">Reveals</span> Novel Antifungal Tolerance Genes</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Hiller, Ekkehard; Istel, Fabian; Tscherner, Michael; Brunke, Sascha; Ames, Lauren; Firon, Arnaud; Green, Brian; Cabral, Vitor; Marcet-Houben, Marina; Jacobsen, Ilse D.; Quintin, Jessica; Seider, Katja; Frohner, Ingrid; Glaser, Walter; Jungwirth, Helmut; Bachellier-Bassi, Sophie; Chauvel, Murielle; Zeidler, Ute; Ferrandon, Dominique; Gabaldón, Toni; Hube, Bernhard; d'Enfert, Christophe; Rupp, Steffen; Cormack, Brendan; Haynes, Ken; Kuchler, Karl</p> <p>2014-01-01</p> <p>The opportunistic fungal pathogen Candida glabrata is a frequent cause of candidiasis, causing infections ranging from superficial to life-threatening disseminated disease. The inherent tolerance of C. glabrata to azole drugs makes this pathogen a serious clinical threat. To identify novel genes implicated in antifungal drug tolerance, we have constructed a <span class="hlt">large-scale</span> C. glabrata deletion library consisting of 619 unique, individually bar-coded mutant strains, each lacking one specific gene, all together representing almost 12% of the genome. Functional analysis of this library in a series of phenotypic and fitness assays identified numerous genes required for growth of C. glabrata under normal or specific stress conditions, as well as a number of novel genes involved in tolerance to clinically important antifungal drugs such as azoles and echinocandins. We identified 38 deletion strains displaying strongly increased susceptibility to caspofungin, 28 of which encoding proteins that have not previously been linked to echinocandin tolerance. Our results demonstrate the potential of the C. glabrata mutant collection as a valuable resource in functional genomics studies of this important fungal pathogen of humans, and to facilitate the identification of putative novel antifungal drug target and virulence genes. PMID:24945925</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/AD1051283','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/AD1051283"><span>Mems: Platform for <span class="hlt">Large-Scale</span> Integrated Vacuum Electronic Circuits</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2017-03-20</p> <p>SECURITY CLASSIFICATION OF: The objective of the LIVEC advanced study project was to develop a platform for <span class="hlt">large-scale</span> integrated vacuum electronic ...Distribution Unlimited UU UU UU UU 20-03-2017 1-Jul-2014 30-Jun-2015 Final Report: MEMS Platform for <span class="hlt">Large-Scale</span> Integrated Vacuum Electronic ... Electronic Circuits (LIVEC) Contract No: W911NF-14-C-0093 COR Dr. James Harvey U.S. ARO RTP, NC 27709-2211 Phone: 702-696-2533 e-mail</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930030027&hterms=inflation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dinflation','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930030027&hterms=inflation&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dinflation"><span>Latest COBE results, <span class="hlt">large-scale</span> data, and predictions of inflation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kashlinsky, A.</p> <p>1992-01-01</p> <p>One of the predictions of the inflationary scenario of cosmology is that the initial spectrum of primordial density fluctuations (PDFs) must have the Harrison-Zeldovich (HZ) form. Here, in order to test the inflationary scenario, predictions of the microwave background radiation (MBR) anisotropies measured by COBE are computed based on <span class="hlt">large-scale</span> data for the universe and assuming Omega-1 and the HZ spectrum on <span class="hlt">large</span> <span class="hlt">scales</span>. It is found that the minimal <span class="hlt">scale</span> where the spectrum can first enter the HZ regime is found, constraining the power spectrum of the mass distribution to within the bias factor b. This factor is determined and used to predict parameters of the MBR anisotropy field. For the spectrum of PDFs that reaches the HZ regime immediately after the <span class="hlt">scale</span> accessible to the APM catalog, the numbers on MBR anisotropies are consistent with the COBE detections and thus the standard inflation can indeed be considered a viable theory for the origin of the <span class="hlt">large-scale</span> structure in the universe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/EJ980462.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/EJ980462.pdf"><span>Managing Risk and Uncertainty in <span class="hlt">Large-Scale</span> University Research Projects</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>Moore, Sharlissa; Shangraw, R. F., Jr.</p> <p>2011-01-01</p> <p>Both publicly and privately funded research projects managed by universities are growing in size and scope. Complex, <span class="hlt">large-scale</span> projects (over $50 million) pose new management challenges and risks for universities. This paper explores the relationship between project success and a variety of factors in <span class="hlt">large-scale</span> university projects. First, we…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3976248','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3976248"><span>Parallel Clustering Algorithm for <span class="hlt">Large-Scale</span> Biological Data Sets</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Wang, Minchao; Zhang, Wu; Ding, Wang; Dai, Dongbo; Zhang, Huiran; Xie, Hao; Chen, Luonan; Guo, Yike; Xie, Jiang</p> <p>2014-01-01</p> <p>Backgrounds Recent explosion of biological data brings a great challenge for the traditional clustering algorithms. With increasing <span class="hlt">scale</span> of data sets, much larger memory and longer runtime are required for the cluster identification problems. The affinity propagation algorithm outperforms many other classical clustering algorithms and is widely applied into the biological researches. However, the time and space complexity become a great bottleneck when handling the <span class="hlt">large-scale</span> data sets. Moreover, the similarity matrix, whose constructing procedure takes long runtime, is required before running the affinity propagation algorithm, since the algorithm clusters data sets based on the similarities between data pairs. Methods Two types of parallel architectures are proposed in this paper to accelerate the similarity matrix constructing procedure and the affinity propagation algorithm. The memory-shared architecture is used to construct the similarity matrix, and the distributed system is taken for the affinity propagation algorithm, because of its <span class="hlt">large</span> memory size and great computing capacity. An appropriate way of data partition and reduction is designed in our method, in order to minimize the global communication cost among processes. Result A speedup of 100 is gained with 128 cores. The runtime is reduced from serval hours to a few seconds, which indicates that parallel algorithm is capable of handling <span class="hlt">large-scale</span> data sets effectively. The parallel affinity propagation also achieves a good performance when clustering <span class="hlt">large-scale</span> gene data (microarray) and detecting families in <span class="hlt">large</span> protein superfamilies. PMID:24705246</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=Programming+AND+paradigm&pg=2&id=ED526667','ERIC'); return false;" href="https://eric.ed.gov/?q=Programming+AND+paradigm&pg=2&id=ED526667"><span>Efficient On-Demand Operations in <span class="hlt">Large-Scale</span> Infrastructures</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>Ko, Steven Y.</p> <p>2009-01-01</p> <p>In <span class="hlt">large-scale</span> distributed infrastructures such as clouds, Grids, peer-to-peer systems, and wide-area testbeds, users and administrators typically desire to perform "on-demand operations" that deal with the most up-to-date state of the infrastructure. However, the <span class="hlt">scale</span> and dynamism present in the operating environment make it challenging to…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=160385&keyword=fluid+AND+cfd&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=160385&keyword=fluid+AND+cfd&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>A FRAMEWORK FOR FINE-<span class="hlt">SCALE</span> COMPUTATIONAL FLUID DYNAMICS <span class="hlt">AIR</span> QUALITY MODELING AND ANALYSIS</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>Fine-<span class="hlt">scale</span> Computational Fluid Dynamics (CFD) simulation of pollutant concentrations within roadway and building microenvironments is feasible using high performance computing. Unlike currently used regulatory <span class="hlt">air</span> quality models, fine-<span class="hlt">scale</span> CFD simulations are able to account rig...</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/2009JGRE..114.2005S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009JGRE..114.2005S"><span><span class="hlt">Scaling</span> relations for <span class="hlt">large</span> Martian valleys</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Som, Sanjoy M.; Montgomery, David R.; Greenberg, Harvey M.</p> <p>2009-02-01</p> <p>The dendritic morphology of Martian valley networks, particularly in the Noachian highlands, has long been argued to imply a warmer, wetter early Martian climate, but the character and extent of this period remains controversial. We analyzed <span class="hlt">scaling</span> relations for the 10 <span class="hlt">large</span> valley systems incised in terrain of various ages, resolvable using the Mars Orbiter Laser Altimeter (MOLA) and the Thermal Emission Imaging System (THEMIS). Four of the valleys originate in point sources with negligible contributions from tributaries, three are very poorly dissected with a few <span class="hlt">large</span> tributaries separated by long uninterrupted trunks, and three exhibit the dendritic, branching morphology typical of terrestrial channel networks. We generated width-area and slope-area relationships for each because these relations are identified as either theoretically predicted or robust terrestrial empiricisms for graded precipitation-fed, perennial channels. We also generated distance-area relationships (Hack's law) because they similarly represent robust characteristics of terrestrial channels (whether perennial or ephemeral). We find that the studied Martian valleys, even the dendritic ones, do not satisfy those empiricisms. On Mars, the width-area <span class="hlt">scaling</span> exponent b of -0.7-4.7 contrasts with values of 0.3-0.6 typical of terrestrial channels; the slope-area <span class="hlt">scaling</span> exponent $\\theta$ ranges from -25.6-5.5, whereas values of 0.3-0.5 are typical on Earth; the length-area, or Hack's exponent n ranges from 0.47 to 19.2, while values of 0.5-0.6 are found on Earth. None of the valleys analyzed satisfy all three relations typical of terrestrial perennial channels. As such, our analysis supports the hypotheses that ephemeral and/or immature channel morphologies provide the closest terrestrial analogs to the dendritic networks on Mars, and point source discharges provide terrestrial analogs best suited to describe the other <span class="hlt">large</span> Martian valleys.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH41B2763L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH41B2763L"><span><span class="hlt">Large-scale</span> particle acceleration by magnetic reconnection during solar flares</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, X.; Guo, F.; Li, H.; Li, G.; Li, S.</p> <p>2017-12-01</p> <p>Magnetic reconnection that triggers explosive magnetic energy release has been widely invoked to explain the <span class="hlt">large-scale</span> particle acceleration during solar flares. While great efforts have been spent in studying the acceleration mechanism in small-<span class="hlt">scale</span> kinetic simulations, there have been rare studies that make predictions to acceleration in the <span class="hlt">large</span> <span class="hlt">scale</span> comparable to the flare reconnection region. Here we present a new arrangement to study this problem. We solve the <span class="hlt">large-scale</span> energetic-particle transport equation in the fluid velocity and magnetic fields from high-Lundquist-number MHD simulations of reconnection layers. This approach is based on examining the dominant acceleration mechanism and pitch-angle scattering in kinetic simulations. Due to the fluid compression in reconnection outflows and merging magnetic islands, particles are accelerated to high energies and develop power-law energy distributions. We find that the acceleration efficiency and power-law index depend critically on upstream plasma beta and the magnitude of guide field (the magnetic field component perpendicular to the reconnecting component) as they influence the compressibility of the reconnection layer. We also find that the accelerated high-energy particles are mostly concentrated in <span class="hlt">large</span> magnetic islands, making the islands a source of energetic particles and high-energy emissions. These findings may provide explanations for acceleration process in <span class="hlt">large-scale</span> magnetic reconnection during solar flares and the temporal and spatial emission properties observed in different flare events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29330495','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29330495"><span><span class="hlt">Large</span> unexplained suite of chemically reactive compounds present in ambient <span class="hlt">air</span> due to biomass fires.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kumar, V; Chandra, B P; Sinha, V</p> <p>2018-01-12</p> <p>Biomass fires impact global atmospheric chemistry. The reactive compounds emitted and formed due to biomass fires drive ozone and organic aerosol formation, affecting both <span class="hlt">air</span> quality and climate. Direct hydroxyl (OH) Reactivity measurements quantify total gaseous reactive pollutant loadings and comparison with measured compounds yields the fraction of unmeasured compounds. Here, we quantified the magnitude and composition of total OH reactivity in the north-west Indo-Gangetic Plain. More than 120% increase occurred in total OH reactivity (28 s -1 to 64 s -1 ) and from no missing OH reactivity in the normal summertime <span class="hlt">air</span>, the missing OH reactivity fraction increased to ~40 % in the post-harvest summertime period influenced by <span class="hlt">large</span> <span class="hlt">scale</span> biomass fires highlighting presence of unmeasured compounds. Increased missing OH reactivity between the two summertime periods was associated with increased concentrations of compounds with strong photochemical source such as acetaldehyde, acetone, hydroxyacetone, nitromethane, amides, isocyanic acid and primary emissions of acetonitrile and aromatic compounds. Currently even the most detailed state-of-the art atmospheric chemistry models exclude formamide, acetamide, nitromethane and isocyanic acid and their highly reactive precursor alkylamines (e.g. methylamine, ethylamine, dimethylamine, trimethylamine). For improved understanding of atmospheric chemistry-<span class="hlt">air</span> quality-climate feedbacks in biomass-fire impacted atmospheric environments, future studies should include these compounds.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880010922','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880010922"><span><span class="hlt">Large-Scale</span> Advanced Prop-Fan (LAP)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Degeorge, C. L.</p> <p>1988-01-01</p> <p>In recent years, considerable attention has been directed toward improving aircraft fuel efficiency. Analytical studies and research with wind tunnel models have demonstrated that the high inherent efficiency of low speed turboprop propulsion systems may now be extended to the Mach .8 flight regime of today's commercial airliners. This can be accomplished with a propeller, employing a <span class="hlt">large</span> number of thin highly swept blades. The term Prop-Fan has been coined to describe such a propulsion system. In 1983 the NASA-Lewis Research Center contracted with Hamilton Standard to design, build and test a near full <span class="hlt">scale</span> Prop-Fan, designated the <span class="hlt">Large</span> <span class="hlt">Scale</span> Advanced Prop-Fan (LAP). This report provides a detailed description of the LAP program. The assumptions and analytical procedures used in the design of Prop-Fan system components are discussed in detail. The manufacturing techniques used in the fabrication of the Prop-Fan are presented. Each of the tests run during the course of the program are also discussed and the major conclusions derived from them stated.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1210150-exact-differential-large-scale-traffic-simulation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1210150-exact-differential-large-scale-traffic-simulation"><span>Exact-Differential <span class="hlt">Large-Scale</span> Traffic Simulation</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>Hanai, Masatoshi; Suzumura, Toyotaro; Theodoropoulos, Georgios</p> <p>2015-01-01</p> <p>Analyzing <span class="hlt">large-scale</span> traffics by simulation needs repeating execution many times with various patterns of scenarios or parameters. Such repeating execution brings about big redundancy because the change from a prior scenario to a later scenario is very minor in most cases, for example, blocking only one of roads or changing the speed limit of several roads. In this paper, we propose a new redundancy reduction technique, called exact-differential simulation, which enables to simulate only changing scenarios in later execution while keeping exactly same results as in the case of whole simulation. The paper consists of two main efforts: (i) amore » key idea and algorithm of the exact-differential simulation, (ii) a method to build <span class="hlt">large-scale</span> traffic simulation on the top of the exact-differential simulation. In experiments of Tokyo traffic simulation, the exact-differential simulation shows 7.26 times as much elapsed time improvement in average and 2.26 times improvement even in the worst case as the whole simulation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900037422&hterms=polska&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpolska','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900037422&hterms=polska&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dpolska"><span>Local gravity and <span class="hlt">large-scale</span> structure</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Juszkiewicz, Roman; Vittorio, Nicola; Wyse, Rosemary F. G.</p> <p>1990-01-01</p> <p>The magnitude and direction of the observed dipole anisotropy of the galaxy distribution can in principle constrain the amount of <span class="hlt">large-scale</span> power present in the spectrum of primordial density fluctuations. This paper confronts the data, provided by a recent redshift survey of galaxies detected by the IRAS satellite, with the predictions of two cosmological models with very different levels of <span class="hlt">large-scale</span> power: the biased Cold Dark Matter dominated model (CDM) and a baryon-dominated model (BDM) with isocurvature initial conditions. Model predictions are investigated for the Local Group peculiar velocity, v(R), induced by mass inhomogeneities distributed out to a given radius, R, for R less than about 10,000 km/s. Several convergence measures for v(R) are developed, which can become powerful cosmological tests when deep enough samples become available. For the present data sets, the CDM and BDM predictions are indistinguishable at the 2 sigma level and both are consistent with observations. A promising discriminant between cosmological models is the misalignment angle between v(R) and the apex of the dipole anisotropy of the microwave background.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EEEV...11..391W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EEEV...11..391W"><span>Feasibility study of a <span class="hlt">large-scale</span> tuned mass damper with eddy current damping mechanism</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Zhihao; Chen, Zhengqing; Wang, Jianhui</p> <p>2012-09-01</p> <p>Tuned mass dampers (TMDs) have been widely used in recent years to mitigate structural vibration. However, the damping mechanisms employed in the TMDs are mostly based on viscous dampers, which have several well-known disadvantages, such as oil leakage and difficult adjustment of damping ratio for an operating TMD. Alternatively, eddy current damping (ECD) that does not require any contact with the main structure is a potential solution. This paper discusses the design, analysis, manufacture and testing of a <span class="hlt">large-scale</span> horizontal TMD based on ECD. First, the theoretical model of ECD is formulated, then one <span class="hlt">large-scale</span> horizontal TMD using ECD is constructed, and finally performance tests of the TMD are conducted. The test results show that the proposed TMD has a very low intrinsic damping ratio, while the damping ratio due to ECD is the dominant damping source, which can be as <span class="hlt">large</span> as 15% in a proper configuration. In addition, the damping ratios estimated with the theoretical model are roughly consistent with those identified from the test results, and the source of this error is investigated. Moreover, it is demonstrated that the damping ratio in the proposed TMD can be easily adjusted by varying the <span class="hlt">air</span> gap between permanent magnets and conductive plates. In view of practical applications, possible improvements and feasibility considerations for the proposed TMD are then discussed. It is confirmed that the proposed TMD with ECD is reliable and feasible for use in structural vibration control.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=holistic+AND+management&pg=5&id=EJ1038123','ERIC'); return false;" href="https://eric.ed.gov/?q=holistic+AND+management&pg=5&id=EJ1038123"><span>Comprehensive School Teachers' Professional Agency in <span class="hlt">Large-Scale</span> Educational Change</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>Pyhältö, Kirsi; Pietarinen, Janne; Soini, Tiina</p> <p>2014-01-01</p> <p>This article explores how comprehensive school teachers' sense of professional agency changes in the context of <span class="hlt">large-scale</span> national educational change in Finland. We analysed the premises on which teachers (n = 100) view themselves and their work in terms of developing their own school, catalysed by the <span class="hlt">large-scale</span> national change. The study…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080031650','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080031650"><span>Previously Unrecognized <span class="hlt">Large</span> Lunar Impact Basins <span class="hlt">Revealed</span> by Topographic Data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Frey, Herbert V.</p> <p>2008-01-01</p> <p>The discovery of a <span class="hlt">large</span> population of apparently buried impact craters on Mars, <span class="hlt">revealed</span> as Quasi- Circular Depressions (QCDs) in Mars Orbiting Laser Altimeter (MOLA) data [1,2,3] and as Circular Thin Areas (CTAs) [4] in crustal thickness model data [5] leads to the obvious question: are there unrecognized impact features on the Moon and other bodies in the solar system? Early analysis of Clementine topography <span class="hlt">revealed</span> several <span class="hlt">large</span> impact basins not previously known [6,7], so the answer certainly is "Yes." How <span class="hlt">large</span> a population of previously undetected impact basins, their size frequency distribution, and how much these added craters and basins will change ideas about the early cratering history and Late Heavy Bombardment on the Moon remains to be determined. Lunar Orbiter Laser Altimeter (LOLA) data [8] will be able to address these issues. As a prelude, we searched the state-of-the-art global topographic grid for the Moon, the Unified Lunar Control Net (ULCN) [9] for evidence of <span class="hlt">large</span> impact features not previously recognized by photogeologic mapping, as summarized by Wilhelms [lo].</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005JPCM...17.2255V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005JPCM...17.2255V"><span><span class="hlt">Large</span> <span class="hlt">scale</span> structures in liquid crystal/clay colloids</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Duijneveldt, Jeroen S.; Klein, Susanne; Leach, Edward; Pizzey, Claire; Richardson, Robert M.</p> <p>2005-04-01</p> <p>Suspensions of three different clays in K15, a thermotropic liquid crystal, have been studied by optical microscopy and small angle x-ray scattering. The three clays were claytone AF, a surface treated natural montmorillonite, laponite RD, a synthetic hectorite, and mined sepiolite. The claytone and laponite were sterically stabilized whereas sepiolite formed a relatively stable suspension in K15 without any surface treatment. Micrographs of the different suspensions <span class="hlt">revealed</span> that all three suspensions contained <span class="hlt">large</span> <span class="hlt">scale</span> structures. The nature of these aggregates was investigated using small angle x-ray scattering. For the clays with sheet-like particles, claytone and laponite, the flocs contain a mixture of stacked and single platelets. The basal spacing in the stacks was independent of particle concentration in the suspension and the phase of the solvent. The number of platelets in the stack and their percentage in the suspension varied with concentration and the aspect ratio of the platelets. The lath shaped sepiolite did not show any tendency to organize into ordered structures. Here the aggregates are networks of randomly oriented single rods.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25443759','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25443759"><span>Search and rescue response to a <span class="hlt">large-scale</span> rockfall disaster.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Procter, Emily; Strapazzon, Giacomo; Balkenhol, Karla; Fop, Ernst; Faggionato, Alessandro; Mayr, Karl; Falk, Markus; Brugger, Hermann</p> <p>2015-03-01</p> <p>To describe the prehospital management and safety of search and rescue (SAR) teams involved in a <span class="hlt">large-scale</span> rockfall disaster and monitor the acute and chronic health effects on personnel with severe dolomitic dust exposure. SAR personnel underwent on-site medical screening and lung function testing 3 months and 3 years after the event. The emergency dispatch center was responsible for central coordination of resources. One hundred fifty SAR members from multidisciplinary <span class="hlt">air</span>- and ground-based teams as well as geotechnical experts were dispatched to a provisionary operation center. Acute exposure to dolomite dust with detectable silicon and magnesium concentrations was not associated with (sub)acute or chronic sequelae or a clinically significant impairment in lung function in exposed personnel. The risk for personnel involved in mountain SAR operations is rarely reported and not easily investigated or quantified. This case exemplifies the importance of a multiskilled team and additional considerations for prehospital management during natural hazard events. Safety plans should include compulsory protective measures and medical monitoring of personnel. Copyright © 2015 Wilderness Medical Society. Published by Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=64836&keyword=Interest+AND+Simple&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=64836&keyword=Interest+AND+Simple&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>METHODOLOGY FOR SITING AMBIENT <span class="hlt">AIR</span> MONITORS AT THE NEIGHBORHOOD <span class="hlt">SCALE</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>In siting a monitor to measure compliance with U.S. National Ambient <span class="hlt">Air</span> Quality Standards for particulate matter (PM), there is a need to characterize variations in PM concentration within a neighborhood-<span class="hlt">scale</span> region in order to achieve monitor siting objectives.<br><br> We p...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008ICRC....2..157B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008ICRC....2..157B"><span><span class="hlt">Large-Angular-Scale</span> Clustering as a Clue to the Source of UHECRs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Berlind, Andreas A.; Farrar, Glennys R.</p> <p></p> <p>We explore what can be learned about the sources of UHECRs from their <span class="hlt">large-angular-scale</span> clustering (referred to as their "bias" by the cosmology community). Exploiting the clustering on <span class="hlt">large</span> <span class="hlt">scales</span> has the advantage over small-<span class="hlt">scale</span> correlations of being insensitive to uncertainties in source direction from magnetic smearing or measurement error. In a Cold Dark Matter cosmology, the amplitude of <span class="hlt">large-scale</span> clustering depends on the mass of the system, with more massive systems such as galaxy clusters clustering more strongly than less massive systems such as ordinary galaxies or AGN. Therefore, studying the <span class="hlt">large-scale</span> clustering of UHECRs can help determine a mass <span class="hlt">scale</span> for their sources, given the assumption that their redshift depth is as expected from the GZK cutoff. We investigate the constraining power of a given UHECR sample as a function of its cutoff energy and number of events. We show that current and future samples should be able to distinguish between the cases of their sources being galaxy clusters, ordinary galaxies, or sources that are uncorrelated with the <span class="hlt">large-scale</span> structure of the universe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24374556','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24374556"><span>A <span class="hlt">large</span>-area diffuse <span class="hlt">air</span> discharge plasma excited by nanosecond pulse under a double hexagon needle-array electrode.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Liu, Zhi-Jie; Wang, Wen-Chun; Yang, De-Zheng; Wang, Sen; Zhang, Shuai; Tang, Kai; Jiang, Peng-Chao</p> <p>2014-01-01</p> <p>A <span class="hlt">large</span>-area diffuse <span class="hlt">air</span> discharge plasma excited by bipolar nanosecond pulse is generated under a double hexagon needle-array electrode at atmospheric pressure. The images of the diffuse discharge, electric characteristics, and the optical emission spectra emitted from the diffuse <span class="hlt">air</span> discharge plasma are obtained. Based on the waveforms of pulse voltage and current, the power consumption, and the power density of the diffuse <span class="hlt">air</span> discharge plasma are investigated under different pulse peak voltages. The electron density and the electron temperature of the diffuse plasma are estimated to be approximately 1.42×10(11) cm(-3) and 4.4 eV, respectively. The optical emission spectra are arranged to determine the rotational and vibrational temperatures by comparing experimental with simulated spectra. Meanwhile, the rotational and vibrational temperatures of the diffuse discharge plasma are also discussed under different pulse peak voltages and pulse repetition rates, respectively. In addition, the diffuse <span class="hlt">air</span> discharge plasma can form an area of about 70×50 mm(2) on the surface of dielectric layer and can be <span class="hlt">scaled</span> up to the required size. Crown Copyright © 2013. Published by Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19.8942L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19.8942L"><span>Multi-<span class="hlt">scale</span> levels of Cs-137 contamination of landscapes of the Bryansk Region (with reference to results of <span class="hlt">air</span> gamma survey)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Linnik, Vitaly; Sokolov, Alexander; Sokolov, Peter</p> <p>2017-04-01</p> <p>As a result of the Chernobyl accident on April 26, 1986, <span class="hlt">large</span> amounts of radionuclides were released into the atmosphere, resulting in high contamination in Belarus, Ukraine, and Russia. High variability of environmental parameters and multi-<span class="hlt">scale</span> nature of initial fallout significantly contributed to very complicated Cs-137 patterns. The first maps of radioactive contamination due to the accident at the Chernobyl nuclear power plant, built in May 1986, already identified a heterogeneous nature of the contamination zones [1]. A complex combination of factors, such as the nature of the deposition (dry, wet), various volumetric activity of radionuclides in the atmosphere during the deposition of aerosols on the earth's surface, led to the formation of multiscale fields of radionuclide contamination, where each <span class="hlt">scale</span> correlates with "pollution spots" having their own specific nature]. <span class="hlt">Air</span> gamma survey was conducted with a grid 100x100 m and it allowed to <span class="hlt">reveal</span> different levels of <span class="hlt">scale</span> "spots" of Cs-137 contamination associated with the movement of polluted <span class="hlt">air</span> and the influence of the underlying surface - forests, river valleys. Cs-137 contamination field has an extraordinary feature - uniqueness of its spatial structure in different districts of the Bryansk region. A maximal area of "cesium" spots up to 30-50 km in size and with a contamination density of more than 1000 kBq/m2 is observed in the western part of the Bryansk Region. Their spatial structure is extremely heterogeneous, the differences in the local density of Cs-137 contamination being due to those in intensity of precipitation (wet deposition). The central part of the Bryansk Region with the density of contamination below 37 kBq/m2 (up to 3-5 kBq/m2 ) is an example of a condensing zone of "dry" deposition. With a larger <span class="hlt">scale</span>, allowing individual elements of Cs-137 contamination to be shown in a more distinct way, it is possible to observe the relationship of contamination with a number of landscape</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=336515','PESTICIDES'); return false;" href="https://cfpub.epa.gov/si/si_public_record_report.cfm?direntryid=336515"><span>Persistence of initial conditions in continental <span class="hlt">scale</span> <span class="hlt">air</span> quality ...</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>This study investigates the effect of initial conditions (IC) for pollutant concentrations in the atmosphere and soil on simulated <span class="hlt">air</span> quality for two continental-<span class="hlt">scale</span> Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model applications. One of these applications was performed for springtime and the second for summertime. Results show that a spin-up period of ten days commonly used in regional-<span class="hlt">scale</span> applications may not be sufficient to reduce the effects of initial conditions to less than 1% of seasonally-averaged surface ozone concentrations everywhere while 20 days were found to be sufficient for the entire domain for the spring case and almost the entire domain for the summer case. For the summer case, differences were found to persist longer aloft due to circulation of <span class="hlt">air</span> masses and even a spin-up period of 30 days was not sufficient to reduce the effects of ICs to less than 1% of seasonally-averaged layer 34 ozone concentrations over the southwestern portion of the modeling domain. Analysis of the effect of soil initial conditions for the CMAQ bidirectional NH3 exchange model shows that during springtime they can have an important effect on simulated inorganic aerosols concentrations for time periods of one month or longer. The effects are less pronounced during other seasons. The results, while specific to the modeling domain and time periods simulated here, suggest that modeling protocols need to be scrutinized for a given application and that it cannot be assum</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4495039','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4495039"><span>Dispersal Mutualism Incorporated into <span class="hlt">Large-Scale</span>, Infrequent Disturbances</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Parker, V. Thomas</p> <p>2015-01-01</p> <p>Because of their influence on succession and other community interactions, <span class="hlt">large-scale</span>, infrequent natural disturbances also should play a major role in mutualistic interactions. Using field data and experiments, I test whether mutualisms have been incorporated into <span class="hlt">large-scale</span> wildfire by whether the outcomes of a mutualism depend on disturbance. In this study a seed dispersal mutualism is shown to depend on infrequent, <span class="hlt">large-scale</span> disturbances. A dominant shrubland plant (Arctostaphylos species) produces seeds that make up a persistent soil seed bank and requires fire to germinate. In post-fire stands, I show that seedlings emerging from rodent caches dominate sites experiencing higher fire intensity. Field experiments show that rodents (Perimyscus californicus, P. boylii) do cache Arctostaphylos fruit and bury most seed caches to a sufficient depth to survive a killing heat pulse that a fire might drive into the soil. While the rodent dispersal and caching behavior itself has not changed compared to other habitats, the environmental transformation caused by wildfire converts the caching burial of seed from a dispersal process to a plant fire adaptive trait, and provides the context for stimulating subsequent life history evolution in the plant host. PMID:26151560</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPS...342..435L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPS...342..435L"><span>A novel rechargeable zinc-<span class="hlt">air</span> battery with molten salt electrolyte</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Shuzhi; Han, Wei; Cui, Baochen; Liu, Xianjun; Zhao, Fulin; Stuart, Jessica; Licht, Stuart</p> <p>2017-02-01</p> <p>Zinc-<span class="hlt">air</span> batteries have been proposed for EV applications and <span class="hlt">large-scale</span> electricity storage such as wind and solar power. Although zinc-<span class="hlt">air</span> batteries are very promising, there are numerous technological barriers to overcome. We demonstrate for the first time, a new rechargeable zinc-<span class="hlt">air</span> battery that utilizes a molten Li0.87Na0.63K0.50CO3 eutectic electrolyte with added NaOH. Cyclic voltammetry <span class="hlt">reveals</span> that a reversible deposition/dissolution of zinc occurs in the molten Li0.87Na0.63K0.50CO3 eutectic. At 550 °C, this zinc-<span class="hlt">air</span> battery performs with a coulombic efficiency of 96.9% over 110 cycles, having an average charging potential of ∼1.43 V and discharge potential of ∼1.04 V. The zinc-<span class="hlt">air</span> battery uses cost effective steel and nickel electrodes without the need for any precious metal catalysts. Moreover, the molten salt electrolyte offers advantages over aqueous electrolytes, avoiding the common aqueous alkaline electrolyte issues of hydrogen evolution, Zn dendrite formation, "drying out", and carbonate precipitation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/5303847-cedar-large-scale-multiprocessor','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/5303847-cedar-large-scale-multiprocessor"><span>Cedar-a <span class="hlt">large</span> <span class="hlt">scale</span> multiprocessor</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>Gajski, D.; Kuck, D.; Lawrie, D.</p> <p>1983-01-01</p> <p>This paper presents an overview of Cedar, a <span class="hlt">large</span> <span class="hlt">scale</span> multiprocessor being designed at the University of Illinois. This machine is designed to accommodate several thousand high performance processors which are capable of working together on a single job, or they can be partitioned into groups of processors where each group of one or more processors can work on separate jobs. Various aspects of the machine are described including the control methodology, communication network, optimizing compiler and plans for construction. 13 references.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5006166','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5006166"><span><span class="hlt">Large-Scale</span> Discovery of Disease-Disease and Disease-Gene Associations</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Gligorijevic, Djordje; Stojanovic, Jelena; Djuric, Nemanja; Radosavljevic, Vladan; Grbovic, Mihajlo; Kulathinal, Rob J.; Obradovic, Zoran</p> <p>2016-01-01</p> <p>Data-driven phenotype analyses on Electronic Health Record (EHR) data have recently drawn benefits across many areas of clinical practice, uncovering new links in the medical sciences that can potentially affect the well-being of millions of patients. In this paper, EHR data is used to discover novel relationships between diseases by studying their comorbidities (co-occurrences in patients). A novel embedding model is designed to extract knowledge from disease comorbidities by learning from a <span class="hlt">large-scale</span> EHR database comprising more than 35 million inpatient cases spanning nearly a decade, <span class="hlt">revealing</span> significant improvements on disease phenotyping over current computational approaches. In addition, the use of the proposed methodology is extended to discover novel disease-gene associations by including valuable domain knowledge from genome-wide association studies. To evaluate our approach, its effectiveness is compared against a held-out set where, again, it <span class="hlt">revealed</span> very compelling results. For selected diseases, we further identify candidate gene lists for which disease-gene associations were not studied previously. Thus, our approach provides biomedical researchers with new tools to filter genes of interest, thus, reducing costly lab studies. PMID:27578529</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('https://www.ncbi.nlm.nih.gov/pubmed/25615592','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25615592"><span>Laminar and dorsoventral molecular organization of the medial entorhinal cortex <span class="hlt">revealed</span> by <span class="hlt">large-scale</span> anatomical analysis of gene expression.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ramsden, Helen L; Sürmeli, Gülşen; McDonagh, Steven G; Nolan, Matthew F</p> <p>2015-01-01</p> <p>Neural circuits in the medial entorhinal cortex (MEC) encode an animal's position and orientation in space. Within the MEC spatial representations, including grid and directional firing fields, have a laminar and dorsoventral organization that corresponds to a similar topography of neuronal connectivity and cellular properties. Yet, in part due to the challenges of integrating anatomical data at the resolution of cortical layers and borders, we know little about the molecular components underlying this organization. To address this we develop a new computational pipeline for high-throughput analysis and comparison of in situ hybridization (ISH) images at laminar resolution. We apply this pipeline to ISH data for over 16,000 genes in the Allen Brain Atlas and validate our analysis with RNA sequencing of MEC tissue from adult mice. We find that differential gene expression delineates the borders of the MEC with neighboring brain structures and <span class="hlt">reveals</span> its laminar and dorsoventral organization. We propose a new molecular basis for distinguishing the deep layers of the MEC and show that their similarity to corresponding layers of neocortex is greater than that of superficial layers. Our analysis identifies ion channel-, cell adhesion- and synapse-related genes as candidates for functional differentiation of MEC layers and for encoding of spatial information at different <span class="hlt">scales</span> along the dorsoventral axis of the MEC. We also <span class="hlt">reveal</span> laminar organization of genes related to disease pathology and suggest that a high metabolic demand predisposes layer II to neurodegenerative pathology. In principle, our computational pipeline can be applied to high-throughput analysis of many forms of neuroanatomical data. Our results support the hypothesis that differences in gene expression contribute to functional specialization of superficial layers of the MEC and dorsoventral organization of the <span class="hlt">scale</span> of spatial representations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4304787','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4304787"><span>Laminar and Dorsoventral Molecular Organization of the Medial Entorhinal Cortex <span class="hlt">Revealed</span> by <span class="hlt">Large-scale</span> Anatomical Analysis of Gene Expression</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Ramsden, Helen L.; Sürmeli, Gülşen; McDonagh, Steven G.; Nolan, Matthew F.</p> <p>2015-01-01</p> <p>Neural circuits in the medial entorhinal cortex (MEC) encode an animal’s position and orientation in space. Within the MEC spatial representations, including grid and directional firing fields, have a laminar and dorsoventral organization that corresponds to a similar topography of neuronal connectivity and cellular properties. Yet, in part due to the challenges of integrating anatomical data at the resolution of cortical layers and borders, we know little about the molecular components underlying this organization. To address this we develop a new computational pipeline for high-throughput analysis and comparison of in situ hybridization (ISH) images at laminar resolution. We apply this pipeline to ISH data for over 16,000 genes in the Allen Brain Atlas and validate our analysis with RNA sequencing of MEC tissue from adult mice. We find that differential gene expression delineates the borders of the MEC with neighboring brain structures and <span class="hlt">reveals</span> its laminar and dorsoventral organization. We propose a new molecular basis for distinguishing the deep layers of the MEC and show that their similarity to corresponding layers of neocortex is greater than that of superficial layers. Our analysis identifies ion channel-, cell adhesion- and synapse-related genes as candidates for functional differentiation of MEC layers and for encoding of spatial information at different <span class="hlt">scales</span> along the dorsoventral axis of the MEC. We also <span class="hlt">reveal</span> laminar organization of genes related to disease pathology and suggest that a high metabolic demand predisposes layer II to neurodegenerative pathology. In principle, our computational pipeline can be applied to high-throughput analysis of many forms of neuroanatomical data. Our results support the hypothesis that differences in gene expression contribute to functional specialization of superficial layers of the MEC and dorsoventral organization of the <span class="hlt">scale</span> of spatial representations. PMID:25615592</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28706893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28706893"><span>Rectal perforation by compressed <span class="hlt">air</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Park, Young Jin</p> <p>2017-07-01</p> <p>As the use of compressed <span class="hlt">air</span> in industrial work has increased, so has the risk of associated pneumatic injury from its improper use. However, damage of <span class="hlt">large</span> intestine caused by compressed <span class="hlt">air</span> is uncommon. Herein a case of pneumatic rupture of the rectum is described. The patient was admitted to the Emergency Room complaining of abdominal pain and distension. His colleague triggered a compressed <span class="hlt">air</span> nozzle over his buttock. On arrival, vital signs were stable but physical examination <span class="hlt">revealed</span> peritoneal irritation and marked distension of the abdomen. Computed tomography showed a <span class="hlt">large</span> volume of <span class="hlt">air</span> in the peritoneal cavity and subcutaneous emphysema at the perineum. A rectal perforation was found at laparotomy and the Hartmann procedure was performed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2001asi..book.....C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2001asi..book.....C"><span><span class="hlt">Air</span>-Sea Interaction</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Csanady, G. T.</p> <p>2001-03-01</p> <p>In recent years <span class="hlt">air</span>-sea interaction has emerged as a subject in its own right, encompassing small-<span class="hlt">scale</span> and <span class="hlt">large-scale</span> processes in both <span class="hlt">air</span> and sea. <span class="hlt">Air</span>-Sea Interaction: Laws and Mechanisms is a comprehensive account of how the atmosphere and the ocean interact to control the global climate, what physical laws govern this interaction, and its prominent mechanisms. The topics covered range from evaporation in the oceans, to hurricanes, and on to poleward heat transport by the oceans. By developing the subject from basic physical (thermodynamic) principles, the book is accessible to graduate students and research scientists in meteorology, oceanography, and environmental engineering. It will also be of interest to the broader physics community involved in the treatment of transfer laws, and thermodynamics of the atmosphere and ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18047271','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18047271"><span>Analyzing <span class="hlt">large-scale</span> proteomics projects with latent semantic indexing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Klie, Sebastian; Martens, Lennart; Vizcaíno, Juan Antonio; Côté, Richard; Jones, Phil; Apweiler, Rolf; Hinneburg, Alexander; Hermjakob, Henning</p> <p>2008-01-01</p> <p>Since the advent of public data repositories for proteomics data, readily accessible results from high-throughput experiments have been accumulating steadily. Several <span class="hlt">large-scale</span> projects in particular have contributed substantially to the amount of identifications available to the community. Despite the considerable body of information amassed, very few successful analyses have been performed and published on this data, leveling off the ultimate value of these projects far below their potential. A prominent reason published proteomics data is seldom reanalyzed lies in the heterogeneous nature of the original sample collection and the subsequent data recording and processing. To illustrate that at least part of this heterogeneity can be compensated for, we here apply a latent semantic analysis to the data contributed by the Human Proteome Organization's Plasma Proteome Project (HUPO PPP). Interestingly, despite the broad spectrum of instruments and methodologies applied in the HUPO PPP, our analysis <span class="hlt">reveals</span> several obvious patterns that can be used to formulate concrete recommendations for optimizing proteomics project planning as well as the choice of technologies used in future experiments. It is clear from these results that the analysis of <span class="hlt">large</span> bodies of publicly available proteomics data by noise-tolerant algorithms such as the latent semantic analysis holds great promise and is currently underexploited.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170011243','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170011243"><span>Fabrication of the HIAD <span class="hlt">Large-Scale</span> Demonstration Assembly</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Swanson, G. T.; Johnson, R. K.; Hughes, S. J.; DiNonno, J. M.; Cheatwood, F. M.</p> <p>2017-01-01</p> <p>Over a decade of work has been conducted in the development of NASA's Hypersonic Inflatable Aerodynamic Decelerator (HIAD) technology. This effort has included multiple ground test campaigns and flight tests culminating in the HIAD projects second generation (Gen-2) deployable aeroshell system and associated analytical tools. NASAs HIAD project team has developed, fabricated, and tested inflatable structures (IS) integrated with flexible thermal protection system (F-TPS), ranging in diameters from 3-6m, with cone angles of 60 and 70 deg.In 2015, United Launch Alliance (ULA) announced that they will use a HIAD (10-12m) as part of their Sensible, Modular, Autonomous Return Technology (SMART) for their upcoming Vulcan rocket. ULA expects SMART reusability, coupled with other advancements for Vulcan, will substantially reduce the cost of access to space. The first booster engine recovery via HIAD is scheduled for 2024. To meet this near-term need, as well as future NASA applications, the HIAD team is investigating taking the technology to the 10-15m diameter <span class="hlt">scale</span>. In the last year, many significant development and fabrication efforts have been accomplished, culminating in the construction of a <span class="hlt">large-scale</span> inflatable structure demonstration assembly. This assembly incorporated the first three tori for a 12m Mars Human-<span class="hlt">Scale</span> Pathfinder HIAD conceptual design that was constructed with the current state of the art material set. Numerous design trades and torus fabrication demonstrations preceded this effort. In 2016, three <span class="hlt">large-scale</span> tori (0.61m cross-section) and six subscale tori (0.25m cross-section) were manufactured to demonstrate fabrication techniques using the newest candidate material sets. These tori were tested to evaluate durability and load capacity. This work led to the selection of the inflatable structures third generation (Gen-3) structural liner. In late 2016, the three tori required for the <span class="hlt">large-scale</span> demonstration assembly were fabricated, and then</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018SPIE10615E..3AL','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018SPIE10615E..3AL"><span>An interactive display system for <span class="hlt">large-scale</span> 3D models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liu, Zijian; Sun, Kun; Tao, Wenbing; Liu, Liman</p> <p>2018-04-01</p> <p>With the improvement of 3D reconstruction theory and the rapid development of computer hardware technology, the reconstructed 3D models are enlarging in <span class="hlt">scale</span> and increasing in complexity. Models with tens of thousands of 3D points or triangular meshes are common in practical applications. Due to storage and computing power limitation, it is difficult to achieve real-time display and interaction with <span class="hlt">large</span> <span class="hlt">scale</span> 3D models for some common 3D display software, such as MeshLab. In this paper, we propose a display system for <span class="hlt">large-scale</span> 3D scene models. We construct the LOD (Levels of Detail) model of the reconstructed 3D scene in advance, and then use an out-of-core view-dependent multi-resolution rendering scheme to realize the real-time display of the <span class="hlt">large-scale</span> 3D model. With the proposed method, our display system is able to render in real time while roaming in the reconstructed scene and 3D camera poses can also be displayed. Furthermore, the memory consumption can be significantly decreased via internal and external memory exchange mechanism, so that it is possible to display a <span class="hlt">large</span> <span class="hlt">scale</span> reconstructed scene with over millions of 3D points or triangular meshes in a regular PC with only 4GB RAM.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3462218','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3462218"><span>Radar Tracking and Motion-Sensitive Cameras on Flowers <span class="hlt">Reveal</span> the Development of Pollinator Multi-Destination Routes over <span class="hlt">Large</span> Spatial <span class="hlt">Scales</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>Reynolds, Andrew M.; Stelzer, Ralph J.; Lim, Ka S.; Smith, Alan D.; Osborne, Juliet L.; Chittka, Lars</p> <p>2012-01-01</p> <p>Central place foragers, such as pollinating bees, typically develop circuits (traplines) to visit multiple foraging sites in a manner that minimizes overall travel distance. Despite being taxonomically widespread, these routing behaviours remain poorly understood due to the difficulty of tracking the foraging history of animals in the wild. Here we examine how bumblebees (Bombus terrestris) develop and optimise traplines over <span class="hlt">large</span> spatial <span class="hlt">scales</span> by setting up an array of five artificial flowers arranged in a regular pentagon (50 m side length) and fitted with motion-sensitive video cameras to determine the sequence of visitation. Stable traplines that linked together all the flowers in an optimal sequence were typically established after a bee made 26 foraging bouts, during which time only about 20 of the 120 possible routes were tried. Radar tracking of selected flights <span class="hlt">revealed</span> a dramatic decrease by 80% (ca. 1500 m) of the total travel distance between the first and the last foraging bout. When a flower was removed and replaced by a more distant one, bees engaged in localised search flights, a strategy that can facilitate the discovery of a new flower and its integration into a novel optimal trapline. Based on these observations, we developed and tested an iterative improvement heuristic to capture how bees could learn and refine their routes each time a shorter route is found. Our findings suggest that complex dynamic routing problems can be solved by small-brained animals using simple learning heuristics, without the need for a cognitive map. PMID:23049479</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3610841','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3610841"><span>DISRUPTION OF <span class="hlt">LARGE-SCALE</span> NEURAL NETWORKS IN NON-FLUENT/AGRAMMATIC VARIANT PRIMARY PROGRESSIVE APHASIA ASSOCIATED WITH FRONTOTEMPORAL DEGENERATION PATHOLOGY</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Grossman, Murray; Powers, John; Ash, Sherry; McMillan, Corey; Burkholder, Lisa; Irwin, David; Trojanowski, John Q.</p> <p>2012-01-01</p> <p>Non-fluent/agrammatic primary progressive aphasia (naPPA) is a progressive neurodegenerative condition most prominently associated with slowed, effortful speech. A clinical imaging marker of naPPA is disease centered in the left inferior frontal lobe. We used multimodal imaging to assess <span class="hlt">large-scale</span> neural networks underlying effortful expression in 15 patients with sporadic naPPA due to frontotemporal lobar degeneration (FTLD) spectrum pathology. Effortful speech in these patients is related in part to impaired grammatical processing, and to phonologic speech errors. Gray matter (GM) imaging shows frontal and anterior-superior temporal atrophy, most prominently in the left hemisphere. Diffusion tensor imaging <span class="hlt">reveals</span> reduced fractional anisotropy in several white matter (WM) tracts mediating projections between left frontal and other GM regions. Regression analyses suggest disruption of three <span class="hlt">large-scale</span> GM-WM neural networks in naPPA that support fluent, grammatical expression. These findings emphasize the role of <span class="hlt">large-scale</span> neural networks in language, and demonstrate associated language deficits in naPPA. PMID:23218686</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28320939','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28320939"><span>Decoupling local mechanics from <span class="hlt">large-scale</span> structure in modular metamaterials.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Nan; Silverberg, Jesse L</p> <p>2017-04-04</p> <p>A defining feature of mechanical metamaterials is that their properties are determined by the organization of internal structure instead of the raw fabrication materials. This shift of attention to engineering internal degrees of freedom has coaxed relatively simple materials into exhibiting a wide range of remarkable mechanical properties. For practical applications to be realized, however, this nascent understanding of metamaterial design must be translated into a capacity for engineering <span class="hlt">large-scale</span> structures with prescribed mechanical functionality. Thus, the challenge is to systematically map desired functionality of <span class="hlt">large-scale</span> structures backward into a design scheme while using finite parameter domains. Such "inverse design" is often complicated by the deep coupling between <span class="hlt">large-scale</span> structure and local mechanical function, which limits the available design space. Here, we introduce a design strategy for constructing 1D, 2D, and 3D mechanical metamaterials inspired by modular origami and kirigami. Our approach is to assemble a number of modules into a voxelized <span class="hlt">large-scale</span> structure, where the module's design has a greater number of mechanical design parameters than the number of constraints imposed by bulk assembly. This inequality allows each voxel in the bulk structure to be uniquely assigned mechanical properties independent from its ability to connect and deform with its neighbors. In studying specific examples of <span class="hlt">large-scale</span> metamaterial structures we show that a decoupling of global structure from local mechanical function allows for a variety of mechanically and topologically complex designs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PNAS..114.3590Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PNAS..114.3590Y"><span>Decoupling local mechanics from <span class="hlt">large-scale</span> structure in modular metamaterials</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yang, Nan; Silverberg, Jesse L.</p> <p>2017-04-01</p> <p>A defining feature of mechanical metamaterials is that their properties are determined by the organization of internal structure instead of the raw fabrication materials. This shift of attention to engineering internal degrees of freedom has coaxed relatively simple materials into exhibiting a wide range of remarkable mechanical properties. For practical applications to be realized, however, this nascent understanding of metamaterial design must be translated into a capacity for engineering <span class="hlt">large-scale</span> structures with prescribed mechanical functionality. Thus, the challenge is to systematically map desired functionality of <span class="hlt">large-scale</span> structures backward into a design scheme while using finite parameter domains. Such “inverse design” is often complicated by the deep coupling between <span class="hlt">large-scale</span> structure and local mechanical function, which limits the available design space. Here, we introduce a design strategy for constructing 1D, 2D, and 3D mechanical metamaterials inspired by modular origami and kirigami. Our approach is to assemble a number of modules into a voxelized <span class="hlt">large-scale</span> structure, where the module’s design has a greater number of mechanical design parameters than the number of constraints imposed by bulk assembly. This inequality allows each voxel in the bulk structure to be uniquely assigned mechanical properties independent from its ability to connect and deform with its neighbors. In studying specific examples of <span class="hlt">large-scale</span> metamaterial structures we show that a decoupling of global structure from local mechanical function allows for a variety of mechanically and topologically complex designs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930039993&hterms=Omega&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DOmega%2B3','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930039993&hterms=Omega&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3DOmega%2B3"><span><span class="hlt">Large</span>- and small-<span class="hlt">scale</span> constraints on power spectra in Omega = 1 universes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gelb, James M.; Gradwohl, Ben-Ami; Frieman, Joshua A.</p> <p>1993-01-01</p> <p>The CDM model of structure formation, normalized on <span class="hlt">large</span> <span class="hlt">scales</span>, leads to excessive pairwise velocity dispersions on small <span class="hlt">scales</span>. In an attempt to circumvent this problem, we study three scenarios (all with Omega = 1) with more <span class="hlt">large-scale</span> and less small-<span class="hlt">scale</span> power than the standard CDM model: (1) cold dark matter with significantly reduced small-<span class="hlt">scale</span> power (inspired by models with an admixture of cold and hot dark matter); (2) cold dark matter with a non-<span class="hlt">scale</span>-invariant power spectrum; and (3) cold dark matter with coupling of dark matter to a long-range vector field. When normalized to COBE on <span class="hlt">large</span> <span class="hlt">scales</span>, such models do lead to reduced velocities on small <span class="hlt">scales</span> and they produce fewer halos compared with CDM. However, models with sufficiently low small-<span class="hlt">scale</span> velocities apparently fail to produce an adequate number of halos.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28626277','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28626277"><span>Linking crop yield anomalies to <span class="hlt">large-scale</span> atmospheric circulation in Europe.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ceglar, Andrej; Turco, Marco; Toreti, Andrea; Doblas-Reyes, Francisco J</p> <p>2017-06-15</p> <p>Understanding the effects of climate variability and extremes on crop growth and development represents a necessary step to assess the resilience of agricultural systems to changing climate conditions. This study investigates the links between the <span class="hlt">large-scale</span> atmospheric circulation and crop yields in Europe, providing the basis to develop seasonal crop yield forecasting and thus enabling a more effective and dynamic adaptation to climate variability and change. Four dominant modes of <span class="hlt">large-scale</span> atmospheric variability have been used: North Atlantic Oscillation, Eastern Atlantic, Scandinavian and Eastern Atlantic-Western Russia patterns. <span class="hlt">Large-scale</span> atmospheric circulation explains on average 43% of inter-annual winter wheat yield variability, ranging between 20% and 70% across countries. As for grain maize, the average explained variability is 38%, ranging between 20% and 58%. Spatially, the skill of the developed statistical models strongly depends on the <span class="hlt">large-scale</span> atmospheric variability impact on weather at the regional level, especially during the most sensitive growth stages of flowering and grain filling. Our results also suggest that preceding atmospheric conditions might provide an important source of predictability especially for maize yields in south-eastern Europe. Since the seasonal predictability of <span class="hlt">large-scale</span> atmospheric patterns is generally higher than the one of surface weather variables (e.g. precipitation) in Europe, seasonal crop yield prediction could benefit from the integration of derived statistical models exploiting the dynamical seasonal forecast of <span class="hlt">large-scale</span> atmospheric circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910007391','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910007391"><span>Effects of <span class="hlt">large-scale</span> wind driven turbulence on sound propagation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Noble, John M.; Bass, Henry E.; Raspet, Richard</p> <p>1990-01-01</p> <p>Acoustic measurements made in the atmosphere have shown significant fluctuations in amplitude and phase resulting from the interaction with time varying meteorological conditions. The observed variations appear to have short term and long term (1 to 5 minutes) variations at least in the phase of the acoustic signal. One possible way to account for this long term variation is the use of a <span class="hlt">large</span> <span class="hlt">scale</span> wind driven turbulence model. From a Fourier analysis of the phase variations, the outer <span class="hlt">scales</span> for the <span class="hlt">large</span> <span class="hlt">scale</span> turbulence is 200 meters and greater, which corresponds to turbulence in the energy-containing subrange. The <span class="hlt">large</span> <span class="hlt">scale</span> turbulence is assumed to be elongated longitudinal vortex pairs roughly aligned with the mean wind. Due to the size of the vortex pair compared to the <span class="hlt">scale</span> of the present experiment, the effect of the vortex pair on the acoustic field can be modeled as the sound speed of the atmosphere varying with time. The model provides results with the same trends and variations in phase observed experimentally.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29477853','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29477853"><span>How do <span class="hlt">large-scale</span> agricultural investments affect land use and the environment on the western slopes of Mount Kenya? Empirical evidence based on small-<span class="hlt">scale</span> farmers' perceptions and remote sensing.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zaehringer, Julie G; Wambugu, Grace; Kiteme, Boniface; Eckert, Sandra</p> <p>2018-05-01</p> <p>Africa has been heavily targeted by <span class="hlt">large-scale</span> agricultural investments (LAIs) throughout the last decade, with scarcely known impacts on local social-ecological systems. In Kenya, a <span class="hlt">large</span> number of LAIs were made in the region northwest of Mount Kenya. These <span class="hlt">large-scale</span> farms produce vegetables and flowers mainly for European markets. However, land use in the region remains dominated by small-<span class="hlt">scale</span> crop and livestock farms with less than 1 ha of land each, who produce both for their own subsistence and for the local markets. We interviewed 100 small-<span class="hlt">scale</span> farmers living near five different LAIs to elicit their perceptions of the impacts that these LAIs have on their land use and the overall environment. Furthermore, we analyzed remotely sensed land cover and land use data to assess land use change in the vicinity of the five LAIs. While land use change did not follow a clear trend, a number of small-<span class="hlt">scale</span> farmers did adapt their crop management to environmental changes such as a reduced river water flows and increased pests, which they attributed to the presence of LAIs. Despite the high number of open conflicts between small-<span class="hlt">scale</span> land users and LAIs around the issue of river water abstraction, the main environmental impact, felt by almost half of the interviewed land users, was <span class="hlt">air</span> pollution with agrochemicals sprayed on the LAIs' land. Even though only a low percentage of local land users and their household members were directly involved with LAIs, a <span class="hlt">large</span> majority of respondents favored the presence of LAIs nearby, as they are believed to contribute to the region's overall economic development. Copyright © 2018 Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013PhDT.......119N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhDT.......119N"><span>The <span class="hlt">Large-scale</span> Structure of the Universe: Probes of Cosmology and Structure Formation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Noh, Yookyung</p> <p></p> <p>The usefulness of <span class="hlt">large-scale</span> structure as a probe of cosmology and structure formation is increasing as <span class="hlt">large</span> deep surveys in multi-wavelength bands are becoming possible. The observational analysis of <span class="hlt">large-scale</span> structure guided by <span class="hlt">large</span> volume numerical simulations are beginning to offer us complementary information and crosschecks of cosmological parameters estimated from the anisotropies in Cosmic Microwave Background (CMB) radiation. Understanding structure formation and evolution and even galaxy formation history is also being aided by observations of different redshift snapshots of the Universe, using various tracers of <span class="hlt">large-scale</span> structure. This dissertation work covers aspects of <span class="hlt">large-scale</span> structure from the baryon acoustic oscillation <span class="hlt">scale</span>, to that of <span class="hlt">large</span> <span class="hlt">scale</span> filaments and galaxy clusters. First, I discuss a <span class="hlt">large</span>- <span class="hlt">scale</span> structure use for high precision cosmology. I investigate the reconstruction of Baryon Acoustic Oscillation (BAO) peak within the context of Lagrangian perturbation theory, testing its validity in a <span class="hlt">large</span> suite of cosmological volume N-body simulations. Then I consider galaxy clusters and the <span class="hlt">large</span> <span class="hlt">scale</span> filaments surrounding them in a high resolution N-body simulation. I investigate the geometrical properties of galaxy cluster neighborhoods, focusing on the filaments connected to clusters. Using mock observations of galaxy clusters, I explore the correlations of scatter in galaxy cluster mass estimates from multi-wavelength observations and different measurement techniques. I also examine the sources of the correlated scatter by considering the intrinsic and environmental properties of clusters.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29105235','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29105235"><span>The biology and polymer physics underlying <span class="hlt">large-scale</span> chromosome organization.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sazer, Shelley; Schiessel, Helmut</p> <p>2018-02-01</p> <p>Chromosome <span class="hlt">large-scale</span> organization is a beautiful example of the interplay between physics and biology. DNA molecules are polymers and thus belong to the class of molecules for which physicists have developed models and formulated testable hypotheses to understand their arrangement and dynamic properties in solution, based on the principles of polymer physics. Biologists documented and discovered the biochemical basis for the structure, function and dynamic spatial organization of chromosomes in cells. The underlying principles of chromosome organization have recently been <span class="hlt">revealed</span> in unprecedented detail using high-resolution chromosome capture technology that can simultaneously detect chromosome contact sites throughout the genome. These independent lines of investigation have now converged on a model in which DNA loops, generated by the loop extrusion mechanism, are the basic organizational and functional units of the chromosome. © 2017 The Authors. Traffic published by John Wiley & Sons Ltd.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1287331','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1287331"><span>FutureGen 2.0 Oxy-combustion <span class="hlt">Large</span> <span class="hlt">Scale</span> Test – Final Report</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>Kenison, LaVesta; Flanigan, Thomas; Hagerty, Gregg</p> <p></p> <p>The primary objectives of the FutureGen 2.0 CO 2 Oxy-Combustion <span class="hlt">Large</span> <span class="hlt">Scale</span> Test Project were to site, permit, design, construct, and commission, an oxy-combustion boiler, gas quality control system, <span class="hlt">air</span> separation unit, and CO 2 compression and purification unit, together with the necessary supporting and interconnection utilities. The project was to demonstrate at commercial <span class="hlt">scale</span> (168MWe gross) the capability to cleanly produce electricity through coal combustion at a retrofitted, existing coal-fired power plant; thereby, resulting in near-zeroemissions of all commonly regulated <span class="hlt">air</span> emissions, as well as 90% CO 2 capture in steady-state operations. The project was to be fully integratedmore » in terms of project management, capacity, capabilities, technical scope, cost, and schedule with the companion FutureGen 2.0 CO 2 Pipeline and Storage Project, a separate but complementary project whose objective was to safely transport, permanently store and monitor the CO 2 captured by the Oxy-combustion Power Plant Project. The FutureGen 2.0 Oxy-Combustion <span class="hlt">Large</span> <span class="hlt">Scale</span> Test Project successfully achieved all technical objectives inclusive of front-end-engineering and design, and advanced design required to accurately estimate and contract for the construction, commissioning, and start-up of a commercial-<span class="hlt">scale</span> "ready to build" power plant using oxy-combustion technology, including full integration with the companion CO 2 Pipeline and Storage project. Ultimately the project did not proceed to construction due to insufficient time to complete necessary EPC contract negotiations and commercial financing prior to expiration of federal co-funding, which triggered a DOE decision to closeout its participation in the project. Through the work that was completed, valuable technical, commercial, and programmatic lessons were learned. This project has significantly advanced the development of near-zero emission technology and will be helpful to plotting the course of, and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=315570&keyword=air+AND+transportation&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=315570&keyword=air+AND+transportation&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>A Community-<span class="hlt">Scale</span> Modeling System to Assess Port-Related <span class="hlt">Air</span> Quality Impacts</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>Near-port <span class="hlt">air</span> pollution has been identified by numerous organizations as a potential public health concern. Based upon multiple near-road and near-source monitoring studies, both busy roadways and <span class="hlt">large</span> emission sources at the ports may impact local <span class="hlt">air</span> quality within several hun...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AAS...21331806Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AAS...21331806Y"><span><span class="hlt">Large-scale</span> Density Structures in Magneto-rotational Disk Turbulence</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Youdin, Andrew; Johansen, A.; Klahr, H.</p> <p>2009-01-01</p> <p>Turbulence generated by the magneto-rotational instability (MRI) is a strong candidate to drive accretion flows in disks, including sufficiently ionized regions of protoplanetary disks. The MRI is often studied in local shearing boxes, which model a small section of the disk at high resolution. I will present simulations of <span class="hlt">large</span>, stratified shearing boxes which extend up to 10 gas <span class="hlt">scale</span>-heights across. These simulations are a useful bridge to fully global disk simulations. We find that MRI turbulence produces <span class="hlt">large-scale</span>, axisymmetric density perturbations . These structures are part of a zonal flow --- analogous to the banded flow in Jupiter's atmosphere --- which survives in near geostrophic balance for tens of orbits. The launching mechanism is <span class="hlt">large-scale</span> magnetic tension generated by an inverse cascade. We demonstrate the robustness of these results by careful study of various box sizes, grid resolutions, and microscopic diffusion parameterizations. These gas structures can trap solid material (in the form of <span class="hlt">large</span> dust or ice particles) with important implications for planet formation. Resolved disk images at mm-wavelengths (e.g. from ALMA) will verify or constrain the existence of these structures.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014APS..DFDR32002D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014APS..DFDR32002D"><span>The role of <span class="hlt">large</span> <span class="hlt">scale</span> motions on passive scalar transport</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dharmarathne, Suranga; Araya, Guillermo; Tutkun, Murat; Leonardi, Stefano; Castillo, Luciano</p> <p>2014-11-01</p> <p>We study direct numerical simulation (DNS) of turbulent channel flow at Reτ = 394 to investigate effect of <span class="hlt">large</span> <span class="hlt">scale</span> motions on fluctuating temperature field which forms a passive scalar field. Statistical description of the <span class="hlt">large</span> <span class="hlt">scale</span> features of the turbulent channel flow is obtained using two-point correlations of velocity components. Two-point correlations of fluctuating temperature field is also examined in order to identify possible similarities between velocity and temperature fields. The two-point cross-correlations betwen the velocity and temperature fluctuations are further analyzed to establish connections between these two fields. In addition, we use proper orhtogonal decompotion (POD) to extract most dominant modes of the fields and discuss the coupling of <span class="hlt">large</span> <span class="hlt">scale</span> features of turbulence and the temperature field.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29457795','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29457795"><span>Random access in <span class="hlt">large-scale</span> DNA data storage.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Organick, Lee; Ang, Siena Dumas; Chen, Yuan-Jyue; Lopez, Randolph; Yekhanin, Sergey; Makarychev, Konstantin; Racz, Miklos Z; Kamath, Govinda; Gopalan, Parikshit; Nguyen, Bichlien; Takahashi, Christopher N; Newman, Sharon; Parker, Hsing-Yeh; Rashtchian, Cyrus; Stewart, Kendall; Gupta, Gagan; Carlson, Robert; Mulligan, John; Carmean, Douglas; Seelig, Georg; Ceze, Luis; Strauss, Karin</p> <p>2018-03-01</p> <p>Synthetic DNA is durable and can encode digital data with high density, making it an attractive medium for data storage. However, recovering stored data on a <span class="hlt">large-scale</span> currently requires all the DNA in a pool to be sequenced, even if only a subset of the information needs to be extracted. Here, we encode and store 35 distinct files (over 200 MB of data), in more than 13 million DNA oligonucleotides, and show that we can recover each file individually and with no errors, using a random access approach. We design and validate a <span class="hlt">large</span> library of primers that enable individual recovery of all files stored within the DNA. We also develop an algorithm that greatly reduces the sequencing read coverage required for error-free decoding by maximizing information from all sequence reads. These advances demonstrate a viable, <span class="hlt">large-scale</span> system for DNA data storage and retrieval.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015PhDT........16G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015PhDT........16G"><span>Improving Design Efficiency for <span class="hlt">Large-Scale</span> Heterogeneous Circuits</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gregerson, Anthony</p> <p></p> <p>Despite increases in logic density, many Big Data applications must still be partitioned across multiple computing devices in order to meet their strict performance requirements. Among the most demanding of these applications is high-energy physics (HEP), which uses complex computing systems consisting of thousands of FPGAs and ASICs to process the sensor data created by experiments at particles accelerators such as the <span class="hlt">Large</span> Hadron Collider (LHC). Designing such computing systems is challenging due to the <span class="hlt">scale</span> of the systems, the exceptionally high-throughput and low-latency performance constraints that necessitate application-specific hardware implementations, the requirement that algorithms are efficiently partitioned across many devices, and the possible need to update the implemented algorithms during the lifetime of the system. In this work, we describe our research to develop flexible architectures for implementing such <span class="hlt">large-scale</span> circuits on FPGAs. In particular, this work is motivated by (but not limited in scope to) high-energy physics algorithms for the Compact Muon Solenoid (CMS) experiment at the LHC. To make efficient use of logic resources in multi-FPGA systems, we introduce Multi-Personality Partitioning, a novel form of the graph partitioning problem, and present partitioning algorithms that can significantly improve resource utilization on heterogeneous devices while also reducing inter-chip connections. To reduce the high communication costs of Big Data applications, we also introduce Information-Aware Partitioning, a partitioning method that analyzes the data content of application-specific circuits, characterizes their entropy, and selects circuit partitions that enable efficient compression of data between chips. We employ our information-aware partitioning method to improve the performance of the hardware validation platform for evaluating new algorithms for the CMS experiment. Together, these research efforts help to improve the efficiency</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ACP....15.8889M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ACP....15.8889M"><span>Tropospheric ozone and its precursors from the urban to the global <span class="hlt">scale</span> from <span class="hlt">air</span> quality to short-lived climate forcer</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Monks, P. S.; Archibald, A. T.; Colette, A.; Cooper, O.; Coyle, M.; Derwent, R.; Fowler, D.; Granier, C.; Law, K. S.; Mills, G. E.; Stevenson, D. S.; Tarasova, O.; Thouret, V.; von Schneidemesser, E.; Sommariva, R.; Wild, O.; Williams, M. L.</p> <p>2015-08-01</p> <p>Ozone holds a certain fascination in atmospheric science. It is ubiquitous in the atmosphere, central to tropospheric oxidation chemistry, yet harmful to human and ecosystem health as well as being an important greenhouse gas. It is not emitted into the atmosphere but is a byproduct of the very oxidation chemistry it <span class="hlt">largely</span> initiates. Much effort is focused on the reduction of surface levels of ozone owing to its health and vegetation impacts, but recent efforts to achieve reductions in exposure at a country <span class="hlt">scale</span> have proved difficult to achieve owing to increases in background ozone at the zonal hemispheric <span class="hlt">scale</span>. There is also a growing realisation that the role of ozone as a short-lived climate pollutant could be important in integrated <span class="hlt">air</span> quality climate change mitigation. This review examines current understanding of the processes regulating tropospheric ozone at global to local <span class="hlt">scales</span> from both measurements and models. It takes the view that knowledge across the <span class="hlt">scales</span> is important for dealing with <span class="hlt">air</span> quality and climate change in a synergistic manner. The review shows that there remain a number of clear challenges for ozone such as explaining surface trends, incorporating new chemical understanding, ozone-climate coupling, and a better assessment of impacts. There is a clear and present need to treat ozone across the range of <span class="hlt">scales</span>, a transboundary issue, but with an emphasis on the hemispheric <span class="hlt">scales</span>. New observational opportunities are offered both by satellites and small sensors that bridge the <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=recruitment&pg=5&id=EJ1162232','ERIC'); return false;" href="https://eric.ed.gov/?q=recruitment&pg=5&id=EJ1162232"><span>Lessons Learned from <span class="hlt">Large-Scale</span> Randomized Experiments</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>Slavin, Robert E.; Cheung, Alan C. K.</p> <p>2017-01-01</p> <p><span class="hlt">Large-scale</span> randomized studies provide the best means of evaluating practical, replicable approaches to improving educational outcomes. This article discusses the advantages, problems, and pitfalls of these evaluations, focusing on alternative methods of randomization, recruitment, ensuring high-quality implementation, dealing with attrition, and…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=159447&keyword=fluid+AND+cfd&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=159447&keyword=fluid+AND+cfd&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>A FRAMEWORK FOR FINE-<span class="hlt">SCALE</span> COMPUTATIONAL FLUID DYNAMICS <span class="hlt">AIR</span> QUALITY MODELING AND ANALYSIS</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 paper discusses a framework for fine-<span class="hlt">scale</span> CFD modeling that may be developed to complement the present Community Multi-<span class="hlt">scale</span> <span class="hlt">Air</span> Quality (CMAQ) modeling system which itself is a computational fluid dynamics model. A goal of this presentation is to stimulate discussions on w...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22524908-nonlinear-modulation-hi-power-spectrum-ultra-large-scales','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22524908-nonlinear-modulation-hi-power-spectrum-ultra-large-scales"><span>Nonlinear modulation of the HI power spectrum on ultra-<span class="hlt">large</span> <span class="hlt">scales</span>. I</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>Umeh, Obinna; Maartens, Roy; Santos, Mario, E-mail: umeobinna@gmail.com, E-mail: roy.maartens@gmail.com, E-mail: mgrsantos@uwc.ac.za</p> <p>2016-03-01</p> <p>Intensity mapping of the neutral hydrogen brightness temperature promises to provide a three-dimensional view of the universe on very <span class="hlt">large</span> <span class="hlt">scales</span>. Nonlinear effects are typically thought to alter only the small-<span class="hlt">scale</span> power, but we show how they may bias the extraction of cosmological information contained in the power spectrum on ultra-<span class="hlt">large</span> <span class="hlt">scales</span>. For linear perturbations to remain valid on <span class="hlt">large</span> <span class="hlt">scales</span>, we need to renormalize perturbations at higher order. In the case of intensity mapping, the second-order contribution to clustering from weak lensing dominates the nonlinear contribution at high redshift. Renormalization modifies the mean brightness temperature and therefore the evolutionmore » bias. It also introduces a term that mimics white noise. These effects may influence forecasting analysis on ultra-<span class="hlt">large</span> <span class="hlt">scales</span>.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=taxation&pg=6&id=EJ734298','ERIC'); return false;" href="https://eric.ed.gov/?q=taxation&pg=6&id=EJ734298"><span>Students' Ideas and Attitudes about <span class="hlt">Air</span> Quality</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>Skamp, Keith; Boyes, Eddie; Stanisstreet, Martin</p> <p>2004-01-01</p> <p>The results of a <span class="hlt">large</span> <span class="hlt">scale</span> (N=1001) cross-sectional (Years 6, 8 and 10) study of students' ideas about the composition of unpolluted <span class="hlt">air</span>, the nature of <span class="hlt">air</span> pollution, the biological consequences of <span class="hlt">air</span> pollution, and about acid rain and the Greenhouse Effect are reported. A range of persistent alternative conceptions were identified, in some…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23866203','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23866203"><span>Factor structure and reliability of the depression, anxiety and stress <span class="hlt">scales</span> in a <span class="hlt">large</span> Portuguese community sample.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Vasconcelos-Raposo, José; Fernandes, Helder Miguel; Teixeira, Carla M</p> <p>2013-01-01</p> <p>The purpose of the present study was to assess the factor structure and reliability of the Depression, Anxiety and Stress <span class="hlt">Scales</span> (DASS-21) in a <span class="hlt">large</span> Portuguese community sample. Participants were 1020 adults (585 women and 435 men), with a mean age of 36.74 (SD = 11.90) years. All <span class="hlt">scales</span> <span class="hlt">revealed</span> good reliability, with Cronbach's alpha values between .80 (anxiety) and .84 (depression). The internal consistency of the total score was .92. Confirmatory factor analysis <span class="hlt">revealed</span> that the best-fitting model (*CFI = .940, *RMSEA = .038) consisted of a latent component of general psychological distress (or negative affectivity) plus orthogonal depression, anxiety and stress factors. The Portuguese version of the DASS-21 showed good psychometric properties (factorial validity and reliability) and thus can be used as a reliable and valid instrument for measuring depression, anxiety and stress symptoms.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhRvD..97f3527A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhRvD..97f3527A"><span>Impact of <span class="hlt">large-scale</span> tides on cosmological distortions via redshift-space power spectrum</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Akitsu, Kazuyuki; Takada, Masahiro</p> <p>2018-03-01</p> <p>Although <span class="hlt">large-scale</span> perturbations beyond a finite-volume survey region are not direct observables, these affect measurements of clustering statistics of small-<span class="hlt">scale</span> (subsurvey) perturbations in <span class="hlt">large-scale</span> structure, compared with the ensemble average, via the mode-coupling effect. In this paper we show that a <span class="hlt">large-scale</span> tide induced by scalar perturbations causes apparent anisotropic distortions in the redshift-space power spectrum of galaxies in a way depending on an alignment between the tide, wave vector of small-<span class="hlt">scale</span> modes and line-of-sight direction. Using the perturbation theory of structure formation, we derive a response function of the redshift-space power spectrum to <span class="hlt">large-scale</span> tide. We then investigate the impact of <span class="hlt">large-scale</span> tide on estimation of cosmological distances and the redshift-space distortion parameter via the measured redshift-space power spectrum for a hypothetical <span class="hlt">large</span>-volume survey, based on the Fisher matrix formalism. To do this, we treat the <span class="hlt">large-scale</span> tide as a signal, rather than an additional source of the statistical errors, and show that a degradation in the parameter is restored if we can employ the prior on the rms amplitude expected for the standard cold dark matter (CDM) model. We also discuss whether the <span class="hlt">large-scale</span> tide can be constrained at an accuracy better than the CDM prediction, if the effects up to a larger wave number in the nonlinear regime can be included.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24191145','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24191145"><span>A topology visualization early warning distribution algorithm for <span class="hlt">large-scale</span> network security incidents.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Hui; Fan, Guotao; Ye, Jianwei; Zhang, Weizhe</p> <p>2013-01-01</p> <p>It is of great significance to research the early warning system for <span class="hlt">large-scale</span> network security incidents. It can improve the network system's emergency response capabilities, alleviate the cyber attacks' damage, and strengthen the system's counterattack ability. A comprehensive early warning system is presented in this paper, which combines active measurement and anomaly detection. The key visualization algorithm and technology of the system are mainly discussed. The <span class="hlt">large-scale</span> network system's plane visualization is realized based on the divide and conquer thought. First, the topology of the <span class="hlt">large-scale</span> network is divided into some small-<span class="hlt">scale</span> networks by the MLkP/CR algorithm. Second, the sub graph plane visualization algorithm is applied to each small-<span class="hlt">scale</span> network. Finally, the small-<span class="hlt">scale</span> networks' topologies are combined into a topology based on the automatic distribution algorithm of force analysis. As the algorithm transforms the <span class="hlt">large-scale</span> network topology plane visualization problem into a series of small-<span class="hlt">scale</span> network topology plane visualization and distribution problems, it has higher parallelism and is able to handle the display of ultra-<span class="hlt">large-scale</span> network topology.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009LNCS.5727..429V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009LNCS.5727..429V"><span>Honeycomb: Visual Analysis of <span class="hlt">Large</span> <span class="hlt">Scale</span> Social Networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>van Ham, Frank; Schulz, Hans-Jörg; Dimicco, Joan M.</p> <p></p> <p>The rise in the use of social network sites allows us to collect <span class="hlt">large</span> amounts of user reported data on social structures and analysis of this data could provide useful insights for many of the social sciences. This analysis is typically the domain of Social Network Analysis, and visualization of these structures often proves invaluable in understanding them. However, currently available visual analysis tools are not very well suited to handle the massive <span class="hlt">scale</span> of this network data, and often resolve to displaying small ego networks or heavily abstracted networks. In this paper, we present Honeycomb, a visualization tool that is able to deal with much larger <span class="hlt">scale</span> data (with millions of connections), which we illustrate by using a <span class="hlt">large</span> <span class="hlt">scale</span> corporate social networking site as an example. Additionally, we introduce a new probability based network metric to guide users to potentially interesting or anomalous patterns and discuss lessons learned during design and implementation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20150005715','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20150005715"><span>Advances in Parallelization for <span class="hlt">Large</span> <span class="hlt">Scale</span> Oct-Tree Mesh Generation</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>O'Connell, Matthew; Karman, Steve L.</p> <p>2015-01-01</p> <p>Despite great advancements in the parallelization of numerical simulation codes over the last 20 years, it is still common to perform grid generation in serial. Generating <span class="hlt">large</span> <span class="hlt">scale</span> grids in serial often requires using special "grid generation" compute machines that can have more than ten times the memory of average machines. While some parallel mesh generation techniques have been proposed, generating very <span class="hlt">large</span> meshes for LES or aeroacoustic simulations is still a challenging problem. An automated method for the parallel generation of very <span class="hlt">large</span> <span class="hlt">scale</span> off-body hierarchical meshes is presented here. This work enables <span class="hlt">large</span> <span class="hlt">scale</span> parallel generation of off-body meshes by using a novel combination of parallel grid generation techniques and a hybrid "top down" and "bottom up" oct-tree method. Meshes are generated using hardware commonly found in parallel compute clusters. The capability to generate very <span class="hlt">large</span> meshes is demonstrated by the generation of off-body meshes surrounding complex aerospace geometries. Results are shown including a one billion cell mesh generated around a Predator Unmanned Aerial Vehicle geometry, which was generated on 64 processors in under 45 minutes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.P43C2904T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.P43C2904T"><span>Investigating a link between <span class="hlt">large</span> and small-<span class="hlt">scale</span> chaos features on Europa</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tognetti, L.; Rhoden, A.; Nelson, D. M.</p> <p>2017-12-01</p> <p>Chaos is one of the most recognizable, and studied, features on Europa's surface. Most models of chaos formation invoke liquid water at shallow depths within the ice shell; the liquid destabilizes the overlying ice layer, breaking it into mobile rafts and destroying pre-existing terrain. This class of model has been applied to both <span class="hlt">large-scale</span> chaos like Conamara and small-<span class="hlt">scale</span> features (i.e. microchaos), which are typically <10 km in diameter. Currently unknown, however, is whether both <span class="hlt">large-scale</span> and small-<span class="hlt">scale</span> features are produced together, e.g. through a network of smaller sills linked to a larger liquid water pocket. If microchaos features do form as satellites of <span class="hlt">large-scale</span> chaos features, we would expect a drop off in the number density of microchaos with increasing distance from the <span class="hlt">large</span> chaos feature; the trend should not be observed in regions without <span class="hlt">large-scale</span> chaos features. Here, we test the hypothesis that <span class="hlt">large</span> chaos features create "satellite" systems of smaller chaos features. Either outcome will help us better understand the relationship between <span class="hlt">large-scale</span> chaos and microchaos. We focus first on regions surrounding the <span class="hlt">large</span> chaos features Conamara and Murias (e.g. the Mitten). We map all chaos features within 90,000 sq km of the main chaos feature and assign each one a ranking (High Confidence, Probable, or Low Confidence) based on the observed characteristics of each feature. In particular, we look for a distinct boundary, loss of preexisting terrain, the existence of rafts or blocks, and the overall smoothness of the feature. We also note features that are chaos-like but lack sufficient characteristics to be classified as chaos. We then apply the same criteria to map microchaos features in regions of similar area ( 90,000 sq km) that lack <span class="hlt">large</span> chaos features. By plotting the distribution of microchaos with distance from the center point of the <span class="hlt">large</span> chaos feature or the mapping region (for the cases without a <span class="hlt">large</span> feature), we</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1998BAAS...30..769C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1998BAAS...30..769C"><span>Soft X-ray Emission from <span class="hlt">Large-Scale</span> Galactic Outflows in Seyfert Galaxies</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Colbert, E. J. M.; Baum, S.; O'Dea, C.; Veilleux, S.</p> <p>1998-01-01</p> <p>Kiloparsec-<span class="hlt">scale</span> soft X-ray nebulae extend along the galaxy minor axes in several Seyfert galaxies, including NGC 2992, NGC 4388 and NGC 5506. In these three galaxies, the extended X-ray emission observed in ROSAT HRI images has 0.2-2.4 keV X-ray luminosities of 0.4-3.5 x 10(40) erg s(-1) . The X-ray nebulae are roughly co-spatial with the <span class="hlt">large-scale</span> radio emission, suggesting that both are produced by <span class="hlt">large-scale</span> galactic outflows. Assuming pressure balance between the radio and X-ray plasmas, the X-ray filling factor is >~ 10(4) times as <span class="hlt">large</span> as the radio plasma filling factor, suggesting that <span class="hlt">large-scale</span> outflows in Seyfert galaxies are predominantly winds of thermal X-ray emitting gas. We favor an interpretation in which <span class="hlt">large-scale</span> outflows originate as AGN-driven jets that entrain and heat gas on kpc <span class="hlt">scales</span> as they make their way out of the galaxy. AGN- and starburst-driven winds are also possible explanations if the winds are oriented along the rotation axis of the galaxy disk. Since <span class="hlt">large-scale</span> outflows are present in at least 50 percent of Seyfert galaxies, the soft X-ray emission from the outflowing gas may, in many cases, explain the ``soft excess" X-ray feature observed below 2 keV in X-ray spectra of many Seyfert 2 galaxies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19750021782','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19750021782"><span>Some aspects of control of a <span class="hlt">large-scale</span> dynamic system</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Aoki, M.</p> <p>1975-01-01</p> <p>Techniques of predicting and/or controlling the dynamic behavior of <span class="hlt">large</span> <span class="hlt">scale</span> systems are discussed in terms of decentralized decision making. Topics discussed include: (1) control of <span class="hlt">large</span> <span class="hlt">scale</span> systems by dynamic team with delayed information sharing; (2) dynamic resource allocation problems by a team (hierarchical structure with a coordinator); and (3) some problems related to the construction of a model of reduced dimension.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008MNRAS.390..545D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008MNRAS.390..545D"><span><span class="hlt">Large-scale</span> magnetic topologies of early M dwarfs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Donati, J.-F.; Morin, J.; Petit, P.; Delfosse, X.; Forveille, T.; Aurière, M.; Cabanac, R.; Dintrans, B.; Fares, R.; Gastine, T.; Jardine, M. M.; Lignières, F.; Paletou, F.; Ramirez Velez, J. C.; Théado, S.</p> <p>2008-10-01</p> <p>We present here additional results of a spectropolarimetric survey of a small sample of stars ranging from spectral type M0 to M8 aimed at investigating observationally how dynamo processes operate in stars on both sides of the full convection threshold (spectral type M4). The present paper focuses on early M stars (M0-M3), that is above the full convection threshold. Applying tomographic imaging techniques to time series of rotationally modulated circularly polarized profiles collected with the NARVAL spectropolarimeter, we determine the rotation period and reconstruct the <span class="hlt">large-scale</span> magnetic topologies of six early M dwarfs. We find that early-M stars preferentially host <span class="hlt">large-scale</span> fields with dominantly toroidal and non-axisymmetric poloidal configurations, along with significant differential rotation (and long-term variability); only the lowest-mass star of our subsample is found to host an almost fully poloidal, mainly axisymmetric <span class="hlt">large-scale</span> field resembling those found in mid-M dwarfs. This abrupt change in the <span class="hlt">large-scale</span> magnetic topologies of M dwarfs (occurring at spectral type M3) has no related signature on X-ray luminosities (measuring the total amount of magnetic flux); it thus suggests that underlying dynamo processes become more efficient at producing <span class="hlt">large-scale</span> fields (despite producing the same flux) at spectral types later than M3. We suspect that this change relates to the rapid decrease in the radiative cores of low-mass stars and to the simultaneous sharp increase of the convective turnover times (with decreasing stellar mass) that models predict to occur at M3; it may also be (at least partly) responsible for the reduced magnetic braking reported for fully convective stars. Based on observations obtained at the Télescope Bernard Lyot (TBL), operated by the Institut National des Science de l'Univers of the Centre National de la Recherche Scientifique of France. E-mail: donati@ast.obs-mip.fr (J-FD); jmorin@ast.obs-mip.fr (JM); petit</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/876345','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/876345"><span>Robust <span class="hlt">large-scale</span> parallel nonlinear solvers for simulations.</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>Bader, Brett William; Pawlowski, Roger Patrick; Kolda, Tamara Gibson</p> <p>2005-11-01</p> <p>This report documents research to develop robust and efficient solution techniques for solving <span class="hlt">large-scale</span> systems of nonlinear equations. The most widely used method for solving systems of nonlinear equations is Newton's method. While much research has been devoted to augmenting Newton-based solvers (usually with globalization techniques), little has been devoted to exploring the application of different models. Our research has been directed at evaluating techniques using different models than Newton's method: a lower order model, Broyden's method, and a higher order model, the tensor method. We have developed <span class="hlt">large-scale</span> versions of each of these models and have demonstrated their usemore » in important applications at Sandia. Broyden's method replaces the Jacobian with an approximation, allowing codes that cannot evaluate a Jacobian or have an inaccurate Jacobian to converge to a solution. Limited-memory methods, which have been successful in optimization, allow us to extend this approach to <span class="hlt">large-scale</span> problems. We compare the robustness and efficiency of Newton's method, modified Newton's method, Jacobian-free Newton-Krylov method, and our limited-memory Broyden method. Comparisons are carried out for <span class="hlt">large-scale</span> applications of fluid flow simulations and electronic circuit simulations. Results show that, in cases where the Jacobian was inaccurate or could not be computed, Broyden's method converged in some cases where Newton's method failed to converge. We identify conditions where Broyden's method can be more efficient than Newton's method. We also present modifications to a <span class="hlt">large-scale</span> tensor method, originally proposed by Bouaricha, for greater efficiency, better robustness, and wider applicability. Tensor methods are an alternative to Newton-based methods and are based on computing a step based on a local quadratic model rather than a linear model. The advantage of Bouaricha's method is that it can use any existing linear solver, which makes it simple</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012SPIE.8499E..1DT','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012SPIE.8499E..1DT"><span>Rotation invariant fast features for <span class="hlt">large-scale</span> recognition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Takacs, Gabriel; Chandrasekhar, Vijay; Tsai, Sam; Chen, David; Grzeszczuk, Radek; Girod, Bernd</p> <p>2012-10-01</p> <p>We present an end-to-end feature description pipeline which uses a novel interest point detector and Rotation- Invariant Fast Feature (RIFF) descriptors. The proposed RIFF algorithm is 15× faster than SURF1 while producing <span class="hlt">large-scale</span> retrieval results that are comparable to SIFT.2 Such high-speed features benefit a range of applications from Mobile Augmented Reality (MAR) to web-<span class="hlt">scale</span> image retrieval and analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13b4011H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13b4011H"><span><span class="hlt">Large-scale</span> bioenergy production: how to resolve sustainability trade-offs?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Humpenöder, Florian; Popp, Alexander; Bodirsky, Benjamin Leon; Weindl, Isabelle; Biewald, Anne; Lotze-Campen, Hermann; Dietrich, Jan Philipp; Klein, David; Kreidenweis, Ulrich; Müller, Christoph; Rolinski, Susanne; Stevanovic, Miodrag</p> <p>2018-02-01</p> <p><span class="hlt">Large-scale</span> 2nd generation bioenergy deployment is a key element of 1.5 °C and 2 °C transformation pathways. However, <span class="hlt">large-scale</span> bioenergy production might have negative sustainability implications and thus may conflict with the Sustainable Development Goal (SDG) agenda. Here, we carry out a multi-criteria sustainability assessment of <span class="hlt">large-scale</span> bioenergy crop production throughout the 21st century (300 EJ in 2100) using a global land-use model. Our analysis indicates that <span class="hlt">large-scale</span> bioenergy production without complementary measures results in negative effects on the following sustainability indicators: deforestation, CO2 emissions from land-use change, nitrogen losses, unsustainable water withdrawals and food prices. One of our main findings is that single-sector environmental protection measures next to <span class="hlt">large-scale</span> bioenergy production are prone to involve trade-offs among these sustainability indicators—at least in the absence of more efficient land or water resource use. For instance, if bioenergy production is accompanied by forest protection, deforestation and associated emissions (SDGs 13 and 15) decline substantially whereas food prices (SDG 2) increase. However, our study also shows that this trade-off strongly depends on the development of future food demand. In contrast to environmental protection measures, we find that agricultural intensification lowers some side-effects of bioenergy production substantially (SDGs 13 and 15) without generating new trade-offs—at least among the sustainability indicators considered here. Moreover, our results indicate that a combination of forest and water protection schemes, improved fertilization efficiency, and agricultural intensification would reduce the side-effects of bioenergy production most comprehensively. However, although our study includes more sustainability indicators than previous studies on bioenergy side-effects, our study represents only a small subset of all indicators relevant for the</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2010Nanos...2.1661L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010Nanos...2.1661L"><span><span class="hlt">Large-scale</span> fabrication of single crystalline tin nanowire arrays</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Luo, Bin; Yang, Dachi; Liang, Minghui; Zhi, Linjie</p> <p>2010-09-01</p> <p><span class="hlt">Large-scale</span> single crystalline tin nanowire arrays with preferred lattice orientation along the [100] direction were fabricated in porous anodic aluminium oxide (AAO) membranes by the electrodeposition method using copper nanorod as a second electrode.<span class="hlt">Large-scale</span> single crystalline tin nanowire arrays with preferred lattice orientation along the [100] direction were fabricated in porous anodic aluminium oxide (AAO) membranes by the electrodeposition method using copper nanorod as a second electrode. Electronic supplementary information (ESI) available: Experimental details and the information for single crystalline copper nanorods. See DOI: 10.1039/c0nr00206b</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008cosp...37.3650Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008cosp...37.3650Z"><span><span class="hlt">Large-scale</span> Activities Associated with the 2005 Sep. 7th Event</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zong, Weiguo</p> <p></p> <p>We present a multi-wavelength study on <span class="hlt">large-scale</span> activities associated with a significant solar event. On 2005 September 7, a flare classified as bigger than X17 was observed. Combining with Hα 6562.8 ˚, He I 10830 ˚and soft X-ray observations, three <span class="hlt">large-scale</span> activities were A A found to propagate over a long distance on the solar surface. 1) The first <span class="hlt">large-scale</span> activity emanated from the flare site, which propagated westward around the solar equator and appeared as sequential brightenings. With MDI longitudinal magnetic field map, the activity was found to propagate along the magnetic network. 2) The second <span class="hlt">large-scale</span> activity could be well identified both in He I 10830 ˚images and soft X-ray images and appeared as diffuse emission A enhancement propagating away. The activity started later than the first one and was not centric on the flare site. Moreover, a rotation was found along with the bright front propagating away. 3) The third activity was ahead of the second one, which was identified as a "winking" filament. The three activities have different origins, which were seldom observed in one event. Therefore this study is useful to understand the mechanism of <span class="hlt">large-scale</span> activities on solar surface.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5507793','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5507793"><span>Rectal perforation by compressed <span class="hlt">air</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></p> <p>2017-01-01</p> <p>As the use of compressed <span class="hlt">air</span> in industrial work has increased, so has the risk of associated pneumatic injury from its improper use. However, damage of <span class="hlt">large</span> intestine caused by compressed <span class="hlt">air</span> is uncommon. Herein a case of pneumatic rupture of the rectum is described. The patient was admitted to the Emergency Room complaining of abdominal pain and distension. His colleague triggered a compressed <span class="hlt">air</span> nozzle over his buttock. On arrival, vital signs were stable but physical examination <span class="hlt">revealed</span> peritoneal irritation and marked distension of the abdomen. Computed tomography showed a <span class="hlt">large</span> volume of <span class="hlt">air</span> in the peritoneal cavity and subcutaneous emphysema at the perineum. A rectal perforation was found at laparotomy and the Hartmann procedure was performed. PMID:28706893</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.H41I..01H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.H41I..01H"><span>Unravelling connections between river flow and <span class="hlt">large-scale</span> climate: experiences from Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hannah, D. M.; Kingston, D. G.; Lavers, D.; Stagge, J. H.; Tallaksen, L. M.</p> <p>2016-12-01</p> <p>The United Nations has identified better knowledge of <span class="hlt">large-scale</span> water cycle processes as essential for socio-economic development and global water-food-energy security. In this context, and given the ever-growing concerns about climate change/ variability and human impacts on hydrology, there is an urgent research need: (a) to quantify space-time variability in regional river flow, and (b) to improve hydroclimatological understanding of climate-flow connections as a basis for identifying current and future water-related issues. In this paper, we draw together studies undertaken at the pan-European <span class="hlt">scale</span>: (1) to evaluate current methods for assessing space-time dynamics for different streamflow metrics (annual regimes, low flows and high flows) and for linking flow variability to atmospheric drivers (circulation indices, <span class="hlt">air</span>-masses, gridded climate fields and vapour flux); and (2) to propose a plan for future research connecting streamflow and the atmospheric conditions in Europe and elsewhere. We believe this research makes a useful, unique contribution to the literature through a systematic inter-comparison of different streamflow metrics and atmospheric descriptors. In our findings, we highlight the need to consider appropriate atmospheric descriptors (dependent on the target flow metric and region of interest) and to develop analytical techniques that best characterise connections in the ocean-atmosphere-land surface process chain. We call for the need to consider not only atmospheric interactions, but also the role of the river basin-<span class="hlt">scale</span> terrestrial hydrological processes in modifying the climate signal response of river flows.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFM.H53G0943C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFM.H53G0943C"><span>Multiresolution comparison of precipitation datasets for <span class="hlt">large-scale</span> models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chun, K. P.; Sapriza Azuri, G.; Davison, B.; DeBeer, C. M.; Wheater, H. S.</p> <p>2014-12-01</p> <p>Gridded precipitation datasets are crucial for driving <span class="hlt">large-scale</span> models which are related to weather forecast and climate research. However, the quality of precipitation products is usually validated individually. Comparisons between gridded precipitation products along with ground observations provide another avenue for investigating how the precipitation uncertainty would affect the performance of <span class="hlt">large-scale</span> models. In this study, using data from a set of precipitation gauges over British Columbia and Alberta, we evaluate several widely used North America gridded products including the Canadian Gridded Precipitation Anomalies (CANGRD), the National Center for Environmental Prediction (NCEP) reanalysis, the Water and Global Change (WATCH) project, the thin plate spline smoothing algorithms (ANUSPLIN) and Canadian Precipitation Analysis (CaPA). Based on verification criteria for various temporal and spatial <span class="hlt">scales</span>, results provide an assessment of possible applications for various precipitation datasets. For long-term climate variation studies (~100 years), CANGRD, NCEP, WATCH and ANUSPLIN have different comparative advantages in terms of their resolution and accuracy. For synoptic and mesoscale precipitation patterns, CaPA provides appealing performance of spatial coherence. In addition to the products comparison, various downscaling methods are also surveyed to explore new verification and bias-reduction methods for improving gridded precipitation outputs for <span class="hlt">large-scale</span> models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NatSR...632380X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NatSR...632380X"><span>Anisotropic shrinkage of insect <span class="hlt">air</span> sacs <span class="hlt">revealed</span> in vivo by X-ray microtomography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xu, Liang; Chen, Rongchang; Du, Guohao; Yang, Yiming; Wang, Feixiang; Deng, Biao; Xie, Honglan; Xiao, Tiqiao</p> <p>2016-09-01</p> <p><span class="hlt">Air</span> sacs are thought to be the bellows for insect respiration. However, their exact mechanism of action as a bellows remains unclear. A direct way to investigate this problem is in vivo observation of the changes in their three-dimensional structures. Therefore, four-dimensional X-ray phase contrast microtomography is employed to solve this puzzle. Quantitative analysis of three-dimensional image series <span class="hlt">reveals</span> that the compression of the <span class="hlt">air</span> sac during respiration in bell crickets exhibits obvious anisotropic characteristics both longitudinally and transversely. Volumetric changes of the tracheal trunks in the prothorax further strengthen the evidence of this finding. As a result, we conclude that the shrinkage and expansion of the insect <span class="hlt">air</span> sac is anisotropic, contrary to the hypothesis of isotropy, thereby providing new knowledge for further research on the insect respiratory system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19870040489&hterms=matter+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmatter%2Btheory','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19870040489&hterms=matter+theory&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dmatter%2Btheory"><span><span class="hlt">Large</span> <span class="hlt">scale</span> structure in universes dominated by cold dark matter</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bond, J. Richard</p> <p>1986-01-01</p> <p>The theory of Gaussian random density field peaks is applied to a numerical study of the <span class="hlt">large-scale</span> structure developing from adiabatic fluctuations in models of biased galaxy formation in universes with Omega = 1, h = 0.5 dominated by cold dark matter (CDM). The angular anisotropy of the cross-correlation function demonstrates that the far-field regions of cluster-<span class="hlt">scale</span> peaks are asymmetric, as recent observations indicate. These regions will generate pancakes or filaments upon collapse. One-dimensional singularities in the <span class="hlt">large-scale</span> bulk flow should arise in these CDM models, appearing as pancakes in position space. They are too rare to explain the CfA bubble walls, but pancakes that are just turning around now are sufficiently abundant and would appear to be thin walls normal to the line of sight in redshift space. <span class="hlt">Large</span> <span class="hlt">scale</span> streaming velocities are significantly smaller than recent observations indicate. To explain the reported 700 km/s coherent motions, mass must be significantly more clustered than galaxies with a biasing factor of less than 0.4 and a nonlinear redshift at cluster <span class="hlt">scales</span> greater than one for both massive neutrino and cold models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814247D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814247D"><span><span class="hlt">Large-scale</span> derived flood frequency analysis based on continuous simulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dung Nguyen, Viet; Hundecha, Yeshewatesfa; Guse, Björn; Vorogushyn, Sergiy; Merz, Bruno</p> <p>2016-04-01</p> <p>There is an increasing need for spatially consistent flood risk assessments at the regional <span class="hlt">scale</span> (several 100.000 km2), in particular in the insurance industry and for national risk reduction strategies. However, most <span class="hlt">large-scale</span> flood risk assessments are composed of smaller-<span class="hlt">scale</span> assessments and show spatial inconsistencies. To overcome this deficit, a <span class="hlt">large-scale</span> flood model composed of a weather generator and catchments models was developed reflecting the spatially inherent heterogeneity. The weather generator is a multisite and multivariate stochastic model capable of generating synthetic meteorological fields (precipitation, temperature, etc.) at daily resolution for the regional <span class="hlt">scale</span>. These fields respect the observed autocorrelation, spatial correlation and co-variance between the variables. They are used as input into catchment models. A long-term simulation of this combined system enables to derive very long discharge series at many catchment locations serving as a basic for spatially consistent flood risk estimates at the regional <span class="hlt">scale</span>. This combined model was set up and validated for major river catchments in Germany. The weather generator was trained by 53-year observation data at 528 stations covering not only the complete Germany but also parts of France, Switzerland, Czech Republic and Australia with the aggregated spatial <span class="hlt">scale</span> of 443,931 km2. 10.000 years of daily meteorological fields for the study area were generated. Likewise, rainfall-runoff simulations with SWIM were performed for the entire Elbe, Rhine, Weser, Donau and Ems catchments. The validation results illustrate a good performance of the combined system, as the simulated flood magnitudes and frequencies agree well with the observed flood data. Based on continuous simulation this model chain is then used to estimate flood quantiles for the whole Germany including upstream headwater catchments in neighbouring countries. This continuous <span class="hlt">large</span> <span class="hlt">scale</span> approach overcomes the several</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17193404','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17193404"><span>Guided growth of <span class="hlt">large-scale</span>, horizontally aligned arrays of single-walled carbon nanotubes and their use in thin-film transistors.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Kocabas, Coskun; Hur, Seung-Hyun; Gaur, Anshu; Meitl, Matthew A; Shim, Moonsub; Rogers, John A</p> <p>2005-11-01</p> <p>A convenient process for generating <span class="hlt">large-scale</span>, horizontally aligned arrays of pristine, single-walled carbon nanotubes (SWNTs) is described. The approach uses guided growth, by chemical vapor deposition (CVD), of SWNTs on miscut single-crystal quartz substrates. Studies of the growth <span class="hlt">reveal</span> important relationships between the density and alignment of the tubes, the CVD conditions, and the morphology of the quartz. Electrodes and dielectrics patterned on top of these arrays yield thin-film transistors that use the SWNTs as effective thin-film semiconductors. The ability to build high-performance devices of this type suggests significant promise for <span class="hlt">large-scale</span> aligned arrays of SWNTs in electronics, sensors, and other applications.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JCoPh.355..144C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JCoPh.355..144C"><span>Fluid-structure interaction simulation of floating structures interacting with complex, <span class="hlt">large-scale</span> ocean waves and atmospheric turbulence with application to floating offshore wind turbines</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Calderer, Antoni; Guo, Xin; Shen, Lian; Sotiropoulos, Fotis</p> <p>2018-02-01</p> <p>We develop a numerical method for simulating coupled interactions of complex floating structures with <span class="hlt">large-scale</span> ocean waves and atmospheric turbulence. We employ an efficient <span class="hlt">large-scale</span> model to develop offshore wind and wave environmental conditions, which are then incorporated into a high resolution two-phase flow solver with fluid-structure interaction (FSI). The <span class="hlt">large-scale</span> wind-wave interaction model is based on a two-fluid dynamically-coupled approach that employs a high-order spectral method for simulating the water motion and a viscous solver with undulatory boundaries for the <span class="hlt">air</span> motion. The two-phase flow FSI solver is based on the level set method and is capable of simulating the coupled dynamic interaction of arbitrarily complex bodies with airflow and waves. The <span class="hlt">large-scale</span> wave field solver is coupled with the near-field FSI solver with a one-way coupling approach by feeding into the latter waves via a pressure-forcing method combined with the level set method. We validate the model for both simple wave trains and three-dimensional directional waves and compare the results with experimental and theoretical solutions. Finally, we demonstrate the capabilities of the new computational framework by carrying out <span class="hlt">large</span>-eddy simulation of a floating offshore wind turbine interacting with realistic ocean wind and waves.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005xmm..prop..184P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005xmm..prop..184P"><span>The XMM <span class="hlt">Large</span> <span class="hlt">Scale</span> Structure Survey</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pierre, Marguerite</p> <p>2005-10-01</p> <p>We propose to complete, by an additional 5 deg2, the XMM-LSS Survey region overlying the Spitzer/SWIRE field. This field already has CFHTLS and Integral coverage, and will encompass about 10 deg2. The resulting multi-wavelength medium-depth survey, which complements XMM and Chandra deep surveys, will provide a unique view of <span class="hlt">large-scale</span> structure over a wide range of redshift, and will show active galaxies in the full range of environments. The complete coverage by optical and IR surveys provides high-quality photometric redshifts, so that cosmological results can quickly be extracted. In the spirit of a Legacy survey, we will make the raw X-ray data immediately public. Multi-band catalogues and images will also be made available on short time <span class="hlt">scales</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22039129-gaia-window-large-scale-motions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22039129-gaia-window-large-scale-motions"><span>GAIA: A WINDOW TO <span class="hlt">LARGE-SCALE</span> MOTIONS</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>Nusser, Adi; Branchini, Enzo; Davis, Marc, E-mail: adi@physics.technion.ac.il, E-mail: branchin@fis.uniroma3.it, E-mail: mdavis@berkeley.edu</p> <p>2012-08-10</p> <p>Using redshifts as a proxy for galaxy distances, estimates of the two-dimensional (2D) transverse peculiar velocities of distant galaxies could be obtained from future measurements of proper motions. We provide the mathematical framework for analyzing 2D transverse motions and show that they offer several advantages over traditional probes of <span class="hlt">large-scale</span> motions. They are completely independent of any intrinsic relations between galaxy properties; hence, they are essentially free of selection biases. They are free from homogeneous and inhomogeneous Malmquist biases that typically plague distance indicator catalogs. They provide additional information to traditional probes that yield line-of-sight peculiar velocities only. Further, becausemore » of their 2D nature, fundamental questions regarding vorticity of <span class="hlt">large-scale</span> flows can be addressed. Gaia, for example, is expected to provide proper motions of at least bright galaxies with high central surface brightness, making proper motions a likely contender for traditional probes based on current and future distance indicator measurements.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016NJPh...18e3036E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016NJPh...18e3036E"><span><span class="hlt">Large-scale</span> quantum networks based on graphs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Epping, Michael; Kampermann, Hermann; Bruß, Dagmar</p> <p>2016-05-01</p> <p>Society relies and depends increasingly on information exchange and communication. In the quantum world, security and privacy is a built-in feature for information processing. The essential ingredient for exploiting these quantum advantages is the resource of entanglement, which can be shared between two or more parties. The distribution of entanglement over <span class="hlt">large</span> distances constitutes a key challenge for current research and development. Due to losses of the transmitted quantum particles, which typically <span class="hlt">scale</span> exponentially with the distance, intermediate quantum repeater stations are needed. Here we show how to generalise the quantum repeater concept to the multipartite case, by describing <span class="hlt">large-scale</span> quantum networks, i.e. network nodes and their long-distance links, consistently in the language of graphs and graph states. This unifying approach comprises both the distribution of multipartite entanglement across the network, and the protection against errors via encoding. The correspondence to graph states also provides a tool for optimising the architecture of quantum networks.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5903G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5903G"><span>Long-term dynamics of hawaiian volcanoes inferred by <span class="hlt">large-scale</span> relative relocations of earthquakes</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Got, J.-L.; Okubo, P.</p> <p>2003-04-01</p> <p>We investigated the microseismicity recorded in an active volcano to infer information concerning the volcano structure and long-term dynamics, by using relative relocations and focal mechanisms of microearthquakes. 32000 earthquakes of Mauna Loa and Kilauea volcanoes were recorded by more than 8 stations of the Hawaiian Volcano Observatory seismic network between 1988 and 1999. We studied 17000 of these events and relocated more than 70% with an accuracy ranging from 10 to 500 meters. About 75% of these relocated events are located in the vicinity of subhorizontal decollement planes, at 8 to 11 km depth. However, the striking features <span class="hlt">revealed</span> by these relocation results are steep south-east dipping fault planes working as reverse faults, clearly located below the decollement plane and which intersect it. If this decollement plane coincides with the pre-Mauna Loa seafloor, as hypothesized by numerous authors, such reverse faults rupture the pre-Mauna Loa oceanic crust. The weight of the volcano and pressure in the magma storage system are possible causes of these ruptures, fully compatible with the local stress tensor computed by Gillard et al. (1996). Reverse faults are suspected of producing scarps <span class="hlt">revealed</span> by km-long horizontal slip-perpendicular lineations along the decollement surface, and therefore <span class="hlt">large-scale</span> roughness, asperities and normal stress variations. These are capable of generating stick-slip, <span class="hlt">large</span> magnitude earthquakes, the spatial microseismic pattern observed in the south flank of Kilauea volcano, and Hilina-type instabilities. Ruptures intersecting the decollement surface, causing its <span class="hlt">large-scale</span> roughness, may be an important parameter controlling the growth of Hawaiian volcanoes. Are there more or less rough decollement planes existing near the base of other volcanoes, such as Piton de la Fournaise or Etna, and able to explain part of their deformation and seismicity ?</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA618038','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA618038"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> Density Estimation of Blue and Fin Whales (LSD)</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2014-09-30</p> <p>172. McDonald, MA, Hildebrand, JA, and Mesnick, S (2009). Worldwide decline in tonal frequencies of blue whale songs . Endangered Species Research 9...1 DISTRIBUTION STATEMENT A. Approved for public release; distribution is unlimited. <span class="hlt">Large</span> <span class="hlt">Scale</span> Density Estimation of Blue and Fin Whales ...estimating blue and fin whale density that is effective over <span class="hlt">large</span> spatial <span class="hlt">scales</span> and is designed to cope with spatial variation in animal density utilizing</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820040199&hterms=sampling+techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsampling%2Btechniques','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820040199&hterms=sampling+techniques&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dsampling%2Btechniques"><span>Conditional sampling technique to test the applicability of the Taylor hypothesis for the <span class="hlt">large-scale</span> coherent structures</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hussain, A. K. M. F.</p> <p>1980-01-01</p> <p>Comparisons of the distributions of <span class="hlt">large</span> <span class="hlt">scale</span> structures in turbulent flow with distributions based on time dependent signals from stationary probes and the Taylor hypothesis are presented. The study investigated an area in the near field of a 7.62 cm circular <span class="hlt">air</span> jet at a Re of 32,000, specifically having coherent structures through small-amplitude controlled excitation and stable vortex pairing in the jet column mode. Hot-wire and X-wire anemometry were employed to establish phase averaged spatial distributions of longitudinal and lateral velocities, coherent Reynolds stress and vorticity, background turbulent intensities, streamlines and pseudo-stream functions. The Taylor hypothesis was used to calculate spatial distributions of the phase-averaged properties, with results indicating that the usage of the local time-average velocity or streamwise velocity produces <span class="hlt">large</span> distortions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010APS..DFD.MW002S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010APS..DFD.MW002S"><span>Low Pressure Seeder Development for PIV in <span class="hlt">Large</span> <span class="hlt">Scale</span> Open Loop Wind Tunnels</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schmit, Ryan</p> <p>2010-11-01</p> <p>A low pressure seeding techniques have been developed for Particle Image Velocimetry (PIV) in <span class="hlt">large</span> <span class="hlt">scale</span> wind tunnel facilities was performed at the Subsonic Aerodynamic Research Laboratory (SARL) facility at Wright-Patterson <span class="hlt">Air</span> Force Base. The SARL facility is an open loop tunnel with a 7 by 10 foot octagonal test section that has 56% optical access and the Mach number varies from 0.2 to 0.5. A low pressure seeder sprayer was designed and tested in the inlet of the wind tunnel. The seeder sprayer was designed to produce an even and uniform distribution of seed while reducing the seeders influence in the test section. ViCount Compact 5000 using Smoke Oil 180 was using as the seeding material. The results show that this low pressure seeder does produce streaky seeding but excellent PIV images are produced.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.5053P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.5053P"><span><span class="hlt">Large-scale</span> dynamics associated with clustering of extratropical cyclones affecting Western Europe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Pinto, Joaquim G.; Gómara, Iñigo; Masato, Giacomo; Dacre, Helen F.; Woollings, Tim; Caballero, Rodrigo</p> <p>2015-04-01</p> <p>Some recent winters in Western Europe have been characterized by the occurrence of multiple extratropical cyclones following a similar path. The occurrence of such cyclone clusters leads to <span class="hlt">large</span> socio-economic impacts due to damaging winds, storm surges, and floods. Recent studies have statistically characterized the clustering of extratropical cyclones over the North Atlantic and Europe and hypothesized potential physical mechanisms responsible for their formation. Here we analyze 4 months characterized by multiple cyclones over Western Europe (February 1990, January 1993, December 1999, and January 2007). The evolution of the eddy driven jet stream, Rossby wave-breaking, and upstream/downstream cyclone development are investigated to infer the role of the <span class="hlt">large-scale</span> flow and to determine if clustered cyclones are related to each other. Results suggest that optimal conditions for the occurrence of cyclone clusters are provided by a recurrent extension of an intensified eddy driven jet toward Western Europe lasting at least 1 week. Multiple Rossby wave-breaking occurrences on both the poleward and equatorward flanks of the jet contribute to the development of these anomalous <span class="hlt">large-scale</span> conditions. The analysis of the daily weather charts <span class="hlt">reveals</span> that upstream cyclone development (secondary cyclogenesis, where new cyclones are generated on the trailing fronts of mature cyclones) is strongly related to cyclone clustering, with multiple cyclones developing on a single jet streak. The present analysis permits a deeper understanding of the physical reasons leading to the occurrence of cyclone families over the North Atlantic, enabling a better estimation of the associated cumulative risk over Europe.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A21A0047D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A21A0047D"><span>National-<span class="hlt">Scale</span> <span class="hlt">Air</span> Quality Data Assessment: Initial Findings from the Near-Road NO2 Monitoring Program</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>DeWinter, J. L.</p> <p>2015-12-01</p> <p>In 2010, the U.S. Environmental Protection Agency (EPA) revised the National Ambient <span class="hlt">Air</span> Quality Standards (NAAQS) for nitrogen dioxide (NO2) to include a primary health-based standard for hourly NO2. NO2 is a reactive gas that is emitted from motor vehicles, such as cars, trucks, and off-road equipment, as well as non-mobile sources, and is known to adversely affect human respiratory health. In conjunction with the NAAQS revision, EPA has mandated <span class="hlt">air</span> quality monitoring next to selected major roadways throughout the United States that are in <span class="hlt">large</span> urban areas where peak hourly NO2 concentrations are expected. Monitoring began in phases during 2012-2015 and included nitrogen dioxide (NO2), carbon monoxide (CO), and particulate matter smaller than 2.5 microns (PM2.5) at 40 monitoring sites nationwide. We conducted a national-<span class="hlt">scale</span> review of near-road <span class="hlt">air</span> pollutant concentrations, identified areas where high concentrations of NO2, PM2.5, and CO occurred, and evaluated how concentrations varied by factors such as location, distance to roadway, fleet mix characteristics, and traffic volume. We present the findings from our national near-road data assessment for the 2014 monitoring year.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA541459','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA541459"><span><span class="hlt">Large-Scale</span> Aerosol Modeling and Analysis</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2007-09-30</p> <p>deserts of the world: Arabian Gulf, Sea of Japan, China Sea , Mediterranean Sea , and the Tropical Atlantic Ocean. NAAPS also accurately predicts the...fate of <span class="hlt">large-scale</span> smoke and pollution plumes. With its global and continuous coverage, 1 Report Documentation Page Form ApprovedOMB No. 0704-0188...origin of dust plumes impacting naval operations in the Red Sea , Mediterranean, eastern Atlantic, Gulf of Guinea, Sea of Japan, Yellow Sea , and East</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('http://adsabs.harvard.edu/abs/2013PhRvE..87e3110P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013PhRvE..87e3110P"><span><span class="hlt">Large-scale</span> dynamo growth rates from numerical simulations and implications for mean-field theories</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Park, Kiwan; Blackman, Eric G.; Subramanian, Kandaswamy</p> <p>2013-05-01</p> <p>Understanding <span class="hlt">large-scale</span> magnetic field growth in turbulent plasmas in the magnetohydrodynamic limit is a goal of magnetic dynamo theory. In particular, assessing how well <span class="hlt">large-scale</span> helical field growth and saturation in simulations match those predicted by existing theories is important for progress. Using numerical simulations of isotropically forced turbulence without <span class="hlt">large-scale</span> shear with its implications, we focus on several additional aspects of this comparison: (1) Leading mean-field dynamo theories which break the field into <span class="hlt">large</span> and small <span class="hlt">scales</span> predict that <span class="hlt">large-scale</span> helical field growth rates are determined by the difference between kinetic helicity and current helicity with no dependence on the nonhelical energy in small-<span class="hlt">scale</span> magnetic fields. Our simulations show that the growth rate of the <span class="hlt">large-scale</span> field from fully helical forcing is indeed unaffected by the presence or absence of small-<span class="hlt">scale</span> magnetic fields amplified in a precursor nonhelical dynamo. However, because the precursor nonhelical dynamo in our simulations produced fields that were strongly subequipartition with respect to the kinetic energy, we cannot yet rule out the potential influence of stronger nonhelical small-<span class="hlt">scale</span> fields. (2) We have identified two features in our simulations which cannot be explained by the most minimalist versions of two-<span class="hlt">scale</span> mean-field theory: (i) fully helical small-<span class="hlt">scale</span> forcing produces significant nonhelical <span class="hlt">large-scale</span> magnetic energy and (ii) the saturation of the <span class="hlt">large-scale</span> field growth is time delayed with respect to what minimalist theory predicts. We comment on desirable generalizations to the theory in this context and future desired work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23767646','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23767646"><span><span class="hlt">Large-scale</span> dynamo growth rates from numerical simulations and implications for mean-field theories.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Park, Kiwan; Blackman, Eric G; Subramanian, Kandaswamy</p> <p>2013-05-01</p> <p>Understanding <span class="hlt">large-scale</span> magnetic field growth in turbulent plasmas in the magnetohydrodynamic limit is a goal of magnetic dynamo theory. In particular, assessing how well <span class="hlt">large-scale</span> helical field growth and saturation in simulations match those predicted by existing theories is important for progress. Using numerical simulations of isotropically forced turbulence without <span class="hlt">large-scale</span> shear with its implications, we focus on several additional aspects of this comparison: (1) Leading mean-field dynamo theories which break the field into <span class="hlt">large</span> and small <span class="hlt">scales</span> predict that <span class="hlt">large-scale</span> helical field growth rates are determined by the difference between kinetic helicity and current helicity with no dependence on the nonhelical energy in small-<span class="hlt">scale</span> magnetic fields. Our simulations show that the growth rate of the <span class="hlt">large-scale</span> field from fully helical forcing is indeed unaffected by the presence or absence of small-<span class="hlt">scale</span> magnetic fields amplified in a precursor nonhelical dynamo. However, because the precursor nonhelical dynamo in our simulations produced fields that were strongly subequipartition with respect to the kinetic energy, we cannot yet rule out the potential influence of stronger nonhelical small-<span class="hlt">scale</span> fields. (2) We have identified two features in our simulations which cannot be explained by the most minimalist versions of two-<span class="hlt">scale</span> mean-field theory: (i) fully helical small-<span class="hlt">scale</span> forcing produces significant nonhelical <span class="hlt">large-scale</span> magnetic energy and (ii) the saturation of the <span class="hlt">large-scale</span> field growth is time delayed with respect to what minimalist theory predicts. We comment on desirable generalizations to the theory in this context and future desired work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20170003692&hterms=systematic+reviews&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsystematic%2Breviews','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20170003692&hterms=systematic+reviews&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dsystematic%2Breviews"><span>North American Extreme Temperature Events and Related <span class="hlt">Large</span> <span class="hlt">Scale</span> Meteorological Patterns: A Review of Statistical Methods, Dynamics, Modeling, and Trends</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Grotjahn, Richard; Black, Robert; Leung, Ruby; Wehner, Michael F.; Barlow, Mathew; Bosilovich, Michael G.; Gershunov, Alexander; Gutowski, William J., Jr.; Gyakum, John R.; Katz, Richard W.; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20170003692'); toggleEditAbsImage('author_20170003692_show'); toggleEditAbsImage('author_20170003692_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20170003692_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20170003692_hide"></p> <p>2015-01-01</p> <p>The objective of this paper is to review statistical methods, dynamics, modeling efforts, and trends related to temperature extremes, with a focus upon extreme events of short duration that affect parts of North America. These events are associated with <span class="hlt">large</span> <span class="hlt">scale</span> meteorological patterns (LSMPs). The statistics, dynamics, and modeling sections of this paper are written to be autonomous and so can be read separately. Methods to define extreme events statistics and to identify and connect LSMPs to extreme temperature events are presented. Recent advances in statistical techniques connect LSMPs to extreme temperatures through appropriately defined covariates that supplement more straightforward analyses. Various LSMPs, ranging from synoptic to planetary <span class="hlt">scale</span> structures, are associated with extreme temperature events. Current knowledge about the synoptics and the dynamical mechanisms leading to the associated LSMPs is incomplete. Systematic studies of: the physics of LSMP life cycles, comprehensive model assessment of LSMP-extreme temperature event linkages, and LSMP properties are needed. Generally, climate models capture observed properties of heat waves and cold <span class="hlt">air</span> outbreaks with some fidelity. However they overestimate warm wave frequency and underestimate cold <span class="hlt">air</span> outbreak frequency, and underestimate the collective influence of low-frequency modes on temperature extremes. Modeling studies have identified the impact of <span class="hlt">large-scale</span> circulation anomalies and landatmosphere interactions on changes in extreme temperatures. However, few studies have examined changes in LSMPs to more specifically understand the role of LSMPs on past and future extreme temperature changes. Even though LSMPs are resolvable by global and regional climate models, they are not necessarily well simulated. The paper concludes with unresolved issues and research questions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA490778','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA490778"><span>No Winglets: What a Drag...Argument for Adding Winglets to <span class="hlt">Large</span> <span class="hlt">Air</span> Force Aircraft</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2008-01-01</p> <p>22134-5068 MASTER OF MILITARY STUDIES NO WINGLETS : WHAT A DRAG... ARGUMENT FOR ADDING WINGLETS TO <span class="hlt">LARGE</span> <span class="hlt">AIR</span> FORCE AIRCRAFT ,SUBMITTED IN PARTIAL...currently valid OMB control number. 1. REPORT DATE 2008 2. REPORT TYPE 3. DATES COVERED 00-00-2008 to 00-00-2008 4. TITLE AND SUBTITLE No Winglets ...What a Drag...Argument for Adding Winglets to <span class="hlt">Large</span> <span class="hlt">Air</span> Force Aircraft 5a. CONTRACT NUMBER 5b. GRANT NUMBER 5c. PROGRAM ELEMENT NUMBER 6. AUTHOR</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=45647&Lab=NERL&keyword=R+AND+programming&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=45647&Lab=NERL&keyword=R+AND+programming&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>REPRESENTATION OF ATMOSPHERIC MOTION IN MODELS OF REGIONAL-<span class="hlt">SCALE</span> <span class="hlt">AIR</span> POLLUTION</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>A method is developed for generating ensembles of wind fields for use in regional <span class="hlt">scale</span> (1000 km) models of transport and diffusion. The underlying objective is a methodology for representing atmospheric motion in applied <span class="hlt">air</span> pollution models that permits explicit treatment of th...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=agent+AND+orange&id=EJ424645','ERIC'); return false;" href="https://eric.ed.gov/?q=agent+AND+orange&id=EJ424645"><span>Considerations for Managing <span class="hlt">Large-Scale</span> Clinical Trials.</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>Tuttle, Waneta C.; And Others</p> <p>1989-01-01</p> <p>Research management strategies used effectively in a <span class="hlt">large-scale</span> clinical trial to determine the health effects of exposure to Agent Orange in Vietnam are discussed, including pre-project planning, organization according to strategy, attention to scheduling, a team approach, emphasis on guest relations, cross-training of personnel, and preparing…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1104917','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1104917"><span><span class="hlt">Large-Scale</span> Optimization for Bayesian Inference in Complex Systems</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>Willcox, Karen; Marzouk, Youssef</p> <p>2013-11-12</p> <p>The SAGUARO (Scalable Algorithms for Groundwater Uncertainty Analysis and Robust Optimization) Project focused on the development of scalable numerical algorithms for <span class="hlt">large-scale</span> Bayesian inversion in complex systems that capitalize on advances in <span class="hlt">large-scale</span> simulation-based optimization and inversion methods. The project was a collaborative effort among MIT, the University of Texas at Austin, Georgia Institute of Technology, and Sandia National Laboratories. The research was directed in three complementary areas: efficient approximations of the Hessian operator, reductions in complexity of forward simulations via stochastic spectral approximations and model reduction, and employing <span class="hlt">large-scale</span> optimization concepts to accelerate sampling. The MIT--Sandia component of themore » SAGUARO Project addressed the intractability of conventional sampling methods for <span class="hlt">large-scale</span> statistical inverse problems by devising reduced-order models that are faithful to the full-order model over a wide range of parameter values; sampling then employs the reduced model rather than the full model, resulting in very <span class="hlt">large</span> computational savings. Results indicate little effect on the computed posterior distribution. On the other hand, in the Texas--Georgia Tech component of the project, we retain the full-order model, but exploit inverse problem structure (adjoint-based gradients and partial Hessian information of the parameter-to-observation map) to implicitly extract lower dimensional information on the posterior distribution; this greatly speeds up sampling methods, so that fewer sampling points are needed. We can think of these two approaches as ``reduce then sample'' and ``sample then reduce.'' In fact, these two approaches are complementary, and can be used in conjunction with each other. Moreover, they both exploit deterministic inverse problem structure, in the form of adjoint-based gradient and Hessian information of the underlying parameter-to-observation map, to achieve</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19760052987&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dneither%2Bdeep%2Bshallow','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19760052987&hterms=neither+deep+shallow&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dneither%2Bdeep%2Bshallow"><span>Response of deep and shallow tropical maritime cumuli to <span class="hlt">large-scale</span> processes</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Yanai, M.; Chu, J.-H.; Stark, T. E.; Nitta, T.</p> <p>1976-01-01</p> <p>The bulk diagnostic method of Yanai et al. (1973) and a simplified version of the spectral diagnostic method of Nitta (1975) are used for a more quantitative evaluation of the response of various types of cumuliform clouds to <span class="hlt">large-scale</span> processes, using the same data set in the Marshall Islands area for a 100-day period in 1956. The dependence of the cloud mass flux distribution on radiative cooling, <span class="hlt">large-scale</span> vertical motion, and evaporation from the sea is examined. It is shown that typical radiative cooling rates in the tropics tend to produce a bimodal distribution of mass spectrum exhibiting deep and shallow clouds. The bimodal distribution is further enhanced when the <span class="hlt">large-scale</span> vertical motion is upward, and a nearly unimodal distribution of shallow clouds prevails when the relative cooling is compensated by the heating due to the <span class="hlt">large-scale</span> subsidence. Both deep and shallow clouds are modulated by <span class="hlt">large-scale</span> disturbances. The primary role of surface evaporation is to maintain the moisture flux at the cloud base.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1332518','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1332518"><span><span class="hlt">Large-scale</span> dynamo action precedes turbulence in shearing box simulations of the magnetorotational instability</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>Bhat, Pallavi; Ebrahimi, Fatima; Blackman, Eric G.</p> <p></p> <p>Here, we study the dynamo generation (exponential growth) of <span class="hlt">large-scale</span> (planar averaged) fields in unstratified shearing box simulations of the magnetorotational instability (MRI). In contrast to previous studies restricted to horizontal (x–y) averaging, we also demonstrate the presence of <span class="hlt">large-scale</span> fields when vertical (y–z) averaging is employed instead. By computing space–time planar averaged fields and power spectra, we find <span class="hlt">large-scale</span> dynamo action in the early MRI growth phase – a previously unidentified feature. Non-axisymmetric linear MRI modes with low horizontal wavenumbers and vertical wavenumbers near that of expected maximal growth, amplify the <span class="hlt">large-scale</span> fields exponentially before turbulence and high wavenumbermore » fluctuations arise. Thus the <span class="hlt">large-scale</span> dynamo requires only linear fluctuations but not non-linear turbulence (as defined by mode–mode coupling). Vertical averaging also allows for monitoring the evolution of the <span class="hlt">large-scale</span> vertical field and we find that a feedback from horizontal low wavenumber MRI modes provides a clue as to why the <span class="hlt">large-scale</span> vertical field sustains against turbulent diffusion in the non-linear saturation regime. We compute the terms in the mean field equations to identify the individual contributions to <span class="hlt">large-scale</span> field growth for both types of averaging. The <span class="hlt">large-scale</span> fields obtained from vertical averaging are found to compare well with global simulations and quasi-linear analytical analysis from a previous study by Ebrahimi & Blackman. We discuss the potential implications of these new results for understanding the <span class="hlt">large-scale</span> MRI dynamo saturation and turbulence.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1332518-large-scale-dynamo-action-precedes-turbulence-shearing-box-simulations-magnetorotational-instability','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1332518-large-scale-dynamo-action-precedes-turbulence-shearing-box-simulations-magnetorotational-instability"><span><span class="hlt">Large-scale</span> dynamo action precedes turbulence in shearing box simulations of the magnetorotational instability</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Bhat, Pallavi; Ebrahimi, Fatima; Blackman, Eric G.</p> <p>2016-07-06</p> <p>Here, we study the dynamo generation (exponential growth) of <span class="hlt">large-scale</span> (planar averaged) fields in unstratified shearing box simulations of the magnetorotational instability (MRI). In contrast to previous studies restricted to horizontal (x–y) averaging, we also demonstrate the presence of <span class="hlt">large-scale</span> fields when vertical (y–z) averaging is employed instead. By computing space–time planar averaged fields and power spectra, we find <span class="hlt">large-scale</span> dynamo action in the early MRI growth phase – a previously unidentified feature. Non-axisymmetric linear MRI modes with low horizontal wavenumbers and vertical wavenumbers near that of expected maximal growth, amplify the <span class="hlt">large-scale</span> fields exponentially before turbulence and high wavenumbermore » fluctuations arise. Thus the <span class="hlt">large-scale</span> dynamo requires only linear fluctuations but not non-linear turbulence (as defined by mode–mode coupling). Vertical averaging also allows for monitoring the evolution of the <span class="hlt">large-scale</span> vertical field and we find that a feedback from horizontal low wavenumber MRI modes provides a clue as to why the <span class="hlt">large-scale</span> vertical field sustains against turbulent diffusion in the non-linear saturation regime. We compute the terms in the mean field equations to identify the individual contributions to <span class="hlt">large-scale</span> field growth for both types of averaging. The <span class="hlt">large-scale</span> fields obtained from vertical averaging are found to compare well with global simulations and quasi-linear analytical analysis from a previous study by Ebrahimi & Blackman. We discuss the potential implications of these new results for understanding the <span class="hlt">large-scale</span> MRI dynamo saturation and turbulence.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016APS..DFDR39006S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016APS..DFDR39006S"><span>Flagellum synchronization inhibits <span class="hlt">large-scale</span> hydrodynamic instabilities in sperm suspensions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schöller, Simon F.; Keaveny, Eric E.</p> <p>2016-11-01</p> <p>Sperm in suspension can exhibit <span class="hlt">large-scale</span> collective motion and form coherent structures. Our picture of such coherent motion is <span class="hlt">largely</span> based on reduced models that treat the swimmers as self-locomoting rigid bodies that interact via steady dipolar flow fields. Swimming sperm, however, have many more degrees of freedom due to elasticity, have a more exotic shape, and generate spatially-complex, time-dependent flow fields. While these complexities are known to lead to phenomena such as flagellum synchronization and attraction, how these effects impact the overall suspension behaviour and coherent structure formation is <span class="hlt">largely</span> unknown. Using a computational model that captures both flagellum beating and elasticity, we simulate suspensions on the order of 103 individual swimming sperm cells whose motion is coupled through the surrounding Stokesian fluid. We find that the tendency for flagella to synchronize and sperm to aggregate inhibits the emergence of the <span class="hlt">large-scale</span> hydrodynamic instabilities often associated with active suspensions. However, when synchronization is repressed by adding noise in the flagellum actuation mechanism, the picture changes and the structures that resemble <span class="hlt">large-scale</span> vortices appear to re-emerge. Supported by an Imperial College PhD scholarship.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1912910L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1912910L"><span>Contractual Duration and Investment Incentives: Evidence from <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units in China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Fang; Feng, Shuyi; D'Haese, Marijke; Lu, Hualiang; Qu, Futian</p> <p>2017-04-01</p> <p><span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units have become important forces in the supply of agricultural commodities and agricultural modernization in China. Contractual duration in farmland transfer to <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units can be considered to reflect land tenure security. Theoretically, long-term tenancy contracts can encourage <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units to increase long-term investments by ensuring land rights stability or favoring access to credit. Using a unique <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units- and plot-level field survey dataset from Jiangsu and Jiangxi Province, this study aims to examine the effect of contractual duration on <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units' soil conservation behaviours. IV method is applied to take into account the endogeneity of contractual duration and unobserved household heterogeneity. Results indicate that farmland transfer contract duration significantly and positively affects land-improving investments. Policies aimed at improving transaction platforms and intermediary organizations in farmland transfer to facilitate <span class="hlt">Large</span> <span class="hlt">Scale</span> Production Units to access farmland with long-term tenancy contracts may therefore play an important role in improving soil quality and land productivity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2585521','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2585521"><span>Clinical Investigation and Mechanism of <span class="hlt">Air</span>-Bone Gaps in <span class="hlt">Large</span>Vestibular Aqueduct Syndrome</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Merchant, Saumil N.; Nakajima, Hideko H.; Halpin, Christopher; Nadol, Joseph B.; Lee, Daniel J.; Innis, William P.; Curtin, Hugh; Rosowski, John J.</p> <p>2008-01-01</p> <p>Objectives Patients with <span class="hlt">large</span> vestibular aqueduct syndrome (LVAS) often demonstrate an <span class="hlt">air</span>-bone gap at the low frequencies on audiometric testing. The mechanism causing such a gap has not been well elucidated. We investigated middle ear sound transmission in patients with LVAS, and present a hypothesis to explain the <span class="hlt">air</span>-bone gap. Methods Observations were made on 8 ears from 5 individuals with LVAS. The diagnosis of LVAS was made by computed tomography in all cases. Investigations included standard audiometry and measurements of umbo velocity by laser Doppler vibrometry (LDV) in all cases, as well as tympanometry, acoustic reflex testing, vestibular evoked myogenic potential (VEMP) testing, distortion product otoacoustic emission (DPOAE) testing, and middle ear exploration in some ears. Results One ear with LVAS had anacusis. The other 7 ears demonstrated <span class="hlt">air</span>-bone gaps at the low frequencies, with mean gaps of 51 dB at 250 Hz, 31 dB at 500 Hz, and 12 dB at 1,000 Hz. In these 7 ears with <span class="hlt">air</span>-bone gaps, LDV showed the umbo velocity to be normal or high normal in all 7; tympanometry was normal in all 6 ears tested; acoustic reflexes were present in 3 of the 4 ears tested; VEMP responses were present in all 3 ears tested; DPOAEs were present in 1 of the 2 ears tested, and exploratory tympanotomy in 1 case showed a normal middle ear. The above data suggest that an <span class="hlt">air</span>-bone gap in LVAS is not due to disease in the middle ear. The data are consistent with the hypothesis that a <span class="hlt">large</span> vestibular aqueduct introduces a third mobile window into the inner ear, which can produce an <span class="hlt">air</span>-bone gap by 1) shunting <span class="hlt">air</span>-conducted sound away from the cochlea, thus elevating <span class="hlt">air</span> conduction thresholds, and 2) increasing the difference in impedance between the scala vestibuli side and the scala tympani side of the cochlear partition during bone conduction testing, thus improving thresholds for bone-conducted sound. Conclusions We conclude that LVAS can present with an <span class="hlt">air</span>-bone gap that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/17727085','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/17727085"><span>Clinical investigation and mechanism of <span class="hlt">air</span>-bone gaps in <span class="hlt">large</span> vestibular aqueduct syndrome.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Merchant, Saumil N; Nakajima, Hideko H; Halpin, Christopher; Nadol, Joseph B; Lee, Daniel J; Innis, William P; Curtin, Hugh; Rosowski, John J</p> <p>2007-07-01</p> <p>Patients with <span class="hlt">large</span> vestibular aqueduct syndrome (LVAS) often demonstrate an <span class="hlt">air</span>-bone gap at the low frequencies on audiometric testing. The mechanism causing such a gap has not been well elucidated. We investigated middle ear sound transmission in patients with LVAS, and present a hypothesis to explain the <span class="hlt">air</span>-bone gap. Observations were made on 8 ears from 5 individuals with LVAS. The diagnosis of LVAS was made by computed tomography in all cases. Investigations included standard audiometry and measurements of umbo velocity by laser Doppler vibrometry (LDV) in all cases, as well as tympanometry, acoustic reflex testing, vestibular evoked myogenic potential (VEMP) testing, distortion product otoacoustic emission (DPOAE) testing, and middle ear exploration in some ears. One ear with LVAS had anacusis. The other 7 ears demonstrated <span class="hlt">air</span>-bone gaps at the low frequencies, with mean gaps of 51 dB at 250 Hz, 31 dB at 500 Hz, and 12 dB at 1,000 Hz. In these 7 ears with <span class="hlt">air</span>-bone gaps, LDV showed the umbo velocity to be normal or high normal in all 7; tympanometry was normal in all 6 ears tested; acoustic reflexes were present in 3 of the 4 ears tested; VEMP responses were present in all 3 ears tested; DPOAEs were present in 1 of the 2 ears tested, and exploratory tympanotomy in 1 case showed a normal middle ear. The above data suggest that an <span class="hlt">air</span>-bone gap in LVAS is not due to disease in the middle ear. The data are consistent with the hypothesis that a <span class="hlt">large</span> vestibular aqueduct introduces a third mobile window into the inner ear, which can produce an <span class="hlt">air</span>-bone gap by 1) shunting <span class="hlt">air</span>-conducted sound away from the cochlea, thus elevating <span class="hlt">air</span> conduction thresholds, and 2) increasing the difference in impedance between the scala vestibuli side and the scala tympani side of the cochlear partition during bone conduction testing, thus improving thresholds for bone-conducted sound. We conclude that LVAS can present with an <span class="hlt">air</span>-bone gap that can mimic middle ear disease. Diagnostic</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16888466','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16888466"><span>Reliability of <span class="hlt">air</span> displacement plethysmography in a <span class="hlt">large</span>, heterogeneous sample.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Noreen, Eric E; Lemon, Peter W R</p> <p>2006-08-01</p> <p>Several studies have assessed the validity of <span class="hlt">air</span> displacement plethysmography (ADP), but few have assessed the reliability of ADP using a <span class="hlt">large</span>, heterogeneous sample. This study was conducted to determine the reliability of ADP using the Bod Pod in a <span class="hlt">large</span>, heterogeneous sample. A total of 980 healthy men and women (30 +/- 15 yr, mean +/- SD) completed two body composition assessments separated by 15-30 min. All testing was done in accordance with the manufacturer's instructions. A significant correlation (r = 0.992, P = 0.001) was found between body density (BD) 1 (1.046 +/- 0.001 kg.L(-1); mean +/- SEM) and BD 2 (1.046 +/- 0.001 kg.L(-1). A paired t-test <span class="hlt">revealed</span> no significant difference between BD 1 and 2 (P = 0.935). The coefficient of variation (CV) for BD was 0.15%. A significant intraclass correlation coefficient (ICC) was found for BD (ICC = 0.996, P = 0.001), and the standard error of measurement (SEM) was 0.001 kg.L(-1). Body mass (BM) 1 and 2 were correlated significantly (r = 0.999, P = 0.001); however, a significant (P = 0.001) decrease was seen from BM 1 (75.510 +/- 0.461 kg) to BM 2 (75.497 +/- 0.461 kg). Body volume (BV) tended to decrease (P = 0.08) from BV 1 (69.900 +/- 0.449 L) to BV 2 (69.884 +/- 0.449 L). ADP using the Bod Pod appears to assess BD reliably; however, the observed CV suggests that multiple trials are necessary to detect small treatment effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/32096','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/32096"><span>Small-<span class="hlt">scale</span> monitoring - can it be integrated with <span class="hlt">large-scale</span> programs?</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>C. M. Downes; J. Bart; B. T. Collins; B. Craig; B. Dale; E. H. Dunn; C. M. Francis; S. Woodley; P. Zorn</p> <p>2005-01-01</p> <p>There are dozens of programs and methodologies for monitoring and inventory of bird populations, differing in geographic scope, species focus, field methods and purpose. However, most of the emphasis has been placed on <span class="hlt">large-scale</span> monitoring programs. People interested in assessing bird numbers and long-term trends in small geographic areas such as a local birding area...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ISPAr42W8...53C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ISPAr42W8...53C"><span>Utilization of <span class="hlt">Large</span> <span class="hlt">Scale</span> Surface Models for Detailed Visibility Analyses</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Caha, J.; Kačmařík, M.</p> <p>2017-11-01</p> <p>This article demonstrates utilization of <span class="hlt">large</span> <span class="hlt">scale</span> surface models with small spatial resolution and high accuracy, acquired from Unmanned Aerial Vehicle scanning, for visibility analyses. The importance of <span class="hlt">large</span> <span class="hlt">scale</span> data for visibility analyses on the local <span class="hlt">scale</span>, where the detail of the surface model is the most defining factor, is described. The focus is not only the classic Boolean visibility, that is usually determined within GIS, but also on so called extended viewsheds that aims to provide more information about visibility. The case study with examples of visibility analyses was performed on river Opava, near the Ostrava city (Czech Republic). The multiple Boolean viewshed analysis and global horizon viewshed were calculated to determine most prominent features and visibility barriers of the surface. Besides that, the extended viewshed showing angle difference above the local horizon, which describes angular height of the target area above the barrier, is shown. The case study proved that <span class="hlt">large</span> <span class="hlt">scale</span> models are appropriate data source for visibility analyses on local level. The discussion summarizes possible future applications and further development directions of visibility analyses.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19790030210&hterms=decentralized&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Ddecentralized','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19790030210&hterms=decentralized&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Ddecentralized"><span>On decentralized control of <span class="hlt">large-scale</span> systems</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Siljak, D. D.</p> <p>1978-01-01</p> <p>A scheme is presented for decentralized control of <span class="hlt">large-scale</span> linear systems which are composed of a number of interconnected subsystems. By ignoring the interconnections, local feedback controls are chosen to optimize each decoupled subsystem. Conditions are provided to establish compatibility of the individual local controllers and achieve stability of the overall system. Besides computational simplifications, the scheme is attractive because of its structural features and the fact that it produces a robust decentralized regulator for <span class="hlt">large</span> dynamic systems, which can tolerate a wide range of nonlinearities and perturbations among the subsystems.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2006RaSc...41.2010F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2006RaSc...41.2010F"><span><span class="hlt">Large-scale</span> modeling of rain fields from a rain cell deterministic model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>FéRal, Laurent; Sauvageot, Henri; Castanet, Laurent; Lemorton, JoëL.; Cornet, FréDéRic; Leconte, Katia</p> <p>2006-04-01</p> <p>A methodology to simulate two-dimensional rain rate fields at <span class="hlt">large</span> <span class="hlt">scale</span> (1000 × 1000 km2, the <span class="hlt">scale</span> of a satellite telecommunication beam or a terrestrial fixed broadband wireless access network) is proposed. It relies on a rain rate field cellular decomposition. At small <span class="hlt">scale</span> (˜20 × 20 km2), the rain field is split up into its macroscopic components, the rain cells, described by the Hybrid Cell (HYCELL) cellular model. At midscale (˜150 × 150 km2), the rain field results from the conglomeration of rain cells modeled by HYCELL. To account for the rain cell spatial distribution at midscale, the latter is modeled by a doubly aggregative isotropic random walk, the optimal parameterization of which is derived from radar observations at midscale. The extension of the simulation area from the midscale to the <span class="hlt">large</span> <span class="hlt">scale</span> (1000 × 1000 km2) requires the modeling of the weather frontal area. The latter is first modeled by a Gaussian field with anisotropic covariance function. The Gaussian field is then turned into a binary field, giving the <span class="hlt">large-scale</span> locations over which it is raining. This transformation requires the definition of the rain occupation rate over <span class="hlt">large-scale</span> areas. Its probability distribution is determined from observations by the French operational radar network ARAMIS. The coupling with the rain field modeling at midscale is immediate whenever the <span class="hlt">large-scale</span> field is split up into midscale subareas. The rain field thus generated accounts for the local CDF at each point, defining a structure spatially correlated at small <span class="hlt">scale</span>, midscale, and <span class="hlt">large</span> <span class="hlt">scale</span>. It is then suggested that this approach be used by system designers to evaluate diversity gain, terrestrial path attenuation, or slant path attenuation for different azimuth and elevation angle directions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AtmEn.160...36H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AtmEn.160...36H"><span>Persistence of initial conditions in continental <span class="hlt">scale</span> <span class="hlt">air</span> quality simulations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hogrefe, Christian; Roselle, Shawn J.; Bash, Jesse O.</p> <p>2017-07-01</p> <p>This study investigates the effect of initial conditions (IC) for pollutant concentrations in the atmosphere and soil on simulated <span class="hlt">air</span> quality for two continental-<span class="hlt">scale</span> Community Multiscale <span class="hlt">Air</span> Quality (CMAQ) model applications. One of these applications was performed for springtime and the second for summertime. Results show that a spin-up period of ten days commonly used in regional-<span class="hlt">scale</span> applications may not be sufficient to reduce the effects of initial conditions to less than 1% of seasonally-averaged surface ozone concentrations everywhere while 20 days were found to be sufficient for the entire domain for the spring case and almost the entire domain for the summer case. For the summer case, differences were found to persist longer aloft due to circulation of <span class="hlt">air</span> masses and even a spin-up period of 30 days was not sufficient to reduce the effects of ICs to less than 1% of seasonally-averaged layer 34 ozone concentrations over the southwestern portion of the modeling domain. Analysis of the effect of soil initial conditions for the CMAQ bidirectional NH3 exchange model shows that during springtime they can have an important effect on simulated inorganic aerosols concentrations for time periods of one month or longer. The effects are less pronounced during other seasons. The results, while specific to the modeling domain and time periods simulated here, suggest that modeling protocols need to be scrutinized for a given application and that it cannot be assumed that commonly-used spin-up periods are necessarily sufficient to reduce the effects of initial conditions on model results to an acceptable level. What constitutes an acceptable level of difference cannot be generalized and will depend on the particular application, time period and species of interest. Moreover, as the application of <span class="hlt">air</span> quality models is being expanded to cover larger geographical domains and as these models are increasingly being coupled with other modeling systems to better represent</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/2018MRE.....5d5046N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MRE.....5d5046N"><span>Facile <span class="hlt">Large-scale</span> synthesis of stable CuO nanoparticles</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nazari, P.; Abdollahi-Nejand, B.; Eskandari, M.; Kohnehpoushi, S.</p> <p>2018-04-01</p> <p>In this work, a novel approach in synthesizing the CuO nanoparticles was introduced. A sequential corrosion and detaching was proposed in the growth and dispersion of CuO nanoparticles in the optimum pH value of eight. The produced CuO nanoparticles showed six nm (±2 nm) in diameter and spherical feather with a high crystallinity and uniformity in size. In this method, a <span class="hlt">large-scale</span> production of CuO nanoparticles (120 grams in an experimental batch) from Cu micro-particles was achieved which may met the market criteria for <span class="hlt">large-scale</span> production of CuO nanoparticles.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/6725226','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/6725226"><span><span class="hlt">Large</span> <span class="hlt">scale</span> preparation and crystallization of neuron-specific enolase.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ishioka, N; Isobe, T; Kadoya, T; Okuyama, T; Nakajima, T</p> <p>1984-03-01</p> <p>A simple method has been developed for the <span class="hlt">large</span> <span class="hlt">scale</span> purification of neuron-specific enolase [EC 4.2.1.11]. The method consists of ammonium sulfate fractionation of brain extract, and two subsequent column chromatography steps on DEAE Sephadex A-50. The chromatography was performed on a short (25 cm height) and thick (8.5 cm inside diameter) column unit that was specially devised for the <span class="hlt">large</span> <span class="hlt">scale</span> preparation. The purified enolase was crystallized in 0.05 M imidazole-HCl buffer containing 1.6 M ammonium sulfate (pH 6.39), with a yield of 0.9 g/kg of bovine brain tissue.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23274216','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23274216"><span>A <span class="hlt">large-scale</span> phylogeny of Synodontis (Mochokidae, Siluriformes) <span class="hlt">reveals</span> the influence of geological events on continental diversity during the Cenozoic.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pinton, Aurélie; Agnèse, Jean-François; Paugy, Didier; Otero, Olga</p> <p>2013-03-01</p> <p>To explain the spatial variability of fish taxa at a <span class="hlt">large</span> <span class="hlt">scale</span>, two alternative proposals are usually evoked. In recent years, the debate has centred on the relative roles of present and historical processes in shaping biodiversity patterns. In Africa, attempts to understand the processes that determine the <span class="hlt">large</span> <span class="hlt">scale</span> distribution of fishes and exploration of historical contingencies have been under-investigated given that most of the phylogenetic studies focus on the history of the Great Lakes. Here, we explore phylogeographic events in the evolutionary history of Synodontis (Mohokidae, Siluriformes) over Africa during the Cenozoic focusing on the putative role of historical processes. We discuss how known geological events together with hydrographical changes contributed to shape Synodontis biogeographical history. Synodontis was chosen on the basis of its high diversity and distribution in Africa: it consists of approximately 120 species that are widely distributed in all hydrographic basins except the Maghreb and South Africa. We propose the most comprehensive phylogeny of this catfish genus. Our results provide support for the 'hydrogeological' hypothesis, which proposes that palaeohydrological changes linked with the geological context may have been the cause of diversification of freshwater fish deep in the Tertiary. More precisely, the two main geological structures that participated to shape the hydrographical network in Africa, namely the Central African Shear zone and the East African rift system, appear as strong drivers of Synodontis diversification and evolution. Copyright © 2012 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JHyd..546..262M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JHyd..546..262M"><span>Multi-time-<span class="hlt">scale</span> hydroclimate dynamics of a regional watershed and links to <span class="hlt">large-scale</span> atmospheric circulation: Application to the Seine river catchment, France</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Massei, N.; Dieppois, B.; Hannah, D. M.; Lavers, D. A.; Fossa, M.; Laignel, B.; Debret, M.</p> <p>2017-03-01</p> <p> approach basically consisted in three steps: 1 - decomposing <span class="hlt">large-scale</span> climate and hydrological signals (SLP field, precipitation or streamflow) using discrete wavelet multiresolution analysis, 2 - generating a statistical downscaling model per time-<span class="hlt">scale</span>, 3 - summing up all <span class="hlt">scale</span>-dependent models in order to obtain a final reconstruction of the predictand. The results obtained <span class="hlt">revealed</span> a significant improvement of the reconstructions for both precipitation and streamflow when using the multiresolution ESD model instead of basic ESD. In particular, the multiresolution ESD model handled very well the significant changes in variance through time observed in either precipitation or streamflow. For instance, the post-1980 period, which had been characterized by particularly high amplitudes in interannual-to-interdecadal variability associated with alternating flood and extremely low-flow/drought periods (e.g., winter/spring 2001, summer 2003), could not be reconstructed without integrating wavelet multiresolution analysis into the model. In accordance with previous studies, the wavelet components detected in SLP, precipitation and streamflow on interannual to interdecadal time-<span class="hlt">scales</span> could be interpreted in terms of influence of the Gulf-Stream oceanic front on atmospheric circulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=63543&keyword=agent+AND+based+AND+modeling&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=63543&keyword=agent+AND+based+AND+modeling&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>AN INTERDISCIPLINARY APPROACH TO ADDRESSING NEIGHBORHOOD <span class="hlt">SCALE</span> <span class="hlt">AIR</span> QUALITY CONCERNS: THE INTEGRATION OF GIS, URBAN MORPHOLOGY, PREDICTIVE METEOROLOGY, AND <span class="hlt">AIR</span> QUALITY MONITORING TOOLS</span></a></p> <p><a target="_blank" href="http://oaspub.epa.gov/eims/query.page">EPA Science Inventory</a></p> <p></p> <p></p> <p>The paper describes a project that combines the capabilities of urban geography, raster-based GIS, predictive meteorological and <span class="hlt">air</span> pollutant diffusion modeling, to support a neighborhood-<span class="hlt">scale</span> <span class="hlt">air</span> quality monitoring pilot study under the U.S. EPA EMPACT Program. The study ha...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED078674.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED078674.pdf"><span>A <span class="hlt">Large</span> <span class="hlt">Scale</span> Computer Terminal Output Controller.</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>Tucker, Paul Thomas</p> <p></p> <p>This paper describes the design and implementation of a <span class="hlt">large</span> <span class="hlt">scale</span> computer terminal output controller which supervises the transfer of information from a Control Data 6400 Computer to a PLATO IV data network. It discusses the cost considerations leading to the selection of educational television channels rather than telephone lines for…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28653410','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28653410"><span>Breeding density, fine-<span class="hlt">scale</span> tracking, and <span class="hlt">large-scale</span> modeling <span class="hlt">reveal</span> the regional distribution of four seabird species.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wakefield, Ewan D; Owen, Ellie; Baer, Julia; Carroll, Matthew J; Daunt, Francis; Dodd, Stephen G; Green, Jonathan A; Guilford, Tim; Mavor, Roddy A; Miller, Peter I; Newell, Mark A; Newton, Stephen F; Robertson, Gail S; Shoji, Akiko; Soanes, Louise M; Votier, Stephen C; Wanless, Sarah; Bolton, Mark</p> <p>2017-10-01</p> <p>Population-level estimates of species' distributions can <span class="hlt">reveal</span> fundamental ecological processes and facilitate conservation. However, these may be difficult to obtain for mobile species, especially colonial central-place foragers (CCPFs; e.g., bats, corvids, social insects), because it is often impractical to determine the provenance of individuals observed beyond breeding sites. Moreover, some CCPFs, especially in the marine realm (e.g., pinnipeds, turtles, and seabirds) are difficult to observe because they range tens to ten thousands of kilometers from their colonies. It is hypothesized that the distribution of CCPFs depends <span class="hlt">largely</span> on habitat availability and intraspecific competition. Modeling these effects may therefore allow distributions to be estimated from samples of individual spatial usage. Such data can be obtained for an increasing number of species using tracking technology. However, techniques for estimating population-level distributions using the telemetry data are poorly developed. This is of concern because many marine CCPFs, such as seabirds, are threatened by anthropogenic activities. Here, we aim to estimate the distribution at sea of four seabird species, foraging from approximately 5,500 breeding sites in Britain and Ireland. To do so, we GPS-tracked a sample of 230 European Shags Phalacrocorax aristotelis, 464 Black-legged Kittiwakes Rissa tridactyla, 178 Common Murres Uria aalge, and 281 Razorbills Alca torda from 13, 20, 12, and 14 colonies, respectively. Using Poisson point process habitat use models, we show that distribution at sea is dependent on (1) density-dependent competition among sympatric conspecifics (all species) and parapatric conspecifics (Kittiwakes and Murres); (2) habitat accessibility and coastal geometry, such that birds travel further from colonies with limited access to the sea; and (3) regional habitat availability. Using these models, we predict space use by birds from unobserved colonies and thereby map the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JSEdT..25..541S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JSEdT..25..541S"><span>Introducing <span class="hlt">Large-Scale</span> Innovation in Schools</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sotiriou, Sofoklis; Riviou, Katherina; Cherouvis, Stephanos; Chelioti, Eleni; Bogner, Franz X.</p> <p>2016-08-01</p> <p>Education reform initiatives tend to promise higher effectiveness in classrooms especially when emphasis is given to e-learning and digital resources. Practical changes in classroom realities or school organization, however, are lacking. A major European initiative entitled Open Discovery Space (ODS) examined the challenge of modernizing school education via a <span class="hlt">large-scale</span> implementation of an open-<span class="hlt">scale</span> methodology in using technology-supported innovation. The present paper describes this innovation scheme which involved schools and teachers all over Europe, embedded technology-enhanced learning into wider school environments and provided training to teachers. Our implementation scheme consisted of three phases: (1) stimulating interest, (2) incorporating the innovation into school settings and (3) accelerating the implementation of the innovation. The scheme's impact was monitored for a school year using five indicators: leadership and vision building, ICT in the curriculum, development of ICT culture, professional development support, and school resources and infrastructure. Based on about 400 schools, our study produced four results: (1) The growth in digital maturity was substantial, even for previously high scoring schools. This was even more important for indicators such as vision and leadership" and "professional development." (2) The evolution of networking is presented graphically, showing the gradual growth of connections achieved. (3) These communities became core nodes, involving numerous teachers in sharing educational content and experiences: One out of three registered users (36 %) has shared his/her educational resources in at least one community. (4) Satisfaction scores ranged from 76 % (offer of useful support through teacher academies) to 87 % (good environment to exchange best practices). Initiatives such as ODS add substantial value to schools on a <span class="hlt">large</span> <span class="hlt">scale</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29226803','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29226803"><span>Quantitative Missense Variant Effect Prediction Using <span class="hlt">Large-Scale</span> Mutagenesis Data.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gray, Vanessa E; Hause, Ronald J; Luebeck, Jens; Shendure, Jay; Fowler, Douglas M</p> <p>2018-01-24</p> <p><span class="hlt">Large</span> datasets describing the quantitative effects of mutations on protein function are becoming increasingly available. Here, we leverage these datasets to develop Envision, which predicts the magnitude of a missense variant's molecular effect. Envision combines 21,026 variant effect measurements from nine <span class="hlt">large-scale</span> experimental mutagenesis datasets, a hitherto untapped training resource, with a supervised, stochastic gradient boosting learning algorithm. Envision outperforms other missense variant effect predictors both on <span class="hlt">large-scale</span> mutagenesis data and on an independent test dataset comprising 2,312 TP53 variants whose effects were measured using a low-throughput approach. This dataset was never used for hyperparameter tuning or model training and thus serves as an independent validation set. Envision prediction accuracy is also more consistent across amino acids than other predictors. Finally, we demonstrate that Envision's performance improves as more <span class="hlt">large-scale</span> mutagenesis data are incorporated. We precompute Envision predictions for every possible single amino acid variant in human, mouse, frog, zebrafish, fruit fly, worm, and yeast proteomes (https://envision.gs.washington.edu/). Copyright © 2017 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA087555','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA087555"><span>Methods for <span class="hlt">Large-Scale</span> Nonlinear Optimization.</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>1980-05-01</p> <p>STANFORD, CALIFORNIA 94305 METHODS FOR <span class="hlt">LARGE-SCALE</span> NONLINEAR OPTIMIZATION by Philip E. Gill, Waiter Murray, I Michael A. Saunden, and Masgaret H. Wright...typical iteration can be partitioned so that where B is an m X m basise matrix. This partition effectively divides the vari- ables into three classes... attention is given to the standard of the coding or the documentation. A much better way of obtaining mathematical software is from a software library</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JPlPh..84c7303K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JPlPh..84c7303K"><span>Generation of <span class="hlt">large-scale</span> vorticity in rotating stratified turbulence with inhomogeneous helicity: mean-field theory</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kleeorin, N.</p> <p>2018-06-01</p> <p>We discuss a mean-field theory of the generation of <span class="hlt">large-scale</span> vorticity in a rotating density stratified developed turbulence with inhomogeneous kinetic helicity. We show that the <span class="hlt">large-scale</span> non-uniform flow is produced due to either a combined action of a density stratified rotating turbulence and uniform kinetic helicity or a combined effect of a rotating incompressible turbulence and inhomogeneous kinetic helicity. These effects result in the formation of a <span class="hlt">large-scale</span> shear, and in turn its interaction with the small-<span class="hlt">scale</span> turbulence causes an excitation of the <span class="hlt">large-scale</span> instability (known as a vorticity dynamo) due to a combined effect of the <span class="hlt">large-scale</span> shear and Reynolds stress-induced generation of the mean vorticity. The latter is due to the effect of <span class="hlt">large-scale</span> shear on the Reynolds stress. A fast rotation suppresses this <span class="hlt">large-scale</span> instability.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017APS..MAR.B7011D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017APS..MAR.B7011D"><span><span class="hlt">Large</span> <span class="hlt">Scale</span> GW Calculations on the Cori System</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Deslippe, Jack; Del Ben, Mauro; da Jornada, Felipe; Canning, Andrew; Louie, Steven</p> <p></p> <p>The NERSC Cori system, powered by 9000+ Intel Xeon-Phi processors, represents one of the largest HPC systems for open-science in the United States and the world. We discuss the optimization of the GW methodology for this system, including both node level and system-<span class="hlt">scale</span> optimizations. We highlight multiple <span class="hlt">large</span> <span class="hlt">scale</span> (thousands of atoms) case studies and discuss both absolute application performance and comparison to calculations on more traditional HPC architectures. We find that the GW method is particularly well suited for many-core architectures due to the ability to exploit a <span class="hlt">large</span> amount of parallelism across many layers of the system. This work was supported by the U.S. Department of Energy, Office of Science, Basic Energy Sciences, Materials Sciences and Engineering Division, as part of the Computational Materials Sciences Program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1454436','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1454436"><span>Lagrangian space consistency relation for <span class="hlt">large</span> <span class="hlt">scale</span> 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>Horn, Bart; Hui, Lam; Xiao, Xiao</p> <p></p> <p>Consistency relations, which relate the squeezed limit of an (N+1)-point correlation function to an N-point function, are non-perturbative symmetry statements that hold even if the associated high momentum modes are deep in the nonlinear regime and astrophysically complex. Recently, Kehagias & Riotto and Peloso & Pietroni discovered a consistency relation applicable to <span class="hlt">large</span> <span class="hlt">scale</span> structure. We show that this can be recast into a simple physical statement in Lagrangian space: that the squeezed correlation function (suitably normalized) vanishes. This holds regardless of whether the correlation observables are at the same time or not, and regardless of whether multiple-streaming is present.more » Furthermore, the simplicity of this statement suggests that an analytic understanding of <span class="hlt">large</span> <span class="hlt">scale</span> structure in the nonlinear regime may be particularly promising in Lagrangian space.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1454436-lagrangian-space-consistency-relation-large-scale-structure','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1454436-lagrangian-space-consistency-relation-large-scale-structure"><span>Lagrangian space consistency relation for <span class="hlt">large</span> <span class="hlt">scale</span> structure</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Horn, Bart; Hui, Lam; Xiao, Xiao</p> <p>2015-09-29</p> <p>Consistency relations, which relate the squeezed limit of an (N+1)-point correlation function to an N-point function, are non-perturbative symmetry statements that hold even if the associated high momentum modes are deep in the nonlinear regime and astrophysically complex. Recently, Kehagias & Riotto and Peloso & Pietroni discovered a consistency relation applicable to <span class="hlt">large</span> <span class="hlt">scale</span> structure. We show that this can be recast into a simple physical statement in Lagrangian space: that the squeezed correlation function (suitably normalized) vanishes. This holds regardless of whether the correlation observables are at the same time or not, and regardless of whether multiple-streaming is present.more » Furthermore, the simplicity of this statement suggests that an analytic understanding of <span class="hlt">large</span> <span class="hlt">scale</span> structure in the nonlinear regime may be particularly promising in Lagrangian space.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1247498-electron-drift-large-scale-solid-xenon','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1247498-electron-drift-large-scale-solid-xenon"><span>Electron drift in a <span class="hlt">large</span> <span class="hlt">scale</span> solid xenon</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Yoo, J.; Jaskierny, W. F.</p> <p>2015-08-21</p> <p>A study of charge drift in a <span class="hlt">large</span> <span class="hlt">scale</span> optically transparent solid xenon is reported. A pulsed high power xenon light source is used to liberate electrons from a photocathode. The drift speeds of the electrons are measured using a 8.7 cm long electrode in both the liquid and solid phase of xenon. In the liquid phase (163 K), the drift speed is 0.193 ± 0.003 cm/μs while the drift speed in the solid phase (157 K) is 0.397 ± 0.006 cm/μs at 900 V/cm over 8.0 cm of uniform electric fields. Furthermore, it is demonstrated that a factor twomore » faster electron drift speed in solid phase xenon compared to that in liquid in a <span class="hlt">large</span> <span class="hlt">scale</span> solid xenon.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatMa..16..139K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatMa..16..139K"><span>Porous microwells for geometry-selective, <span class="hlt">large-scale</span> microparticle arrays</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kim, Jae Jung; Bong, Ki Wan; Reátegui, Eduardo; Irimia, Daniel; Doyle, Patrick S.</p> <p>2017-01-01</p> <p><span class="hlt">Large-scale</span> microparticle arrays (LSMAs) are key for material science and bioengineering applications. However, previous approaches suffer from trade-offs between scalability, precision, specificity and versatility. Here, we present a porous microwell-based approach to create <span class="hlt">large-scale</span> microparticle arrays with complex motifs. Microparticles are guided to and pushed into microwells by fluid flow through small open pores at the bottom of the porous well arrays. A <span class="hlt">scaling</span> theory allows for the rational design of LSMAs to sort and array particles on the basis of their size, shape, or modulus. Sequential particle assembly allows for proximal and nested particle arrangements, as well as particle recollection and pattern transfer. We demonstrate the capabilities of the approach by means of three applications: high-throughput single-cell arrays; microenvironment fabrication for neutrophil chemotaxis; and complex, covert tags by the transfer of an upconversion nanocrystal-laden LSMA.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1513170E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1513170E"><span>Can global hydrological models reproduce <span class="hlt">large</span> <span class="hlt">scale</span> river flood regimes?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Eisner, Stephanie; Flörke, Martina</p> <p>2013-04-01</p> <p>River flooding remains one of the most severe natural hazards. On the one hand, major flood events pose a serious threat to human well-being, causing deaths and considerable economic damage. On the other hand, the periodic occurrence of flood pulses is crucial to maintain the functioning of riverine floodplains and wetlands, and to preserve the ecosystem services the latter provide. In many regions, river floods <span class="hlt">reveal</span> a distinct seasonality, i.e. they occur at a particular time during the year. This seasonality is related to regionally dominant flood generating processes which can be expressed in river flood types. While in data-rich regions (esp. Europe and North America) the analysis of flood regimes can be based on observed river discharge time series, this data is sparse or lacking in many other regions of the world. This gap of knowledge can be filled by global modeling approaches. However, to date most global modeling studies have focused on mean annual or monthly water availability and their change over time while simulating discharge extremes, both floods and droughts, still remains a challenge for <span class="hlt">large</span> <span class="hlt">scale</span> hydrological models. This study will explore the ability of the global hydrological model WaterGAP3 to simulate the <span class="hlt">large</span> <span class="hlt">scale</span> patterns of river flood regimes, represented by seasonal pattern and the dominant flood type. WaterGAP3 simulates the global terrestrial water balance on a 5 arc minute spatial grid (excluding Greenland and Antarctica) at a daily time step. The model accounts for human interference on river flow, i.e. water abstraction for various purposes, e.g. irrigation, and flow regulation by <span class="hlt">large</span> dams and reservoirs. Our analysis will provide insight in the general ability of global hydrological models to reproduce river flood regimes and thus will promote the creation of a global map of river flood regimes to provide a spatially inclusive and comprehensive picture. Understanding present-day flood regimes can support both flood risk</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1193L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1193L"><span>Connecting the <span class="hlt">large</span>- and the small-<span class="hlt">scale</span> magnetic fields of solar-like stars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lehmann, L. T.; Jardine, M. M.; Mackay, D. H.; Vidotto, A. A.</p> <p>2018-05-01</p> <p>A key question in understanding the observed magnetic field topologies of cool stars is the link between the small- and the <span class="hlt">large-scale</span> magnetic field and the influence of the stellar parameters on the magnetic field topology. We examine various simulated stars to connect the small-<span class="hlt">scale</span> with the observable <span class="hlt">large-scale</span> field. The highly resolved 3D simulations we used couple a flux transport model with a non-potential coronal model using a magnetofrictional technique. The surface magnetic field of these simulations is decomposed into spherical harmonics which enables us to analyse the magnetic field topologies on a wide range of length <span class="hlt">scales</span> and to filter the <span class="hlt">large-scale</span> magnetic field for a direct comparison with the observations. We show that the <span class="hlt">large-scale</span> field of the self-consistent simulations fits the observed solar-like stars and is mainly set up by the global dipolar field and the <span class="hlt">large-scale</span> properties of the flux pattern, e.g. the averaged latitudinal position of the emerging small-<span class="hlt">scale</span> field and its global polarity pattern. The stellar parameters flux emergence rate, differential rotation and meridional flow affect the <span class="hlt">large-scale</span> magnetic field topology. An increased flux emergence rate increases the magnetic flux in all field components and an increased differential rotation increases the toroidal field fraction by decreasing the poloidal field. The meridional flow affects the distribution of the magnetic energy across the spherical harmonic modes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=scientific+AND+method&pg=2&id=EJ820206','ERIC'); return false;" href="https://eric.ed.gov/?q=scientific+AND+method&pg=2&id=EJ820206"><span>The <span class="hlt">Large-Scale</span> Structure of Scientific Method</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>Kosso, Peter</p> <p>2009-01-01</p> <p>The standard textbook description of the nature of science describes the proposal, testing, and acceptance of a theoretical idea almost entirely in isolation from other theories. The resulting model of science is a kind of piecemeal empiricism that misses the important network structure of scientific knowledge. Only the <span class="hlt">large-scale</span> description of…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://cfpub.epa.gov/si/si_public_record_report.cfm?dirEntryId=139303&keyword=ted&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=139303&keyword=ted&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>RESOLVING FINE <span class="hlt">SCALE</span> IN <span class="hlt">AIR</span> TOXICS MODELING AND THE IMPORTANCE OF ITS SUB-GRID VARIABILITY FOR EXPOSURE ESTIMATES</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 presentation explains the importance of the fine-<span class="hlt">scale</span> features for <span class="hlt">air</span> toxics exposure modeling. The paper presents a new approach to combine local-<span class="hlt">scale</span> and regional model results for the National <span class="hlt">Air</span> Toxic Assessment. The technique has been evaluated with a chemical tra...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li class="active"><span>25</span></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_25 --> <div class="footer-extlink text-muted" style="margin-bottom:1rem; text-align:center;">Some links on this page may take you to non-federal websites. 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