Sample records for trade wind region

  1. Differences between nonprecipitating tropical and trade wind marine shallow cumuli

    DOE PAGES

    Ghate, Virendra P.; Miller, Mark A.; Zhu, Ping

    2015-11-13

    In this study, marine nonprecipitating cumulus topped boundary layers (CTBLs) observed in a tropical and in a trade wind region are contrasted based on their cloud macrophysical, dynamical, and radiative structures. Data from the Atmospheric Radiation Measurement (ARM) observational site previously operating at Manus Island, Papua New Guinea, and data collected during the deployment of ARM Mobile Facility at the island of Graciosa, in the Azores, were used in this study. The tropical marine CTBLs were deeper, had higher surface fluxes and boundary layer radiative cooling, but lower wind speeds compared to their trade wind counterparts. The radiative velocity scalemore » was 50%-70% of the surface convective velocity scale at both locations, highlighting the prominent role played by radiation in maintaining turbulence in marine CTBLs. Despite greater thicknesses, the chord lengths of tropical cumuli were on average lower than those of trade wind cumuli, and as a result of lower cloud cover, the hourly averaged (cloudy and clear) liquid water paths of tropical cumuli were lower than the trade wind cumuli. At both locations ~70% of the cloudy profiles were updrafts, while the average amount of updrafts near cloud base stronger than 1 m s –1 was ~22% in tropical cumuli and ~12% in the trade wind cumuli. The mean in-cloud radar reflectivity within updrafts and mean updraft velocity was higher in tropical cumuli than the trade wind cumuli. Despite stronger vertical velocities and a higher number of strong updrafts, due to lower cloud fraction, the updraft mass flux was lower in the tropical cumuli compared to the trade wind cumuli. The observations suggest that the tropical and trade wind marine cumulus clouds differ significantly in their macrophysical and dynamical structures« less

  2. Differences between nonprecipitating tropical and trade wind marine shallow cumuli

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

    Ghate, Virendra P.; Miller, Mark A.; Zhu, Ping

    In this study, marine nonprecipitating cumulus topped boundary layers (CTBLs) observed in a tropical and in a trade wind region are contrasted based on their cloud macrophysical, dynamical, and radiative structures. Data from the Atmospheric Radiation Measurement (ARM) observational site previously operating at Manus Island, Papua New Guinea, and data collected during the deployment of ARM Mobile Facility at the island of Graciosa, in the Azores, were used in this study. The tropical marine CTBLs were deeper, had higher surface fluxes and boundary layer radiative cooling, but lower wind speeds compared to their trade wind counterparts. The radiative velocity scalemore » was 50%-70% of the surface convective velocity scale at both locations, highlighting the prominent role played by radiation in maintaining turbulence in marine CTBLs. Despite greater thicknesses, the chord lengths of tropical cumuli were on average lower than those of trade wind cumuli, and as a result of lower cloud cover, the hourly averaged (cloudy and clear) liquid water paths of tropical cumuli were lower than the trade wind cumuli. At both locations ~70% of the cloudy profiles were updrafts, while the average amount of updrafts near cloud base stronger than 1 m s –1 was ~22% in tropical cumuli and ~12% in the trade wind cumuli. The mean in-cloud radar reflectivity within updrafts and mean updraft velocity was higher in tropical cumuli than the trade wind cumuli. Despite stronger vertical velocities and a higher number of strong updrafts, due to lower cloud fraction, the updraft mass flux was lower in the tropical cumuli compared to the trade wind cumuli. The observations suggest that the tropical and trade wind marine cumulus clouds differ significantly in their macrophysical and dynamical structures« less

  3. Hemispherically asymmetric trade wind changes as signatures of past ITCZ shifts

    NASA Astrophysics Data System (ADS)

    McGee, David; Moreno-Chamarro, Eduardo; Green, Brian; Marshall, John; Galbraith, Eric; Bradtmiller, Louisa

    2018-01-01

    The atmospheric Hadley cells, which meet at the Intertropical Convergence Zone (ITCZ), play critical roles in transporting heat, driving ocean circulation and supplying precipitation to the most heavily populated regions of the globe. Paleo-reconstructions can provide concrete evidence of how these major features of the atmospheric circulation can change in response to climate perturbations. While most such reconstructions have focused on ITCZ-related rainfall, here we show that trade wind proxies can document dynamical aspects of meridional ITCZ shifts. Theoretical expectations based on angular momentum constraints and results from freshwater hosing simulations with two different climate models predict that ITCZ shifts due to anomalous cooling of one hemisphere would be accompanied by a strengthening of the Hadley cell and trade winds in the colder hemisphere, with an opposite response in the warmer hemisphere. This expectation of hemispherically asymmetric trade wind changes is confirmed by proxy data of coastal upwelling and windblown dust from the Atlantic basin during Heinrich stadials, showing trade wind strengthening in the Northern Hemisphere and weakening in the Southern Hemisphere subtropics in concert with southward ITCZ shifts. Data from other basins show broadly similar patterns, though improved constraints on past trade wind changes are needed outside the Atlantic Basin. The asymmetric trade wind changes identified here suggest that ITCZ shifts are also marked by intensification of the ocean's wind-driven subtropical cells in the cooler hemisphere and a weakening in the warmer hemisphere, which induces cross-equatorial oceanic heat transport into the colder hemisphere. This response would be expected to prevent extreme meridional ITCZ shifts in response to asymmetric heating or cooling. Understanding trade wind changes and their coupling to cross-equatorial ocean cells is key to better constraining ITCZ shifts and ocean and atmosphere dynamical

  4. Clouds at Barbados are representative of clouds across the trade wind regions in observations and climate models

    PubMed Central

    Nuijens, Louise

    2016-01-01

    Trade wind regions cover most of the tropical oceans, and the prevailing cloud type is shallow cumulus. These small clouds are parameterized by climate models, and changes in their radiative effects strongly and directly contribute to the spread in estimates of climate sensitivity. This study investigates the structure and variability of these clouds in observations and climate models. The study builds upon recent detailed model evaluations using observations from the island of Barbados. Using a dynamical regimes framework, satellite and reanalysis products are used to compare the Barbados region and the broader tropics. It is shown that clouds in the Barbados region are similar to those across the trade wind regions, implying that observational findings from the Barbados Cloud Observatory are relevant to clouds across the tropics. The same methods are applied to climate models to evaluate the simulated clouds. The models generally capture the cloud radiative effect, but underestimate cloud cover and show an array of cloud vertical structures. Some models show strong biases in the environment of the Barbados region in summer, weakening the connection between the regional biases and those across the tropics. Even bearing that limitation in mind, it is shown that covariations of cloud and environmental properties in the models are inconsistent with observations. The models tend to misrepresent sensitivity to moisture variations and inversion characteristics. These model errors are likely connected to cloud feedback in climate projections, and highlight the importance of the representation of shallow cumulus convection. PMID:27185925

  5. Clouds at Barbados are representative of clouds across the trade wind regions in observations and climate models.

    PubMed

    Medeiros, Brian; Nuijens, Louise

    2016-05-31

    Trade wind regions cover most of the tropical oceans, and the prevailing cloud type is shallow cumulus. These small clouds are parameterized by climate models, and changes in their radiative effects strongly and directly contribute to the spread in estimates of climate sensitivity. This study investigates the structure and variability of these clouds in observations and climate models. The study builds upon recent detailed model evaluations using observations from the island of Barbados. Using a dynamical regimes framework, satellite and reanalysis products are used to compare the Barbados region and the broader tropics. It is shown that clouds in the Barbados region are similar to those across the trade wind regions, implying that observational findings from the Barbados Cloud Observatory are relevant to clouds across the tropics. The same methods are applied to climate models to evaluate the simulated clouds. The models generally capture the cloud radiative effect, but underestimate cloud cover and show an array of cloud vertical structures. Some models show strong biases in the environment of the Barbados region in summer, weakening the connection between the regional biases and those across the tropics. Even bearing that limitation in mind, it is shown that covariations of cloud and environmental properties in the models are inconsistent with observations. The models tend to misrepresent sensitivity to moisture variations and inversion characteristics. These model errors are likely connected to cloud feedback in climate projections, and highlight the importance of the representation of shallow cumulus convection.

  6. Parameter Trade Studies For Coherent Lidar Wind Measurements of Wind from Space

    NASA Technical Reports Server (NTRS)

    Kavaya, Michael J.; Frehlich, Rod G.

    2007-01-01

    The design of an orbiting wind profiling lidar requires selection of dozens of lidar, measurement scenario, and mission geometry parameters; in addition to prediction of atmospheric parameters. Typical mission designs do not include a thorough trade optimization of all of these parameters. We report here the integration of a recently published parameterization of coherent lidar wind velocity measurement performance with an orbiting coherent wind lidar computer simulation; and the use of these combined tools to perform some preliminary parameter trades. We use the 2006 NASA Global Wind Observing Sounder mission design as the starting point for the trades.

  7. SLS Trade Study 0058: Day of Launch (DOL) Wind Biasing

    NASA Technical Reports Server (NTRS)

    Decker, Ryan K.; Duffin, Paul; Hill, Ashley; Beck, Roger; Dukeman, Greg

    2014-01-01

    SLS heritage hardware and legacy designs have shown load exceedances at several locations during Design Analysis Cycles (DAC): MPCV Z bending moments; ICPS Electro-Mechanical Actuator (EMA) loads; Core Stage loads just downstream of Booster forward interface. SLS Buffet Loads Mitigation Task Team (BLMTT) tasked to study issue. Identified low frequency buffet load responses are a function of the vehicle's total angle of attack (AlphaTotal). SLS DOL Wind Biasing Trade team to analyze DOL wind biasing methods to limit maximum AlphaTotal in the M0.8 - 2.0 altitude region for EM-1 and EM-2 missions through investigating: Trajectory design process; Wind wavelength filtering options; Launch availability; DOL process to achieve shorter processing/uplink timeline. Trade Team consisted of personnel supporting SLS, MPCV, GSDO programs.

  8. Why do modelled and observed surface wind stress climatologies differ in the trade wind regions?

    NASA Astrophysics Data System (ADS)

    Simpson, I.; Bacmeister, J. T.; Sandu, I.; Rodwell, M. J.

    2017-12-01

    Global climate models (GCMs) exhibit stronger easterly zonal surface wind stress and near surface winds in the Northern Hemisphere (NH) trade winds than observationally constrained reanalyses or other observational products. A comparison, between models and reanalyses, of the processes that contribute to the zonal mean, vertically integrated balance of momentum, reveals that this wind stress discrepancy cannot be explained by either the resolved dynamics or parameterized tendencies that are common to each. Rather, a substantial residual exists in the momentum balance of the reanalyses, pointing toward a role for the analysis increments. Indeed, they are found to systematically weaken the NH near surface easterlies in winter, thereby reducing the surface wind stress. Similar effects are found in the Southern Hemisphere and further analysis of the spatial structure and seasonality of these increments, demonstrates that they act to weaken the near surface flow over much of the low latitude oceans in both summer and winter. This suggests an erroneous /missing process in GCMs that constitutes a missing drag on the low level zonal flow over oceans. Either this indicates a mis-representation of the drag between the surface and the atmosphere, or a missing internal atmospheric process that amounts to an additional drag on the low level zonal flow. If the former is true, then observation based surface stress products, which rely on similar drag formulations to GCMs, may be underestimating the strength of the easterly surface wind stress.

  9. 76 FR 61342 - Foreign-Trade Zone 72 Temporary/Interim Manufacturing Authority Brevini Wind USA, Inc., (Wind...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-10-04

    ... DEPARTMENT OF COMMERCE Foreign-Trade Zones Board [Docket T-3-2011] Foreign-Trade Zone 72 Temporary/Interim Manufacturing Authority Brevini Wind USA, Inc., (Wind Turbine Gear Boxes); Notice of Approval On... manufacturing (T/IM) authority, on behalf of Brevini Wind USA, Inc., to manufacture wind turbine gear boxes...

  10. Wind speed variability over the Canary Islands, 1948-2014: focusing on trend differences at the land-ocean interface and below-above the trade-wind inversion layer

    NASA Astrophysics Data System (ADS)

    Azorin-Molina, Cesar; Menendez, Melisa; McVicar, Tim R.; Acevedo, Adrian; Vicente-Serrano, Sergio M.; Cuevas, Emilio; Minola, Lorenzo; Chen, Deliang

    2017-08-01

    This study simultaneously examines wind speed trends at the land-ocean interface, and below-above the trade-wind inversion layer in the Canary Islands and the surrounding Eastern North Atlantic Ocean: a key region for quantifying the variability of trade-winds and its response to large-scale atmospheric circulation changes. Two homogenized data sources are used: (1) observed wind speed from nine land-based stations (1981-2014), including one mountain weather station (Izaña) located above the trade-wind inversion layer; and (2) simulated wind speed from two atmospheric hindcasts over ocean (i.e., SeaWind I at 30 km for 1948-2014; and SeaWind II at 15 km for 1989-2014). The results revealed a widespread significant negative trend of trade-winds over ocean for 1948-2014, whereas no significant trends were detected for 1989-2014. For this recent period wind speed over land and ocean displayed the same multi-decadal variability and a distinct seasonal trend pattern with a strengthening (late spring and summer; significant in May and August) and weakening (winter-spring-autumn; significant in April and September) of trade-winds. Above the inversion layer at Izaña, we found a predominance of significant positive trends, indicating a decoupled variability and opposite wind speed trends when compared to those reported in boundary layer. The analysis of the Trade Wind Index (TWI), the North Atlantic Oscillation Index (NAOI) and the Eastern Atlantic Index (EAI) demonstrated significant correlations with the wind speed variability, revealing that the correlation patterns of the three indices showed a spatio-temporal complementarity in shaping wind speed trends across the Eastern North Atlantic.

  11. Wind speed variability over the Canary Islands, 1948-2014: focusing on trend differences at the land-ocean interface and below-above the trade-wind inversion layer

    NASA Astrophysics Data System (ADS)

    Azorin-Molina, Cesar; Menendez, Melisa; McVicar, Tim R.; Acevedo, Adrian; Vicente-Serrano, Sergio M.; Cuevas, Emilio; Minola, Lorenzo; Chen, Deliang

    2018-06-01

    This study simultaneously examines wind speed trends at the land-ocean interface, and below-above the trade-wind inversion layer in the Canary Islands and the surrounding Eastern North Atlantic Ocean: a key region for quantifying the variability of trade-winds and its response to large-scale atmospheric circulation changes. Two homogenized data sources are used: (1) observed wind speed from nine land-based stations (1981-2014), including one mountain weather station (Izaña) located above the trade-wind inversion layer; and (2) simulated wind speed from two atmospheric hindcasts over ocean (i.e., SeaWind I at 30 km for 1948-2014; and SeaWind II at 15 km for 1989-2014). The results revealed a widespread significant negative trend of trade-winds over ocean for 1948-2014, whereas no significant trends were detected for 1989-2014. For this recent period wind speed over land and ocean displayed the same multi-decadal variability and a distinct seasonal trend pattern with a strengthening (late spring and summer; significant in May and August) and weakening (winter-spring-autumn; significant in April and September) of trade-winds. Above the inversion layer at Izaña, we found a predominance of significant positive trends, indicating a decoupled variability and opposite wind speed trends when compared to those reported in boundary layer. The analysis of the Trade Wind Index (TWI), the North Atlantic Oscillation Index (NAOI) and the Eastern Atlantic Index (EAI) demonstrated significant correlations with the wind speed variability, revealing that the correlation patterns of the three indices showed a spatio-temporal complementarity in shaping wind speed trends across the Eastern North Atlantic.

  12. Credit Trading and Wind Power: Issues and Opportunities

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

    Kevin Rackstraw, John Palmisano

    2001-01-15

    OAK-B135 This paper focuses on credits that are derived from wind energy technology, but the same concepts apply to other renewable energy technologies as well. Credit trading can be applied to a wide variety of policies, programs and private market activities and represents a means of tapping into revenue streams that heretofore have largely excluded wind and other renewables. In addition, credit trading can help to ''create'' new revenue streams for wind and other renewables by helping to grow new markets.

  13. 78 FR 70276 - Trade Mission to Colombia, Peru, Chile, Panama, and Ecuador in Conjunction With Trade Winds-The...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-11-25

    ..., Panama, and Ecuador in Conjunction With Trade Winds--The Americas, May 15-23, 2014 AGENCY: International..., Chile, Panama and Ecuador that will include the Trade Winds--The Americas business forum in Bogot[aacute... Ecuador. Each trade mission stop will include one-on-one business appointments with pre-screened potential...

  14. Insitu aircraft verification of the quality of satellite cloud winds over oceanic regions

    NASA Technical Reports Server (NTRS)

    Hasler, A. F.; Skillman, W. C.

    1979-01-01

    A five year aircraft experiment to verify the quality of satellite cloud winds over oceans using in situ aircraft inertial navigation system wind measurements is presented. The final results show that satellite measured cumulus cloud motions are very good estimators of the cloud base wind for trade wind and subtropical high regions. The average magnitude of the vector differences between the cloud motion and the cloud base wind is given. For cumulus clouds near frontal regions, the cloud motion agreed best with the mean cloud layer wind. For a very limited sample, cirrus cloud motions also most closely followed the mean wind in the cloud layer.

  15. 77 FR 55455 - Approval for Manufacturing Authority Foreign-Trade Zone 72, Brevini Wind USA, Inc., (Wind Turbine...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-09-10

    ... Authority Foreign-Trade Zone 72, Brevini Wind USA, Inc., (Wind Turbine Gear Boxes), Yorktown, IN Pursuant to... Wind USA, Inc., within FTZ 72 in Yorktown, Indiana (FTZ Docket 54-2011, filed 8-11-2011); Whereas... procedures within FTZ 72 on behalf of Brevini Wind USA, Inc., as described in the application and Federal...

  16. Towards an Optimal Noise Versus Resolution Trade-Off in Wind Scatterometry

    NASA Technical Reports Server (NTRS)

    Williams, Brent A.

    2011-01-01

    A scatterometer is a radar that measures the normalized radar cross section sigma(sup 0) of the Earth's surface. Over the ocean this signal is related to the wind via the geophysical model function (GMF). The objective of wind scatterometry is to estimate the wind vector field from sigma(sup 0) measurements; however, there are many subtleties that complicate this problem-making it difficult to obtain a unique wind field estimate. Conventionally, wind estimation is split into two stages: a wind retrieval stage in which several ambiguous solutions are obtained, and an ambiguity removal stage in which ambiguities are chosen to produce an appropriate wind vector field estimate. The most common approach to wind field estimation is to grid the scatterometer swath into wind vector cells and estimate wind vector ambiguities independently for each cell. Then, field wise structure is imposed on the solution by an ambiguity selection routine. Although this approach is simple and practical, it neglects field wise structure in the retrieval step and does not account for the spatial correlation imposed by the sampling. This makes it difficult to develop a theoretically appropriate noise versus resolution trade-off using pointwise retrieval. Fieldwise structure may be imposed in the retrieval step using a model-based approach. However, this approach is generally only practical if a low order wind field model is applied, which may discard more information than is desired. Furthermore, model-based approaches do not account for the structure imposed by the sampling. A more general fieldwise approach is to estimate all the wind vectors for all the WVCs simultaneously from all the measurements. This approach can account for structure of the wind field as well as structure imposed by the sampling in the wind retrieval step. Williams and Long in 2010 developed a fieldwise retrieval method based on maximum a posteriori estimation (MAP). This MAP approach can be extended to perform a

  17. Twin Cyclones Result From Shift in the Trade Winds

    NASA Technical Reports Server (NTRS)

    2002-01-01

    QuikSCAT, a NASA satellite instrument that measures winds, observed a strong typhoon threatening the Philippines on March 4, 2002, (top) unusual in the winter season, and a similar tropical cyclone passing along the Australian coast towards Nuomea. These unusual phenomena are results of the westerly winds (blowing from Indonesia towards the American coast) along the equator which started back in February 25, (lower) as QuikSCAT revealed. Color in these images relates to wind speed, arrows indicate direction. The reversal of the usual Trade Winds (which blow from the American coast towards Asia) generally triggers Kelvin waves (warm surface water that moves along the equator from Indonesia to the coast of Peru) and twin cyclones, which are early indicators of El Nino. The equatorial westerly winds generate a counter-clockwise vortex in the Northern Hemisphere and a clockwise vortex in the Southern Hemisphere. The Trade Winds push warm water from east to west across the Pacific, reaching the American coast in one to two months. The increase in frequency and strength of the Kelvin Waves may lead to El Nino. Strong westerly winds and twin cyclones were also observed by QuikSCAT during last Christmas season (2001) and the Kelvin wave triggered at that time reached South America in Early March 2002. Images courtesy Liu, Xie, and Tang, QuikSCAT Science Team

  18. Towards an Optimal Noise Versus Resolution Trade-Off in Wind Scatterometry

    NASA Technical Reports Server (NTRS)

    Williams, Brent A.

    2011-01-01

    This paper approaches the noise versus resolution trade-off in wind scatterometry from a field-wise retrieval perspective. Theoretical considerations are discussed and practical implementation using a MAP estimator is applied to the Sea-Winds scatterometer. The approach is compared to conventional approaches as well as numerical weather predictions. The new approach incorporates knowledge of the wind spectrum to reduce the impact of components of the wind signal that are expected to be noisy.

  19. Observations of the trade wind wakes of Kauai and Oahu

    NASA Astrophysics Data System (ADS)

    Yang, Yang; Ma, Jian; Xie, Shang-Ping

    2008-02-01

    The Hawaiian islands of Kauai and Oahu stand in the path of the east-northeasterly trade winds, creating wakes in the lee. For the first time, the structure of the wakes and their diurnal cycle were observed on a cruise during 18-20 December 2006. The dynamic wakes, characterized by reduced trades, extend about 1 km in height with strong wind shear at the top. Thermal forcing of these small islands also affects the wake circulations. Sea breezes develop in the afternoon turning the winds into westerly near the shore in the wakes. At night, land breezes advect cool air from the islands, creating a shallow cool layer between the sea surface and a capping inversion. The warming in the wake in the afternoon extends much deeper (1.4 km) than the cool layer (0.5 km) at night. The effect of diurnal changes on cloud formation in the wakes is discussed, and the sharp variations in wind velocity lee of the islands may affect ocean currents, waves and mixing.

  20. Hawaii Regional Sediment Management Needs Assessment

    DTIC Science & Technology

    2014-07-01

    and trade wind waves from the northeast. The East region is typically impacted by trade wind waves while the South region is oriented in the direction...North Pacific swell in winter and northeast trade wind waves throughout the year. The beaches tend to be steep and are composed of coarse-grained...coast is characterized by embayments and fringing reef systems. The shore is exposed to northeast trade winds . Streams and rivers flow into the

  1. Mechanisms and Model Diversity of Trade-Wind Shallow Cumulus Cloud Feedbacks: A Review.

    PubMed

    Vial, Jessica; Bony, Sandrine; Stevens, Bjorn; Vogel, Raphaela

    2017-01-01

    Shallow cumulus clouds in the trade-wind regions are at the heart of the long standing uncertainty in climate sensitivity estimates. In current climate models, cloud feedbacks are strongly influenced by cloud-base cloud amount in the trades. Therefore, understanding the key factors controlling cloudiness near cloud-base in shallow convective regimes has emerged as an important topic of investigation. We review physical understanding of these key controlling factors and discuss the value of the different approaches that have been developed so far, based on global and high-resolution model experimentations and process-oriented analyses across a range of models and for observations. The trade-wind cloud feedbacks appear to depend on two important aspects: (1) how cloudiness near cloud-base is controlled by the local interplay between turbulent, convective and radiative processes; (2) how these processes interact with their surrounding environment and are influenced by mesoscale organization. Our synthesis of studies that have explored these aspects suggests that the large diversity of model responses is related to fundamental differences in how the processes controlling trade cumulus operate in models, notably, whether they are parameterized or resolved. In models with parameterized convection, cloudiness near cloud-base is very sensitive to the vigor of convective mixing in response to changes in environmental conditions. This is in contrast with results from high-resolution models, which suggest that cloudiness near cloud-base is nearly invariant with warming and independent of large-scale environmental changes. Uncertainties are difficult to narrow using current observations, as the trade cumulus variability and its relation to large-scale environmental factors strongly depend on the time and/or spatial scales at which the mechanisms are evaluated. New opportunities for testing physical understanding of the factors controlling shallow cumulus cloud responses using

  2. Mechanisms and Model Diversity of Trade-Wind Shallow Cumulus Cloud Feedbacks: A Review

    NASA Astrophysics Data System (ADS)

    Vial, Jessica; Bony, Sandrine; Stevens, Bjorn; Vogel, Raphaela

    2017-11-01

    Shallow cumulus clouds in the trade-wind regions are at the heart of the long standing uncertainty in climate sensitivity estimates. In current climate models, cloud feedbacks are strongly influenced by cloud-base cloud amount in the trades. Therefore, understanding the key factors controlling cloudiness near cloud-base in shallow convective regimes has emerged as an important topic of investigation. We review physical understanding of these key controlling factors and discuss the value of the different approaches that have been developed so far, based on global and high-resolution model experimentations and process-oriented analyses across a range of models and for observations. The trade-wind cloud feedbacks appear to depend on two important aspects: (1) how cloudiness near cloud-base is controlled by the local interplay between turbulent, convective and radiative processes; (2) how these processes interact with their surrounding environment and are influenced by mesoscale organization. Our synthesis of studies that have explored these aspects suggests that the large diversity of model responses is related to fundamental differences in how the processes controlling trade cumulus operate in models, notably, whether they are parameterized or resolved. In models with parameterized convection, cloudiness near cloud-base is very sensitive to the vigor of convective mixing in response to changes in environmental conditions. This is in contrast with results from high-resolution models, which suggest that cloudiness near cloud-base is nearly invariant with warming and independent of large-scale environmental changes. Uncertainties are difficult to narrow using current observations, as the trade cumulus variability and its relation to large-scale environmental factors strongly depend on the time and/or spatial scales at which the mechanisms are evaluated. New opportunities for testing physical understanding of the factors controlling shallow cumulus cloud responses using

  3. Mechanisms and Model Diversity of Trade-Wind Shallow Cumulus Cloud Feedbacks: A Review

    NASA Astrophysics Data System (ADS)

    Vial, Jessica; Bony, Sandrine; Stevens, Bjorn; Vogel, Raphaela

    Shallow cumulus clouds in the trade-wind regions are at the heart of the long standing uncertainty in climate sensitivity estimates. In current climate models, cloud feedbacks are strongly influenced by cloud-base cloud amount in the trades. Therefore, understanding the key factors controlling cloudiness near cloud-base in shallow convective regimes has emerged as an important topic of investigation. We review physical understanding of these key controlling factors and discuss the value of the different approaches that have been developed so far, based on global and high-resolution model experimentations and process-oriented analyses across a range of models and for observations. The trade-wind cloud feedbacks appear to depend on two important aspects: (1) how cloudiness near cloud-base is controlled by the local interplay between turbulent, convective and radiative processes; (2) how these processes interact with their surrounding environment and are influenced by mesoscale organization. Our synthesis of studies that have explored these aspects suggests that the large diversity of model responses is related to fundamental differences in how the processes controlling trade cumulus operate in models, notably, whether they are parameterized or resolved. In models with parameterized convection, cloudiness near cloud-base is very sensitive to the vigor of convective mixing in response to changes in environmental conditions. This is in contrast with results from high-resolution models, which suggest that cloudiness near cloud-base is nearly invariant with warming and independent of large-scale environmental changes. Uncertainties are difficult to narrow using current observations, as the trade cumulus variability and its relation to large-scale environmental factors strongly depend on the time and/or spatial scales at which the mechanisms are evaluated. New opportunities for testing physical understanding of the factors controlling shallow cumulus cloud responses using

  4. Multilateral, regional and bilateral energy trade governance

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

    Leal-Arcas, Rafael; Grasso, Costantino; Rios, Juan Alemany

    The current international energy trade governance system is fragmented and multi-layered. Streamlining it for greater legal cohesiveness and international political and economic cooperation would promote global energy security. The current article explores three levels of energy trade governance: multilateral, regional and bilateral. Most energy-rich countries are part of the multilateral trading system, which is institutionalized by the World Trade Organization (WTO). The article analyzes the multilateral energy trade governance system by focusing on the WTO and energy transportation issues. Regionally, the article focuses on five major regional agreements and their energy-related aspects and examines the various causes that explain themore » proliferation of regional trade agreements, their compatibility with WTO law, and then provides several examples of regional energy trade governance throughout the world. When it comes to bilateral energy trade governance, this article only addresses the European Union’s (EU) bilateral energy trade relations. The article explores ways in which gaps could be filled and overlaps eliminated whilst remaining true to the high-level normative framework, concentrating on those measures that would enhance EU energy security.« less

  5. Model under-representation of decadal Pacific trade wind trends and its link to tropical Atlantic bias

    NASA Astrophysics Data System (ADS)

    Kajtar, Jules B.; Santoso, Agus; McGregor, Shayne; England, Matthew H.; Baillie, Zak

    2018-02-01

    The strengthening of the Pacific trade winds in recent decades has been unmatched in the observational record stretching back to the early twentieth century. This wind strengthening has been connected with numerous climate-related phenomena, including accelerated sea-level rise in the western Pacific, alterations to Indo-Pacific ocean currents, increased ocean heat uptake, and a slow-down in the rate of global-mean surface warming. Here we show that models in the Coupled Model Intercomparison Project phase 5 underestimate the observed range of decadal trends in the Pacific trade winds, despite capturing the range in decadal sea surface temperature (SST) variability. Analysis of observational data suggests that tropical Atlantic SST contributes considerably to the Pacific trade wind trends, whereas the Atlantic feedback in coupled models is muted. Atmosphere-only simulations forced by observed SST are capable of recovering the time-variation and the magnitude of the trade wind trends. Hence, we explore whether it is the biases in the mean or in the anomalous SST patterns that are responsible for the under-representation in fully coupled models. Over interannual time-scales, we find that model biases in the patterns of Atlantic SST anomalies are the strongest source of error in the precipitation and atmospheric circulation response. In contrast, on decadal time-scales, the magnitude of the model biases in Atlantic mean SST are directly linked with the trade wind variability response.

  6. 77 FR 34935 - Foreign-Trade Zone 161; Temporary/Interim Manufacturing Authority; Siemens Energy, Inc., (Wind...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2012-06-12

    ... DEPARTMENT OF COMMERCE Foreign-Trade Zones Board [Docket T-4-2012] Foreign-Trade Zone 161; Temporary/Interim Manufacturing Authority; Siemens Energy, Inc., (Wind Turbine Nacelles and Hubs); Notice of Approval On April 2, 2012, the Executive Secretary of the Foreign-Trade Zones (FTZ) Board filed an application submitted by the Board of County...

  7. Characteristics and Trade-Offs of Doppler Lidar Global Wind Profiling

    NASA Technical Reports Server (NTRS)

    Kavaya, Michael J.; Emmitt, G David

    2004-01-01

    Accurate, global profiling of wind velocity is highly desired by NASA, NOAA, the DOD/DOC/NASA Integrated Program Office (IPO)/NPOESS, DOD, and others for many applications such as validation and improvement of climate models, and improved weather prediction. The most promising technology to deliver this measurement from space is Doppler Wind Lidar (DWL). The NASA/NOAA Global Tropospheric Wind Sounder (GTWS) program is currently in the process of generating the science requirements for a space-based sensor. In order to optimize the process of defining science requirements, it is important for the scientific and user community to understand the nature of the wind measurements that DWL can make. These measurements are very different from those made by passive imaging sensors or by active radar sensors. The purpose of this paper is to convey the sampling characteristics and data product trade-offs of an orbiting DWL.

  8. Constraining 20th Century Pacific Trade-Wind Variability Using Coral Mn/Ca

    NASA Astrophysics Data System (ADS)

    Sayani, H. R.; Thompson, D. M.; Carilli, J.; Ireland, T. J.; Cobb, K. M.; Atwood, A. R.; Grothe, P. R.; Miller, S. J.; Hitt, N. T.; O'Connor, G.

    2017-12-01

    Global mean surface temperatures during the 20th century are characterized by multidecadal periods of either accelerated or reduced rates of warming that cannot be explained by external forcings alone. Both observations and modeling studies suggest that the reduced rate of global surface warming during the early-2000s can be largely explained by decadal climate variability in the tropical Pacific, specifically changes in trade-wind strength [e.g. Meehl et al., 2016]. However, the relationship between Pacific trade-wind strength and global surface warming is poorly constrained due to the lack of instrumental wind observations prior to the 1970s. Surface corals are now routinely used to generate records of past sea-surface temperature (SST) change, and have dramatically improved our understanding of oceanic variability in the tropical Pacific. Yet, there are few direct measurements of the atmospheric response to this SST variability. Skeletal Mn/Ca ratios in corals from Tarawa Atoll (1.3˚N, 173˚E) have been shown to track El Niño-related westerly wind events on interannual timescales [Shen et al., 1992], and the strength of Pacific trade winds on decadal timescales [Thompson et al., 2015]. Here, we investigate the utility of this novel wind proxy at Kiritimati Atoll (Christmas Island; 2˚N, 157.5˚W), a site that is hydrographically similar to Tarawa. We use a series of seawater samples collected across the 2015/16 El Niño to characterize and quantify the relationship between westerly wind events and seawater Mn variability around Kiritimati. Anchored by this modern-day calibration, we present a new reconstruction of westerly winds across the late-20thcentury from Kiritimati Atoll. We also assess the reproducibility of coral Mn/Ca across cores collected at varying distances from the lagoon, which represents the primary source of seawater Mn to the reef at our site. Lastly, we discuss the strengths and limitations of this novel proxy, as well as the potential for

  9. The role of external forcing and Pacific trade winds in recent changes of the global climate system

    NASA Astrophysics Data System (ADS)

    Friedman, Andrew; Gastineau, Guillaume; Khodri, Myriam

    2017-04-01

    The Pacific trade winds experienced an unprecedented strengthening since the mid 1990s. Several studies have proposed that the increased Pacific trade winds were associated with the reduced rate of global mean surface temperature warming in the first decade of the 21st century, as well as far-reaching atmospheric teleconnections. We designed a set of ensemble partial coupling experiments using the IPSL-CM5A-LR coupled model that allow us to cleanly distinguish the influence of Pacific trade wind variability from that of external forcing over the past few decades. In this study, we quantify the respective impacts of these processes on surface temperature, ocean heat content, and atmospheric teleconnections. We designed two ensembles of coupled simulations using partial coupling with the IPSL-CM5A-LR model to separate the Pacific internal variability and that of external radiative forcing. We prescribe surface wind stress in the tropical Pacific (20°S to 20°N) from 1979-2014 in two ensembles of 30 members each: (1) Prescribed climatological model wind stress, which allows us to estimate the influence of external radiative forcing in the absence of variability within the Pacific Ocean. (2) Wind stress anomalies from ERA-Interim reanalysis added to the model wind stress climatology, which accounts for the effects of both external radiative forcing and the wind stress variability. We find that the observed wind stress anomalies account for the pattern of eastern tropical Pacific cooling when compared to the climatology experiment, so that it resembles the observed trends from 1992-2011. The tropical Pacific shows dominant heat uptake in the western Pacific above the 20°C isotherm, which contributed to slow the warming of tropical SST during the 2000s. The trade wind increase is associated with a strengthening of the Pacific Walker circulation, and zonal shifts in tropical rainfall. Despite tropical SST biases which affect the response of tropical rainfall and the

  10. 78 FR 53004 - Requested Administrative Waiver of the Coastwise Trade Laws: Vessel SECOND WIND; Invitation for...

    Federal Register 2010, 2011, 2012, 2013, 2014

    2013-08-27

    ... DEPARTMENT OF TRANSPORTATION Maritime Administration [Docket No. MARAD 2013 0093] Requested Administrative Waiver of the Coastwise Trade Laws: Vessel SECOND WIND; Invitation for Public Comments AGENCY... SECOND WIND is: Intended Commercial Use of Vessel: ``Breakfast, lunch, and dinner cruises featuring...

  11. Disentangling regional trade agreements, trade flows and tobacco affordability in sub-Saharan Africa.

    PubMed

    Appau, Adriana; Drope, Jeffrey; Labonté, Ronald; Stoklosa, Michal; Lencucha, Raphael

    2017-11-14

    In principle, trade and investment agreements are meant to boost economic growth. However, the removal of trade barriers and the provision of investment incentives to attract foreign direct investments may facilitate increased trade in and/or more efficient production of commodities considered harmful to health such as tobacco. We analyze existing evidence on trade and investment liberalization and its relationship to tobacco trade in Sub-Saharan African countries. We compare tobacco trading patterns to foreign direct investments made by tobacco companies. We estimate and compare changes in the Konjunkturforschungsstelle (KOF) Economic Globalization measure, relative price measure and cigarette prices. Preferential regional trade agreements appear to have encouraged the consolidation of cigarette production, which has shaped trading patterns of tobacco leaf. Since 2002, British American Tobacco has invested in tobacco manufacturing facilities in Nigeria, Kenya and South Africa strategically located to serve different regions in Africa. Following this, British America Tobacco closed factories in Ghana, Rwanda, Uganda, Mauritius and Angola. At the same time, Malawi and Tanzania exported a large percentage of tobacco leaf to European countries. After 2010, there was an increase in tobacco exports from Malawi and Zambia to China, which may be a result of preferential trade agreements the EU and China have with these countries. Economic liberalization has been accompanied by greater cigarette affordability for the countries included in our analysis. However, only excise taxes and income have an effect on cigarette prices within the region. These results suggest that the changing economic structures of international trade and investment are likely heightening the efficiency and effectiveness of the tobacco industry. As tobacco control advocates consider supply-side tobacco control interventions, they must consider carefully the effects of these economic agreements and

  12. WIND-TUNNEL SIMULATIONS TO ASSESS DISPERSION AROUND THE WORLD TRADE CENTER SITE

    EPA Science Inventory

    A wind-tunnel study was conducted of dispersion from the site of the destroyed World Trade Center (WTC) in New York City. A scale model of lower Manhattan, including a scaled representation of the rubble pile, was constructed. The first phases of the study involved smoke visua...

  13. Effects of trade openness and market scale on different regions

    NASA Astrophysics Data System (ADS)

    Tian, Renqu; Yang, Zisheng

    2017-04-01

    This paper revisits the relationship between growth, trade openness and market scale. Empirical studies have provided that area develops lopsided problem in China is increasingly serious, while large trade openness and market scale bring about more economic growth. We use a number of data set from province-level’s gross domestic product and socio-economic, as well as statistical methods panel ordinary least squares and instrumental variables estimation techniques to explore the effects of trade openness and regional market scale on the three major economic regions. The results indicate: Firstly, the impact of market scale and trade openness on economic growth is found to be positive. Secondly, the overall regional disparity is owing to the trade openness, market scale and macroeconomic policies. Thirdly, midland and western region should take advantage of regional geographical location and resource to expand exports and narrow the regional difference.

  14. The environment of the wind-wind collision region of η Carinae

    NASA Astrophysics Data System (ADS)

    Panagiotou, C.; Walter, R.

    2018-02-01

    Context. η Carinae is a colliding wind binary hosting two of the most massive stars and featuring the strongest wind collision mechanical luminosity. The wind collision region of this system is detected in X-rays and γ-rays and offers a unique laboratory for the study of particle acceleration and wind magneto-hydrodynamics. Aim. Our main goal is to use X-ray observations of η Carinae around periastron to constrain the wind collision zone geometry and understand the reasons for its variability. Methods: We analysed 10 Nuclear Spectroscopic Telescope Array (NuSTAR) observations, which were obtained around the 2014 periastron. The NuSTAR array monitored the source from 3 to 30 keV, which allowed us to grasp the continuum and absorption parameters with very good accuracy. We were able to identify several physical components and probe their variability. Results: The X-ray flux varied in a similar way as observed during previous periastrons and largely as expected if generated in the wind collision region. The flux detected within 10 days of periastron is lower than expected, suggesting a partial disruption of the central region of the wind collision zone. The Fe Kα line is likely broadened by the electrons heated along the complex shock fronts. The variability of its equivalent width indicates that the fluorescence region has a complex geometry and that the source obscuration varies quickly with the line of sight.

  15. SeaWinds - Oceans, Land, Polar Regions

    NASA Technical Reports Server (NTRS)

    1999-01-01

    The SeaWinds scatterometer on the QuikScat satellite makes global radar measurements -- day and night, in clear sky and through clouds. The radar data over the oceans provide scientists and weather forecasters with information on surface wind speed and direction. Scientists also use the radar measurements directly to learn about changes in vegetation and ice extent over land and polar regions.

    This false-color image is based entirely on SeaWinds measurements obtained over oceans, land, and polar regions. Over the ocean, colors indicate wind speed with orange as the fastest wind speeds and blue as the slowest. White streamlines indicate the wind direction. The ocean winds in this image were measured by SeaWinds on September 20, 1999. The large storm in the Atlantic off the coast of Florida is Hurricane Gert. Tropical storm Harvey is evident as a high wind region in the Gulf of Mexico, while farther west in the Pacific is tropical storm Hilary. An extensive storm is also present in the South Atlantic Ocean near Antarctica.

    The land image was made from four days of SeaWinds data with the aid of a resolution enhancement algorithm developed by Dr. David Long at Brigham Young University. The lightest green areas correspond to the highest radar backscatter. Note the bright Amazon and Congo rainforests compared to the dark Sahara desert. The Amazon River is visible as a dark line running horizontally though the bright South American rain forest. Cities appear as bright spots on the images, especially in the U.S. and Europe.

    The image of Greenland and the north polar ice cap was generated from data acquired by SeaWinds on a single day. In the polar region portion of the image, white corresponds to the largest radar return, while purple is the lowest. The variations in color in Greenland and the polar ice cap reveal information about the ice and snow conditions present.

    NASA's Earth Science Enterprise is a long-term research and technology program designed to

  16. Miocene shift of European atmospheric circulation from trade wind to westerlies

    PubMed Central

    Quan, Cheng; Liu, Yu-Sheng (Christopher); Tang, Hui; Utescher, Torsten

    2014-01-01

    The modern European climatic regime is peculiar, due to its unitary winter but diverse summer climates and a pronounced Mediterranean climate in the south. However, little is known on its evolution in the deep time. Here we reconstruct the European summer climate conditions in the Tortonian (11.62–7.246 Ma) using plant fossil assemblages from 75 well-dated sites across Europe. Our results clearly show that the Tortonian Europe mainly had humid to subhumid summers and no arid climate has been conclusively detected, indicating that the summer-dry Mediterranean-type climate has not yet been established along most of the Mediterranean coast at least by the Tortonian. More importantly, the reconstructed distribution pattern of summer precipitation reveals that the Tortonian European must have largely been controlled by westerlies, resulting in higher precipitation in the west and the lower in the east. The Tortonian westerly wind field appears to differ principally from the trade wind pattern of the preceding Serravallian (13.82–11.62 Ma), recently deduced from herpetofaunal fossils. Such a shift in atmospheric circulation, if ever occurred, might result from the development of ice caps and glaciers in the polar region during the Late Miocene global cooling, the then reorganization of oceanic circulation, and/or the Himalayan-Tibetan uplift. PMID:25012454

  17. Observed and modeled patterns of covariability between low-level cloudiness and the structure of the trade-wind layer

    DOE PAGES

    Nuijens, Louise; Medeiros, Brian; Sandu, Irina; ...

    2015-11-06

    We present patterns of covariability between low-level cloudiness and the trade-wind boundary layer structure using long-term measurements at a site representative of dynamical regimes with moderate subsidence or weak ascent. We compare these with ECMWF’s Integrated Forecast System and 10 CMIP5 models. By using single-time step output at a single location, we find that models can produce a fairly realistic trade-wind layer structure in long-term means, but with unrealistic variability at shorter-time scales. The unrealistic variability in modeled cloudiness near the lifting condensation level (LCL) is due to stronger than observed relationships with mixed-layer relative humidity (RH) and temperature stratificationmore » at the mixed-layer top. Those relationships are weak in observations, or even of opposite sign, which can be explained by a negative feedback of convection on cloudiness. Cloudiness near cumulus tops at the tradewind inversion instead varies more pronouncedly in observations on monthly time scales, whereby larger cloudiness relates to larger surface winds and stronger trade-wind inversions. However, these parameters appear to be a prerequisite, rather than strong controlling factors on cloudiness, because they do not explain submonthly variations in cloudiness. Models underestimate the strength of these relationships and diverge in particular in their responses to large-scale vertical motion. No model stands out by reproducing the observed behavior in all respects. As a result, these findings suggest that climate models do not realistically represent the physical processes that underlie the coupling between trade-wind clouds and their environments in present-day climate, which is relevant for how we interpret modeled cloud feedbacks.« less

  18. Observed and modeled patterns of covariability between low-level cloudiness and the structure of the trade-wind layer

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

    Nuijens, Louise; Medeiros, Brian; Sandu, Irina

    We present patterns of covariability between low-level cloudiness and the trade-wind boundary layer structure using long-term measurements at a site representative of dynamical regimes with moderate subsidence or weak ascent. We compare these with ECMWF’s Integrated Forecast System and 10 CMIP5 models. By using single-time step output at a single location, we find that models can produce a fairly realistic trade-wind layer structure in long-term means, but with unrealistic variability at shorter-time scales. The unrealistic variability in modeled cloudiness near the lifting condensation level (LCL) is due to stronger than observed relationships with mixed-layer relative humidity (RH) and temperature stratificationmore » at the mixed-layer top. Those relationships are weak in observations, or even of opposite sign, which can be explained by a negative feedback of convection on cloudiness. Cloudiness near cumulus tops at the tradewind inversion instead varies more pronouncedly in observations on monthly time scales, whereby larger cloudiness relates to larger surface winds and stronger trade-wind inversions. However, these parameters appear to be a prerequisite, rather than strong controlling factors on cloudiness, because they do not explain submonthly variations in cloudiness. Models underestimate the strength of these relationships and diverge in particular in their responses to large-scale vertical motion. No model stands out by reproducing the observed behavior in all respects. As a result, these findings suggest that climate models do not realistically represent the physical processes that underlie the coupling between trade-wind clouds and their environments in present-day climate, which is relevant for how we interpret modeled cloud feedbacks.« less

  19. Synergizing High-Resolution EOS Terra Satellite Data and S-POLKa Radar Reflectivity to Assess Trade Wind Cumuli Precipitation

    NASA Astrophysics Data System (ADS)

    Snodgrass, E. R.; di Girolamo, L.; Rauber, R.; Zhao, G.

    2005-12-01

    During the RICO field campaign, the EOS Terra Spacecraft and NCAR's S-POLKa radar collected coincident high-resolution visible and near-IR satellite data and dual-polarized S-band and Ka-band radar reflectivity data to understand trade wind cumuli cloud distribution and precipitation. In this paper, the comparison of the trade wind cloud field's satellite-derived cloud properties and radar-derived precipitation characteristics are presented. Specifically, these results focus on the relationship between radar reflectivity and derived rain rate to the satellite visible radiance, cloud fraction, height and thickness. Also results concerning the relationship between cloud area estimated by satellite and cloud boundary estimated by radar Bragg and Rayleigh scattering will be presented. The resolution effects between visible satellite data from the ASTER instrument at 15m ground-resolution and the S-POLKa radar data will be reviewed. The potential applications of these results to the estimation of trade wind cumuli's role in returning water to the ocean through precipitation, and to cloud and climate model parameterization will be discussed.

  20. Wind-induced upwelling in the Kerguelen Plateau region

    NASA Astrophysics Data System (ADS)

    Gille, S. T.; Carranza, M. M.; Cambra, R.

    2014-11-01

    In contrast to most of the Southern Ocean, the Kerguelen Plateau supports an unusually strong spring chlorophyll (Chl a) bloom, likely because the euphotic zone in the region is supplied with higher iron concentrations. This study uses satellite wind, sea surface temperature (SST), and ocean color data to explore the impact of wind-driven processes on upwelling of cold (presumably iron-rich) water to the euphotic zone. Results show that, in the Kerguelen region, cold SSTs correlate with high wind speeds, implying that wind-mixing leads to enhanced vertical mixing. Cold SSTs also correlate with negative wind-stress curl, implying that Ekman pumping can further enhance upwelling. In the moderate to high eddy kinetic energy (EKE) regions surrounding Kerguelen, we find evidence of coupling between winds and SST gradients associated with mesoscale eddies, which can locally modulate the wind-stress curl. This coupling introduces persistent wind-stress curl patterns and Ekman pumping around these long-lived eddies, which may modulate the evolution of Chl a in the downstream plume far offshore. Close to the plateau, this eddy coupling breaks down. Kerguelen has a significant wind shadow on its downwind side, which changes position depending on the prevailing wind and which generates a wind-stress curl dipole that shifts location depending on wind direction. This leads to locally enhanced Ekman pumping for a few hundred kilometers downstream from the Kerguelen Plateau; Chl a values tend to be more elevated in places where wind-stress curl induces Ekman upwelling than in locations of downwelling, although the estimated upwelling rates are too small for this relationship to derive from direct effects on upward iron supply, and thus other processes, which remain to be determined, must also be involved in the establishment of these correlations. During the October and November (2011) KErguelen Ocean and Plateau compared Study (KEOPS-2) field program, wind conditions were fairly

  1. Networks of global bird invasion altered by regional trade ban

    PubMed Central

    Reino, Luís; Figueira, Rui; Beja, Pedro; Araújo, Miguel B.; Capinha, César; Strubbe, Diederik

    2017-01-01

    Wildlife trade is a major pathway for introduction of invasive species worldwide. However, how exactly wildlife trade influences invasion risk, beyond the transportation of individuals to novel areas, remains unknown. We analyze the global trade network of wild-caught birds from 1995 to 2011 as reported by CITES (Convention on International Trade in Endangered Species of Wild Fauna and Flora). We found that before the European Union ban on imports of wild-caught birds, declared in 2005, invasion risk was closely associated with numbers of imported birds, diversity of import sources, and degree of network centrality of importer countries. After the ban, fluxes of global bird trade declined sharply. However, new trade routes emerged, primarily toward the Nearctic, Afrotropical, and Indo-Malay regions. Although regional bans can curtail invasion risk globally, to be fully effective and prevent rerouting of trade flows, bans should be global. PMID:29181443

  2. Networks of global bird invasion altered by regional trade ban.

    PubMed

    Reino, Luís; Figueira, Rui; Beja, Pedro; Araújo, Miguel B; Capinha, César; Strubbe, Diederik

    2017-11-01

    Wildlife trade is a major pathway for introduction of invasive species worldwide. However, how exactly wildlife trade influences invasion risk, beyond the transportation of individuals to novel areas, remains unknown. We analyze the global trade network of wild-caught birds from 1995 to 2011 as reported by CITES (Convention on International Trade in Endangered Species of Wild Fauna and Flora). We found that before the European Union ban on imports of wild-caught birds, declared in 2005, invasion risk was closely associated with numbers of imported birds, diversity of import sources, and degree of network centrality of importer countries. After the ban, fluxes of global bird trade declined sharply. However, new trade routes emerged, primarily toward the Nearctic, Afrotropical, and Indo-Malay regions. Although regional bans can curtail invasion risk globally, to be fully effective and prevent rerouting of trade flows, bans should be global.

  3. Trade in health services in the ASEAN region.

    PubMed

    Arunanondchai, Jutamas; Fink, Carsten

    2006-12-01

    Promoting quality health services to large population segments is a key ingredient to human and economic development. At its core, healthcare policymaking involves complex trade-offs between promoting equitable and affordable access to a basic set of health services, creating incentives for efficiencies in the healthcare system and managing constraints in government budgets. International trade in health services influences these trade-offs. It presents opportunities for cost savings and access to better quality care, but it also raises challenges in promoting equitable and affordable access. This paper offers a discussion of trade policy in health services for the ASEAN region. It reviews the existing patterns of trade and identifies policy measures that could further harness the benefits from trade in health services and address potential pitfalls that deeper integration may bring about.

  4. Estimation of regional differences in wind erosion sensitivity in Hungary

    NASA Astrophysics Data System (ADS)

    Mezősi, G.; Blanka, V.; Bata, T.; Kovács, F.; Meyer, B.

    2015-01-01

    In Hungary, wind erosion is one of the most serious natural hazards. Spatial and temporal variation in the factors that determine the location and intensity of wind erosion damage are not well known, nor are the regional and local sensitivities to erosion. Because of methodological challenges, no multi-factor, regional wind erosion sensitivity map is available for Hungary. The aim of this study was to develop a method to estimate the regional differences in wind erosion sensitivity and exposure in Hungary. Wind erosion sensitivity was modelled using the key factors of soil sensitivity, vegetation cover and wind erodibility as proxies. These factors were first estimated separately by factor sensitivity maps and later combined by fuzzy logic into a regional-scale wind erosion sensitivity map. Large areas were evaluated by using publicly available data sets of remotely sensed vegetation information, soil maps and meteorological data on wind speed. The resulting estimates were verified by field studies and examining the economic losses from wind erosion as compensated by the state insurance company. The spatial resolution of the resulting sensitivity map is suitable for regional applications, as identifying sensitive areas is the foundation for diverse land development control measures and implementing management activities.

  5. Dynamics of a developing economy with a remote region: Agglomeration, trade integration and trade patterns

    NASA Astrophysics Data System (ADS)

    Commendatore, Pasquale; Kubin, Ingrid; Sushko, Iryna

    2018-05-01

    We consider a three-region developing economy with poor transport infrastructures. Two models are related to different stages of development: in the first all regions are autarkic; in the second two of the regions begin to integrate with the third region still not accessible to trade. The properties of the two models are studied also considering the interplay between industry location and trade patterns. Dynamics of these models are described by two-dimensional piecewise smooth maps, characterized by multistability and complex bifurcation structure of the parameter space. We obtain analytical results related to stability of various fixed points and illustrate several bifurcation structures by means of two-dimensional bifurcation diagrams and basins of coexisting attractors.

  6. A study of rotor and platform design trade-offs for large-scale floating vertical axis wind turbines

    NASA Astrophysics Data System (ADS)

    Griffith, D. Todd; Paquette, Joshua; Barone, Matthew; Goupee, Andrew J.; Fowler, Matthew J.; Bull, Diana; Owens, Brian

    2016-09-01

    Vertical axis wind turbines are receiving significant attention for offshore siting. In general, offshore wind offers proximity to large populations centers, a vast & more consistent wind resource, and a scale-up opportunity, to name a few beneficial characteristics. On the other hand, offshore wind suffers from high levelized cost of energy (LCOE) and in particular high balance of system (BoS) costs owing to accessibility challenges and limited project experience. To address these challenges associated with offshore wind, Sandia National Laboratories is researching large-scale (MW class) offshore floating vertical axis wind turbines (VAWTs). The motivation for this work is that floating VAWTs are a potential transformative technology solution to reduce offshore wind LCOE in deep-water locations. This paper explores performance and cost trade-offs within the design space for floating VAWTs between the configurations for the rotor and platform.

  7. The Relative Importance of Convective and Trade-wind Orographic Precipitation to Streamflow in the Luquillo Mountains, Eastern Puerto Rico

    NASA Astrophysics Data System (ADS)

    Scholl, M. A.; Shanley, J. B.; Occhi, M.; Scatena, F. N.

    2012-12-01

    Like many mountainous areas in the tropics, watersheds in the Luquillo Mountains of Puerto Rico (18.3° N) have abundant rainfall and stream discharge, but relatively little storage capacity. Therefore, the water supply is vulnerable to drought and water availability may be affected by projected changes in regional temperature and atmospheric dynamics due to global warming. To help determine the links between climate and water availability, precipitation patterns were analyzed, and stable-isotope signatures of precipitation from different seasonal weather systems were established to identify those that are most important in maintaining streamflow and groundwater recharge. Stable isotope data include cloud water, rainfall, throughfall, streamflow, and groundwater from the Rio Mameyes and Rio Icacos/ Rio Blanco watersheds. Precipitation inputs have a wide range of stable isotope values, from fog/cloud water with δ2H and δ18O averaging +3.2‰, -1.74‰ respectively, to tropical storm rain with values as low as -154‰, -20.4‰. Spatial and temporal patterns of water isotopic values on this Caribbean island are different than higher latitude, continental watersheds. The data exhibit a 'reverse seasonality', with higher isotopic values in winter and lower values in summer; and stable isotope values of stream water do not decrease as expected with increasing altitude, because of cloud water input. Rain isotopic values vary predictably with local and mesoscale weather patterns and correlate strongly with cloud altitude. This correlation allows us to assign isotopic signatures to different sources of precipitation, and to investigate which climate patterns contribute to streamflow and groundwater recharge. At a measurement site at 615 m in the Luquillo Mountains, the average length of time between rain events was 15 h, and 45% of the rain events were <2 mm, reflecting the frequent small rain events of the trade-wind orographic rainfall weather pattern. Long

  8. Wind bubbles within H ii regions around slowly moving stars

    NASA Astrophysics Data System (ADS)

    Mackey, Jonathan; Gvaramadze, Vasilii V.; Mohamed, Shazrene; Langer, Norbert

    2015-01-01

    Interstellar bubbles around O stars are driven by a combination of the star's wind and ionizing radiation output. The wind contribution is uncertain because the boundary between the wind and interstellar medium is difficult to observe. Mid-infrared observations (e.g., of the H ii region RCW 120) show arcs of dust emission around O stars, contained well within the H ii region bubble. These arcs could indicate the edge of an asymmetric stellar wind bubble, distorted by density gradients and/or stellar motion. We present two-dimensional, radiation-hydrodynamics simulations investigating the evolution of wind bubbles and H ii regions around massive stars moving through a dense (nH = 3000 cm-3), uniform medium with velocities ranging from 4 to 16 km s-1. The H ii region morphology is strongly affected by stellar motion, as expected, but the wind bubble is also very aspherical from birth, even for the lowest space velocity considered. Wind bubbles do not fill their H ii regions (we find filling factors of 10-20 per cent), at least for a main sequence star with mass M⋆ ~ 30 M⊙. Furthermore, even for supersonic velocities the wind bow shock does not significantly trap the ionization front. X-ray emission from the wind bubble is soft, faint, and comes mainly from the turbulent mixing layer between the wind bubble and the H ii region. The wind bubble radiates <1 per cent of its energy in X-rays; it loses most of its energy by turbulent mixing with cooler photoionized gas. Comparison of the simulations with the H ii region RCW 120 shows that its dynamical age is ≲0.4 Myr and that stellar motion ≲4 km s-1 is allowed, implying that the ionizing source is unlikely to be a runaway star but more likely formed in situ. The region's youth, and apparent isolation from other O or B stars, makes it very interesting for studies of massive star formation and of initial mass functions. Movies are available in electronic form at http://www.aanda.org

  9. Performance of the CORDEX regional climate models in simulating offshore wind and wind potential

    NASA Astrophysics Data System (ADS)

    Kulkarni, Sumeet; Deo, M. C.; Ghosh, Subimal

    2018-03-01

    This study is oriented towards quantification of the skill addition by regional climate models (RCMs) in the parent general circulation models (GCMs) while simulating wind speed and wind potential with particular reference to the Indian offshore region. To arrive at a suitable reference dataset, the performance of wind outputs from three different reanalysis datasets is evaluated. The comparison across the RCMs and their corresponding parent GCMs is done on the basis of annual/seasonal wind statistics, intermodel bias, wind climatology, and classes of wind potential. It was observed that while the RCMs could simulate spatial variability of winds, well for certain subregions, they generally failed to replicate the overall spatial pattern, especially in monsoon and winter. Various causes of biases in RCMs were determined by assessing corresponding maps of wind vectors, surface temperature, and sea-level pressure. The results highlight the necessity to carefully assess the RCM-yielded winds before using them for sensitive applications such as coastal vulnerability and hazard assessment. A supplementary outcome of this study is in form of wind potential atlas, based on spatial distribution of wind classes. This could be beneficial in suitably identifying viable subregions for developing offshore wind farms by intercomparing both the RCM and GCM outcomes. It is encouraging that most of the RCMs and GCMs indicate that around 70% of the Indian offshore locations in monsoon would experience mean wind potential greater than 200 W/m2.

  10. 2016 State of Wind Development in the United States by Region

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

    Baranowski, Ruth; Oteri, Frank; Baring-Gould, Ian

    Significant expansion of wind energy development will be required to achieve the scenarios outlined in the U.S. Department of Energy's (DOE)'s Wind Vision: 20% wind energy by 2030 and 35% wind energy by 2050. Wind energy currently provides nearly 5% of the nation's electricity but has the potential to provide much more. The wind industry and the DOE's Wind Energy Technologies Office are addressing technical wind energy challenges, such as reducing turbine costs and increasing energy production and reliability. The Office recognizes that public acceptance of wind energy can be challenging, depending on the proximity of proposed wind farms tomore » local populations. Informed decision makers and communities equipped with unbiased information about the benefits and impacts of wind energy development are better prepared to navigate the sometimes contentious development process. In 2014, DOE established six Regional Resource Centers (RRCs) across the United States to communicate unbiased, credible information about wind energy to stakeholders through regional networks. The RRCs provide ready access to this information to familiarize the public with wind energy; raise awareness about potential benefits and issues; and disseminate data on siting considerations such as turbine sound and wildlife habitat protection. This document summarizes the status and drivers for U.S. wind energy development during 2016. RRC leaders provided a report of wind energy development in their regions, which was combined with findings from National Renewable Energy Laboratory (NREL) researchers to provide an account of the state of the regions, as well as updates on developments in individual states. NREL researchers and state partners added updates for all states that are not directly supported by an RRC. Accounts for each region include updates on renewable portfolio standards, the Clean Power Plan, workforce development, manufacturing and economic development, and individual state updates

  11. Evidence of active region imprints on the solar wind structure

    NASA Technical Reports Server (NTRS)

    Hick, P.; Jackson, B. V.

    1995-01-01

    A common descriptive framework for discussing the solar wind structure in the inner heliosphere uses the global magnetic field as a reference: low density, high velocity solar wind emanates from open magnetic fields, with high density, low speed solar wind flowing outward near the current sheet. In this picture, active regions, underlying closed magnetic field structures in the streamer belt, leave little or no imprint on the solar wind. We present evidence from interplanetary scintillation measurements of the 'disturbance factor' g that active regions play a role in modulating the solar wind and possibly contribute to the solar wind mass output. Hence we find that the traditional view of the solar wind, though useful in understanding many features of solar wind structure, is oversimplified and possibly neglects important aspects of solar wind dynamics

  12. A study of the solar wind deceleration in the Earth's foreshock region

    NASA Technical Reports Server (NTRS)

    Zhang, T.-L.; Schwingenschuh, K.; Russell, C. T.

    1995-01-01

    Previous observations have shown that the solar wind is decelerated and deflected in the earth's upstream region populated by long-period waves. This deceleration is corelated with the 'diffuse' but not with the 'reflected' ion population. The speed of the solar wind may decrease tens of km/s in the foreshock region. The solar wind dynamic pressure exerted on the magnetopause may vary due to the fluctuation of the solar wind speed and density in the foreshock region. In this study, we examine this solar wind deceleration and determine how the solar wind deceleration varies in the foreshock region.

  13. Roles of production, consumption and trade in global and regional aerosol radiative forcing

    NASA Astrophysics Data System (ADS)

    Lin, J.; Tong, D.; Davis, S. J.; Ni, R.; Tan, X.; Pan, D.; Zhao, H.; Lu, Z.; Streets, D. G.; Feng, T.; Zhang, Q.; Yan, Y.; Hu, Y.; Li, J.; Liu, Z.; Jiang, X.; Geng, G.; He, K.; Huang, Y.; Guan, D.

    2016-12-01

    Anthropogenic aerosols exert strong radiative forcing on the climate system. Prevailing view regards aerosol radiative forcing as a result of emissions from regions' economic production, with China and other developing regions having the largest contributions to radiative forcing at present. However, economic production is driven by global demand for computation, and international trade allows for separation of regions consuming goods and services from regions where goods and related aerosol pollution are produced. It has recently been recognized that regions' consumption and trade have profoundly altered the spatial distribution of aerosol emissions and pollution. Building upon our previous work, this study quantifies for the first time the roles of trade and consumption in aerosol climate forcing attributed to different regions. We contrast the direct radiative forcing of aerosols related to regions' consumption of goods and services against the forcing due to emissions produced in each region. Aerosols assessed include black carbon, primary organic aerosol, and secondary inorganic aerosols including sulfate, nitrate and ammonium. We find that global aerosol radiative forcing due to emissions produced in East Asia is much stronger than the forcing related to goods and services ultimately consumed in that region because of its large net export of emissions-intensive goods. The opposite is true for net importers like Western Europe and North America: global radiative forcing related to consumption is much greater than the forcing due to emissions produced in these regions. Overall, trade is associated with a shift of radiative forcing from net importing to net exporting regions. Compared to greenhouse gases such as carbon dioxide, the short atmospheric lifetimes of aerosols cause large localized differences in radiative forcing. International efforts to reduce emissions in the exporting countries will help alleviate trade-related climate and health impacts of

  14. Effects of trade-wind strength and direction on the leeside circulations and rainfall of the island of Hawaii

    Treesearch

    Yang Yang; Yi-Leng Chen; Francis M. Fujioka

    2009-01-01

    The leeside circulations and weather of the island of Hawaii were studied from the fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5) land surface model simulations for eight strong (∼7.9 m s−1) and eight weak (∼5.2 m s−1) trade-wind days and for five days with southeasterly trades (∼7.1 m s

  15. Virtual Water Trade: Revisiting the Assessments to Incorporate Regional Water Stress

    NASA Astrophysics Data System (ADS)

    Perveen, S.; Puma, M. J.; Troy, T. J.; Browne, M.; Ghosh, M.

    2011-12-01

    Virtual water (VW) refers to the volume of freshwater embedded in the production and shipment of a commodity, which can include agricultural or industrial products, and the trade of commodities can then be viewed as the trade of one region's water resources to another. The premise behind this trade is that countries with a comparative water advantage may choose to export crops, and countries with scarce water resources may focus economic activity on non-water intensive sectors. However, this assumption is not always true given food self-sufficiency policies; water scarce regions often choose to unsustainably mine aquifers for irrigation. Recent studies have shown no correlation between dependency on VW imports and water scarcity for nations, suggesting that politico-economic considerations rather than resource scarcity considerations may dominate the current VW dynamics. Existing VW computations do not take into account water-scarcity value or the full-cost pricing of commodities. This study aims to fill in this gap by focusing on three countries - the United States, India, and Japan - and their production, imports and exports of crop, livestock and industrial commodities. These countries offer three different perspectives on virtual water, with Japan as a net importer of agriculture virtual water and a major industrial nation. The United States, on the other hand, exports significant quantities of grain. India is a developing country with a strong focus on food self-sufficiency. We first quantify the amount of water used in the production of each commodity and then examine the virtual water trade balance for each country, examining the tradeoffs each country has made between agriculture and industrial water use; given that water resources are finite. To examine the interplay between virtual water trade and water scarcity, we focus on two sub-regions, the Ogallala Aquifer in the US and the Punjab region in India, both of which have significant agricultural

  16. Lead isotopes in trade wind aerosols at Barbados - The influence of European emissions over the North Atlantic

    NASA Technical Reports Server (NTRS)

    Hamelin, B.; Grousset, F. E.; Biscaye, P. E.; Zindler, A.; Prospero, J. M.

    1989-01-01

    Previous studies have shown that Pb can be used as a transient tracer in the atmosphere and the ocean because of strong time-variability of industrial inputs and because Pb isotopic composition can be used to identify contributions from different sources. Pb isotopic measurements on aerosols collected from the North Atlantic Ocean in the trade wind belt are presented. Aerosols sampled at Barbados during the 1969-1985 period have a Pb isotopic composition different from that observed by previous investigators in Bermuda corals and Sargasso Sea waters. Barbados aerosols appear to contain significant amounts of relatively unradiogenic industrial and automotive Pb that is derived from Europe and carried to Barbados by the trade winds. In contrast, Bermuda corals and Sargasso sea waters are influenced mainly by U.S.-derived emissions, which contain more radiogenic Pb originating from Missouri-type ores. This difference generates a strong latitudinal Europe-U.S.A. isotopic gradient, thus allowing study of trans-Atlantic atmospheric transport and ocean mixing processes.

  17. Opportunities for Wind Power In Low- and Mid-Quality Resource Regions

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

    Lantz, Eric; Mai, Trieu; Heimiller, Donna

    2016-05-25

    In this presentation for American Wind Energy Association (AWEA) WINDPOWER 2016 conference, the authors discuss wind power today in low and mid-quality resource regions, the anticipated role of wind power in the future electric sector, market potential in low and mid-quality resource regions, and anticipated innovations to capture that market potential.

  18. REGIONAL-SCALE WIND FIELD CLASSIFICATION EMPLOYING CLUSTER ANALYSIS

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

    Glascoe, L G; Glaser, R E; Chin, H S

    2004-06-17

    The classification of time-varying multivariate regional-scale wind fields at a specific location can assist event planning as well as consequence and risk analysis. Further, wind field classification involves data transformation and inference techniques that effectively characterize stochastic wind field variation. Such a classification scheme is potentially useful for addressing overall atmospheric transport uncertainty and meteorological parameter sensitivity issues. Different methods to classify wind fields over a location include the principal component analysis of wind data (e.g., Hardy and Walton, 1978) and the use of cluster analysis for wind data (e.g., Green et al., 1992; Kaufmann and Weber, 1996). The goalmore » of this study is to use a clustering method to classify the winds of a gridded data set, i.e, from meteorological simulations generated by a forecast model.« less

  19. China’s Trade Opening: Implications for Regional Stability

    DTIC Science & Technology

    2002-08-01

    China’s Trade Opening: Implications for Regional Stability by Howard M. Krawitz Strategic Forum China’s entry into the World Trade Orga-nization...Strategic Studies National Defense University Key Points No. 193, August 2002 Strategic Forum 1 Report Documentation Page Form ApprovedOMB No. 0704-0188...As the rule of law concept gains ground, it should promote development of a better- educated , more professional Chinese legal community (that is, law

  20. Solar wind stream interaction regions throughout the heliosphere

    NASA Astrophysics Data System (ADS)

    Richardson, Ian G.

    2018-01-01

    This paper focuses on the interactions between the fast solar wind from coronal holes and the intervening slower solar wind, leading to the creation of stream interaction regions that corotate with the Sun and may persist for many solar rotations. Stream interaction regions have been observed near 1 AU, in the inner heliosphere (at ˜ 0.3-1 AU) by the Helios spacecraft, in the outer and distant heliosphere by the Pioneer 10 and 11 and Voyager 1 and 2 spacecraft, and out of the ecliptic by Ulysses, and these observations are reviewed. Stream interaction regions accelerate energetic particles, modulate the intensity of Galactic cosmic rays and generate enhanced geomagnetic activity. The remote detection of interaction regions using interplanetary scintillation and white-light imaging, and MHD modeling of interaction regions will also be discussed.

  1. Methane at Ascension Island, southern tropical Atlantic Ocean: continuous ground measurement and vertical profiling above the Trade-Wind Inversion

    NASA Astrophysics Data System (ADS)

    Lowry, David; Brownlow, Rebecca; Fisher, Rebecca; Nisbet, Euan; Lanoisellé, Mathias; France, James; Thomas, Rick; Mackenzie, Rob; Richardson, Tom; Greatwood, Colin; Freer, Jim; Cain, Michelle; Warwick, Nicola; Pyle, John

    2015-04-01

    Methane mixing ratios have been rising rapidly worldwide since 2007. At Ascension Island (8oS in the equatorial Atlantic), a sustained rise has occurred. Prior to 2010, growth was comparable to other regions, but in 2010-11, during a strong la Nina event, the increase was 10ppb year-on-year. Reduced growth followed in 2011-12, but in 2012-13 strong growth resumed and continues. This rise has been accompanied by a shift to lighter δ13CCH4 values in 2010-11 in the equatorial tropics. The most likely cause of this shift is emissions from isotopically 'light' biological sources in the equatorial and savanna tropics. Ascension Island is in the Trade Wind belt of the tropical Atlantic, perfectly located to measure the South Atlantic marine boundary layer. The SE Trade Winds are almost invariant, derived from the deep South Atlantic and with little contact with Africa. However, above the Trade Wind Inversion (TWI) at about 1200-2000m asl, the air masses are very different, coming dominantly from tropical Africa and occasionally S. America. Depending on season, air above the TWI is sourced from the African southern savanna grasslands or the equatorial wetlands of Congo and Uganda, with inputs of air also from southern tropical S. America (Brazil, Paraguay, Bolivia). African methane sources are a major contributor to the global methane budget, but although local campaign studies have been made, African emissions are not well studied in bulk. In September 2014, an octocopter was used to retrieve air samples from heights up to 2700m asl on Ascension (see Thomas, R. et al, this volume). This allowed sampling through the marine boundary layer, across the TWI cloud layer, and into the mid-troposphere. Samples were collected in part-filled 5L Tedlar bags, which were analysed for CH4 concentration using Royal Holloway's Picarro 1301 CRDS system at the Met Office, Ascension. This has high precision and accuracy, with a 6-gas calibration suite. Bags were then analysed in the UK for

  2. Revealing Environmental Inequality Hidden in China's Inter-regional Trade.

    PubMed

    Zhang, Wei; Liu, Yu; Feng, Kuishuang; Hubacek, Klaus; Wang, Jinnan; Liu, Miaomiao; Jiang, Ling; Jiang, Hongqiang; Liu, Nianlei; Zhang, Pengyan; Zhou, Ying; Bi, Jun

    2018-06-14

    Trade among regions or countries not only allows the exchange of goods and services but also leads to the transfer of pollution. The unequal exchange of goods and services and associated value added and pollution may be subject to environmental inequality in China given that Chinese provinces are in different development stages. By using the latest multiregional input-output tables and the sectoral air pollutant emission inventory in 2012, we traced emissions and value added along China's domestic supply chains. Here, we show that 62%-76% of the consumption-based air-pollutant emissions of richer regions (Beijing-Tianjin, East Coast and South Coast) were outsourced to other regions; however, approximately 70% of the value added triggered by these region's final consumption was retained within the region. Some provinces in western China, such as Guizhou, Ningxia, and Yunnan, not only incurred net pollution inflows but also suffered a negative balance of value added when trading with rich provinces. Addressing such inequalities could provide not only a basis for determining each province's responsibility for pollution control but also a model for other emerging economies.

  3. Wind energy: Resources, systems, and regional strategies

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

    Grubb, M.J.; Meyer, N.I.

    1993-12-31

    Wind power is already cost competitive with conventional modes of electricity generation under certain conditions and could, if widely exploited, meet 20 percent or more of the world`s electricity needs within the next four to five decades. The greatest wind potential exists in North America, the former Soviet Union, Africa, and (to a lesser extent), South America, Australia, southern Asia, and parts of Europe. In all these areas, wind can make a significant contribution to the energy supply. In regions of the developing world and in island communities, wind can operate with storage and displace diesel fuel. In more developedmore » areas, wind-generated electricity can be channeled directly into the grid, providing an environmentally benign alternative to fossil fuels. Indeed, wind power can contribute as much as 25 to 45 percent of a grid`s energy supply before economic penalties become prohibitive; the presence of storage facilities or hydroelectric power would increase wind`s share still further. Despite a promising future, opportunities for wind power development are probably being missed because too little is known about either the resource or the technology. International efforts are badly needed to obtain better data and to disseminate technological information around the world. Even then, the extent to which wind is exploited will depend on public reaction and on the willingness of governments to embrace the technology. Action that governments might take to promote wind include providing strategic incentives to further its deployment, funding research on wind resources, taxing fossil fuels to reflect their social costs, and allowing independent wind generators adequate access to electricity systems. 74 refs., 15 figs., 10 tabs.« less

  4. Regional Input-Output Tables and Trade Flows: an Integrated and Interregional Non-survey Approach

    DOE PAGES

    Boero, Riccardo; Edwards, Brian Keith; Rivera, Michael Kelly

    2017-03-20

    Regional input–output tables and trade flows: an integrated and interregional non-survey approach. Regional Studies. Regional analyses require detailed and accurate information about dynamics happening within and between regional economies. However, regional input–output tables and trade flows are rarely observed and they must be estimated using up-to-date information. Common estimation approaches vary widely but consider tables and flows independently. Here, by using commonly used economic assumptions and available economic information, this paper presents a method that integrates the estimation of regional input–output tables and trade flows across regions. Examples of the method implementation are presented and compared with other approaches, suggestingmore » that the integrated approach provides advantages in terms of estimation accuracy and analytical capabilities.« less

  5. Regional Input-Output Tables and Trade Flows: an Integrated and Interregional Non-survey Approach

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

    Boero, Riccardo; Edwards, Brian Keith; Rivera, Michael Kelly

    Regional input–output tables and trade flows: an integrated and interregional non-survey approach. Regional Studies. Regional analyses require detailed and accurate information about dynamics happening within and between regional economies. However, regional input–output tables and trade flows are rarely observed and they must be estimated using up-to-date information. Common estimation approaches vary widely but consider tables and flows independently. Here, by using commonly used economic assumptions and available economic information, this paper presents a method that integrates the estimation of regional input–output tables and trade flows across regions. Examples of the method implementation are presented and compared with other approaches, suggestingmore » that the integrated approach provides advantages in terms of estimation accuracy and analytical capabilities.« less

  6. Simulating Turbulent Wind Fields for Offshore Turbines in Hurricane-Prone Regions (Poster)

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

    Guo, Y.; Damiani, R.; Musial, W.

    Extreme wind load cases are one of the most important external conditions in the design of offshore wind turbines in hurricane prone regions. Furthermore, in these areas, the increase in load with storm return-period is higher than in extra-tropical regions. However, current standards have limited information on the appropriate models to simulate wind loads from hurricanes. This study investigates turbulent wind models for load analysis of offshore wind turbines subjected to hurricane conditions. Suggested extreme wind models in IEC 61400-3 and API/ABS (a widely-used standard in oil and gas industry) are investigated. The present study further examines the wind turbinemore » response subjected to Hurricane wind loads. Three-dimensional wind simulator, TurbSim, is modified to include the API wind model. Wind fields simulated using IEC and API wind models are used for an offshore wind turbine model established in FAST to calculate turbine loads and response.« less

  7. Lead isotopes in trade wind aerosols at Barbados: the influence of European emissions over the North Atlantic

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

    Hamelin, B.; Grousset, F.E.; Biscaye, P.E.

    1989-11-15

    Previous studies have shown that Pb can be used as a transient tracer in the atmosphere and the ocean because of strong time-variability of industrial inputs and because Pb isotopic composition can be used to identify contribution from different sources. We present Pb isotopic measurements on aerosols collected from the North Atlantic Ocean in the trade wind belt. Aerosols sampled at Barbados during the 1969--1985 period have a Pb isotopic compositions different from that observed by previous investigators in Bermuda corals and Sargasso Sea waters. Barbados aerosols appear to contain significant amounts of relatively unradiogenic industrial and automotive Pb thatmore » is derived from Europe and carried to Barbados by the trade winds. In contrast, Bermuda corals and Sargasso sea waters are influenced mainly by U.S.-derived emissions, which contain more radiogenic Pb originating from Missouri-type ores. This difference generates a strong latitudinal Europe-U.S.A. isotopic gradient, thus allowing study of trans-Atlantic atmospheric transport and ocean mixing processes. {copyright} American Geophysical Union 1989« less

  8. Wind tunnel study of the wind turbine interaction with a boundary-layer flow: Upwind region, turbine performance, and wake region

    NASA Astrophysics Data System (ADS)

    Bastankhah, M.; Porté-Agel, F.

    2017-06-01

    Comprehensive wind tunnel experiments were carried out to study the interaction of a turbulent boundary layer with a wind turbine operating under different tip-speed ratios and yaw angles. Force and power measurements were performed to characterize the variation of thrust force (both magnitude and direction) and generated power of the wind turbine under different operating conditions. Moreover, flow measurements, collected using high-resolution particle-image velocimetry as well as hot-wire anemometry, were employed to systematically study the flow in the upwind, near-wake, and far-wake regions. These measurements provide new insights into the effect of turbine operating conditions on flow characteristics in these regions. For the upwind region, the results show a strong lateral asymmetry under yawed conditions. For the near-wake region, the evolution of tip and root vortices was studied with the use of both instantaneous and phase-averaged vorticity fields. The results suggest that the vortex breakdown position cannot be determined based on phase-averaged statistics, particularly for tip vortices under turbulent inflow conditions. Moreover, the measurements in the near-wake region indicate a complex velocity distribution with a speed-up region in the wake center, especially for higher tip-speed ratios. In order to elucidate the meandering tendency of far wakes, particular focus was placed on studying the characteristics of large turbulent structures in the boundary layer and their interaction with wind turbines. Although these structures are elongated in the streamwise direction, their cross sections are found to have a size comparable to the rotor area, so that they can be affected by the presence of the turbine. In addition, the study of spatial coherence in turbine wakes reveals that any statistics based on streamwise velocity fluctuations cannot provide reliable information about the size of large turbulent structures in turbine wakes due to the effect of wake

  9. Mapping hotspots of threatened species traded in bushmeat markets in the Cross-Sanaga rivers region.

    PubMed

    Fa, John E; Farfán, Miguel Angel; Marquez, Ana Luz; Duarte, Jesús; Nackoney, Janet; Hall, Amy; Dupain, Jef; Seymour, Sarah; Johnson, Paul J; MacDonald, David W; Vargas, J Mario

    2014-02-01

    Bushmeat markets exist in many countries in West and Central Africa, and data on species sold can be used to detect patterns of wildlife trade in a region. We surveyed 89 markets within the Cross-Sanaga rivers region, West Africa. In each market, we counted the number of carcasses of each taxon sold. During a 6-month period (7594 market days), 44 mammal species were traded. Thirteen species were on the International Union for Conservation of Nature (IUCN) Red List or protected under national legislation, and at least 1 threatened species was traded in 88 of the 89 markets. We used these data to identify market groups that traded similar species assemblages. Using cluster analyses, we detected 8 market groups that were also geographically distinct. Market groups differed in the diversity of species, evenness of species, and dominant, prevalent, and characteristic species traded. We mapped the distribution of number of threatened species traded across the study region. Most threatened species were sold in markets nearest 2 national parks, Korup National Park in Cameroon and Cross River in Nigeria. To assess whether the threatened-species trade hotspots coincided with the known ranges of these species, we mapped the overlap of all threatened species traded. Markets selling more threatened species overlapped with those regions that had higher numbers of these. Our study can provide wildlife managers in the region with better tools to discern zones within which to focus policing efforts and reduce threats to species that are threatened by the bushmeat trade. © 2013 Society for Conservation Biology.

  10. Numerical simulations of island-scale airflow over Maui and the Maui vortex under summer trade wind conditions

    Treesearch

    DaNa L. Carlis; Yi-Leng Chen; Vernon R. Morris

    2010-01-01

    The fifth-generation Pennsylvania State University–NCAR Mesoscale Model (MM5) coupled with the Noah land surface model (LSM) is employed to simulate island-scale airflow and circulations over Maui County, Hawaii, under summer trade wind conditions, during July–August 2005. The model forecasts are validated by surface observations with good agreement.

  11. Scaling up from field to region for wind erosion prediction using a field-scale wind erosion model and GIS

    USGS Publications Warehouse

    Zobeck, T.M.; Parker, N.C.; Haskell, S.; Guoding, K.

    2000-01-01

    Factors that affect wind erosion such as surface vegetative and other cover, soil properties and surface roughness usually change spatially and temporally at the field-scale to produce important field-scale variations in wind erosion. Accurate estimation of wind erosion when scaling up from fields to regions, while maintaining meaningful field-scale process details, remains a challenge. The objectives of this study were to evaluate the feasibility of using a field-scale wind erosion model with a geographic information system (GIS) to scale up to regional levels and to quantify the differences in wind erosion estimates produced by different scales of soil mapping used as a data layer in the model. A GIS was used in combination with the revised wind erosion equation (RWEQ), a field-scale wind erosion model, to estimate wind erosion for two 50 km2 areas. Landsat Thematic Mapper satellite imagery from 1993 with 30 m resolution was used as a base map. The GIS database layers included land use, soils, and other features such as roads. The major land use was agricultural fields. Data on 1993 crop management for selected fields of each crop type were collected from local government agency offices and used to 'train' the computer to classify land areas by crop and type of irrigation (agroecosystem) using commercially available software. The land area of the agricultural land uses was overestimated by 6.5% in one region (Lubbock County, TX, USA) and underestimated by about 21% in an adjacent region (Terry County, TX, USA). The total estimated wind erosion potential for Terry County was about four times that estimated for adjacent Lubbock County. The difference in potential erosion among the counties was attributed to regional differences in surface soil texture. In a comparison of different soil map scales in Terry County, the generalised soil map had over 20% more of the land area and over 15% greater erosion potential in loamy sand soils than did the detailed soil map. As

  12. Equilibrium pricing in electricity markets with wind power

    NASA Astrophysics Data System (ADS)

    Rubin, Ofir David

    Estimates from the World Wind Energy Association assert that world total wind power installed capacity climbed from 18 Gigawatt (GW) to 152 GW from 2000 to 2009. Moreover, according to their predictions, by the end of 2010 global wind power capacity will reach 190 GW. Since electricity is a unique commodity, this remarkable expansion brings forward several key economic questions regarding the integration of significant amount of wind power capacity into deregulated electricity markets. The overall dissertation objective is to develop a comprehensive theoretical framework that enables the modeling of the performance and outcome of wind-integrated electricity markets. This is relevant because the state of knowledge of modeling electricity markets is insufficient for the purpose of wind power considerations. First, there is a need to decide about a consistent representation of deregulated electricity markets. Surprisingly, the related body of literature does not agree on the very economic basics of modeling electricity markets. That is important since we need to capture the fundamentals of electricity markets before we introduce wind power to our study. For example, the structure of the electric industry is a key. If market power is present, the integration of wind power has large consequences on welfare distribution. Since wind power uncertainty changes the dynamics of information it also impacts the ability to manipulate market prices. This is because the quantity supplied by wind energy is not a decision variable. Second, the intermittent spatial nature of wind over a geographical region is important because the market value of wind power capacity is derived from its statistical properties. Once integrated into the market, the distribution of wind will impact the price of electricity produced from conventional sources of energy. Third, although wind power forecasting has improved in recent years, at the time of trading short-term electricity forwards, forecasting

  13. Hourly Wind Speed Interval Prediction in Arid Regions

    NASA Astrophysics Data System (ADS)

    Chaouch, M.; Ouarda, T.

    2013-12-01

    The long and extended warm and dry summers, the low rate of rain and humidity are the main factors that explain the increase of electricity consumption in hot arid regions. In such regions, the ventilating and air-conditioning installations, that are typically the most energy-intensive among energy consumption activities, are essential for securing healthy, safe and suitable indoor thermal conditions for building occupants and stored materials. The use of renewable energy resources such as solar and wind represents one of the most relevant solutions to overcome the increase of the electricity demand challenge. In the recent years, wind energy is gaining more importance among the researchers worldwide. Wind energy is intermittent in nature and hence the power system scheduling and dynamic control of wind turbine requires an estimate of wind energy. Accurate forecast of wind speed is a challenging task for the wind energy research field. In fact, due to the large variability of wind speed caused by the unpredictable and dynamic nature of the earth's atmosphere, there are many fluctuations in wind power production. This inherent variability of wind speed is the main cause of the uncertainty observed in wind power generation. Furthermore, producing wind power forecasts might be obtained indirectly by modeling the wind speed series and then transforming the forecasts through a power curve. Wind speed forecasting techniques have received substantial attention recently and several models have been developed. Basically two main approaches have been proposed in the literature: (1) physical models such as Numerical Weather Forecast and (2) statistical models such as Autoregressive integrated moving average (ARIMA) models, Neural Networks. While the initial focus in the literature has been on point forecasts, the need to quantify forecast uncertainty and communicate the risk of extreme ramp events has led to an interest in producing probabilistic forecasts. In short term

  14. Near-surface wind variability over the broader Adriatic region: insights from an ensemble of regional climate models

    NASA Astrophysics Data System (ADS)

    Belušić, Andreina; Prtenjak, Maja Telišman; Güttler, Ivan; Ban, Nikolina; Leutwyler, David; Schär, Christoph

    2018-06-01

    Over the past few decades the horizontal resolution of regional climate models (RCMs) has steadily increased, leading to a better representation of small-scale topographic features and more details in simulating dynamical aspects, especially in coastal regions and over complex terrain. Due to its complex terrain, the broader Adriatic region represents a major challenge to state-of-the-art RCMs in simulating local wind systems realistically. The objective of this study is to identify the added value in near-surface wind due to the refined grid spacing of RCMs. For this purpose, we use a multi-model ensemble composed of CORDEX regional climate simulations at 0.11° and 0.44° grid spacing, forced by the ERA-Interim reanalysis, a COSMO convection-parameterizing simulation at 0.11° and a COSMO convection-resolving simulation at 0.02° grid spacing. Surface station observations from this region and satellite QuikSCAT data over the Adriatic Sea have been compared against daily output obtained from the available simulations. Both day-to-day wind and its frequency distribution are examined. The results indicate that the 0.44° RCMs rarely outperform ERA-Interim reanalysis, while the performance of the high-resolution simulations surpasses that of ERA-Interim. We also disclose that refining the grid spacing to a few km is needed to properly capture the small-scale wind systems. Finally, we show that the simulations frequently yield the accurate angle of local wind regimes, such as for the Bora flow, but overestimate the associated wind magnitude. Finally, spectral analysis shows good agreement between measurements and simulations, indicating the correct temporal variability of the wind speed.

  15. Climate information for the wind energy industry in the Mediterranean Region

    NASA Astrophysics Data System (ADS)

    Calmanti, Sandro; Davis, Melanie; Schmidt, Peter; Dell'Aquila, Alessandro

    2013-04-01

    According to the World Wind Energy Association the total wind generation capacity worldwide has come close to cover 3% of the world's electricity demand in 2011. Thanks to the enormous resource potential and the relatively low costs of construction and maintenance of wind power plants, the wind energy sector will remain one of the most attractive renewable energy investment options. Studies reveal that climate variability and change pose a new challenge to the entire renewable energy sector, and in particular for wind energy. Stakeholders in the wind energy sector mainly use, if available, site-specific historical climate information to assess wind resources at a given project site. So far, this is the only source of information that investors (e.g., banks) are keen to accept for decisions concerning the financing of wind energy projects. However, one possible wind energy risk at the seasonal scale is the volatility of earnings from year to year investment. The most significant risk is therefore that not enough units of energy (or megawatt hours) can be generated from the project to capture energy sales to pay down debt in any given quarter or year. On the longer time scale the risk is that a project's energy yields fall short of their estimated levels, resulting in revenues that consistently come in below their projection, over the life of the project. The nature of the risk exposure determines considerable interest in wind scenarios, as a potential component of both the planning and operational phase of a renewable energy project. Fundamentally, by using climate projections, the assumption of stationary wind regimes can be compared to other scenarios where large scale changes in atmospheric circulation patterns may affect local wind regimes. In the framework of CLIM-RUN EU FP7 project, climate experts are exploring the potential of seasonal to decadal climate forecast techniques (time-frame 2012-2040) and regional climate scenarios (time horizon 2040+) over the

  16. Wind Powering America's Regional Stakeholder Meetings and Priority State Reports: FY11 Summary

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

    Not Available

    2013-06-01

    Beginning in 2010, DOE conducted an assessment of Wind Powering America (WPA) activities to determine whether the methods the department had used to help grow the wind industry to provide 2% of the nation's electrical energy should be the same methods used to achieve 20% of the nation's energy from wind (as described in the report 20% Wind Energy by 2030: Increasing Wind Energy's Contribution to U.S. Electricity Supply). After the assessment, it was determined that the initiative's state-based activities should be phased out as part of a shift to regional-based approaches. To assist with this transition, WPA hosted amore » series of 1-day regional meetings at six strategic locations around the country and a single teleconference for island states, U.S. territories, and remote communities. This report summarizes the results of the inaugural regional meetings and the state reports with a focus on ongoing wind deployment barriers in each region.« less

  17. Wind Powering America's Regional Stakeholder Meetings and Priority State Reports: FY11 Summary

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

    Baring-Gould, Ian

    2013-06-01

    Beginning in 2010, DOE conducted an assessment of Wind Powering America (WPA) activities to determine whether the methods the department had used to help grow the wind industry to provide 2% of the nation's electrical energy should be the same methods used to achieve 20% of the nation's energy from wind (as described in the report 20% Wind Energy by 2030: Increasing Wind Energy's Contribution toU.S. Electricity Supply). After the assessment, it was determined that the initiative's state-based activities should be phased out as part of a shift to regional-based approaches. To assist with this transition, WPA hosted a seriesmore » of 1-day regional meetings at six strategic locations around the country and a single teleconference for island states, U.S. territories, and remote communities.This report summarizes the results of the inaugural regional meetings and the state reports with a focus on ongoing wind deployment barriers in each region.« less

  18. Mapping the Solar Wind from its Source Region into the Outer Corona

    NASA Technical Reports Server (NTRS)

    Esser, Ruth

    1997-01-01

    Knowledge of the radial variation of the plasma conditions in the coronal source region of the solar wind is essential to exploring coronal heating and solar wind acceleration mechanisms. The goal of the proposal was to determine as many plasma parameters in the solar wind acceleration region and beyond as possible by coordinating different observational techniques, such as Interplanetary Scintillation Observations, spectral line intensity observations, polarization brightness measurements and X-ray observations. The inferred plasma parameters were then used to constrain solar wind models.

  19. 2017 State of Wind Development in the United States by Region

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

    Oteri, Frank A; Baranowski, Ruth E; Baring-Gould, Edward I

    This document summarizes the status and drivers for U.S. wind energy development during 2017. Regional Resource Center (RRC) leaders provided a report of wind energy development in their regions, which was combined with findings from National Renewable Energy Laboratory (NREL) researchers to provide an account of the state of the regions, as well as updates on developments in individual states. NREL researchers and state partners added updates for all states that are not directly supported by an RRC. Accounts for each region include updates on renewable portfolio standards, workforce development, manufacturing and economic development, and individual state updates for installedmore » wind capacity, ongoing policy developments, planned projects and their status, transmission progress reports, etc. This report also highlights the efforts of the RRCs to engage stakeholders in their individual regions.« less

  20. Signatures of Slow Solar Wind Streams from Active Regions in the Inner Corona

    NASA Astrophysics Data System (ADS)

    Slemzin, V.; Harra, L.; Urnov, A.; Kuzin, S.; Goryaev, F.; Berghmans, D.

    2013-08-01

    The identification of solar-wind sources is an important question in solar physics. The existing solar-wind models ( e.g., the Wang-Sheeley-Arge model) provide the approximate locations of the solar wind sources based on magnetic field extrapolations. It has been suggested recently that plasma outflows observed at the edges of active regions may be a source of the slow solar wind. To explore this we analyze an isolated active region (AR) adjacent to small coronal hole (CH) in July/August 2009. On 1 August, Hinode/EUV Imaging Spectrometer observations showed two compact outflow regions in the corona. Coronal rays were observed above the active-region coronal hole (ARCH) region on the eastern limb on 31 July by STEREO-A/EUVI and at the western limb on 7 August by CORONAS- Photon/TESIS telescopes. In both cases the coronal rays were co-aligned with open magnetic-field lines given by the potential field source surface model, which expanded into the streamer. The solar-wind parameters measured by STEREO-B, ACE, Wind, and STEREO-A confirmed the identification of the ARCH as a source region of the slow solar wind. The results of the study support the suggestion that coronal rays can represent signatures of outflows from ARs propagating in the inner corona along open field lines into the heliosphere.

  1. Great Lakes O shore Wind Project: Utility and Regional Integration Study

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

    Sajadi, Amirhossein; Loparo, Kenneth A.; D'Aquila, Robert

    This project aims to identify transmission system upgrades needed to facilitate offshore wind projects as well as operational impacts of offshore generation on operation of the regional transmission system in the Great Lakes region. A simulation model of the US Eastern Interconnection was used as the test system as a case study for investigating the impact of the integration of a 1000MW offshore wind farm operating in Lake Erie into FirstEnergy/PJM service territory. The findings of this research provide recommendations on offshore wind integration scenarios, the locations of points of interconnection, wind profile modeling and simulation, and computational methods tomore » quantify performance, along with operating changes and equipment upgrades needed to mitigate system performance issues introduced by an offshore wind project.« less

  2. Regional trade and the nutrition transition: opportunities to strengthen NCD prevention policy in the Southern African Development Community.

    PubMed

    Thow, Anne Marie; Sanders, David; Drury, Eliza; Puoane, Thandi; Chowdhury, Syeda N; Tsolekile, Lungiswa; Negin, Joel

    2015-01-01

    Addressing diet-related non-communicable diseases (NCDs) will require a multisectoral policy approach that includes the food supply and trade, but implementing effective policies has proved challenging. The Southern African Development Community (SADC) has experienced significant trade and economic liberalization over the past decade; at the same time, the nutrition transition has progressed rapidly in the region. This analysis considers the relationship between regional trade liberalization and changes in the food environment associated with poor diets and NCDs, with the aim of identifying feasible and proactive policy responses to support healthy diets. Changes in trade and investment policy for the SADC were documented and compared with time-series graphs of import data for soft drinks and snack foods to assess changes in imports and source country in relation to trade and investment liberalization. Our analysis focuses on regional trade flows. Diets and the burden of disease in the SADC have changed since the 1990s in parallel with trade and investment liberalization. Imports of soft drinks increased by 76% into SADC countries between 1995 and 2010, and processed snack foods by 83%. South Africa acts as a regional trade and investment hub; it is the major source of imports and investment related to these products into other SADC countries. At the same time, imports of processed foods and soft drinks from outside the region - largely from Asia and the Middle East - are increasing at a dramatic rate with soft drink imports growing by almost 1,200% and processed snack foods by 750%. There is significant intra-regional trade in products associated with the nutrition transition; however, growing extra-regional trade means that countries face new pressures in implementing strong policies to prevent the increasing burden of diet-related NCDs. Implementation of a regional nutrition policy framework could complement the SADC's ongoing commitment to regional trade policy.

  3. Acceleration region of the slow solar wind in corona

    NASA Astrophysics Data System (ADS)

    Abbo, L.; Antonucci, E.; Mikić, Z.; Riley, P.; Dodero, M. A.; Giordano, S.

    We present the results of a study concerning the physical parameters of the plasma of the extended corona in the low-latitude and equatorial regions, in order to investigate the sources of the slow solar wind during the minimum of solar activity. The equatorial streamer belt has been observed with the Ultraviolet Coronagraph Spectrometer (UVCS) onboard SOHO from August 19 to September 1, 1996. The spectroscopic diagnostic technique applied in this study, based on the OVI 1032, 1037 Ålines, allows us to determine both the solar wind velocity and the electron density of the extended corona. The main result of the analysis is the identification of the acceleration region of the slow wind, whose outflow velocity is measured in the range from 1.7 up to 3.5 solar radii.

  4. Detecting stellar-wind bubbles through infrared arcs in H II regions

    NASA Astrophysics Data System (ADS)

    Mackey, Jonathan; Haworth, Thomas J.; Gvaramadze, Vasilii V.; Mohamed, Shazrene; Langer, Norbert; Harries, Tim J.

    2016-02-01

    Mid-infrared arcs of dust emission are often seen near ionizing stars within H II regions. A possible explanations for these arcs is that they could show the outer edges of asymmetric stellar wind bubbles. We use two-dimensional, radiation-hydrodynamics simulations of wind bubbles within H II regions around individual stars to predict the infrared emission properties of the dust within the H II region. We assume that dust and gas are dynamically well-coupled and that dust properties (composition, size distribution) are the same in the H II region as outside it, and that the wind bubble contains no dust. We post-process the simulations to make synthetic intensity maps at infrared wavebands using the torus code. We find that the outer edge of a wind bubble emits brightly at 24 μm through starlight absorbed by dust grains and re-radiated thermally in the infrared. This produces a bright arc of emission for slowly moving stars that have asymmetric wind bubbles, even for cases where there is no bow shock or any corresponding feature in tracers of gas emission. The 24 μm intensity decreases exponentially from the arc with increasing distance from the star because the dust temperature decreases with distance. The size distribution and composition of the dust grains has quantitative but not qualitative effects on our results. Despite the simplifications of our model, we find good qualitative agreement with observations of the H II region RCW 120, and can provide physical explanations for any quantitative differences. Our model produces an infrared arc with the same shape and size as the arc around CD -38°11636 in RCW 120, and with comparable brightness. This suggests that infrared arcs around O stars in H II regions may be revealing the extent of stellar wind bubbles, although we have not excluded other explanations.

  5. Non-Economic Obstacles to Wind Deployment: Issues and Regional Differences (Presentation)

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

    Baring-Gould, I.

    2014-05-01

    This presentation provides an overview of national obstacles to wind deployment, with regional assessments. A special mention of offshore projects and distributed wind projects is provided. Detailed maps examine baseline capacity, military and flight radar, golden and bald eagle habitat, bat habitat, whooping crane habitat, and public lands. Regional deployment challenges are also discussed.

  6. Root region airfoil for wind turbine

    DOEpatents

    Tangler, James L.; Somers, Dan M.

    1995-01-01

    A thick airfoil for the root region of the blade of a wind turbine. The airfoil has a thickness in a range from 24%-26% and a Reynolds number in a range from 1,000,000 to 1,800,000. The airfoil has a maximum lift coefficient of 1.4-1.6 that has minimum sensitivity to roughness effects.

  7. Science 101: What Causes Major Wind Patterns, Such as Trade Winds?

    ERIC Educational Resources Information Center

    Robertson, Bill

    2014-01-01

    A convenient place to begin discussing overall wind patterns on Earth is to explain coastal winds. If you live near the coast (that would be near an ocean) or even near a large lake, you probably know the general pattern of winds there. During the day, breezes tend to blow from the water in toward the land, and at night, this tends to reverse,…

  8. Regional trade and the nutrition transition: opportunities to strengthen NCD prevention policy in the Southern African Development Community

    PubMed Central

    Thow, Anne Marie; Sanders, David; Drury, Eliza; Puoane, Thandi; Chowdhury, Syeda N.; Tsolekile, Lungiswa; Negin, Joel

    2015-01-01

    Background Addressing diet-related non-communicable diseases (NCDs) will require a multisectoral policy approach that includes the food supply and trade, but implementing effective policies has proved challenging. The Southern African Development Community (SADC) has experienced significant trade and economic liberalization over the past decade; at the same time, the nutrition transition has progressed rapidly in the region. This analysis considers the relationship between regional trade liberalization and changes in the food environment associated with poor diets and NCDs, with the aim of identifying feasible and proactive policy responses to support healthy diets. Design Changes in trade and investment policy for the SADC were documented and compared with time-series graphs of import data for soft drinks and snack foods to assess changes in imports and source country in relation to trade and investment liberalization. Our analysis focuses on regional trade flows. Results Diets and the burden of disease in the SADC have changed since the 1990s in parallel with trade and investment liberalization. Imports of soft drinks increased by 76% into SADC countries between 1995 and 2010, and processed snack foods by 83%. South Africa acts as a regional trade and investment hub; it is the major source of imports and investment related to these products into other SADC countries. At the same time, imports of processed foods and soft drinks from outside the region – largely from Asia and the Middle East – are increasing at a dramatic rate with soft drink imports growing by almost 1,200% and processed snack foods by 750%. Conclusions There is significant intra-regional trade in products associated with the nutrition transition; however, growing extra-regional trade means that countries face new pressures in implementing strong policies to prevent the increasing burden of diet-related NCDs. Implementation of a regional nutrition policy framework could complement the SADC

  9. International Trade, Pollution Accumulation and Sustainable Growth: A VAR Estimation from the Pearl River Delta Region

    NASA Astrophysics Data System (ADS)

    Zuo, Hui; Tian, Lu

    2018-03-01

    In order to investigate international trade influence in the regional environment. This paper constructs a vector auto-regression (VAR) model and estimates the equations with the environment and trade data of the Pearl River Delta Region. The major mechanisms to the lag are discussed and the fit simulation of the environmental change by the international impulse is given. The result shows that impulse of pollution-intensive export deteriorates the environment continuously and impulse of such import improves it. These effects on the environment are insignificantly correlated with contemporary regional income but significantly correlative to early-stage trade feature. To a typical trade-dependent economy, both export and import have hysteresis influence in the regional environment. The lagged impulse will change environmental development in the turning point, maximal pollution level and convergence.

  10. Post World War II trends in tropical Pacific surface trades

    NASA Technical Reports Server (NTRS)

    Harrison, D. E.

    1989-01-01

    Multidecadal time series of surface winds from central tropical Pacific islands are used to compute trends in the trade winds between the end of WWII and 1985. Over this period, averaged over the whole region, there is no statistically significant trend in speed or zonal or meridional wind (or pseudostress). However, there is some tendency, within a few degrees of the equator, toward weakening of the easterlies and increased meridional flow toward the equator. Anomalous conditions subsequent to the 1972-73 ENSO event make a considerable contribution to the long-term trends. The period 1974-80 has been noted previously to have been anomalous, and trends over that period are sharply greater than those over the longer records.

  11. Root region airfoil for wind turbine

    DOEpatents

    Tangler, J.L.; Somers, D.M.

    1995-05-23

    A thick airfoil is described for the root region of the blade of a wind turbine. The airfoil has a thickness in a range from 24%--26% and a Reynolds number in a range from 1,000,000 to 1,800,000. The airfoil has a maximum lift coefficient of 1.4--1.6 that has minimum sensitivity to roughness effects. 3 Figs.

  12. Offshore Wind Jobs and Economic Development Impact: Four Regional Scenarios (Presentation)

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

    Tegen, S.

    NREL's Jobs and Economic Development Impact (JEDI) Model for Offshore Wind, is a computer tool for studying the economic impacts of fixed-bottom offshore wind projects in the United States. This presentation provides the results of an analysis of four offshore wind development scenarios in the Southeast Atlantic, Great Lakes, Mid-Atlantic, and Gulf of Mexico regions.

  13. Mapping the Solar Wind from its Source Region into the Outer Corona

    NASA Technical Reports Server (NTRS)

    Esser, Ruth

    1998-01-01

    Knowledge of the radial variation of the plasma conditions in the coronal source region of the solar wind is essential to exploring coronal heating and solar wind acceleration mechanisms. The goal of the present proposal is to determine as many plasma parameters in that region as possible by coordinating different observational techniques, such as Interplanetary Scintillation Observations, spectral line intensity observations, polarization brightness measurements and X-ray observations. The inferred plasma parameters are then used to constrain solar wind models.

  14. Strongly-sheared wind-forced currents in the nearshore regions of the central Southern California Bight

    USGS Publications Warehouse

    Noble, Marlene A.; Rosenberger, Kurt; Robertson, George L.

    2015-01-01

    Contrary to many previous reports, winds do drive currents along the shelf in the central portion of the Southern California Bight (SCB). Winds off Huntington Beach CA are the dominant forcing for currents over the nearshore region of the shelf (water depths less than 20 m). Winds control about 50–70% of the energy in nearshore alongshelf surface currents. The wind-driven current amplitudes are also anomalously high. For a relatively weak 1 dyne/cm2 wind stress, the alongshelf surface current amplitudes in this region can reach 80 cm/s or more. Mid-depth current amplitudes for the same wind stress are around 30–40 cm/s. These wind-driven surface current amplitudes are much larger than previously measured over other nearshore shelf regions, perhaps because this program is one of the few that measured currents within a meter of the surface. The near-bed cross-shelf currents over the nearshore region of the Huntington Beach shelf have an Ekman response to winds in that they upwell (downwell) for down (up) coast winds. This response disappears further offshore. Hence, there is upwelling in the SCB, but it does not occur across the entire shelf. Subthermocline water in the nearshore region that may contain nutrients and plankton move onshore when winds are southeastward, but subthermocline water over the shelf break is not transported to the beach. The currents over the outer shelf are not predominately controlled by winds, consistent with previous reports. Instead, they are mainly driven by cross-shelf pressure gradients that are independent of local wind stress.

  15. Regional modeling of wind erosion in the North West and South West of Iran

    NASA Astrophysics Data System (ADS)

    Mirmousavi, S. H.

    2016-08-01

    About two-thirds of the Iran's area is located in the arid and semiarid region. Lack of soil moisture and vegetation is poor in most areas can lead to soil erosion caused by wind. So that the annual suffered severe damage to large areas of rich soils. Modeling studies of wind erosion in Iran is very low and incomplete. Therefore, this study aimed to wind erosion modeling, taking into three factors: wind speed, vegetation and soil types have been done. Wind erosion sensitivity was modeled using the key factors of soil sensitivity, vegetation cover and wind erodibility as proxies. These factors were first estimated separately by factor sensitivity maps and later combined by fuzzy logic into a regional-scale wind erosion sensitivity map. Large areas were evaluated by using publicly available datasets of remotely sensed vegetation information, soil maps and meteorological data on wind speed. The resulting estimates were verified by field studies and examining the economic losses from wind erosion as compensated by the state insurance company. The spatial resolution of the resulting sensitivity map is suitable for regional applications, as identifying sensitive areas is the foundation for diverse land development control measures and implementing management activities.

  16. [Distribution of Regional Pollution and the Characteristics of Vertical Wind Field in the Pearl River Delta].

    PubMed

    Liu, Jian; Wu, Dui; Fan, Shao-jia

    2015-11-01

    Based on the data of hourly PM2.5 concentration of 56 environmental monitoring stations and 9 cities over the Pearl River Delta (PRD) region, the distributions of PM2.5 pollution in PRD region were analyzed by systematic cluster analysis and correlational analysis. It was found that the regional pollution could be divided into 3 types. The first type was the pollution occurred in Dongguan, Guangzhou, Foshan and Jiangmen (I type), and the second type was the pollution occurred in Zhongshan, Zhuhai, Shenzhen and Huizhou (II type), while the last type was the pollution only occurred in Zhaoqing (III type). During the study period, they occurred 47, 7 and 128 days, respectively. During events of pollution type I, except Zhuhai, Shenzhen and Huizhou, the PM2.5 concentrations of other cities were generally high, while the PM2.5 concentration in whole PRD region was over 50.0 μg x m(-3) during events of pollution type II. The regions with higher PM2.5 concentration was mainly concentrated in Zhaoqing, Guangzhou and Foshan during events of pollution type III. The wind data from 4 wind profile radars located in PRD region was used to study the characteristics of vertical wind field of these 3 pollution types. It was found that the wind profiles of type I and III were similar that low layer and high layer were controlled by the southeast wind and the southwest wind, respectively. For type II, the low layer and high layer were influenced by northerly wind and westerly wind, respectively. Compared with other types, the wind speed and ventilation index of type II. were much higher, and the variation of wind direction at lower-middle-layer was much smaller. When PRD region was influenced by northerly winds, the PM2.5 concentration in the entire PRD region was higher. When PRD region was controlled by southeast wind, the PM2.5 concentrations of I and II areas were relatively lower, while the pollution in III area was relatively heavier.

  17. Trade wind inversion variability, dynamics and future change in Hawai'i

    NASA Astrophysics Data System (ADS)

    Cao, Guangxia

    Using 1979-2003 radiosonde data at Hilo and Lihu'e, Hawai'i, the trade-wind inversion (TWI) is found to occur approximately 82% of the time at each station, with average base heights of 2225 +/- 14.3 m (781.9 +/- 1.4 hPa) for Hilo and 2076 +/- 12.5 m (798.8 +/- 1.2 hPa) for Lihu'e. A Weather Research and Forecast (WRF) meso-scale meteorological simulation suggests that island topography and heating contribute to the lifting of the TWI base at Hilo. Inversion base height has a September maximum and a secondary maximum in April. Frequency of inversion occurrence is significantly higher during winters and lower during summers of El Nino years. During the period of 1979-2003, the inversion frequency of occurrence is on upward trend at Hilo for spring (MAM), summer (JJA), and fall (SON) seasons and at Lihu'e for all seasons and for annual values. Composite analysis shows that patterns of geopotential height (GPH), air temperature, u- and v-wind, omega wind, relative and specific humidity, upward longwave radiation flux, net longwave radiation flux, precipitable water, convective precipitation rate, and total cloud cover significantly respond to the TWI base height. For example, the GPH pattern contains a distinctive Pacific North America Teleconnection (PNA) signature, and the magnitudes of PNA centers over 45°N, 165°W for the difference between none and inversion is over 40 m at 200 hPa and 25 m at 850 hPa. The monthly composites show that months with lower (higher) inversion base height and higher (lower) inversion occurrence frequency are linked with the following characteristics: lower (higher) GPH anomalies centered at 30°N, 160°W, lower (higher) temperature anomalies within 300--700 hPa, stronger (weaker) easterly at low levels and northerly anomaly over Hawai'i, and small upward (downward) vertical wind or rising (sinking) motion north of Hawai'i. Using the above characteristics to study the Community Climate System Model (CCSM) composites leads to the

  18. Ozone peaks associated with a subtropical tropopause fold and with the trade wind inversion: A case study from the airborne campaign TROPOZ II over the Caribbean in winter

    NASA Astrophysics Data System (ADS)

    Gouget, Hervé; Cammas, Jean-Pierre; Marenco, Alain; Rosset, Robert; JonquièRes, Isabelle

    1996-11-01

    Aircraft measurements of ozone, methane, carbon monoxide, relative humidity, and equivalent potential temperature were performed during the TROPOZ II campaign. During the aircraft descent down to Pointe-à-Pitre (16.3°N, 61.5°W), at 2100 UTC on January 12, 1991, two ozone peaks (75 ppb) are observed, one at an altitude of 7.5 km and the other at 3.0 km. A physicochemical interpretation for each ozone peak is proposed in connection with the meteorological context, using radiosounding data, total ozone content from TOMS/NIMBUS 7 and diagnoses issued from analyses by the European Centre for Medium-Range Weather Forecasts, Reading, England. The stratospheric origin of the 7.5-km ozone peak is inferred from negative correlations between ozone and its precursors and from diagnoses based on potential vorticity and ageostrophic circulations depicting the structure of the tropopause fold embedded in the subtropical jet front system. Using an appropriate method to isolate cross- and along-front ageostrophic circulations, we show that much of the observed structure of the tropopause fold can be ascribed to transverse and vertical circulations associated with the irrotational part of the flow. Though the downward extent of the subtropical tropopause fold (400 hPa) is restricted in comparison with typical extratropical tropopause ones (700 hPa), the present results suggest that subtropical tropopause folds may significantly contribute to the global stratosphere-troposphere ozone exchange. The origin of the 3.0-km ozone peak trapped just below the trade wind inversion cannot be ascribed precisely. Analogies with other measurements of dust and aerosols transported over the Atlantic or Pacific in the summer season are discussed. Various possibilities are examined: (1) an earlier stratospheric intrusion event, (2) long-range transport by the trade winds of biomass burning species emitted over West Africa, and (3) fast photochemical ozone formation occurring just below the trade

  19. Potential Economic Impacts from Offshore Wind in the Gulf of Mexico Region (Fact Sheet)

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

    Flores, F.; Keyser, D.; Tegen, S.

    2014-01-01

    Offshore wind is a clean, renewable source of energy and can be an economic driver in the United States. To better understand the employment opportunities and other potential regional economic impacts from offshore wind development, the U.S. Department of Energy (DOE) funded research that focuses on four regions of the country. The studies use multiple scenarios with various local job and domestic manufacturing content assumptions. Each regional study uses the new offshore wind Jobs and Economic Development Impacts (JEDI) model, developed by the National Renewable Energy Laboratory. This fact sheet summarizes the potential economic impacts for the Gulf of Mexicomore » region.« less

  20. Regional frequency analysis to asses wind resource spatial and temporal variations in Washington State

    NASA Astrophysics Data System (ADS)

    Mortuza, M.; Demissie, D.

    2013-12-01

    According to the U.S. Department of Energy's annual wind technologies market report, the wind power capacity in the country grew from 2.5 gigawatts in early 2000 to 60 gigawatts in 2012, making it one of the largest new sources of electric capacity additions in the U.S. in recent years. With over 2.8 gigawatts of current capacity (eighth largest in the nation), Washington State plays a significant role in this rapidly increasing energy resource. To further expand and/or optimize these capacities, assessment of wind resource and its spatial and temporal variations are important. However, since at-site frequency analysis using meteorological data is not adequate for extending wind frequency to locations with no data, longer return period, and heterogeneous topography and surface, a regional frequency analysis based on L-moment method is adopted in this study to estimate regional wind speed patterns and return periods in Washington State using hourly mean wind speed data from 1979 - 2010. The analysis applies the k-means, hierarchical and self-organizing map clustering techniques to explore potential clusters or regions; statistical tests are then applied to identify homogeneous regions and appropriate probability distribution models. The result from the analysis is expected to provide essential knowledge about the areas with potential capacity of constructing wind power plants, which can also be readily extended to assist decisions on their daily operations.

  1. Security region-based small signal stability analysis of power systems with FSIG based wind farm

    NASA Astrophysics Data System (ADS)

    Qin, Chao; Zeng, Yuan; Yang, Yang; Cui, Xiaodan; Xu, Xialing; Li, Yong

    2018-02-01

    Based on the Security Region approach, the impact of fixed-speed induction generator based wind farm on the small signal stability of power systems is analyzed. Firstly, the key factors of wind farm on the small signal stability of power systems are analyzed and the parameter space for small signal stability region is formed. Secondly, the small signal stability region of power systems with wind power is established. Thirdly, the corresponding relation between the boundary of SSSR and the dominant oscillation mode is further studied. Results show that the integration of fixed-speed induction generator based wind farm will cause the low frequency oscillation stability of the power system deteriorate. When the output of wind power is high, the oscillation stability of the power system is mainly concerned with the inter-area oscillation mode caused by the integration of the wind farm. Both the active power output and the capacity of reactive power compensation of the wind farm have a significant influence on the SSSR. To improve the oscillation stability of power systems with wind power, it is suggested to reasonably set the reactive power compensation capacity for the wind farm through SSSR.

  2. Wind energy potential assessment to estimate performance of selected wind turbine in northern coastal region of Semarang-Indonesia

    NASA Astrophysics Data System (ADS)

    Premono, B. S.; Tjahjana, D. D. D. P.; Hadi, S.

    2017-01-01

    The aims of this paper are to investigate the characteristic of the wind speed and wind energy potential in the northern coastal region of Semarang, Central Java, Indonesia. The wind data was gained from Meteorological Station of Semarang, with ten-min average time series wind data for one year period, at the height of 10 m. Weibull distribution has been used to determine the wind power density and wind energy density of the site. It was shown that the value of the two parameters, shape parameter k, and scale parameter c, were 3.37 and 5.61 m/s, respectively. The annual mean wind speed and wind speed carrying the maximum energy were 5.32 m/s and 6.45 m/s, respectively. Further, the annual energy density at the site was found at a value of 103.87 W/m2, and based on Pacific North-west Laboratory (PNL) wind power classification, at the height of 10 m, the value of annual energy density is classified into class 2. The commercial wind turbine is chosen to simulate the wind energy potential of the site. The POLARIS P25-100 is most suitable to the site. It has the capacity factor 29.79% and can produce energy 261 MWh/year.

  3. Trading Tradition. Issues Arising from an Evaluation of the Experiences of Female Apprentices in Male-Dominated Trades in the Hunter Region of New South Wales. Summary.

    ERIC Educational Resources Information Center

    Moran, Patricia; And Others

    A study examined the measures taken in seven colleges in the Hunter Region of New South Wales to promote the entry of women into nontraditional trades. Questionnaires were given to all female apprentices in nontraditional trades and a random sample of male apprentices in the same trades in 1983; all female apprentices who withdrew from training in…

  4. Resolving the Hα-emitting Region in the Wind of η Carinae

    NASA Astrophysics Data System (ADS)

    Wu, Ya-Lin; Smith, Nathan; Close, Laird M.; Males, Jared R.; Morzinski, Katie M.

    2017-05-01

    The massive evolved star η Carinae is the most luminous star in the Milky Way and has the highest steady wind mass-loss rate of any known star. Radiative transfer models of the spectrum by Hillier et al. predict that Hα is mostly emitted in regions of the wind at radii of 6-60 au from the star (2.5-25 mas at 2.35 kpc). We present diffraction-limited images (FWHM ˜ 25 mas) with Magellan adaptive optics in two epochs, showing that η Carinae consistently appears ˜2.5-3 mas wider in Hα emission compared to the adjacent 643 nm continuum. This implies that the Hα line-forming region may have a characteristic emitting radius of 12 mas or ˜30 au, in very good agreement with the Hillier stellar-wind model. This provides direct confirmation that the physical wind parameters of that model are roughly correct, including the mass-loss rate of \\dot{M}={10}-3 {M}⊙ {{yr}}-1, plus the clumping factor, and the terminal velocity. Comparison of the Hα images (ellipticity and PA) to the continuum images reveals no significant asymmetries at Hα. Hence, any asymmetry induced by a companion or by the primary’s rotation do not strongly influence the global Hα emission in the outer wind.

  5. 76 FR 58774 - Trade Mission to Southeast Asia in Conjunction With Trade Winds-Asia

    Federal Register 2010, 2011, 2012, 2013, 2014

    2011-09-22

    ... trade mission stop in either: Malaysia (Kuala Lumpur) or Indonesia (Jakarta). Each trade mission stop... cross section of industries with growth potential in Singapore, Vietnam, Thailand, Malaysia and... equipment, safety and security equipment, automotive parts and service equipment, and logistics and...

  6. Wind utilization in remote regions: An economic study. [for comparison with diesel engines

    NASA Technical Reports Server (NTRS)

    Vansant, J. H.

    1973-01-01

    A wind driven generator was considered as a supplement to a diesel group, for the purpose of economizing fuel when wind power is available. A specific location on Hudson's Bay, Povognituk, was selected. Technical and economic data available for a wind machine of 10-kilowatt nominal capacity and available wind data for that region were used for the study. After subtracting the yearly wind machine costs from savings in fuel costs, a net savings of $1400 per year is realized. These values are approximate, but are though to be highly conservative.

  7. Wintertime slope winds and its turbulent characteristics in the Yeongdong region of Korea

    NASA Astrophysics Data System (ADS)

    Jeon, H. R.; Eun, S. H.; Kim, B. G.; Lee, Y. H.

    2015-12-01

    The Yeongdong region has various meteorological phenomenons by virtue of complicated geographical characteristics with high Taebaek Mountains running from the north to the south and an adjacent East Sea to the east. There are few studies on the slope winds and its turbulent characteristics over the complex terrain, which are critical information in mountain climbing, hiking, paragliding, even winter sports such as alpine skiing and ski jump etc. For the understanding of diverse mountain winds in the complex terrain in Yeongdong, hot-wire anemometers (Campbell Scientific) have been installed at a couple of sites since October 2014 and several automatic weather stations at several sites around the mountainous region in Yeongdong since November 2012.WRF model simulations have been also done with an ultra-fine horizontal resolution of 300 m for 10 years. Generally, model and observation show that the dominant wind is westerly, approximately more than 75%. It is quite consistent that wind fields from both model and observation agree with each other in the valley region and at the top of the mountain, but there is a significant disagreement in wind direction specifically in the slide slope. Probably this implies model's performance with even an ultra-fine resolution is still not enough for the slide slope domain of complex terrains. Despite that, the observation clearly showed up- and down slope winds for the weak synoptic conditions carefully selected such as strong insolation and a synoptic wind less than 5m/s in the 850 hPa. The up- and down slope flows are also demonstrated in the snow-covered condition as well as grass ground. Further, planar fit transformation algorithm against the coordinate tilt has been applied to raw wind data (10Hz) of the slope site for the analysis of turbulence properties. Turbulence also increases with synoptic wind strength. Detailed analysis of mechanical turbulence and buoyance will be discussed for different surface properties (grass

  8. Implications of the cattle trade network in Cameroon for regional disease prevention and control

    PubMed Central

    Motta, Paolo; Porphyre, Thibaud; Handel, Ian; Hamman, Saidou M.; Ngu Ngwa, Victor; Tanya, Vincent; Morgan, Kenton; Christley, Rob; Bronsvoort, Barend M. deC.

    2017-01-01

    Movement of live animals is a major risk factor for the spread of livestock diseases and zoonotic infections. Understanding contact patterns is key to informing cost-effective surveillance and control strategies. In West and Central Africa some of the most rapid urbanization globally is expected to increase the demand for animal-source foods and the need for safer and more efficient animal production. Livestock trading points represent a strategic contact node in the dissemination of multiple pathogens. From October 2014 to May 2015 official transaction records were collected and a questionnaire-based survey was carried out in cattle markets throughout Western and Central-Northern Cameroon. The data were used to analyse the cattle trade network including a total of 127 livestock markets within Cameroon and five neighboring countries. This study explores for the first time the influence of animal trade on infectious disease spread in the region. The investigations showed that national borders do not present a barrier against pathogen dissemination and that non-neighbouring countries are epidemiologically connected, highlighting the importance of a regional approach to disease surveillance, prevention and control. Furthermore, these findings provide evidence for the benefit of strategic risk-based approaches for disease monitoring, surveillance and control, as well as for communication and training purposes through targeting key regions, highly connected livestock markets and central trading links. PMID:28266589

  9. Implications of the cattle trade network in Cameroon for regional disease prevention and control

    NASA Astrophysics Data System (ADS)

    Motta, Paolo; Porphyre, Thibaud; Handel, Ian; Hamman, Saidou M.; Ngu Ngwa, Victor; Tanya, Vincent; Morgan, Kenton; Christley, Rob; Bronsvoort, Barend M. Dec.

    2017-03-01

    Movement of live animals is a major risk factor for the spread of livestock diseases and zoonotic infections. Understanding contact patterns is key to informing cost-effective surveillance and control strategies. In West and Central Africa some of the most rapid urbanization globally is expected to increase the demand for animal-source foods and the need for safer and more efficient animal production. Livestock trading points represent a strategic contact node in the dissemination of multiple pathogens. From October 2014 to May 2015 official transaction records were collected and a questionnaire-based survey was carried out in cattle markets throughout Western and Central-Northern Cameroon. The data were used to analyse the cattle trade network including a total of 127 livestock markets within Cameroon and five neighboring countries. This study explores for the first time the influence of animal trade on infectious disease spread in the region. The investigations showed that national borders do not present a barrier against pathogen dissemination and that non-neighbouring countries are epidemiologically connected, highlighting the importance of a regional approach to disease surveillance, prevention and control. Furthermore, these findings provide evidence for the benefit of strategic risk-based approaches for disease monitoring, surveillance and control, as well as for communication and training purposes through targeting key regions, highly connected livestock markets and central trading links.

  10. Best Practices for Wind Energy Development in the Great Lakes Region

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

    Pebbles, Victoria; Hummer, John; Haven, Celia

    2011-07-19

    This report offers a menu of 18 different, yet complementary, preferred practices and policies. The best practices cover all phases of the wind energy development process - from the policies that allow for wind development, to the sustainable operation of a wind project, to the best practices for decommissioning a spent turbine - including applications for offshore wind. Each best practice describes the opportunities and challenges (pros and cons), and offers a case example that illustrates how that best practice is being utilized by a particular jurisdiction or wind project. The practices described in this publication were selected by amore » diverse group of interests from the Great Lakes Wind Collaborative that included environmental groups, industry, academia, and federal, state and local government regulators. The practices were identified through a year-long process that included a literature review, online survey and interviews with individuals from the public, private and non-profit sectors. Optimally, a suite of these best practices would be applied in an appropriate combination to fit the conditions of a particular wind project or a set of wind projects within a given locality or region.« less

  11. Adaptive Control of a Utility-Scale Wind Turbine Operating in Region 3

    NASA Technical Reports Server (NTRS)

    Frost, Susan A.; Balas, Mark J.; Wright, Alan D.

    2009-01-01

    Adaptive control techniques are well suited to nonlinear applications, such as wind turbines, which are difficult to accurately model and which have effects from poorly known operating environments. The turbulent and unpredictable conditions in which wind turbines operate create many challenges for their operation. In this paper, we design an adaptive collective pitch controller for a high-fidelity simulation of a utility scale, variable-speed horizontal axis wind turbine. The objective of the adaptive pitch controller in Region 3 is to regulate generator speed and reject step disturbances. The control objective is accomplished by collectively pitching the turbine blades. We use an extension of the Direct Model Reference Adaptive Control (DMRAC) approach to track a reference point and to reject persistent disturbances. The turbine simulation models the Controls Advanced Research Turbine (CART) of the National Renewable Energy Laboratory in Golden, Colorado. The CART is a utility-scale wind turbine which has a well-developed and extensively verified simulator. The adaptive collective pitch controller for Region 3 was compared in simulations with a bas celliansesical Proportional Integrator (PI) collective pitch controller. In the simulations, the adaptive pitch controller showed improved speed regulation in Region 3 when compared with the baseline PI pitch controller and it demonstrated robustness to modeling errors.

  12. Transient behavior of flare-associated solar wind. II - Gas dynamics in a nonradial open field region

    NASA Technical Reports Server (NTRS)

    Nagai, F.

    1984-01-01

    Transient behavior of flare-associated solar wind in the nonradial open field region is numerically investigated, taking into account the thermal and dynamical coupling between the chromosphere and the corona. A realistic steady solar wind is constructed which passes through the inner X-type critical point in the rapidly diverging region. The wind speed shows a local maximum at the middle, O-type, critical point. The wind's density and pressure distributions decrease abruptly in the rapidly diverging region of the flow tube. The transient behavior of the wind following flare energy deposition includes ascending and descending conduction fronts. Thermal instability occurs in the lower corona, and ascending material flows out through the throat after the flare energy input ceases. A local density distribution peak is generated at the shock front due to the pressure deficit just behind the shock front.

  13. Seasonal variability in winds in the north polar region of Mars

    NASA Astrophysics Data System (ADS)

    Smith, Isaac B.; Spiga, Aymeric

    2018-07-01

    Surface features near Mars' polar regions are very active, suggesting that they are among the most dynamic places on the planet. Much of that activity is driven by seasonal winds that strongly influence the distribution of water ice and other particulates. Morphologic features such as the spiral troughs, Chasma Boreale, and prominent circumpolar dune fields have experienced persistent winds for several Myr. Therefore, detailing the pattern of winds throughout the year is an important step to understanding what processes affect the martian surface in contemporary and past epochs. In this study, we provide polar-focused mesoscale simulations from northern spring to summer to understand variability from the diurnal to the seasonal scales. We find that there is a strong seasonality to the diurnal surface wind speeds driven primarily by the retreat of the seasonal CO2 until about summer solstice, when the CO2 is gone. The fastest winds are found when the CO2 cap boundary is on the slopes of the north polar layered deposits, providing a strong thermal gradient that enhances the season-long katabatic effect. Mid-summer winds, while not as fast as spring winds, may play a role in dune migration for some dune fields. Late summer wind speeds pick up as the seasonal cap returns.

  14. Gap winds and their effects on regional oceanography Part II: Kodiak Island, Alaska

    NASA Astrophysics Data System (ADS)

    Ladd, Carol; Cheng, Wei; Salo, Sigrid

    2016-10-01

    Frequent gap winds, defined here as offshore-directed flow channeled through mountain gaps, have been observed near Kodiak Island in the Gulf of Alaska (GOA). Gap winds from the Iliamna Lake gap were investigated using QuikSCAT wind data. The influence of these wind events on the regional ocean was examined using satellite and in situ data combined with Regional Ocean Modeling System (ROMS) model runs. Gap winds influence the entire shelf width (> 200 km) northeast of Kodiak Island and extend an additional 150 km off-shelf. Due to strong gradients in the along-shelf direction, they can result in vertical velocities in the ocean of over 20 m d-1 due to Ekman pumping. The wind events also disrupt flow of the Alaska Coastal Current (ACC), resulting in decreased flow down Shelikof Strait and increased velocities on the outer shelf. This disruption of the ACC has implications for freshwater transport into the Bering Sea. The oceanographic response to gap winds may influence the survival of larval fishes as Arrowtooth Flounder recruitment is negatively correlated with the interannual frequency of gap-wind events, and Pacific Cod recruitment is positively correlated. The frequency of offshore directed winds exhibits a strong seasonal cycle averaging 7 days per month during winter and 2 days per month during summer. Interannual variability is correlated with the Pacific North America Index and shows a linear trend, increasing by 1.35 days per year. An accompanying paper discusses part I of our study (Ladd and Cheng, 2016) focusing on gap-wind events flowing out of Cross Sound in the eastern GOA.

  15. Wind Patterns in Jupiter's Equatorial Region (Time set 1)

    NASA Technical Reports Server (NTRS)

    1997-01-01

    Wind patterns of Jupiter's equatorial region. This mosaic covers an area of 34,000 kilometers by 22,000 kilometers and was taken using the 756 nanometer (nm) near-infrared continuum filter. The dark region near the center of the mosaic is an equatorial 'hotspot' similar to the Galileo Probe entry site. The near-infrared continuum filter shows the features of Jupiter's main visible cloud deck.

    Jupiter's atmospheric circulation is dominated by alternating jets of east/west (zonal) winds. The bands have different widths and wind speeds but have remained constant as long as telescopes and spacecraft have measured them. The top half of these mosaics lies within Jupiter's North Equatorial Belt, a westward (left) current. The bottom half shows part of the Equatorial Zone, a fast moving eastward current. The clouds near the hotspot are the fastest moving features in these mosaics, moving at about 100 meters per second, or 224 miles per hour.

    Superimposed on the zonal wind currents is the Jovian 'weather'. The arrows show the winds measured by an observer moving eastward (right) at the speed of the hotspot. (The observer's perspective is that the hotspot is 'still' while the rest of the planet moves around it.) Clouds south of the hotspot appear to be moving towards it, as seen in the flow aligned with cloud streaks to the southwest and in the clockwise flow to the southeast. Interestingly, there is little cloud motion away from the hotspot in any direction. This is consistent with the idea that dry air is converging over this region and sinking, maintaining the cloud-free nature of the hotspot.

    North is at the top. The mosaic covers latitudes 1 to 19 degrees and is centered at longitude 336 degrees West. The smallest resolved features are tens of kilometers in size. These images were taken on December 17, 1996, at a range of 1.5 million kilometers by the Solid State Imaging system aboard NASA's Galileo spacecraft.

    The Jet Propulsion Laboratory, Pasadena, CA

  16. Wind-Related Topography in Phoenix's Region of Mars (Animation)

    NASA Technical Reports Server (NTRS)

    2008-01-01

    [figure removed for brevity, see original site] Click on image for animation

    This movie shifts from a global zoom indicating the Phoenix landing area on Mars to a topographical map indicating relative elevations in the landing region. The elevations could affect wind patterns at the site.

    In particular, Phoenix is in a broad, shallow valley. The edge of the valley, about 150 meters (500 feet) above the floor, may provide enough of a slope to the east of Phoenix to explain winds coming from the east during nights at the site. Cooler, denser air could be sinking down the slope and toward the lander.

    Atmospheric scientists on the Phoenix team are analyzing wind patterns to distiguish effects of nearby topography from larger-scale movement of the atmosphere in the polar region.

    The elevation information for this topographical mapping comes from the Mars Orbiter Laser Altimeter on NASA's Mars Global Surveyor orbiter. The blue-coded area is the valley floor. Orange and yellow indicate relatively higher elevations.

    The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver. JPL managed the Mars Global Surveyor mission for the NASA Science Mission Directorate.

  17. Advanced wind turbine design

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

    Jamieson, P.M.; Jaffrey, A.

    1995-09-01

    Garrad Hassan have a project in progress funded by the UK Department of Trade and Industry (DTI) to assess the prospects and cost benefits of advanced wind turbine design. In the course of this work, a new concept, the coned rotor design, has been developed. This enables a wind turbine system to operate in effect with variable rotor diameter augmenting energy capture in light winds and shedding loads in storm conditions. Comparisons with conventional design suggest that a major benefit in reduced cost of wind generated electricity may be possible.

  18. Advanced wind turbine design

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

    Jamieson, P.M.; Jaffrey, A.

    1997-11-01

    Garrad Hassan have a project in progress funded by the U.K. Department of Trade and Industry (DTI) to assess the prospects and cost benefits of advanced wind turbine design. In the course of this work, a new concept, the coned rotor design, has been developed. This enables a wind turbine system to operate in effect with variable rotor diameter augmenting energy capture in light winds and shedding loads in storm conditions. Comparisons with conventional design suggest that a major benefit in reduced cost of wind-generated electricity may be possible.

  19. Strategic trade between two regions with partial local consumer protection - General setup and nash equilibria

    NASA Astrophysics Data System (ADS)

    Iordanov, Iordan V.; Vassilev, Andrey A.

    2017-12-01

    We construct a model of the trade relations between two regions for the case when the trading entities (consumers) compete for a scarce good and there is an element of strategic interdependence in the trading process. Additionally, local consumers enjoy partial protection in the form of guaranteed access to a part of the locally-supplied quantity of the good. The model is formulated for the general asymmetric case, where the two regions differ in terms of parameters such as income, size of the local market supply, degree of protection and transportation costs. For this general model we establish the existence of Nash equilibria and obtain their form as a function of the model parameters, producing a typology of the equilibria. This is a required step in order to rigorously study various types of price dynamics for the model.

  20. Modified Adaptive Control for Region 3 Operation in the Presence of Wind Turbine Structural Modes

    NASA Technical Reports Server (NTRS)

    Frost, Susan Alane; Balas, Mark J.; Wright, Alan D.

    2010-01-01

    Many challenges exist for the operation of wind turbines in an efficient manner that is reliable and avoids component fatigue and failure. Turbines operate in highly turbulent environments resulting in aerodynamic loads that can easily excite turbine structural modes, possibly causing component fatigue and failure. Wind turbine manufacturers are highly motivated to reduce component fatigue and failure that can lead to loss of revenue due to turbine down time and maintenance costs. The trend in wind turbine design is toward larger, more flexible turbines that are ideally suited to adaptive control methods due to the complexity and expense required to create accurate models of their dynamic characteristics. In this paper, we design an adaptive collective pitch controller for a high-fidelity simulation of a utility-scale, variable-speed horizontal axis wind turbine operating in Region 3. The objective of the adaptive pitch controller is to regulate generator speed, accommodate wind gusts, and reduce the excitation of structural modes in the wind turbine. The control objective is accomplished by collectively pitching the turbine blades. The adaptive collective pitch controller for Region 3 was compared in simulations with a baseline classical Proportional Integrator (PI) collective pitch controller. The adaptive controller will demonstrate the ability to regulate generator speed in Region 3, while accommodating gusts, and reducing the excitation of certain structural modes in the wind turbine.

  1. On the Role of Hyper-arid Regions within the Virtual Water Trade Network

    NASA Astrophysics Data System (ADS)

    Aggrey, James; Alshamsi, Aamena; Molini, Annalisa

    2016-04-01

    Climate change, economic development, and population growth are bound to increasingly impact global water resources, posing a significant threat to the sustainable development of arid regions, where water consumption highly exceeds the natural carrying capacity, population growth rate is high, and climate variability is going to impact both water consumption and availability. Virtual Water Trade (VWT) - i.e. the international trade network of water-intensive products - has been proposed as a possible solution to optimize the allocation of water resources on the global scale. By increasing food availability and lowering food prices it may in fact help the rapid development of water-scarce regions. The structure of the VWT network has been analyzed by a number of authors both in connection with trade policies, socioeconomic constrains and agricultural efficiency. However a systematic analysis of the structure and the dynamics of the VWT network conditional to aridity, climatic forcing and energy availability, is still missing. Our goal is hence to analyze the role of arid and hyper-arid regions within the VWN under diverse climatic, demographic, and energy constraints with an aim to contribute to the ongoing Energy-Water-Food nexus discussion. In particular, we focus on the hyper-arid lands of the Arabian Peninsula, the role they play in the global network and the assessment of their specific criticalities, as reflected in the VWN resilience.

  2. Modeling wind energy potential in a data-poor region: A geographic information systems model for Iraq

    NASA Astrophysics Data System (ADS)

    Khayyat, Abdulkareem Hawta Abdullah Kak Ahmed

    Scope and Method of Study: Most developing countries, including Iraq, have very poor wind data. Existing wind speed measurements of poor quality may therefore be a poor guide to where to look for the best wind resources. The main focus of this study is to examine how effectively a GIS spatial model estimates wind power potential in regions where high-quality wind data are very scarce, such as Iraq. The research used a mixture of monthly and hourly wind data from 39 meteorological stations. The study applied spatial analysis statistics and GIS techniques in modeling wind power potential. The model weighted important human, environmental and geographic factors that impact wind turbine siting, such as roughness length, land use⪉nd cover type, airport locations, road access, transmission lines, slope and aspect. Findings and Conclusions: The GIS model provided estimations for wind speed and wind power density and identified suitable areas for wind power projects. Using a high resolution (30*30m) digital elevation model DEM improved the GIS wind suitability model. The model identified areas suitable for wind farm development on different scales. The model showed that there are many locations available for large-scale wind turbines in the southern part of Iraq. Additionally, there are many places in central and northern parts (Kurdistan Region) for smaller scale wind turbine placement.

  3. Wind energy development in the United States: Can state-level policies promote efficient development of wind energy capacity?

    NASA Astrophysics Data System (ADS)

    Goldstein, Blair S.

    In the absence of strong U.S. federal renewable energy policies, state governments have taken the lead in passing legislation to promote wind energy. Studies have shown that many of these policies, including Renewable Portfolio Standards (RPS), have aided in the development of wind energy capacity nationwide. This paper seeks to analyze whether these state-level policies have led to an efficient development of U.S. wind energy. For the purposes of this paper, wind energy development is considered efficient if competitive markets enable wind capacity to be built in the most cost effective manner, allowing states to trade wind energy between high wind potential states and low wind potential states. This concept is operationalized by analyzing how state policies that incentivize the in-state development of wind energy impact where wind capacity is developed. A multivariate regression model examining wind capacity in the 48 contiguous United States that had some wind capacity between 1999 and 2008 found these in-state policies are associated with increased wind capacity, controlling for states' wind potential. The results suggest that state-level policies are distorting where wind is developed. These findings support the enactment of a more comprehensive federal energy policy, such as a national RPS, a cap-and-trade program, or a targeted federal transmission policy. These federal policies could spur national markets that would result in the more efficient development of U.S. wind energy.

  4. He II lambda-4686 in Eta Carinae: Collapse of the Wind-Wind Collision Region During Periastron Passage

    NASA Technical Reports Server (NTRS)

    Teodoro, M.; Damineli, A.; Arias, J. I.; DeAraujo, F. X.; Barba, R. H.; Corcoran, M. F.; Fernandes, M. Borges; Fernandez-Lajus, E.; Fraga, L.; Gamen, R. C.; hide

    2012-01-01

    The periodic spectroscopic events in Eta Carinae are now well established and occur near the periastron passage of two massive stars in a very eccentric orbit. Several mechanisms have been proposed to explain the variations of different spectral features, such as an eclipse by the wind-wind collision boundary, a shell ejection from the primary star or accretion of its wind onto the secondary. All of them have problems explaining all the observed phenomena. To better understand the nature of the cyclic events we performed a dense monitoring of Eta Carinae with 5 Southern telescopes during the 2009 low excitation event, resulting in a set of data of unprecedented quality and sampling. The intrinsic luminosity of the He II lambda-4686 emission line (L approx 310 solar L) just before periastron reveals the presence of a very luminous transient source of extreme UV radiation emitted in the wind-wind collision (WWC) region. Clumps in the primary's wind probably explain the flare-like behavior of both the X-ray and He II lambda-4686 light-curves. After a short-lived minimum, He II lambda-4686 emission rises again to a new maximum, when X-rays are still absent or very weak. We interpret this as a collapse of the WWC onto the "surface" of the secondary star, switching off the hard X-ray source and diminishing the WWC shock cone. The recovery from this state is controlled by the momentum balance between the secondary's wind and the clumps in the primary's wind.

  5. Regional climate model simulations indicate limited climatic impacts by operational and planned European wind farms.

    PubMed

    Vautard, Robert; Thais, Françoise; Tobin, Isabelle; Bréon, François-Marie; Devezeaux de Lavergne, Jean-Guy; Colette, Augustin; Yiou, Pascal; Ruti, Paolo Michele

    2014-01-01

    The rapid development of wind energy has raised concerns about environmental impacts. Temperature changes are found in the vicinity of wind farms and previous simulations have suggested that large-scale wind farms could alter regional climate. However, assessments of the effects of realistic wind power development scenarios at the scale of a continent are missing. Here we simulate the impacts of current and near-future wind energy production according to European Union energy and climate policies. We use a regional climate model describing the interactions between turbines and the atmosphere, and find limited impacts. A statistically significant signal is only found in winter, with changes within ±0.3 °C and within 0-5% for precipitation. It results from the combination of local wind farm effects and changes due to a weak, but robust, anticyclonic-induced circulation over Europe. However, the impacts remain much weaker than the natural climate interannual variability and changes expected from greenhouse gas emissions.

  6. Microphysical, Macrophysical and Radiative Signatures of Volcanic Aerosols in Trade Wind Cumulus Observed by the A-Train

    NASA Technical Reports Server (NTRS)

    Yuan, T.; Remer, L. A.; Yu, H.

    2011-01-01

    Increased aerosol concentrations can raise planetary albedo not only by reflecting sunlight and increasing cloud albedo, but also by changing cloud amount. However, detecting aerosol effect on cloud amount has been elusive to both observations and modeling due to potential buffering mechanisms and convolution of meteorology. Here through a natural experiment provided by long-tem1 degassing of a low-lying volcano and use of A-Train satellite observations, we show modifications of trade cumulus cloud fields including decreased droplet size, decreased precipitation efficiency and increased cloud amount are associated with volcanic aerosols. In addition we find significantly higher cloud tops for polluted clouds. We demonstrate that the observed microphysical and macrophysical changes cannot be explained by synoptic meteorology or the orographic effect of the Hawaiian Islands. The "total shortwave aerosol forcin", resulting from direct and indirect forcings including both cloud albedo and cloud amount. is almost an order of magnitude higher than aerosol direct forcing alone. Furthermore, the precipitation reduction associated with enhanced aerosol leads to large changes in the energetics of air-sea exchange and trade wind boundary layer. Our results represent the first observational evidence of large-scale increase of cloud amount due to aerosols in a trade cumulus regime, which can be used to constrain the representation of aerosol-cloud interactions in climate models. The findings also have implications for volcano-climate interactions and climate mitigation research.

  7. Offshore Wind Jobs and Economic Development Impacts in the United States: Four Regional Scenarios

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

    Tegen, S.; Keyser, D.; Flores-Espino, F.

    This report uses the offshore wind Jobs and Economic Development Impacts (JEDI) model and provides four case studies of potential offshore deployment scenarios in different regions of the United States: the Southeast, the Great Lakes, the Gulf Coast, and the Mid-Atlantic. Researchers worked with developers and industry representatives in each region to create potential offshore wind deployment and supply chain growth scenarios, specific to their locations. These scenarios were used as inputs into the offshore JEDI model to estimate jobs and other gross economic impacts in each region.

  8. Exploration of Solar Wind Acceleration Region Using Interplanetary Scintillation of Water Vapor Maser Source and Quasars

    NASA Technical Reports Server (NTRS)

    Tokumaru, Munetoshi; Yamauchi, Yohei; Kondo, Tetsuro

    2001-01-01

    Single-station observations of interplanetary scintillation UPS) at three microwave frequencies 2, 8, and 22GHz, were carried out between 1989 and 1998 using a large (34-micro farad) radio telescope at the Kashima Space Research Center of the Communications Research Laboratory. The aim of these observations was to explore the near-sun solar wind, which is the key region for the study of the solar wind acceleration mechanism. Strong quasars, 3C279 and 3C273B, were used for the Kashima IPS observations at 2 and 8GHz, and a water-vapor maser source, IRC20431, was used for the IPS observations at 22GHz. Solar wind speeds derived from Kashima IPS data suggest that the solar wind acceleration takes place at radial distances between 10 and 30 solar radii (Rs) from the sun. The properties of the turbulence spectrum (e.g. anisotropy, spectral index, inner scale) inferred from the Kashima data were found to change systematically in the solar wind acceleration region. While the solar wind in the maximum phase appears to be dominated by the slow wind, fast and rarefied winds associated with the coronal holes were found to develop significantly at high latitudes as the solar activity declined. Nevertheless, the Kashima data suggests that the location of the acceleration region is stable throughout the solar cycle.

  9. Exploration of Solar Wind Acceleration Region Using Interplanetary Scintillation of Water Vapor Maser Source and Quasars

    NASA Technical Reports Server (NTRS)

    Tokumaru, Munetoshi; Yamauchi, Yohei; Kondo, Tetsuro

    2001-01-01

    Single-station observations of interplanetary scintillation (IPS) at three microwave frequencies; 2 GHz, 8 GHz and 22 GHz have been carried out between 1989 and 1998 using a large (34 m farad) radio telescope at the Kashima Space Research Center of the Communications Research Laboratory. The aim of these observations is to explore the near-sun solar wind, which is the key region for the study of the solar wind acceleration mechanism. Strong quasars; 3C279 and 3C273B were used for Kashima IPS observations at 2 GHz and 8 GHz, and a water vapor maser source, IRC20431 was used for the IPS observations at 22 GHz. Solar wind velocities derived from Kashima IPS data suggest that the solar wind acceleration takes place at radial distances between 10 and 30 solar radii (R(sub s)) from the sun. Properties of the turbulence spectrum (e.g. anisotropy, spectral index, inner scale) inferred from Kashima data are found to change systematically in the solar wind acceleration region. While the solar wind in the maximum phase appears to be dominated by the slow wind, fast and rarefied winds associated with coronal holes are found to develop significantly at high latitudes as the solar activity declines. Nevertheless, Kashima data suggests that the location of the acceleration region is stable throughout the solar cycle.

  10. An Anomalous Composition in Slow Solar Wind as a Signature of Magnetic Reconnection in its Source Region

    NASA Astrophysics Data System (ADS)

    Zhao, L.; Landi, E.; Lepri, S. T.; Kocher, M.; Zurbuchen, T. H.; Fisk, L. A.; Raines, J. M.

    2017-01-01

    In this paper, we study a subset of slow solar winds characterized by an anomalous charge state composition and ion temperatures compared to average solar wind distributions, and thus referred to as an “Outlier” wind. We find that although this wind is slower and denser than normal slow wind, it is accelerated from the same source regions (active regions and quiet-Sun regions) as the latter and its occurrence rate depends on the solar cycle. The defining property of the Outlier wind is that its charge state composition is the same as that of normal slow wind, with the only exception being a very large decrease in the abundance of fully charged species (He2+, C6+, N7+, O8+, Mg12+), resulting in a significant depletion of the He and C element abundances. Based on these observations, we suggest three possible scenarios for the origin of this wind: (1) local magnetic waves preferentially accelerating non-fully stripped ions over fully stripped ions from a loop opened by reconnection; (2) depleted fully stripped ions already contained in the corona magnetic loops before they are opened up by reconnection; or (3) fully stripped ions depleted by Coulomb collision after magnetic reconnection in the solar corona. If any one of these three scenarios is confirmed, the Outlier wind represents a direct signature of slow wind release through magnetic reconnection.

  11. Evaluating the effects of climate change on US agricultural systems: sensitivity to regional impact and trade expansion scenarios

    NASA Astrophysics Data System (ADS)

    Baker, Justin S.; Havlík, Petr; Beach, Robert; Leclère, David; Schmid, Erwin; Valin, Hugo; Cole, Jefferson; Creason, Jared; Ohrel, Sara; McFarland, James

    2018-06-01

    Agriculture is one of the sectors that is expected to be most significantly impacted by climate change. There has been considerable interest in assessing these impacts and many recent studies investigating agricultural impacts for individual countries and regions using an array of models. However, the great majority of existing studies explore impacts on a country or region of interest without explicitly accounting for impacts on the rest of the world. This approach can bias the results of impact assessments for agriculture given the importance of global trade in this sector. Due to potential impacts on relative competitiveness, international trade, global supply, and prices, the net impacts of climate change on the agricultural sector in each region depend not only on productivity impacts within that region, but on how climate change impacts agricultural productivity throughout the world. In this study, we apply a global model of agriculture and forestry to evaluate climate change impacts on US agriculture with and without accounting for climate change impacts in the rest of the world. In addition, we examine scenarios where trade is expanded to explore the implications for regional allocation of production, trade volumes, and prices. To our knowledge, this is one of the only attempts to explicitly quantify the relative importance of accounting for global climate change when conducting regional assessments of climate change impacts. The results of our analyses reveal substantial differences in estimated impacts on the US agricultural sector when accounting for global impacts vs. US-only impacts, particularly for commodities where the United States has a smaller share of global production. In addition, we find that freer trade can play an important role in helping to buffer regional productivity shocks.

  12. Methane mole fraction and δ13C above and below the trade wind inversion at Ascension Island in air sampled by aerial robotics

    NASA Astrophysics Data System (ADS)

    Brownlow, R.; Lowry, D.; Thomas, R. M.; Fisher, R. E.; France, J. L.; Cain, M.; Richardson, T. S.; Greatwood, C.; Freer, J.; Pyle, J. A.; MacKenzie, A. R.; Nisbet, E. G.

    2016-11-01

    Ascension Island is a remote South Atlantic equatorial site, ideal for monitoring tropical background CH4. In September 2014 and July 2015, octocopters were used to collect air samples in Tedlar bags from different heights above and below the well-defined Trade Wind Inversion (TWI), sampling a maximum altitude of 2700 m above mean sea level. Sampling captured both remote air in the marine boundary layer below the TWI and also air masses above the TWI that had been lofted by convective systems in the African tropics. Air above the TWI was characterized by higher CH4, but no distinct shift in δ13C was observed compared to the air below. Back trajectories indicate that lofted CH4 emissions from Southern Hemisphere Africa have bulk δ13CCH4 signatures similar to background, suggesting mixed emissions from wetlands, agriculture, and biomass burning. The campaigns illustrate the usefulness of unmanned aerial system sampling and Ascension's value for atmospheric measurement in an understudied region.

  13. The Learning Process and Technological Change in Wind Power: Evidence from China's CDM Wind Projects

    ERIC Educational Resources Information Center

    Tang, Tian; Popp, David

    2016-01-01

    The Clean Development Mechanism (CDM) is a project-based carbon trade mechanism that subsidizes the users of climate-friendly technologies and encourages technology transfer. The CDM has provided financial support for a large share of Chinese wind projects since 2002. Using pooled cross-sectional data of 486 registered CDM wind projects in China…

  14. Mesoscale modeling of smoke transport over Central Africa: influences of trade winds, subtropical high, ITCZ and vertical statistics

    NASA Astrophysics Data System (ADS)

    Yang, Z.; Wang, J.; Hyer, E. J.; Ichoku, C. M.

    2012-12-01

    A fully-coupled meteorology-chemistry-aerosol model, Weather Research and Forecasting model with Chemistry (WRF-Chem), is used to simulate the transport of smoke aerosol over the Central Africa during February 2008. Smoke emission used in this study is specified from the Fire Locating and Modeling of Burning Emissions (FLAMBE) database derived from Moderate Resolution Imaging Spectroradiometer (MODIS) fire products. Model performance is evaluated using MODIS true color images, measured Aerosol Optical Depth (AOD) from space-borne MODIS (550 nm) and ground-based AERONET (500 nm), and Cloud-Aerosol Lidar data with Orthogonal Polarization (CALIOP) level 1 and 2 products. The simulated smoke transport is in good agreement with the validation data. Analyzing from three smoke events, smoke is constrained in a narrow belt between the Equator and 10°N near the surface, with the interplay of trade winds, subtropical high, and ITCZ. At the 700 hpa level, smoke expands farther meridionally. Topography blocks the smoke transport to the southeast of study area, because of high mountains located near the Great Rift Valley region. The simulation with injection height of 650 m is consistent with CALIOP measurements. The particular phenomenon, aerosol above cloud, is studied statistically from CALIOP observations. The total percentage of aerosol above cloud is about 5%.

  15. MiniSODAR(TradeMark) Evaluation

    NASA Technical Reports Server (NTRS)

    Short, David A.; Wheeler, Mark M.

    2003-01-01

    This report describes results of the AMU's Instrumentation and Measurement task for evaluation of the Doppler miniSODAR(TradeMark) System (DmSS). The DmSS is an acoustic wind profiler providing high resolution data to a height of approx. 410 ft. The Boeing Company installed a DmSS near Space Launch Complex 37 in mid-2002 as a substitute for a tall wind tower and plans to use DmSS data for the analysis and forecasting of winds during ground and launch operations. Peak wind speed data are of particular importance to Launch Weather Officers of the 45th Weather Squadron for evaluating user Launch Commit Criteria. The AMU performed a comparative analysis of wind data between the DmSS and nearby wind towers from August 2002 to July 2003. The DmSS vertical profile of average wind speed showed good agreement with the wind towers. However, the DMSS peak wind speeds were higher, on average, than the wind tower peak wind speeds by about 25%. A statistical model of an idealized Doppler profiler was developed and it predicted that average wind speeds would be well determined but peak wind speeds would be over-estimated due to an under-specification of vertical velocity variations in the atmosphere over the Profiler.

  16. Diurnal, monthly and seasonal variation of mean winds in the MLT region observed over Kolhapur using MF radar

    NASA Astrophysics Data System (ADS)

    Sharma, A. K.; Gaikwad, H. P.; Ratnam, M. Venkat; Gurav, O. B.; Ramanjaneyulu, L.; Chavan, G. A.; Sathishkumar, S.

    2018-04-01

    Medium Frequency (MF) radar located at Kolhapur (16.8°N, 74.2°E) has been upgraded in August 2013. Since then continuous measurements of zonal and meridional winds are obtained covering larger altitudes from the Mesosphere and Lower Thermosphere (MLT) region. Diurnal, monthly and seasonal variation of these mean winds is presented in this study using four years (2013-2017) of observations. The percentage occurrence of radar echoes show maximum between 80 and 105 km. The mean meridional wind shows Annual Oscillation (AO) between 80 and 90 km altitudes with pole-ward motion during December solstice and equatorial motion during June solstice. Quasi-biennial oscillation (QBO) with weaker amplitudes are also observed between 90 and 104 km. Zonal winds show semi-annual oscillation (SAO) with westward winds during equinoxes and eastward winds during solstices between 80 and 90 km. AO with eastward winds during December solstice and westward wind in the June solstice is also observed in the mean zonal wind between 100 and 110 km. These results match well with that reported from other latitudes within Indian region between 80 and 90 km. However, above 90 km the results presented here provide true mean background winds for the first time over Indian low latitude region as the present station is away from equatorial electro-jet and are not contaminated by ionospheric processes. Further, the results presented earlier with an old version of this radar are found contaminated due to unknown reasons and are corrected in the present work. This upgraded MF radar together with other MLT radars in the Indian region forms unique network to investigate the vertical and lateral coupling.

  17. Downscaling wind and wavefields for 21st century coastal flood hazard projections in a region of complex terrain

    USGS Publications Warehouse

    O'Neill, Andrea; Erikson, Li; Barnard, Patrick

    2017-01-01

    While global climate models (GCMs) provide useful projections of near-surface wind vectors into the 21st century, resolution is not sufficient enough for use in regional wave modeling. Statistically downscaled GCM projections from Multivariate Adaptive Constructed Analogues provide daily averaged near-surface winds at an appropriate spatial resolution for wave modeling within the orographically complex region of San Francisco Bay, but greater resolution in time is needed to capture the peak of storm events. Short-duration high wind speeds, on the order of hours, are usually excluded in statistically downscaled climate models and are of key importance in wave and subsequent coastal flood modeling. Here we present a temporal downscaling approach, similar to constructed analogues, for near-surface winds suitable for use in local wave models and evaluate changes in wind and wave conditions for the 21st century. Reconstructed hindcast winds (1975–2004) recreate important extreme wind values within San Francisco Bay. A computationally efficient method for simulating wave heights over long time periods was used to screen for extreme events. Wave hindcasts show resultant maximum wave heights of 2.2 m possible within the Bay. Changes in extreme over-water wind speeds suggest contrasting trends within the different regions of San Francisco Bay, but 21th century projections show little change in the overall magnitude of extreme winds and locally generated waves.

  18. Simulation of Extreme Surface Winds by Regional Climate Models in the NARCCAP Archive

    NASA Astrophysics Data System (ADS)

    Hatteberg, R.; Takle, E. S.

    2011-12-01

    Surface winds play a significant role in many natural processes as well as providing a very important ecological service for many human activities. Surface winds ventilate pollutants and heat from our cities, contribute to pollination for our crops, and regulate the fluxes of heat, moisture, and carbon dioxide from the earth's surface. Many environmental models such as biogeochemical models, crop models, lake models, pollutant transport models, etc., use surface winds as a key variable. Studies of the impacts of climate change and climate variability on a wide range of natural systems and coupled human-natural systems frequently need information on how surface wind speeds will change as greenhouse gas concentrations in the earth's atmosphere change. We have studied the characteristics of extreme winds - both high winds and low winds - created by regional climate models (RCMs) in the NARCCAP archives. We evaluated the capabilities of five RCMs forced by NCEP reanalysis data as well as global climate model (GCM) data for contemporary and future scenario climates to capture the observed statistical distribution of surface winds, both high-wind events and low-wind conditions. Our domain is limited to the Midwest (37°N to 49°N, -82°W to -101°W) with the Great Lakes masked out, which eliminates orographic effects that may contribute to regional circulations. The majority of this study focuses on the warm seasonal in order to examine derechos on the extreme high end and air pollution and plant processes on the low wind speed end. To examine extreme high winds we focus on derechos, which are long-lasting convectively driven extreme wind events that frequently leave a swath of damage extending across multiple states. These events are unusual in that, despite their relatively small spatial scale, they can persist for hours or even days, drawing energy from well-organized larger mesoscale or synoptic scale processes. We examine the ability of NARCCAP RCMs to reproduce

  19. Synoptic versus regional causes of icing on wind turbines at an exposed wind farm site in Germany

    NASA Astrophysics Data System (ADS)

    Weissinger, Maximilian; Strauss, Lukas; Serafin, Stefano; Dorninger, Manfred; Burchhart, Thomas; Fink, Martin

    2017-04-01

    Ice accretion on wind turbine blades can lead to significant power production loss or even permanent structural damage on the turbine. With the ongoing construction of wind farms at sites with increased icing potential in cold climates, accurate icing predictions are needed to optimise power plant operation. To this end, the frequency of occurrence and the causes of meteorological icing need to be better understood. The project ICE CONTROL, an Austrian research initiative, aims to improve icing forecasts through measurements, probabilistic forecasting, and verification of icing on wind turbine blades. The project focuses on a wind farm site near Ellern, Germany, located on the Hunsrück, a hilly terrain rising above the surrounding plain by 200-300 metres. Production data from the last three winters show that icing events tend to occur more often at the wind turbines on top of the highest hills. The present study aims to investigate historical cases of wind turbine icing and their meteorological causes at the Ellern wind farm. The data available consists of a three-year period (2013-2016) of operational data from the Ellern wind farm as well as meteorological measurements at nearby stations operated by the German Weather Service (DWD). In addition, radiosondes and weather charts are taken into account. The main objective of this work is, first, to link the local and regional weather conditions to larger-scale weather patterns and prevailing air masses, and second, to determine the types of icing (in-cloud vs. freezing precipation). Results show that in most icing cases the cloud base height was below the hub height while the temperature was just below the freezing point. Precipitation was absent in most cases. This suggests that most of the observed icing events were due to in-cloud icing. Icing conditions occurred often (but not exclusively) under specific synoptic-scale weather conditions, such as north-westerly flow advecting maritime polar air masses to Central

  20. Mesopause region wind, temperature and airglow irradiance above Eureka, Nunavut

    NASA Astrophysics Data System (ADS)

    Kristoffersen, Samuel; Ward, William E.; Vail, Christopher; Shepherd, Marianna

    2016-07-01

    The PEARL All Sky Imager (PASI, airglow images), the Spectral Airglow Temperature Imager (SATI, airglow irradiance and temperature) and the E-Region Wind Interferometer II (ERWIN2, wind, airglow irradiance and temperature) are co-located at the Polar Environment Atmospheric Research Laboratory (PEARL)in Eureka, Nunavut (80 N, 86 W). These instruments view the wind, temperature and airglow irradiance of hydroxyl (all three) O2 (ERWIN2 and SATI), sodium (PASI), and oxygen green line (PASI and ERWIN2). The viewing locations and specific emissions of the various instruments differ. Nevertheless, the co-location of these instruments provides an excellent opportunity for case studies of specific events and for intercomparison between the different techniques. In this paper we discuss the approach we are using to combine observations from the different instruments. Case studies show that at times the various instruments are in good agreement but at other times they differ. Of particular interest are situations where gravity wave signatures are evident for an extended period of time and one such situation is presented. The discussion includes consideration of the filtering effect of viewing through airglow layers and the extent to which wind, airglow and temperature variations can be associated with the same gravity wave.

  1. Safe application of regionalization for trade in poultry and poultry products during highly pathogenic avian influenza outbreaks in the USA.

    PubMed

    Swayne, David E; Hill, Rick E; Clifford, John

    2017-04-01

    The 2014-2015 H5Nx high pathogenicity avian influenza (HPAI) outbreak affected 211 commercial premises, 21 backyard flocks, 75 individual wild birds and four captive-reared raptors in 21 Western and upper Midwestern states, resulting in death or culling of over 50.4 million poultry in the stamping-out programme that cost the US government $850 million. The outbreak had a negative $3.3 billion impact on the economy. Seventeen trading partners suspended imports of all US-origin poultry and poultry products while 38 trading partners regionalized the United States, and allowed trade in poultry and poultry products to continue from areas of the US not affected by HPAI. Disease response and control activities in addition to the use of comprehensive surveillance and regionalization (zoning) as prescribed by the OIE Terrestrial Animal Health Code are a scientifically valid and effective means to maintain safe trade in poultry and poultry products. This was further realized during the 2016 H7N8 HPAI outbreak in Dubois County, Indiana, with greater acceptance of regionalization and continuity in trade with a more limited cost of $30 million for eradication.

  2. The NO{sub x} Budget trading program: a collaborative, innovative approach to solving a regional air pollution problem

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

    Napolitano, Sam; Stevens, Gabrielle; Schreifels, Jeremy

    2007-11-15

    The NO{sub x} Budget Trading Program showed that regional cap-and-trade programs are adaptable to more than one pollutant, time period, and geographic scale, and can achieve compliance results similar to the Acid Rain Program. Here are 11 specific lessons that have emerged from the experience. (author)

  3. Operation of Power Grids with High Penetration of Wind Power

    NASA Astrophysics Data System (ADS)

    Al-Awami, Ali Taleb

    The integration of wind power into the power grid poses many challenges due to its highly uncertain nature. This dissertation involves two main components related to the operation of power grids with high penetration of wind energy: wind-thermal stochastic dispatch and wind-thermal coordinated bidding in short-term electricity markets. In the first part, a stochastic dispatch (SD) algorithm is proposed that takes into account the stochastic nature of the wind power output. The uncertainty associated with wind power output given the forecast is characterized using conditional probability density functions (CPDF). Several functions are examined to characterize wind uncertainty including Beta, Weibull, Extreme Value, Generalized Extreme Value, and Mixed Gaussian distributions. The unique characteristics of the Mixed Gaussian distribution are then utilized to facilitate the speed of convergence of the SD algorithm. A case study is carried out to evaluate the effectiveness of the proposed algorithm. Then, the SD algorithm is extended to simultaneously optimize the system operating costs and emissions. A modified multi-objective particle swarm optimization algorithm is suggested to identify the Pareto-optimal solutions defined by the two conflicting objectives. A sensitivity analysis is carried out to study the effect of changing load level and imbalance cost factors on the Pareto front. In the second part of this dissertation, coordinated trading of wind and thermal energy is proposed to mitigate risks due to those uncertainties. The problem of wind-thermal coordinated trading is formulated as a mixed-integer stochastic linear program. The objective is to obtain the optimal tradeoff bidding strategy that maximizes the total expected profits while controlling trading risks. For risk control, a weighted term of the conditional value at risk (CVaR) is included in the objective function. The CVaR aims to maximize the expected profits of the least profitable scenarios, thus

  4. Application of the Wind Erosion Prediction System in the AIRPACT regional air quality modeling framework

    USDA-ARS?s Scientific Manuscript database

    Wind erosion of soil is a major concern of the agricultural community as it removes the most fertile part of the soil and thus degrades soil productivity. Furthermore, dust emissions due to wind erosion contribute to poor air quality, reduce visibility, and cause perturbations to regional radiation ...

  5. Giant stellar-wind shell associated with the H II region M16

    NASA Astrophysics Data System (ADS)

    Sofue, Y.; Handa, T.; Fuerst, E.; Reich, W.; Reich, P.

    The detection of a giant radio continuum shell associated with the bright H II region M16, one of the most active star-forming sites in the Sagittarius arm, is reported. The shell structure agrees with that predicted by the stellar wind bubble model. The innermost regions of the shell is a cavity dominated by a stellar wind from early-type stars and is bounded by shocked H II gas. The shell is observed as a thermal radio emission loop. The rate of kinetic energy injection from the central O stars is estimated to be 3.3 x 10 to the 36th ergs/s, and the corresponding mass loss rate is 2.6 x 10 to the -6th solar mass/yr, with an age of the shell being about 7 million yr.

  6. Mid-Atlantic Regional Training Center for Residential Construction Trades. Final Program Evaluation Report.

    ERIC Educational Resources Information Center

    Wasdyke (R. G.) & Associates, Annapolis, MD.

    A group of partners headed by the Home Builders Institute (HBI) created the Mid-Atlantic Regional Training (MART) Center for Residential Construction, with a primary focus on providing education and training services related to the masonry and carpentry trades at existing institutions in the District of Columbia, Maryland, Virginia, and West…

  7. The effect of vegetation patterns on wind-blown mass transport at the regional scale: A wind tunnel experiment

    NASA Astrophysics Data System (ADS)

    Youssef, Feras; Visser, Saskia M.; Karssenberg, Derek; Erpul, Gunay; Cornelis, Wim M.; Gabriels, Donald; Poortinga, Ate

    2012-07-01

    Wind erosion is a global environmental problem. Re-vegetating land is a commonly used method to reduce the negative effects of wind erosion. However, there is limited knowledge on the effect of vegetation pattern on wind-blown mass transport. The objective of this study was to investigate the effect of vegetation pattern on this phenomenon within a land unit and at the border between land units. Wind tunnel experiments were conducted with artificial shrubs representing Atriplex halimus. Wind runs at a speed of 11 m s- 1 were conducted and sand translocation was measured after 200-230 s using a graph paper prepared for this purpose. This research showed that: 1) the transport within a land unit is affected by the neighboring land units and by the vegetation pattern within both the unit itself and the neighboring land units; 2) re-vegetation plans for degraded land can take into account the 'streets' effect (zones of erosion areas similar to streets); 3) the effect of neighboring land units includes sheltering effect and the regulation of sediment passing from one land unit to the neighboring land units and 4) in addition to investigation of the general effect of vegetation pattern on erosion and deposition within the region, it is important to investigate the redistribution of sediment at smaller scales depending on the scope of the project.

  8. Influence of interplanetary magnetic field and solar wind on auroral brightness in different regions

    NASA Astrophysics Data System (ADS)

    Yang, Y. F.; Lu, J. Y.; Wang, J.-S.; Peng, Z.; Zhou, L.

    2013-01-01

    Abstract<p label="1">By integrating and averaging the auroral brightness from Polar Ultraviolet Imager auroral images, which have the whole auroral ovals, and combining the observation data of interplanetary magnetic field (IMF) and solar <span class="hlt">wind</span> from NASA Operating Missions as a Node on the Internet (OMNI), we investigate the influence of IMF and solar <span class="hlt">wind</span> on auroral activities, and analyze the separate roles of the solar <span class="hlt">wind</span> dynamic pressure, density, and velocity on aurora, respectively. We statistically analyze the relations between the interplanetary conditions and the auroral brightness in dawnside, dayside, duskside, and nightside. It is found that the three components of the IMF have different effects on the auroral brightness in the different <span class="hlt">regions</span>. Different from the nightside auroral brightness, the dawnside, dayside, and duskside auroral brightness are affected by the IMF Bx, and By components more significantly. The IMF Bx and By components have different effects on these three <span class="hlt">regional</span> auroral brightness under the opposite polarities of the IMF Bz. As expected, the nightside aurora is mainly affected by the IMF Bz, and under southward IMF, the larger the |Bz|, the brighter the nightside aurora. The IMF Bx and By components have no visible effects. On the other hand, it is also found that the aurora is not intensified singly with the increase of the solar <span class="hlt">wind</span> dynamic pressure: when only the dynamic pressure is high, but the solar <span class="hlt">wind</span> velocity is not very fast, the aurora will not necessarily be intensified significantly. These results can be used to qualitatively predict the auroral activities in different <span class="hlt">regions</span> for various interplanetary conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.4253Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.4253Z"><span>Local and <span class="hlt">regional</span> effects of large scale atmospheric circulation patterns on winter <span class="hlt">wind</span> power output in 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>Zubiate, Laura; McDermott, Frank; Sweeney, Conor; O'Malley, Mark</p> <p>2014-05-01</p> <p>Recent studies (Brayshaw, 2009, Garcia-Bustamante, 2010, Garcia-Bustamante, 2013) have drawn attention to the sensitivity of <span class="hlt">wind</span> speed distributions and likely <span class="hlt">wind</span> energy power output in Western Europe to changes in low-frequency, large scale atmospheric circulation patterns such as the North Atlantic Oscillation (NAO). <span class="hlt">Wind</span> speed variations and directional shifts as a function of the NAO state can be larger or smaller depending on the North Atlantic <span class="hlt">region</span> that is considered. <span class="hlt">Wind</span> speeds in Ireland and the UK for example are approximately 20 % higher during NAO + phases, and up to 30 % lower during NAO - phases relative to the long-term (30 year) climatological means. By contrast, in southern Europe, <span class="hlt">wind</span> speeds are 15 % lower than average during NAO + phases and 15 % higher than average during NAO - phases. Crucially however, some <span class="hlt">regions</span> such as Brittany in N.W. France have been identified in which there is negligible variability in <span class="hlt">wind</span> speeds as a function of the NAO phase, as observed in the ERA-Interim 0.5 degree gridded reanalysis database. However, the magnitude of these effects on <span class="hlt">wind</span> conditions is temporally and spatially non-stationary. As described by Comas-Bru and McDermott (2013) for temperature and precipitation, such non-stationarity is caused by the influence of two other patterns, the East Atlantic pattern, (EA), and the Scandinavian pattern, (SCA), which modulate the position of the NAO dipole. This phenomenon has also implications for <span class="hlt">wind</span> speeds and directions, which has been assessed using the ERA-Interim reanalysis dataset and the indices obtained from the PC analysis of sea level pressure over the Atlantic <span class="hlt">region</span>. In order to study the implications for power production, the interaction of the NAO and the other teleconnection patterns with local topography was also analysed, as well as how these interactions ultimately translate into <span class="hlt">wind</span> power output. The objective is to have a better defined relationship between <span class="hlt">wind</span> speed and power</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20080018955&hterms=wind+monitor&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwind%2Bmonitor','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20080018955&hterms=wind+monitor&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dwind%2Bmonitor"><span>The Solar <span class="hlt">Wind</span> and Geomagnetic Activity as a Function of Time Relative to Corotating Interaction <span class="hlt">Regions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>McPherron, Robert L.; Weygand, James</p> <p>2006-01-01</p> <p>Corotating interaction <span class="hlt">regions</span> during the declining phase of the solar cycle are the cause of recurrent geomagnetic storms and are responsible for the generation of high fluxes of relativistic electrons. These <span class="hlt">regions</span> are produced by the collision of a high-speed stream of solar <span class="hlt">wind</span> with a slow-speed stream. The interface between the two streams is easily identified with plasma and field data from a solar <span class="hlt">wind</span> monitor upstream of the Earth. The properties of the solar <span class="hlt">wind</span> and interplanetary magnetic field are systematic functions of time relative to the stream interface. Consequently the coupling of the solar <span class="hlt">wind</span> to the Earth's magnetosphere produces a predictable sequence of events. Because the streams persist for many solar rotations it should be possible to use terrestrial observations of past magnetic activity to predict future activity. Also the high-speed streams are produced by large unipolar magnetic <span class="hlt">regions</span> on the Sun so that empirical models can be used to predict the velocity profile of a stream expected at the Earth. In either case knowledge of the statistical properties of the solar <span class="hlt">wind</span> and geomagnetic activity as a function of time relative to a stream interface provides the basis for medium term forecasting of geomagnetic activity. In this report we use lists of stream interfaces identified in solar <span class="hlt">wind</span> data during the years 1995 and 2004 to develop probability distribution functions for a variety of different variables as a function of time relative to the interface. The results are presented as temporal profiles of the quartiles of the cumulative probability distributions of these variables. We demonstrate that the storms produced by these interaction <span class="hlt">regions</span> are generally very weak. Despite this the fluxes of relativistic electrons produced during those storms are the highest seen in the solar cycle. We attribute this to the specific sequence of events produced by the organization of the solar <span class="hlt">wind</span> relative to the stream interfaces. We also</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26540068','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26540068"><span><span class="hlt">Trade</span>-Off and Synergy among Ecosystem Services in the Guanzhong-Tianshui Economic <span class="hlt">Region</span> of China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Qin, Keyu; Li, Jing; Yang, Xiaonan</p> <p>2015-11-03</p> <p>Natural ecosystems provide society with important goods and services. With rapidly increasing populations and excessive utilization of natural resources, humans have been enhancing the production of some services at the expense of others. Although the need for certain <span class="hlt">trade</span>-offs between conservation and development is urgent, having only a small number of efficient methods to assess such <span class="hlt">trade</span>-offs has impeded progress. This study focuses on the evaluation of ecosystem services under different land use schemes. It reveals the spatial and temporal distributions of and changes in ecosystem services. Based on a correlation rate model and distribution mapping, the <span class="hlt">trade</span>-offs and synergies of these ecosystem services can be found. Here, we also describe a new simple approach to quantify the relationships of every <span class="hlt">trade</span>-off and synergy. The results show that all ecosystem services possess <span class="hlt">trade</span>-offs and synergies in the study area. The trend of improving carbon sequestration and water interception indicate that these key ecosystem services have the strongest synergy. And the decrease in <span class="hlt">regional</span> agricultural production and other services, except water yield, may be considered as <span class="hlt">trade</span>-offs. The synergy between water yield and agricultural production was the most significant, while the <span class="hlt">trade</span>-off between water interception and carbon sequestration was the most apparent, according to our interaction quantification model. The results of this study have implications for planning and monitoring the future management of natural capital and ecosystem services, and can be integrated into land use decision-making.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4661635','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4661635"><span><span class="hlt">Trade</span>-Off and Synergy among Ecosystem Services in the Guanzhong-Tianshui Economic <span class="hlt">Region</span> of China</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Qin, Keyu; Li, Jing; Yang, Xiaonan</p> <p>2015-01-01</p> <p>Natural ecosystems provide society with important goods and services. With rapidly increasing populations and excessive utilization of natural resources, humans have been enhancing the production of some services at the expense of others. Although the need for certain <span class="hlt">trade</span>-offs between conservation and development is urgent, having only a small number of efficient methods to assess such <span class="hlt">trade</span>-offs has impeded progress. This study focuses on the evaluation of ecosystem services under different land use schemes. It reveals the spatial and temporal distributions of and changes in ecosystem services. Based on a correlation rate model and distribution mapping, the <span class="hlt">trade</span>-offs and synergies of these ecosystem services can be found. Here, we also describe a new simple approach to quantify the relationships of every <span class="hlt">trade</span>-off and synergy. The results show that all ecosystem services possess <span class="hlt">trade</span>-offs and synergies in the study area. The trend of improving carbon sequestration and water interception indicate that these key ecosystem services have the strongest synergy. And the decrease in <span class="hlt">regional</span> agricultural production and other services, except water yield, may be considered as <span class="hlt">trade</span>-offs. The synergy between water yield and agricultural production was the most significant, while the <span class="hlt">trade</span>-off between water interception and carbon sequestration was the most apparent, according to our interaction quantification model. The results of this study have implications for planning and monitoring the future management of natural capital and ecosystem services, and can be integrated into land use decision-making. PMID:26540068</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003A%26A...406..345L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003A%26A...406..345L"><span>Transition <span class="hlt">region</span>, coronal heating and the fast solar <span class="hlt">wind</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Li, Xing</p> <p>2003-07-01</p> <p>It is assumed that magnetic flux tubes are strongly concentrated at the boundaries of supergranule convection cells. A power law spectrum of high frequency Alfvén waves with a spectral index -1 originating from the sun is assumed to supply all the energy needed to energize the plasma flowing in such magnetic flux tubes. At the high frequency end, the waves are eroded by ions due to ion cyclotron resonance. The magnetic flux concentration is essential since it allows a sufficiently strong energy flux to be carried by high frequency ion cyclotron waves and these waves can be readily released at the coronal base by cyclotron resonance. The main results are: 1. The waves are capable of creating a steep transition <span class="hlt">region</span>, a hot corona and a fast solar <span class="hlt">wind</span> if both the wave frequency is high enough and the magnetic flux concentration is sufficiently strong in the boundaries of the supergranule convection zone. 2. By primarily heating alpha particles only, it is possible to produce a steep transition <span class="hlt">region</span>, a hot corona and a fast solar <span class="hlt">wind</span>. Coulomb coupling plays a key role in transferring the thermal energy of alpha particles to protons and electrons at the corona base. The electron thermal conduction then does the remaining job to create a sharp transition <span class="hlt">region</span>. 3. Plasma species (even ions) may already partially lose thermal equilibrium in the transition <span class="hlt">region</span>, and minor ions may already be faster than protons at the very base of the corona. 4. The model predicts high temperature alpha particles (Talpha ~ 2 x 107 K) and low proton temperatures (Tp < 106 K) between 2 and 4 solar radii, suggesting that hydrogen Lyman lines observed by UVCS above coronal holes may be primarily broadened by Alfvén waves in this range.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMSH13B4118L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMSH13B4118L"><span>Analysis of Solar <span class="hlt">Wind</span> Plasma Properties of Co-Rotating Interaction <span class="hlt">Regions</span> at Mars with MSL/RAD</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lohf, H.; Kohler, J.; Zeitlin, C. J.; Ehresmann, B.; Guo, J.; Wimmer-Schweingruber, R. F.; Hassler, D.; Reitz, G.; Posner, A.; Heber, B.; Appel, J. K.; Matthiae, D.; Brinza, D. E.; Weigle, E.; Böttcher, S. I.; Burmeister, S.; Martin-Garcia, C.; Boehm, E.; Rafkin, S. C.; Kahanpää, H.; Martín-Torres, J.; Zorzano, M. P.</p> <p>2014-12-01</p> <p>The measurements of the Radiation Assessment Detector (RAD) onboard Mars Science Laboratory's rover Curiosity have given us the very first opportunity to evaluate the radiation environment on the surface of Mars, which consists mostly of Galactic Cosmic Rays (GCRs) and secondary particles created in the Martian Atmosphere. The solar <span class="hlt">wind</span> can have an influence on the modulation of the GCR, e.g. when the fast solar <span class="hlt">wind</span> (~ 750 km/s) interacts with the slow solar <span class="hlt">wind</span> (~ 400 km/s) at so-called Stream Interaction <span class="hlt">Regions</span> (SIRs) resulting in an enhancement of the local magnetic field which could affect the shielding of GCRs. SIRs often occur periodically as Co-rotating Interaction <span class="hlt">Regions</span> (CIRs) which may-be observed at Mars as a decrease in the radiation data measured by MSL/RAD. Considering the difference of the Earth-Mars orbit, we correlate these in-situ radiation data at Mars with the solar <span class="hlt">wind</span> properties measured by spacecrafts at 1 AU, with the aim to eventually determine the solar <span class="hlt">wind</span> properties at Mars based on MSL/RAD measurements.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/6135838-region-neutral-winds-from-ionosonde-measurements-sub-mf2-low-latitude-magnetic-conjugate-regions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/6135838-region-neutral-winds-from-ionosonde-measurements-sub-mf2-low-latitude-magnetic-conjugate-regions"><span>F-<span class="hlt">region</span> neutral <span class="hlt">winds</span> from ionosonde measurements of h/sub mF2/ at low-latitude magnetic conjugate <span class="hlt">regions</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>Bittencourt, J.A.</p> <p>1977-08-01</p> <p>The behavior of the F2-peak height difference, delta h/sub F2/, between low-latitude magnetic conjugate points, is known to be governed by thermospheric <span class="hlt">winds</span> blowing along the magnetic meridian. Ground-based ionosonde measurement of h/sub m F2/, at two pairs of magnetic conjugate stations, were analyzed in conjunction with the results of a realistic dynamic computer model of the tropical ionospheric F-<span class="hlt">region</span>, to determine thermospheric <span class="hlt">wind</span> velocities. The behavior of monthly average values of the sun, at conjugate points, of the thermospheric horizontal <span class="hlt">wind</span> velocity component in the magnetic meridian, at low latitudes, is inferred for months of solstice and equinox, asmore » well as for periods of low and high solar activity.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-12-29/pdf/2010-32868.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-12-29/pdf/2010-32868.pdf"><span>75 FR 82130 - WTO Dispute Settlement Proceeding Regarding China-Subsidies on <span class="hlt">Wind</span> Power Equipment</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-12-29</p> <p>...--Subsidies on <span class="hlt">Wind</span> Power Equipment AGENCY: Office of the United States <span class="hlt">Trade</span> Representative. ACTION: Notice... certain subsidies provided by the People's Republic of China (China) on <span class="hlt">wind</span> power equipment. The... Special Fund for Industrialization of <span class="hlt">Wind</span> Power Equipment'' (``<span class="hlt">Wind</span> Power Equipment Fund''). The <span class="hlt">Wind</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/38904','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/38904"><span>Climate and climate variability of the <span class="hlt">wind</span> power resources in the Great Lakes <span class="hlt">region</span> of the United States</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>X. Li; S. Zhong; X. Bian; W.E. Heilman</p> <p>2010-01-01</p> <p>The climate and climate variability of low-level <span class="hlt">winds</span> over the Great Lakes <span class="hlt">region</span> of the United States is examined using 30 year (1979-2008) <span class="hlt">wind</span> records from the recently released North American <span class="hlt">Regional</span> Reanalysis (NARR), a three-dimensional, high-spatial and temporal resolution, and dynamically consistent climate data set. The analyses focus on spatial distribution...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4391724','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4391724"><span>LPV Control for the Full <span class="hlt">Region</span> Operation of a <span class="hlt">Wind</span> Turbine Integrated with Synchronous Generator</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Grigoriadis, Karolos M.; Nyanteh, Yaw D.</p> <p>2015-01-01</p> <p><span class="hlt">Wind</span> turbine conversion systems require feedback control to achieve reliable <span class="hlt">wind</span> turbine operation and stable current supply. A robust linear parameter varying (LPV) controller is proposed to reduce the structural loads and improve the power extraction of a horizontal axis <span class="hlt">wind</span> turbine operating in both the partial load and the full load <span class="hlt">regions</span>. The LPV model is derived from the <span class="hlt">wind</span> turbine state space models extracted by FAST (fatigue, aerodynamics, structural, and turbulence) code linearization at different operating points. In order to assure a smooth transition between the two <span class="hlt">regions</span>, appropriate frequency-dependent varying scaling parametric weighting functions are designed in the LPV control structure. The solution of a set of linear matrix inequalities (LMIs) leads to the LPV controller. A synchronous generator model is connected with the closed LPV control loop for examining the electrical subsystem performance obtained by an inner speed control loop. Simulation results of a 1.5 MW horizontal axis <span class="hlt">wind</span> turbine model on the FAST platform illustrates the benefit of the LPV control and demonstrates the advantages of this proposed LPV controller, when compared with a traditional gain scheduling PI control and prior LPV control configurations. Enhanced structural load mitigation, improved power extraction, and good current performance were obtained from the proposed LPV control. PMID:25884036</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25884036','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25884036"><span>LPV control for the full <span class="hlt">region</span> operation of a <span class="hlt">wind</span> turbine integrated with synchronous generator.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Cao, Guoyan; Grigoriadis, Karolos M; Nyanteh, Yaw D</p> <p>2015-01-01</p> <p><span class="hlt">Wind</span> turbine conversion systems require feedback control to achieve reliable <span class="hlt">wind</span> turbine operation and stable current supply. A robust linear parameter varying (LPV) controller is proposed to reduce the structural loads and improve the power extraction of a horizontal axis <span class="hlt">wind</span> turbine operating in both the partial load and the full load <span class="hlt">regions</span>. The LPV model is derived from the <span class="hlt">wind</span> turbine state space models extracted by FAST (fatigue, aerodynamics, structural, and turbulence) code linearization at different operating points. In order to assure a smooth transition between the two <span class="hlt">regions</span>, appropriate frequency-dependent varying scaling parametric weighting functions are designed in the LPV control structure. The solution of a set of linear matrix inequalities (LMIs) leads to the LPV controller. A synchronous generator model is connected with the closed LPV control loop for examining the electrical subsystem performance obtained by an inner speed control loop. Simulation results of a 1.5 MW horizontal axis <span class="hlt">wind</span> turbine model on the FAST platform illustrates the benefit of the LPV control and demonstrates the advantages of this proposed LPV controller, when compared with a traditional gain scheduling PI control and prior LPV control configurations. Enhanced structural load mitigation, improved power extraction, and good current performance were obtained from the proposed LPV control.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140010435','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140010435"><span>Particle-In-Cell Simulations of the Solar <span class="hlt">Wind</span> Interaction with Lunar Crustal Magnetic Anomalies: Magnetic Cusp <span class="hlt">Regions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Poppe, A. R.; Halekas, J. S.; Delory, G. T.; Farrell, W. M.</p> <p>2012-01-01</p> <p>As the solar <span class="hlt">wind</span> is incident upon the lunar surface, it will occasionally encounter lunar crustal remanent magnetic fields. These magnetic fields are small-scale, highly non-dipolar, have strengths up to hundreds of nanotesla, and typically interact with the solar <span class="hlt">wind</span> in a kinetic fashion. Simulations, theoretical analyses, and spacecraft observations have shown that crustal fields can reflect solar <span class="hlt">wind</span> protons via a combination of magnetic and electrostatic reflection; however, analyses of surface properties have suggested that protons may still access the lunar surface in the cusp <span class="hlt">regions</span> of crustal magnetic fields. In this first report from a planned series of studies, we use a 1 1/2-dimensional, electrostatic particle-in-cell code to model the self-consistent interaction between the solar <span class="hlt">wind</span>, the cusp <span class="hlt">regions</span> of lunar crustal remanent magnetic fields, and the lunar surface. We describe the self-consistent electrostatic environment within crustal cusp <span class="hlt">regions</span> and discuss the implications of this work for the role that crustal fields may play regulating space weathering of the lunar surface via proton bombardment.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_6");'>6</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li class="active"><span>8</span></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_8 --> <div id="page_9" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_7");'>7</a></li> <li><a href="#" onclick='return showDiv("page_8");'>8</a></li> <li class="active"><span>9</span></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="161"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19730023957&hterms=coastal+erosion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcoastal%2Berosion','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19730023957&hterms=coastal+erosion&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dcoastal%2Berosion"><span>Mariner 9 evidence for <span class="hlt">wind</span> erosion in the equatorial and mid-latitude <span class="hlt">regions</span> of Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Mccauley, J. F.</p> <p>1973-01-01</p> <p>Evidence for extensive <span class="hlt">wind</span> erosion principally in the equatorial and mid-latitude <span class="hlt">regions</span> of Mars is presented and compared with selected erosional landforms from the coastal desert of Peru known to be of eolian origin. The evidence for widespread erosion on Mars prompted an examination of certain aspects of its <span class="hlt">wind</span> regime that are thought to be significant geologically.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH23D2692D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH23D2692D"><span>Remote Sensing of the Solar <span class="hlt">Wind</span> Density, Speed, and Temperature in the <span class="hlt">Region</span> between the Sun and Parker Solar Probe</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Davila, J. M.; Reginald, N. L.</p> <p>2017-12-01</p> <p>A coronagraph is the tool of choice to understand and observe the structure of the corona from space. The novel coronagraph concept presented her provides a new scientific capability that will allow the measurement of density, temperature, and flow velocity in the solar atmosphere. This instrument will provide the first remote sensing measurement of the global solar <span class="hlt">wind</span> temperature, density, and flow speed in the <span class="hlt">regions</span> between 3 and 8 Rsun. It is in this <span class="hlt">region</span> that the manority of the solar <span class="hlt">wind</span> acceleration takes place, and where the ion compsition of the solar <span class="hlt">wind</span> is "frozen in". This is also the <span class="hlt">region</span> of the corona that links the surface of the Sun to the Parker Solar Probe and to Solar Orbiter. The observations suggested here would dramatically improve our understanding of solar <span class="hlt">wind</span> formation and evolution in this critical <span class="hlt">region</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018CSF...109..118L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018CSF...109..118L"><span>Multifractal analysis of the time series of daily means of <span class="hlt">wind</span> speed in complex <span class="hlt">regions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laib, Mohamed; Golay, Jean; Telesca, Luciano; Kanevski, Mikhail</p> <p>2018-04-01</p> <p>In this paper, we applied the multifractal detrended fluctuation analysis to the daily means of <span class="hlt">wind</span> speed measured by 119 weather stations distributed over the territory of Switzerland. The analysis was focused on the inner time fluctuations of <span class="hlt">wind</span> speed, which could be more linked with the local conditions of the highly varying topography of Switzerland. Our findings point out to a persistent behaviour of all the measured <span class="hlt">wind</span> speed series (indicated by a Hurst exponent significantly larger than 0.5), and to a high multifractality degree indicating a relative dominance of the large fluctuations in the dynamics of <span class="hlt">wind</span> speed, especially in the Swiss plateau, which is comprised between the Jura and Alp mountain ranges. The study represents a contribution to the understanding of the dynamical mechanisms of <span class="hlt">wind</span> speed variability in mountainous <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29189756','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29189756"><span>The Role of China in the UK Relative Imports from Three Selected <span class="hlt">Trading</span> <span class="hlt">Regions</span>: The Case of Textile Raw Material Industry.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Xu, Junqian</p> <p>2017-11-30</p> <p>The UK textile industry was very prosperous in the past but in the 1970s Britain started to import textile materials from abroad. Since 1990, half of its textile materials have been imported from the EEA (European Economic Area), ASEAN (Association of Southeast Asian Nations) and North America countries. Meanwhile, UK imports from China have increased dramatically. Through comparisons, this paper calculates the <span class="hlt">trade</span> competitiveness index and relative competitive advantages of <span class="hlt">regions</span> and investigates the impact of Chinese textiles on UK imports from three key free <span class="hlt">trade</span> <span class="hlt">regions</span> across the textile sectors in the period 1990-2016 on the basis of United Nation Comtrade Rev. 3. We find that China's textile prices, product techniques, political <span class="hlt">trade</span> barriers and even tax system have made a varied impact on the UK's imports across related sectors in the context of green <span class="hlt">trade</span> and the strengthening of barriers, which helps us recognize China's competitiveness in international <span class="hlt">trading</span> and also provides advice on China's sustainable development of textile exports.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AdSR...11...49A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AdSR...11...49A"><span>Comparison of the economic impact of different <span class="hlt">wind</span> power forecast systems for producers</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Alessandrini, S.; Davò, F.; Sperati, S.; Benini, M.; Delle Monache, L.</p> <p>2014-05-01</p> <p>Deterministic forecasts of <span class="hlt">wind</span> production for the next 72 h at a single <span class="hlt">wind</span> farm or at the <span class="hlt">regional</span> level are among the main end-users requirement. However, for an optimal management of <span class="hlt">wind</span> power production and distribution it is important to provide, together with a deterministic prediction, a probabilistic one. A deterministic forecast consists of a single value for each time in the future for the variable to be predicted, while probabilistic forecasting informs on probabilities for potential future events. This means providing information about uncertainty (i.e. a forecast of the PDF of power) in addition to the commonly provided single-valued power prediction. A significant probabilistic application is related to the <span class="hlt">trading</span> of energy in day-ahead electricity markets. It has been shown that, when <span class="hlt">trading</span> future <span class="hlt">wind</span> energy production, using probabilistic <span class="hlt">wind</span> power predictions can lead to higher benefits than those obtained by using deterministic forecasts alone. In fact, by using probabilistic forecasting it is possible to solve economic model equations trying to optimize the revenue for the producer depending, for example, on the specific penalties for forecast errors valid in that market. In this work we have applied a probabilistic <span class="hlt">wind</span> power forecast systems based on the "analog ensemble" method for bidding <span class="hlt">wind</span> energy during the day-ahead market in the case of a <span class="hlt">wind</span> farm located in Italy. The actual hourly income for the plant is computed considering the actual selling energy prices and penalties proportional to the unbalancing, defined as the difference between the day-ahead offered energy and the actual production. The economic benefit of using a probabilistic approach for the day-ahead energy bidding are evaluated, resulting in an increase of 23% of the annual income for a <span class="hlt">wind</span> farm owner in the case of knowing "a priori" the future energy prices. The uncertainty on price forecasting partly reduces the economic benefit gained by using a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A33C0163B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A33C0163B"><span>Isotope and methane dynamics above and below the <span class="hlt">Trade</span> <span class="hlt">Wind</span> Inversion at Ascension Island using UAVs</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Brownlow, R.; Lowry, D.; Nisbet, E. G.; Fisher, R. E.; France, J.; Lanoisellé, M.; Thomas, R.; Richardson, T.; Greatwood, C.; Freer, J. E.; MacKenzie, A. R.</p> <p>2015-12-01</p> <p>Ascension Island (8oS, 14 oW) is a South Atlantic background site for atmospheric measurement. Royal Holloway, in collaboration with the UK Met Office, installed a Picarro 1301 CRDS in 2010 for continuous methane monitoring. This has high precision and accuracy, with a 6-gas calibration and target suite, to measure long term methane mole fraction. Regular flask sampling is also carried out for NOAA and RHUL (co-located), to measure δ13CCH4 isotopic trends.Ascension Island experiences near-constant SE <span class="hlt">Trade</span> <span class="hlt">winds</span> below the <span class="hlt">Trade</span> <span class="hlt">Wind</span> Inversion (TWI), with air from the remote S. Atlantic. In flask samples and in continuous monitoring at the Airhead location, atmospheric methane mole fraction has been increasing since 2007 whilst the δ13CCH4 isotope record has shifted to more depleted values. Above the normally well-defined TWI (1200 - 1800m altitude), variable tropical air masses pass over Ascension. This air last mixed with the boundary layer over Africa or South America. Field work undertaken in September 2014 and July 2015, in collaboration with U. Bristol and U. Birmingham, using UAVs (octocopters) collected samples with Tedlar bags or aluminium flasks from different heights above and below the TWI. The maximum altitude reached was 2700masl. Sample bags were immediately analysed on Ascension for CH4 mole fraction using the Picarro CRDS and subsequently analysed at RHUL for δ13CCH4 using continuous-flow gas chromatography/isotope-ratio mass spectrometry (CF-GC/IRMS). The TWI was clearly identified by an increase in CH4 mole fraction above the TWI. Back trajectory analysis was used to distinguish the origins of the air masses, with air above showing inputs from the land surfaces of equatorial and southern Africa, and from southern S. America.The campaigns have extended the envelope of altitudes accessed by micro-UAVs for atmospheric science, demonstrating their utility for probing the remote free troposphere and for penetrating the TWI. Sampling at Ascension is</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.dtic.mil/docs/citations/ADA524190','DTIC-ST'); return false;" href="http://www.dtic.mil/docs/citations/ADA524190"><span>U.S. <span class="hlt">Trade</span> Policy and the Caribbean: From <span class="hlt">Trade</span> Preferences to Free <span class="hlt">Trade</span> Agreements</span></a></p> <p><a target="_blank" href="http://www.dtic.mil/">DTIC Science & Technology</a></p> <p></p> <p>2010-06-22</p> <p>countries, long involved in dependent economic relationships, appear content to take a cautious path toward any new <span class="hlt">trade</span> arrangement with the United...Service Contents U.S. Preferential <span class="hlt">Trade</span> Programs and the Caribbean <span class="hlt">Region</span>.......................................................1 Background...finished products may then re-export them back to the United States, with duties levied only on the value added abroad (no tariff on U.S. content ).3</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A54A..07W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A54A..07W"><span><span class="hlt">Trade</span> cumulus clouds embedded in a deep <span class="hlt">regional</span> haze: Results from Indian Ocean CARDEX experiment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wilcox, E. M.; Thomas, R. M.; Praveen, P. S.; Pistone, K.; Bender, F.; Feng, Y.; Ramanathan, V.</p> <p>2013-12-01</p> <p>During the winter monsoon, <span class="hlt">trade</span> cumulus clouds over the North Indian Ocean are embedded within a deep <span class="hlt">regional</span> haze described as an atmospheric brown cloud. While the <span class="hlt">trade</span>-cu clouds are largely confined to the marine boundary layer, the sooty brown cloud extends from the boundary layer to as high as 3 km; well above the tops of the cumulus. The boundary layer pollution is persistent and limits drizzle in the cumulus over a period of greater than a month at the Maldives Climate Observatory located at Hanimaadhoo Island. The elevated haze from 1 to 3 km altitude is episodic and strongly modulated by synoptic variability in the 700 hPa flow. The elevated plume enhances heating above the marine boundary layer through daytime absorption of sunlight by the haze particles. The interplay between the microphysical modification of clouds by boundary layer pollution and the episodic elevated heating by the atmospheric brown cloud are explored in in-situ observations from UAVs and surface remote sensing during the CARDEX field campaign of winter 2012 and supported by multi-year analysis of satellite remote sensing observations. These observations document the variability in pollution at the surface and above the marine boundary layer and the effects of pollution on the microphysics of the <span class="hlt">trade</span>-cu clouds, the depth of the marine boundary layer, the liquid water path of <span class="hlt">trade</span>-cu clouds, and the profile of turbulent moisture flux through the boundary layer. The consequences of these effects for the radiative forcing of <span class="hlt">regional</span> climate will be discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMNG23A..07G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMNG23A..07G"><span>Sensitivity Analysis of Expected <span class="hlt">Wind</span> Extremes over the Northwestern Sahara and High Atlas <span class="hlt">Region</span>.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Garcia-Bustamante, E.; González-Rouco, F. J.; Navarro, J.</p> <p>2017-12-01</p> <p>A robust statistical framework in the scientific literature allows for the estimation of probabilities of occurrence of severe <span class="hlt">wind</span> speeds and <span class="hlt">wind</span> gusts, but does not prevent however from large uncertainties associated with the particular numerical estimates. An analysis of such uncertainties is thus required. A large portion of this uncertainty arises from the fact that historical observations are inherently shorter that the timescales of interest for the analysis of return periods. Additional uncertainties stem from the different choices of probability distributions and other aspects related to methodological issues or physical processes involved. The present study is focused on historical observations over the Ouarzazate Valley (Morocco) and in a high-resolution <span class="hlt">regional</span> simulation of the <span class="hlt">wind</span> in the area of interest. The aim is to provide extreme <span class="hlt">wind</span> speed and <span class="hlt">wind</span> gust return values and confidence ranges based on a systematic sampling of the uncertainty space for return periods up to 120 years.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3718187','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3718187"><span><span class="hlt">Regional</span> variations in the health, environmental, and climate benefits of <span class="hlt">wind</span> and solar generation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Siler-Evans, Kyle; Azevedo, Inês Lima; Morgan, M. Granger; Apt, Jay</p> <p>2013-01-01</p> <p>When <span class="hlt">wind</span> or solar energy displace conventional generation, the reduction in emissions varies dramatically across the United States. Although the Southwest has the greatest solar resource, a solar panel in New Jersey displaces significantly more sulfur dioxide, nitrogen oxides, and particulate matter than a panel in Arizona, resulting in 15 times more health and environmental benefits. A <span class="hlt">wind</span> turbine in West Virginia displaces twice as much carbon dioxide as the same turbine in California. Depending on location, we estimate that the combined health, environmental, and climate benefits from <span class="hlt">wind</span> or solar range from $10/MWh to $100/MWh, and the sites with the highest energy output do not yield the greatest social benefits in many cases. We estimate that the social benefits from existing <span class="hlt">wind</span> farms are roughly 60% higher than the cost of the Production Tax Credit, an important federal subsidy for <span class="hlt">wind</span> energy. However, that same investment could achieve greater health, environmental, and climate benefits if it were differentiated by <span class="hlt">region</span>. PMID:23798431</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23798431','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23798431"><span><span class="hlt">Regional</span> variations in the health, environmental, and climate benefits of <span class="hlt">wind</span> and solar generation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Siler-Evans, Kyle; Azevedo, Inês Lima; Morgan, M Granger; Apt, Jay</p> <p>2013-07-16</p> <p>When <span class="hlt">wind</span> or solar energy displace conventional generation, the reduction in emissions varies dramatically across the United States. Although the Southwest has the greatest solar resource, a solar panel in New Jersey displaces significantly more sulfur dioxide, nitrogen oxides, and particulate matter than a panel in Arizona, resulting in 15 times more health and environmental benefits. A <span class="hlt">wind</span> turbine in West Virginia displaces twice as much carbon dioxide as the same turbine in California. Depending on location, we estimate that the combined health, environmental, and climate benefits from <span class="hlt">wind</span> or solar range from $10/MWh to $100/MWh, and the sites with the highest energy output do not yield the greatest social benefits in many cases. We estimate that the social benefits from existing <span class="hlt">wind</span> farms are roughly 60% higher than the cost of the Production Tax Credit, an important federal subsidy for <span class="hlt">wind</span> energy. However, that same investment could achieve greater health, environmental, and climate benefits if it were differentiated by <span class="hlt">region</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/56027','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/56027"><span>Implications for U.S. <span class="hlt">trade</span> and nonindigenous species risk resulting from increased economic integration of the Asia-Pacific <span class="hlt">Region</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Amanda M. Countryman; Travis Warziniack; Erin Grey</p> <p>2018-01-01</p> <p>This work investigates how potential changes in <span class="hlt">trade</span> patterns resulting from increased economic integration in the Asia-Pacific <span class="hlt">region</span> may affect the risk for nonindigenous species spread to the United States. We construct an invasion risk index utilizing the results from a global economic modeling framework in tandem with data for climate similarities between <span class="hlt">trade</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19880005127','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19880005127"><span>Long-period variations of <span class="hlt">wind</span> parameters in the mesopause <span class="hlt">region</span> and the solar cycle dependence</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Greisiger, K. M.; Schminder, R.; Kuerschner, D.</p> <p>1987-01-01</p> <p>The solar cycle dependence of <span class="hlt">wind</span> parameters below 100 km on the basis of long term continuous ionospheric drift measurements in the low frequency range is discussed. For the meridional prevailing <span class="hlt">wind</span> no significant variation was found. The same comparison as for winter was done for summer where the previous investigations gave no correlation. Now the radar meteor <span class="hlt">wind</span> measurement values, too, showed a significant negative correlation of the zonal prevailing <span class="hlt">wind</span> with solar activity for the years 1976 to 1983. The ionospheric drift measurement results of Collm have the same tendency but a larger dispersion due to the lower accuracy of the harmonic analysis because of the shorter daily measuring interval in summer. Continuous <span class="hlt">wind</span> observations in the upper mesopause <span class="hlt">region</span> over more than 20 years revealed distinct long term variations, the origin of which cannot be explained with the present knowledge.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29793079','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29793079"><span>Shifts in <span class="hlt">wind</span> energy potential following land-use driven vegetation dynamics in complex terrain.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fang, Jiannong; Peringer, Alexander; Stupariu, Mihai-Sorin; Pǎtru-Stupariu, Ileana; Buttler, Alexandre; Golay, Francois; Porté-Agel, Fernando</p> <p>2018-10-15</p> <p>Many mountainous <span class="hlt">regions</span> with high <span class="hlt">wind</span> energy potential are characterized by multi-scale variabilities of vegetation in both spatial and time dimensions, which strongly affect the spatial distribution of <span class="hlt">wind</span> resource and its time evolution. To this end, we developed a coupled interdisciplinary modeling framework capable of assessing the shifts in <span class="hlt">wind</span> energy potential following land-use driven vegetation dynamics in complex mountain terrain. It was applied to a case study area in the Romanian Carpathians. The results show that the overall shifts in <span class="hlt">wind</span> energy potential following the changes of vegetation pattern due to different land-use policies can be dramatic. This suggests that the planning of <span class="hlt">wind</span> energy project should be integrated with the land-use planning at a specific site to ensure that the expected energy production of the planned <span class="hlt">wind</span> farm can be reached over its entire lifetime. Moreover, the changes in the spatial distribution of <span class="hlt">wind</span> and turbulence under different scenarios of land-use are complex, and they must be taken into account in the micro-siting of <span class="hlt">wind</span> turbines to maximize <span class="hlt">wind</span> energy production and minimize fatigue loads (and associated maintenance costs). The proposed new modeling framework offers, for the first time, a powerful tool for assessing long-term variability in local <span class="hlt">wind</span> energy potential that emerges from land-use change driven vegetation dynamics over complex terrain. Following a previously unexplored pathway of cause-effect relationships, it demonstrates a new linkage of agro- and forest policies in landscape development with an ultimate <span class="hlt">trade</span>-off between renewable energy production and biodiversity targets. Moreover, it can be extended to study the potential effects of micro-climatic changes associated with <span class="hlt">wind</span> farms on vegetation development (growth and patterning), which could in turn have a long-term feedback effect on <span class="hlt">wind</span> resource distribution in mountainous <span class="hlt">regions</span>. Copyright © 2018 Elsevier B.V. All rights</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017SPIE10466E..4XL','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017SPIE10466E..4XL"><span>Statistical modeling of temperature, humidity and <span class="hlt">wind</span> fields in the atmospheric boundary layer over the Siberian <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lomakina, N. Ya.</p> <p>2017-11-01</p> <p>The work presents the results of the applied climatic division of the Siberian <span class="hlt">region</span> into districts based on the methodology of objective classification of the atmospheric boundary layer climates by the "temperature-moisture-<span class="hlt">wind</span>" complex realized with using the method of principal components and the special similarity criteria of average profiles and the eigen values of correlation matrices. On the territory of Siberia, it was identified 14 homogeneous <span class="hlt">regions</span> for winter season and 10 <span class="hlt">regions</span> were revealed for summer. The local statistical models were constructed for each <span class="hlt">region</span>. These include vertical profiles of mean values, mean square deviations, and matrices of interlevel correlation of temperature, specific humidity, zonal and meridional <span class="hlt">wind</span> velocity. The advantage of the obtained local statistical models over the <span class="hlt">regional</span> models is shown.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-10-18/pdf/2012-25647.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-10-18/pdf/2012-25647.pdf"><span>77 FR 64106 - Renewable Energy and Energy Efficiency <span class="hlt">Trade</span> Policy Mission to Chile</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-10-18</p> <p>... competitiveness of U.S. <span class="hlt">wind</span>, solar, geothermal, biomass, hydropower, waste-to-energy, smart grid, and energy... development. Opportunities are expected in the <span class="hlt">wind</span>, solar, geothermal, biomass, hydropower, and energy... DEPARTMENT OF COMMERCE International <span class="hlt">Trade</span> Administration Renewable Energy and Energy Efficiency...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015JGRA..120.9004K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015JGRA..120.9004K"><span>Equatorial F <span class="hlt">region</span> neutral <span class="hlt">winds</span> and shears near sunset measured with chemical release techniques</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kiene, A.; Larsen, M. F.; Kudeki, E.</p> <p>2015-10-01</p> <p>The period near sunset is a dynamic and critical time for the daily development of the equatorial nighttime ionosphere and the instabilities that occur there. It is during these hours that the preconditions necessary for the later development of Equatorial Spread F (ESF) plasma instabilities occur. The neutral dynamics of the sunset ionosphere are also of critical importance to the generation of currents and electric fields; however, the behavior of the neutrals is experimentally understood primarily through very limited single-altitude measurements or measurements that provide weighted altitude means of the <span class="hlt">winds</span> as a function of time. To date, there have been very few vertically resolved neutral <span class="hlt">wind</span> measurements in the F <span class="hlt">region</span> at sunset. We present two sets of sounding rocket chemical release measurements, one from a launch in the Marshall Islands on Kwajalein atoll and one from Alcantara, Brazil. Analysis of the release motions has yielded vertically resolved neutral <span class="hlt">wind</span> profiles that show both the mean horizontal <span class="hlt">winds</span> and the vertical shears in the <span class="hlt">winds</span>. In both experiments, we observe significant vertical gradients in the zonal <span class="hlt">wind</span> that are unexpected by classical assumptions about the behavior of the neutral <span class="hlt">wind</span> at these altitudes at sunset near the geomagnetic equator.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29855433','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29855433"><span>Design of transcranial magnetic stimulation coils with optimal <span class="hlt">trade</span>-off between depth, focality, and energy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Gomez, Luis J; Goetz, Stefan M; Peterchev, Angel V</p> <p>2018-08-01</p> <p>Transcranial magnetic stimulation (TMS) is a noninvasive brain stimulation technique used for research and clinical applications. Existent TMS coils are limited in their precision of spatial targeting (focality), especially for deeper targets. This paper presents a methodology for designing TMS coils to achieve optimal <span class="hlt">trade</span>-off between the depth and focality of the induced electric field (E-field), as well as the energy required by the coil. A multi-objective optimization technique is used for computationally designing TMS coils that achieve optimal <span class="hlt">trade</span>-offs between E-field focality, depth, and energy (fdTMS coils). The fdTMS coil <span class="hlt">winding(s</span>) maximize focality (minimize the volume of the brain <span class="hlt">region</span> with E-field above a given threshold) while reaching a target at a specified depth and not exceeding predefined peak E-field strength and required coil energy. Spherical and MRI-derived head models are used to compute the fundamental depth-focality <span class="hlt">trade</span>-off as well as focality-energy <span class="hlt">trade</span>-offs for specific target depths. Across stimulation target depths of 1.0-3.4 cm from the brain surface, the suprathreshold volume can be theoretically decreased by 42%-55% compared to existing TMS coil designs. The suprathreshold volume of a figure-8 coil can be decreased by 36%, 44%, or 46%, for matched, doubled, or quadrupled energy. For matched focality and energy, the depth of a figure-8 coil can be increased by 22%. Computational design of TMS coils could enable more selective targeting of the induced E-field. The presented results appear to be the first significant advancement in the depth-focality <span class="hlt">trade</span>-off of TMS coils since the introduction of the figure-8 coil three decades ago, and likely represent the fundamental physical limit.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014GBioC..28..909R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014GBioC..28..909R"><span>Sensitivity of ocean oxygenation to variations in tropical zonal <span class="hlt">wind</span> stress magnitude</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ridder, Nina N.; England, Matthew H.</p> <p>2014-09-01</p> <p>Ocean oxygenation has been observed to have changed over the past few decades and is projected to change further under global climate change due to an interplay of several mechanisms. In this study we isolate the effect of modified tropical surface <span class="hlt">wind</span> stress conditions on the evolution of ocean oxygenation in a numerical climate model. We find that ocean oxygenation varies inversely with low-latitude surface <span class="hlt">wind</span> stress. Approximately one third of this response is driven by sea surface temperature anomalies; the remaining two thirds result from changes in ocean circulation and marine biology. Global mean O2 concentration changes reach maximum values of +4 μM and -3.6 μM in the two most extreme perturbation cases of -30% and +30% <span class="hlt">wind</span> change, respectively. Localized changes lie between +92 μM under 30% reduced <span class="hlt">winds</span> and -56 μM for 30% increased <span class="hlt">winds</span>. Overall, we find that the extent of the global low-oxygen volume varies with the same sign as the <span class="hlt">wind</span> perturbation; namely, weaker <span class="hlt">winds</span> reduce the low-oxygen volume on the global scale and vice versa for increased <span class="hlt">trade</span> <span class="hlt">winds</span>. We identify two <span class="hlt">regions</span>, one in the Pacific Ocean off Chile and the other in the Indian Ocean off Somalia, that are of particular importance for the evolution of oxygen minimum zones in the global ocean.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19778373','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19778373"><span>Needle traits of an evergreen, coniferous shrub growing at <span class="hlt">wind</span>-exposed and protected sites in a mountain <span class="hlt">region</span>: does Pinus pumila produce needles with greater mass per area under <span class="hlt">wind</span>-stress conditions?</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Nagano, S; Nakano, T; Hikosaka, K; Maruta, E</p> <p>2009-11-01</p> <p>Snow depth is one of the most important determinants of vegetation, especially in mountainous <span class="hlt">regions</span>. In such <span class="hlt">regions</span>, snow depth tends to be low at <span class="hlt">wind</span>-exposed sites such as ridges, where stand height and productivity are limited by stressful environmental conditions during winter. Siberian dwarf pine (Pinus pumila Regel) is a dominant species in mountainous <span class="hlt">regions</span> of Japan. We hypothesized that P. pumila produces needles with greater mass per area at <span class="hlt">wind</span>-exposed sites than at <span class="hlt">wind</span>-protected sites because it invests more nitrogen (N) in cell walls at the expense of N investment in the photosynthetic apparatus, resulting in increased photosynthetic N use efficiency (PNUE). Contrary to our hypothesis, plants at <span class="hlt">wind</span>-exposed site invested less resources in needles, as exhibited by lower biomass, N, Rubisco and cell wall mass per unit area, and had higher photosynthetic capacity, higher PNUE and shorter needle life-span than plants at a <span class="hlt">wind</span>-protected site. N partitioning was not significantly different between sites. These results suggest that P. pumila at <span class="hlt">wind</span>-exposed sites produces needles at low cost with high productivity to compensate for a short leaf life-span, which may be imposed by <span class="hlt">wind</span> stress when needles appear above the snow surface in winter.</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.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5750899','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5750899"><span>The Role of China in the UK Relative Imports from Three Selected <span class="hlt">Trading</span> <span class="hlt">Regions</span>: The Case of Textile Raw Material Industry</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Xu, Junqian</p> <p>2017-01-01</p> <p>The UK textile industry was very prosperous in the past but in the 1970s Britain started to import textile materials from abroad. Since 1990, half of its textile materials have been imported from the EEA (European Economic Area), ASEAN (Association of Southeast Asian Nations) and North America countries. Meanwhile, UK imports from China have increased dramatically. Through comparisons, this paper calculates the <span class="hlt">trade</span> competitiveness index and relative competitive advantages of <span class="hlt">regions</span> and investigates the impact of Chinese textiles on UK imports from three key free <span class="hlt">trade</span> <span class="hlt">regions</span> across the textile sectors in the period 1990–2016 on the basis of United Nation Comtrade Rev. 3. We find that China’s textile prices, product techniques, political <span class="hlt">trade</span> barriers and even tax system have made a varied impact on the UK’s imports across related sectors in the context of green <span class="hlt">trade</span> and the strengthening of barriers, which helps us recognize China’s competitiveness in international <span class="hlt">trading</span> and also provides advice on China’s sustainable development of textile exports. PMID:29189756</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA20799.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA20799.html"><span><span class="hlt">Wind</span> Etching</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2016-08-09</p> <p>Today's VIS image is located in a <span class="hlt">region</span> that has been heavily modified by <span class="hlt">wind</span> action. The narrow ridge/valley system seen in this image are a feature called yardangs. Yardangs form when unidirectional <span class="hlt">winds</span> blow across poorly cemented materials. Multiple yardang directions can indicate changes in <span class="hlt">regional</span> <span class="hlt">wind</span> regimes. Orbit Number: 64188 Latitude: -0.629314 Longitude: 206.572 Instrument: VIS Captured: 2016-06-03 01:20 http://photojournal.jpl.nasa.gov/catalog/PIA20799</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JGRA..123..211D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JGRA..123..211D"><span>On the Relation Between Soft Electron Precipitations in the Cusp <span class="hlt">Region</span> and Solar <span class="hlt">Wind</span> Coupling Functions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dang, Tong; Zhang, Binzheng; Wiltberge, Michael; Wang, Wenbin; Varney, Roger; Dou, Xiankang; Wan, Weixing; Lei, Jiuhou</p> <p>2018-01-01</p> <p>In this study, the correlations between the fluxes of precipitating soft electrons in the cusp <span class="hlt">region</span> and solar <span class="hlt">wind</span> coupling functions are investigated utilizing the Lyon-Fedder-Mobarry global magnetosphere model simulations. We conduct two simulation runs during periods from 20 March 2008 to 16 April 2008 and from 15 to 24 December 2014, which are referred as "Equinox Case" and "Solstice Case," respectively. The simulation results of Equinox Case show that the plasma number density in the high-latitude cusp <span class="hlt">region</span> scales well with the solar <span class="hlt">wind</span> number density (ncusp/nsw=0.78), which agrees well with the statistical results from the Polar spacecraft measurements. For the Solstice Case, the plasma number density of high-latitude cusp in both hemispheres increases approximately linearly with upstream solar <span class="hlt">wind</span> number density with prominent hemispheric asymmetry. Due to the dipole tilt effect, the average number density ratio ncusp/nsw in the Southern (summer) Hemisphere is nearly 3 times that in the Northern (winter) Hemisphere. In addition to the solar <span class="hlt">wind</span> number density, 20 solar <span class="hlt">wind</span> coupling functions are tested for the linear correlation with the fluxes of precipitating cusp soft electrons. The statistical results indicate that the solar <span class="hlt">wind</span> dynamic pressure p exhibits the highest linear correlation with the cusp electron fluxes for both equinox and solstice conditions, with correlation coefficients greater than 0.75. The linear regression relations for equinox and solstice cases may provide an empirical calculation for the fluxes of cusp soft electron precipitation based on the upstream solar <span class="hlt">wind</span> driving conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017NatEn...217134M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017NatEn...217134M"><span>The climate and air-quality benefits of <span class="hlt">wind</span> and solar power in the 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>Millstein, Dev; Wiser, Ryan; Bolinger, Mark; Barbose, Galen</p> <p>2017-09-01</p> <p><span class="hlt">Wind</span> and solar energy reduce combustion-based electricity generation and provide air-quality and greenhouse gas emission benefits. These benefits vary dramatically by <span class="hlt">region</span> and over time. From 2007 to 2015, solar and <span class="hlt">wind</span> power deployment increased rapidly while regulatory changes and fossil fuel price changes led to steep cuts in overall power-sector emissions. Here we evaluate how <span class="hlt">wind</span> and solar climate and air-quality benefits evolved during this time period. We find cumulative <span class="hlt">wind</span> and solar air-quality benefits of 2015 US$29.7-112.8 billion mostly from 3,000 to 12,700 avoided premature mortalities, and cumulative climate benefits of 2015 US$5.3-106.8 billion. The ranges span results across a suite of air-quality and health impact models and social cost of carbon estimates. We find that binding cap-and-<span class="hlt">trade</span> pollutant markets may reduce these cumulative benefits by up to 16%. In 2015, based on central estimates, combined marginal benefits equal 7.3 ¢ kWh-1 (<span class="hlt">wind</span>) and 4.0 ¢ kWh-1 (solar).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1157F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018MNRAS.tmp.1157F"><span>Helium abundance and speed difference between helium ions and protons in the solar <span class="hlt">wind</span> from coronal holes, active <span class="hlt">regions</span>, and quiet Sun</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Fu, Hui; Madjarska, M. S.; Li, Bo; Xia, LiDong; Huang, ZhengHua</p> <p>2018-05-01</p> <p>Two main models have been developed to explain the mechanisms of release, heating and acceleration of the nascent solar <span class="hlt">wind</span>, the wave-turbulence-driven (WTD) models and reconnection-loop-opening (RLO) models, in which the plasma release processes are fundamentally different. Given that the statistical observational properties of helium ions produced in magnetically diverse solar <span class="hlt">regions</span> could provide valuable information for the solar <span class="hlt">wind</span> modelling, we examine the statistical properties of the helium abundance (AHe) and the speed difference between helium ions and protons (vαp) for coronal holes (CHs), active <span class="hlt">regions</span> (ARs) and the quiet Sun (QS). We find bimodal distributions in the space of AHeand vαp/vA(where vA is the local Alfvén speed) for the solar <span class="hlt">wind</span> as a whole. The CH <span class="hlt">wind</span> measurements are concentrated at higher AHeand vαp/vAvalues with a smaller AHedistribution range, while the AR and QS <span class="hlt">wind</span> is associated with lower AHeand vαp/vA, and a larger AHedistribution range. The magnetic diversity of the source <span class="hlt">regions</span> and the physical processes related to it are possibly responsible for the different properties of AHeand vαp/vA. The statistical results suggest that the two solar <span class="hlt">wind</span> generation mechanisms, WTD and RLO, work in parallel in all solar <span class="hlt">wind</span> source <span class="hlt">regions</span>. In CH <span class="hlt">regions</span> WTD plays a major role, whereas the RLO mechanism is more important in AR and QS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-02-15/pdf/2013-03728.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-02-15/pdf/2013-03728.pdf"><span>78 FR 11152 - Utility Scale <span class="hlt">Wind</span> Towers from the People's Republic of China: Countervailing Duty Order</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-02-15</p> <p>... DEPARTMENT OF COMMERCE International <span class="hlt">Trade</span> Administration [C-570-982] Utility Scale <span class="hlt">Wind</span> Towers...''), the Department is issuing a countervailing duty order on utility scale <span class="hlt">wind</span> towers (``<span class="hlt">wind</span> towers..., 2012, the Department published the final determination in the countervailing duty investigation of <span class="hlt">wind</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1117052','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1117052"><span>The <span class="hlt">Wind</span> Integration National Dataset (<span class="hlt">WIND</span>) toolkit (Presentation)</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>Caroline Draxl: NREL</p> <p>2014-01-01</p> <p><span class="hlt">Regional</span> <span class="hlt">wind</span> integration studies require detailed <span class="hlt">wind</span> power output data at many locations to perform simulations of how the power system will operate under high penetration scenarios. The <span class="hlt">wind</span> datasets that serve as inputs into the study must realistically reflect the ramping characteristics, spatial and temporal correlations, and capacity factors of the simulated <span class="hlt">wind</span> plants, as well as being time synchronized with available load profiles.As described in this presentation, the <span class="hlt">WIND</span> Toolkit fulfills these requirements by providing a state-of-the-art national (US) <span class="hlt">wind</span> resource, power production and forecast dataset.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26938494','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26938494"><span>The effect of inter-annual variability of consumption, production, <span class="hlt">trade</span> and climate on crop-related green and blue water footprints and inter-<span class="hlt">regional</span> virtual water <span class="hlt">trade</span>: A study for China (1978-2008).</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhuo, La; Mekonnen, Mesfin M; Hoekstra, Arjen Y</p> <p>2016-05-01</p> <p>Previous studies into the relation between human consumption and indirect water resources use have unveiled the remote connections in virtual water (VW) <span class="hlt">trade</span> networks, which show how communities externalize their water footprint (WF) to places far beyond their own <span class="hlt">region</span>, but little has been done to understand variability in time. This study quantifies the effect of inter-annual variability of consumption, production, <span class="hlt">trade</span> and climate on WF and VW <span class="hlt">trade</span>, using China over the period 1978-2008 as a case study. Evapotranspiration, crop yields and green and blue WFs of crops are estimated at a 5 × 5 arc-minute resolution for 22 crops, for each year in the study period, thus accounting for climate variability. The results show that crop yield improvements during the study period helped to reduce the national average WF of crop consumption per capita by 23%, with a decreasing contribution to the total from cereals and increasing contribution from oil crops. The total consumptive WFs of national crop consumption and crop production, however, grew by 6% and 7%, respectively. By 2008, 28% of total water consumption in crop fields in China served the production of crops for export to other <span class="hlt">regions</span> and, on average, 35% of the crop-related WF of a Chinese consumer was outside its own province. Historically, the net VW within China was from the water-rich South to the water-scarce North, but intensifying North-to-South crop <span class="hlt">trade</span> reversed the net VW flow since 2000, which amounted 6% of North's WF of crop production in 2008. South China thus gradually became dependent on food supply from the water-scarce North. Besides, during the whole study period, China's domestic inter-<span class="hlt">regional</span> VW flows went dominantly from areas with a relatively large to areas with a relatively small blue WF per unit of crop, which in 2008 resulted in a <span class="hlt">trade</span>-related blue water loss of 7% of the national total blue WF of crop production. The case of China shows that domestic <span class="hlt">trade</span>, as governed by</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010ems..confE.213M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010ems..confE.213M"><span>Dynamical downscaling of <span class="hlt">wind</span> fields for <span class="hlt">wind</span> power applications</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mengelkamp, H.-T.; Huneke, S.; Geyer, J.</p> <p>2010-09-01</p> <p>Dynamical downscaling of <span class="hlt">wind</span> fields for <span class="hlt">wind</span> power applications H.-T. Mengelkamp*,**, S. Huneke**, J, Geyer** *GKSS Research Center Geesthacht GmbH **anemos Gesellschaft für Umweltmeteorologie mbH Investments in <span class="hlt">wind</span> power require information on the long-term mean <span class="hlt">wind</span> potential and its temporal variations on daily to annual and decadal time scales. This information is rarely available at specific <span class="hlt">wind</span> farm sites. Short-term on-site measurements usually are only performed over a 12 months period. These data have to be set into the long-term perspective through correlation to long-term consistent <span class="hlt">wind</span> data sets. Preliminary <span class="hlt">wind</span> information is often asked for to select favourable <span class="hlt">wind</span> sites over <span class="hlt">regional</span> and country wide scales. Lack of high-quality <span class="hlt">wind</span> measurements at weather stations was the motivation to start high resolution <span class="hlt">wind</span> field simulations The simulations are basically a refinement of global scale reanalysis data by means of high resolution simulations with an atmospheric mesoscale model using high-resolution terrain and land-use data. The 3-dimensional representation of the atmospheric state available every six hours at 2.5 degree resolution over the globe, known as NCAR/NCEP reanalysis data, forms the boundary conditions for continuous simulations with the non-hydrostatic atmospheric mesoscale model MM5. MM5 is nested in itself down to a horizontal resolution of 5 x 5 km². The simulation is performed for different European countries and covers the period 2000 to present and is continuously updated. Model variables are stored every 10 minutes for various heights. We have analysed the <span class="hlt">wind</span> field primarily. The <span class="hlt">wind</span> data set is consistent in space and time and provides information on the <span class="hlt">regional</span> distribution of the long-term mean <span class="hlt">wind</span> potential, the temporal variability of the <span class="hlt">wind</span> potential, the vertical variation of the <span class="hlt">wind</span> potential, and the temperature, and pressure distribution (air density). In the context of <span class="hlt">wind</span> power these data are used </p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.1940C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.1940C"><span>A <span class="hlt">Wind</span> Forecasting System for Energy Application</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Courtney, Jennifer; Lynch, Peter; Sweeney, Conor</p> <p>2010-05-01</p> <p> probabilistic <span class="hlt">wind</span> forecasts which will be invaluable in <span class="hlt">wind</span> energy management. In brief, this method turns the ensemble forecasts into a calibrated predictive probability distribution. Each ensemble member is provided with a 'weight' determined by its relative predictive skill over a training period of around 30 days. Verification of data is carried out using observed <span class="hlt">wind</span> data from operational <span class="hlt">wind</span> farms. These are then compared to existing forecasts produced by ECMWF and Met Eireann in relation to skill scores. We are developing decision-making models to show the benefits achieved using the data produced by our <span class="hlt">wind</span> energy forecasting system. An energy <span class="hlt">trading</span> model will be developed, based on the rules currently used by the Single Electricity Market Operator for energy <span class="hlt">trading</span> in Ireland. This <span class="hlt">trading</span> model will illustrate the potential for financial savings by using the forecast data generated by this research.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AtmRe.122..486W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AtmRe.122..486W"><span>Mesoscale modeling of smoke transport over the Southeast Asian Maritime Continent: Interplay of sea breeze, <span class="hlt">trade</span> <span class="hlt">wind</span>, typhoon, and topography</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Jun; Ge, Cui; Yang, Zhifeng; Hyer, Edward J.; Reid, Jeffrey S.; Chew, Boon-Ning; Mahmud, Mastura; Zhang, Yongxin; Zhang, Meigen</p> <p>2013-03-01</p> <p>The online-coupled Weather Research and Forecasting model with Chemistry (WRFchem) is used to simulate the transport of smoke particles over the Southeast Asian Maritime Continent during September-October 2006. In this period, dry conditions associated with the moderate El Niño event caused the largest <span class="hlt">regional</span> biomass burning outbreak since 1997. Smoke emission in WRFchem is specified according to the Fire Locating and Modeling of Burning Emissions (FLAMBE) database derived from Moderate Resolution Imaging Spectroradiometer (MODIS) fire products. The modeled smoke transport pathway is found to be consistent with the MODIS true color images and measured mass concentration of surface PM10 (particulate matter with diameter less than 10 μm). The interplay of sea/land breezes, typhoons and storms over the subtropical western Pacific Ocean, <span class="hlt">trade</span> <span class="hlt">winds</span>, and topographic effects, can be clearly seen in the model simulation. The most severe smoke events in 1-5 October 2006 are found to be associated with the meteorological responses to the typhoon Xangsane (#18) over the western subtropical Pacific Ocean, which moved smoke from Sumatra eastward in the lower troposphere (below 700 hPa), forming smoke layers mixed with and above the boundary layer clouds over Borneo. In contrast, the second largest week-long smoke transport event of 15-18 October 2006 was associated with the seasonal monsoonal transition period, during which smoke plumes were wide spread over the 5°S-5°N zone as a result of (a) the near surface divergence coupled with the 700 hPa bifurcation of <span class="hlt">wind</span> (flowing both to the west and to the east), and (b) the near-surface southeasterly and easterly <span class="hlt">winds</span> along the equator transporting smoke from Borneo to Sumatra and Peninsular Malaysia. Analysis of data from the Cloud-Aerosol Lidar with Orthogonal Polarisation (CALIOP) shows that smoke particles in October 2006 were primarily located within 3.5 km above the surface. Smoke particles contributed roughly half</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018DyAtO..82...76Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018DyAtO..82...76Y"><span>The 10-30-day oscillation of winter zonal <span class="hlt">wind</span> in the entrance <span class="hlt">region</span> of the East Asian subtropical jet and its relationship with precipitation in southern China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yao, Chenyu; Huang, Qian; Zhu, Bin; Liu, Fei</p> <p>2018-06-01</p> <p>Using ECMWF ERA-Interim 6-h reanalysis data, zonal <span class="hlt">wind</span> intra-seasonal oscillations (ISOs) in the entrance <span class="hlt">region</span> of the East Asian subtropical westerly jet (EASWJ) in winter from 1979/1980 to 2012/2013 are studied. The results first show that there is an area with large ISO strength in the northwest of the EASWJ; in the key <span class="hlt">region</span>, zonal <span class="hlt">wind</span> has a dominant period of 10-30 days. The composite analysis reveals that zonal <span class="hlt">wind</span> at 200 hPa in this key <span class="hlt">region</span> has 10-30-day oscillation characteristics. On the 10-30-day time scale, the center of zonal <span class="hlt">wind</span> anomaly moves eastward. The propagation of zonal <span class="hlt">wind</span> oscillation relates to temperature tendencies at different latitudes. The remarkable increase (or decrease) in zonal <span class="hlt">wind</span> in the key <span class="hlt">region</span> is mostly determined by temperature anomalies to the north. The 10-30-day filtered temperature advection to the north of the key <span class="hlt">region</span> leads to either a decrease or an increase in temperature; on the other hand, temperature variations south of the key <span class="hlt">region</span> have trends opposite of the northern trends, which changes the temperature gradient. On the 10-30-day time scale, zonal <span class="hlt">wind</span> anomalies are associated with precipitation in southern China. When there are easterly <span class="hlt">wind</span> anomalies over the key <span class="hlt">region</span>, precipitation occurs over the Yangtze River basin and its south. Diabatic heating during precipitation corresponds with warming to the south of the key <span class="hlt">region</span>, which combines with the temperature advection to weaken the easterly <span class="hlt">wind</span> and strengths the westerly <span class="hlt">wind</span>. Then, the intra-seasonal precipitation moves to southwest China with warm advection and the enhanced westerly <span class="hlt">wind</span>, which brings the positive relative vorticity advection there.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018JASTP.171...64R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018JASTP.171...64R"><span>The influence of tidal <span class="hlt">winds</span> in the formation of blanketing sporadic e-layer over equatorial Brazilian <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resende, Laysa Cristina Araujo; Batista, Inez Staciarini; Denardini, Clezio Marcos; Batista, Paulo Prado; Carrasco, Alexander José; Andrioli, Vânia Fátima; Moro, Juliano</p> <p>2018-06-01</p> <p>This work analysis the blanketing sporadic layers (Esb) behavior over São Luís, Brazil (2° 31‧ S, 44° 16‧ W, dip: -4.80) which is classified as a transition <span class="hlt">region</span> between equatorial and low-latitude. Hence, some peculiarities can appear as Esb occurrence instead of the common Esq, which is a non-blanketing irregularity layer. The analysis presented here was obtained using a modified version of a theoretical model for the E <span class="hlt">region</span> (MIRE), which computes the densities of the metallic ions (Fe+ and Mg+) and the densities of the main molecular ions (NO+, O2+, N2+) by solving the continuity and momentum equations for each one of them. In that model, the Es layer physics driven by both diurnal and semidiurnal tidal <span class="hlt">winds</span> are taken into account and it was extended in height coverage by adding a novel neutral <span class="hlt">wind</span> model derived from the all-sky meteor radar measurements. Thus, we provide more trustworthy results related to the Es layer formation in the equatorial <span class="hlt">region</span>. We verified the contribution of each tidal <span class="hlt">wind</span> component to the Esb layer formation in this equatorial <span class="hlt">region</span>. Additionally, we compared the Es layer electron density computed by MIRE with the data obtained by using the blanketing frequency parameter (fbEs) deduced from ionograms. The results show that the diurnal component of the tidal <span class="hlt">wind</span> is more important in the Esb layer formation whereas the semidiurnal component has a little contribution in our simulations. Finally, it was verified that the modified MIRE presented here can be used to study the Esb layers occurrence over the equatorial <span class="hlt">region</span> in the Brazilian sector.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20070032968&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbackground%2Bwind','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20070032968&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3Dbackground%2Bwind"><span>Dust Devil Tracks and <span class="hlt">Wind</span> Streaks in the North Polar <span class="hlt">Region</span> of Mars: A Study of the 2007 Phoenix Mars Lander Sites</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Drake, Nathan B.; Tamppari, Leslie K.; Baker, R. David; Cantor, Bruce A.; Hale, Amy S.</p> <p>2006-01-01</p> <p>The 65-72 latitude band of the North Polar <span class="hlt">Region</span> of Mars, where the 2007 Phoenix Mars Lander will land, was studied using satellite images from the Mars Global Surveyor (MGS) Mars Orbiter Camera Narrow-Angle (MOC-NA) camera. Dust devil tracks (DDT) and <span class="hlt">wind</span> streaks (WS) were observed and recorded as surface evidence for <span class="hlt">winds</span>. No active dust devils (DDs) were observed. 162 MOC-NA images, 10.3% of total images, contained DDT/WS. Phoenix landing <span class="hlt">Region</span> C (295-315W) had the highest concentration of images containing DDT/WS per number of available images (20.9%); <span class="hlt">Region</span> D (130-150W) had the lowest (3.5%). DDT and WS direction were recorded for Phoenix landing <span class="hlt">regions</span> A (110-130W), B (240-260W), and C to infer local <span class="hlt">wind</span> direction. <span class="hlt">Region</span> A showed dominant northwest-southeast DDT/WS, <span class="hlt">Region</span> B showed dominant north-south, east-west and northeast-southwest DDT/WS, and <span class="hlt">region</span> C showed dominant west/northwest - east/southeast DDT/ WS. Results indicate the 2007 Phoenix Lander has the highest probability of landing near DDT/WS in landing <span class="hlt">Region</span> C. Based on DDT/WS linearity, we infer Phoenix would likely encounter directionally consistent background <span class="hlt">wind</span> in any of the three <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1449846','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=1449846"><span>Global <span class="hlt">Trade</span> and Public Health</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Shaffer, Ellen R.; Waitzkin, Howard; Brenner, Joseph; Jasso-Aguilar, Rebeca</p> <p>2005-01-01</p> <p>Global <span class="hlt">trade</span> and international <span class="hlt">trade</span> agreements have transformed the capacity of governments to monitor and to protect public health, to regulate occupational and environmental health conditions and food products, and to ensure affordable access to medications. Proposals under negotiation for the World <span class="hlt">Trade</span> Organization’s General Agreement on <span class="hlt">Trade</span> in Services (GATS) and the <span class="hlt">regional</span> Free <span class="hlt">Trade</span> Area of the Americas (FTAA) agreement cover a wide range of health services, health facilities, clinician licensing, water and sanitation services, and tobacco and alcohol distribution services. Public health professionals and organizations rarely participate in <span class="hlt">trade</span> negotiations or in resolution of <span class="hlt">trade</span> disputes. The linkages among global <span class="hlt">trade</span>, international <span class="hlt">trade</span> agreements, and public health deserve more attention than they have received to date. PMID:15623854</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-02-15/pdf/2013-03727.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-02-15/pdf/2013-03727.pdf"><span>78 FR 11146 - Utility Scale <span class="hlt">Wind</span> Towers From the People's Republic of China: Antidumping Duty Order</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-02-15</p> <p>... DEPARTMENT OF COMMERCE International <span class="hlt">Trade</span> Administration [A-570-981] Utility Scale <span class="hlt">Wind</span> Towers...''), the Department is issuing an antidumping duty order on utility scale <span class="hlt">wind</span> towers (``<span class="hlt">wind</span> towers... investigation of <span class="hlt">wind</span> towers from the PRC.\\1\\ On February 8, 2013, the ITC notified the Department of its...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27872902','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27872902"><span><span class="hlt">Wind</span> energy potential assessment of Cameroon's coastal <span class="hlt">regions</span> for the installation of an onshore <span class="hlt">wind</span> farm.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Arreyndip, Nkongho Ayuketang; Joseph, Ebobenow; David, Afungchui</p> <p>2016-11-01</p> <p>For the future installation of a <span class="hlt">wind</span> farm in Cameroon, the <span class="hlt">wind</span> energy potentials of three of Cameroon's coastal cities (Kribi, Douala and Limbe) are assessed using NASA average monthly <span class="hlt">wind</span> data for 31 years (1983-2013) and compared through Weibull statistics. The Weibull parameters are estimated by the method of maximum likelihood, the mean power densities, the maximum energy carrying <span class="hlt">wind</span> speeds and the most probable <span class="hlt">wind</span> speeds are also calculated and compared over these three cities. Finally, the cumulative <span class="hlt">wind</span> speed distributions over the wet and dry seasons are also analyzed. The results show that the shape and scale parameters for Kribi, Douala and Limbe are 2.9 and 2.8, 3.9 and 1.8 and 3.08 and 2.58, respectively. The mean power densities through Weibull analysis for Kribi, Douala and Limbe are 33.7 W/m2, 8.0 W/m2 and 25.42 W/m2, respectively. Kribi's most probable <span class="hlt">wind</span> speed and maximum energy carrying <span class="hlt">wind</span> speed was found to be 2.42 m/s and 3.35 m/s, 2.27 m/s and 3.03 m/s for Limbe and 1.67 m/s and 2.0 m/s for Douala, respectively. Analysis of the <span class="hlt">wind</span> speed and hence power distribution over the wet and dry seasons shows that in the wet season, August is the windiest month for Douala and Limbe while September is the windiest month for Kribi while in the dry season, March is the windiest month for Douala and Limbe while February is the windiest month for Kribi. In terms of mean power density, most probable <span class="hlt">wind</span> speed and <span class="hlt">wind</span> speed carrying maximum energy, Kribi shows to be the best site for the installation of a <span class="hlt">wind</span> farm. Generally, the <span class="hlt">wind</span> speeds at all three locations seem quite low, average <span class="hlt">wind</span> speeds of all the three studied locations fall below 4.0m/s which is far below the cut-in <span class="hlt">wind</span> speed of many modern <span class="hlt">wind</span> turbines. However we recommend the use of low cut-in speed <span class="hlt">wind</span> turbines like the Savonius for stand alone low energy needs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...843L..19M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...843L..19M"><span>Superluminous Transients at AGN Centers from Interaction between Black Hole Disk <span class="hlt">Winds</span> and Broad-line <span class="hlt">Region</span> Clouds</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Moriya, Takashi J.; Tanaka, Masaomi; Morokuma, Tomoki; Ohsuga, Ken</p> <p>2017-07-01</p> <p>We propose that superluminous transients that appear at central <span class="hlt">regions</span> of active galactic nuclei (AGNs) such as CSS100217:102913+404220 (CSS100217) and PS16dtm, which reach near- or super-Eddington luminosities of the central black holes, are powered by the interaction between accretion-disk <span class="hlt">winds</span> and clouds in broad-line <span class="hlt">regions</span> (BLRs) surrounding them. If the disk luminosity temporarily increases by, e.g., limit-cycle oscillations, leading to a powerful radiatively driven <span class="hlt">wind</span>, strong shock waves propagate in the BLR. Because the dense clouds in the AGN BLRs typically have similar densities to those found in SNe IIn, strong radiative shocks emerge and efficiently convert the ejecta kinetic energy to radiation. As a result, transients similar to SNe IIn can be observed at AGN central <span class="hlt">regions</span>. Since a typical black hole disk-<span class="hlt">wind</span> velocity is ≃0.1c, where c is the speed of light, the ejecta kinetic energy is expected to be ≃1052 erg when ≃1 M ⊙ is ejected. This kinetic energy is transformed to radiation energy in a timescale for the <span class="hlt">wind</span> to sweep up a similar mass to itself in the BLR, which is a few hundred days. Therefore, both luminosities (˜1044 erg s-1) and timescales (˜100 days) of the superluminous transients from AGN central <span class="hlt">regions</span> match those expected in our interaction model. If CSS100217 and PS16dtm are related to the AGN activities triggered by limit-cycle oscillations, they become bright again in coming years or decades.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814782S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814782S"><span><span class="hlt">Regional</span> Climate Modelling of the Western Iberian Low-Level <span class="hlt">Wind</span> Jet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soares, Pedro M. M.; Lima, Daniela C. A.; Cardoso, Rita M.; Semedo, Álvaro</p> <p>2016-04-01</p> <p>The Iberian coastal low-level jet (CLLJ) is one the less studied boundary layer <span class="hlt">wind</span> jet features in the Eastern Boundary Currents Systems (EBCS). These <span class="hlt">regions</span> are amongst the most productive ocean ecosystems, where the atmosphere-land-ocean feedbacks, which include marine boundary layer clouds, coastal jets, upwelling and inland soil temperature and moisture, play an important role in defining the <span class="hlt">regional</span> climate along the sub-tropical mid-latitude western coastal areas. Recently, the present climate western Iberian CLLJ properties were extensively described using a high resolution <span class="hlt">regional</span> climate hindcast simulation. A summer maximum frequency of occurrence above 30% was found, with mean maximum <span class="hlt">wind</span> speeds around 15 ms-1, between 300 and 400m heights (at the jet core). Since the 1990s the climate change impact on the EBCS is being studied, nevertheless some lack of consensus still persists regarding the evolution of upwelling and other components of the climate system in these areas. However, recently some authors have shown that changes are to be expected concerning the timing, intensity and spatial homogeneity of coastal upwelling and of CLLJs, in response to future warming, especially at higher latitudes, namely in Iberia and Canaries. In this study, the first climate change assessment study regarding the Western Iberian CLLJ, using a high resolution (9km) <span class="hlt">regional</span> climate simulation, is presented. The properties of this CLLJ are studied and compared using two 30 years simulations: one historical simulation for the 1971-2000 period, and another simulation for future climate, in agreement with the RCP8.5 scenario, for the 2071-2100 period. Robust and consistent changes are found: 1) the hourly frequency of occurrence of the CLLJ is expected to increase in summer along the western Iberian coast, from mean maximum values of around 35% to approximately 50%; 2) the relative increase of the CLLJ frequency of occurrence is higher in the north off western Iberia</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-10-09/pdf/2012-23238.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-10-09/pdf/2012-23238.pdf"><span>77 FR 61477 - Approval and Promulgation of Implementation Plans; State of Hawaii; <span class="hlt">Regional</span> Haze Federal...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-10-09</p> <p>... Maui is subjected to strong <span class="hlt">trade</span> <span class="hlt">winds</span> on many days, and plantation practices of clearing and tilling... harvest, the cane fields are left bare and the loose topsoil is picked up by the <span class="hlt">trade</span> <span class="hlt">winds</span> and carried...</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/2017JPhCS.901a2006J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.901a2006J"><span>Time variations of oxygen emission lines and solar <span class="hlt">wind</span> dynamic parameters in low latitude <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jamlongkul, P.; Wannawichian, S.; Mkrtichian, D.; Sawangwit, U.; A-thano, N.</p> <p>2017-09-01</p> <p>Aurora phenomenon is an effect of collision between precipitating particles with gyromotion along Earth’s magnetic field and Earth’s ionospheric atoms or molecules. The particles’ precipitation occurs normally around polar <span class="hlt">regions</span>. However, some auroral particles can reach lower latitude <span class="hlt">regions</span> when they are highly energetic. A clear emission from Earth’s aurora is mostly from atomic oxygen. Moreover, the sun’s activities can influence the occurrence of the aurora as well. This work studies time variations of oxygen emission lines and solar <span class="hlt">wind</span> parameters, simultaneously. The emission’s spectral lines were observed by Medium Resolution Echelle Spectrograph (MRES) along with 2.4 meters diameter telescope at Thai National Observatory, Intanon Mountain, Chiang Mai, Thailand. Oxygen (OI) emission lines were calibrated by Dech-Fits spectra processing program and Dech95 2D image processing program. The correlations between oxygen emission lines and solar <span class="hlt">wind</span> dynamics will be analyzed. This result could be an evidence of the aurora in low latitude <span class="hlt">region</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1290783-variability-large-scale-wind-power-generation-variability-large-scale-wind-power-generation','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1290783-variability-large-scale-wind-power-generation-variability-large-scale-wind-power-generation"><span>Variability in large-scale <span class="hlt">wind</span> power generation: Variability in large-scale <span class="hlt">wind</span> power generation</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>Kiviluoma, Juha; Holttinen, Hannele; Weir, David</p> <p>2015-10-25</p> <p>The paper demonstrates the characteristics of <span class="hlt">wind</span> power variability and net load variability in multiple power systems based on real data from multiple years. Demonstrated characteristics include probability distribution for different ramp durations, seasonal and diurnal variability and low net load events. The comparison shows <span class="hlt">regions</span> with low variability (Sweden, Spain and Germany), medium variability (Portugal, Ireland, Finland and Denmark) and <span class="hlt">regions</span> with higher variability (Quebec, Bonneville Power Administration and Electric Reliability Council of Texas in North America; Gansu, Jilin and Liaoning in China; and Norway and offshore <span class="hlt">wind</span> power in Denmark). For <span class="hlt">regions</span> with low variability, the maximum 1more » h <span class="hlt">wind</span> ramps are below 10% of nominal capacity, and for <span class="hlt">regions</span> with high variability, they may be close to 30%. <span class="hlt">Wind</span> power variability is mainly explained by the extent of geographical spread, but also higher capacity factor causes higher variability. It was also shown how <span class="hlt">wind</span> power ramps are autocorrelated and dependent on the operating output level. When <span class="hlt">wind</span> power was concentrated in smaller area, there were outliers with high changes in <span class="hlt">wind</span> output, which were not present in large areas with well-dispersed <span class="hlt">wind</span> power.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820046923&hterms=WIND+STORMS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DWIND%2BSTORMS','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820046923&hterms=WIND+STORMS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DWIND%2BSTORMS"><span>The influence of solar active <span class="hlt">region</span> evolution on solar <span class="hlt">wind</span> streams, coronal hole boundaries and geomagnetic storms</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gold, R. E.; Dodson-Prince, H. W.; Hedeman, E. R.; Roelof, E. C.</p> <p>1982-01-01</p> <p>Solar and interplanetary data are examined, taking into account the identification of the heliographic longitudes of the coronal source <span class="hlt">regions</span> of high speed solar <span class="hlt">wind</span> (SW) streams by Nolte and Roelof (1973). Nolte and Roelof have 'mapped' the velocities measured near earth back to the sun using the approximation of constant radial velocity. The 'Carrington carpet' for rotations 1597-1616 is shown in a graph. Coronal sources of high speed streams appear in the form of solid black areas. The contours of the stream sources are laid on 'evolutionary charts' of solar active <span class="hlt">region</span> histories for the Southern and Northern Hemispheres. Questions regarding the interplay of active <span class="hlt">regions</span> and solar <span class="hlt">wind</span> are investigated, giving attention to developments during the years 1973, 1974, and 1975.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A51H2179Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A51H2179Z"><span>Distinctive Features of Surface <span class="hlt">Winds</span> over Indian Ocean Between Strong and Weak Indian Summer Monsoons: Implications With Respect To <span class="hlt">Regional</span> Rainfall Change in India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zheng, Y.; Bourassa, M. A.; Ali, M. M.</p> <p>2017-12-01</p> <p>This observational study focuses on characterizing the surface <span class="hlt">winds</span> in the Arabian Sea (AS), the Bay of Bengal (BoB), and the southern Indian Ocean (SIO) with special reference to the strong and weak Indian summer monsoon rainfall (ISMR) using the latest daily gridded rainfall dataset provided by the Indian Meteorological Department (IMD) and the Cross-Calibrated Multi-Platform (CCMP) gridded <span class="hlt">wind</span> product version 2.0 produced by Remote Sensing System (RSS) over the overlapped period 1991-2014. The potential links between surface <span class="hlt">winds</span> and Indian <span class="hlt">regional</span> rainfall are also examined. Results indicate that the surface <span class="hlt">wind</span> speeds in AS and BoB during June-August are almost similar during strong ISMRs and weak ISMRs, whereas significant discrepancies are observed during September. By contrast, the surface <span class="hlt">wind</span> speeds in SIO during June-August are found to be significantly different between strong and weak ISMRs, where they are similar during September. The significant differences in monthly mean surface <span class="hlt">wind</span> convergence between strong and weak ISMRs are not coherent in space in the three <span class="hlt">regions</span>. However, the probability density function (PDF) distributions of daily mean area-averaged values are distinctive between strong and weak ISMRs in the three <span class="hlt">regions</span>. The correlation analysis indicates the area-averaged surface <span class="hlt">wind</span> speeds in AS and the area-averaged <span class="hlt">wind</span> convergence in BoB are highly correlated with <span class="hlt">regional</span> rainfall for both strong and weak ISMRs. The <span class="hlt">wind</span> convergence in BoB during strong ISMRs is relatively better correlated with <span class="hlt">regional</span> rainfall than during weak ISMRs. The surface <span class="hlt">winds</span> in SIO do not greatly affect Indian rainfall in short timescales, however, they will ultimately affect the strength of monsoon circulation by modulating Indian Ocean Dipole (IOD) mode via atmosphere-ocean interactions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPP43B1347F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPP43B1347F"><span>Changing Dust Provenance to the South Atlantic Since the Last Glacial Maximum and Implications for the Southern Hemisphere <span class="hlt">Wind</span> Belts</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Franzese, A. M.; Goldstein, S. L.; Hemming, S. R.</p> <p>2017-12-01</p> <p>The Southern Hemisphere Westerly <span class="hlt">Winds</span> are known to be important for climate due to their effects on the global carbon cycle and on the global thermohaline circulation (THC). Numerous proxy records have been interpreted to indicate significant glacial to interglacial changes in the SHWW. There is no clear consensus regarding their strength and position during the Last Glacial Maximum (LGM), though most observations are consistent with an equatorward displacement of the glacial <span class="hlt">wind</span> belts. We test this hypothesis using geochemical provenance measurements of deep-sea sediments deposited along the Mid-Atlantic Ridge between 24°S and 37°S. In the central South Atlantic, dust can be delivered from South America via the Westerlies, or from Africa via the <span class="hlt">Trade</span> <span class="hlt">Winds</span>. The dust sources on South America and Africa have very different geochemical signatures, making it possible to distinguish between eolian transport via the Westerlies vs. the <span class="hlt">Trade</span> <span class="hlt">Winds</span>. Any northward shift in the Southern Hemisphere Westerlies should increase the northward extent of a South American provenance in sediments dominated by eolian sources. We measured major and trace element concentrations, and radiogenic isotopes of Ar, Sr, Nd, and Pb on the <5 μm lithogenic sediments from a latitudinal transect of cores along the flanks of the Mid-Atlantic Ridge. In general, the data point to an older continental provenance for the northernmost sites, and a much younger provenance for the southernmost sites, consistent with western Africa as the primary source of sediment in the north, and South American sediments being delivered to the south. Glacial sediments display a clear compositional boundary near 30°S, which likely reflects the boundary between the Westerlies and the <span class="hlt">Trade</span> <span class="hlt">Winds</span>. The data are therefore not consistent with northward shifted <span class="hlt">wind</span> belts at the LGM. The observed variations in terrigenous sediment composition at these sites may, however, be consistent with an equatorward displacement</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23479867','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23479867"><span>[Sediment-yielding process and its mechanisms of slope erosion in <span class="hlt">wind</span>-water erosion crisscross <span class="hlt">region</span> of Loess Plateau, Northwest China].</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Tuo, Deng-Feng; Xu, Ming-Xiang; Zheng, Shi-Qing; Li, Qiang</p> <p>2012-12-01</p> <p>Due to the coupling effects of <span class="hlt">wind</span> and water erosions in the <span class="hlt">wind</span>-water erosion crisscross <span class="hlt">region</span> of Loess Plateau, the slope erosion in the <span class="hlt">region</span> was quite serious, and the erosion process was quite complicated. By using <span class="hlt">wind</span> tunnel combined with simulated rainfall, this paper studied the sediment-yielding process and its mechanisms of slope erosion under the effects of <span class="hlt">wind</span>-water alternate erosion, and quantitatively analyzed the efffects of <span class="hlt">wind</span> erosion on water erosion and the relationships between <span class="hlt">wind</span> and water erosions. There was an obvious positive interaction between <span class="hlt">wind</span> and water erosions. <span class="hlt">Wind</span> erosion promoted the development of microtopography, and altered the quantitative relationship between the sediment-yielding under water erosion and the variation of rainfall intensity. At the rainfall intensity of 60 and 80 mm x h(-1), the sediment-yielding without <span class="hlt">wind</span> erosion decreased with the duration of rainfall and tended to be stable, but the sediment-yielding with <span class="hlt">wind</span> erosion decreased to a certain valley value first, and then showed an increasing trend. At the rainfall intensity of 60, 80, and 100 mm x h(-1), the sediment-yielding with the <span class="hlt">wind</span> erosion at speeds of 11 and 14 m x s(-1) increased by 7.3%-27.9% and 23.2%-39.0%, respectively, as compared with the sediment-yielding without <span class="hlt">wind</span> erosion. At the rainfall intensity of 120 and 150 mm x h(-1) and in the rainfall duration of 15 minutes, the sediment-yielding with and without <span class="hlt">wind</span> erosion presented a decreasing trend, but, with the increase of rainfall duration, the sediment-yielding with <span class="hlt">wind</span> erosion showed a trend of decreasing first and increasing then, as compared with the sediment-yielding without <span class="hlt">wind</span> erosion. The mechanisms of <span class="hlt">wind</span>-water alternate erosion were complicated, reflecting in the mutual relation and mutual promotion of <span class="hlt">wind</span> erosion and water erosion in the aspects of temporal-spatial distribution, energy supply, and action mode of erosion forces.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1107455','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1107455"><span>Advancements in <span class="hlt">Wind</span> Integration Study Data Modeling: The <span class="hlt">Wind</span> Integration National Dataset (<span class="hlt">WIND</span>) Toolkit; Preprint</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>Draxl, C.; Hodge, B. M.; Orwig, K.</p> <p>2013-10-01</p> <p><span class="hlt">Regional</span> <span class="hlt">wind</span> integration studies in the United States require detailed <span class="hlt">wind</span> power output data at many locations to perform simulations of how the power system will operate under high-penetration scenarios. The <span class="hlt">wind</span> data sets that serve as inputs into the study must realistically reflect the ramping characteristics, spatial and temporal correlations, and capacity factors of the simulated <span class="hlt">wind</span> plants, as well as be time synchronized with available load profiles. The <span class="hlt">Wind</span> Integration National Dataset (<span class="hlt">WIND</span>) Toolkit described in this paper fulfills these requirements. A <span class="hlt">wind</span> resource dataset, <span class="hlt">wind</span> power production time series, and simulated forecasts from a numerical weather predictionmore » model run on a nationwide 2-km grid at 5-min resolution will be made publicly available for more than 110,000 onshore and offshore <span class="hlt">wind</span> power production sites.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20040015279&hterms=warm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dwarm','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20040015279&hterms=warm&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dwarm"><span>Influence of Transient Atmospheric Circulation on the Surface Heating of the Pacific Warm Pool</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Chou, Ming-Dah; Chou, Shu-Hsien; Chan, Pui-King</p> <p>2003-01-01</p> <p>Analyses of data on clouds, <span class="hlt">winds</span>, and surface heat fluxes show that the transient behavior of basin-wide large-scale circulation has a significant influence on the warm pool sea surface temperature (SST). <span class="hlt">Trade</span> <span class="hlt">winds</span> converge to <span class="hlt">regions</span> of the highest SST in the equatorial western Pacific. These <span class="hlt">regions</span> have the largest cloud cover and smallest <span class="hlt">wind</span> speed. Both surface solar heating and evaporative cooling are weak. The reduced evaporative cooling due to weakened <span class="hlt">winds</span> exceeds the reduced solar heating due to enhanced cloudiness. The result is a maximum surface heating in the strong convective and high SST <span class="hlt">regions</span>. Data also show that the maximum surface heating in strong convective <span class="hlt">regions</span> is interrupted by transient atmospheric and oceanic circulation. Due to the seasonal variation of the insolation at the top of the atmosphere, <span class="hlt">trade</span> <span class="hlt">winds</span> and clouds also experience seasonal variations. <span class="hlt">Regions</span> of high SST and low-level convergence follow the Sun, where the surface heating is a maximum. As the Sun moves away from a convective <span class="hlt">region</span>, the strong <span class="hlt">trade</span> <span class="hlt">winds</span> set in, and the evaporative cooling enhances, resulting in a net cooling of the surface. During an El Nino, the maximum SST and convective <span class="hlt">region</span> shifts eastward from the maritime continent to the equatorial central Pacific. Following the eastward shift of the maximum SST, the <span class="hlt">region</span> of maximum cloudiness and surface heating also shift eastward. As the atmospheric and oceanic circulation returns to normal situations, the <span class="hlt">trade</span> <span class="hlt">winds</span> increase and the surface heating decreases. We conclude that the evaporative cooling associated with the seasonal and interannual variations of <span class="hlt">trade</span> <span class="hlt">winds</span> is one of the major factors that modulate the SST distribution of the Pacific warm pool.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1987A%26A...177..243D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1987A%26A...177..243D"><span>Hollow H II <span class="hlt">regions</span>. II - Mechanism for <span class="hlt">wind</span> energy dissipation and diffuse X-ray emission</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dorland, H.; Montmerle, T.</p> <p>1987-05-01</p> <p>The mechanism by which stellar-<span class="hlt">wind</span> energy is dissipated near the shock in a hollow H II <span class="hlt">region</span> (HHR) around a massive star is investigated theoretically, in the context of the HHR model developed by Dorland et al. (1986). The principles of nonlinear thermal conduction (especially the delocalizaton of conductive heat flux postulated for laboratory fusion plasmas) are reviewed; expressions for estimating heat fluxes are derived; a two-temperature approximation is employed to describe coupling between thermal conduction and <span class="hlt">wind</span>-energy dissipation; and the determination of the flux-limit factor from X-ray observations is explained. The model is then applied to observational data for the Rosette nebula and Eta Car, and the results are presented graphically. The diffuse X-ray temperatures of HHRs are found to be in the range 2-16 keV and to depend uniquely on stellar-<span class="hlt">wind</span> velocity, the value for an O star with <span class="hlt">wind</span> velocity 2500 km/s being about 5 keV.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26702431','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26702431"><span>Systemic <span class="hlt">trade</span> risk of critical resources.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Klimek, Peter; Obersteiner, Michael; Thurner, Stefan</p> <p>2015-11-01</p> <p>In the wake of the 2008 financial crisis, the role of strongly interconnected markets in causing systemic instability has been increasingly acknowledged. <span class="hlt">Trade</span> networks of commodities are susceptible to cascades of supply shocks that increase systemic <span class="hlt">trade</span> risks and pose a threat to geopolitical stability. We show that supply risk, scarcity, and price volatility of nonfuel mineral resources are intricately connected with the structure of the worldwide <span class="hlt">trade</span> networks spanned by these resources. At the global level, we demonstrate that the scarcity of a resource is closely related to the susceptibility of the <span class="hlt">trade</span> network with respect to cascading shocks. At the <span class="hlt">regional</span> level, we find that, to some extent, <span class="hlt">region</span>-specific price volatility and supply risk can be understood by centrality measures that capture systemic <span class="hlt">trade</span> risk. The resources associated with the highest systemic <span class="hlt">trade</span> risk indicators are often those that are produced as by-products of major metals. We identify significant strategic shortcomings in the management of systemic <span class="hlt">trade</span> risk, in particular in the European Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4681334','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4681334"><span>Systemic <span class="hlt">trade</span> risk of critical resources</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Klimek, Peter; Obersteiner, Michael; Thurner, Stefan</p> <p>2015-01-01</p> <p>In the wake of the 2008 financial crisis, the role of strongly interconnected markets in causing systemic instability has been increasingly acknowledged. <span class="hlt">Trade</span> networks of commodities are susceptible to cascades of supply shocks that increase systemic <span class="hlt">trade</span> risks and pose a threat to geopolitical stability. We show that supply risk, scarcity, and price volatility of nonfuel mineral resources are intricately connected with the structure of the worldwide <span class="hlt">trade</span> networks spanned by these resources. At the global level, we demonstrate that the scarcity of a resource is closely related to the susceptibility of the <span class="hlt">trade</span> network with respect to cascading shocks. At the <span class="hlt">regional</span> level, we find that, to some extent, <span class="hlt">region</span>-specific price volatility and supply risk can be understood by centrality measures that capture systemic <span class="hlt">trade</span> risk. The resources associated with the highest systemic <span class="hlt">trade</span> risk indicators are often those that are produced as by-products of major metals. We identify significant strategic shortcomings in the management of systemic <span class="hlt">trade</span> risk, in particular in the European Union. PMID:26702431</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH34A..03W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH34A..03W"><span>Solar <span class="hlt">Wind</span> 0.1-1 keV Electrons in the Corotating Interaction <span class="hlt">Regions</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, L.; Tao, J.; Li, G.; Wimmer-Schweingruber, R. F.; Jian, L. K.; He, J.; Tu, C.; Tian, H.; Bale, S. D.</p> <p>2017-12-01</p> <p>Here we present a statistical study of the 0.1-1 keV suprathermal electrons in the undisturbed and compressed slow/fast solar <span class="hlt">wind</span>, for the 71 corotating interaction <span class="hlt">regions</span> (CIRs) with good measurements from the <span class="hlt">WIND</span> 3DP and MFI instruments from 1995 to 1997. For each of these CIRs, we separate the strahl and halo electrons based on their different behaviors in pitch angle distributions in the undisturbed and compressed solar <span class="hlt">wind</span>. We fit both the strahl and halo energy spectra to a kappa function with an index κ index and effective temperature Teff, and calculate the pitch-angle width at half-maximum (PAHM) of the strahl population. We also integrate the electron measurements between 0.1 and 1.0 keV to obtain the number density n and average energy Eavg for the strahl and halo populations. We find that for both the strahl and halo populations within and around these CIRs, the fitted κ index strongly correlates with Teff, similar to the quiet-time solar <span class="hlt">wind</span> (Tao et al., ApJ, 2016). The number density of both the strahl and halo shows a strong positive correlation with the electron core temperature. The strahl number density ns is correlated with the magnitude of interplanetary magnetic field, and the strahl PAHM width is anti-correlated with the solar <span class="hlt">wind</span> speed. These results suggest that the origin of strahl electrons from the solar corona is likely related to the electron core temperature and magnetic field strength, while the production of halo electrons in the interplanetary medium could depend on the solar <span class="hlt">wind</span> velocity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1914802A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1914802A"><span>Local and <span class="hlt">regional</span> characterisation of the diurnal mountain <span class="hlt">wind</span> systems in the Guadarrama mountain range (Spain)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arrillaga, Jon A.; Cano, Darío; Sastre, Mariano; Román-Cascón, Carlos; Maqueda, Gregorio; Morales, Gema; Viana, Samuel; Inclán, Rosa M.; Fidel González-Roúco, J.; Santolaria, Edmundo; Durán, Luis; Yagüe, Carlos</p> <p>2017-04-01</p> <p>Diurnal mountain <span class="hlt">wind</span> systems that develop in the surroundings of the Guadarrama mountain range (Spain) are studied in this work. This area is highly interesting: the city of Madrid is located at approximately 50 km towards the SE; and on the other hand, unlike in other mountainous <span class="hlt">regions</span>, the summers are characterised to be significantly dry, providing an interesting case study of energy balance in the context of complex orography. Slope and basin circulations formed play an important role in the development of fog and pollution episodes in the whole <span class="hlt">region</span>. On top of that, when upslope basin <span class="hlt">winds</span> strengthened by diurnal convection exceed 10 m s-1, the runway configuration at the airport of Madrid needs to be modified. Continuous meteorological data and turbulent fluxes of carbon dioxide, water vapour, momentum and heat are provided since June 2016 from measurements at a 10 m tower at La Herrería site, which is located at the foot of the Guadarrama mountain range. Besides, a 4 m high portable station is available for complementary measurements. La Herrería is part of the Guadarrama Monitoring Network (GuMNet; www.ucm.es/gumnet/), an atmospheric and subsurface observational facility distributed over the Guadarrama mountain range. As a support for the analysis, data from conventional meteorological stations within the <span class="hlt">region</span> and a <span class="hlt">wind</span> profiler at the airport are also employed. The <span class="hlt">wind</span> roses for the period analysed (summer 2016) show how the diurnal cycle of the flows is influenced by local slopes and by the configuration of the basin. The irruption of the downslope flow in the evening produces a significant increase of the turbulence intensity and the eventual breakdown of the surface-based thermal inversion. However, the severe drying out of the soil throughout the summer, evident from the evolution of the surface latent and sensible heat fluxes, seems to play a role in altering the characteristics of the mountain-breeze system and its impact on turbulence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22654443-superluminous-transients-agn-centers-from-interaction-between-black-hole-disk-winds-broad-line-region-clouds','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22654443-superluminous-transients-agn-centers-from-interaction-between-black-hole-disk-winds-broad-line-region-clouds"><span>Superluminous Transients at AGN Centers from Interaction between Black Hole Disk <span class="hlt">Winds</span> and Broad-line <span class="hlt">Region</span> Clouds</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>Moriya, Takashi J.; Tanaka, Masaomi; Ohsuga, Ken</p> <p></p> <p>We propose that superluminous transients that appear at central <span class="hlt">regions</span> of active galactic nuclei (AGNs) such as CSS100217:102913+404220 (CSS100217) and PS16dtm, which reach near- or super-Eddington luminosities of the central black holes, are powered by the interaction between accretion-disk <span class="hlt">winds</span> and clouds in broad-line <span class="hlt">regions</span> (BLRs) surrounding them. If the disk luminosity temporarily increases by, e.g., limit–cycle oscillations, leading to a powerful radiatively driven <span class="hlt">wind</span>, strong shock waves propagate in the BLR. Because the dense clouds in the AGN BLRs typically have similar densities to those found in SNe IIn, strong radiative shocks emerge and efficiently convert the ejecta kineticmore » energy to radiation. As a result, transients similar to SNe IIn can be observed at AGN central <span class="hlt">regions</span>. Since a typical black hole disk-<span class="hlt">wind</span> velocity is ≃0.1 c , where c is the speed of light, the ejecta kinetic energy is expected to be ≃10{sup 52} erg when ≃1 M {sub ⊙} is ejected. This kinetic energy is transformed to radiation energy in a timescale for the <span class="hlt">wind</span> to sweep up a similar mass to itself in the BLR, which is a few hundred days. Therefore, both luminosities (∼10{sup 44} erg s{sup −1}) and timescales (∼100 days) of the superluminous transients from AGN central <span class="hlt">regions</span> match those expected in our interaction model. If CSS100217 and PS16dtm are related to the AGN activities triggered by limit–cycle oscillations, they become bright again in coming years or decades.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BoLMe.158..311C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BoLMe.158..311C"><span>Characterization of the Marine Boundary Layer and the <span class="hlt">Trade-Wind</span> Inversion over the Sub-tropical North Atlantic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carrillo, J.; Guerra, J. C.; Cuevas, E.; Barrancos, J.</p> <p>2016-02-01</p> <p>The stability of the lower troposphere along the east side of the sub-tropical North Atlantic is analyzed and characterized using upper air meteorological long-term records at the Canary Islands (Tenerife), Madeira (Madeira) and Azores (Terceira) archipelagos. The most remarkable characteristic is the strong stratification observed in the lower troposphere, with a strengthening of stability centred at levels near 900 and 800 hPa in a significant percentage of soundings (ranging from 17 % in Azores to 33 % in Güimar, Canary Islands). We show that this double structure is associated with the top of the marine boundary layer (MBL) and the <span class="hlt">trade-wind</span> inversion (TWI) respectively. The top of the MBL coincides with the base of the first temperature inversion (≈ 900 hPa) where a sharp change in water vapour mixing ratio is observed. A second temperature inversion is found near 800 hPa, which is characterized by a large directional <span class="hlt">wind</span> shear just above the inversion layer, tied to the TWI. We find that seasonal and latitudinal variations of the height and strength of both temperature inversions are driven by large-scale subsiding air from the upper troposphere associated with the descent branch of the Hadley cell. Increased general subsidence in summertime enhances stability in the lower troposphere, more markedly in the southern stations, where the inversion-layer heights are found at lower levels enhancing the main features of these two temperature inversions. A simple conceptual model that explains the lower tropospheric inversion enhancement by subsidence is proposed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=wind+AND+turbine+AND+problems&id=EJ714410','ERIC'); return false;" href="https://eric.ed.gov/?q=wind+AND+turbine+AND+problems&id=EJ714410"><span>Global <span class="hlt">Wind</span> Map</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>Journal of College Science Teaching, 2005</p> <p>2005-01-01</p> <p>This brief article describes a new global <span class="hlt">wind</span>-power map that has quantified global <span class="hlt">wind</span> power and may help planners place turbines in locations that can maximize power from the <span class="hlt">winds</span> and provide widely available low-cost energy. The researchers report that their study can assist in locating <span class="hlt">wind</span> farms in <span class="hlt">regions</span> known for strong and consistent…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22522525-complex-north-transition-region-centaurus-galactic-wind','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22522525-complex-north-transition-region-centaurus-galactic-wind"><span>THE COMPLEX NORTH TRANSITION <span class="hlt">REGION</span> OF CENTAURUS A: A GALACTIC <span class="hlt">WIND</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>Neff, Susan G.; Eilek, Jean A.; Owen, Frazer N., E-mail: susan.g.neff@nasa.gov</p> <p>2015-04-01</p> <p>We present deep GALEX images of NGC 5128, the parent galaxy of Centaurus A. We detect a striking “weather ribbon” of far-UV (FUV) and Hα emission which extends more than 35 kpc northeast of the galaxy. This ribbon is associated with a knotty ridge of radio/X-ray emission and is an extension of the previously known string of optical emission-line filaments. Many phenomena in the <span class="hlt">region</span> are too short-lived to have survived transit out from the inner galaxy; something must be driving them locally. We also detect FUV emission from the galaxy’s central dust lane. Combining this with previous radio andmore » far-IR measurements, we infer an active starburst in the central galaxy which is currently forming stars at ∼2 M{sub ☉} yr{sup −1}, and has been doing so for 50–100 Myr. If the <span class="hlt">wind</span> from this starburst is enhanced by energy and mass driven out from the active galactic nucleus, the powerful augmented <span class="hlt">wind</span> can be the driver needed for the northern weather system. We argue that both the diverse weather system, and the enhanced radio emission in the same <span class="hlt">region</span>, result from the wind’s encounter with cool gas left by one of the recent merger/encounter events in the history of NGC 5128.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1126840','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1126840"><span>Estimating the <span class="hlt">Wind</span> Resource in Uttarakhand: Comparison of Dynamic Downscaling with Doppler Lidar <span class="hlt">Wind</span> Measurements</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>Lundquist, J. K.; Pukayastha, A.; Martin, C.</p> <p></p> <p>Previous estimates of the <span class="hlt">wind</span> resources in Uttarakhand, India, suggest minimal <span class="hlt">wind</span> resources in this <span class="hlt">region</span>. To explore whether or not the complex terrain in fact provides localized <span class="hlt">regions</span> of <span class="hlt">wind</span> resource, the authors of this study employed a dynamic down scaling method with the Weather Research and Forecasting model, providing detailed estimates of <span class="hlt">winds</span> at approximately 1 km resolution in the finest nested simulation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20931984','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20931984"><span>Cost of <span class="hlt">wind</span> energy: comparing distant <span class="hlt">wind</span> resources to local resources in the midwestern United States.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hoppock, David C; Patiño-Echeverri, Dalia</p> <p>2010-11-15</p> <p>The best <span class="hlt">wind</span> sites in the United States are often located far from electricity demand centers and lack transmission access. Local sites that have lower quality <span class="hlt">wind</span> resources but do not require as much power transmission capacity are an alternative to distant <span class="hlt">wind</span> resources. In this paper, we explore the <span class="hlt">trade</span>-offs between developing new <span class="hlt">wind</span> generation at local sites and installing <span class="hlt">wind</span> farms at remote sites. We first examine the general relationship between the high capital costs required for local <span class="hlt">wind</span> development and the relatively lower capital costs required to install a <span class="hlt">wind</span> farm capable of generating the same electrical output at a remote site,with the results representing the maximum amount an investor should be willing to pay for transmission access. We suggest that this analysis can be used as a first step in comparing potential <span class="hlt">wind</span> resources to meet a state renewable portfolio standard (RPS). To illustrate, we compare the cost of local <span class="hlt">wind</span> (∼50 km from the load) to the cost of distant <span class="hlt">wind</span> requiring new transmission (∼550-750 km from the load) to meet the Illinois RPS. We find that local, lower capacity factor <span class="hlt">wind</span> sites are the lowest cost option for meeting the Illinois RPS if new long distance transmission is required to access distant, higher capacity factor <span class="hlt">wind</span> resources. If higher capacity <span class="hlt">wind</span> sites can be connected to the existing grid at minimal cost, in many cases they will have lower costs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19810030288&hterms=lazarus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D90%26Ntt%3Dlazarus','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19810030288&hterms=lazarus&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAuthor-Name%26N%3D0%26No%3D90%26Ntt%3Dlazarus"><span>Deceleration of the solar <span class="hlt">wind</span> in the earth's foreshock <span class="hlt">region</span> - Isee 2 and Imp 8 observations</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bonifazi, C.; Moreno, G.; Lazarus, A. J.; Sullivan, J. D.</p> <p>1980-01-01</p> <p>The deceleration of the solar <span class="hlt">wind</span> in the <span class="hlt">region</span> of the interplanetary space filled by ions backstreaming from the earth's bow shock and associated waves is studied using a two-spacecraft technique. This deceleration depends on the solar <span class="hlt">wind</span> bulk velocity; at low velocities (below 300 km/s) the velocity decrease is about 5 km/s, while at higher velocities (above 400 km/s) the decrease may be as large as 30 km/s. The energy balance shows that the kinetic energy loss far exceeds the thermal energy which is possibly gained by the solar <span class="hlt">wind</span>; therefore at least part of this energy must go into waves and/or into the backstreaming ions.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_9");'>9</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li class="active"><span>11</span></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_11 --> <div id="page_12" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="221"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22663557-small-coronal-holes-near-active-regions-sources-slow-solar-wind','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22663557-small-coronal-holes-near-active-regions-sources-slow-solar-wind"><span>Small Coronal Holes Near Active <span class="hlt">Regions</span> as Sources of Slow Solar <span class="hlt">Wind</span></span></a></p> <p><a target="_blank" href="http://www.osti.gov/search">DOE Office of Scientific and Technical Information (OSTI.GOV)</a></p> <p>Wang, Y.-M., E-mail: yi.wang@nrl.navy.mil</p> <p></p> <p>We discuss the nature of the small areas of rapidly diverging, open magnetic flux that form in the strong unipolar fields at the peripheries of active <span class="hlt">regions</span> (ARs), according to coronal extrapolations of photospheric field measurements. Because such <span class="hlt">regions</span> usually have dark counterparts in extreme-ultraviolet (EUV) images, we refer to them as coronal holes, even when they appear as narrow lanes or contain sunspots. Revisiting previously identified “AR sources” of slow solar <span class="hlt">wind</span> from 1998 and 1999, we find that they are all associated with EUV coronal holes; the absence of well-defined He i 1083.0 nm counterparts to some ofmore » these holes is attributed to the large flux of photoionizing radiation from neighboring AR loops. Examining a number of AR-associated EUV holes during the 2014 activity maximum, we confirm that they are characterized by <span class="hlt">wind</span> speeds of ∼300–450 km s{sup −1}, O{sup 7+}/O{sup 6+} ratios of ∼0.05–0.4, and footpoint field strengths typically of order 30 G. The close spacing between ARs at sunspot maximum limits the widths of unipolar <span class="hlt">regions</span> and their embedded holes, while the continual emergence of new flux leads to rapid changes in the hole boundaries. Because of the highly nonradial nature of AR fields, the smaller EUV holes are often masked by the overlying canopy of loops, and may be more visible toward one solar limb than at central meridian. As sunspot activity declines, the AR remnants merge to form much larger, weaker, and longer-lived unipolar <span class="hlt">regions</span>, which harbor the “classical” coronal holes that produce recurrent high-speed streams.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/50387','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/50387"><span>Climatology and trend of <span class="hlt">wind</span> power resources in China and its surrounding <span class="hlt">regions</span>: a revisit using Climate Forecast System Reanalysis data</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Lejiang Yu; Shiyuan Zhong; Xindi Bian; Warren E. Heilman</p> <p>2015-01-01</p> <p>The mean climatology, seasonal and interannual variability and trend of <span class="hlt">wind</span> speeds at the hub height (80 m) of modern <span class="hlt">wind</span> turbines over China and its surrounding <span class="hlt">regions</span> are revisited using 33-year (1979–2011) <span class="hlt">wind</span> data from the Climate Forecast System Reanalysis (CFSR) that has many improvements including higher spatial resolution over previous global reanalysis...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-07-12/pdf/2013-16784.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-07-12/pdf/2013-16784.pdf"><span>78 FR 41911 - Foreign-<span class="hlt">Trade</span> Zone 161-Sedgwick County, Kansas; Authorization of Production Activity; Siemens...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-07-12</p> <p>... DEPARTMENT OF COMMERCE Foreign-<span class="hlt">Trade</span> Zones Board [B-27-2013] Foreign-<span class="hlt">Trade</span> Zone 161--Sedgwick County, Kansas; Authorization of Production Activity; Siemens Energy, Inc. (<span class="hlt">Wind</span> Turbine Nacelles and Hubs); Hutchinson, Kansas On March 7, 2013, Siemens Energy, Inc., an operator of FTZ 161, submitted a notification of proposed production activity to...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20170000769','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20170000769"><span>Using Buoy and Radar Data to Study Sudden <span class="hlt">Wind</span> Gusts Over Coastal <span class="hlt">Regions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Priftis, Georgios; Chronis, Themis; Lang, Timothy J.</p> <p>2017-01-01</p> <p>Significant sudden <span class="hlt">wind</span> gusts can pose a threat to aviation near the coastline, as well as small (sailing) boats and commercial ships approaching the ports. Such cases can result in <span class="hlt">wind</span> speed changes of more than an order of magnitude within 5 minutes, which can then last up to 20 minutes or more. Although the constellation of scatterometers is a good means of studying maritime convection, those sudden gusts are not easily captured because of the low time resolution. The National Data Buoy Center (NDBC) provides continuous measurements of <span class="hlt">wind</span> speed and direction along the US coastal <span class="hlt">regions</span> every 6 minutes. Buoys are platforms placed at specific places on the seas, especially along coastlines, providing data for atmospheric and oceanic studies. Next Generation Radars (NEXRADs), after the recent upgrade of the network to dual-pol systems, offer enhanced capabilities to study atmospheric phenomena. NEXRADs provide continuous full-volume scans approximately every 5 minutes and therefore are close to the time resolution of the buoy measurements. Use of single- Doppler retrievals might also provide a means of further validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1910102W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1910102W"><span>Links between global meat <span class="hlt">trade</span> and organic river pollution</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wen, Yingrong; Schoups, Gerrit; van de Giesen, Nick</p> <p>2017-04-01</p> <p>Rising demand of meat boosts livestock farming intensification. Due to international meat <span class="hlt">trade</span>, the environmental costs of production are becoming increasingly separated from where the meat is consumed. However, little is known about the impact of <span class="hlt">trade</span> on the environment for both importers and exporters. Combining multi-scale (national, <span class="hlt">regional</span> and gridded) data, we present a new method to quantify the impacts of international meat <span class="hlt">trade</span> on global river organic pollution. We computed spatially distributed organic pollution in global river networks with and without meat <span class="hlt">trade</span>, where the without-<span class="hlt">trade</span> scenario assumes that meat imports are replaced by local production. Our analysis indicates high potential savings of livestock population and pollutants production at the global scale due to the international meat <span class="hlt">trade</span>. The spatially detailed analysis shows that current <span class="hlt">trade</span> contributes to organic pollution reductions in meat importing <span class="hlt">regions</span>, especially in rich nations. The deterioration of river water quality, especially in developing <span class="hlt">regions</span>, points to an urgent need for affordable infrastructure and technology development and wastewater solutions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19950032354&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsolar%2Bintensity%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19950032354&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D70%26Ntt%3Dsolar%2Bintensity%2Bmeasurement"><span>Latitudinal variation of speed and mass flux in the acceleration <span class="hlt">region</span> of the solar <span class="hlt">wind</span> inferred from spectral broadening measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Woo, Richard; Goldstein, Richard M.</p> <p>1994-01-01</p> <p>Spectral broadening measurements conducted at S-band (13-cm wavelength) during solar minimum conditions in the heliocentric distance range of 3-8 R(sub O) by Mariner 4, Pioneer 10, Mariner 10, Helios 1, Helios 2, and Viking have been combined to reveal a factor of 2.6 reduction in bandwidth from equator to pole. Since spectral broadening bandwidth depends on electron density fluctuation and solar <span class="hlt">wind</span> speed, and latitudinal variation of the former is available from coherence bandwidth measurements, the remote sensing spectral broadening measurements provide the first determination of the latitudinal variation of solar <span class="hlt">wind</span> speed in the acceleration <span class="hlt">region</span>. When combined with electron density measurements deduced from white-light coronagraphs, this result also leads to the first determination of the latitudinal variation of mass flux in the acceleration <span class="hlt">region</span>. From equator to pole, solar <span class="hlt">wind</span> speed increases by a factor of 2.2, while mass flux decreases by a factor of 2.3. These results are consistent with measurements of solar <span class="hlt">wind</span> speed by multi-station intensity scintillation measurements, as well as measurements of mass flux inferred from Lyman alpha observations, both of which pertain to the solar <span class="hlt">wind</span> beyond 0.5 AU. The spectral broadening observations, therefore, strengthen earlier conclusions about the latitudinal variation of solar <span class="hlt">wind</span> speed and mass flux, and reinforce current solar coronal models and their implications for solar <span class="hlt">wind</span> acceleration and solar <span class="hlt">wind</span> modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA13606.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA13606.html"><span><span class="hlt">Wind</span> Texture</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2010-11-10</p> <p>One of the most active agent of erosion on Mars today is the <span class="hlt">wind</span>. This <span class="hlt">region</span>, near Nicholson crater, has been sculpted by untold years of blowing grit and <span class="hlt">wind</span>, as shown in this image captured by NASA Mars Odyssey.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/8727','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/8727"><span>Modeling Japan-South Seas <span class="hlt">trade</span> in forest products.</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>J.R. Vincent</p> <p>1987-01-01</p> <p>The international <span class="hlt">trade</span> of forest products has generated increasing research interest, yet experience with modeling such <span class="hlt">trade</span> is limited. Primary issues include the effects of <span class="hlt">trade</span> barriers and exchange rates on <span class="hlt">trade</span> patterns and national welfare. This paper attempts to add to experience by modeling hardwood log, lumber, and plywood <span class="hlt">trade</span> in a <span class="hlt">region</span> that has been...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUOSPC14C2080G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUOSPC14C2080G"><span>Effects of Southern Hemispheric <span class="hlt">Wind</span> Changes on Global Oxygen and the Pacific Oxygen Minimum Zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Getzlaff, J.; Dietze, H.; Oschlies, A.</p> <p>2016-02-01</p> <p>We use a coupled ocean biogeochemistry-circulation model to compare the impact of changes in southern hemispheric <span class="hlt">winds</span> with that of warming induced buoyancy fluxes on dissolved oxygen. Changes in the southern hemispheric <span class="hlt">wind</span> fields, which are in line with an observed shift of the southern annual mode, are a combination of a strengthening and poleward shift of the southern westerlies. We differentiate between effects caused by a strengthening of the westerlies and effects of a southward shift of the westerlies that is accompanied by a poleward expansion of the tropical <span class="hlt">trade</span> <span class="hlt">winds</span>. Our results confirm that the Southern Ocean plays an important role for the marine oxygen supply: a strengthening of the southern westerlies, that leads to an increase of the water formation rates of the oxygen rich deep and intermediate water masses, can counteract part of the warming-induced decline in marine oxygen levels. The <span class="hlt">wind</span> driven intensification of the Southern Ocean meridional overturning circulation drives an increase of the global oxygen supply. Furthermore the results show that the shift of the boundary between westerlies and <span class="hlt">trades</span> results in an increase of subantarctic mode water and an anti-correlated decrease of deep water formation and reduces the oceanic oxygen supply. In addition we find that the increased meridional extension of the southern <span class="hlt">trade</span> <span class="hlt">winds</span>, results in a strengthening and southward shift of the subtropical <span class="hlt">wind</span> stress curl. This alters the subtropical gyre circulation (intensification and southward shift) and with it decreases the water mass transport into the oxygen minimum zone. In a business-as-usual CO2 emission scenario, the poleward shift of the <span class="hlt">trade</span>-to-westerlies boundary is as important for the future evolution of the suboxic volume as direct warming-induced changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..19..153A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..19..153A"><span><span class="hlt">Wind</span> power forecasting for a real onshore <span class="hlt">wind</span> farm on complex terrain using WRF high resolution simulations.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ángel Prósper Fernández, Miguel; Casal, Carlos Otero; Canoura Fernández, Felipe; Miguez-Macho, Gonzalo</p> <p>2017-04-01</p> <p><span class="hlt">Regional</span> meteorological models are becoming a generalized tool for forecasting <span class="hlt">wind</span> resource, due to their capacity to simulate local flow dynamics impacting <span class="hlt">wind</span> farm production. This study focuses on the production forecast and validation of a real onshore <span class="hlt">wind</span> farm using high horizontal and vertical resolution WRF (Weather Research and Forecasting) model simulations. The <span class="hlt">wind</span> farm is located in Galicia, in the northwest of Spain, in a complex terrain <span class="hlt">region</span> with high <span class="hlt">wind</span> resource. Utilizing the Fitch scheme, specific for <span class="hlt">wind</span> farms, a period of one year is simulated with a daily operational forecasting set-up. Power and <span class="hlt">wind</span> predictions are obtained and compared with real data provided by the management company. Results show that WRF is able to yield good <span class="hlt">wind</span> power operational predictions for this kind of <span class="hlt">wind</span> farms, due to a good representation of the planetary boundary layer behaviour of the <span class="hlt">region</span> and the good performance of the Fitch scheme under these conditions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=522003','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=522003"><span>Assigning African elephant DNA to geographic <span class="hlt">region</span> of origin: Applications to the ivory <span class="hlt">trade</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>Wasser, Samuel K.; Shedlock, Andrew M.; Comstock, Kenine; Ostrander, Elaine A.; Mutayoba, Benezeth; Stephens, Matthew</p> <p>2004-01-01</p> <p>Resurgence of illicit <span class="hlt">trade</span> in African elephant ivory is placing the elephant at renewed risk. Regulation of this <span class="hlt">trade</span> could be vastly improved by the ability to verify the geographic origin of tusks. We address this need by developing a combined genetic and statistical method to determine the origin of poached ivory. Our statistical approach exploits a smoothing method to estimate geographic-specific allele frequencies over the entire African elephants' range for 16 microsatellite loci, using 315 tissue and 84 scat samples from forest (Loxodonta africana cyclotis) and savannah (Loxodonta africana africana) elephants at 28 locations. These geographic-specific allele frequency estimates are used to infer the geographic origin of DNA samples, such as could be obtained from tusks of unknown origin. We demonstrate that our method alleviates several problems associated with standard assignment methods in this context, and the absolute accuracy of our method is high. Continent-wide, 50% of samples were located within 500 km, and 80% within 932 km of their actual place of origin. Accuracy varied by <span class="hlt">region</span> (median accuracies: West Africa, 135 km; Central Savannah, 286 km; Central Forest, 411 km; South, 535 km; and East, 697 km). In some cases, allele frequencies vary considerably over small geographic <span class="hlt">regions</span>, making much finer discriminations possible and suggesting that resolution could be further improved by collection of samples from locations not represented in our study. PMID:15459317</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.usgs.gov/pp/p1598/','USGSPUBS'); return false;" href="https://pubs.usgs.gov/pp/p1598/"><span>Desert <span class="hlt">winds</span>: Monitoring <span class="hlt">wind</span>-related surface processes in Arizona, New Mexico, and California</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Breed, Carol S.; Reheis, Marith C.</p> <p>1999-01-01</p> <p>The 18-year Desert <span class="hlt">Winds</span> Project established instrumented field sites in the five major <span class="hlt">regions</span> of the North American Desert to obtain meteorological, geological, and vegetation data for natural desert sites affected by <span class="hlt">wind</span> erosion. The eight chapters in this volume describe the settings and operation of the stations and summarize eolian-related research to date around the stations. The report includes studies of the sand-moving effectiveness of storm <span class="hlt">winds</span>, <span class="hlt">wind</span>-erosion susceptibility of different ground-surface types, relations of dust storms to meteorological conditions, mediation of <span class="hlt">wind</span> erosion by vegetation, remote sensing to detect vegetation changes related to climate change, and comparison of <span class="hlt">regional</span> dust deposition to that near Owens (dry) Lake.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFM.A51S..02F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFM.A51S..02F"><span>Scheduling whole-air samples above the <span class="hlt">Trade</span> <span class="hlt">Wind</span> Inversion from SUAS using real-time sensors</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Freer, J. E.; Greatwood, C.; Thomas, R.; Richardson, T.; Brownlow, R.; Lowry, D.; MacKenzie, A. R.; Nisbet, E. G.</p> <p>2015-12-01</p> <p>Small Unmanned Air Systems (SUAS) are increasingly being used in science applications for a range of applications. Here we explore their use to schedule the sampling of air masses up to 2.5km above ground using computer controlled bespoked Octocopter platforms. Whole-air sampling is targeted above, within and below the <span class="hlt">Trade</span> <span class="hlt">Wind</span> Inversion (TWI). On-board sensors profiled the TWI characteristics in real time on ascent and, hence, guided the altitudes at which samples were taken on descent. The science driver for this research is investigation of the Southern Methane Anomaly and, more broadly, the hemispheric-scale transport of long-lived atmospheric tracers in the remote troposphere. Here we focus on the practical application of SUAS for this purpose. Highlighting the need for mission planning, computer control, onboard sensors and logistics in deploying such technologies for out of line-of-sight applications. We show how such a platform can be deployed successfully, resulting in some 60 sampling flights within a 10 day period. Challenges remain regarding the deployment of such platforms routinely and cost-effectively, particularly regarding training and support. We present some initial results from the methane sampling and its implication for exploring and understanding the Southern Methane Anomaly.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ApJ...829...71S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ApJ...829...71S"><span>The Baryon Cycle at High Redshifts: Effects of Galactic <span class="hlt">Winds</span> on Galaxy Evolution in Overdense and Average <span class="hlt">Regions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sadoun, Raphael; Shlosman, Isaac; Choi, Jun-Hwan; Romano-Díaz, Emilio</p> <p>2016-10-01</p> <p>We employ high-resolution cosmological zoom-in simulations focusing on a high-sigma peak and an average cosmological field at z ˜ 6-12 in order to investigate the influence of environment and baryonic feedback on galaxy evolution in the reionization epoch. Strong feedback, e.g., galactic <span class="hlt">winds</span>, caused by elevated star formation rates (SFRs) is expected to play an important role in this evolution. We compare different outflow prescriptions: (I) constant <span class="hlt">wind</span> velocity (CW), (II) variable <span class="hlt">wind</span> scaling with galaxy properties (VW), and (III) no outflows (NW). The overdensity leads to accelerated evolution of dark matter and baryonic structures, absent from the “normal” <span class="hlt">region</span>, and to shallow galaxy stellar mass functions at the low-mass end. Although CW shows little dependence on the environment, the more physically motivated VW model does exhibit this effect. In addition, VW can reproduce the observed specific SFR (sSFR) and the sSFR-stellar mass relation, which CW and NW fail to satisfy simultaneously. <span class="hlt">Winds</span> also differ substantially in affecting the state of the intergalactic medium (IGM). The difference lies in the volume-filling factor of hot, high-metallicity gas, which is near unity for CW, while such gas remains confined in massive filaments for VW, and locked up in galaxies for NW. Such gas is nearly absent from the normal <span class="hlt">region</span>. Although all <span class="hlt">wind</span> models suffer from deficiencies, the VW model seems to be promising in correlating the outflow properties with those of host galaxies. Further constraints on the state of the IGM at high z are needed to separate different <span class="hlt">wind</span> models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRA..122.4500A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRA..122.4500A"><span>Strong temperature gradients and vertical <span class="hlt">wind</span> shear on MLT <span class="hlt">region</span> associated to instability source at 23°S</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Andrioli, V. F.; Batista, P. P.; Xu, Jiyao; Yang, Guotao; Chi, Wang; Zhengkuan, Liu</p> <p>2017-04-01</p> <p>Na lidar temperature measurements were taken successfully from 2007 to 2009 in the mesopause <span class="hlt">region</span> over São José dos Campos (23.1°S, 45.9°W). Strong gradients on these vertical temperature profiles are often observed. A simple theoretical study has shown that temperature gradient of at least -8 K/km is required concurrently with the typical tidal <span class="hlt">wind</span> shear in order to generate dynamical instability in the MLT <span class="hlt">region</span>. We have studied vertical shear in horizontal <span class="hlt">wind</span> related to atmospheric tides, inferred by meteor radar, with the aim of analyzing instability occurrence. These <span class="hlt">wind</span> measurements were taken from an all-sky meteor radar at Cachoeira Paulista (22.7°S, 45°W). Two years of simultaneous data, <span class="hlt">wind</span> and temperature, were used in this analysis which represent 79 days, totalizing 589 h of simultaneous observations. We realize that the condition for the local Richardson number (Ri) dropping below the critical value of instability (Ri < 0.25) is often reached in 98% of the analyzed cases. The mean probabilities for occurrence of convective and dynamical instabilities, in the altitude <span class="hlt">region</span> between 82 and 98 km, were observed to be about 3% and 17.5%, respectively. Additionally, vertical distribution of these probabilities has revealed a weak occurrence of dynamical instability around 90 km, and this fact can be related to the double mesopause typically observed in this site.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1314133','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1314133"><span>Developing high-resolution spatial data of migration corridors for avian species of concern in <span class="hlt">regions</span> of high potential <span class="hlt">wind</span> development</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>Katzner, Todd</p> <p>2014-06-15</p> <p>The future of the US economy, our national security, and our environmental quality all depend on decreasing our reliance on foreign oil and on fossil fuels. An essential component of decreasing this reliance is the development of alternative energy sources. <span class="hlt">Wind</span> power is among the most important alternative energy sources currently available, and the mid-Atlantic <span class="hlt">region</span> is a primary focus for <span class="hlt">wind</span> power development. In addition to being important to the development of <span class="hlt">wind</span> power, the mid-Atlantic <span class="hlt">region</span> holds a special responsibility for the conservation of the eastern North America's golden eagles (Aquila chrysaetos). This small population breeds in northeasternmore » Canada, winters in the southern Appalachians, and nearly all of these birds pass through the mid-Atlantic <span class="hlt">region</span> twice each year. Movement of these birds is not random and, particularly during spring and autumn, migrating golden eagles concentrate in a narrow 30-50 mile wide corridor in central Pennsylvania. Thus, because the fate of these rare birds may depend on responsible management of the habitat they use it is critical to use research to identify ways to mitigate prospective impacts on this and similar raptor species. The goal of this project was to develop high-resolution spatial risk maps showing migration corridors of and habitat use by eastern golden eagles in <span class="hlt">regions</span> of high potential for <span class="hlt">wind</span> development. To accomplish this, we first expanded existing models of raptor migration for the eastern USA to identify broad-scale migration patterns. We then used data from novel high-resolution tracking devices to discover routes of passage and detailed flight behavior of individual golden eagles throughout the eastern USA. Finally, we integrated these data and models to predict population-level migration patterns and individual eagle flight behavior on migration. We then used this information to build spatially explicit, probabilistic maps showing relative risk to birds from <span class="hlt">wind</span> development</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMGC13K0880W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC13K0880W"><span>Assessment of <span class="hlt">Wind</span> Datasets for Estimating Offshore <span class="hlt">Wind</span> Energy along the Central California Coast</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Y. H.; Walter, R. K.; Ruttenberg, B.; White, C.</p> <p>2017-12-01</p> <p>Offshore renewable energy along the central California coastline has gained significant interest in recent years. We present a comprehensive analysis of near-surface <span class="hlt">wind</span> datasets available in this <span class="hlt">region</span> to facilitate future estimates of <span class="hlt">wind</span> power generation potential. The analyses are based on local NDBC buoys, satellite-based measurements (QuickSCAT and CCMP V2.0), reanalysis products (NARR and MERRA), and a <span class="hlt">regional</span> climate model (WRF). There are substantial differences in the diurnal signal during different months among the various products (i.e., satellite-based, reanalysis, and modeled) relative to the local buoys. Moreover, the datasets tended to underestimate <span class="hlt">wind</span> speed under light <span class="hlt">wind</span> conditions and overestimate under strong <span class="hlt">wind</span> conditions. In addition to point-to-point comparisons against local buoys, the spatial variations of bias and error in both the reanalysis products and WRF model data in this <span class="hlt">region</span> were compared against satellite-based measurements. NARR's bias and root-mean-square-error were generally small in the study domain and decreased with distance from coastlines. Although its smaller spatial resolution is likely to be insufficient to reveal local effects, the small bias and error in near-surface <span class="hlt">winds</span>, as well as the availability of <span class="hlt">wind</span> data at the proposed turbine hub heights, suggests that NARR is an ideal candidate for use in offshore <span class="hlt">wind</span> energy production estimates along the central California coast. The framework utilized here could be applied in other site-specific <span class="hlt">regions</span> where offshore renewable energy is being considered.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2013-09-09/pdf/2013-21897.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2013-09-09/pdf/2013-21897.pdf"><span>78 FR 55057 - Authorization of Production Activity, Foreign-<span class="hlt">Trade</span> Subzone 123E, Vestas Nacelles America, Inc...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2013-09-09</p> <p>... DEPARTMENT OF COMMERCE Foreign-<span class="hlt">Trade</span> Zones Board [B-47-2013] Authorization of Production Activity, Foreign-<span class="hlt">Trade</span> Subzone 123E, Vestas Nacelles America, Inc., (<span class="hlt">Wind</span> Turbines), Brighton, Denver, Pueblo, and Windsor, Colorado On May 3, 2013, Vestas Nacelles America, Inc., operator of Subzone 123E in Brighton, Denver, Pueblo, and Windsor, Colorado,...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JGRE..122.1119C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JGRE..122.1119C"><span>Earth aeolian <span class="hlt">wind</span> streaks: Comparison to <span class="hlt">wind</span> data from model and stations</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cohen-Zada, A. L.; Maman, S.; Blumberg, D. G.</p> <p>2017-05-01</p> <p><span class="hlt">Wind</span> streak is a collective term for a variety of aeolian features that display distinctive albedo surface patterns. <span class="hlt">Wind</span> streaks have been used to map near-surface <span class="hlt">winds</span> and to estimate atmospheric circulation patterns on Mars and Venus. However, because <span class="hlt">wind</span> streaks have been studied mostly on Mars and Venus, much of the knowledge regarding the mechanism and time frame of their formation and their relationship to the atmospheric circulation cannot be verified. This study aims to validate previous studies' results by a comparison of real and modeled <span class="hlt">wind</span> data with <span class="hlt">wind</span> streak orientations as measured from remote-sensing images. Orientations of Earth <span class="hlt">wind</span> streaks were statistically correlated to resultant drift direction (RDD) values calculated from reanalysis and <span class="hlt">wind</span> data from 621 weather stations. The results showed good agreement between <span class="hlt">wind</span> streak orientations and reanalysis RDD (r = 0.78). A moderate correlation was found between the <span class="hlt">wind</span> streak orientations and the weather station data (r = 0.47); a similar trend was revealed on a <span class="hlt">regional</span> scale when the analysis was performed by continent, with r ranging from 0.641 in North America to 0.922 in Antarctica. At sites where <span class="hlt">wind</span> streak orientations did not correspond to the RDDs (i.e., a difference of 45°), seasonal and diurnal variations in the <span class="hlt">wind</span> flow were found to be responsible for deviation from the global pattern. The study thus confirms that Earth <span class="hlt">wind</span> streaks were formed by the present <span class="hlt">wind</span> regime and they are indeed indicative of the long-term prevailing <span class="hlt">wind</span> direction on global and <span class="hlt">regional</span> scales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/25599','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/25599"><span>Severe <span class="hlt">wind</span> and fire regimes in northern forests: historical variability at the <span class="hlt">regional</span> scale</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Lisa A. Schulte; David J. Mladenoff</p> <p>2005-01-01</p> <p>Within the northern Great Lakes <span class="hlt">region</span>, mesoscale (10s to 100s of km2) forest patterning is driven by disturbance dynamics. Using original Public Land Survey (PLS) records in northern Wisconsin, USA, we study spatial patterns of <span class="hlt">wind</span> and fire disturbances during the pre-Euroamerican settlement period (ca. 1850). Our goals were: (1) to...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_10");'>10</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li class="active"><span>12</span></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_12 --> <div id="page_13" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="241"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840027190','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840027190"><span>Participation in the Mars data analysis program: Global and <span class="hlt">regional</span> studies of <span class="hlt">wind</span>-indicators on the surface of Mars</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Veverka, J.; Thomas, P.</p> <p>1984-01-01</p> <p>Global and <span class="hlt">regional</span> patterns on Mars were inferred from surface aeolian features, such as <span class="hlt">wind</span> streaks and dune deposits, which were visible in Viking Orbiter images. Precise measurements of the dimensions of topographic obstacles, i.e., craters, hills, ridges, on Mars as well as their associated <span class="hlt">wind</span> streaks were used to determine the aerodynamic shape of an obstacle affects near surface airflow. A classification of Martian <span class="hlt">wind</span> streaks was developed on the basis of albedo contrast and the presence or absence of either topographic obstacles or sediment deposits at the point of origin of the <span class="hlt">wind</span> streaks. It was concluded that local meteorological conditions, such as the stability of the atmospheric boundary layer, play a major role in determining why some Martian craters produce depositional <span class="hlt">wind</span> streaks while others produce erosional ones.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1980STIN...8128576L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1980STIN...8128576L"><span>Economics of <span class="hlt">wind</span> energy for irrigation pumping</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lansford, R. R.; Supalla, R. J.; Gilley, J. R.; Martin, D. L.</p> <p>1980-07-01</p> <p>The economic questions associated with <span class="hlt">wind</span> power as an energy source for irrigation under different situations with seven <span class="hlt">regions</span> of the nation were studied. Target investment costs for <span class="hlt">wind</span> turbines used for irrigation pumping and policy makers with bases for adjusting taxes to make alternative sources of energy investments more attractive are analyzed. Three types of <span class="hlt">wind</span> systems are considered for each of the seven <span class="hlt">regions</span>. The three types of <span class="hlt">wind</span> powered irrigation systems evaluated for each <span class="hlt">region</span> are: (1) <span class="hlt">wind</span> assist combustion engines (diesel, natural gas, propane panel); (2) <span class="hlt">wind</span> assist electric engines, with or without sale of surplus electricity; and (3) stand alone reservoir systems with gravity flow reservoirs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017JPhCS.901a2013H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017JPhCS.901a2013H"><span>Auroral bright spot in Jupiter’s active <span class="hlt">region</span> in corresponding to solar <span class="hlt">wind</span> dynamic</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Haewsantati, K.; Wannawichian, S.; Clarke, J. T.; Nichols, J. D.</p> <p>2017-09-01</p> <p>Jupiter’s polar emission has brightness whose behavior appears to be unstable. This work focuses on the bright spot in active <span class="hlt">region</span> which is a section of Jupiter’s polar emission. Images of the aurora were taken by Advanced Camera for Surveys (ACS) onboard the Hubble Space Telescope (HST). Previously, two bright spots, which were found on 13 th May 2007, were suggested to be fixed on locations described by system III longitude. The bright spot’s origin in equatorial plane was proposed to be at distance 80-90 Jovian radii and probably associated with the solar <span class="hlt">wind</span> properties. This study analyzes additional data on May 2007 to study long-term variation of brightness and locations of bright spots. The newly modified magnetosphere-ionosphere mapping based on VIP4 and VIPAL model is used to locate the origin of bright spot in magnetosphere. Furthermore, the Michigan Solar <span class="hlt">Wind</span> Model or mSWiM is also used to study the variation of solar <span class="hlt">wind</span> dynamic pressure during the time of bright spot’s observation. We found that the bright spots appear in similar locations which correspond to similar origins in magnetosphere. In addition, the solar <span class="hlt">wind</span> dynamic pressure should probably affect the bright spot’s variation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010AGUFM.A41F0178C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010AGUFM.A41F0178C"><span>A U.S. <span class="hlt">Wind</span> Climatology: new tools to monitor <span class="hlt">wind</span> trends across the contiguous 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>Crouch, J.; Wallis, T. W.; Arndt, D.</p> <p>2010-12-01</p> <p>NOAA’s National Climatic Data Center has developed a new monthly and seasonal product to provide a spatially continuous <span class="hlt">wind</span> climatology for the contiguous U.S. using NCEP reanalysis data. Surface <span class="hlt">wind</span> observations are sparse over specific <span class="hlt">regions</span> of the country, and are subject to many local effects. By utilizing the sigma .995 level of the reanalysis data we can monitor <span class="hlt">wind</span> conditions and trends of the lower troposphere across the entire U.S. The <span class="hlt">wind</span> data are interpolated from a 2.5 x 2.5 degree grid to 0.25 degrees to provide additional detail. Data are analyzed from January 1950 to the most current month. Monthly averaged <span class="hlt">winds</span> and <span class="hlt">wind</span> anomalies are calculated with respect to the 1971-2000 base period, and time series for each grid point show how <span class="hlt">regional</span> <span class="hlt">winds</span> have changed over the 60 year period of record. The goal of this new climatology product is to provide <span class="hlt">regional</span> decision support for the emerging <span class="hlt">wind</span> energy sector, in addition to others who are interested in the current state of <span class="hlt">wind</span> conditions. The U.S. Department of Energy has outlined a plan for 20 percent of U.S. electricity production to be from <span class="hlt">wind</span> by 2030, and having a temporally and spatially continuous <span class="hlt">wind</span> dataset, updated on a monthly basis, will be beneficial to understanding <span class="hlt">wind</span> trends nationwide.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900044371&hterms=Champagne&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DChampagne','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900044371&hterms=Champagne&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DChampagne"><span>Cometary compact H II <span class="hlt">regions</span> are stellar-<span class="hlt">wind</span> bow shocks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Van Buren, Dave; Mac Low, Mordecai-Mark; Wood, Douglas O. S.; Churchwell, ED</p> <p>1990-01-01</p> <p>Comet-shaped H II <span class="hlt">regions</span>, like G34.3 + 0.2, are easily explained as bow shocks created by <span class="hlt">wind</span>-blowing massive stars moving supersonically through molecular clouds. The required velocities of the stars through dense clumps are less than about 10 km/s, comparable to the velocity dispersion of stars in OB associations. An analytic model of bow shocks matches the gross characteristics seen in the radio continuum and the velocity structure inferred from hydrogen recombination and molecular line observations. The champagne flow model cannot account for these structures. VLBI observations of masers associated with the shells of cometary compact H II <span class="hlt">regions</span> should reveal tailward proper motions predominantly parallel to the shell, rather than perpendicular. It is predicted that over a decade baseline, high signal-to-noise VLA observations of this class of objects will show headward pattern motion in the direction of the symmetry axis, but not expansion. Finally, shock-generated and coronal infrared lines are also predicted.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140011312','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140011312"><span><span class="hlt">Wind</span> Turbine Contingency Control Through Generator De-Rating</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Frost, Susan; Goebel, Kai; Balas, Mark</p> <p>2013-01-01</p> <p>Maximizing turbine up-time and reducing maintenance costs are key technology drivers for <span class="hlt">wind</span> turbine operators. Components within <span class="hlt">wind</span> turbines are subject to considerable stresses due to unpredictable environmental conditions resulting from rapidly changing local dynamics. In that context, systems health management has the aim to assess the state-of-health of components within a <span class="hlt">wind</span> turbine, to estimate remaining life, and to aid in autonomous decision-making to minimize damage to the turbine. Advanced contingency control is one way to enable autonomous decision-making by providing the mechanism to enable safe and efficient turbine operation. The work reported herein explores the integration of condition monitoring of <span class="hlt">wind</span> turbines with contingency control to balance the <span class="hlt">trade</span>-offs between maintaining system health and energy capture. The contingency control involves de-rating the generator operating point to achieve reduced loads on the <span class="hlt">wind</span> turbine. Results are demonstrated using a high fidelity simulator of a utility-scale <span class="hlt">wind</span> turbine.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/wind/systems-engineering-workshop-2015.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/wind/systems-engineering-workshop-2015.html"><span>Systems Engineering 2015 Workshop | <span class="hlt">Wind</span> | NREL</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>Dhert, University of Michigan High-Fidelity Aerodynamic <em>Shape</em> Optimization for <span class="hlt">Wind</span> Turbines Kristian ; Different design approaches are applied to determine the <em>shape</em> as well as the structural composition of the turbine that also found a significant <span class="hlt">trade</span>-off between the lighter <em>blades</em> and a heavier tower moving from</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19740051276&hterms=WIND+STORMS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DWIND%2BSTORMS','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19740051276&hterms=WIND+STORMS&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3DWIND%2BSTORMS"><span>Observations of neutral <span class="hlt">winds</span> in the auroral E <span class="hlt">region</span> during the magnetospheric storm of August 3-9, 1972</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Brekke, A.; Doupnik, J. R.; Banks, P. M.</p> <p>1974-01-01</p> <p>Auroral zone E-<span class="hlt">region</span> neutral <span class="hlt">winds</span> have been derived from simultaneous measurements of ion drift velocities in different altitudes by the incoherent radar facility at Chatanika, Alaska, on a quiet day before and during the great magnetospheric storm of Aug. 3-9, 1972. The neutral <span class="hlt">wind</span> expected for a day-night pressure asymmetry appears to be strongly opposed by ion drag and local pressure gradients in the auroral oval.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13f4012D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13f4012D"><span>Should future <span class="hlt">wind</span> speed changes be taken into account in <span class="hlt">wind</span> farm development?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Devis, Annemarie; Van Lipzig, Nicole P. M.; Demuzere, Matthias</p> <p>2018-06-01</p> <p>Accurate <span class="hlt">wind</span> resource assessments are crucial in the development of <span class="hlt">wind</span> farm projects. However, it is common practice to estimate the <span class="hlt">wind</span> yield over the next 20 years from short-term measurements and reanalysis data of the past 20 years, even though <span class="hlt">wind</span> climatology is expected to change under the future climate. The present work examines future changes in <span class="hlt">wind</span> power output over Europe using an ensemble of ESMs. The power output is calculated using the entire <span class="hlt">wind</span> speed PDF and a non-constant power conversion coefficient. Based on this method, the ESM ensemble projects changes in near-future power outputs with a spatially varying magnitude between ‑12% and 8%. The most extreme changes occur over the Mediterranean <span class="hlt">region</span>. For the first time, the sensitivity of these future change in power output to the type of <span class="hlt">wind</span> turbine is also investigated. The analysis reveals that the projected <span class="hlt">wind</span> power changes may vary in up to half of their magnitude, depending on the type of turbine and <span class="hlt">region</span> of interest. As such, we recommend that <span class="hlt">wind</span> industries fully account for projected near-future changes in <span class="hlt">wind</span> power output by taking them into account as a well-defined loss/gain and uncertainty when estimating the yield of a future <span class="hlt">wind</span> farm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/1413179-wind-solar-resource-data-sets-wind-solar-resource-data-sets','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/1413179-wind-solar-resource-data-sets-wind-solar-resource-data-sets"><span><span class="hlt">Wind</span> and solar resource data sets: <span class="hlt">Wind</span> and solar resource data sets</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>Clifton, Andrew; Hodge, Bri-Mathias; Draxl, Caroline</p> <p></p> <p>The range of resource data sets spans from static cartography showing the mean annual <span class="hlt">wind</span> speed or solar irradiance across a <span class="hlt">region</span> to high temporal and high spatial resolution products that provide detailed information at a potential <span class="hlt">wind</span> or solar energy facility. These data sets are used to support continental-scale, national, or <span class="hlt">regional</span> renewable energy development; facilitate prospecting by developers; and enable grid integration studies. This review first provides an introduction to the <span class="hlt">wind</span> and solar resource data sets, then provides an overview of the common methods used for their creation and validation. A brief history of <span class="hlt">wind</span> and solarmore » resource data sets is then presented, followed by areas for future research.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29720682','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29720682"><span>Meteorological Controls on Local and <span class="hlt">Regional</span> Volcanic Ash Dispersal.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Poulidis, Alexandros P; Phillips, Jeremy C; Renfrew, Ian A; Barclay, Jenni; Hogg, Andrew; Jenkins, Susanna F; Robertson, Richard; Pyle, David M</p> <p>2018-05-02</p> <p>Volcanic ash has the capacity to impact human health, livestock, crops and infrastructure, including international air traffic. For recent major eruptions, information on the volcanic ash plume has been combined with relatively coarse-resolution meteorological model output to provide simulations of <span class="hlt">regional</span> ash dispersal, with reasonable success on the scale of hundreds of kilometres. However, to predict and mitigate these impacts locally, significant improvements in modelling capability are required. Here, we present results from a dynamic meteorological-ash-dispersion model configured with sufficient resolution to represent local topographic and convectively-forced flows. We focus on an archetypal volcanic setting, Soufrière, St Vincent, and use the exceptional historical records of the 1902 and 1979 eruptions to challenge our simulations. We find that the evolution and characteristics of ash deposition on St Vincent and nearby islands can be accurately simulated when the <span class="hlt">wind</span> shear associated with the <span class="hlt">trade</span> <span class="hlt">wind</span> inversion and topographically-forced flows are represented. The <span class="hlt">wind</span> shear plays a primary role and topographic flows a secondary role on ash distribution on local to <span class="hlt">regional</span> scales. We propose a new explanation for the downwind ash deposition maxima, commonly observed in volcanic eruptions, as resulting from the detailed forcing of mesoscale meteorology on the ash plume.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.749a2021S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.749a2021S"><span><span class="hlt">Wind</span> offering in energy and reserve markets</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Soares, T.; Pinson, P.; Morais, H.</p> <p>2016-09-01</p> <p>The increasing penetration of <span class="hlt">wind</span> generation in power systems to fulfil the ambitious European targets will make <span class="hlt">wind</span> power producers to play an even more important role in the future power system. <span class="hlt">Wind</span> power producers are being incentivized to participate in reserve markets to increase their revenue, since currently <span class="hlt">wind</span> turbine/farm technologies allow them to provide ancillary services. Thus, <span class="hlt">wind</span> power producers are to develop offering strategies for participation in both energy and reserve markets, accounting for market rules, while ensuring optimal revenue. We consider a proportional offering strategy to optimally decide upon participation in both markets by maximizing expected revenue from day-ahead decisions while accounting for estimated regulation costs for failing to provide the services. An evaluation of considering the same proportional splitting of energy and reserve in both day- ahead and balancing market is performed. A set of numerical examples illustrate the behavior of such strategy. An important conclusion is that the optimal split of the available <span class="hlt">wind</span> power between energy and reserve strongly depends upon prices and penalties on both market <span class="hlt">trading</span> floors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ClDy...45..441K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ClDy...45..441K"><span>Evaluating <span class="hlt">wind</span> extremes in CMIP5 climate models</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kumar, Devashish; Mishra, Vimal; Ganguly, Auroop R.</p> <p>2015-07-01</p> <p><span class="hlt">Wind</span> extremes have consequences for renewable energy sectors, critical infrastructures, coastal ecosystems, and insurance industry. Considerable debates remain regarding the impacts of climate change on <span class="hlt">wind</span> extremes. While climate models have occasionally shown increases in <span class="hlt">regional</span> <span class="hlt">wind</span> extremes, a decline in the magnitude of mean and extreme near-surface <span class="hlt">wind</span> speeds has been recently reported over most <span class="hlt">regions</span> of the Northern Hemisphere using observed data. Previous studies of <span class="hlt">wind</span> extremes under climate change have focused on selected <span class="hlt">regions</span> and employed outputs from the <span class="hlt">regional</span> climate models (RCMs). However, RCMs ultimately rely on the outputs of global circulation models (GCMs), and the value-addition from the former over the latter has been questioned. <span class="hlt">Regional</span> model runs rarely employ the full suite of GCM ensembles, and hence may not be able to encapsulate the most likely projections or their variability. Here we evaluate the performance of the latest generation of GCMs, the Coupled Model Intercomparison Project phase 5 (CMIP5), in simulating extreme <span class="hlt">winds</span>. We find that the multimodel ensemble (MME) mean captures the spatial variability of annual maximum <span class="hlt">wind</span> speeds over most <span class="hlt">regions</span> except over the mountainous terrains. However, the historical temporal trends in annual maximum <span class="hlt">wind</span> speeds for the reanalysis data, ERA-Interim, are not well represented in the GCMs. The historical trends in extreme <span class="hlt">winds</span> from GCMs are statistically not significant over most <span class="hlt">regions</span>. The MME model simulates the spatial patterns of extreme <span class="hlt">winds</span> for 25-100 year return periods. The projected extreme <span class="hlt">winds</span> from GCMs exhibit statistically less significant trends compared to the historical reference period.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22667397-baryon-cycle-high-redshifts-effects-galactic-winds-galaxy-evolution-overdense-average-regions','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22667397-baryon-cycle-high-redshifts-effects-galactic-winds-galaxy-evolution-overdense-average-regions"><span>THE BARYON CYCLE AT HIGH REDSHIFTS: EFFECTS OF GALACTIC <span class="hlt">WINDS</span> ON GALAXY EVOLUTION IN OVERDENSE AND AVERAGE <span class="hlt">REGIONS</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>Sadoun, Raphael; Shlosman, Isaac; Choi, Jun-Hwan</p> <p>2016-10-01</p> <p>We employ high-resolution cosmological zoom-in simulations focusing on a high-sigma peak and an average cosmological field at z ∼ 6–12 in order to investigate the influence of environment and baryonic feedback on galaxy evolution in the reionization epoch. Strong feedback, e.g., galactic <span class="hlt">winds</span>, caused by elevated star formation rates (SFRs) is expected to play an important role in this evolution. We compare different outflow prescriptions: (i) constant <span class="hlt">wind</span> velocity (CW), (ii) variable <span class="hlt">wind</span> scaling with galaxy properties (VW), and (iii) no outflows (NW). The overdensity leads to accelerated evolution of dark matter and baryonic structures, absent from the “normal” <span class="hlt">region</span>,more » and to shallow galaxy stellar mass functions at the low-mass end. Although CW shows little dependence on the environment, the more physically motivated VW model does exhibit this effect. In addition, VW can reproduce the observed specific SFR (sSFR) and the sSFR–stellar mass relation, which CW and NW fail to satisfy simultaneously. <span class="hlt">Winds</span> also differ substantially in affecting the state of the intergalactic medium (IGM). The difference lies in the volume-filling factor of hot, high-metallicity gas, which is near unity for CW, while such gas remains confined in massive filaments for VW, and locked up in galaxies for NW. Such gas is nearly absent from the normal <span class="hlt">region</span>. Although all <span class="hlt">wind</span> models suffer from deficiencies, the VW model seems to be promising in correlating the outflow properties with those of host galaxies. Further constraints on the state of the IGM at high z are needed to separate different <span class="hlt">wind</span> models.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://www.ars.usda.gov/research/publications/publication/?seqNo115=324277','TEKTRAN'); return false;" href="http://www.ars.usda.gov/research/publications/publication/?seqNo115=324277"><span>Evaluation of two empirical <span class="hlt">wind</span> erosion models in arid and semi-arid <span class="hlt">regions</span> of China and the USA</span></a></p> <p><a target="_blank" href="https://www.ars.usda.gov/research/publications/find-a-publication/">USDA-ARS?s Scientific Manuscript database</a></p> <p></p> <p></p> <p>The Tarim Basin in China and Columbia Plateau in the USA are important agricultural <span class="hlt">regions</span> as well as source <span class="hlt">regions</span> of windblown dust that impact air quality in Asia and North America. <span class="hlt">Wind</span> erosion models are important tools for assessing the potential erodibility of soils and best management prac...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1376666','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1376666"><span>Connecting Communities to <span class="hlt">Wind</span> Resources</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>Baring-Gould, Edward I</p> <p>2017-08-18</p> <p>WINDExchange is the platform for the U.S. Department of Energy's (DOE's) <span class="hlt">Wind</span> Energy Technologies Office to disseminate credible <span class="hlt">wind</span> energy information on a national level. Stakeholder engagement and outreach activities are designed to enable well-informed decisions about appropriate <span class="hlt">wind</span> energy deployment. WINDExchange focuses on <span class="hlt">wind</span> energy outreach at the national level while managing and supporting similar <span class="hlt">regional</span> efforts through the implementation of DOE <span class="hlt">Regional</span> Resource Centers (RRCs). This fact sheet provides an overview of DOE's WINDExchange initiative and the RRCs. Examples of RRC activities are provided.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1182264','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1182264"><span>Application of global weather and climate model output to the design and operation of <span class="hlt">wind</span>-energy 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>Curry, Judith</p> <p></p> <p>This project addressed the challenge of providing weather and climate information to support the operation, management and planning for <span class="hlt">wind</span>-energy systems. The need for forecast information is extending to longer projection windows with increasing penetration of <span class="hlt">wind</span> power into the grid and also with diminishing reserve margins to meet peak loads during significant weather events. Maintenance planning and natural gas <span class="hlt">trading</span> is being influenced increasingly by anticipation of <span class="hlt">wind</span> generation on timescales of weeks to months. Future scenarios on decadal time scales are needed to support assessment of <span class="hlt">wind</span> farm siting, government planning, long-term <span class="hlt">wind</span> purchase agreements and the regulatorymore » environment. The challenge of making <span class="hlt">wind</span> forecasts on these longer time scales is associated with a wide range of uncertainties in general circulation and <span class="hlt">regional</span> climate models that make them unsuitable for direct use in the design and planning of <span class="hlt">wind</span>-energy systems. To address this challenge, CFAN has developed a hybrid statistical/dynamical forecasting scheme for delivering probabilistic forecasts on time scales from one day to seven months using what is arguably the best forecasting system in the world (European Centre for Medium Range Weather Forecasting, ECMWF). The project also provided a framework to assess future <span class="hlt">wind</span> power through developing scenarios of interannual to decadal climate variability and change. The Phase II research has successfully developed an operational <span class="hlt">wind</span> power forecasting system for the U.S., which is being extended to Europe and possibly Asia.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A33E0289O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A33E0289O"><span><span class="hlt">Regional</span> downscaling of temporal resolution in near-surface <span class="hlt">wind</span> from statistically downscaled Global Climate Models (GCMs) for use in San Francisco Bay coastal flood modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>O'Neill, A.; Erikson, L. H.; Barnard, P.</p> <p>2013-12-01</p> <p>While Global Climate Models (GCMs) provide useful projections of near-surface <span class="hlt">wind</span> vectors into the 21st century, resolution is not sufficient enough for use in <span class="hlt">regional</span> wave modeling. Statistically downscaled GCM projections from Multivariate Adaptive Constructed Analogues (MACA) provide daily near-surface <span class="hlt">winds</span> at an appropriate spatial resolution for wave modeling within San Francisco Bay. Using 30 years (1975-2004) of climatological data from four representative stations around San Francisco Bay, a library of example daily <span class="hlt">wind</span> conditions for four corresponding over-water sub-<span class="hlt">regions</span> is constructed. Empirical cumulative distribution functions (ECDFs) of station conditions are compared to MACA GFDL hindcasts to create correction factors, which are then applied to 21st century MACA <span class="hlt">wind</span> projections. For each projection day, a best match example is identified via least squares error among all stations from the library. The best match's daily variation in velocity components (u/v) is used as an analogue of representative <span class="hlt">wind</span> variation and is applied at 3-hour increments about the corresponding sub-<span class="hlt">region</span>'s projected u/v values. High temporal resolution reconstructions using this methodology on hindcast MACA fields from 1975-2004 accurately recreate extreme <span class="hlt">wind</span> values within the San Francisco Bay, and because these extremes in <span class="hlt">wind</span> forcing are of key importance in wave and subsequent coastal flood modeling, this represents a valuable method of generating near-surface <span class="hlt">wind</span> vectors for use in coastal flood modeling.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/984676','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/984676"><span>Development of <span class="hlt">Regional</span> <span class="hlt">Wind</span> Resource and <span class="hlt">Wind</span> Plant Output Datasets for the Hawaiian Islands</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>Manobianco, J.; Alonge, C.; Frank, J.</p> <p></p> <p>In March 2009, AWS Truepower was engaged by the National Renewable Energy Laboratory (NREL) to develop a set of <span class="hlt">wind</span> resource and plant output data for the Hawaiian Islands. The objective of this project was to expand the methods and techniques employed in the Eastern <span class="hlt">Wind</span> Integration and Transmission Study (EWITS) to include the state of Hawaii.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EaFut...2..458D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EaFut...2..458D"><span>Feeding humanity through global food <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>D'Odorico, Paolo; Carr, Joel A.; Laio, Francesco; Ridolfi, Luca; Vandoni, Stefano</p> <p>2014-09-01</p> <p>The recent intensification of international <span class="hlt">trade</span> has led to a globalization of food commodities and to an increased disconnection between human populations and the land and water resources that support them through crop and livestock production. Several countries are not self-sufficient and depend on imports from other <span class="hlt">regions</span>. Despite the recognized importance of the role of <span class="hlt">trade</span> in global and <span class="hlt">regional</span> food security, the societal reliance on domestic production and international <span class="hlt">trade</span> remains poorly quantified. Here we investigate the global patterns of food <span class="hlt">trade</span> and evaluate the dependency of food security on imports. We investigate the relationship existing between the <span class="hlt">trade</span> of food calories and the virtual transfer of water used for their production. We show how the amount of food calories <span class="hlt">traded</span> in the international market has more than doubled between 1986 and 2009, while the number of links in the <span class="hlt">trade</span> network has increased by more than 50%. Likewise, global food production has increased by more than 50% in the same period, providing an amount of food that is overall sufficient to support the global population at a rate of 2700-3000 kcal per person per day. About 23% of the food produced for human consumption is <span class="hlt">traded</span> internationally. The water use efficiency of food <span class="hlt">trade</span> (i.e., food calories produced per unit volume of water used) has declined in the last few decades. The water use efficiency of food production overall increases with the countries' affluence; this trend is likely due to the use of more advanced technology.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_11");'>11</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li class="active"><span>13</span></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_13 --> <div id="page_14" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_12");'>12</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li class="active"><span>14</span></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="261"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017GSL.....4...24R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017GSL.....4...24R"><span>Surface <span class="hlt">wind</span> mixing in the <span class="hlt">Regional</span> Ocean Modeling System (ROMS)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Robertson, Robin; Hartlipp, Paul</p> <p>2017-12-01</p> <p>Mixing at the ocean surface is key for atmosphere-ocean interactions and the distribution of heat, energy, and gases in the upper ocean. <span class="hlt">Winds</span> are the primary force for surface mixing. To properly simulate upper ocean dynamics and the flux of these quantities within the upper ocean, models must reproduce mixing in the upper ocean. To evaluate the performance of the <span class="hlt">Regional</span> Ocean Modeling System (ROMS) in replicating the surface mixing, the results of four different vertical mixing parameterizations were compared against observations, using the surface mixed layer depth, the temperature fields, and observed diffusivities for comparisons. The vertical mixing parameterizations investigated were Mellor- Yamada 2.5 level turbulent closure (MY), Large- McWilliams- Doney Kpp (LMD), Nakanishi- Niino (NN), and the generic length scale (GLS) schemes. This was done for one temperate site in deep water in the Eastern Pacific and three shallow water sites in the Baltic Sea. The model reproduced the surface mixed layer depth reasonably well for all sites; however, the temperature fields were reproduced well for the deep site, but not for the shallow Baltic Sea sites. In the Baltic Sea, the models overmixed the water column after a few days. Vertical temperature diffusivities were higher than those observed and did not show the temporal fluctuations present in the observations. The best performance was by NN and MY; however, MY became unstable in two of the shallow simulations with high <span class="hlt">winds</span>. The performance of GLS nearly as good as NN and MY. LMD had the poorest performance as it generated temperature diffusivities that were too high and induced too much mixing. Further observational comparisons are needed to evaluate the effects of different stratification and <span class="hlt">wind</span> conditions and the limitations on the vertical mixing parameterizations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSA11A2244J','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSA11A2244J"><span>The variations of oxygen emissions in corresponding to Earth's aurora in low latitude <span class="hlt">region</span> under influence of solar <span class="hlt">wind</span> dynamics</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Jamlongkul, P.; Wannawichian, S.</p> <p>2017-12-01</p> <p>Earth's aurora in low latitude <span class="hlt">region</span> was studied via time variations of oxygen emission spectra, simultaneously with solar <span class="hlt">wind</span> data. The behavior of spectrum intensity, in corresponding with solar <span class="hlt">wind</span> condition, could be a trace of aurora in low latitude <span class="hlt">region</span> including some effects of high energetic auroral particles. Oxygen emission spectral lines were observed by Medium Resolution Echelle Spectrograph (MRES) at 2.4-m diameter telescope at Thai National Observatory, Inthanon Mountain, Chiang Mai, Thailand, during 1-5 LT on 5 and 6 February 2017. The observed spectral lines were calibrated via Dech95 - 2D image processing program and Dech-Fits spectra processing program for spectrum image processing and spectrum wavelength calibration, respectively. The variations of observed intensities each day were compared with solar <span class="hlt">wind</span> parameters, which are magnitude of IMF (|BIMF|) including IMF in RTN coordinate (BR, BT, BN), ion density (ρ), plasma flow pressure (P), and speed (v). The correlation coefficients between oxygen spectral emissions and different solar <span class="hlt">wind</span> parameters were found to vary in both positive and negative behaviors.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19840041504&hterms=Open+Field&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DOpen%2BField','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19840041504&hterms=Open+Field&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DOpen%2BField"><span>Transient behavior of a flare-associated solar <span class="hlt">wind</span>. I - Gas dynamics in a radial open field <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Nagai, F.</p> <p>1984-01-01</p> <p>A numerical investigation is conducted into the way in which a solar <span class="hlt">wind</span> model initially satisfying both steady state and energy balance conditions is disturbed and deformed, under the assumption of heating that correspoonds to the energy release of solar flares of an importance value of approximately 1 which occur in radial open field <span class="hlt">regions</span>. Flare-associated solar <span class="hlt">wind</span> transient behavior is modeled for 1-8 solar radii. The coronal temperature around the heat source <span class="hlt">region</span> rises, and a large thermal conductive flux flows inward to the chromosphere and outward to interplanetary space along field lines. The speed of the front of expanding chromospheric material generated by the impingement of the conduction front on the upper chromosphere exceeds the local sound velocity in a few minutes and eventually exceeds 100 million cm/sec.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950011783','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950011783"><span>Microburst vertical <span class="hlt">wind</span> estimation from horizontal <span class="hlt">wind</span> measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Vicroy, Dan D.</p> <p>1994-01-01</p> <p>The vertical <span class="hlt">wind</span> or downdraft component of a microburst-generated <span class="hlt">wind</span> shear can significantly degrade airplane performance. Doppler radar and lidar are two sensor technologies being tested to provide flight crews with early warning of the presence of hazardous <span class="hlt">wind</span> shear. An inherent limitation of Doppler-based sensors is the inability to measure velocities perpendicular to the line of sight, which results in an underestimate of the total <span class="hlt">wind</span> shear hazard. One solution to the line-of-sight limitation is to use a vertical <span class="hlt">wind</span> model to estimate the vertical component from the horizontal <span class="hlt">wind</span> measurement. The objective of this study was to assess the ability of simple vertical <span class="hlt">wind</span> models to improve the hazard prediction capability of an airborne Doppler sensor in a realistic microburst environment. Both simulation and flight test measurements were used to test the vertical <span class="hlt">wind</span> models. The results indicate that in the altitude <span class="hlt">region</span> of interest (at or below 300 m), the simple vertical <span class="hlt">wind</span> models improved the hazard estimate. The radar simulation study showed that the magnitude of the performance improvement was altitude dependent. The altitude of maximum performance improvement occurred at about 300 m.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-06-01/pdf/2012-13361.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-06-01/pdf/2012-13361.pdf"><span>77 FR 32497 - Grant of Authority for Subzone Status; Mitsubishi Power Systems Americas, Inc. (<span class="hlt">Wind</span> Turbine...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-06-01</p> <p>... DEPARTMENT OF COMMERCE Foreign-<span class="hlt">Trade</span> Zones Board [Order No. 1832] Grant of Authority for Subzone Status; Mitsubishi Power Systems Americas, Inc. (<span class="hlt">Wind</span> Turbine Nacelles and Generating Sets) Fort Smith, AR Pursuant to its authority under the Foreign-<span class="hlt">Trade</span> Zones Act of June 18, 1934, as amended (19 U.S.C. 81a-81u), the Foreign-<span class="hlt">Trade</span> Zones Board (th...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20070032710','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20070032710"><span>Lidar and Mission Parameter <span class="hlt">Trade</span> Study of Space-Based Coherent <span class="hlt">Wind</span> Measurement Centered on NASA's 2006 GWOS <span class="hlt">Wind</span> Mission Study Parameters</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kavaya, Michael J.; Frehlich, Rod G.</p> <p>2007-01-01</p> <p>The global measurement of vertical profiles of horizontal vector <span class="hlt">winds</span> has been highly desired for many years by NASA, NOAA and the Integrated Program Office (IPO) implementing the National Polar-orbiting Operational Environmental Satellite Systems (NPOESS). Recently the global <span class="hlt">wind</span> mission was one of 15 missions recommended to NASA by the first ever NRC Earth Sciences Decadal Survey. Since before 1978, the most promising method to make this space-based measurement has been pulsed Doppler lidar. The favored technology and technique has evolved over the years from obtaining line-of-sight (LOS) <span class="hlt">wind</span> profiles from a single laser shot using pulsed CO2 gas laser technology to the current plans to use both a coherent-detection and direct-detection pulsed Doppler <span class="hlt">wind</span> lidar systems with each lidar employing multiple shot accumulation to produce an LOS <span class="hlt">wind</span> profile. The idea of using two lidars (hybrid concept) entails coherent detection using the NASA LaRC-developed pulsed 2-micron solid state laser technology, and direct detection using pulsed Nd:YAG laser technology tripled in frequency to 355 nm wavelength.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA13907.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA13907.html"><span><span class="hlt">Wind</span> and Rock</span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2011-03-09</p> <p>This image from NASA Mars Odyssey is located west of Zephyria Planum. Surfaces in this <span class="hlt">region</span> have undergone extensive erosion by the <span class="hlt">wind</span>. <span class="hlt">Wind</span> is one of the most active processes of erosion on the surface of Mars today.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017PhDT.......160S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017PhDT.......160S"><span>The Impact of Coastal Terrain on Offshore <span class="hlt">Wind</span> and Implications for <span class="hlt">Wind</span> Energy</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Strobach, Edward Justin</p> <p></p> <p>The development of offshore <span class="hlt">wind</span> energy is moving forward as one of several options for carbon-free energy generation along the populous US east coast. Accurate assessments of the <span class="hlt">wind</span> resource are essential and can significantly lower financing costs that have been a barrier to development. <span class="hlt">Wind</span> resource assessment in the Mid-Atlantic <span class="hlt">region</span> is challenging since there are no long-term measurements of <span class="hlt">winds</span> across the rotor span. Features of the coastal and inland terrain, such as such as the Appalachian mountains and the Chesapeake Bay, are known to lead to complex mesoscale <span class="hlt">wind</span> regimes onshore, including low-level jets (LLJs), downslope <span class="hlt">winds</span> and sea breezes. Little is known, however, about whether or how the inland physiography impacts the <span class="hlt">winds</span> offshore. This research is based on the first comprehensive set of offshore <span class="hlt">wind</span> observations in the Maryland <span class="hlt">Wind</span> Energy Area gathered during a UMBC measurement campaign. The presentation will include a case study of a strong nocturnal LLJ that persisted for several hours before undergoing a rapid breakdown and loss of energy to smaller scales. Measurements from an onshore <span class="hlt">wind</span> profiler and radiosondes, together with North American <span class="hlt">Regional</span> Analysis (NARR) and a high resolution Weather Research and Forecast (WRF) model simulation, are used to untangle the forcing mechanisms on synoptic, <span class="hlt">regional</span> and local scales that led to the jet and its collapse. The results suggest that the evolution of LLJs were impacted by a downslope <span class="hlt">wind</span> from the Appalachians that propagated offshore riding atop a shallow near-surface boundary layer across the coastal plain. Baroclinic forcing from low sea surface temperatures (SSTs) due to coastal upwelling is also discussed. Smaller scale details of the LLJ breakdown are analyzed using a wave/mean flow/turbulence interaction approach. The case study illustrates several characteristics of low-level <span class="hlt">winds</span> offshore that are important for <span class="hlt">wind</span> energy, including LLJs, strong <span class="hlt">wind</span> shear, turbulence</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013EGUGA..1510133D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013EGUGA..1510133D"><span>The Etesian <span class="hlt">wind</span> system and <span class="hlt">wind</span> energy potential over the Aegean Sea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dafka, Stella; Xoplaki, Elena; Garcia-Bustamante, Elena; Toreti, Andrea; Zanis, Prodromos; Luterbacher, Juerg</p> <p>2013-04-01</p> <p>The Mediterranean <span class="hlt">region</span> lies in an area of great climatic interest since it is influenced by some of the most relevant mechanisms of the global climate system. In the frame of the three Europe 2020 priorities for a smart, sustainable and inclusive economy delivering high levels of employment, productivity and social cohesion, the Mediterranean energy plan is of paramount importance at the European level, being an area with a significant potential for renewable energy from natural sources that could play an important role in responding to climate change effects over the <span class="hlt">region</span>. We present preliminary results on a study of the Etesian <span class="hlt">winds</span> in the past, present and future time. We investigate the variability and predictability of the <span class="hlt">wind</span> field over the Aegean. Statistical downscaling based on several methodologies will be applied (e.g. canonical correlation analysis and multiple linear regression). Instrumental time series, Era-Interim and the 20CR reanalyses will be used. Large-scale climate drivers as well as the influence of local/<span class="hlt">regional</span> factors and their interaction with the Etesian <span class="hlt">wind</span> field will be addressed. Finally, the Etesian <span class="hlt">wind</span> resources on the present and future climate will be assessed in order to identify the potential areas suitable for the establishment of <span class="hlt">wind</span> farms and the production of <span class="hlt">wind</span> power in the Aegean Sea.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-08-18/pdf/2011-21143.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-08-18/pdf/2011-21143.pdf"><span>76 FR 51349 - Foreign-<span class="hlt">Trade</span> Zone 72-Indianapolis, IN; Application for Manufacturing Authority, Brevini <span class="hlt">Wind</span> USA...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-08-18</p> <p>...--Indianapolis, IN; Application for Manufacturing Authority, Brevini <span class="hlt">Wind</span> USA, Inc., (<span class="hlt">Wind</span> Turbine Gear Boxes... Airport Authority, grantee of FTZ 72, requesting manufacturing authority on behalf of Brevini <span class="hlt">Wind</span> USA, Inc. (Brevini), to manufacture <span class="hlt">wind</span> turbine gear boxes under FTZ procedures within FTZ 72. The...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25617767','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25617767"><span>A nonlinear dynamics approach for incorporating <span class="hlt">wind</span>-speed patterns into <span class="hlt">wind</span>-power project evaluation.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Huffaker, Ray; Bittelli, Marco</p> <p>2015-01-01</p> <p><span class="hlt">Wind</span>-energy production may be expanded beyond <span class="hlt">regions</span> with high-average <span class="hlt">wind</span> speeds (such as the Midwest U.S.A.) to sites with lower-average speeds (such as the Southeast U.S.A.) by locating favorable <span class="hlt">regional</span> matches between natural <span class="hlt">wind</span>-speed and energy-demand patterns. A critical component of <span class="hlt">wind</span>-power evaluation is to incorporate <span class="hlt">wind</span>-speed dynamics reflecting documented diurnal and seasonal behavioral patterns. Conventional probabilistic approaches remove patterns from <span class="hlt">wind</span>-speed data. These patterns must be restored synthetically before they can be matched with energy-demand patterns. How to accurately restore <span class="hlt">wind</span>-speed patterns is a vexing problem spurring an expanding line of papers. We propose a paradigm shift in <span class="hlt">wind</span> power evaluation that employs signal-detection and nonlinear-dynamics techniques to empirically diagnose whether synthetic pattern restoration can be avoided altogether. If the complex behavior of observed <span class="hlt">wind</span>-speed records is due to nonlinear, low-dimensional, and deterministic system dynamics, then nonlinear dynamics techniques can reconstruct <span class="hlt">wind</span>-speed dynamics from observed <span class="hlt">wind</span>-speed data without recourse to conventional probabilistic approaches. In the first study of its kind, we test a nonlinear dynamics approach in an application to Sugarland <span class="hlt">Wind</span>-the first utility-scale <span class="hlt">wind</span> project proposed in Florida, USA. We find empirical evidence of a low-dimensional and nonlinear <span class="hlt">wind</span>-speed attractor characterized by strong temporal patterns that match up well with regular daily and seasonal electricity demand patterns.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-03-09/pdf/2012-5785.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-03-09/pdf/2012-5785.pdf"><span>77 FR 14342 - Utility Scale <span class="hlt">Wind</span> Towers From the People's Republic of China: Notice of Postponement of...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-03-09</p> <p>... DEPARTMENT OF COMMERCE International <span class="hlt">Trade</span> Administration [C-570-982] Utility Scale <span class="hlt">Wind</span> Towers... 202-482-1503, respectively. SUPPLEMENTARY INFORMATION: Background On January 18, 2012, the Department of Commerce (the Department) initiated the countervailing duty investigation of utility scale <span class="hlt">wind</span>...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2964241','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2964241"><span>Impacts of <span class="hlt">wind</span> farms on surface air temperatures</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Baidya Roy, Somnath; Traiteur, Justin J.</p> <p>2010-01-01</p> <p>Utility-scale large <span class="hlt">wind</span> farms are rapidly growing in size and numbers all over the world. Data from a meteorological field campaign show that such <span class="hlt">wind</span> farms can significantly affect near-surface air temperatures. These effects result from enhanced vertical mixing due to turbulence generated by <span class="hlt">wind</span> turbine rotors. The impacts of <span class="hlt">wind</span> farms on local weather can be minimized by changing rotor design or by siting <span class="hlt">wind</span> farms in <span class="hlt">regions</span> with high natural turbulence. Using a 25-y-long climate dataset, we identified such <span class="hlt">regions</span> in the world. Many of these <span class="hlt">regions</span>, such as the Midwest and Great Plains in the United States, are also rich in <span class="hlt">wind</span> resources, making them ideal candidates for low-impact <span class="hlt">wind</span> farms. PMID:20921371</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004cosp...35..230C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004cosp...35..230C"><span>Results of the horizontal and meridional thermospheric <span class="hlt">winds</span> in the cachoeira paulista (22.5s; 45w), a low latitude station in Brazilian <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Castilho, V. M.; Sobral, J. H. A.; Abdu, M. A.; Takahashi, H.; Arruda, D. C. S.</p> <p></p> <p>At this point, 74 nights have been observed during the period of May 2002 to March 2003, high to low solar activity period, by Fabry-Perot Interferometer operating at Cachoeira Paulista - CP (22.5S; 45W). This study focuses the monthly and seasonal analysis of the horizontal and meridional components of the thermospheric <span class="hlt">winds</span> at CP. For the studied <span class="hlt">region</span>, the zonal component of the thermospheric <span class="hlt">winds</span> is predominantly eastward during the nocturnal hours and the meridional component is southward in the initial nocturnal hours and northward in the end of the night. Undesturbed F-<span class="hlt">region</span> e-filds at low latitudes are primarily generated by the thermospheric <span class="hlt">winds</span>. Ionosphere plasma drifts and thermospheric <span class="hlt">winds</span> are important transport mechanisms that affect the electron density distribution. The results observed are compared with HWM93 model. KEY WORDS: Fabry Perot Interferometer, Thermospheric <span class="hlt">Winds</span>, OI 630nm.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA04134&hterms=landscape&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlandscape','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA04134&hterms=landscape&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3Dlandscape"><span><span class="hlt">Wind</span>-Eroded Landscape</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2005-01-01</p> <p><p/> 5 August 2005 This Mars Global Surveyor (MGS) Mars Orbiter Camera (MOC) image shows a dust-mantled, <span class="hlt">wind</span>-eroded landscape in the Medusae Sulci <span class="hlt">region</span> of Mars. <span class="hlt">Wind</span> eroded the bedrock in this <span class="hlt">region</span>, and then, later, windblown dust covered much of the terrain. <p/> <i>Location near</i>: 5.7oS, 160.2oW <i>Image width</i>: width: 3 km (1.9 mi) <i>Illumination from</i>: lower left <i>Season</i>: Southern Spring</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4305325','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4305325"><span>A Nonlinear Dynamics Approach for Incorporating <span class="hlt">Wind</span>-Speed Patterns into <span class="hlt">Wind</span>-Power Project Evaluation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Huffaker, Ray; Bittelli, Marco</p> <p>2015-01-01</p> <p><span class="hlt">Wind</span>-energy production may be expanded beyond <span class="hlt">regions</span> with high-average <span class="hlt">wind</span> speeds (such as the Midwest U.S.A.) to sites with lower-average speeds (such as the Southeast U.S.A.) by locating favorable <span class="hlt">regional</span> matches between natural <span class="hlt">wind</span>-speed and energy-demand patterns. A critical component of <span class="hlt">wind</span>-power evaluation is to incorporate <span class="hlt">wind</span>-speed dynamics reflecting documented diurnal and seasonal behavioral patterns. Conventional probabilistic approaches remove patterns from <span class="hlt">wind</span>-speed data. These patterns must be restored synthetically before they can be matched with energy-demand patterns. How to accurately restore <span class="hlt">wind</span>-speed patterns is a vexing problem spurring an expanding line of papers. We propose a paradigm shift in <span class="hlt">wind</span> power evaluation that employs signal-detection and nonlinear-dynamics techniques to empirically diagnose whether synthetic pattern restoration can be avoided altogether. If the complex behavior of observed <span class="hlt">wind</span>-speed records is due to nonlinear, low-dimensional, and deterministic system dynamics, then nonlinear dynamics techniques can reconstruct <span class="hlt">wind</span>-speed dynamics from observed <span class="hlt">wind</span>-speed data without recourse to conventional probabilistic approaches. In the first study of its kind, we test a nonlinear dynamics approach in an application to Sugarland Wind—the first utility-scale <span class="hlt">wind</span> project proposed in Florida, USA. We find empirical evidence of a low-dimensional and nonlinear <span class="hlt">wind</span>-speed attractor characterized by strong temporal patterns that match up well with regular daily and seasonal electricity demand patterns. PMID:25617767</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018AeoRe..32...24S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018AeoRe..32...24S"><span>Application of fuzzy logic approach for <span class="hlt">wind</span> erosion hazard mapping in Laghouat <span class="hlt">region</span> (Algeria) using remote sensing and GIS</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saadoud, Djouher; Hassani, Mohamed; Martin Peinado, Francisco José; Guettouche, Mohamed Saïd</p> <p>2018-06-01</p> <p><span class="hlt">Wind</span> erosion is one of the most serious environmental problems in Algeria that threatens human activities and socio-economic development. The main goal of this study is to apply a fuzzy logic approach to <span class="hlt">wind</span> erosion sensitivity mapping in the Laghouat <span class="hlt">region</span>, Algeria. Six causative factors, obtained by applying fuzzy membership functions to each used parameter, are considered: soil, vegetation cover, <span class="hlt">wind</span> factor, soil dryness, land topography and land cover sensitivity. Different fuzzy operators (AND, OR, SUM, PRODUCT, and GAMMA) are applied to generate <span class="hlt">wind</span>-erosion hazard map. Success rate curves reveal that the fuzzy gamma (γ) operator, with γ equal to 0.9, gives the best prediction accuracy with an area under curve of 85.2%. The resulting <span class="hlt">wind</span>-erosion sensitivity map delineates the area into different zones of five relative sensitivity classes: very high, high, moderate, low and very low. The estimated result was verified by field measurements and the high statistically significant value of a chi-square test.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4404753','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4404753"><span>Managing dynamic epidemiological risks through <span class="hlt">trade</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>Horan, Richard D.; Fenichel, Eli P.; Finnoff, David; Wolf, Christopher A.</p> <p>2015-01-01</p> <p>There is growing concern that <span class="hlt">trade</span>, by connecting geographically isolated <span class="hlt">regions</span>, unintentionally facilitates the spread of invasive pathogens and pests – forms of biological pollution that pose significant risks to ecosystem and human health. We use a bioeconomic framework to examine whether <span class="hlt">trade</span> always increases private risks, focusing specifically on pathogen risks from live animal <span class="hlt">trade</span>. When the pathogens have already established and traders bear some private risk, we find two results that run counter to the conventional wisdom on <span class="hlt">trade</span>. First, uncertainty about the disease status of individual animals held in inventory may increase the incentives to <span class="hlt">trade</span> relative to the disease-free case. Second, <span class="hlt">trade</span> may facilitate reduced long-run disease prevalence among buyers. These results arise because disease risks are endogenous due to dynamic feedback processes involving valuable inventories, and markets facilitate the management of private risks that producers face with or without <span class="hlt">trade</span>. PMID:25914431</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ERL....12c4022V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ERL....12c4022V"><span>Prospects for generating electricity by large onshore and offshore <span class="hlt">wind</span> farms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Volker, Patrick J. H.; Hahmann, Andrea N.; Badger, Jake; Jørgensen, Hans E.</p> <p>2017-03-01</p> <p>The decarbonisation of energy sources requires additional investments in renewable technologies, including the installation of onshore and offshore <span class="hlt">wind</span> farms. For <span class="hlt">wind</span> energy to remain competitive, <span class="hlt">wind</span> farms must continue to provide low-cost power even when covering larger areas. Inside very large <span class="hlt">wind</span> farms, <span class="hlt">winds</span> can decrease considerably from their free-stream values to a point where an equilibrium <span class="hlt">wind</span> speed is reached. The magnitude of this equilibrium <span class="hlt">wind</span> speed is primarily dependent on the balance between turbine drag force and the downward momentum influx from above the <span class="hlt">wind</span> farm. We have simulated for neutral atmospheric conditions, the <span class="hlt">wind</span> speed field inside different <span class="hlt">wind</span> farms that range from small (25 km2) to very large (105 km2) in three <span class="hlt">regions</span> with distinct <span class="hlt">wind</span> speed and roughness conditions. Our results show that the power density of very large <span class="hlt">wind</span> farms depends on the local free-stream <span class="hlt">wind</span> speed, the surface characteristics, and the turbine density. In onshore <span class="hlt">regions</span> with moderate <span class="hlt">winds</span> the power density of very large <span class="hlt">wind</span> farms reaches 1 W m-2, whereas in offshore <span class="hlt">regions</span> with very strong <span class="hlt">winds</span> it exceeds 3 W m-2. Despite a relatively low power density, onshore <span class="hlt">regions</span> with moderate <span class="hlt">winds</span> offer potential locations for very large <span class="hlt">wind</span> farms. In offshore <span class="hlt">regions</span>, clusters of smaller <span class="hlt">wind</span> farms are generally preferable; under very strong <span class="hlt">winds</span> also very large offshore <span class="hlt">wind</span> farms become efficient.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGC41D0860G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGC41D0860G"><span>Characterization of <span class="hlt">wind</span> power resource and its intermittency</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gunturu, U. B.; Schlosser, C. A.</p> <p>2011-12-01</p> <p><span class="hlt">Wind</span> resource in the continental and offshore United States has been calculated and characterized using metrics that describe - apart from abundance - its availability, persistence and intermittency. The Modern Era Retrospective-Analysis for Research and Applications (MERRA) boundary layer flux data has been used to construct <span class="hlt">wind</span> power density profiles at 50, 80, 100 and 120 m turbine hub heights. The <span class="hlt">wind</span> power density estimates at 50 m are qualitatively similar to those in the US <span class="hlt">wind</span> atlas developed by the National Renewable Energy Laboratory (NREL), but quantitatively a class less in some <span class="hlt">regions</span>, but are within the limits of uncertainty. We also show that for long tailed distributions like those of the <span class="hlt">wind</span> power density, the mean is an overestimation and median is a more robust metric for summary representation of <span class="hlt">wind</span> power resource.Generally speaking, the largest and most available <span class="hlt">wind</span> power density resources are found in off-shore <span class="hlt">regions</span> of the Atlantic and Pacific coastline, and the largest on-shore resource potential lies in the central United States. However, the intermittency and widespread synchronicity of on-shore <span class="hlt">wind</span> power density are substantial, and highlights areas where considerable back-up generation technologies will be required. Generation-duration curves are also presented for the independent systems operator (ISO) zones of the U.S. to highlight the <span class="hlt">regions</span> with the largest capacity factor (MISO, ERCOT, and SWPP) as well as the periods and extent to which all ISOs contain no <span class="hlt">wind</span> power and the potential benefits of aggregation on <span class="hlt">wind</span> power intermittency in each <span class="hlt">region</span>. The impact of raising the <span class="hlt">wind</span> turbine hub height on metrics of abundance, persistence, variability and intermittency is analyzed. There is a general increase in availability and abundance of <span class="hlt">wind</span> resource but there is also an increase in intermittency with respect to a 'usable <span class="hlt">wind</span> power' crossing level in low resource <span class="hlt">regions</span>. A similar perspective of <span class="hlt">wind</span> resource for</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2016EP%26S...68..201R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EP%26S...68..201R"><span>Competition between <span class="hlt">winds</span> and electric fields in the formation of blanketing sporadic E layers at equatorial <span class="hlt">regions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Resende, Laysa Cristina Araújo; Batista, Inez Staciarini; Denardini, Clezio Marcos; Carrasco, Alexander José; de Fátima Andrioli, Vânia; Moro, Juliano; Batista, Paulo Prado; Chen, Sony Su</p> <p>2016-12-01</p> <p>In the present work, we analyze the competition between tidal <span class="hlt">winds</span> and electric fields in the formation of blanketing sporadic E layers (Esb) over São Luís, Brazil (2° 31' S, 44° 16' W), a quasi-equatorial station. To investigate this competition, we have used an ionospheric E <span class="hlt">region</span> model (MIRE) that is able to model the Esb layers taking into account the E <span class="hlt">region</span> <span class="hlt">winds</span> and electric fields. The model calculates the densities for the main molecular and metallic ions by solving the continuity and momentum equations for each of the species. Thus, the main purpose of this analysis is to verify the electric fields role in the occurrence or disruption of Esb layers through simulations. The first results of the simulations show that the Esb layer is usually present when only the tidal <span class="hlt">winds</span> were considered. In addition, when the zonal component of the electric field is introduced in the simulation, the Esb layers do not show significant changes. However, the simulations show the disruption of the Esb layers when the vertical electric field is included. In this study, we present two specific cases in which Esb layers appear during some hours over São Luís. We can see that these layers appear when the vertical electric field was weak, which means that the tidal components were more effective during these hours. Therefore, the vertical component of the electric field is the main agent responsible for the Esb layer disruption. [Figure not available: see fulltext. Caption: Ionograms from São Luís on January 5, 2005, show a clear case of the competition between electric fields and <span class="hlt">wind</span> effects in the Es layer formation. In ionograms, the Esq trace is clearly seen and identified by a blue arrow. Besides the Esq, we can identify another Es trace at 1415 UT (identified by a black arrow) that persists until 1600 UT. This layer becomes stronger in each ionogram, as can be seen by its effect on partially blocking the reflection from the low-frequency end of F <span class="hlt">region</span> above</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=trading&pg=4&id=EJ696601','ERIC'); return false;" href="https://eric.ed.gov/?q=trading&pg=4&id=EJ696601"><span>Asset Prices and <span class="hlt">Trading</span> Volume under Fixed Transactions Costs.</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>Lo, Andrew W.; Mamaysky, Harry; Wang, Jiang</p> <p>2004-01-01</p> <p>We propose a dynamic equilibrium model of asset prices and <span class="hlt">trading</span> volume when agents face fixed transactions costs. We show that even small fixed costs can give rise to large "no-<span class="hlt">trade</span>" <span class="hlt">regions</span> for each agent's optimal <span class="hlt">trading</span> policy. The inability to <span class="hlt">trade</span> more frequently reduces the agents' asset demand and in equilibrium gives rise to a…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800017495','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800017495"><span>Vector <span class="hlt">wind</span> profile gust model</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Adelfang, S. I.</p> <p>1979-01-01</p> <p>Work towards establishing a vector <span class="hlt">wind</span> profile gust model for the Space Transportation System flight operations and <span class="hlt">trade</span> studies is reported. To date, all the statistical and computational techniques required were established and partially implemented. An analysis of <span class="hlt">wind</span> profile gust at Cape Kennedy within the theoretical framework is presented. The variability of theoretical and observed gust magnitude with filter type, altitude, and season is described. Various examples are presented which illustrate agreement between theoretical and observed gust percentiles. The preliminary analysis of the gust data indicates a strong variability with altitude, season, and wavelength regime. An extension of the analyses to include conditional distributions of gust magnitude given gust length, distributions of gust modulus, and phase differences between gust components has begun.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-08-01/pdf/2011-19404.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-08-01/pdf/2011-19404.pdf"><span>76 FR 45772 - Proposed Foreign-<span class="hlt">Trade</span> Zone-Brunswick, ME; Application</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-08-01</p> <p>... DEPARTMENT OF COMMERCE Foreign-<span class="hlt">Trade</span> Zones Board [Docket 49-2011] Proposed Foreign-<span class="hlt">Trade</span> Zone--Brunswick, ME; Application An application has been submitted to the Foreign-<span class="hlt">Trade</span> Zones Board (the Board) by the Midcoast <span class="hlt">Regional</span> Redevelopment Authority to establish a general-purpose foreign-<span class="hlt">trade</span> zone at a...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29156391','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29156391"><span>Optimal allocation of physical water resources integrated with virtual water <span class="hlt">trade</span> in water scarce <span class="hlt">regions</span>: A case study for Beijing, China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Ye, Quanliang; Li, Yi; Zhuo, La; Zhang, Wenlong; Xiong, Wei; Wang, Chao; Wang, Peifang</p> <p>2018-02-01</p> <p>This study provides an innovative application of virtual water <span class="hlt">trade</span> in the traditional allocation of physical water resources in water scarce <span class="hlt">regions</span>. A multi-objective optimization model was developed to optimize the allocation of physical water and virtual water resources to different water users in Beijing, China, considering the <span class="hlt">trade</span>-offs between economic benefit and environmental impacts of water consumption. Surface water, groundwater, transferred water and reclaimed water constituted the physical resource of water supply side, while virtual water flow associated with the <span class="hlt">trade</span> of five major crops (barley, corn, rice, soy and wheat) and three livestock products (beef, pork and poultry) in agricultural sector (calculated by the <span class="hlt">trade</span> quantities of products and their virtual water contents). Urban (daily activities and public facilities), industry, environment and agriculture (products growing) were considered in water demand side. As for the traditional allocation of physical water resources, the results showed that agriculture and urban were the two predominant water users (accounting 54% and 28%, respectively), while groundwater and surface water satisfied around 70% water demands of different users (accounting 36% and 34%, respectively). When considered the virtual water <span class="hlt">trade</span> of eight agricultural products in water allocation procedure, the proportion of agricultural consumption decreased to 45% in total water demand, while the groundwater consumption decreased to 24% in total water supply. Virtual water <span class="hlt">trade</span> overturned the traditional components of water supplied from different sources for agricultural consumption, and became the largest water source in Beijing. Additionally, it was also found that environmental demand took a similar percentage of water consumption in each water source. Reclaimed water was the main water source for industrial and environmental users. The results suggest that physical water resources would mainly satisfy the consumption</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2004AGUFMSF43A0784G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2004AGUFMSF43A0784G"><span>GPS Ocean Reflection Experiment (GORE) <span class="hlt">Wind</span> Explorer (<span class="hlt">Wind</span>Ex) Instrument Design and Development</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ganoe, G.</p> <p>2004-12-01</p> <p>This paper describes the design and development of the <span class="hlt">Wind</span>Ex instrument, and the technology implemented by it. The important design <span class="hlt">trades</span> will be covered along with the justification for the options selected. An evaluation of the operation of the instrument, and plans for continued development and enhancements will also be given. The <span class="hlt">Wind</span>Ex instrument consists of a processor that receives data from an included GPS Surface reflection receiver, and computes ocean surface <span class="hlt">wind</span> speeds in real time utilizing an algorithm developed at LaRC by Dr. Stephen J. Katzberg. The <span class="hlt">Wind</span>Ex performs a windspeed server function as well as acting as a repository for the client moving map applications, and providing a web page with instructions on the installation and use of the <span class="hlt">Wind</span>Ex system. The server receives the GPS reflection data produced by the receiver, performs <span class="hlt">wind</span> speed processing, then makes the <span class="hlt">wind</span> speed data available as a moving map display to requesting client processors on the aircraft network. The client processors are existing systems used by the research personnel onboard. They can be configured to be WINDEX clients by downloading the Java client application from the WINDEX server. The client application provides a graphical display of a moving map that shows the aircraft position along with the position of the reflection point from the surface of the ocean where the <span class="hlt">wind</span> speed is being estimated, and any coastlines within the field of view. Information associated with the reflection point includes the estimated <span class="hlt">wind</span> speed, and a confidence factor that gives the researcher an idea about the reliability of the <span class="hlt">wind</span> speed measurement. The instrument has been installed on one of NOAA's Hurricane Hunters, a Gulfstream IV, whose nickname is "Gonzo". Based at MacDill AFB, Florida, "Gonzo" flies around the periphery of the storm deploying GPS-based dropsondes which measure local <span class="hlt">winds</span>. The dropsondes are the "gold-standard" for determining surface <span class="hlt">winds</span>, but can only be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016GeoRL..43..728G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016GeoRL..43..728G"><span>Simulated effects of southern hemispheric <span class="hlt">wind</span> changes on the Pacific oxygen minimum zone</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Getzlaff, Julia; Dietze, Heiner; Oschlies, Andreas</p> <p>2016-01-01</p> <p>A coupled ocean biogeochemistry-circulation model is used to investigate the impact of observed past and anticipated future <span class="hlt">wind</span> changes in the Southern Hemisphere on the oxygen minimum zone in the tropical Pacific. We consider the industrial period until the end of the 21st century and distinguish effects due to a strengthening of the westerlies from effects of a southward shift of the westerlies that is accompanied by a poleward expansion of the tropical <span class="hlt">trade</span> <span class="hlt">winds</span>. Our model results show that a strengthening of the westerlies counteracts part of the warming-induced decline in the global marine oxygen inventory. A poleward shift of the <span class="hlt">trade</span>-westerlies boundary, however, triggers a significant decrease of oxygen in the tropical oxygen minimum zone. In a business-as-usual CO2 emission scenario, the poleward shift of the <span class="hlt">trade</span>-westerlies boundary and warming-induced increase in stratification contribute equally to the expansion of suboxic waters in the tropical Pacific.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014JIEIA..95..157R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014JIEIA..95..157R"><span>Stochastic Analysis of <span class="hlt">Wind</span> Energy for <span class="hlt">Wind</span> Pump Irrigation in Coastal Andhra Pradesh, India</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Raju, M. M.; Kumar, A.; Bisht, D.; Rao, D. B.</p> <p>2014-09-01</p> <p>The rapid escalation in the prices of oil and gas as well as increasing demand for energy has attracted the attention of scientists and researchers to explore the possibility of generating and utilizing the alternative and renewable sources of <span class="hlt">wind</span> energy in the long coastal belt of India with considerable <span class="hlt">wind</span> energy resources. A detailed analysis of <span class="hlt">wind</span> potential is a prerequisite to harvest the <span class="hlt">wind</span> energy resources efficiently. Keeping this in view, the present study was undertaken to analyze the <span class="hlt">wind</span> energy potential to assess feasibility of the <span class="hlt">wind</span>-pump operated irrigation system in the coastal <span class="hlt">region</span> of Andhra Pradesh, India, where high ground water table conditions are available. The stochastic analysis of <span class="hlt">wind</span> speed data were tested to fit a probability distribution, which describes the <span class="hlt">wind</span> energy potential in the <span class="hlt">region</span>. The normal and Weibull probability distributions were tested; and on the basis of Chi square test, the Weibull distribution gave better results. Hence, it was concluded that the Weibull probability distribution may be used to stochastically describe the annual <span class="hlt">wind</span> speed data of coastal Andhra Pradesh with better accuracy. The size as well as the complete irrigation system with mass curve analysis was determined to satisfy various daily irrigation demands at different risk levels.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26249172','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26249172"><span>E-commerce <span class="hlt">trade</span> in invasive plants.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Humair, Franziska; Humair, Luc; Kuhn, Fabian; Kueffer, Christoph</p> <p>2015-12-01</p> <p>Biological invasions are a major concern in conservation, especially because global transport of species is still increasing rapidly. Conservationists hope to anticipate and thus prevent future invasions by identifying and regulating potentially invasive species through species risk assessments and international <span class="hlt">trade</span> regulations. Among many introduction pathways of non-native species, horticulture is a particularly important driver of plant invasions. In recent decades, the horticultural industry expanded globally and changed structurally through the emergence of new distribution channels, including internet <span class="hlt">trade</span> (e-commerce). Using an automated search algorithm, we surveyed, on a daily basis, e-commerce <span class="hlt">trade</span> on 10 major online auction sites (including eBay) of approximately three-fifths of the world's spermatophyte flora. Many recognized invasive plant species (>500 species) (i.e., species associated with ecological or socio-economic problems) were <span class="hlt">traded</span> daily worldwide on the internet. A markedly higher proportion of invasive than non-invasive species were available online. Typically, for a particular plant family, 30-80% of recognized invasive species were detected on an auction site, but only a few percentages of all species in the plant family were detected on a site. Families that were more <span class="hlt">traded</span> had a higher proportion of invasive species than families that were less <span class="hlt">traded</span>. For woody species, there was a significant positive relationship between the number of <span class="hlt">regions</span> where a species was sold and the number of <span class="hlt">regions</span> where it was invasive. Our results indicate that biosecurity is not effectively regulating online plant <span class="hlt">trade</span>. In the future, automated monitoring of e-commerce may help prevent the spread of invasive species, provide information on emerging <span class="hlt">trade</span> connectivity across national borders, and be used in horizon scanning exercises for early detection of new species and their geographic source areas in international <span class="hlt">trade</span>. © 2015 Society for</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..17.6008S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..17.6008S"><span>An attempt to quantify aerosol-cloud effects in fields of precipitating <span class="hlt">trade</span> <span class="hlt">wind</span> cumuli</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Seifert, Axel; Heus, Thijs</p> <p>2015-04-01</p> <p>Aerosol indirect effects are notoriously difficult to understand and quantify. Using large-eddy simulations (LES) we attempt to quantify the impact of aerosols on the albedo and the precipitation formation in <span class="hlt">trade</span> <span class="hlt">wind</span> cumulus clouds. Having performed a set of large-domain Giga-LES runs we are able to capture the mesoscale self-organization of the cloud field. Our simulations show that self-organization is intrinsically tied to precipitation formation in this cloud regime making previous studies that did not consider cloud organization questionable. We find that aerosols, here modeled just as a perturbation in cloud droplet number concentration, have a significant impact on the transient behavior, i.e., how fast rain is formed and self-organization of the cloud field takes place. Though, for longer integration times, all simulations approach the same radiative-convective equilibrium and aerosol effects become small. The sensitivity to aerosols becomes even smaller when we include explicit cloud-radiation interaction as this leads to a much faster and more vigorous response of the cloud layer. Overall we find that aerosol-cloud interactions, like cloud lifetime effects etc., are small or even negative when the cloud field is close to equilibrium. Consequently, the Twomey effect does already provide an upper bound on the albedo effects of aerosol perturbations. Our analysis also highlights that current parameterizations that predict only the grid-box mean of the cloud field and do not take into account cloud organization are not able to describe aerosol indirect effects correctly, but overestimate them due to that lack of cloud dynamical and mesoscale buffering.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920041687&hterms=Bedini&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBedini','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920041687&hterms=Bedini&qs=N%3D0%26Ntk%3DAll%26Ntx%3Dmode%2Bmatchall%26Ntt%3DBedini"><span>The Solar <span class="hlt">Wind</span> Ion Composition Spectrometer</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Gloeckler, G.; Geiss, J.; Balsiger, H.; Bedini, P.; Cain, J. C.; Fisher, J.; Fisk, L. A.; Galvin, A. B.; Gliem, F.; Hamilton, D. C.</p> <p>1992-01-01</p> <p>The Solar <span class="hlt">Wind</span> Ion Composition Spectrometer (SWICS) on Ulysses is designed to determine uniquely the elemental and ionic-charge composition, and the temperatures and mean speeds of all major solar-<span class="hlt">wind</span> ions, from H through Fe, at solar <span class="hlt">wind</span> speeds ranging from 175 km/s (protons) to 1280 km/s (Fe(8+)). The instrument, which covers an energy per charge range from 0.16 to 59.6 keV/e in about 13 min, combines an electrostatic analyzer with postacceleration, followed by a time-of-flight and energy measurement. The measurements made by SWICS will have an impact on many areas of solar and heliospheric physics, in particular providing essential and unique information on: (1) conditions and processes in the <span class="hlt">region</span> of the corona where the solar <span class="hlt">wind</span> is accelerated; (2) the location of the source <span class="hlt">regions</span> of the solar <span class="hlt">wind</span> in the corona; (3) coronal heating processes; (4) the extent and causes of variations in the composition of the solar atmosphere; (5) plasma processes in the solar <span class="hlt">wind</span>; (6) the acceleration of energetic particles in the solar <span class="hlt">wind</span>; (7) the thermalization and acceleration of interstellar ions in the solar <span class="hlt">wind</span>, and their composition; and (8) the composition, charge states, and behavior of the plasma in various <span class="hlt">regions</span> of the Jovian magnetosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2007JGRA..112.8104O','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2007JGRA..112.8104O"><span>Solar <span class="hlt">wind</span> structure suggested by bimodal correlations of solar <span class="hlt">wind</span> speed and density between the spacecraft SOHO and <span class="hlt">Wind</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ogilvie, K. W.; Coplan, M. A.; Roberts, D. A.; Ipavich, F.</p> <p>2007-08-01</p> <p>We calculate the cross-spacecraft maximum lagged-cross-correlation coefficients for 2-hour intervals of solar <span class="hlt">wind</span> speed and density measurements made by the plasma instruments on the Solar and Heliospheric Observatory (SOHO) and <span class="hlt">Wind</span> spacecraft over the period from 1996, the minimum of solar cycle 23, through the end of 2005. During this period, SOHO was located at L1, about 200 R E upstream from the Earth, while <span class="hlt">Wind</span> spent most of the time in the interplanetary medium at distances of more than 100 R E from the Earth. Yearly histograms of the maximum, time-lagged correlation coefficients for both the speed and density are bimodal in shape, suggesting the existence of two distinct solar <span class="hlt">wind</span> regimes. The larger correlation coefficients we suggest are due to structured solar <span class="hlt">wind</span>, including discontinuities and shocks, while the smaller are likely due to Alfvénic turbulence. While further work will be required to firmly establish the physical nature of the two populations, the results of the analysis are consistent with a solar <span class="hlt">wind</span> that consists of turbulence from quiet <span class="hlt">regions</span> of the Sun interspersed with highly filamentary structures largely convected from <span class="hlt">regions</span> in the inner solar corona. The bimodal appearance of the distributions is less evident in the solar <span class="hlt">wind</span> speed than in the density correlations, consistent with the observation that the filamentary structures are convected with nearly constant speed by the time they reach 1 AU. We also find that at solar minimum the fits for the density correlations have smaller high-correlation components than at solar maximum. We interpret this as due to the presence of more relatively uniform Alfvénic <span class="hlt">regions</span> at solar minimum than at solar maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010JGRE..115.8005E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010JGRE..115.8005E"><span>Dune field pattern formation and recent transporting <span class="hlt">winds</span> in the Olympia Undae Dune Field, north polar <span class="hlt">region</span> of Mars</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ewing, Ryan C.; Peyret, Aymeric-Pierre B.; Kocurek, Gary; Bourke, Mary</p> <p>2010-08-01</p> <p>High-Resolution Imaging Science Experiment (HiRISE) imagery of the central Olympia Undae Dune Field in the north polar <span class="hlt">region</span> of Mars shows a reticulate dune pattern consisting of two sets of nearly orthogonal dune crestlines, with apparent slipfaces on the primary crests, ubiquitous <span class="hlt">wind</span> ripples, areas of coarse-grained <span class="hlt">wind</span> ripples, and deflated interdune areas. Geomorphic evidence and dune field pattern analysis of dune crest length, spacing, defect density, and orientation indicates that the pattern is complex, representing two constructional generations of dunes. The oldest and best-organized generation forms the primary crestlines and is transverse to circumpolar easterly <span class="hlt">winds</span>. Gross bed form-normal analysis of the younger pattern of crestlines indicates that it emerged with both circumpolar easterly <span class="hlt">winds</span> and NE <span class="hlt">winds</span> and is reworking the older pattern. Mapping of secondary flow fields over the dunes indicates that the most recent transporting <span class="hlt">winds</span> were from the NE. The younger pattern appears to represent an influx of sediment to the dune field associated with the development of the Olympia Cavi reentrant, with NE katabatic <span class="hlt">winds</span> channeling through the reentrant. A model of the pattern reformation based upon the reconstructed primary <span class="hlt">winds</span> and resulting secondary flow fields shows that the development of the secondary pattern is controlled by the boundary condition of the older dune topography.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017EGUGA..1915352R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017EGUGA..1915352R"><span>Wave-Current Interactions in a <span class="hlt">wind</span>-jet <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ràfols, Laura; Grifoll, Manel; Espino, Manuel; Cerralbo, Pablo; Sairouní, Abdel; Bravo, Manel; Sánchez-Arcilla, Agustín</p> <p>2017-04-01</p> <p>The Wave-Current Interactions (WCI) are investigated examining the influences of coupling two numerical models. The <span class="hlt">Regional</span> Ocean Model System (ROMS; Shchepetkin and McWilliams, 2005) and the Simulating Waves Nearshore (SWAN; Booij et al. 1999) are used in a high resolution domain (350 m). For the initial and boundary conditions, data from the IBI-MFC products have been used and the atmospheric forcing fields have been obtained from the Catalan Meteorological Service (SMC). Results from uncoupled numerical models are compared with one-way and two-way coupling simulations. The study area is located at the northern margin of the Ebro Shelf (NW Mediterranean Sea), where episodes of strong cross-shelf <span class="hlt">wind</span> occur. The results show that during these episodes, the water currents obtained in the two-way simulation have better agreement with the observations compared with the other simulations. Additionally, when the water currents are considered, the wave energy (and thus the significant wave heigh) decrease when the current flows in the same direction as waves propagate. The relative importance of the different terms of the momentum balance equation is also analyzed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFM.A13G0305V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFM.A13G0305V"><span>Could Crop Height Impact the <span class="hlt">Wind</span> Resource at Agriculturally Productive <span class="hlt">Wind</span> Farm Sites?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vanderwende, B. J.; Lundquist, J. K.</p> <p>2013-12-01</p> <p>The agriculture-intensive United States Midwest and Great Plains <span class="hlt">regions</span> feature some of the best <span class="hlt">wind</span> resources in the nation. Collocation of cropland and <span class="hlt">wind</span> turbines introduces complex meteorological interactions that could affect both agriculture and <span class="hlt">wind</span> power production. Crop management practices may modify the <span class="hlt">wind</span> resource through alterations of land-surface properties. In this study, we used the Weather Research and Forecasting (WRF) model to estimate the impact of crop height variations on the <span class="hlt">wind</span> resource in the presence of a large turbine array. We parameterized a hypothetical array of 121 1.8 MW turbines at the site of the 2011 Crop/<span class="hlt">Wind</span>-energy Experiment field campaign using the WRF <span class="hlt">wind</span> farm parameterization. We estimated the impact of crop choices on power production by altering the aerodynamic roughness length in a <span class="hlt">region</span> approximately 65 times larger than that occupied by the turbine array. Roughness lengths of 10 cm and 25 cm represent a mature soy crop and a mature corn crop respectively. Results suggest that the presence of the mature corn crop reduces hub-height <span class="hlt">wind</span> speeds and increases rotor-layer <span class="hlt">wind</span> shear, even in the presence of a large <span class="hlt">wind</span> farm which itself modifies the flow. During the night, the influence of the surface was dependent on the boundary layer stability, with strong stability inhibiting the surface drag from modifying the <span class="hlt">wind</span> resource aloft. Further investigation is required to determine the optimal size, shape, and crop height of the roughness modification to maximize the economic benefit and minimize the cost of such crop management practices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19920040726&hterms=astronomia&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dastronomia','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19920040726&hterms=astronomia&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Dastronomia"><span><span class="hlt">Winds</span> from T Tauri stars. II - Balmer line profiles for inner disk <span class="hlt">winds</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Calvet, Nuria; Hartmann, Lee; Hewett, Robert</p> <p>1992-01-01</p> <p>Results are presented of calculations of Balmer emission line profiles using escape probability methods for T Tauri <span class="hlt">wind</span> models with nonspherically symmetric geometry. The <span class="hlt">wind</span> is assumed to originate in the inner <span class="hlt">regions</span> of an accretion disk surrounding the T Tauri star, and flows outward in a 'cone' geometry. Two types of <span class="hlt">wind</span> models are considered, both with monotonically increasing expansion velocities as a function of radial distance. For flows with large turbulent velocities, such as the HF Alfven wave-driven <span class="hlt">wind</span> models, the effect of cone geometry is to increase the blue wing emission, and to move the absorption reversal close to line center. Line profiles for a <span class="hlt">wind</span> model rotating with the same angular velocity as the inner disk are also calculated. The Balmer lines of this model are significantly broader than observed in most objects, suggesting that the observed emission lines do not arise in a <span class="hlt">region</span> rotating at Keplerian velocity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ERL....11c5008G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ERL....11c5008G"><span>Vulnerability to shocks in the global seafood <span class="hlt">trade</span> network</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gephart, Jessica A.; Rovenskaya, Elena; Dieckmann, Ulf; Pace, Michael L.; Brännström, Åke</p> <p>2016-03-01</p> <p><span class="hlt">Trade</span> can allow countries to overcome local or <span class="hlt">regional</span> losses (shocks) to their food supply, but reliance on international food <span class="hlt">trade</span> also exposes countries to risks from external perturbations. Countries that are nutritionally or economically dependent on international <span class="hlt">trade</span> of a commodity may be adversely affected by such shocks. While exposure to shocks has been studied in financial markets, communication networks, and some infrastructure systems, it has received less attention in food-<span class="hlt">trade</span> networks. Here, we develop a forward shock-propagation model to quantify how <span class="hlt">trade</span> flows are redistributed under a range of shock scenarios and assess the food-security outcomes by comparing changes in national fish supplies to indices of each country’s nutritional fish dependency. Shock propagation and distribution among <span class="hlt">regions</span> are modeled on a network of historical bilateral seafood <span class="hlt">trade</span> data from UN Comtrade using 205 reporting territories grouped into 18 <span class="hlt">regions</span>. In our model exposure to shocks increases with total imports and the number of import partners. We find that Central and West Africa are the most vulnerable to shocks, with their vulnerability increasing when a willingness-to-pay proxy is included. These findings suggest that countries can reduce their overall vulnerability to shocks by reducing reliance on imports and diversifying food sources. As international seafood <span class="hlt">trade</span> grows, identifying these types of potential risks and vulnerabilities is important to build a more resilient food system.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3776385','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3776385"><span><span class="hlt">Wind</span> Tunnel Tests for <span class="hlt">Wind</span> Pressure Distribution on Gable Roof Buildings</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>2013-01-01</p> <p>Gable roof buildings are widely used in industrial buildings. Based on <span class="hlt">wind</span> tunnel tests with rigid models, <span class="hlt">wind</span> pressure distributions on gable roof buildings with different aspect ratios were measured simultaneously. Some characteristics of the measured <span class="hlt">wind</span> pressure field on the surfaces of the models were analyzed, including mean <span class="hlt">wind</span> pressure, fluctuating <span class="hlt">wind</span> pressure, peak negative <span class="hlt">wind</span> pressure, and characteristics of proper orthogonal decomposition results of the measured <span class="hlt">wind</span> pressure field. The results show that extremely high local suctions often occur in the leading edges of longitudinal wall and windward roof, roof corner, and roof ridge which are the severe damaged locations under strong <span class="hlt">wind</span>. The aspect ratio of building has a certain effect on the mean <span class="hlt">wind</span> pressure coefficients, and the effect relates to <span class="hlt">wind</span> attack angle. Compared with experimental results, the <span class="hlt">region</span> division of roof corner and roof ridge from AIJ2004 is more reasonable than those from CECS102:2002 and MBMA2006.The contributions of the first several eigenvectors to the overall <span class="hlt">wind</span> pressure distributions become much bigger. The investigation can offer some basic understanding for estimating <span class="hlt">wind</span> load distribution on gable roof buildings and facilitate <span class="hlt">wind</span>-resistant design of cladding components and their connections considering <span class="hlt">wind</span> load path. PMID:24082851</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24082851','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24082851"><span><span class="hlt">Wind</span> tunnel tests for <span class="hlt">wind</span> pressure distribution on gable roof buildings.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jing, Xiao-kun; Li, Yuan-qi</p> <p>2013-01-01</p> <p>Gable roof buildings are widely used in industrial buildings. Based on <span class="hlt">wind</span> tunnel tests with rigid models, <span class="hlt">wind</span> pressure distributions on gable roof buildings with different aspect ratios were measured simultaneously. Some characteristics of the measured <span class="hlt">wind</span> pressure field on the surfaces of the models were analyzed, including mean <span class="hlt">wind</span> pressure, fluctuating <span class="hlt">wind</span> pressure, peak negative <span class="hlt">wind</span> pressure, and characteristics of proper orthogonal decomposition results of the measured <span class="hlt">wind</span> pressure field. The results show that extremely high local suctions often occur in the leading edges of longitudinal wall and windward roof, roof corner, and roof ridge which are the severe damaged locations under strong <span class="hlt">wind</span>. The aspect ratio of building has a certain effect on the mean <span class="hlt">wind</span> pressure coefficients, and the effect relates to <span class="hlt">wind</span> attack angle. Compared with experimental results, the <span class="hlt">region</span> division of roof corner and roof ridge from AIJ2004 is more reasonable than those from CECS102:2002 and MBMA2006.The contributions of the first several eigenvectors to the overall <span class="hlt">wind</span> pressure distributions become much bigger. The investigation can offer some basic understanding for estimating <span class="hlt">wind</span> load distribution on gable roof buildings and facilitate <span class="hlt">wind</span>-resistant design of cladding components and their connections considering <span class="hlt">wind</span> load path.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012NatCC...2..539Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012NatCC...2..539Z"><span>Impacts of <span class="hlt">wind</span> farms on land surface temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, Liming; Tian, Yuhong; Baidya Roy, Somnath; Thorncroft, Chris; Bosart, Lance F.; Hu, Yuanlong</p> <p>2012-07-01</p> <p>The <span class="hlt">wind</span> industry in the United States has experienced a remarkably rapid expansion of capacity in recent years and this fast growth is expected to continue in the future. While converting <span class="hlt">wind</span>'s kinetic energy into electricity, <span class="hlt">wind</span> turbines modify surface-atmosphere exchanges and the transfer of energy, momentum, mass and moisture within the atmosphere. These changes, if spatially large enough, may have noticeable impacts on local to <span class="hlt">regional</span> weather and climate. Here we present observational evidence for such impacts based on analyses of satellite data for the period of 2003-2011 over a <span class="hlt">region</span> in west-central Texas, where four of the world's largest <span class="hlt">wind</span> farms are located. Our results show a significant warming trend of up to 0.72°C per decade, particularly at night-time, over <span class="hlt">wind</span> farms relative to nearby non-<span class="hlt">wind</span>-farm <span class="hlt">regions</span>. We attribute this warming primarily to <span class="hlt">wind</span> farms as its spatial pattern and magnitude couples very well with the geographic distribution of <span class="hlt">wind</span> turbines.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_13");'>13</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li class="active"><span>15</span></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_15 --> <div id="page_16" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="301"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1375460','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1375460"><span><span class="hlt">WIND</span> Toolkit Offshore Summary Dataset</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>Draxl, Caroline; Musial, Walt; Scott, George</p> <p></p> <p>This dataset contains summary statistics for offshore <span class="hlt">wind</span> resources for the continental United States derived from the <span class="hlt">Wind</span> Integration National Datatset (<span class="hlt">WIND</span>) Toolkit. These data are available in two formats: GDB - Compressed geodatabases containing statistical summaries aligned with lease blocks (aliquots) stored in a GIS format. These data are partitioned into Pacific, Atlantic, and Gulf resource <span class="hlt">regions</span>. HDF5 - Statistical summaries of all points in the offshore Pacific, Atlantic, and Gulf offshore <span class="hlt">regions</span>. These data are located on the original <span class="hlt">WIND</span> Toolkit grid and have not been reassigned or downsampled to lease blocks. These data were developed under contractmore » by NREL for the Bureau of Oceanic Energy Management (BOEM).« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28768893','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28768893"><span>Performance <span class="hlt">trade</span>-offs and ageing in the 'world's greatest athletes'.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Careau, Vincent; Wilson, Robbie S</p> <p>2017-08-16</p> <p>The mechanistic foundations of performance <span class="hlt">trade</span>-offs are clear: because body size and shape constrains movement, and muscles vary in strength and fibre type, certain physical traits should act in opposition with others (e.g. sprint versus endurance). Yet performance <span class="hlt">trade</span>-offs are rarely detected, and traits are often positively correlated. A potential resolution to this conundrum is that within -individual performance <span class="hlt">trade</span>-offs can be masked by among -individual variation in 'quality'. Although there is a current debate on how to unambiguously define and account for quality, no previous studies have partitioned trait correlations at the within- and among-individual levels. Here, we evaluate performance <span class="hlt">trade</span>-offs among and within 1369 elite athletes that performed in a total of 6418 combined-events competitions (decathlon and heptathlon). Controlling for age, experience and <span class="hlt">wind</span> conditions, we detected strong <span class="hlt">trade</span>-offs between groups of functionally similar events (throwing versus jumping versus running) occurring at the among-individual level. We further modelled individual (co)variation in age-related plasticity of performance and found previously unseen <span class="hlt">trade</span>-offs in throwing versus running performance that manifest through ageing. Our results verify that human performance is limited by fundamental genetic, environmental and ageing constraints that preclude the simultaneous improvement of performance in multiple dimensions. Identifying these constraints is fundamental to understanding performance <span class="hlt">trade</span>-offs and predicting the ageing of motor function. © 2017 The Author(s).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008GeoRL..35.9804L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008GeoRL..35.9804L"><span>Surface <span class="hlt">wind</span> accuracy for modeling mineral dust emissions: Comparing two <span class="hlt">regional</span> models in a Bodélé case study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Laurent, B.; Heinold, B.; Tegen, I.; Bouet, C.; Cautenet, G.</p> <p>2008-05-01</p> <p>After a decade of research on improving the description of surface and soil features in desert <span class="hlt">regions</span> to accurately model mineral dust emissions, we now emphasize the need for deeper evaluating the accuracy of modeled 10-m surface <span class="hlt">wind</span> speeds U 10 . Two mesoscale models, the Lokal-Modell (LM) and the <span class="hlt">Regional</span> Atmospheric Modeling System (RAMS), coupled with an explicit dust emission model have previously been used to simulate mineral dust events in the Bodélé <span class="hlt">region</span>. We compare LM and RAMS U 10 , together with measurements at the Chicha site (BoDEx campaign) and Faya-Largeau meteorological station. Surface features and soil schemes are investigated to correctly simulate U 10 intensity and diurnal variability. The uncertainties in dust emissions computed with LM and RAMS U 10 and different soil databases are estimated. This sensitivity study shows the importance of accurate computation of surface <span class="hlt">winds</span> to improve the quantification of <span class="hlt">regional</span> dust emissions from the Bodélé</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011PhyA..390..398W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011PhyA..390..398W"><span>Characteristics of real futures <span class="hlt">trading</span> networks</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Wang, Junjie; Zhou, Shuigeng; Guan, Jihong</p> <p>2011-01-01</p> <p>Futures <span class="hlt">trading</span> is the core of futures business, and it is considered as one of the typical complex systems. To investigate the complexity of futures <span class="hlt">trading</span>, we employ the analytical method of complex networks. First, we use real <span class="hlt">trading</span> records from the Shanghai Futures Exchange to construct futures <span class="hlt">trading</span> networks, in which nodes are <span class="hlt">trading</span> participants, and two nodes have a common edge if the two corresponding investors appear simultaneously in at least one <span class="hlt">trading</span> record as a purchaser and a seller, respectively. Then, we conduct a comprehensive statistical analysis on the constructed futures <span class="hlt">trading</span> networks. Empirical results show that the futures <span class="hlt">trading</span> networks exhibit features such as scale-free behavior with interesting odd-even-degree divergence in low-degree <span class="hlt">regions</span>, small-world effect, hierarchical organization, power-law betweenness distribution, disassortative mixing, and shrinkage of both the average path length and the diameter as network size increases. To the best of our knowledge, this is the first work that uses real data to study futures <span class="hlt">trading</span> networks, and we argue that the research results can shed light on the nature of real futures business.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19840005036','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19840005036"><span>Solar <span class="hlt">wind</span> disturbances in th outer heliosphere caused by successive solar flares from the same active <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Akasofu, S. I.; Hakamada, K.</p> <p>1983-01-01</p> <p>Solar <span class="hlt">wind</span> disturbances caused by successive flares from the same active <span class="hlt">region</span> are traced to about 20 AU, using the modeling method developed by Hakamada and Akasofu (1982). It is shown that the flare-generated shock waves coalesce with the co-rotating interaction <span class="hlt">region</span> of the interplanetary magnetic field, resulting in a large-scale magnetic field structure in the outer heliosphere. Such a structure may have considerable effects on the propagation of galactic cosmic rays.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016ApJ...829..117S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016ApJ...829..117S"><span>On Solar <span class="hlt">Wind</span> Origin and Acceleration: Measurements from ACE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Stakhiv, Mark; Lepri, Susan T.; Landi, Enrico; Tracy, Patrick; Zurbuchen, Thomas H.</p> <p>2016-10-01</p> <p>The origin and acceleration of the solar <span class="hlt">wind</span> are still debated. In this paper, we search for signatures of the source <span class="hlt">region</span> and acceleration mechanism of the solar <span class="hlt">wind</span> in the plasma properties measured in situ by the Advanced Composition Explorer spacecraft. Using the elemental abundances as a proxy for the source <span class="hlt">region</span> and the differential velocity and ion temperature ratios as a proxy for the acceleration mechanism, we are able to identify signatures pointing toward possible source <span class="hlt">regions</span> and acceleration mechanisms. We find that the fast solar <span class="hlt">wind</span> in the ecliptic plane is the same as that observed from the polar <span class="hlt">regions</span> and is consistent with wave acceleration and coronal-hole origin. We also find that the slow <span class="hlt">wind</span> is composed of two components: one similar to the fast solar <span class="hlt">wind</span> (with slower velocity) and the other likely originating from closed magnetic loops. Both components of the slow solar <span class="hlt">wind</span> show signatures of wave acceleration. From these findings, we draw a scenario that envisions two types of <span class="hlt">wind</span>, with different source <span class="hlt">regions</span> and release mechanisms, but the same wave acceleration mechanism.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20080017203','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20080017203"><span>Expected Characteristics of Global <span class="hlt">Wind</span> Profile Measurements with a Scanning, Hybrid, Doppler Lidar System</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kavaya, Michael J.</p> <p>2008-01-01</p> <p>Over 20 years of investigation by NASA and NOAA scientists and Doppler lidar technologists into a global <span class="hlt">wind</span> profiling mission from earth orbit have led to the current favored concept of an instrument with both coherent- and direct-detection pulsed Doppler lidars (i.e., a hybrid Doppler lidar) and a stepstare beam scanning approach covering several azimuth angles with a fixed nadir angle. The nominal lidar wavelengths are 2 microns for coherent detection, and 0.355 microns for direct detection. The two agencies have also generated two sets of sophisticated <span class="hlt">wind</span> measurement requirements for a space mission: science demonstration requirements and operational requirements. The requirements contain the necessary details to permit mission design and optimization by lidar technologists. Simulations have been developed that connect the science requirements to the <span class="hlt">wind</span> measurement requirements, and that connect the <span class="hlt">wind</span> measurement requirements to the Doppler lidar parameters. The simulations also permit <span class="hlt">trade</span> studies within the multi-parameter space. These tools, combined with knowledge of the state of the Doppler lidar technology, have been used to conduct space instrument and mission design activities to validate the feasibility of the chosen mission and lidar parameters. Recently, the NRC Earth Science Decadal Survey recommended the <span class="hlt">wind</span> mission to NASA as one of 15 recommended missions. A full description of the <span class="hlt">wind</span> measurement product from these notional missions and the possible <span class="hlt">trades</span> available are presented in this paper.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016BoLMe.158..409V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016BoLMe.158..409V"><span>Could Crop Height Affect the <span class="hlt">Wind</span> Resource at Agriculturally Productive <span class="hlt">Wind</span> Farm Sites?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Vanderwende, Brian; Lundquist, Julie K.</p> <p>2016-03-01</p> <p>The collocation of cropland and <span class="hlt">wind</span> turbines in the US Midwest <span class="hlt">region</span> introduces complex meteorological interactions that could influence both agriculture and <span class="hlt">wind</span>-power production. Crop management practices may affect the <span class="hlt">wind</span> resource through alterations of land-surface properties. We use the weather research and forecasting (WRF) model to estimate the impact of crop height variations on the <span class="hlt">wind</span> resource in the presence of a large turbine array. A hypothetical <span class="hlt">wind</span> farm consisting of 121 1.8-MW turbines is represented using the WRF model <span class="hlt">wind</span>-farm parametrization. We represent the impact of selecting soybeans rather than maize by altering the aerodynamic roughness length in a <span class="hlt">region</span> approximately 65 times larger than that occupied by the turbine array. Roughness lengths of 0.1 and 0.25 m represent the mature soy crop and a mature maize crop, respectively. In all but the most stable atmospheric conditions, statistically significant hub-height <span class="hlt">wind</span>-speed increases and rotor-layer <span class="hlt">wind</span>-shear reductions result from switching from maize to soybeans. Based on simulations for the entire month of August 2013, <span class="hlt">wind</span>-farm energy output increases by 14 %, which would yield a significant monetary gain. Further investigation is required to determine the optimal size, shape, and crop height of the roughness modification to maximize the economic benefit and minimize the cost of such crop-management practices. These considerations must be balanced by other influences on crop choice such as soil requirements and commodity prices.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/pages/biblio/1240086-could-crop-height-affect-wind-resource-agriculturally-productive-wind-farm-sites','SCIGOV-DOEP'); return false;" href="https://www.osti.gov/pages/biblio/1240086-could-crop-height-affect-wind-resource-agriculturally-productive-wind-farm-sites"><span>Could crop height affect the <span class="hlt">wind</span> resource at agriculturally productive <span class="hlt">wind</span> farm sites?</span></a></p> <p><a target="_blank" href="http://www.osti.gov/pages">DOE PAGES</a></p> <p>Vanderwende, Brian; Lundquist, Julie K.</p> <p>2015-11-07</p> <p>The collocation of cropland and <span class="hlt">wind</span> turbines in the US Midwest <span class="hlt">region</span> introduces complex meteorological interactions that could influence both agriculture and <span class="hlt">wind</span>-power production. Crop management practices may affect the <span class="hlt">wind</span> resource through alterations of land-surface properties. We use the weather research and forecasting (WRF) model to estimate the impact of crop height variations on the <span class="hlt">wind</span> resource in the presence of a large turbine array. A hypothetical <span class="hlt">wind</span> farm consisting of 121 1.8-MW turbines is represented using the WRF model <span class="hlt">wind</span>-farm parametrization. We represent the impact of selecting soybeans rather than maize by altering the aerodynamic roughness length inmore » a <span class="hlt">region</span> approximately 65 times larger than that occupied by the turbine array. Roughness lengths of 0.1 and 0.25 m represent the mature soy crop and a mature maize crop, respectively. In all but the most stable atmospheric conditions, statistically significant hub-height <span class="hlt">wind</span>-speed increases and rotor-layer <span class="hlt">wind</span>-shear reductions result from switching from maize to soybeans. Based on simulations for the entire month of August 2013, <span class="hlt">wind</span>-farm energy output increases by 14 %, which would yield a significant monetary gain. Further investigation is required to determine the optimal size, shape, and crop height of the roughness modification to maximize the economic benefit and minimize the cost of such crop-management practices. As a result, these considerations must be balanced by other influences on crop choice such as soil requirements and commodity prices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1240086','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1240086"><span>Could crop height affect the <span class="hlt">wind</span> resource at agriculturally productive <span class="hlt">wind</span> farm sites?</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>Vanderwende, Brian; Lundquist, Julie K.</p> <p></p> <p>The collocation of cropland and <span class="hlt">wind</span> turbines in the US Midwest <span class="hlt">region</span> introduces complex meteorological interactions that could influence both agriculture and <span class="hlt">wind</span>-power production. Crop management practices may affect the <span class="hlt">wind</span> resource through alterations of land-surface properties. We use the weather research and forecasting (WRF) model to estimate the impact of crop height variations on the <span class="hlt">wind</span> resource in the presence of a large turbine array. A hypothetical <span class="hlt">wind</span> farm consisting of 121 1.8-MW turbines is represented using the WRF model <span class="hlt">wind</span>-farm parametrization. We represent the impact of selecting soybeans rather than maize by altering the aerodynamic roughness length inmore » a <span class="hlt">region</span> approximately 65 times larger than that occupied by the turbine array. Roughness lengths of 0.1 and 0.25 m represent the mature soy crop and a mature maize crop, respectively. In all but the most stable atmospheric conditions, statistically significant hub-height <span class="hlt">wind</span>-speed increases and rotor-layer <span class="hlt">wind</span>-shear reductions result from switching from maize to soybeans. Based on simulations for the entire month of August 2013, <span class="hlt">wind</span>-farm energy output increases by 14 %, which would yield a significant monetary gain. Further investigation is required to determine the optimal size, shape, and crop height of the roughness modification to maximize the economic benefit and minimize the cost of such crop-management practices. As a result, these considerations must be balanced by other influences on crop choice such as soil requirements and commodity prices.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950015967','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950015967"><span>Solar <span class="hlt">wind</span> composition</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Ogilvie, K. W.; Coplan, M. A.</p> <p>1995-01-01</p> <p>Advances in instrumentation have resulted in the determination of the average abundances of He, C, N, O, Ne, Mg, Si, S, and Fe in the solar <span class="hlt">wind</span> to approximately 10%. Comparisons with solar energetic particle (SEP) abundances and galactic cosmic ray abundances have revealed many similarities, especially when compared with solar photospheric abundances. It is now well established that fractionation in the corona results in an overabundance (with respect to the photosphere) of elements with first ionization potentials less than 10 eV. These observations have in turn led to the development of fractionation models that are reasonably successful in reproducing the first ionization (FIP) effect. Under some circumstances it has been possible to relate solar <span class="hlt">wind</span> observations to particular source <span class="hlt">regions</span> in the corona. The magnetic topologies of the source <span class="hlt">regions</span> appear to have a strong influence on the fractionation of elements. Comparisons with spectroscopic data are particularly useful in classifying the different topologies. Ions produced from interstellar neutral atoms are also found in the solar <span class="hlt">wind</span>. These ions are picked up by the solar <span class="hlt">wind</span> after ionization by solar radiation or charge exchange and can be identified by their velocity in the solar <span class="hlt">wind</span>. The pick-up ions provide most of the pressure in the interplanetary medium at large distances. Interstellar abundances can be derived from the observed fluxes of solar <span class="hlt">wind</span> pick-up ions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014AGUFMSH33A4129L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014AGUFMSH33A4129L"><span>Solar Corona/<span class="hlt">Wind</span> Composition and Origins of the Solar <span class="hlt">Wind</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lepri, S. T.; Gilbert, J. A.; Landi, E.; Shearer, P.; von Steiger, R.; Zurbuchen, T.</p> <p>2014-12-01</p> <p>Measurements from ACE and Ulysses have revealed a multifaceted solar <span class="hlt">wind</span>, with distinctly different kinetic and compositional properties dependent on the source <span class="hlt">region</span> of the <span class="hlt">wind</span>. One of the major outstanding issues in heliophysics concerns the origin and also predictability of quasi-stationary slow solar <span class="hlt">wind</span>. While the fast solar <span class="hlt">wind</span> is now proven to originate within large polar coronal holes, the source of the slow solar <span class="hlt">wind</span> remains particularly elusive and has been the subject of long debate, leading to models that are stationary and also reconnection based - such as interchange or so-called S-web based models. Our talk will focus on observational constraints of solar <span class="hlt">wind</span> sources and their evolution during the solar cycle. In particular, we will point out long-term variations of <span class="hlt">wind</span> composition and dynamic properties, particularly focused on the abundance of elements with low First Ionization Potential (FIP), which have been routinely measured on both ACE and Ulysses spacecraft. We will use these in situ observations, and remote sensing data where available, to provide constraints for solar <span class="hlt">wind</span> origin during the solar cycle, and on their correspondence to predictions for models of the solar <span class="hlt">wind</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ClDy..tmp...37R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ClDy..tmp...37R"><span>Comparison of different <span class="hlt">wind</span> data interpolation methods for a <span class="hlt">region</span> with complex terrain in Central Asia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Reinhardt, Katja; Samimi, Cyrus</p> <p>2018-01-01</p> <p>While climatological data of high spatial resolution are largely available in most developed countries, the network of climatological stations in many other <span class="hlt">regions</span> of the world still constitutes large gaps. Especially for those <span class="hlt">regions</span>, interpolation methods are important tools to fill these gaps and to improve the data base indispensible for climatological research. Over the last years, new hybrid methods of machine learning and geostatistics have been developed which provide innovative prospects in spatial predictive modelling. This study will focus on evaluating the performance of 12 different interpolation methods for the <span class="hlt">wind</span> components \\overrightarrow{u} and \\overrightarrow{v} in a mountainous <span class="hlt">region</span> of Central Asia. Thereby, a special focus will be on applying new hybrid methods on spatial interpolation of <span class="hlt">wind</span> data. This study is the first evaluating and comparing the performance of several of these hybrid methods. The overall aim of this study is to determine whether an optimal interpolation method exists, which can equally be applied for all pressure levels, or whether different interpolation methods have to be used for the different pressure levels. Deterministic (inverse distance weighting) and geostatistical interpolation methods (ordinary kriging) were explored, which take into account only the initial values of \\overrightarrow{u} and \\overrightarrow{v} . In addition, more complex methods (generalized additive model, support vector machine and neural networks as single methods and as hybrid methods as well as regression-kriging) that consider additional variables were applied. The analysis of the error indices revealed that regression-kriging provided the most accurate interpolation results for both <span class="hlt">wind</span> components and all pressure heights. At 200 and 500 hPa, regression-kriging is followed by the different kinds of neural networks and support vector machines and for 850 hPa it is followed by the different types of support vector machine and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MNRAS.466.1857G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MNRAS.466.1857G"><span>IRAS 18153-1651: an H II <span class="hlt">region</span> with a possible <span class="hlt">wind</span> bubble blown by a young main-sequence B star</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gvaramadze, V. V.; Mackey, J.; Kniazev, A. Y.; Langer, N.; Chené, A.-N.; Castro, N.; Haworth, T. J.; Grebel, E. K.</p> <p>2017-04-01</p> <p>We report the results of spectroscopic observations and numerical modelling of the H II <span class="hlt">region</span> IRAS 18153-1651. Our study was motivated by the discovery of an optical arc and two main-sequence stars of spectral type B1 and B3 near the centre of IRAS 18153-1651. We interpret the arc as the edge of the <span class="hlt">wind</span> bubble (blown by the B1 star), whose brightness is enhanced by the interaction with a photoevaporation flow from a nearby molecular cloud. This interpretation implies that we deal with a unique case of a young massive star (the most massive member of a recently formed low-mass star cluster) caught just tens of thousands of years after its stellar <span class="hlt">wind</span> has begun to blow a bubble into the surrounding dense medium. Our 2D, radiation-hydrodynamics simulations of the <span class="hlt">wind</span> bubble and the H II <span class="hlt">region</span> around the B1 star provide a reasonable match to observations, both in terms of morphology and absolute brightness of the optical and mid-infrared emission, and verify the young age of IRAS 18153-1651. Taken together our results strongly suggest that we have revealed the first example of a <span class="hlt">wind</span> bubble blown by a main-sequence B star.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70115060','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70115060"><span>Centennial changes in North Pacific anoxia linked to tropical <span class="hlt">trade</span> <span class="hlt">winds</span></span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Deutsch, Curtis; Berelson, William; Thunell, Robert; Weber, Thomas; Tems, Caitlin; McManus, James; Crusius, John; Ito, Taka; Baumgartner, Timothy; Ferreira, Vicente; Mey, Jacob; van Geen, Alexander</p> <p>2014-01-01</p> <p>Climate warming is expected to reduce oxygen (O2) supply to the ocean and expand its oxygen minimum zones (OMZs). We reconstructed variations in the extent of North Pacific anoxia since 1850 using a geochemical proxy for denitrification (δ15N) from multiple sediment cores. Increasing δ15N since ~1990 records an expansion of anoxia, consistent with observed O2 trends. However, this was preceded by a longer declining δ15N trend that implies that the anoxic zone was shrinking for most of the 20th century. Both periods can be explained by changes in <span class="hlt">winds</span> over the tropical Pacific that drive upwelling, biological productivity, and O2 demand within the OMZ. If equatorial Pacific <span class="hlt">winds</span> resume their predicted weakening trend, the ocean’s largest anoxic zone will contract despite a global O2 decline.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19910008039','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19910008039"><span>Laser Atmospheric <span class="hlt">Wind</span> Sounder (LAWS) phase 1. Volume 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1990-01-01</p> <p>This report summarizes and documents the results of the 12-month phase 1 work effort. The objective of phase 1 was to establish the conceptional definition of the laser atmospheric <span class="hlt">wind</span> sounder (LAWS) sensor system, including accommodations analyses to ensure compatibility with the Space Station Freedom (SSF) and the Earth Observing System (EOS) Polar Orbiting Platform (POP). Various concepts were investigated with <span class="hlt">trade</span> studies performed to select the configuration to be carried forward to the phase 2 Preliminary Design Definition. A summary of the LAWS system and subsystem <span class="hlt">trade</span> studies that were performed leading to the baseline design configuration is presented in the appendix. The overall objective of the LAWS Project is to define, design, and implement an operational space based facility, LAWS, for accurate measurement of Earth <span class="hlt">wind</span> profiles. Phase 1 addressed three major areas: (1) requirements definition; (2) instrument concepts and configurations; and (3) performance analysis. For the LAWS instrument concepts and configurations, the issues which press the technological state of the art are reliable detector lifetime and laser performance and lifetime. Lag angle compensation, pointing accuracy, satellite navigation, and telescope design are significant technical issues, but they are considered to be currently state of the art. The primary issues for performance analysis concern interaction with the atmosphere in terms of backscatter and attenuation, <span class="hlt">wind</span> variance, and cloud blockage. The phase 1 tasks were formulated to address these significant technical issues and demonstrate the technical feasibility of the LAWS concept. Primary emphasis was placed on analysis/<span class="hlt">trade</span> and identification of candidate concepts. Promising configurations were evaluated for performance, sensitivities, risks, and budgetary costs. Lockheed's baseline LAWS configuration is presented.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-09-27/pdf/2010-24064.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-09-27/pdf/2010-24064.pdf"><span>75 FR 59291 - In the Matter of: Certain <span class="hlt">Wind</span> and Solar-Powered Light Posts and Street Lamps; Notice of...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-09-27</p> <p>... INTERNATIONAL <span class="hlt">TRADE</span> COMMISSION [Inv. No. 337-TA-736] In the Matter of: Certain <span class="hlt">Wind</span> and Solar... solar-powered light posts and street lamps by reason of infringement of the claimed design of U.S... certain <span class="hlt">wind</span> and solar- [[Page 59292</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=export-import&pg=7&id=ED311247','ERIC'); return false;" href="https://eric.ed.gov/?q=export-import&pg=7&id=ED311247"><span><span class="hlt">Trading</span> Away Jobs: The Effects of the US Merchandise <span class="hlt">Trade</span> Deficit on Employment. Working Paper No. 102.</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>Duchin, Faye; Lange, Glenn-Marie</p> <p></p> <p>A study was conducted to describe the segments of the U.S. labor force that have been affected by the recent deterioration in U.S. <span class="hlt">trade</span>. The methodology involved computer modeling of the effects of eliminating the 1987 merchandise <span class="hlt">trade</span> deficit on employment by detailed industry and occupation, by geographic <span class="hlt">region</span>, and by wage group. This was…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRC..121.2231R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRC..121.2231R"><span><span class="hlt">Wind</span>-driven changes of surface current, temperature, and chlorophyll observed by satellites north of New Guinea</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Radenac, Marie-Hélène; Léger, Fabien; Messié, Monique; Dutrieux, Pierre; Menkes, Christophe; Eldin, Gérard</p> <p>2016-04-01</p> <p>Satellite observations of <span class="hlt">wind</span>, sea level and derived currents, sea surface temperature (SST), and chlorophyll are used to expand our understanding of the physical and biological variability of the ocean surface north of New Guinea. Based on scarce cruise and mooring data, previous studies differentiated a <span class="hlt">trade</span> <span class="hlt">wind</span> situation (austral winter) when the New Guinea Coastal Current (NGCC) flows northwestward and a northwest monsoon situation (austral summer) when a coastal upwelling develops and the NGCC reverses. This circulation pattern is confirmed by satellite observations, except in Vitiaz Strait where the surface northwestward flow persists. We find that intraseasonal and seasonal time scale variations explain most of the variance north of New Guinea. SST and chlorophyll variabilities are mainly driven by two processes: penetration of Solomon Sea waters and coastal upwelling. In the <span class="hlt">trade</span> <span class="hlt">wind</span> situation, the NGCC transports cold Solomon Sea waters through Vitiaz Strait in a narrow vein hugging the coast. Coastal upwelling is generated in westerly <span class="hlt">wind</span> situations (westerly <span class="hlt">wind</span> event, northwest monsoon). Highly productive coastal waters are advected toward the equator and, during some westerly <span class="hlt">wind</span> events, toward the eastern part of the warm pool. During El Niño, coastal upwelling events and northward penetration of Solomon Sea waters combine to influence SST and chlorophyll anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A21E2201B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A21E2201B"><span><span class="hlt">Regional</span> Analysis of Long-term Local and Synoptic Effects on <span class="hlt">Wind</span> Velocity and Energy Patterns in Complex Terrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Belu, R.; Koracin, D. R.</p> <p>2017-12-01</p> <p> that the <span class="hlt">regional</span> synoptic processes are dominant for <span class="hlt">wind</span> variability.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_14");'>14</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li class="active"><span>16</span></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_16 --> <div id="page_17" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="321"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A23J..11C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A23J..11C"><span>The New <span class="hlt">Wind</span>ForS <span class="hlt">Wind</span> Energy Test Site in Southern Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clifton, A. J.</p> <p>2017-12-01</p> <p><span class="hlt">Wind</span> turbines are increasingly being installed in complex terrain where patchy landcover, forestry, steep slopes, and complex <span class="hlt">regional</span> and local atmospheric conditions lead to major challenges for traditional numerical weather prediction methods. In this presentation, the new <span class="hlt">Wind</span>ForS complex terrain test site will be introduced. <span class="hlt">Wind</span>ForS is a southern Germany-based research consortium of more than 20 groups at higher education and research institutes, with strong links to <span class="hlt">regional</span> government and industry. The new test site will be located in the hilly, forested terrain of the Swabian Alps between Stuttgart and Germany, and will consist of two <span class="hlt">wind</span> turbines with four meteorological towers. The test site will be used for accompanying ecological research and will also have mobile eddy covariance measurement stations as well as bird and bat monitoring systems. Seismic and noise monitoring systems are also planned. The large number of auxiliary measurements at this facility are intended to allow the complete atmosphere-<span class="hlt">wind</span> turbine-environment-people system to be characterized. This presentation will show some of the numerical weather prediction work and measurements done at the site so far, and inform the audience about <span class="hlt">Wind</span>ForS' plans for the future. A major focus of the presentation will be on opportunities for collaboration through field campaigns or model validation.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-12-04/pdf/2012-29293.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-12-04/pdf/2012-29293.pdf"><span>77 FR 71780 - U.S. <span class="hlt">Trade</span> Mission to Asia in Conjunction With <span class="hlt">Trade</span> <span class="hlt">Winds</span>-Asia, The Philippines, Hong Kong...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-12-04</p> <p>..., environmental technologies and services, financial services, franchising, healthcare & medical, hotel/restaurant... selection criteria as outlined below. A minimum of 65 companies and/or <span class="hlt">trade</span> associations will be selected.... content. Selection Criteria for Participation Selection will be based on the following criteria...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24633049','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24633049"><span>Soil dust aerosols and <span class="hlt">wind</span> as predictors of seasonal meningitis incidence in Niger.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Pérez García-Pando, Carlos; Stanton, Michelle C; Diggle, Peter J; Trzaska, Sylwia; Miller, Ron L; Perlwitz, Jan P; Baldasano, José M; Cuevas, Emilio; Ceccato, Pietro; Yaka, Pascal; Thomson, Madeleine C</p> <p>2014-07-01</p> <p>Epidemics of meningococcal meningitis are concentrated in sub-Saharan Africa during the dry season, a period when the <span class="hlt">region</span> is affected by the Harmattan, a dry and dusty northeasterly <span class="hlt">trade</span> <span class="hlt">wind</span> blowing from the Sahara into the Gulf of Guinea. We examined the potential of climate-based statistical forecasting models to predict seasonal incidence of meningitis in Niger at both the national and district levels. We used time series of meningitis incidence from 1986 through 2006 for 38 districts in Niger. We tested models based on data that would be readily available in an operational framework, such as climate and dust, population, and the incidence of early cases before the onset of the meningitis season in January-May. Incidence was used as a proxy for immunological state, susceptibility, and carriage in the population. We compared a range of negative binomial generalized linear models fitted to the meningitis data. At the national level, a model using early incidence in December and averaged November-December zonal <span class="hlt">wind</span> provided the best fit (pseudo-R2 = 0.57), with zonal <span class="hlt">wind</span> having the greatest impact. A model with surface dust concentration as a predictive variable performed indistinguishably well. At the district level, the best spatiotemporal model included zonal <span class="hlt">wind</span>, dust concentration, early incidence in December, and population density (pseudo-R2 = 0.41). We showed that <span class="hlt">wind</span> and dust information and incidence in the early dry season predict part of the year-to-year variability of the seasonal incidence of meningitis at both national and district levels in Niger. Models of this form could provide an early-season alert that <span class="hlt">wind</span>, dust, and other conditions are potentially conducive to an epidemic.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-12-17/pdf/2012-30234.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-12-17/pdf/2012-30234.pdf"><span>77 FR 74694 - Utility Scale <span class="hlt">Wind</span> Towers From China and Vietnam; Commission Determination To Deny a Request To...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-12-17</p> <p>...)] Utility Scale <span class="hlt">Wind</span> Towers From China and Vietnam; Commission Determination To Deny a Request To Hold a Portion of a Hearing in Camera AGENCY: U.S. International <span class="hlt">Trade</span> Commission. ACTION: Commission..., Office of the General Counsel, U.S. International <span class="hlt">Trade</span> Commission, telephone 202- 205-3041. Hearing...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19930044166&hterms=hawley&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhawley%2Bw','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19930044166&hterms=hawley&qs=N%3D0%26Ntk%3DAuthor-Name%26Ntx%3Dmode%2Bmatchall%26Ntt%3Dhawley%2Bw"><span>Performance of a 1-micron, 1-joule Coherent Launch Site Atmospheric <span class="hlt">Wind</span> Sounder</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Hawley, James G.; Targ, Russell; Bruner, Richard; Henderson, Sammy W.; Hale, Charles P.; Vetorino, Steven; Lee, R. W.; Harper, Scott; Khan, Tayyab</p> <p>1992-01-01</p> <p>The paper describes the design and performance of the Coherent Launch Site Atmospheric <span class="hlt">Wind</span> Sounder (CLAWS), which is a test and demonstration program designed for monitoring <span class="hlt">winds</span> with a solid-state lidar in real time for the launch site vehicle guidance and control application. Analyses were conducted to <span class="hlt">trade</span> off CO2 (9.11- and 10.6-microns), Ho:YAG (2.09 microns), and Nd:YAG (1.06-micron) laser-based lidars. The measurements set a new altitude record (26 km) for coherent <span class="hlt">wind</span> measurements in the stratosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1049318','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1049318"><span>A Habitat-based <span class="hlt">Wind</span>-Wildlife Collision Model with Application to the Upper Great Plains <span class="hlt">Region</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>Forcey, Greg, M.</p> <p></p> <p>Most previous studies on collision impacts at <span class="hlt">wind</span> facilities have taken place at the site-specific level and have only examined small-scale influences on mortality. In this study, we examine landscape-level influences using a hierarchical spatial model combined with existing datasets and life history knowledge for: Horned Lark, Red-eyed Vireo, Mallard, American Avocet, Golden Eagle, Whooping Crane, red bat, silver-haired bat, and hoary bat. These species were modeled in the central United States within Bird Conservation <span class="hlt">Regions</span> 11, 17, 18, and 19. For the bird species, we modeled bird abundance from existing datasets as a function of habitat variables known tomore » be preferred by each species to develop a relative abundance prediction for each species. For bats, there are no existing abundance datasets so we identified preferred habitat in the landscape for each species and assumed that greater amounts of preferred habitat would equate to greater abundance of bats. The abundance predictions for bird and bats were modeled with additional exposure factors known to influence collisions such as visibility, <span class="hlt">wind</span>, temperature, precipitation, topography, and behavior to form a final mapped output of predicted collision risk within the study <span class="hlt">region</span>. We reviewed published mortality studies from <span class="hlt">wind</span> farms in our study <span class="hlt">region</span> and collected data on reported mortality of our focal species to compare to our modeled predictions. We performed a sensitivity analysis evaluating model performance of 6 different scenarios where habitat and exposure factors were weighted differently. We compared the model performance in each scenario by evaluating observed data vs. our model predictions using spearmans rank correlations. Horned Lark collision risk was predicted to be highest in the northwestern and west-central portions of the study <span class="hlt">region</span> with lower risk predicted elsewhere. Red-eyed Vireo collision risk was predicted to be the highest in the eastern portions of the study <span class="hlt">region</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22540777','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22540777"><span>Information <span class="hlt">trade</span>-offs for optical quantum communication.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wilde, Mark M; Hayden, Patrick; Guha, Saikat</p> <p>2012-04-06</p> <p>Recent work has precisely characterized the achievable <span class="hlt">trade</span>-offs between three key information processing tasks-classical communication (generation or consumption), quantum communication (generation or consumption), and shared entanglement (distribution or consumption), measured in bits, qubits, and ebits per channel use, respectively. Slices and corner points of this three-dimensional <span class="hlt">region</span> reduce to well-known protocols for quantum channels. A <span class="hlt">trade</span>-off coding technique can attain any point in the <span class="hlt">region</span> and can outperform time sharing between the best-known protocols for accomplishing each information processing task by itself. Previously, the benefits of <span class="hlt">trade</span>-off coding that had been found were too small to be of practical value (viz., for the dephasing and the universal cloning machine channels). In this Letter, we demonstrate that the associated performance gains are in fact remarkably high for several physically relevant bosonic channels that model free-space or fiber-optic links, thermal-noise channels, and amplifiers. We show that significant performance gains from <span class="hlt">trade</span>-off coding also apply when <span class="hlt">trading</span> photon-number resources between transmitting public and private classical information simultaneously over secret-key-assisted bosonic channels. © 2012 American Physical Society</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMPA21D0357L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMPA21D0357L"><span>Earth Observations in Support of Offshore <span class="hlt">Wind</span> Energy Management in the Euro-Atlantic <span class="hlt">Region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Liberato, M. L. R.</p> <p>2017-12-01</p> <p>Climate change is one of the most important challenges in the 21st century and the energy sector is a major contributor to GHG emissions. Therefore greater attention has been given to the evaluation of offshore <span class="hlt">wind</span> energy potentials along coastal areas, as it is expected offshore <span class="hlt">wind</span> energy to be more efficient and cost-effective in the near future. Europe is developing offshore sites for over two decades and has been growing at gigawatt levels in annual capacity. Portugal is among these countries, with the development of a 25MW <span class="hlt">Wind</span>Float Atlantic <span class="hlt">wind</span> farm project. The international scientific community has developed robust ability on the research of the climate system components and their interactions. Climate scientists have gained expertise in the observation and analysis of the climate system as well as on the improvement of model and predictive capabilities. Developments on climate science allow advancing our understanding and prediction of the variability and change of Earth's climate on all space and time scales, while improving skilful climate assessments and tools for dealing with future challenges of a warming planet. However the availability of greater datasets amplifies the complexity on manipulation, representation and consequent analysis and interpretation of such datasets. Today the challenge is to translate scientific understanding of the climate system into climate information for society and decision makers. Here we discuss the development of an integration tool for multidisciplinary research, which allows access, management, tailored pre-processing and visualization of datasets, crucial to foster research as a service to society. One application is the assessment and monitoring of renewable energy variability, such as <span class="hlt">wind</span> or solar energy, at several time and space scales. We demonstrate the ability of the e-science platform for planning, monitoring and management of renewable energy, particularly offshore <span class="hlt">wind</span> energy in the Euro</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22667380-solar-wind-origin-acceleration-measurements-from-ace','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22667380-solar-wind-origin-acceleration-measurements-from-ace"><span>ON SOLAR <span class="hlt">WIND</span> ORIGIN AND ACCELERATION: MEASUREMENTS FROM ACE</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>Stakhiv, Mark; Lepri, Susan T.; Landi, Enrico</p> <p></p> <p>The origin and acceleration of the solar <span class="hlt">wind</span> are still debated. In this paper, we search for signatures of the source <span class="hlt">region</span> and acceleration mechanism of the solar <span class="hlt">wind</span> in the plasma properties measured in situ by the Advanced Composition Explorer spacecraft. Using the elemental abundances as a proxy for the source <span class="hlt">region</span> and the differential velocity and ion temperature ratios as a proxy for the acceleration mechanism, we are able to identify signatures pointing toward possible source <span class="hlt">regions</span> and acceleration mechanisms. We find that the fast solar <span class="hlt">wind</span> in the ecliptic plane is the same as that observed frommore » the polar <span class="hlt">regions</span> and is consistent with wave acceleration and coronal-hole origin. We also find that the slow <span class="hlt">wind</span> is composed of two components: one similar to the fast solar <span class="hlt">wind</span> (with slower velocity) and the other likely originating from closed magnetic loops. Both components of the slow solar <span class="hlt">wind</span> show signatures of wave acceleration. From these findings, we draw a scenario that envisions two types of <span class="hlt">wind</span>, with different source <span class="hlt">regions</span> and release mechanisms, but the same wave acceleration mechanism.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/7168186-power-interconnection-projects-asean-region-definitional-mission-report-export-trade-information','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/7168186-power-interconnection-projects-asean-region-definitional-mission-report-export-trade-information"><span>Power interconnection projects in the ASEAN <span class="hlt">region</span>: Definitional-mission report No. 1. Export <span class="hlt">trade</span> information</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>Not Available</p> <p>1992-06-01</p> <p>In response to a request from the Association of Southeast Asian Nations (ASEAN), the U.S. <span class="hlt">Trade</span> and Development Program (TDP) conducted a definitional mission to evaluate the prospects of TDP funding for five Power Interconnection Projects in the ASEAN <span class="hlt">region</span>. These projects included: Batam-Singapore Interconnection; Sumatera-Peninsular Malaysia Interconnection; Sarawak-West Kalimantan Interconnection; Sarawak-Brunei-Sabah Interconnection; and Java-Sumatera Interconnection. Based on a review of the proposed scopes of work for the projects and the discussions in the field, the report summarizes the technical details and the costs of implementation for the projects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018BoLMe.tmp..178G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018BoLMe.tmp..178G"><span>On <span class="hlt">Wind</span> Forces in the Forest-Edge <span class="hlt">Region</span> During Extreme-Gust Passages and Their Implications for Damage Patterns</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Gromke, Christof; Ruck, Bodo</p> <p>2018-03-01</p> <p>A damage pattern that is occasionally found after a period of strong <span class="hlt">winds</span> shows an area of damaged trees inside a forest stand behind an intact stripe of trees directly at the windward edge. In an effort to understand the mechanism leading to this damage pattern, <span class="hlt">wind</span> loading in the forest-edge <span class="hlt">region</span> during passages of extreme gusts with different characteristics are investigated using a scaled forest model in the <span class="hlt">wind</span> tunnel. The interaction of a transient extreme gust with the stationary atmospheric boundary layer (ABL) as a background flow at the forest edge leads to the formation of a vortex at the top of the canopy. This vortex intensifies when travelling downstream and subsequently deflects high-momentum air from above the canopy downwards resulting in increased <span class="hlt">wind</span> loading on the tree crowns. Under such conditions, the decrease in <span class="hlt">wind</span> loading in the streamwise direction can be relatively weak compared to stationary ABL approach flows. The resistance of trees with streamwise distance from the forest edge, however, is the result of adaptive growth to <span class="hlt">wind</span> loading under stationary flow conditions and shows a rapid decline within two to three tree heights behind the windward edge. For some of the extreme gusts realized, an exceedance of the <span class="hlt">wind</span> loading over the resistance of the trees is found at approximately three tree heights behind the forest edge, suggesting that the damage pattern described above can be caused by the interaction of a transient extreme gust with the stationary ABL flow.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19720011641','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19720011641"><span>The requirements for a new full scale subsonic <span class="hlt">wind</span> tunnel</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Kelly, M. W.; Mckinney, M. O.; Luidens, R. W.</p> <p>1972-01-01</p> <p>Justification and requirements are presented for a large subsonic <span class="hlt">wind</span> tunnel capable of testing full scale aircraft, rotor systems, and advanced V/STOL propulsion systems. The design considerations and constraints for such a facility are reviewed, and the <span class="hlt">trades</span> between facility test capability and costs are discussed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eosweb.larc.nasa.gov/project/polarwindsii/polarwindsii_table','SCIGOV-ASDC'); return false;" href="https://eosweb.larc.nasa.gov/project/polarwindsii/polarwindsii_table"><span>Polar<span class="hlt">Winds</span> I & II</span></a></p> <p><a target="_blank" href="http://eosweb.larc.nasa.gov/">Atmospheric Science Data Center </a></p> <p></p> <p>2018-04-20</p> <p>... (Organized Large Eddies), and near surface <span class="hlt">winds</span> over open water, transitional ice zones and the Greenland Ice Cap. Polar <span class="hlt">Winds</span> I was ... total, twenty-four individual missions with over 80 hours of research flights were flown in the Arctic <span class="hlt">region</span> near Greenland and Iceland ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JGRA..121..949E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JGRA..121..949E"><span>Solar <span class="hlt">wind</span> interaction with comet 67P: Impacts of corotating interaction <span class="hlt">regions</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Edberg, N. J. T.; Eriksson, A. I.; Odelstad, E.; Vigren, E.; Andrews, D. J.; Johansson, F.; Burch, J. L.; Carr, C. M.; Cupido, E.; Glassmeier, K.-H.; Goldstein, R.; Halekas, J. S.; Henri, P.; Koenders, C.; Mandt, K.; Mokashi, P.; Nemeth, Z.; Nilsson, H.; Ramstad, R.; Richter, I.; Wieser, G. Stenberg</p> <p>2016-02-01</p> <p>We present observations from the Rosetta Plasma Consortium of the effects of stormy solar <span class="hlt">wind</span> on comet 67P/Churyumov-Gerasimenko. Four corotating interaction <span class="hlt">regions</span> (CIRs), where the first event has possibly merged with a coronal mass ejection, are traced from Earth via Mars (using Mars Express and Mars Atmosphere and Volatile EvolutioN mission) to comet 67P from October to December 2014. When the comet is 3.1-2.7 AU from the Sun and the neutral outgassing rate ˜1025-1026 s-1, the CIRs significantly influence the cometary plasma environment at altitudes down to 10-30 km. The ionospheric low-energy (˜5 eV) plasma density increases significantly in all events, by a factor of >2 in events 1 and 2 but less in events 3 and 4. The spacecraft potential drops below -20 V upon impact when the flux of electrons increases. The increased density is likely caused by compression of the plasma environment, increased particle impact ionization, and possibly charge exchange processes and acceleration of mass-loaded plasma back to the comet ionosphere. During all events, the fluxes of suprathermal (˜10-100 eV) electrons increase significantly, suggesting that the heating mechanism of these electrons is coupled to the solar <span class="hlt">wind</span> energy input. At impact the magnetic field strength in the coma increases by a factor of 2-5 as more interplanetary magnetic field piles up around the comet. During two CIR impact events, we observe possible plasma boundaries forming, or moving past Rosetta, as the strong solar <span class="hlt">wind</span> compresses the cometary plasma environment. We also discuss the possibility of seeing some signatures of the ionospheric response to tail disconnection events.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012EGUGA..1413019Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012EGUGA..1413019Z"><span><span class="hlt">Wind</span>-tunnel experiments of scalar transport in aligned and staggered <span class="hlt">wind</span> farms</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, W.; Markfort, C. D.; Porté-Agel, F.</p> <p>2012-04-01</p> <p><span class="hlt">Wind</span> energy is the fastest growing renewable energy worldwide, and it is expected that many more large-scale <span class="hlt">wind</span> farms will be built and will cover a significant portion of land and ocean surfaces. By extracting kinetic energy from the atmospheric boundary layer, <span class="hlt">wind</span> farms may affect the exchange/transport of momentum, heat and moisture between the atmosphere and land surface. To ensure the long-term sustainability of <span class="hlt">wind</span> energy, it is important to understand the influence of large-scale <span class="hlt">wind</span> farms on land-atmosphere interaction. Knowledge of this impact will also be useful to improve parameterizations of <span class="hlt">wind</span> farms in numerical prediction tools, such as large-scale weather models and large-eddy simulation. Here, we present <span class="hlt">wind</span>-tunnel measurements of the surface scalar (heat) flux from model <span class="hlt">wind</span> farms, consisting of more than 10 rows of <span class="hlt">wind</span> turbines, in a turbulent boundary layer with a surface heat source. Spatially distributed surface heat flux was obtained in idealized aligned and staggered <span class="hlt">wind</span> farm layouts, having the same turbine distribution density. Measurements, using surface-mounted heat flux sensors, were taken at the 11th out of 12 rows of <span class="hlt">wind</span> turbines, where the mean flow achieves a quasi-equilibrium state. In the aligned farm, there exist two distinct <span class="hlt">regions</span> of increased and decreased surface heat flux on either side of turbine columns. The <span class="hlt">regions</span> are correlated with coherent wake rotation in the turbine-array. On the upwelling side there is decreased flux, while on the downwelling side cool air moves towards the surface causing increased flux. For the staggered farm, the surface heat flux exhibits a relatively uniform distribution and an overall reduction with respect to the boundary layer flow, except in the vicinity of the turbine tower. This observation is also supported by near-surface temperature and turbulent heat flux measured using a customized x-wire/cold-wire. The overall surface heat flux, relative to that of the boundary layer</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..217a2019M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..217a2019M"><span>Assessment of C-Type Darrieus <span class="hlt">Wind</span> Turbine Under Low <span class="hlt">Wind</span> Speed Condition</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Misaran, M. S.; Rahman, Md. M.; Muzammil, W. K.; Ismail, M. A.</p> <p>2017-07-01</p> <p>Harvesting <span class="hlt">wind</span> energy in in a low <span class="hlt">wind</span> speed <span class="hlt">region</span> is deem un-economical if not daunting task. Study shows that a minimum cut in speed of 3.5 m/s is required to extract a meaningful <span class="hlt">wind</span> energy for electricity while a mean speed of 6 m/s is preferred. However, in Malaysia the mean speed is at 2 m/s with certain potential areas having 3 m/s mean speed. Thus, this work aims to develop a <span class="hlt">wind</span> turbine that able to operate at lower cut-in speed and produce meaningful power for electricity generation. A C-type Darrieus blade is selected as it shows good potential to operate in arbitrary <span class="hlt">wind</span> speed condition. The <span class="hlt">wind</span> turbine is designed and fabricated in UMS labs while the performance of the <span class="hlt">wind</span> turbine is evaluated in a simulated <span class="hlt">wind</span> condition. Test result shows that the <span class="hlt">wind</span> turbine started to rotate at 1 m/s compared to a NACA 0012 Darrieus turbine that started to rotate at 3 m/s. The performance of the turbine shows that it have good potential to be used in an intermittent arbitrary <span class="hlt">wind</span> speed condition as well as low mean <span class="hlt">wind</span> speed condition.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1711318K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1711318K"><span>Evaluation of representativeness of near-surface <span class="hlt">winds</span> in station measurements, global and <span class="hlt">regional</span> reanalysis for Germany</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kaspar, Frank; Kaiser-Weiss, Andrea K.; Heene, Vera; Borsche, Michael; Keller, Jan</p> <p>2015-04-01</p> <p>Within the preparation activities for a European COPERNICUS Climate Change Service (C3S) several ongoing research projects analyse the potential of global and <span class="hlt">regional</span> model-based climate reanalyses for applications. A user survey in the FP7-project CORE-CLIMAX revealed that surface <span class="hlt">wind</span> (10 m) is among the most frequently used parameters of global reanalysis products. The FP7 project UERRA (Uncertainties in Ensembles of <span class="hlt">Regional</span> Re-Analysis) has the focus on <span class="hlt">regional</span> European reanalysis and the associated uncertainties, also from a user perspective. Especially in the field of renewable energy planning and production there is a need for climatological information across all spatial scales, i.e., from climatology at a certain site to the spatial scale of national or continental renewable energy production. Here, we focus on a comparison of <span class="hlt">wind</span> measurements of the Germany's meteorological service (Deutscher Wetterdienst, DWD) with global reanalyses of ECWMF and a <span class="hlt">regional</span> reanalysis for Europe based on DWD's NWP-model COSMO (performed by the Hans-Ertel-Center for Weather Research, University of Bonn). Reanalyses can provide valuable additional information on larger scale variability, e.g. multi-annual variation over Germany. However, changes in the observing system, model errors and biases have to be carefully considered. On the other hand, the ground-based observation networks partly suffer from change of the station distribution, changes in instrumentation, measurements procedures and quality control as well as local changes which might modify their spatial representativeness. All these effects might often been unknown or hard to characterize, although plenty of the meta-data information has been recorded for the German stations. One focus of the presentation will be the added-value of the <span class="hlt">regional</span> reanalysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017E3SWC..2309001A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017E3SWC..2309001A"><span>The Feasibility of Utilizing <span class="hlt">Wind</span> Energy in Commercial Buildings With Special Reference to the Kingdom of Bahrain</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Abdulrahim Saeed, Saeed</p> <p>2017-11-01</p> <p>This article shall investigate the feasibility of utilizing <span class="hlt">wind</span> energy for commercial buildings with special reference to the Kingdom of Bahrain. Bahrain World <span class="hlt">Trade</span> Center which was built in 2008, is located in the city of Manama. The fifty-story complex contains identical twin towers that rise over 240 meters in height. The towers are connected by three bridges which hold three turbines each 29 meters long. The three turbines were originally design to provide electric energy required for lighting. The Bahrain World <span class="hlt">Trade</span> Center was selected as a case study to investigate the feasibility of utilizing <span class="hlt">wind</span> energy technologies in skyscrapers with special reference to the Kingdom of Bahrain. It is hoped that the findings and conclusion of the study shall be of some value for future utilization of <span class="hlt">wind</span> energy in the GCC countries and the world at large.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018PhDT.........2X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018PhDT.........2X"><span>Understanding Large <span class="hlt">Wind</span> Farm Impacts on <span class="hlt">Regional</span> Climate and Vegetation Growth from Observational and Modeling Perspectives</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xia, Geng</p> <p></p> <p>In the most recent decade, <span class="hlt">wind</span> energy has experienced exponential growth worldwide and this rapid increase is expected to continue, particularly over farmlands in the United States. This poses an important question regarding whether the widespread deployment of <span class="hlt">wind</span> turbines (WTs) will influence surface/near-surface microclimate and vegetation growth. In this dissertation, I investigate the potential <span class="hlt">wind</span> farm (WF) impacts on <span class="hlt">regional</span> climate and vegetation growth from both observational and modeling perspectives. High resolution satellite, radiosonde and field observations are used to determine the magnitude and variability of WF-induced changes on surface/near-surface temperatures while the Weather Research and Forecasting (WRF) model is used to simulate these changes in real-world WFs at <span class="hlt">regional</span> scales and to uncover the physical processes behind the simulated temperature changes. First, the primary physical mechanisms controlling the seasonal and diurnal variations of WF impacts on land surface temperature (LST) are investigated by analyzing both satellite data and field observations. It is found that the turbine-induced turbulent kinetic energy (TKE) relative to the background TKE determines the magnitude and variability of such impacts. In addition, atmospheric stability also matters in determining the sign and strength of the net downward heat transport as well as the magnitude of the background TKE. Second, the WRF's ability in simulating the observed WF impacts on LST is examined by conducting real-world WF experiments driven by realistic initial and boundary conditions. Overall, the WRF model can moderately reproduce the observed spatiotemporal variations of the background LST but has difficulties in reproducing such variations for the turbine-induced LST change signals at pixel levels. However, the model is still able to reproduce the coherent and consistent responses of the observed WF-induced LST changes at <span class="hlt">regional</span> scales. Third, the spatiotemporal</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2012-05-17/pdf/2012-11980.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2012-05-17/pdf/2012-11980.pdf"><span>77 FR 29315 - Utility Scale <span class="hlt">Wind</span> Towers From the People's Republic of China and the Socialist Republic of...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2012-05-17</p> <p>... DEPARTMENT OF COMMERCE International <span class="hlt">Trade</span> Administration [A-570-981, A-552-814] Utility Scale... duty investigations of utility scale <span class="hlt">wind</span> towers from the People's Republic of China and the Socialist... investigations are currently due no later than June 6, 2012. \\1\\ See Utility Scale <span class="hlt">Wind</span> Towers From the People's...</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_15");'>15</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li class="active"><span>17</span></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_17 --> <div id="page_18" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_16");'>16</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li class="active"><span>18</span></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="341"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://images.nasa.gov/#/details-PIA20365.html','SCIGOVIMAGE-NASA'); return false;" href="https://images.nasa.gov/#/details-PIA20365.html"><span>NASA RapidScat Observes El Nino Blowing in the <span class="hlt">Winds</span></span></a></p> <p><a target="_blank" href="https://images.nasa.gov/">NASA Image and Video Library</a></p> <p></p> <p>2016-01-21</p> <p>While El Niño events have a significant impact on the entire Earth System, they are most easily visible in measurements of sea surface temperature (SST), sea surface height (SSH) and ocean <span class="hlt">winds</span> near the surface. In fact, the precursor and the main driver of El Niño events is manifested in the weakening of the normally westward blowing <span class="hlt">trade</span> <span class="hlt">winds</span>, or even their complete reversal to blow from west to east, in the Western and Central tropical Pacific. http://photojournal.jpl.nasa.gov/catalog/PIA20365</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014ClDy...42.1067T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014ClDy...42.1067T"><span>Circulation effect: response of precipitation δ18O to the ENSO cycle in monsoon <span class="hlt">regions</span> of China</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tan, Ming</p> <p>2014-02-01</p> <p>Inter-annual variation in the ratio of 18O to 16O of precipitation (δ18Op) in the monsoon <span class="hlt">regions</span> of China (MRC, area approximately east of 100°E) has not yet been fully analyzed. Based on an analysis of the relationships between the time series of amount-weighted mean annual δ18O in precipitation (δ18Ow) and meteorological variables such as temperature, precipitation as well as atmospheric/oceanic circulation indices, it is recognized that the El Niño-Southern Oscillation (ENSO) cycle appears to be the dominant control on the inter-annual variation in δ18Op in the MRC. Further analysis shows that the <span class="hlt">trade</span> <span class="hlt">wind</span> plays a role in governing δ18Ow through affecting the intensity of the different summer monsoon circulations which are closely linked to the weakening (weaker than normal) and strengthening (stronger than normal) of the <span class="hlt">trade</span> <span class="hlt">wind</span> and gives the δ18Ow different values at or over inter-annual timescales. The southwest monsoon (SWM) drives long-distance transport of water vapor from Indian Ocean to the MRC, and along this pathway increasing rainout leads to more negative δ18Ow via Rayleigh distillation processes. In contrast, the southeast monsoon (SEM), which is consistent with the changes in the strength of the West Pacific subtropical high, drives short-distance water vapor transport from the West Pacific Ocean to the MRC and leads to less negative δ18Ow. Therefore, the δ18Ow value directly reflects the differences in influence between the SWM, which is strong when the SE <span class="hlt">trade</span> <span class="hlt">wind</span> is strong, and the SEM, which is strong when the SE <span class="hlt">trade</span> <span class="hlt">wind</span> is weak. In addition, the South China Sea Monsoon also transports local water vapor as well as plays a role in achieving the synchronization between the δ18Ow and ENSO. The author thus terms the δ18Op rhythm in the MRC the "circulation effect". In turn, the δ18Op variation in the MRC has the potential to provide information on atmospheric circulation and the signal of δ18Op recorded in natural archives</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC32B..02L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC32B..02L"><span><span class="hlt">Trade</span> in water and commodities as adaptations to global change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lammers, R. B.; Hertel, T. W.; Prousevitch, A.; Baldos, U. L. C.; Frolking, S. E.; Liu, J.; Grogan, D. S.</p> <p>2015-12-01</p> <p>The human capacity for altering the water cycle has been well documented and given the expected change due to population, income growth, biofuels, climate, and associated land use change, there remains great uncertainty in both the degree of increased pressure on land and water resources and in our ability to adapt to these changes. Alleviating <span class="hlt">regional</span> shortages in water supply can be carried out in a spatial hierarchy through i) direct <span class="hlt">trade</span> of water between all <span class="hlt">regions</span>, ii) development of infrastructure to improve water availability within <span class="hlt">regions</span> (e.g. impounding rivers), iii) via inter-basin hydrological transfer between neighboring <span class="hlt">regions</span> and, iv) via virtual water <span class="hlt">trade</span>. These adaptation strategies can be managed via market <span class="hlt">trade</span> in water and commodities to identify those strategies most likely to be adopted. This work combines the physically-based University of New Hampshire Water Balance Model (WBM) with the macro-scale Purdue University Simplified International Model of agricultural Prices Land use and the Environment (SIMPLE) to explore the interaction of supply and demand for fresh water globally. In this work we use a newly developed grid cell-based version of SIMPLE to achieve a more direct connection between the two modeling paradigms of physically-based models with optimization-driven approaches characteristic of economic models. We explore questions related to the global and <span class="hlt">regional</span> impact of water scarcity and water surplus on the ability of <span class="hlt">regions</span> to adapt to future change. Allowing for a variety of adaptation strategies such as direct <span class="hlt">trade</span> of water and expanding the built water infrastructure, as well as indirect <span class="hlt">trade</span> in commodities, will reduce overall global water stress and, in some <span class="hlt">regions</span>, significantly reduce their vulnerability to these future changes.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=PIA03789&hterms=Volcano+Facts&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DVolcano%2BFacts','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=PIA03789&hterms=Volcano+Facts&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D20%26Ntt%3DVolcano%2BFacts"><span>Cerberus <span class="hlt">Wind</span> Streaks</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>2002-01-01</p> <p>(Released 6 May 2002) The Science Cerberus is a dark <span class="hlt">region</span> on Mars that has shrunk down from a continuous length of about 1000 km to roughly three discontinuous spots a few 100 kms in length in less than 20 years. There are two competing processes at work in the Cerberus <span class="hlt">region</span> that produce the bright and dark features seen in this THEMIS image. Bright dust settles out of the atmosphere, especially after global dust storms, depositing a layer just thick enough to brighten the dark surfaces. Deposition occurs preferentially in the low <span class="hlt">wind</span> 'shadow zones' within craters and downwind of crater rims, producing the bright streaks. The direction of the streaks clearly indicates that the dominant <span class="hlt">winds</span> come from the northeast. Dust deposition would completely blot out the dark areas if it were not for the action of <span class="hlt">wind</span>-blown sand grains scouring the surface and lifting the dust back into the atmosphere. Again, the shadow zones are protected from the blowing sand, preserving the bright layer of dust. Also visible in this image are lava flow features extending from the flanks of the huge Elysium volcanoes to the northwest. Two shallow channels and a raised flow lobe are just barely discernable. The lava channel in the middle of the image crosses the boundary of the bright and dark surfaces without any obvious change in its morphology. This demonstrates that the bright dust layer is very thin in this location, perhaps as little as a few millimeters. The Story Mars is an ever-changing land of spectacular contrasts. This THEMIS image shows the Cerberus <span class="hlt">region</span> of Mars, a dark area located near the Elysium volcanoes and fittingly named after the three-headed, dragon-tailed dog who guards the door of the underworld. Two opposing processes are at work here: a thin layer of dust falling from the atmosphere and/or dust storms creating brighter surface areas (e.g. the top left portion of this image) and dust being scoured away by the action of the Martian <span class="hlt">wind</span> disturbing the sand</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19820058209&hterms=debye+length&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddebye%2Blength','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19820058209&hterms=debye+length&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D60%26Ntt%3Ddebye%2Blength"><span>Observations of structuring in the downstream <span class="hlt">region</span> of a large spherical model in a laboratory simulated solar <span class="hlt">wind</span> plasma</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Intriligator, D. S.; Steele, G. R.</p> <p>1982-01-01</p> <p>The effects of inserting a spherical conducting model, large in comparison with the Debye length, into a free streaming high-energy 1 kV) unmagnetized hydrogen plasma are investigated in order to measure energies and compositions directly relevant to solar <span class="hlt">wind</span> and astrophysical plasma phenomena. Holding the incident plasma parameters constant, transverse profiles of the net Langmuir probe current are plotted at various locations downstream in the model wake and are divided into three <span class="hlt">regions</span> (the shadow, transition, and boundary). Results attributable to the use of a high-energy plasma show that enhancements in the shadow exist at downstream locations where the Mach ratio is less than one, and turbulence exists in the transition <span class="hlt">region</span> on the shadow edges and outside in the boundary <span class="hlt">region</span>. In addition, a small current enhancement is found in the boundary and can be attributed to the plasma/model interaction. It is concluded that many similar features observed by spacecraft downstream from planetary bodies are relatively permanent and are due to the intrinsic nature of the interaction between the solar <span class="hlt">wind</span> plasma and the obstacle.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015AGUFMGC53E1248K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015AGUFMGC53E1248K"><span>A Study of Spatio-Temporal Variability in Future <span class="hlt">Wind</span> Energy over the Korean Peninsula Using <span class="hlt">Regional</span> Climate Model Ensemble Projections</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>KIM, Y.; Lim, Y. J.; Kim, Y. H.; Kim, B. J.</p> <p>2015-12-01</p> <p>The impacts of climate change on <span class="hlt">wind</span> speed, <span class="hlt">wind</span> energy density (WED), and potential electronic production (PEP) over the Korean peninsula have been investigated by using five <span class="hlt">regional</span> climate models (HadGEM3-RA, RegCM, WRF, GRIMs and MM5) ensemble projection data. HadGEM2-AO based two RCP scenarios (RCP4.5/8.5) data have been used for initial and boundary condition to all RCMs. <span class="hlt">Wind</span> energy density and its annual and seasonal variability have been estimated based on monthly near-surface <span class="hlt">wind</span> speeds, and the potential electronic production and its change have been also analyzed. As a result of comparison ensemble models based annual mean <span class="hlt">wind</span> speed for 25-yr historical period (1981-2005) to the ERA-interim, it is shown that all RCMs overestimate near-surface <span class="hlt">wind</span> speed compared to the reanalysis data but the results of HadGEM3-RA are most comparable. The changes annual and seasonal mean of WED and PEP for the historical period and comparison results to future projection (2021-2050) will be presented in this poster session. We also scrutinize the changes in mean sea level pressure and mean sea level pressure gradient in driving GCM/RCM as a factor inducing the variations. Our results can be used as a background data for devising a plan to develop and operate <span class="hlt">wind</span> farm over the Korean Peninsula.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/15007087','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/15007087"><span><span class="hlt">Wind</span> Power Today and Tomorrow</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>Not Available</p> <p></p> <p><span class="hlt">Wind</span> Power Today and Tomorrow is an annual publication that provides an overview of the <span class="hlt">wind</span> research conducted under the U.S. Department of Energy's <span class="hlt">Wind</span> and Hydropower Technologies Program. The purpose of <span class="hlt">Wind</span> Power Today and Tomorrow is to show how DOE supports <span class="hlt">wind</span> turbine research and deployment in hopes of furthering the advancement of <span class="hlt">wind</span> technologies that produce clean, low-cost, reliable energy. Content objectives include: educate readers about the advantages and potential for widespread deployment of <span class="hlt">wind</span> energy; explain the program's objectives and goals; describe the program's accomplishments in research and application; examine the barriers to widespread deployment; describemore » the benefits of continued research and development; facilitate technology transfer; and attract cooperative <span class="hlt">wind</span> energy projects with industry. This 2003 edition of the program overview also includes discussions about <span class="hlt">wind</span> industry growth in 2003, how DOE is taking advantage of low <span class="hlt">wind</span> speed <span class="hlt">region</span> s through advancing technology, and distributed applications for small <span class="hlt">wind</span> turbines.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982STIN...8323779Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982STIN...8323779Z"><span><span class="hlt">Wind</span> energy converter with high-speed vertical axis rotor and straight rotor blades</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zelck, G.</p> <p>1982-11-01</p> <p>Complete documents for a <span class="hlt">wind</span> energy converter with a vertical axis rotor and straight blades (H-rotor) were developed. The 2 blade rotor with rigid and rectangular air foils in wooden construction reaches the nominal output of 75 KVA from 11,4 m/sec. <span class="hlt">wind</span> velocity onwards. The development activities are supported by <span class="hlt">wind</span> tunnel and component tests. The final design selected was based upon previous development work. <span class="hlt">Trade</span> offs show that the design is more advantageous compared to other designs. The use of wood as a material for the rotary and horizontal blade supports gives positive result.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22122963','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22122963"><span>Impact of <span class="hlt">wind</span> turbine noise in the Netherlands.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Verheijen, Edwin; Jabben, Jan; Schreurs, Eric; Smith, Kevin B</p> <p>2011-01-01</p> <p>The Dutch government aims at an increase of <span class="hlt">wind</span> energy up to 6 000 MW in 2020 by placing new <span class="hlt">wind</span> turbines on land or offshore. At the same time, the existing noise legislation for <span class="hlt">wind</span> turbines is being reconsidered. For the purpose of establishing a new noise reception limit value expressed in L den , the impact of <span class="hlt">wind</span> turbine noise under the given policy targets needs to be explored. For this purpose, the consequences of different reception limit values for the new Dutch noise legislation have been studied, both in terms of effects on the population and regarding sustainable energy policy targets. On the basis of a nation-wide noise map containing all <span class="hlt">wind</span> turbines in The Netherlands, it is calculated that 3% of the inhabitants of The Netherlands are currently exposed to noise from <span class="hlt">wind</span> turbines above 28 dB(A) at the faηade. Newly established dose-response relationships indicate that about 1500 of these inhabitants are likely to be severely annoyed inside their dwellings. The available space for new <span class="hlt">wind</span> turbines strongly depends on the noise limit value that will be chosen. This study suggests an outdoor A-weighted reception limit of L den = 45 dB as a <span class="hlt">trade</span>-off between the need for protection against noise annoyance and the feasibility of national targets for renewable energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981IJAmE...2..197F','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981IJAmE...2..197F"><span>Possibilities and limitations of <span class="hlt">wind</span> energy utilisation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Feustel, J.</p> <p>1981-10-01</p> <p>The existing <span class="hlt">wind</span> resource, the most favorable locations, applications, and designs of windpowered generators are reviewed, along with descriptions of current and historic <span class="hlt">wind</span> turbines and lines of research. Coastal <span class="hlt">regions</span>, plains, hill summits, and mountains with funneling <span class="hlt">regions</span> are noted to have the highest annual <span class="hlt">wind</span> averages, with energy densities exceeding the annual solar insolation at average <span class="hlt">wind</span> speeds of 5-7.9 m/sec. Applications for utility-grade power production, for irrigation, for mechanical heat production, and for pumped storage in water towers or reservoirs are mentioned, as well as electrical power production in remote areas and for hydrogen production by electrolysis. Power coefficients are discussed, with attention given to the German Growian 3 MW machine. It is shown that the least economically sound <span class="hlt">wind</span> turbines, the machines with outputs below 100 kW, can vie with diesel plant economics in a good <span class="hlt">wind</span> regime if the <span class="hlt">wind</span> turbine operates for 15 yr.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033267','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033267"><span>Soil slip/debris flow localized by site attributes and <span class="hlt">wind</span>-driven rain in the San Francisco Bay <span class="hlt">region</span> storm of January 1982</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Pike, R.J.; Sobieszczyk, S.</p> <p>2008-01-01</p> <p>GIS analysis at 30-m resolution reveals that effectiveness of slope-destabilizing processes in the San Francisco Bay area varies with compass direction. Nearly half the soil slip/debris flows mapped after the catastrophic rainstorm of 3-5 January 1982 occurred on slopes that face S to WSW, whereas fewer than one-quarter have a northerly aspect. Azimuthal analysis of hillside properties for susceptible terrain near the city of Oakland suggests that the skewed aspect of these landslides primarily reflects vegetation type, ridge and valley alignment, and storm-<span class="hlt">wind</span> direction. Bedrock geology, soil expansivity, and terrain height and gradient also were influential but less so; the role of surface curvature is not wholly resolved. Normalising soil-slip aspect by that of the <span class="hlt">region</span>'s NNW-striking topography shifts the modal azimuth of soil-slip aspect from SW to SE, the direction of origin of <span class="hlt">winds</span> during the 1982 storm-but opposite that of the prevailing WNW <span class="hlt">winds</span>. <span class="hlt">Wind</span> from a constant direction increases rainfall on windward slopes while diminishing it on leeward slopes, generating a modelled difference in hydrologically effective rainfall of up to 2:1 on steep hillsides in the Oakland area. This contrast is consistent with numerical simulations of <span class="hlt">wind</span>-driven rain and with rainfall thresholds for debris-flow activity. We conclude that storm <span class="hlt">winds</span> from the SE in January 1982 raised the vulnerability of the Bay <span class="hlt">region</span>'s many S-facing hillsides, most of which are covered in shallow-rooted shrub and grass that offer minimal resistance to soil slip. <span class="hlt">Wind</span>-driven rainfall also appears to have controlled debris-flow location in a major 1998 storm and probably others. Incorporating this overlooked influence into GIS models of debris-flow likelihood would improve predictions of the hazard in central California and elsewhere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5889628','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5889628"><span>Earliest isotopic evidence in the Maya <span class="hlt">region</span> for animal management and long-distance <span class="hlt">trade</span> at the site of Ceibal, Guatemala</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Emery, Kitty F.; Inomata, Takeshi; Triadan, Daniela; Kamenov, George D.; Krigbaum, John</p> <p>2018-01-01</p> <p>This study uses a multiisotope (carbon, nitrogen, oxygen, and strontium) approach to examine early animal management in the Maya <span class="hlt">region</span>. An analysis of faunal specimens across almost 2,000 years (1000 BC to AD 950) at the site of Ceibal, Guatemala, reveals the earliest evidence for live-<span class="hlt">traded</span> dogs and possible captive-reared taxa in the Americas. These animals may have been procured for ceremonial functions based on their location in the monumental site core, suggesting that animal management and <span class="hlt">trade</span> began in the Maya area to promote special events, activities that were critical in the development of state society. Isotopic evidence for animal captivity at Ceibal reveals that animal management played a greater role in Maya communities than previously believed. PMID:29555750</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.H11H1280C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.H11H1280C"><span>History and geography of virtual water <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Carr, J. A.; D'Odorico, P.; Laio, F.; Ridolfi, L.</p> <p>2012-12-01</p> <p>The global <span class="hlt">trade</span> of goods is associated with a virtual transfer of the water required for their production. The way changes in <span class="hlt">trade</span> affect the virtual redistribution of freshwater resources has been recently documented through the analysis of the virtual water network. It is, however, unclear how these changes are contributed by different types of products and <span class="hlt">regions</span> of the world. Here we show how the global patterns of virtual water transport are contributed by the <span class="hlt">trade</span> of different commodity types, including plant, animal, luxury (e.g., coffee, tea, and alcohol), and other products (non-edible plant and animal products typically used for manufacturing). Major contributors to the virtual water network exhibit different <span class="hlt">trade</span> patterns with regard to these commodity types with the net importers of virtual water relying on the supply of virtual water from a small percentage of the global population. Discrepancies exist among the different commodity networks. Surprisingly, while the total virtual water flux through the network has increased between 1986 and 2008, the global proportions associated with the four commodity groups have remained relatively stable. Here we discuss some major changes in the global patterns of virtual water <span class="hlt">trade</span> with a focus on the increase in <span class="hlt">regional</span> dependencies on foreign virtual water. The increase in virtual water <span class="hlt">trade</span> and the percentage of the total virtual water flux in the network corresponding to plant, animals, luxury, and other commodities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=mechanical+AND+final+AND+year+AND+project&pg=2&id=ED362775','ERIC'); return false;" href="https://eric.ed.gov/?q=mechanical+AND+final+AND+year+AND+project&pg=2&id=ED362775"><span>B-WEST <span class="hlt">Regional</span> Workforce Training Center. Building Workers Entering Skilled <span class="hlt">Trades</span>. Final Report.</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>Portland Community Coll., OR.</p> <p></p> <p>The B-WEST (Building Workers Entering Skilled <span class="hlt">Trades</span>) project was an 18-month demonstration project at a campus of Portland Community College (Oregon). During the B-WEST project, the following programs/components were developed: (1) a model building construction (electrical, mechanical, construction) <span class="hlt">trades</span> program for unemployed and underemployed…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005PhDT.......159L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005PhDT.......159L"><span>Near real time <span class="hlt">wind</span> energy forecasting incorporating <span class="hlt">wind</span> tunnel modeling</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lubitz, William David</p> <p></p> <p>A series of experiments and investigations were carried out to inform the development of a day-ahead <span class="hlt">wind</span> power forecasting system. An experimental near-real time <span class="hlt">wind</span> power forecasting system was designed and constructed that operates on a desktop PC and forecasts 12--48 hours in advance. The system uses model output of the Eta <span class="hlt">regional</span> scale forecast (RSF) to forecast the power production of a <span class="hlt">wind</span> farm in the Altamont Pass, California, USA from 12 to 48 hours in advance. It is of modular construction and designed to also allow diagnostic forecasting using archived RSF data, thereby allowing different methods of completing each forecasting step to be tested and compared using the same input data. <span class="hlt">Wind</span>-tunnel investigations of the effect of <span class="hlt">wind</span> direction and hill geometry on <span class="hlt">wind</span> speed-up above a hill were conducted. Field data from an Altamont Pass, California site was used to evaluate several speed-up prediction algorithms, both with and without <span class="hlt">wind</span> direction adjustment. These algorithms were found to be of limited usefulness for the complex terrain case evaluated. <span class="hlt">Wind</span>-tunnel and numerical simulation-based methods were developed for determining a <span class="hlt">wind</span> farm power curve (the relation between meteorological conditions at a point in the <span class="hlt">wind</span> farm and the power production of the <span class="hlt">wind</span> farm). Both methods, as well as two methods based on fits to historical data, ultimately showed similar levels of accuracy: mean absolute errors predicting power production of 5 to 7 percent of the <span class="hlt">wind</span> farm power capacity. The downscaling of RSF forecast data to the <span class="hlt">wind</span> farm was found to be complicated by the presence of complex terrain. Poor results using the geostrophic drag law and regression methods motivated the development of a database search method that is capable of forecasting not only <span class="hlt">wind</span> speeds but also power production with accuracy better than persistence.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28630802','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28630802"><span>Effects of a <span class="hlt">wind</span> farm installation on the understory bat community of a highly biodiverse tropical <span class="hlt">region</span> in Mexico.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Briones-Salas, Miguel; Lavariega, Mario C; Moreno, Claudia E</p> <p>2017-01-01</p> <p><span class="hlt">Wind</span> energy has rapidly become an important alternative among renewable energies, and it is generally considered clean. However, little is known about its impact at the level of ecological communities, especially in biodiversity hotspots. The Isthmus of Tehuantepec is a highly biodiverse <span class="hlt">region</span> in Mesoamerica, and has the highest potential for generating <span class="hlt">wind</span> energy in Mexico. To assess the effects of installing a <span class="hlt">wind</span> farm on the understory bat community in a landscape of fragmented habitat, we assessed its diversity and composition over four stages of installation (site preparation, construction, and two stages of operation). We captured 919 bats belonging to 22 species. Species richness, functional diversity and phylogenetic diversity decreased during construction and the first stage of operation. However, these components of biodiversity increased during the second stage of operation, and species composition began to resemble that of the site preparation stage. No species considered as sensitive to disturbance was recorded at any stage. This is the first study to reveal the diversity of a Neotropical bat community after <span class="hlt">wind</span> turbines begin to operate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5474091','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5474091"><span>Effects of a <span class="hlt">wind</span> farm installation on the understory bat community of a highly biodiverse tropical <span class="hlt">region</span> in Mexico</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Lavariega, Mario C.; Moreno, Claudia E.</p> <p>2017-01-01</p> <p><span class="hlt">Wind</span> energy has rapidly become an important alternative among renewable energies, and it is generally considered clean. However, little is known about its impact at the level of ecological communities, especially in biodiversity hotspots. The Isthmus of Tehuantepec is a highly biodiverse <span class="hlt">region</span> in Mesoamerica, and has the highest potential for generating <span class="hlt">wind</span> energy in Mexico. To assess the effects of installing a <span class="hlt">wind</span> farm on the understory bat community in a landscape of fragmented habitat, we assessed its diversity and composition over four stages of installation (site preparation, construction, and two stages of operation). We captured 919 bats belonging to 22 species. Species richness, functional diversity and phylogenetic diversity decreased during construction and the first stage of operation. However, these components of biodiversity increased during the second stage of operation, and species composition began to resemble that of the site preparation stage. No species considered as sensitive to disturbance was recorded at any stage. This is the first study to reveal the diversity of a Neotropical bat community after <span class="hlt">wind</span> turbines begin to operate. PMID:28630802</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSA52A..05C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSA52A..05C"><span>Do Transient Electrodynamic Processes Support Enhanced Neutral Mass Densities in Earth's Cusp-<span class="hlt">Region</span> Thermosphere via Divergent Upward <span class="hlt">Winds</span>?</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Conde, M.; Larsen, M. F.; Troyer, R.; Gillespie, D.; Kosch, M.</p> <p>2017-12-01</p> <p>Satellite accelerometer measurements show that Earth's thermosphere contains two substantial and permanent <span class="hlt">regions</span> of enhanced mass density that are located at around 400 km altitude near the footprints of the north and south geomagnetic cusps. The additional mass in these <span class="hlt">regions</span> must be supported against gravity, which requires that similarly localized perturbations must occur in one or more of the other fields (beyond mass density) that appear in the momentum conservation equation for the thermospheric neutral fluid. However more than a decade after the density enhancements were first discovered, there are still no observations of any other corresponding perturbations to terms appearing directly in this equation that would indicate what is supporting the extra mass. To date, most candidate mechanisms involve high-altitude transient electrodynamic heating (at 250 km and above) that drives upwelling and associated horizontal divergence. Indeed, there are very few viable mechanisms that don't ultimately cause substantial localized neutral <span class="hlt">wind</span> perturbations to occur near the density anomalies. Thus, we report here on a study to search for signatures of these localized perturbations in <span class="hlt">winds</span>, using several data sources. These are the WATS instrument that flew aboard the DE-2 spacecraft, the C-REX-1 rocket flight through the CUSP in 2014, and two ground-based Fabry-Perot instruments that are located in Antarctica at latitudes that pass under the geomagnetic cusps - i.e. at McMurdo and South Pole stations. Using these data, we will present both climatological averages and also individual case studies to illustrate what localized signatures occur (if any) in the neutral <span class="hlt">wind</span> fields near the cusp-<span class="hlt">region</span> density anomalies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/928610','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/928610"><span>New England <span class="hlt">Wind</span> Forum: A <span class="hlt">Wind</span> Powering America Project, Volume 1, Issue 4 -- May 2008 (Newsletter)</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>Grace, R. C.; Gifford, J.</p> <p>2008-05-01</p> <p>The New England <span class="hlt">Wind</span> Forum electronic newsletter summarizes the latest news in <span class="hlt">wind</span> energy development activity, markets, education, and policy in the New England <span class="hlt">region</span>. It also features an interview with a key figure influencing New England's <span class="hlt">wind</span> energy development. Volume 1, Issue 4 features an interview with Brian Fairbank, president and CEO of Jiminy Peak Mountain Resort.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017ApJ...846...86B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017ApJ...846...86B"><span>Exploring the Inner Acceleration <span class="hlt">Region</span> of Solar <span class="hlt">Wind</span>: A Study Based on Coronagraphic UV and Visible Light Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bemporad, A.</p> <p>2017-09-01</p> <p>This work combined coronagraphic visible light (VL) and UV data to provide with an unprecedented view of the inner corona where the nascent solar <span class="hlt">wind</span> is accelerated. The UV (H I Lyα) and VL (polarized brightness) images (reconstructed with SOHO/UVCS, LASCO, and Mauna Loa data) have been analyzed with the Doppler dimming technique to provide for the first time daily 2D images of the radial <span class="hlt">wind</span> speed between 1 and 6 R ⊙ over 1 month of observations. Results show that both polar and equatorial <span class="hlt">regions</span> are characterized at the base of the corona by plasma outflows at speeds > 100 km s-1. The plasma is then decelerated within ˜1.5 R ⊙ at the poles and ˜2.0 R ⊙ at the equator, where local minima of the expansion speeds are reached, and gently reaccelerated higher up, reaching speeds typical of fast and slow <span class="hlt">wind</span> components. The mass flux is highly variable with latitude and time at the equator and more uniform and stable over the poles. The polar flow is asymmetric, with speeds above the south pole lower than those above the north pole. A correlation (anticorrelation) between the <span class="hlt">wind</span> speed and its density is found below (above) ˜1.8 R ⊙. The 2D distribution of forces responsible for deceleration and reacceleration of solar <span class="hlt">wind</span> is provided and interpreted in terms of Alfvén waves. These results provide a possible connection between small-scale outflows reported with other instruments at the base of the corona and bulk <span class="hlt">wind</span> flows measured higher up.</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://ntrs.nasa.gov/search.jsp?R=20100002919&hterms=eta&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deta','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20100002919&hterms=eta&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3Deta"><span>3D Modeling of Forbidden Line Emission in the Binary <span class="hlt">Wind</span> Interaction <span class="hlt">Region</span> of Eta Carinae</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Madura, Thomas; Gull, T. R.; Owocki, S.; Okazaki, A. T.; Russell, C. M. P.</p> <p>2010-01-01</p> <p>We present recent work using three-dimensional (3D) Smoothed Particle Hydrodynamics (SPH) simulations to model the high ([Fe III], [Ar III], [Ne III] and [S III]) and low ([Fe II], [Ni II]) ionization forbidden emission lines observed in Eta Carinae using the HST/STIS. These structures are interpreted as the time-averaged, outer extensions of the primary <span class="hlt">wind</span> and the <span class="hlt">wind-wind</span> interaction <span class="hlt">region</span> directly excited by the FUV of the hot companion star of this massive binary system. We discuss how analyzing the results of the 3D SPH simulations and synthetic slit spectra and comparing them to the spectra obtained with the HST/STIS helps us determine the absolute orientation of the binary orbit and helps remove the degeneracy inherent to models based solely on the observed RXTE X-ray light curve. A key point of this work is that spatially resolved observations like those with HST/STIS and comparison to 3D models are necessary to determine the alignment or misalignment of the orbital angular momentum axis with the Homunculus, or correspondingly, the alignment of the orbital plane with the Homunculus skirt.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSA11A2238S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSA11A2238S"><span>Derivation of the horizontal <span class="hlt">wind</span> field in the polar mesopause <span class="hlt">region</span> by using successive images of noctilucent clouds observed by a color digital camera in Iceland</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Suzuki, H.; Yamashita, R.</p> <p>2017-12-01</p> <p>It is important to quantify amplitude of turbulent motion to understand the energy and momentum budgets and distribution of minor constituents in the upper mesosphere. In particular, to know the eddy diffusion coefficient of minor constituents which are locally and impulsively produced by energetic particle precipitations in the polar mesopause is one of the most important subjects in the upper atmospheric science. One of the straight methods to know the amplitude of the eddy motion is to measure the <span class="hlt">wind</span> field with both spatial and temporal domain. However, observation technique satisfying such requirements is limited in this <span class="hlt">region</span>. In this study, derivation of the horizontal <span class="hlt">wind</span> field in the polar mesopause <span class="hlt">region</span> by tracking the motion of noctilucent clouds (NLCs) is performed. NLC is the highest cloud in the Earth which appears in a mesopause <span class="hlt">region</span> during summer season in both polar <span class="hlt">regions</span>. Since the vertical structure of the NLC is sufficiently thin ( within several hundred meters in typical), the apparent horizontal motion observed from ground can be regarded as the result of transportation by the horizontal <span class="hlt">winds</span> at a single altitude. In this presentation, initial results of <span class="hlt">wind</span> field derivation by tracking a motion of noctilucent clouds (NLC) observed by a ground-based color digital camera in Iceland is reported. The procedure for <span class="hlt">wind</span> field estimation consists with 3 steps; (1) projects raw images to a geographical map (2) enhances NLC structures by using FFT method (3) determines horizontal velocity vectors by applying template matching method to two sequential images. In this talk, a result of the <span class="hlt">wind</span> derivation by using successive images of NLC with 3 minutes interval and 1.5h duration observed on the night of Aug 1st, 2013 will be reported as a case study.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009AGUFMGC33B..07S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009AGUFMGC33B..07S"><span>Local and Remote Influences on Vertical <span class="hlt">Wind</span> Shear over the Northern Tropical Atlantic <span class="hlt">Region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Saravanan, R.; Zhu, X.</p> <p>2009-12-01</p> <p>Vertical <span class="hlt">wind</span> shear is one of the most important parameters controlling the frequency and intensity of Atlantic hurricanes. It has been argued that in global warming scenarios, the mechanical effect of changing vertical <span class="hlt">wind</span> shear may even trump the thermodynamic effect of increasing Atlantic sea surface temperatures, when it comes to projected trends in Atlantic hurricane activity. Despite its importance, little is known about the connection between vertical shear in the north Atlantic <span class="hlt">region</span> and the global atmospheric circulation, apart from the well-known positive correlation with El Nino-Southern Oscillation (ENSO). In this study, we analyze the statistical relationship between vertical shear and features of the large-scale circulation such as the distribution of sea surface temperature and vertical motion. We examine whether this relationship is different on interannual timescales associated with ENSO as compared to the decadal timescales associated with the Atlantic Multidecadal Oscillation (AMO). We also investigate how well the global general circulation models manage to simulate the observed vertical shear in this <span class="hlt">region</span>, and its relationship to the large-scale circulation. Our analyses reveal an interesting sensitivity to air-sea coupling in model simulations of vertical shear. Another interesting property of vertical shear, as defined in the context of hurricane studies, is that it is positive definite, rather like precipitation. This means that it has a very nongaussian probability distribution on short timescales. We analyze how this nongaussianity changes when averaged over longer timescales.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20188398','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20188398"><span>Modeling climate change impacts on water <span class="hlt">trading</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Luo, Bin; Maqsood, Imran; Gong, Yazhen</p> <p>2010-04-01</p> <p>This paper presents a new method of evaluating the impacts of climate change on the long-term performance of water <span class="hlt">trading</span> programs, through designing an indicator to measure the mean of periodic water volume that can be released by <span class="hlt">trading</span> through a water-use system. The indicator is computed with a stochastic optimization model which can reflect the random uncertainty of water availability. The developed method was demonstrated in the Swift Current Creek watershed of Prairie Canada under two future scenarios simulated by a Canadian <span class="hlt">Regional</span> Climate Model, in which total water availabilities under future scenarios were estimated using a monthly water balance model. Frequency analysis was performed to obtain the best probability distributions for both observed and simulated water quantity data. Results from the case study indicate that the performance of a <span class="hlt">trading</span> system is highly scenario-dependent in future climate, with <span class="hlt">trading</span> effectiveness highly optimistic or undesirable under different future scenarios. <span class="hlt">Trading</span> effectiveness also largely depends on <span class="hlt">trading</span> costs, with high costs resulting in failure of the <span class="hlt">trading</span> program. (c) 2010 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/grid/wind-sensing-modeling.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/grid/wind-sensing-modeling.html"><span><span class="hlt">Wind</span> Sensing and Modeling | Grid Modernization | NREL</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>Simulation at the <em>turbine</em>, <em><span class="hlt">wind</span></em> plant, and <span class="hlt">regional</span> scales for resource prospecting, resource assessment Sensing and Modeling <em><span class="hlt">Wind</span></em> Sensing and Modeling NREL's <em><span class="hlt">wind</span></em> sensing and modeling work supports the deployment of <em><span class="hlt">wind</span></em>-based generation technologies for all stages of a plant's life, from resource estimates to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/16905715','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/16905715"><span>Glossary on the World <span class="hlt">Trade</span> Organisation and public health: part 2.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Labonte, Ronald; Sanger, Matthew</p> <p>2006-09-01</p> <p>Part 1 of this glossary introduced different health and <span class="hlt">trade</span> arguments, overviewed the history of the World <span class="hlt">Trade</span> Organisation (WTO), defined key "<span class="hlt">trade</span> talk" terms, and reviewed three WTO treaties concerned with <span class="hlt">trade</span> in goods (GATT 1994, the Agreement on Agriculture, and the Agreement on Sanitary and Phytosanitary Measures). Part 2 reviews five more agreements and the growing number of bilateral and <span class="hlt">regional</span> <span class="hlt">trade</span> agreements, and concludes with a commentary on different strategies proposed to ensure that health is not compromised by <span class="hlt">trade</span> liberalization treaties.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19967941','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19967941"><span>Livestock policy and <span class="hlt">trade</span> issues in SADC.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hulman, B</p> <p>2009-03-01</p> <p>As from 2001, the Southern African Development Community (SADC) has embarked on a course to deepen <span class="hlt">regional</span> integration through restructuring. Under the new structure SADC has centralised the coordination of its activities to the Secretariat in Gaborone. The former Sector Coordinating Units have been merged into four directorates, one of which is the Food, Agriculture and Natural Resources (FANR) Directorate, which comprises, amongst others, the Livestock Development Unit (LDU). The LDU, under the aegis of the FANR, formulates policies for <span class="hlt">regional</span> livestock development in order to respond to the objectives of the <span class="hlt">Regional</span> Indicative Strategic Development Plan (RISDP), and which are mainly to: Contribute to improved food security, Promote wealth creation, Enhance rural livelihood, Enhance livestock as a tradable and consumable commodity. Following the launch of the SADC Economic Partnership Agreement (EPA) negotiations, the eight SADC EPA member states identified sanitary and phytosanitary and technical barriers to <span class="hlt">trade</span> to be major <span class="hlt">trade</span> barriers for access to international markets, especially the EU market where standards are normally set beyond international standards. SADC has already brought some of the issues related to beef exports to the OIE <span class="hlt">Regional</span> Commission for Africa as SADC member states feel that a few of the present requirements do not have a scientific basis. The paper discusses the process that the LDU follows in the formulation of policies and strategies in <span class="hlt">regional</span> livestock development with the objective of bolstering intra and extra <span class="hlt">regional</span> <span class="hlt">trade</span> in livestock and livestock products.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016PhDT........66T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016PhDT........66T"><span>Explaining technological change of <span class="hlt">wind</span> power in China and the United States: Roles of energy policies, technological learning, and collaboration</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tang, Tian</p> <p></p> <p>The following dissertation explains how technological change of <span class="hlt">wind</span> power, in terms of cost reduction and performance improvement, is achieved in China and the US through energy policies, technological learning, and collaboration. The objective of this dissertation is to understand how energy policies affect key actors in the power sector to promote renewable energy and achieve cost reductions for climate change mitigation in different institutional arrangements. The dissertation consists of three essays. The first essay examines the learning processes and technological change of <span class="hlt">wind</span> power in China. I integrate collaboration and technological learning theories to model how <span class="hlt">wind</span> technologies are acquired and diffused among various <span class="hlt">wind</span> project participants in China through the Clean Development Mechanism (CDM)--an international carbon <span class="hlt">trade</span> program, and empirically test whether different learning channels lead to cost reduction of <span class="hlt">wind</span> power. Using pooled cross-sectional data of Chinese CDM <span class="hlt">wind</span> projects and spatial econometric models, I find that a <span class="hlt">wind</span> project developer's previous experience (learning-by-doing) and industrywide <span class="hlt">wind</span> project experience (spillover effect) significantly reduce the costs of <span class="hlt">wind</span> power. The spillover effect provides justification for subsidizing users of <span class="hlt">wind</span> technologies so as to offset <span class="hlt">wind</span> farm investors' incentive to free-ride on knowledge spillovers from other <span class="hlt">wind</span> energy investors. The CDM has played such a role in China. Most importantly, this essay provides the first empirical evidence of "learning-by-interacting": CDM also drives <span class="hlt">wind</span> power cost reduction and performance improvement by facilitating technology transfer through collaboration between foreign turbine manufacturers and local <span class="hlt">wind</span> farm developers. The second essay extends this learning framework to the US <span class="hlt">wind</span> power sector, where I examine how state energy policies, restructuring of the electricity market, and learning among actors in <span class="hlt">wind</span> industry lead to</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20050185098','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20050185098"><span>Scientific Impacts of <span class="hlt">Wind</span> Direction Errors</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Liu, W. Timothy; Kim, Seung-Bum; Lee, Tong; Song, Y. Tony; Tang, Wen-Qing; Atlas, Robert</p> <p>2004-01-01</p> <p>An assessment on the scientific impact of random errors in <span class="hlt">wind</span> direction (less than 45 deg) retrieved from space-based observations under weak <span class="hlt">wind</span> (less than 7 m/s ) conditions was made. averages, and these weak <span class="hlt">winds</span> cover most of the tropical, sub-tropical, and coastal oceans. Introduction of these errors in the semi-daily <span class="hlt">winds</span> causes, on average, 5% changes of the yearly mean Ekman and Sverdrup volume transports computed directly from the <span class="hlt">winds</span>, respectively. These poleward movements of water are the main mechanisms to redistribute heat from the warmer tropical <span class="hlt">region</span> to the colder high- latitude <span class="hlt">regions</span>, and they are the major manifestations of the ocean's function in modifying Earth's climate. Simulation by an ocean general circulation model shows that the <span class="hlt">wind</span> errors introduce a 5% error in the meridional heat transport at tropical latitudes. The simulation also shows that the erroneous <span class="hlt">winds</span> cause a pile-up of warm surface water in the eastern tropical Pacific, similar to the conditions during El Nino episode. Similar <span class="hlt">wind</span> directional errors cause significant change in sea-surface temperature and sea-level patterns in coastal oceans in a coastal model simulation. Previous studies have shown that assimilation of scatterometer <span class="hlt">winds</span> improves 3-5 day weather forecasts in the Southern Hemisphere. When directional information below 7 m/s was withheld, approximately 40% of the improvement was lost</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ERL....13b4014E','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ERL....13b4014E"><span>The resilience of Australian <span class="hlt">wind</span> energy to climate change</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Evans, Jason P.; Kay, Merlinde; Prasad, Abhnil; Pitman, Andy</p> <p>2018-02-01</p> <p>The Paris Agreement limits global average temperature rise to 2 °C and commits to pursuing efforts in limiting warming to 1.5 °C above pre-industrial levels. This will require rapid reductions in the emissions of greenhouse gases and the eventual decarbonisation of the global economy. <span class="hlt">Wind</span> energy is an established technology to help achieve emissions reductions, with a cumulative global installed capacity of ~486 GW (2016). Focusing on Australia, we assess the future economic viability of <span class="hlt">wind</span> energy using a 12-member ensemble of high-resolution <span class="hlt">regional</span> climate simulations forced by Coupled Model Intercomparison Project (CMIP) output. We examine both near future (around 2030) and far future (around 2070) changes. Extractable <span class="hlt">wind</span> power changes vary across the continent, though the most spatially coherent change is a small but significant decrease across southern <span class="hlt">regions</span>. The cost of future <span class="hlt">wind</span> energy generation, measured via the Levelised Cost of Energy (LCOE), increases negligibly in the future in <span class="hlt">regions</span> with significant existing installed capacity. Technological developments in <span class="hlt">wind</span> energy generation more than compensate for projected small reductions in <span class="hlt">wind</span>, decreasing the LCOE by around 30%. These developments ensure viability for existing <span class="hlt">wind</span> farms, and enhance the economic viability of proposed <span class="hlt">wind</span> farms in Western Australian and Tasmania. <span class="hlt">Wind</span> energy is therefore a resilient source of electricity over most of Australia and technological innovation entering the market will open new <span class="hlt">regions</span> for energy production in the future.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005nrao.pres...12.','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005nrao.pres...12."><span>Scientists Track Collision of Powerful Stellar <span class="hlt">Winds</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p></p> <p>2005-04-01</p> <p>Astronomers using the National Science Foundation's Very Long Baseline Array (VLBA) radio telescope have tracked the motion of a violent <span class="hlt">region</span> where the powerful <span class="hlt">winds</span> of two giant stars slam into each other. The collision <span class="hlt">region</span> moves as the stars, part of a binary pair, orbit each other, and the precise measurement of its motion was the key to unlocking vital new information about the stars and their <span class="hlt">winds</span>. WR 140 Image Sequence Motion of <span class="hlt">Wind</span> Collision <span class="hlt">Region</span> Graphic superimposes VLBA images of <span class="hlt">wind</span> collision <span class="hlt">region</span> on diagram of orbit of Wolf-Rayet (WR) star and its giant (O) companion. Click on image for larger version (412K) CREDIT: Dougherty et al., NRAO/AUI/NSF In Motion: Shockwave File Animated Gif File AVI file Both stars are much more massive than the Sun -- one about 20 times the mass of the Sun and the other about 50 times the Sun's mass. The 20-solar-mass star is a type called a Wolf-Rayet star, characterized by a very strong <span class="hlt">wind</span> of particles propelled outward from its surface. The more massive star also has a strong outward <span class="hlt">wind</span>, but one less intense than that of the Wolf-Rayet star. The two stars, part of a system named WR 140, circle each other in an elliptical orbit roughly the size of our Solar System. "The spectacular feature of this system is the <span class="hlt">region</span> where the stars' <span class="hlt">winds</span> collide, producing bright radio emission. We have been able to track this collision <span class="hlt">region</span> as it moves with the orbits of the stars," said Sean Dougherty, an astronomer at the Herzberg Institute for Astrophysics in Canada. Dougherty and his colleagues presented their findings in the April 10 edition of the Astrophysical Journal. The supersharp radio "vision" of the continent-wide VLBA allowed the scientists to measure the motion of the <span class="hlt">wind</span> collision <span class="hlt">region</span> and then to determine the details of the stars' orbits and an accurate distance to the system. "Our new calculations of the orbital details and the distance are vitally important to understanding the nature of these</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/964208','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/964208"><span><span class="hlt">Wind</span> for Schools: Developing Education Programs to Train the Next Generation of the <span class="hlt">Wind</span> Energy Workforce</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>Baring-Gould, I.; Flowers, L.; Kelly, M.</p> <p>2009-08-01</p> <p>This paper provides an overview of the <span class="hlt">Wind</span> for Schools project elements, including a description of host and collegiate school curricula developed for <span class="hlt">wind</span> energy and the status of the current projects. The paper also provides focused information on how schools, <span class="hlt">regions</span>, or countries can become involved or implement similar projects to expand the social acceptance and understanding of <span class="hlt">wind</span> energy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2566018','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2566018"><span>Glossary on the World <span class="hlt">Trade</span> Organisation and public health: part 2</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Labonte, Ronald; Sanger, Matthew</p> <p>2006-01-01</p> <p>Part 1 of this glossary introduced different health and <span class="hlt">trade</span> arguments, overviewed the history of the World <span class="hlt">Trade</span> Organisation (WTO), defined key “<span class="hlt">trade</span> talk” terms, and reviewed three WTO treaties concerned with <span class="hlt">trade</span> in goods (GATT 1994, the Agreement on Agriculture, and the Agreement on Sanitary and Phytosanitary Measures). Part 2 reviews five more agreements and the growing number of bilateral and <span class="hlt">regional</span> <span class="hlt">trade</span> agreements, and concludes with a commentary on different strategies proposed to ensure that health is not compromised by <span class="hlt">trade</span> liberalisation treaties. PMID:16905715</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1149654','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1149654"><span><span class="hlt">Wind</span> Resource Assessment of Gujarat (India)</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>Draxl, C.; Purkayastha, A.; Parker, Z.</p> <p></p> <p>India is one of the largest <span class="hlt">wind</span> energy markets in the world. In 1986 Gujarat was the first Indian state to install a <span class="hlt">wind</span> power project. In February 2013, the installed <span class="hlt">wind</span> capacity in Gujarat was 3,093 MW. Due to the uncertainty around existing <span class="hlt">wind</span> energy assessments in India, this analysis uses the Weather Research and Forecasting (WRF) model to simulate the <span class="hlt">wind</span> at current hub heights for one year to provide more precise estimates of <span class="hlt">wind</span> resources in Gujarat. The WRF model allows for accurate simulations of <span class="hlt">winds</span> near the surface and at heights important for <span class="hlt">wind</span> energy purposes.more » While previous resource assessments published <span class="hlt">wind</span> power density, we focus on average <span class="hlt">wind</span> speeds, which can be converted to <span class="hlt">wind</span> power densities by the user with methods of their choice. The <span class="hlt">wind</span> resource estimates in this study show <span class="hlt">regions</span> with average annual <span class="hlt">wind</span> speeds of more than 8 m/s.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19950004596','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19950004596"><span>Comparison of NOAA/NMC stratospheric <span class="hlt">wind</span> analyses with UARS high resolution Doppler Imager <span class="hlt">wind</span> measurements</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Miller, A. J.; Hays, P. B.; Abreu, V.; Long, C.; Kann, D.</p> <p>1994-01-01</p> <p>The NOAA National Weather Service currently derives global stratospheric <span class="hlt">wind</span> analyses via several procedures. The first is the operational data assimilation system that extends from the surface up to about 50 mb and is in process of being tested to about 10 mb. In addition, a balanced <span class="hlt">wind</span> is determined from the available Climate Analysis Center stratospheric height analyses that encompass the 70-0.4 mb <span class="hlt">region</span>. The High Resolution Doppler Imager (HRDI) recently launched as a member of the Upper Atmosphere Research Satellite (UARS) is the first satellite instrument designed to measure <span class="hlt">winds</span> in this stratospheric <span class="hlt">region</span> and, thus, provide a basic evaluation of the NMC derived products. The HRDI accomplishes this by utilizing a triple-etalon Fabry-Perot interferometer that allows one to measure the Doppler shift of O2 absorption and emission features of the atmosphere, from which the <span class="hlt">wind</span> field can be determined.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982STIN...8323947K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982STIN...8323947K"><span>Feasibility study of <span class="hlt">wind</span>-generated electricity for rural applications in southwestern Ohio</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kohring, G. W.</p> <p></p> <p>The parameters associated with domestic production of <span class="hlt">wind</span> generated electricity for direct use by small farms and rural homes in the southwestern Ohio <span class="hlt">region</span> are discussed. The project involves direct utility interfaced electricity generation from a horizontal axis, down-<span class="hlt">wind</span>, fixed pitch, <span class="hlt">wind</span> powered induction generator system. Goals of the project are to determine: the ability to produce useful amounts of domestic <span class="hlt">wind</span> generated electricity in the southwestern Ohio <span class="hlt">region</span>; economic justification for domestic <span class="hlt">wind</span> generated electrical production; and the potential of domestic <span class="hlt">wind</span> generated electricity for reducing dependence on non-renewable energy resources in the southwestern Ohio <span class="hlt">region</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://rosap.ntl.bts.gov/view/dot/16881','DOTNTL'); return false;" href="https://rosap.ntl.bts.gov/view/dot/16881"><span>The U.S.-Brazil-China <span class="hlt">trade</span> and transportation triangle : implications for the southwest <span class="hlt">region</span>.</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>2009-03-01</p> <p>The advent of globalization and more integrated international <span class="hlt">trade</span> has placed increased demands : on transportation infrastructure. This report assesses the impacts of triangular <span class="hlt">trade</span> between and among : the United States, Brazil and China with an ...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=slaves&id=EJ673805','ERIC'); return false;" href="https://eric.ed.gov/?q=slaves&id=EJ673805"><span>The Transatlantic Slave <span class="hlt">Trade</span> and Colonial Chesapeake Slavery.</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>Walsh, Lorena S.</p> <p>2003-01-01</p> <p>Explores the slave <span class="hlt">trade</span> system that brought slaves to the Chesapeake Bay area during the eighteenth century colonial United States. Uses information from the "Trans-Atlantic Slave <span class="hlt">Trade</span>: A Database on CD-ROM" to examine slave routes. Provides information on the origins and distribution of slaves in the Chesapeake Bay <span class="hlt">region</span> and the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGC52B..05L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGC52B..05L"><span>Economically Feasible Potentials for <span class="hlt">Wind</span> Power in China and the US</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lu, X.; McElroy, M. B.; Chris, N. P.; Tchou, J.</p> <p>2011-12-01</p> <p>The present study is intended to explore the economic feasible potentials for <span class="hlt">wind</span> energy in China and the U.S. subject to their policy systems for renewable energy. These two countries were chosen as subject locales for three reasons: first, they are the two largest countries responsible for energy consumption and CO2 emissions; second, these two countries have the largest installed capacities and the fastest annual growth of <span class="hlt">wind</span> power in the world; third, China and the U.S. have adopted two distinct but representative incentive policies to accelerate exploitation of the renewable energy source from <span class="hlt">wind</span>. Investments in large-scale <span class="hlt">wind</span> farms in China gain privileges from the concession policy established under China's Renewable Energy Law. The electricity generated from <span class="hlt">wind</span> can be sold at a guaranteed price for a concession period (typically the first ten operational years of a <span class="hlt">wind</span> farm) to ensure the profitability of the <span class="hlt">wind</span> farm development. The effectiveness of this policy has been evidenced by the swift growth of total installed capacities for <span class="hlt">wind</span> power over the past five years in China. A spatial financial model was developed to evaluate the bus-bar prices of <span class="hlt">wind</span>-generated electricity in China following this <span class="hlt">wind</span> concession policy. The results indicated that <span class="hlt">wind</span> could accommodate all of the demand for electricity projected for 2030 assuming a guaranteed bus-bar price of 7.6 U.S. Cents per kWh over the concession period. It is noteworthy that the prices of <span class="hlt">wind</span>-generated electricity could be as cheap as conventional power generation in the years following the concession period. The power market in the U.S. is more deregulated and electricity is normally <span class="hlt">traded</span> in a bidding process an hour to a day ahead of real time. Accordingly, the market-oriented policy instrument of PTC subsidies was instituted in the U.S. to ensure the competitiveness of <span class="hlt">wind</span> power compared to the conventional power generation in the <span class="hlt">regional</span> power markets. The spatial financial</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/353433-accounting-location-timing-sub-emission-trading-programs-final-report','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/353433-accounting-location-timing-sub-emission-trading-programs-final-report"><span>Accounting for location and timing in NO{sub x} emission <span class="hlt">trading</span> programs. 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>Nichols, A.L.</p> <p>1997-12-01</p> <p>This report describes approaches to designing emission <span class="hlt">trading</span> programs for nitrogen oxides (NO{sub x}) to account for the locations of emission sources. When a <span class="hlt">trading</span> <span class="hlt">region</span> is relatively small, program managers can assume that the location of the sources engaging in <span class="hlt">trades</span> has little or no effect. However, if policy makers extend the program to larger <span class="hlt">regions</span>, this assumption may be questioned. Therefore, EPRI has undertaken a survey of methods for incorporating location considerations into <span class="hlt">trading</span> programs. Application of the best method may help to preserve, and even enhance, the flexibility and savings afforded utilities by emission <span class="hlt">trading</span>.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_17");'>17</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li class="active"><span>19</span></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_19 --> <div id="page_20" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="381"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29555750','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29555750"><span>Earliest isotopic evidence in the Maya <span class="hlt">region</span> for animal management and long-distance <span class="hlt">trade</span> at the site of Ceibal, Guatemala.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Sharpe, Ashley E; Emery, Kitty F; Inomata, Takeshi; Triadan, Daniela; Kamenov, George D; Krigbaum, John</p> <p>2018-04-03</p> <p>This study uses a multiisotope (carbon, nitrogen, oxygen, and strontium) approach to examine early animal management in the Maya <span class="hlt">region</span>. An analysis of faunal specimens across almost 2,000 years (1000 BC to AD 950) at the site of Ceibal, Guatemala, reveals the earliest evidence for live-<span class="hlt">traded</span> dogs and possible captive-reared taxa in the Americas. These animals may have been procured for ceremonial functions based on their location in the monumental site core, suggesting that animal management and <span class="hlt">trade</span> began in the Maya area to promote special events, activities that were critical in the development of state society. Isotopic evidence for animal captivity at Ceibal reveals that animal management played a greater role in Maya communities than previously believed. Copyright © 2018 the Author(s). Published by PNAS.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5028745','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=5028745"><span><span class="hlt">Regional</span> drivers of clutch loss reveal important <span class="hlt">trade</span>-offs for beach-nesting birds</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Schlacher, Thomas A.; Weston, Michael A.; Huijbers, Chantal M.; Anderson, Chris; Gilby, Ben L.; Olds, Andrew D.; Connolly, Rod M.; Schoeman, David S.</p> <p>2016-01-01</p> <p>Coastal birds are critical ecosystem constituents on sandy shores, yet are threatened by depressed reproductive success resulting from direct and indirect anthropogenic and natural pressures. Few studies examine clutch fate across the wide range of environments experienced by birds; instead, most focus at the small site scale. We examine survival of model shorebird clutches as an index of true clutch survival at a <span class="hlt">regional</span> scale (∼200 km), encompassing a variety of geomorphologies, predator communities, and human use regimes in southeast Queensland, Australia. Of the 132 model nests deployed and monitored with cameras, 45 (34%) survived the experimental exposure period. Thirty-five (27%) were lost to flooding, 32 (24%) were depredated, nine (7%) buried by sand, seven (5%) destroyed by people, three (2%) failed by unknown causes, and one (1%) was destroyed by a dog. Clutch fate differed substantially among <span class="hlt">regions</span>, particularly with respect to losses from flooding and predation. ‘Topographic’ exposure was the main driver of mortality of nests placed close to the drift line near the base of dunes, which were lost to waves (particularly during storms) and to a lesser extent depredation. Predators determined the fate of clutches not lost to waves, with the depredation probability largely influenced by <span class="hlt">region</span>. Depredation probability declined as nests were backed by higher dunes and were placed closer to vegetation. This study emphasizes the scale at which clutch fate and survival varies within a <span class="hlt">regional</span> context, the prominence of corvids as egg predators, the significant role of flooding as a source of nest loss, and the multiple <span class="hlt">trade</span>-offs faced by beach-nesting birds and those that manage them. PMID:27672510</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/27672510','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/27672510"><span><span class="hlt">Regional</span> drivers of clutch loss reveal important <span class="hlt">trade</span>-offs for beach-nesting birds.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Maslo, Brooke; Schlacher, Thomas A; Weston, Michael A; Huijbers, Chantal M; Anderson, Chris; Gilby, Ben L; Olds, Andrew D; Connolly, Rod M; Schoeman, David S</p> <p>2016-01-01</p> <p>Coastal birds are critical ecosystem constituents on sandy shores, yet are threatened by depressed reproductive success resulting from direct and indirect anthropogenic and natural pressures. Few studies examine clutch fate across the wide range of environments experienced by birds; instead, most focus at the small site scale. We examine survival of model shorebird clutches as an index of true clutch survival at a <span class="hlt">regional</span> scale (∼200 km), encompassing a variety of geomorphologies, predator communities, and human use regimes in southeast Queensland, Australia. Of the 132 model nests deployed and monitored with cameras, 45 (34%) survived the experimental exposure period. Thirty-five (27%) were lost to flooding, 32 (24%) were depredated, nine (7%) buried by sand, seven (5%) destroyed by people, three (2%) failed by unknown causes, and one (1%) was destroyed by a dog. Clutch fate differed substantially among <span class="hlt">regions</span>, particularly with respect to losses from flooding and predation. 'Topographic' exposure was the main driver of mortality of nests placed close to the drift line near the base of dunes, which were lost to waves (particularly during storms) and to a lesser extent depredation. Predators determined the fate of clutches not lost to waves, with the depredation probability largely influenced by <span class="hlt">region</span>. Depredation probability declined as nests were backed by higher dunes and were placed closer to vegetation. This study emphasizes the scale at which clutch fate and survival varies within a <span class="hlt">regional</span> context, the prominence of corvids as egg predators, the significant role of flooding as a source of nest loss, and the multiple <span class="hlt">trade</span>-offs faced by beach-nesting birds and those that manage them.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013APS..MAR.V1189B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013APS..MAR.V1189B"><span>A ``Cyber <span class="hlt">Wind</span> Facility'' for HPC <span class="hlt">Wind</span> Turbine Field Experiments</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; Paterson, Eric; Schmitz, Sven; Campbell, Robert; Vijayakumar, Ganesh; Lavely, Adam; Jayaraman, Balaji; Nandi, Tarak; Jha, Pankaj; Dunbar, Alex; Motta-Mena, Javier; Craven, Brent; Haupt, Sue</p> <p>2013-03-01</p> <p>The Penn State ``Cyber <span class="hlt">Wind</span> Facility'' (CWF) is a high-fidelity multi-scale high performance computing (HPC) environment in which ``cyber field experiments'' are designed and ``cyber data'' collected from <span class="hlt">wind</span> turbines operating within the atmospheric boundary layer (ABL) environment. Conceptually the ``facility'' is akin to a high-tech <span class="hlt">wind</span> tunnel with controlled physical environment, but unlike a <span class="hlt">wind</span> tunnel it replicates commercial-scale <span class="hlt">wind</span> turbines operating in the field and forced by true atmospheric turbulence with controlled stability state. The CWF is created from state-of-the-art high-accuracy technology geometry and grid design and numerical methods, and with high-resolution simulation strategies that blend unsteady RANS near the surface with high fidelity large-eddy simulation (LES) in separated boundary layer, blade and rotor wake <span class="hlt">regions</span>, embedded within high-resolution LES of the ABL. CWF experiments complement physical field facility experiments that can capture wider ranges of meteorological events, but with minimal control over the environment and with very small numbers of sensors at low spatial resolution. I shall report on the first CWF experiments aimed at dynamical interactions between ABL turbulence and space-time <span class="hlt">wind</span> turbine loadings. Supported by DOE and NSF.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29679175','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29679175"><span>Numerical simulation of <span class="hlt">wind</span>-sand movement in the reversed flow <span class="hlt">region</span> of a sand dune with a bridge built downstream.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Wei; Huang, Ning; Xu, Bin; Wang, Wenbo</p> <p>2018-04-23</p> <p>A bridge built inside the reversed flow <span class="hlt">region</span> of a sand dune will change the characteristics of <span class="hlt">wind</span>-sand movement in this <span class="hlt">region</span>. The Reynolds-averaged Navier-Stokes simulation and discrete particle tracing are used to simulate the <span class="hlt">wind</span>-sand movement around a sand dune with a bridge built inside the reversed <span class="hlt">region</span>. Three cases with different bridge positions are studied. The results show that 1) compared with the isolated dune case, a tall bridge built at the leeward toe leads to an increase in the deposition rate on the leeward slope and a longer reversed flow <span class="hlt">region</span> downstream of the sand dune; meanwhile, the high speed of crosswind on the bridge indicates that some measures should be taken to protect trains from strong crosswind; 2) a low bridge at the leeward toe has little effect on the sand deposition and reversed flow <span class="hlt">region</span> of the dune; however, low sand transport rate and crosswind speed on the bridge show that anti-crosswind/sand measures should be taken according to the actual situation and 3) a low bridge on the leeward slope has little effect on the length of reversed flow <span class="hlt">region</span>, however, high crosswind speed and sand flux on the bridge reveal the need of anti-crosswind/sand measures on the bridge. Moreover, the bridges in the reversed flow <span class="hlt">region</span> increase the sand flux near the leeward crest; as a result, the moving patterns of the sand dune are changed.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29672852','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29672852"><span>Responses of insect herbivores and their food plants to <span class="hlt">wind</span> exposure and the importance of predation risk.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Cong; Biere, Arjen; Gols, Rieta; Halfwerk, Wouter; van Oers, Kees; Harvey, Jeffrey A</p> <p>2018-04-19</p> <p><span class="hlt">Wind</span> is an important abiotic factor that influences an array of biological processes, but it is rarely considered in studies on plant-herbivore interactions. Here, we tested whether <span class="hlt">wind</span> exposure could directly or indirectly affect the performance of two insect herbivores, Plutella xylostella and Pieris brassicae, feeding on Brassica nigra plants. In a greenhouse study using a factorial design, B. nigra plants were exposed to different <span class="hlt">wind</span> regimes generated by fans before and after caterpillars were introduced on plants in an attempt to separate the effects of direct and indirect <span class="hlt">wind</span> exposure on herbivores. <span class="hlt">Wind</span> exposure delayed flowering, decreased plant height and increased leaf concentrations of amino acids and glucosinolates. Plant-mediated effects of <span class="hlt">wind</span> on herbivores, that is effects of exposure of plants to <span class="hlt">wind</span> prior to herbivore feeding, were generally small. However, development time of both herbivores was extended and adult body mass of P. xylostella was reduced when they were directly exposed to <span class="hlt">wind</span>. By contrast, <span class="hlt">wind</span>-exposed adult P. brassicae butterflies were significantly larger, revealing a <span class="hlt">trade</span>-off between development time and adult size. Based on these results, we conducted a behavioural experiment to study preference by an avian predator, the great tit (Parus major) for last instar P. brassicae caterpillars on plants that were exposed to either control (no <span class="hlt">wind</span>) or <span class="hlt">wind</span> (fan-exposed) treatments. Tits captured significantly more caterpillars on still than on <span class="hlt">wind</span>-exposed plants. Our results suggest that P. brassicae caterpillars are able to perceive the abiotic environment and to <span class="hlt">trade</span> off the costs of extended development time against the benefits of increased size depending on the perceived risk of predation mediated by <span class="hlt">wind</span> exposure. Such adaptive phenotypic plasticity in insects has not yet been described in response to <span class="hlt">wind</span> exposure. © 2018 The Author. Journal of Animal Ecology published by John Wiley & Sons Ltd on behalf of</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1050033','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1050033"><span>Western <span class="hlt">Wind</span> Strategy: Addressing Critical Issues for <span class="hlt">Wind</span> Deployment</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>Douglas Larson; Thomas Carr</p> <p>2012-03-30</p> <p>The goal of the Western <span class="hlt">Wind</span> Strategy project was to help remove critical barriers to <span class="hlt">wind</span> development in the Western Interconnection. The four stated objectives of this project were to: (1) identify the barriers, particularly barriers to the operational integration of renewables and barriers identified by load-serving entities (LSEs) that will be buying <span class="hlt">wind</span> generation, (2) communicate the barriers to state officials, (3) create a collaborative process to address those barriers with the Western states, utilities and the renewable industry, and (4) provide a role model for other <span class="hlt">regions</span>. The project has been on the forefront of identifying and informingmore » state policy makers and utility regulators of critical issues related to <span class="hlt">wind</span> energy and the integration of variable generation. The project has been a critical component in the efforts of states to push forward important reforms and innovations that will enable states to meet their renewable energy goals and lower the cost to consumers of integrating variable generation.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25104384','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25104384"><span>Oceanography. Centennial changes in North Pacific anoxia linked to tropical <span class="hlt">trade</span> <span class="hlt">winds</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Deutsch, Curtis; Berelson, William; Thunell, Robert; Weber, Thomas; Tems, Caitlin; McManus, James; Crusius, John; Ito, Taka; Baumgartner, Timothy; Ferreira, Vicente; Mey, Jacob; van Geen, Alexander</p> <p>2014-08-08</p> <p>Climate warming is expected to reduce oxygen (O2) supply to the ocean and expand its oxygen minimum zones (OMZs). We reconstructed variations in the extent of North Pacific anoxia since 1850 using a geochemical proxy for denitrification (δ(15)N) from multiple sediment cores. Increasing δ(15)N since ~1990 records an expansion of anoxia, consistent with observed O2 trends. However, this was preceded by a longer declining δ(15)N trend that implies that the anoxic zone was shrinking for most of the 20th century. Both periods can be explained by changes in <span class="hlt">winds</span> over the tropical Pacific that drive upwelling, biological productivity, and O2 demand within the OMZ. If equatorial Pacific <span class="hlt">winds</span> resume their predicted weakening trend, the ocean's largest anoxic zone will contract despite a global O2 decline. Copyright © 2014, American Association for the Advancement of Science.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20140013100','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20140013100"><span>Resource Prospector Lander: Architecture and <span class="hlt">Trade</span> Studies</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Moore, Josh; Calvert, Derek; Frady, Greg; Chavers, Greg; Wayne, Andrew; Hull, Patrick; Lowery, Eric; Farmer, Jeff; Trinh, Huu; Rojdev, Kristina; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20140013100'); toggleEditAbsImage('author_20140013100_show'); toggleEditAbsImage('author_20140013100_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20140013100_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20140013100_hide"></p> <p>2014-01-01</p> <p>NASA's Resource Prospector (RP) is a multi-center and multi-institution collaborative project to investigate the polar <span class="hlt">regions</span> of the Moon in search of volatiles. The mission is rated Class D and is approximately 10 days. The RP vehicle comprises three elements: the Lander, the Rover, and the Payload. The Payload is housed on the Rover and the Rover is on top of the Lander. The focus of this paper is on the Lander element for the RP vehicle. The design of the Lander was requirements driven and focused on a low-cost approach. To arrive at the final configuration, several <span class="hlt">trade</span> studies were conducted. Of those <span class="hlt">trade</span> studies, there were six primary <span class="hlt">trade</span> studies that were instrumental in determining the final design. This paper will discuss each of these <span class="hlt">trades</span> in further detail and show how these <span class="hlt">trades</span> led to the final architecture of the RP Lander.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23019353','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23019353"><span>Saturation <span class="hlt">wind</span> power potential and its implications for <span class="hlt">wind</span> energy.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Jacobson, Mark Z; Archer, Cristina L</p> <p>2012-09-25</p> <p><span class="hlt">Wind</span> turbines convert kinetic to electrical energy, which returns to the atmosphere as heat to regenerate some potential and kinetic energy. As the number of <span class="hlt">wind</span> turbines increases over large geographic <span class="hlt">regions</span>, power extraction first increases linearly, but then converges to a saturation potential not identified previously from physical principles or turbine properties. These saturation potentials are >250 terawatts (TW) at 100 m globally, approximately 80 TW at 100 m over land plus coastal ocean outside Antarctica, and approximately 380 TW at 10 km in the jet streams. Thus, there is no fundamental barrier to obtaining half (approximately 5.75 TW) or several times the world's all-purpose power from <span class="hlt">wind</span> in a 2030 clean-energy economy.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19810007124','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19810007124"><span>Determination of <span class="hlt">wind</span> from NIMBUS 6 satellite sounding data</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Carle, W. E.; Scoggins, J. R.</p> <p>1981-01-01</p> <p>Objective methods of computing upper level and surface <span class="hlt">wind</span> fields from NIMBUS 6 satellite sounding data are developed. These methods are evaluated by comparing satellite derived and rawinsonde <span class="hlt">wind</span> fields on gridded constant pressure charts in four geographical <span class="hlt">regions</span>. Satellite-derived and hourly observed surface <span class="hlt">wind</span> fields are compared. Results indicate that the best satellite-derived <span class="hlt">wind</span> on constant pressure charts is a geostrophic <span class="hlt">wind</span> derived from highly smoothed fields of geopotential height. Satellite-derived <span class="hlt">winds</span> computed in this manner and rawinsonde <span class="hlt">winds</span> show similar circulation patterns except in areas of small height gradients. Magnitudes of the standard deviation of the differences between satellite derived and rawinsonde <span class="hlt">wind</span> speeds range from approximately 3 to 12 m/sec on constant pressure charts and peak at the jet stream level. Fields of satellite-derived surface <span class="hlt">wind</span> computed with the logarithmic <span class="hlt">wind</span> law agree well with fields of observed surface <span class="hlt">wind</span> in most <span class="hlt">regions</span>. Magnitudes of the standard deviation of the differences in surface <span class="hlt">wind</span> speed range from approximately 2 to 4 m/sec, and satellite derived surface <span class="hlt">winds</span> are able to depict flow across a cold front and around a low pressure center.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29738231','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29738231"><span>Virtual CO2 Emission Flows in the Global Electricity <span class="hlt">Trade</span> Network.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Qu, Shen; Li, Yun; Liang, Sai; Yuan, Jiahai; Xu, Ming</p> <p>2018-06-05</p> <p>Quantifying greenhouse gas emissions due to electricity consumption is crucial for climate mitigation in the electric power sector. Current practices primarily use production-based emission factors to quantify emissions for electricity consumption, assuming production and consumption of electricity take place within the same <span class="hlt">region</span>. The increasingly intensified cross-border electricity <span class="hlt">trade</span> complicates the accounting for emissions of electricity consumption. This study employs a network approach to account for the flows in the whole electricity <span class="hlt">trade</span> network to estimate CO 2 emissions of electricity consumption for 137 major countries/<span class="hlt">regions</span> in 2014. Results show that in some countries, especially those in Europe and Southern Africa, the impacts of electricity <span class="hlt">trade</span> on the estimation of emission factors and embodied emissions are significant. The changes made to emission factors by considering intergrid electricity <span class="hlt">trade</span> can have significant implications for emission accounting and climate mitigation when multiplied by total electricity consumption of the corresponding countries/<span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19740008686','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19740008686"><span>NASA presentation. [<span class="hlt">wind</span> energy conversion systems planning</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Thomas, R. L.</p> <p>1973-01-01</p> <p>The development of a <span class="hlt">wind</span> energy system is outlined that supplies reliable energy at a cost competitive with other energy systems. A government directed industry program with strong university support is recommended that includes meteorological studies to estimate <span class="hlt">wind</span> energy potentials and determines favorable <span class="hlt">regions</span> and sites for <span class="hlt">wind</span> power installations. Key phases of the overall program are <span class="hlt">wind</span> energy conversion systems, meteorological <span class="hlt">wind</span> studies, energy storage systems, and environmental impact studies. Performance testing with a prototype <span class="hlt">wind</span> energy conversion and storage system is projected for Fiscal 1977.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/26075','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/26075"><span>The <span class="hlt">Wind</span> River Arboretum 1912-1956.</span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Roy R. Silen; Leonard R. Woike</p> <p>1959-01-01</p> <p><span class="hlt">Wind</span> River Arboretum, located in the <span class="hlt">Wind</span> River valley near Carson, Wash., was established in 1912 with the planting of a few species of introduced trees on stump land adjacent to the <span class="hlt">Wind</span> River Nursery. It is the oldest arboretum in the Northwest and ranks among the earliest forestry projects of an experimental nature still in existence in the <span class="hlt">region</span>. The initial...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/827201','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/827201"><span><span class="hlt">Wind</span> Generation Feasibility Study in Bethel, AK</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>Tom Humphrey, YKHC; Lance Kincaid, EMCOR Energy & Technologies</p> <p>2004-07-31</p> <p>This report studies the <span class="hlt">wind</span> resources in the Yukon-Kuskokwim Health Corporation (YKHC) <span class="hlt">region</span>, located in southwestern Alaska, and the applicability of <span class="hlt">wind</span> generation technologies to YKHC facilities.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AtmEn.139...98C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AtmEn.139...98C"><span>Microscale anthropogenic pollution modelling in a small tropical island during weak <span class="hlt">trade</span> <span class="hlt">winds</span>: Lagrangian particle dispersion simulations using real nested LES meteorological fields</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Cécé, Raphaël; Bernard, Didier; Brioude, Jérome; Zahibo, Narcisse</p> <p>2016-08-01</p> <p>Tropical islands are characterized by thermal and orographical forcings which may generate microscale air mass circulations. The Lesser Antilles Arc includes small tropical islands (width lower than 50 km) where a total of one-and-a-half million people live. Air quality over this <span class="hlt">region</span> is affected by anthropogenic and volcanic emissions, or saharan dust. To reduce risks for the population health, the atmospheric dispersion of emitted pollutants must be predicted. In this study, the dispersion of anthropogenic nitrogen oxides (NOx) is numerically modelled over the densely populated area of the Guadeloupe archipelago under weak <span class="hlt">trade</span> <span class="hlt">winds</span>, during a typical case of severe pollution. The main goal is to analyze how microscale resolutions affect air pollution in a small tropical island. Three resolutions of domain grid are selected: 1 km, 333 m and 111 m. The Weather Research and Forecasting model (WRF) is used to produce real nested microscale meteorological fields. Then the weather outputs initialize the Lagrangian Particle Dispersion Model (FLEXPART). The forward simulations of a power plant plume showed good ability to reproduce nocturnal peaks recorded by an urban air quality station. The increase in resolution resulted in an improvement of model sensitivity. The nesting to subkilometer grids helped to reduce an overestimation bias mainly because the LES domains better simulate the turbulent motions governing nocturnal flows. For peaks observed at two air quality stations, the backward sensitivity outputs identified realistic sources of NOx in the area. The increase in resolution produced a sharper inverse plume with a more accurate source area. This study showed the first application of the FLEXPART-WRF model to microscale resolutions. Overall, the coupling model WRF-LES-FLEXPART is useful to simulate the pollutant dispersion during a real case of calm <span class="hlt">wind</span> regime over a complex terrain area. The forward and backward simulation results showed clearly that the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/19167056','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/19167056"><span><span class="hlt">Trade</span> and health: an agenda for action.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Smith, Richard D; Lee, Kelley; Drager, Nick</p> <p>2009-02-28</p> <p>The processes of contemporary globalisation are creating ever-closer ties between individuals and populations across different countries. The health of a population, and the systems in place to deliver health care, are affected increasingly by factors beyond the population and health system. The Lancet's Series on <span class="hlt">trade</span> and health has provided an overview of these links between international <span class="hlt">trade</span>, <span class="hlt">trade</span> liberalisation, and health, and raised the key issues that face the health community. In this final paper in the Series, we call for a substantial and sustained effort by those within the health profession to engage with issues of <span class="hlt">trade</span>, to strengthen institutional capacity in this area, and to place health higher on the agenda of <span class="hlt">trade</span> negotiations. The rapid rise of <span class="hlt">trade</span> agreements and treaties, as well as <span class="hlt">trade</span> that occurs beyond these institutional boundaries, means that further action is required by a range of actors, including WHO, the World Bank, the World <span class="hlt">Trade</span> Organization (WTO), <span class="hlt">regional</span> agencies, foundations, national governments, civil society, non-governmental organisations, and academics. The stewardship of a domestic health system in the 21st century requires a sophisticated understanding of how <span class="hlt">trade</span> affects, and will affect, a country's health system and policy, to optimise opportunities to benefit health and health care while minimising the risks posed though the assertion of health goals in <span class="hlt">trade</span> policy. To acheive this will place a premium on all those engaged in health to understand the importance of <span class="hlt">trade</span> and to engage with their counterparts involved in <span class="hlt">trade</span> and <span class="hlt">trade</span> policy. We hope that this Series has prompted the reader to become involved in these efforts.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2726935','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=2726935"><span><span class="hlt">Trade</span> and health: an agenda for action</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Smith, Richard D; Lee, Kelley; Drager, Nick</p> <p>2009-01-01</p> <p>The processes of contemporary globalisation are creating ever-closer ties between individuals and populations across different countries. The health of a population, and the systems in place to deliver health care, are affected increasingly by factors beyond the population and health system. The Lancet’s Series on <span class="hlt">trade</span> and health has provided an overview of these links between international <span class="hlt">trade</span>, <span class="hlt">trade</span> liberalisation, and health, and raised the key issues that face the health community. In this final paper in the Series, we call for a substantial and sustained effort by those within the health profession to engage with issues of <span class="hlt">trade</span>, to strengthen institutional capacity in this area, and to place health higher on the agenda of <span class="hlt">trade</span> negotiations. The rapid rise of <span class="hlt">trade</span> agreements and treaties, as well as <span class="hlt">trade</span> that occurs beyond these institutional boundaries, means that further action is required by a range of actors, including WHO, the World Bank, the World <span class="hlt">Trade</span> Organization (WTO), <span class="hlt">regional</span> agencies, foundations, national governments, civil society, non-governmental organisations, and academics. The stewardship of a domestic health system in the 21st century requires a sophisticated understanding of how <span class="hlt">trade</span> affects, and will affect, a country’s health system and policy, to optimise opportunities to benefit health and health care while minimising the risks posed though the assertion of health goals in <span class="hlt">trade</span> policy. To acheive this will place a premium on all those engaged in health to understand the importance of <span class="hlt">trade</span> and to engage with their counterparts involved in <span class="hlt">trade</span> and <span class="hlt">trade</span> policy. We hope that this Series has prompted the reader to become involved in these efforts. PMID:19167056</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26002998','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26002998"><span>Understanding the poultry <span class="hlt">trade</span> network in Kenya: Implications for <span class="hlt">regional</span> disease prevention and control.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>McCarron, Margaret; Munyua, Peninah; Cheng, Po-Yung; Manga, Thomas; Wanjohi, Cathryn; Moen, Ann; Mounts, Anthony; Katz, Mark A</p> <p>2015-07-01</p> <p>Infectious diseases in poultry can spread quickly and lead to huge economic losses. In the past decade, on multiple continents, the accelerated spread of highly pathogenic avian Influenza A (H5N1) virus, often through informal <span class="hlt">trade</span> networks, has led to the death and culling of hundreds of millions of poultry. Endemic poultry diseases like Newcastle disease and fowl typhoid can also be devastating in many parts of the world. Understanding <span class="hlt">trade</span> networks in unregulated systems can inform policy decisions concerning disease prevention and containment. From June to December 2008 we conducted a cross-sectional survey of backyard farmers, market traders, and middlemen in 5/8 provinces in Kenya. We administered a standardized questionnaire to each type of actor using convenience, random, snowball, and systematic sampling. Questionnaires addressed frequency, volume, and geography of <span class="hlt">trade</span>, as well as biosecurity practices. We created a network diagram identifying the most important locations for <span class="hlt">trade</span>. Of 380 respondents, 51% were backyard farmers, 24% were middlemen and 25% were market traders. Half (50%) of backyard farmers said they raised poultry both for household consumption and for sale. Compared to market traders, middlemen bought their poultry from a greater number of villages (median 4.2 villages for middlemen vs. 1.9 for market traders). Traders were most likely to purchase poultry from backyard farmers. Of the backyard farmers who sold poultry, 51% [CI 40-63] reported selling poultry to market traders, and 54% [CI 44-63] sold to middlemen. Middlemen moved the largest volume of poultry on a weekly basis (median purchases: 187 birds/week [IQR 206]; median sales: 188 birds/week [IQR 412.5]). The highest numbers of birds were <span class="hlt">traded</span> in Nairobi - Kenya's capital city. Nairobi was the most prominent <span class="hlt">trading</span> node in the network (61 degrees of centrality). Many smaller sub-networks existed as a result of clustered local <span class="hlt">trade</span>. Market traders were also integral to the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/18181453','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/18181453"><span>Health risks of including alcohol and tobacco in PICTA free <span class="hlt">trade</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hill, Linda</p> <p>2004-03-01</p> <p>In April 2005 Pacific Forum leaders will decide whether to include alcohol and tobacco in the Pacific Island Countries <span class="hlt">Trade</span> Agreement (PICTA). This article presents arguments for keeping alcohol out of <span class="hlt">regional</span> free <span class="hlt">trade</span> agreements. Inclusion will allow <span class="hlt">regional</span> rationalisation of production, increased alcohol availability, competition and marketing, and lower prices. These <span class="hlt">trade</span> goals are inappropriate for alcohol and tobacco. Pacific public health organisations are concerned that official advice has focused on fiscal impacts, not health and social impacts. The World Health Organization has identified alcohol as the leading factor in injury and disease for low-mortality developing countries. Effective policies to reduce alcohol related harm include restrictions on availability, as well as excise taxes affecting price. Under <span class="hlt">trade</span> agreements elsewhere, national alcohol policies have been challenged as 'non-tariff barriers to <span class="hlt">trade</span>'. Hazardous drinking is of increasingly concern in the Pacific and decisions about alcohol should not reflect commercial interests.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_18");'>18</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li class="active"><span>20</span></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_20 --> <div id="page_21" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="401"> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.A21E0222S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.A21E0222S"><span>United States Offshore <span class="hlt">Wind</span> Resource Assessment</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Schwartz, M.; Haymes, S.; Heimiller, D.</p> <p>2008-12-01</p> <p>The utilization of the offshore <span class="hlt">wind</span> resource will be necessary if the United States is to meet the goal of having 20% of its electricity generated by <span class="hlt">wind</span> power because many of the electrical load centers in the country are located along the coastlines. The United States Department of Energy, through its National Renewable Energy Laboratory (NREL), has supported an ongoing project to assess the <span class="hlt">wind</span> resource for the offshore <span class="hlt">regions</span> of the contiguous United States including the Great Lakes. Final offshore maps with a horizontal resolution of 200 meters (m) have been completed for Texas, Louisiana, Georgia, northern New England, and the Great Lakes. The ocean <span class="hlt">wind</span> resource maps extend from the coastline to 50 nautical miles (nm) offshore. The Great Lake maps show the resource for all of the individual lakes. These maps depict the <span class="hlt">wind</span> resource at 50 m above the water as classes of <span class="hlt">wind</span> power density. Class 1 represents the lowest available <span class="hlt">wind</span> resource, while Class 7 is the highest resource. Areas with Class 5 and higher <span class="hlt">wind</span> resource can be economical for offshore project development. As offshore <span class="hlt">wind</span> turbine technology improves, areas with Class 4 and higher resource should become economically viable. The <span class="hlt">wind</span> resource maps are generated using output from a modified numerical weather prediction model combined with a <span class="hlt">wind</span> flow model. The preliminary modeling is performed by AWS Truewind under subcontract to NREL. The preliminary model estimates are sent to NREL to be validated. NREL validates the preliminary estimates by comparing 50 m model data to available measurements that are extrapolated to 50 m. The validation results are used to modify the preliminary map and produce the final resource map. The sources of offshore <span class="hlt">wind</span> measurement data include buoys, automated stations, lighthouses, and satellite- derived ocean <span class="hlt">wind</span> speed data. The <span class="hlt">wind</span> electric potential is represented as Megawatts (MW) of potential installed capacity and is based on the square</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29409591','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29409591"><span>Optimal supplementary frequency controller design using the <span class="hlt">wind</span> farm frequency model and controller parameters stability <span class="hlt">region</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Toulabi, Mohammadreza; Bahrami, Shahab; Ranjbar, Ali Mohammad</p> <p>2018-03-01</p> <p>In most of the existing studies, the frequency response in the variable speed <span class="hlt">wind</span> turbines (VSWTs) is simply realized by changing the torque set-point via appropriate inputs such as frequency deviations signal. However, effective dynamics and systematic process design have not been comprehensively discussed yet. Accordingly, this paper proposes a proportional-derivative frequency controller and investigates its performance in a <span class="hlt">wind</span> farm consisting of several VSWTs. A band-pass filter is deployed before the proposed controller to avoid responding to either steady state frequency deviations or high rate of change of frequency. To design the controller, the frequency model of the <span class="hlt">wind</span> farm is first characterized. The proposed controller is then designed based on the obtained open loop system. The stability <span class="hlt">region</span> associated with the controller parameters is analytically determined by decomposing the closed-loop system's characteristic polynomial into the odd and even parts. The performance of the proposed controller is evaluated through extensive simulations in MATLAB/Simulink environment in a power system comprising a high penetration of VSWTs equipped with the proposed controller. Finally, based on the obtained feasible area and appropriate objective function, the optimal values associated with the controller parameters are determined using the genetic algorithm (GA). Copyright © 2018 ISA. Published by Elsevier Ltd. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20160001311','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20160001311"><span>Soil Dust Aerosols and <span class="hlt">Wind</span> as Predictors of Seasonal Meningitis Incidence in Niger</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Perez Garcia Pando, Carlos; Stanton, Michelle C.; Diggle, Peter J.; Trzaska, Sylwia; Miller, Ron L.; Perlwitz, Jan P.; Baldasano, Jose M.; Cuevas, Emilio; Ceccato, Pietro; Yaka, Pascal; <a style="text-decoration: none; " href="javascript:void(0); " onClick="displayelement('author_20160001311'); toggleEditAbsImage('author_20160001311_show'); toggleEditAbsImage('author_20160001311_hide'); "> <img style="display:inline; width:12px; height:12px; " src="images/arrow-up.gif" width="12" height="12" border="0" alt="hide" id="author_20160001311_show"> <img style="width:12px; height:12px; display:none; " src="images/arrow-down.gif" width="12" height="12" border="0" alt="hide" id="author_20160001311_hide"></p> <p>2014-01-01</p> <p>Background: Epidemics of meningococcal meningitis are concentrated in sub-Saharan Africa during the dry season, a period when the <span class="hlt">region</span> is affected by the Harmattan, a dry and dusty northeasterly <span class="hlt">trade</span> <span class="hlt">wind</span> blowing from the Sahara into the Gulf of Guinea.Objectives: We examined the potential of climate-based statistical forecasting models to predict seasonal incidence of meningitis in Niger at both the national and district levels.Data and methods: We used time series of meningitis incidence from 1986 through 2006 for 38 districts in Niger. We tested models based on data that would be readily available in an operational framework, such as climate and dust, population, and the incidence of early cases before the onset of the meningitis season in January-May. Incidence was used as a proxy for immunological state.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017nova.pres.2278K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017nova.pres.2278K"><span>Escape for the Slow Solar <span class="hlt">Wind</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Kohler, Susanna</p> <p>2017-05-01</p> <p>Plasma from the Sun known as the slow solar <span class="hlt">wind</span> has been observed far away from where scientists thought it was produced. Now new simulations may have resolved the puzzle of where the slow solar <span class="hlt">wind</span> comes from and how it escapes the Sun to travel through our solar system.An Origin PuzzleA full view of a coronal hole (dark portion) from SDO. The edges of the coronal hole mark the boundary between open and closed magnetic field lines. [SDO; adapted from Higginson et al. 2017]The Suns atmosphere, known as the corona, is divided into two types of <span class="hlt">regions</span> based on the behavior of magnetic field lines. In closed-field <span class="hlt">regions</span>, the magnetic field is firmly anchored in the photosphere at both ends of field lines, so traveling plasma is confined to coronal loops and must return to the Suns surface. In open-field <span class="hlt">regions</span>, only one end of each magnetic field line is anchored in the photosphere, so plasma is able to stream from the Suns surface out into the solar system.This second type of <span class="hlt">region</span> known as a coronal hole is thought to be the origin of fast-moving plasma measured in our solar system and known as the fast solar <span class="hlt">wind</span>. But we also observe a slow solar <span class="hlt">wind</span>: plasma that moves at speeds of less than 500 km/s.The slow solar <span class="hlt">wind</span> presents a conundrum. Its observational properties strongly suggest it originates in the hot, closed corona rather than the cooler, open <span class="hlt">regions</span>. But if the slow solar <span class="hlt">wind</span> plasma originates in closed-field <span class="hlt">regions</span> of the Suns atmosphere, then how does it escape from the Sun?Slow <span class="hlt">Wind</span> from Closed FieldsA team of scientists led by Aleida Higginson (University of Michigan) has now used high-resolution, three-dimensional magnetohydrodynamic simulations to show how the slow solar <span class="hlt">wind</span> can be generated from plasma that starts outin closed-field parts of the Sun.A simulated heliospheric arc, composed of open magnetic field lines. [Higginson et al. 2017]Motions on the Suns surface near the boundary between open and closed-field <span class="hlt">regions</span> the boundary</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2012AGUFM.A31F0098Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2012AGUFM.A31F0098Z"><span>Impacts of <span class="hlt">Wind</span> Farms on Local Land Surface Temperature</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhou, L.; Tian, Y.; Baidya Roy, S.; Thorncroft, C.; Bosart, L. F.; Hu, Y.</p> <p>2012-12-01</p> <p>The U.S. <span class="hlt">wind</span> industry has experienced a remarkably rapid expansion of capacity in recent years and this rapid growth is expected to continue in the future. While converting <span class="hlt">wind</span>'s kinetic energy into electricity, <span class="hlt">wind</span> turbines modify surface-atmosphere exchanges and transfer of energy, momentum, mass and moisture within the atmosphere. These changes, if spatially large enough, may have noticeable impacts on local to <span class="hlt">regional</span> weather and climate. Here we present observational evidence for such impacts based on analyses of satellite derived land surface temperature (LST) data at ~1.1 km for the period of 2003-2011 over a <span class="hlt">region</span> in West-Central Texas, where four of the world's largest <span class="hlt">wind</span> farms are located. Our results show a warming effect of up to 0.7 degrees C at nighttime for the 9-year period during which data was collected, over <span class="hlt">wind</span> farms relative to nearby non <span class="hlt">wind</span> farm <span class="hlt">regions</span> and this warming is gradually enhanced with time, while the effect at daytime is small. The spatial pattern and magnitude of this warming effect couple very well with the geographic distribution of <span class="hlt">wind</span> turbines and such coupling is stronger at nighttime than daytime and in summer than winter. These results suggest that the warming effect is very likely attributable to the development of <span class="hlt">wind</span> farms. This inference is consistent with the increasing number of operational <span class="hlt">wind</span> turbines with time during the study period, the diurnal and seasonal variations in the frequency of <span class="hlt">wind</span> speed and direction distribution, and the changes in near-surface atmospheric boundary layer conditions due to <span class="hlt">wind</span> farm operations. Figure 1: Nighttime land surface temperature (LST, C) differences between 2010 and 2003 (2010 minus 2003) in summer (June-July-August). Pixels with plus symbol have at least one <span class="hlt">wind</span> turbine. A <span class="hlt">regional</span> mean value (0.592 C) was removed to emphasize the relative LST changes at pixel level and so the resulting warming or cooling rate represents a change relative to the <span class="hlt">regional</span> mean</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1994JApMe..33...85L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1994JApMe..33...85L"><span>Extreme <span class="hlt">Winds</span> in the Pampa del Castillo Plateau, Patagonia, Argentina, with Reference to <span class="hlt">Wind</span> Farm Settlement.</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Labraga, Juan C.</p> <p>1994-01-01</p> <p><span class="hlt">Wind</span> farm settlement in Argentina is likely to be initiated in the extended and uniform Pampa del Castillo tablelands (5100 km2) in central cast Patagonia, due to its suitable <span class="hlt">wind</span> regime and local economic factors. The magnitude of these investments requires not only a detailed <span class="hlt">wind</span> energy assessment and optimum site selection but also a comprehensive evaluation of the extreme <span class="hlt">winds</span> experienced in the <span class="hlt">region</span>.Statistical results, with emphasis on severe <span class="hlt">winds</span>, of two <span class="hlt">regional</span> programs of one-year observations at four levels above the ground are presented in this paper. The highest frequencies of hourly mean <span class="hlt">wind</span> velocities above 40, 60, and 80 km h1 are observed during November and December. The spring power spectrum shows a considerable amount of energy in components with a periodicity ranging from 2.5 to 4 days. Severe <span class="hlt">wind</span> episodes are usually related to the displacement of low pressure systems from the Atlantic to the Pacific Ocean through the Drake Passage with a periodicity consistent with spectral results. The highest hourly mean <span class="hlt">wind</span> speed registered in each experimental period (at 60 m AGL) is about 25 m s1. The estimated modal value of the theoretical probability distribution of annual extreme values is in good agreement with observed values. The annual peak gust for an averaging time of 240 s is about 27 m s. The gust factor was computed for different averaging intervals and compared with empirical formulations. Its variation with height and time of year was also analyzed. The general form of the vertical <span class="hlt">wind</span> profile and its dependence on stability conditions was characterized and compared with that of typical episodes of severe <span class="hlt">winds</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1223839','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1223839"><span><span class="hlt">Wind</span> Power Curve Modeling Using Statistical Models: An Investigation of Atmospheric Input Variables at a Flat and Complex Terrain <span class="hlt">Wind</span> Farm</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>Wharton, S.; Bulaevskaya, V.; Irons, Z.</p> <p></p> <p>The goal of our FY15 project was to explore the use of statistical models and high-resolution atmospheric input data to develop more accurate prediction models for turbine power generation. We modeled power for two operational <span class="hlt">wind</span> farms in two <span class="hlt">regions</span> of the country. The first site is a 235 MW <span class="hlt">wind</span> farm in Northern Oklahoma with 140 GE 1.68 turbines. Our second site is a 38 MW <span class="hlt">wind</span> farm in the Altamont Pass <span class="hlt">Region</span> of Northern California with 38 Mitsubishi 1 MW turbines. The farms are very different in topography, climatology, and turbine technology; however, both occupy high <span class="hlt">wind</span> resourcemore » areas in the U.S. and are representative of typical <span class="hlt">wind</span> farms found in their respective areas.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70033389','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70033389"><span>Northerly surface <span class="hlt">winds</span> over the eastern North Pacific Ocean in spring and summer</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Taylor, S.V.; Cayan, D.R.; Graham, N.E.; Georgakakos, K.P.</p> <p>2008-01-01</p> <p>Persistent spring and summer northerly surface <span class="hlt">winds</span> are the defining climatological feature of the western coast of North America, especially south of the Oregon coast. Northerly surface <span class="hlt">winds</span> are important for upwelling and a vast array of other biological, oceanic, and atmospheric processes. Intermittence in northerly coastal surface <span class="hlt">wind</span> is characterized and <span class="hlt">wind</span> events are quantitatively defined using coastal buoy data south of Cape Mendocino on the northern California coast. The defined <span class="hlt">wind</span> events are then used as a basis for composites in order to explain the spatial evolution of various atmospheric and oceanic processes. <span class="hlt">Wind</span> events involve large-scale changes in the three-dimensional atmospheric circulation including the eastern North Pacific subtropical anticyclone and southeast <span class="hlt">trade</span> <span class="hlt">winds</span>. Composites of QSCAT satellite scatterometer <span class="hlt">wind</span> estimates from 1999 to 2005 based on a single coastal buoy indicate that <span class="hlt">wind</span> events typically last 72-96 h and result in anomalies in surface <span class="hlt">wind</span> and Ekman pumping that extend over 1000 kin from the west coast of North America. It may be useful to consider ocean circulation and dependent ecosystem dynamics and the distribution of temperature, moisture, and aerosols in the atmospheric boundary layer in the context of <span class="hlt">wind</span> events defined herein. Copyright 2008 by the American Geophysical Union.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016JPhCS.753c2032Y','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016JPhCS.753c2032Y"><span>Characterization of <span class="hlt">wind</span> velocities in the wake of a full scale <span class="hlt">wind</span> turbine using three ground-based synchronized <span class="hlt">Wind</span>Scanners</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Yazicioglu, Hasan; Angelou, Nikolas; Mikkelsen, Torben; José Trujillo, Juan</p> <p>2016-09-01</p> <p>The <span class="hlt">wind</span> energy community is in need of detailed full-field measurements in the wake of <span class="hlt">wind</span> turbines. Here, three dimensional(3D) <span class="hlt">wind</span> vector field measurements obtained in the near-wake <span class="hlt">region</span> behind a full-scale test turbine are presented. Specifically, the wake of a NEG Nordtank turbine, installed at Risoe test field, has been measured from 0 to 2 diameters downstream. For this, three ground-based synchronised short-range <span class="hlt">Wind</span>Scanners and a spinner lidar have been used. The 3D <span class="hlt">wind</span> velocity field has been reconstructed in horizontal and vertical planes crossing the hub. The 10-min mean values of the three <span class="hlt">wind</span> components reveal detailed information regarding the wake properties while propagating downwind over flat terrain. Furthermore, the wake centre is tracked from the measurements and its meander is investigated as function of yaw misalignment of the turbine. The centre-line wake deficit is calculated both in a Nacelle and Moving Frame of Reference. The results can be used in quantitative validation of numerical wake models.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017CSR...151...40T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017CSR...151...40T"><span>Nearshore circulation on a sea breeze dominated beach during intense <span class="hlt">wind</span> events</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Torres-Freyermuth, Alec; Puleo, Jack A.; DiCosmo, Nick; Allende-Arandía, Ma. Eugenia; Chardón-Maldonado, Patricia; López, José; Figueroa-Espinoza, Bernardo; de Alegria-Arzaburu, Amaia Ruiz; Figlus, Jens; Roberts Briggs, Tiffany M.; de la Roza, Jacobo; Candela, Julio</p> <p>2017-12-01</p> <p>A field experiment was conducted on the northern Yucatan coast from April 1 to April 12, 2014 to investigate the role of intense <span class="hlt">wind</span> events on coastal circulation from the inner shelf to the swash zone. The study area is characterized by a micro-tidal environment, low-energy wave conditions, and a wide and shallow continental shelf. Furthermore, easterly <span class="hlt">trade</span> <span class="hlt">winds</span>, local breezes, and synoptic-scale events, associated with the passage of cold-fronts known as Nortes, are ubiquitous in this <span class="hlt">region</span>. Currents were measured concurrently at different cross-shore locations during both local and synoptic-scale intense <span class="hlt">wind</span> events to investigate the influence of different forcing mechanisms (i.e., large-scale currents, <span class="hlt">winds</span>, tides, and waves) on the nearshore circulation. Field observations revealed that nearshore circulation across the shelf is predominantly alongshore-directed (westward) during intense <span class="hlt">winds</span>. However, the mechanisms responsible for driving instantaneous spatial and temporal current variability depend on the weather conditions and the across-shelf location. During local strong sea breeze events (W > 10 m s-1 from the NE) occurring during spring tide, westward circulation is controlled by the tides, <span class="hlt">wind</span>, and waves at the inner-shelf, shallow waters, and inside the surf/swash zone, respectively. The nearshore circulation is relaxed during intense land breeze events (W ≈ 9 m s-1 from the SE) associated with the low atmospheric pressure system that preceded a Norte event. During the Norte event (Wmax≈ 15 m s-1 from the NNW), westward circulation dominated outside the surf zone and was correlated to the Yucatan Current, whereas wave breaking forces eastward currents inside the surf/swash zone. The latter finding implies the existence of large alongshore velocity shear at the offshore edge of the surf zone during the Norte event, which enhances mixing between the surf zone and the inner shelf. These findings suggest that both sea breezes and Nortes play</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014PhPro..55..192C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014PhPro..55..192C"><span>Assessment Parameters and Matching between the Sites and <span class="hlt">Wind</span> Turbines</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Chermitti, A.; Bencherif, M.; Nakoul, Z.; Bibitriki, N.; Benyoucef, B.</p> <p></p> <p>The objective of this paper is to introduce the assessment parameters of the <span class="hlt">wind</span> energy production of sites and pairing between the sites and <span class="hlt">wind</span> turbines. The exploration is made with the <span class="hlt">wind</span> data gathered at 10 m high is based on the atlas of the <span class="hlt">wind</span> of Algeria established by the National office of the Meteorology runs 37 stations of measures. The data is used for a feasibility analysis of optimum future utilization of <span class="hlt">Wind</span> generator potentiality in five promising sites covering a part of landscape types and <span class="hlt">regions</span> in Algeria. Detailed technical assessment for the ten most promising potential <span class="hlt">wind</span> sites was made using the capacity factor and the site effectiveness approach. The investigation was performed assuming several models of small, medium and big size <span class="hlt">wind</span> machines representing different ranges of characteristic speeds and rated power suitable for water pumping and electric supply. The results show that small <span class="hlt">wind</span> turbines could be installed in some coast <span class="hlt">region</span> and medium <span class="hlt">wind</span> turbines could be installed in the high plateau and some desert <span class="hlt">regions</span> and utilized for water supply and electrical power generation, the sites having an important <span class="hlt">wind</span> deposit, in high plateau we find Tiaret site's but in the desert there is some sites for example Adrar, Timimoun and In Amenas, in these sites could be installed a medium and big size <span class="hlt">wind</span> turbines.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015ERL....10b5001B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015ERL....10b5001B"><span>A vast range of opportunities for feeding the world in 2050: <span class="hlt">trade</span>-off between diet, N contamination and international <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Billen, Gilles; Lassaletta, Luis; Garnier, Josette</p> <p>2015-02-01</p> <p>Through a detailed analysis of the FAO database, we have constructed a generalized representation of the nitrogen transfers characterizing the current agro-food system (GRAFS) of 12 macro-<span class="hlt">regions</span> of the world in terms of functional relationships between crop farming, livestock breeding and human nutrition. Based on this model, and maintaining the current cropland areas and the performance of cropping and livestock systems in each <span class="hlt">region</span>, we have assessed the possibilities of meeting the protein requirements of the estimated world population in 2050, according to various combinations of three critical drivers namely human diet (total amount of protein consumed and share of animal protein in this total), <span class="hlt">regional</span> livestock production and crop fertilization intensity, in each <span class="hlt">region</span>. The results show that feeding the projected 2050 world population would generally imply higher levels of inter-<span class="hlt">regional</span> <span class="hlt">trade</span> and of environmental nitrogen contamination than the current levels, but that the scenarios with less recourse to inter-<span class="hlt">regional</span> <span class="hlt">trade</span> generally produce less N losses to the environment. If an equitable human diet (in terms of protein consumption) is to be established globally (the same in all <span class="hlt">regions</span> of the world), the fraction of animal protein should not exceed 40% of a total ingestion of 4 kgN capita-1 yr-1, or 25% of a total consumption of 5 kgN capita-1 yr-1. Our results show that slightly improving the agronomical performance in the most deficient <span class="hlt">regions</span> (namely Maghreb, the Middle East, sub-Saharan Africa, and India) would make it possible not only to meet the global protein requirements with much less international <span class="hlt">trade</span> (hence more food sovereignty), but also to reduce N environmental contamination the most efficiently.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28256314','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28256314"><span>Intra-EU agricultural <span class="hlt">trade</span>, virtual water flows and policy implications.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Antonelli, M; Tamea, S; Yang, H</p> <p>2017-06-01</p> <p>The development of approaches to tackle the European Union (EU) water-related challenges and shift towards sustainable water management and use is one of the main objectives of Horizon 2020, the EU strategy to lead a smart, sustainable and inclusive growth. The EU is an increasingly water challenged area and is a major agricultural trader. As agricultural <span class="hlt">trade</span> entails an exchange of water embodied in goods as a factor of production, this study investigates the <span class="hlt">region</span>'s water-food-<span class="hlt">trade</span> nexus by analysing intra-<span class="hlt">regional</span> virtual water <span class="hlt">trade</span> (VWT) in agricultural products. The analysed period (1993-2011) comprises the enactment of the Water Framework Directive (WFD) in the year 2000. Aspects of the VWT that are relevant for the WFD are explored. The EU is a net importer of virtual water (VW) from the rest of the world, but intra-<span class="hlt">regional</span> VWT represents 46% of total imports and 75% of total exports. Five countries account for 60% of total VW imports (Germany, France, Italy, The Netherlands, Belgium) and 65% of total VW exports (The Netherlands, France, Germany, Belgium and Spain). Intra-EU VWT more than doubled over the period considered, while <span class="hlt">trade</span> with extra-EU countries did not show such a marked trend. In the same period, blue VWT increased significantly within the <span class="hlt">region</span> and net import from the rest of the world slightly decreased. Water scarce countries, such as Spain and Italy, are major exporters of blue water in the <span class="hlt">region</span>. The <span class="hlt">traded</span> volumes of VW have been increasing almost monotonically over the years, and with a substantial increase after 2000. The overall trend in changes in VWT does not seem to be in accordance with the WFD goals. This study demonstrated that VWT analyses can help evaluate intertwining effects of water, agriculture and <span class="hlt">trade</span> policies which are often made separately in respective sectors. Copyright © 2017 Elsevier B.V. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20020086296','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20020086296"><span>Investigation of Solar <span class="hlt">Wind</span> Correlations and Solar <span class="hlt">Wind</span> Modifications Near Earth by Multi-Spacecraft Observations: IMP 8, <span class="hlt">WIND</span> and INTERBALL-1</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Paularena, Karolen I.; Richardson, John D.; Zastenker, Georgy N.</p> <p>2002-01-01</p> <p>The foundation of this Project is use of the opportunity available during the ISTP (International Solar-Terrestrial Physics) era to compare solar <span class="hlt">wind</span> measurements obtained simultaneously by three spacecraft - IMP 8, <span class="hlt">WIND</span> and INTERBALL-1 at wide-separated points. Using these data allows us to study three important topics: (1) the size and dynamics of near-Earth mid-scale (with dimension about 1-10 million km) and small-scale (with dimension about 10-100 thousand km) solar <span class="hlt">wind</span> structures; (2) the reliability of the common assumption that solar <span class="hlt">wind</span> conditions at the upstream Lagrangian (L1) point accurately predict the conditions affecting Earth's magnetosphere; (3) modification of the solar <span class="hlt">wind</span> plasma and magnetic field in the <span class="hlt">regions</span> near the Earth magnetosphere, the foreshock and the magnetosheath. Our Project was dedicated to these problems. Our research has made substantial contributions to the field and has lead others to undertake similar work.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3465402','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=3465402"><span>Saturation <span class="hlt">wind</span> power potential and its implications for <span class="hlt">wind</span> energy</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Jacobson, Mark Z.; Archer, Cristina L.</p> <p>2012-01-01</p> <p><span class="hlt">Wind</span> turbines convert kinetic to electrical energy, which returns to the atmosphere as heat to regenerate some potential and kinetic energy. As the number of <span class="hlt">wind</span> turbines increases over large geographic <span class="hlt">regions</span>, power extraction first increases linearly, but then converges to a saturation potential not identified previously from physical principles or turbine properties. These saturation potentials are >250 terawatts (TW) at 100 m globally, approximately 80 TW at 100 m over land plus coastal ocean outside Antarctica, and approximately 380 TW at 10 km in the jet streams. Thus, there is no fundamental barrier to obtaining half (approximately 5.75 TW) or several times the world’s all-purpose power from <span class="hlt">wind</span> in a 2030 clean-energy economy. PMID:23019353</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://files.eric.ed.gov/fulltext/ED362778.pdf','ERIC'); return false;" href="http://files.eric.ed.gov/fulltext/ED362778.pdf"><span>B-WEST <span class="hlt">Regional</span> Workforce Training Center. Building Workers Entering Skilled <span class="hlt">Trades</span>. Program Development 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>Portland Community Coll., OR.</p> <p></p> <p>This program development guide outlines the procedures for replicating the B-WEST (Building Workers Entering Skilled <span class="hlt">Trades</span>) program, a two-term professional certificate program designed to prepare women for skilled jobs in the traditionally male-dominated electrical, mechanical, and construction <span class="hlt">trades</span>. The components and major activities of the…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.fs.usda.gov/treesearch/pubs/33321','TREESEARCH'); return false;" href="https://www.fs.usda.gov/treesearch/pubs/33321"><span>Globalization and world <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://www.fs.usda.gov/treesearch/">Treesearch</a></p> <p>Peter J. Ince; Joseph Buongiorno</p> <p>2007-01-01</p> <p>This chapter discusses economic globalization and world <span class="hlt">trade</span> in relation to forest sector modeling for the US/North American <span class="hlt">region</span>. It discusses drivers of economic globalization and related structural changes in US forest product markets, including currency exchange rates and differences in manufacturing costs that have contributed to the displacement of global...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015LatJP..52b..26B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015LatJP..52b..26B"><span>Assessment of <span class="hlt">Wind</span> Shear and <span class="hlt">Wind</span> Energy Potential in the Baltic Sea <span class="hlt">Region</span> of Latvia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bezrukovs, V.; Bezrukovs, Vl.; Zacepins, A.; Komashilovs, V.</p> <p>2015-04-01</p> <p>The paper is devoted to the investigation into the <span class="hlt">wind</span> energy potential based on long-term observations of the <span class="hlt">wind</span> speed and energy density fluctuations at heights from 10 to 160 m on the Baltic Sea coast of Latvia. During the observations (2004 - 2013), the <span class="hlt">wind</span> speed and direction values were measured, and the statistical database was accumulated using a LOGGER 9200 Symphonie measuring systems mounted on 60 m masts - one on the western coast and another on the north-east of Latvia. From June 2011 to May 2012, these measurements were complemented with the data for the heights from 40 to 160 m obtained by means of a ZephIR lidar and with the metrological data provided by "Latvian Environment, Geology and Meteorology Centre" for the same period. The graphs of seasonal fluctuations in the <span class="hlt">wind</span> speed were obtained for the heights up to 160 m by measurements over the period of 2007 - 2013. The results of the research on the <span class="hlt">wind</span> speed distribution up to 200 m are promising for evaluation of the <span class="hlt">wind</span> energy potential of Latvia and will be helpful in assessment of prospective sites for construction of WPPs. Zinātniskais raksts ir veltīts pētījumam par vēja enerģijas potenciālu Latvijas teritorijā, Baltijas jūras piekrastē, balstoties uz ilgtermiņa vēja ātruma un vēja enerģijas blīvuma svārstību novērojumiem no 10 līdz 160 metriem augstumā. Vēja ātruma un vēja virziena mērījumu dati tika iegūti un apkopoti statistiskajā datubāzē laika periodā no 2004 līdz 2013. gadam, izmantojot mērīšanas sistēmu LOGGER 9200 Symphonie, kas bija ierīkotā uz 60 metru augsta masta - viena rietumu piekrastē un otra Latvijas ziemeļu-austrumos. No 2011. gada jūnija līdz 2012. gada maijam mērījumu datubāze tika papildināta ar datiem, kas tika iegūti ar lidaruZephIR augstumos no 40 līdz 160 metriem, un datiem no "Latvijas Vides, ģeoloģijas un meteoroloģijas centra" tam pašam laika periodam. Analizējot mērījumus 2007. g.-2013. g., grafiki ar</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26245251','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26245251"><span>Commentary: Moving towards policy coherence in <span class="hlt">trade</span> and health.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Walls, Helen; Baker, Phillip; Smith, Richard</p> <p>2015-11-01</p> <p>International <span class="hlt">trade</span> has brought economic benefits to many countries, but the association of <span class="hlt">trade</span> and investment liberalisation with poor health outcomes concerns the public health community. The need to secure more 'healthy' <span class="hlt">trade</span> is a recognised priority, especially as countries move from global to <span class="hlt">regional</span>/bilateral <span class="hlt">trade</span> agreements - with greater public health risks. However, a transition towards 'healthier <span class="hlt">trade</span>' may be hindered by worldview differences between the <span class="hlt">trade</span> and health communities. There is a tendency for health actors to perceive <span class="hlt">trade</span> as a threat to population health, and for <span class="hlt">trade</span> actors to view health as a constraint to <span class="hlt">trade</span> objectives of reducing barriers to cross-border commercial flows and economic growth. Unless such differing worldviews can be aligned, finding ways forward for addressing public health in <span class="hlt">trade</span> policy is likely to be difficult. Moving forward will involve understanding the values and drivers of the respective groups, and developing solutions palatable to their various interests. Given the power imbalances between the two areas, it is likely that the health community will have to make the first moves in this respect. This article outlines the key issues involved and suggests areas where such moves have been, and may be made.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/biblio/22520043-energy-dissipation-processes-solar-wind-turbulence','SCIGOV-STC'); return false;" href="https://www.osti.gov/biblio/22520043-energy-dissipation-processes-solar-wind-turbulence"><span>ENERGY DISSIPATION PROCESSES IN SOLAR <span class="hlt">WIND</span> TURBULENCE</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, Y.; Wei, F. S.; Feng, X. S.</p> <p></p> <p>Turbulence is a chaotic flow regime filled by irregular flows. The dissipation of turbulence is a fundamental problem in the realm of physics. Theoretically, dissipation ultimately cannot be achieved without collisions, and so how turbulent kinetic energy is dissipated in the nearly collisionless solar <span class="hlt">wind</span> is a challenging problem. Wave particle interactions and magnetic reconnection (MR) are two possible dissipation mechanisms, but which mechanism dominates is still a controversial topic. Here we analyze the dissipation <span class="hlt">region</span> scaling around a solar <span class="hlt">wind</span> MR <span class="hlt">region</span>. We find that the MR <span class="hlt">region</span> shows unique multifractal scaling in the dissipation range, while the ambientmore » solar <span class="hlt">wind</span> turbulence reveals a monofractal dissipation process for most of the time. These results provide the first observational evidences for intermittent multifractal dissipation <span class="hlt">region</span> scaling around a MR site, and they also have significant implications for the fundamental energy dissipation process.« less</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_19");'>19</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li class="active"><span>21</span></li> <li><a href="#" onclick='return showDiv("page_22");'>22</a></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div><!-- col-sm-12 --> </div><!-- row --> </div><!-- page_21 --> <div id="page_22" class="hiddenDiv"> <div class="row"> <div class="col-sm-12"> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_20");'>20</a></li> <li><a href="#" onclick='return showDiv("page_21");'>21</a></li> <li class="active"><span>22</span></li> <li><a href="#" onclick='return showDiv("page_23");'>23</a></li> <li><a href="#" onclick='return showDiv("page_24");'>24</a></li> <li><a href="#" onclick='return showDiv("page_25");'>»</a></li> </ul> </div> </div> </div> <div class="row"> <div class="col-sm-12"> <ol class="result-class" start="421"> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900027052&hterms=Fran&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DFran','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900027052&hterms=Fran&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D30%26Ntt%3DFran"><span>Pluto's interaction with the solar <span class="hlt">wind</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Bagenal, Fran; Mcnutt, Ralph L., Jr.</p> <p>1989-01-01</p> <p>If Pluto's atmospheric escape rate is significantly greater than 1.5 x 10 to the 27th molecules/s then the interaction with the tenuous solar <span class="hlt">wind</span> at 30 A.U. will be like that of a comet. There will be extensive ion pick-up upstream and the size of the interaction <span class="hlt">region</span> will vary directly with variations in the solar <span class="hlt">wind</span> flux. If the escape flux is much less, then one expects that the solar <span class="hlt">wind</span> will be deflected around Pluto's ionosphere in a Venus-like interaction. In either case, the weak interplanetary magnetic field at 30 A.U. results in very large gyroradii for the picked-up ions and a thick bow shock, necessitating a kinetic treatment of the interaction. Strong variations in the size of the interaction <span class="hlt">region</span> are expected on time scales of days due to changes in the solar <span class="hlt">wind</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1044598','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1044598"><span>Mid-Atlantic <span class="hlt">Wind</span> - Overcoming the Challenges</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>Daniel F. Ancona III; Kathryn E. George; Lynn Sparling</p> <p>2012-06-29</p> <p>This study, supported by the US Department of Energy, <span class="hlt">Wind</span> Powering America Program, Maryland Department of Natural Resources and Chesapeake Bay Foundation, analyzed barriers to <span class="hlt">wind</span> energy development in the Mid-Atlantic <span class="hlt">region</span> along with options for overcoming or mitigating them. The Mid-Atlantic States including Delaware, Maryland, North Carolina and Virginia, have excellent <span class="hlt">wind</span> energy potential and growing demand for electricity, but only two utility-scale projects have been installed to date. Reasons for this apathetic development of <span class="hlt">wind</span> resources were analyzed and quantified for four markets. Specific applications are: 1) Appalachian mountain ridgeline sites, 2) on coastal plains and peninsulas, 3)more » at shallow water sites in Delaware and Chesapeake Bays, Albemarle and Pamlico Sounds, and 4) at deeper water sites off the Atlantic coast. Each market has distinctly different opportunities and barriers. The primary barriers to <span class="hlt">wind</span> development described in this report can be grouped into four categories; state policy and regulatory issues, <span class="hlt">wind</span> resource technical uncertainty, economic viability, and public interest in environmental issues. The properties of these typologies are not mutually independent and do interact. The report concluded that there are no insurmountable barriers to land-based <span class="hlt">wind</span> energy projects and they could be economically viable today. Likewise potential sites in sheltered shallow waters in <span class="hlt">regional</span> bay and sounds have been largely overlooked but could be viable currently. Offshore ocean-based applications face higher costs and technical and <span class="hlt">wind</span> resource uncertainties. The ongoing research and development program, revision of state incentive policies, additional <span class="hlt">wind</span> measurement efforts, transmission system expansion, environmental baseline studies and outreach to private developers and stakeholders are needed to reduce barriers to <span class="hlt">wind</span> energy development.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970026045','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970026045"><span>National <span class="hlt">Wind</span> Tunnel Complex (NWTC)</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1996-01-01</p> <p>The National <span class="hlt">Wind</span> Tunnel Complex (NWTC) Final Report summarizes the work carried out by a unique Government/Industry partnership during the period of June 1994 through May 1996. The objective of this partnership was to plan, design, build and activate 'world class' <span class="hlt">wind</span> tunnel facilities for the development of future-generation commercial and military aircraft. The basis of this effort was a set of performance goals defined by the National Facilities Study (NFS) Task Group on Aeronautical Research and Development Facilities which established two critical measures of improved <span class="hlt">wind</span> tunnel performance; namely, higher Reynolds number capability and greater productivity. Initial activities focused upon two high-performance tunnels (low-speed and transonic). This effort was later descoped to a single multipurpose tunnel. Beginning in June 1994, the NWTC Project Office defined specific performance requirements, planned site evaluation activities, performed a series of technical/cost <span class="hlt">trade</span> studies, and completed preliminary engineering to support a proposed conceptual design. Due to budget uncertainties within the Federal government, the NWTC project office was directed to conduct an orderly closure following the Systems Design Review in March 1996. This report provides a top-level status of the project at that time. Additional details of all work performed have been archived and are available for future reference.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29679724','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29679724"><span>Harvest and <span class="hlt">trade</span> of caterpillar mushroom (Ophiocordyceps sinensis) and the implications for sustainable use in the Tibet <span class="hlt">Region</span> of Southwest China.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>He, Jun</p> <p>2018-07-15</p> <p>Caterpillar mushroom (Ophiocordyceps sinensis) is a unique medicinal fungi which is only found in alpine grasslands in Himalayan mountain <span class="hlt">regions</span> and the Tibetan Plateau. Known locally as Yartsa Gunbu, it has been widely used in Tibetan and Chinese Medicine for centuries. It is crucial to understand local commercial harvest and <span class="hlt">trade</span> practices of caterpillar mushroom to support the sustainable management of this valuable resource. However, data derived from empirically grounded research is currently limited, particularly in China. The research aims to provide the most up-to-date insights into caterpillar mushroom harvest and <span class="hlt">trade</span> in the main production area of the Tibet <span class="hlt">Region</span> in Southwest China and to generate policy recommendations for sustainable use. The research was conducted in 2015-2016 in six Tibetan communities located in two counties in Diqing Tibetan Autonomous Prefecture, Southwest China. Quantitative and qualitative data were collected from in-depth interviews with local households engaged in caterpillar mushroom harvesting (n = 157), local caterpillar mushroom traders (n = 14), and from focus groups discussions (n = 5) with <span class="hlt">regional</span> caterpillar mushroom industry stakeholders. The research found large <span class="hlt">regional</span>- and community-level differences in caterpillar mushroom harvest practices. The harvest practices of communities involved in the co-management of a Nature Reserve were more sustainable than those communities not involved in such a scheme, and this was due to the external support and training provided via the co-management scheme. Moreover, a customary tenure system was proving effective for avoiding competition over caterpillar mushroom collection. However, in both counties, narrow marketing channel and non-grading system in <span class="hlt">trade</span> limits the possibility of improving the local benefits generated from the commercial harvest of caterpillar mushroom. Meanwhile, the local traders play an important bridging role in the value chain and</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1993PhDT.......198H','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1993PhDT.......198H"><span>Westerly <span class="hlt">Wind</span> Bursts: a Synoptic-Dynamic Study</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Hartten, Leslie Marie</p> <p></p> <p>This research examines the synoptic and climatological settings of westerly <span class="hlt">wind</span> bursts (WWBs) during the 1980s and the dynamical processes active during them. Probabilities of strong westerly and easterly 1000 mb <span class="hlt">winds</span> over the western equatorial Pacific are presented. Westerlies exhibit a clear annual cycle, appearing in the north in July, moving southeastward as the year progresses, and disappearing by June. Conditional probabilities, dependent on the value of the SOI, show that strong westerlies are more likely and more geographically extensive when the SOI is low, especially from July through January. A newly developed two-dimensional classification scheme qualitatively describes the near-surface synoptic flow of almost 90% of the 131 WWBs identified during the decade. Only 8% of the WWBs are described by the pattern involving twin cyclonic circulations straddling the equator. The <span class="hlt">trades</span>, tropical cyclones, and the southeast Asian monsoon are all at times linked to WWBs, and the synoptic patterns often contain a significant barotropic component. Breaks in WWB activity are well correlated with a cooler than normal western Pacific warm pool. However, near-equatorial WWBs do not show a good correlation with the Madden-Julian Oscillation. Four near-equatorial WWBs are examined in detail. All are associated with broad cross-equatorial flow; two also have a cyclonic circulation poleward of the westerlies. Anticyclonic relative vorticity equatorward of the burst displaces the zero line of absolute vorticity, eta, into the burst hemisphere. In the three Southern Hemisphere cases, horizontal advection in a <span class="hlt">region</span> extending from north of New Guinea east-southeast toward the dateline is crucial to the generation and maintenance of the eta pattern. Vorticity stretching associated with convection helps maintain a tight gradient of eta near and poleward of the burst, but also drives the eta = 0 line back towards the equator as the burst ends. In the Northern Hemisphere case</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMIN11B0033T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMIN11B0033T"><span>Statistical Compression of <span class="hlt">Wind</span> Speed Data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tagle, F.; Castruccio, S.; Crippa, P.; Genton, M.</p> <p>2017-12-01</p> <p>In this work we introduce a lossy compression approach that utilizes a stochastic <span class="hlt">wind</span> generator based on a non-Gaussian distribution to reproduce the internal climate variability of daily <span class="hlt">wind</span> speed as represented by the CESM Large Ensemble over Saudi Arabia. Stochastic <span class="hlt">wind</span> generators, and stochastic weather generators more generally, are statistical models that aim to match certain statistical properties of the data on which they are trained. They have been used extensively in applications ranging from agricultural models to climate impact studies. In this novel context, the parameters of the fitted model can be interpreted as encoding the information contained in the original uncompressed data. The statistical model is fit to only 3 of the 30 ensemble members and it adequately captures the variability of the ensemble in terms of seasonal internannual variability of daily <span class="hlt">wind</span> speed. To deal with such a large spatial domain, it is partitioned into 9 <span class="hlt">region</span>, and the model is fit independently to each of these. We further discuss a recent refinement of the model, which relaxes this assumption of <span class="hlt">regional</span> independence, by introducing a large-scale component that interacts with the fine-scale <span class="hlt">regional</span> effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19960021269&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbackground%2Bwind','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19960021269&hterms=background+wind&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D80%26Ntt%3Dbackground%2Bwind"><span>A kinetic study of solar <span class="hlt">wind</span> electrons in the transition <span class="hlt">region</span> from collision dominated to collisionless flow</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Lie-Svendsen, O.; Leer, E.</p> <p>1995-01-01</p> <p>We have studied the evolution of the velocity distribution function of a test population of electrons in the solar corona and inner solar <span class="hlt">wind</span> <span class="hlt">region</span>, using a recently developed kinetic model. The model solves the time dependent, linear transport equation, with a Fokker-Planck collision operator to describe Coulomb collisions between the 'test population' and a thermal background of charged particles, using a finite differencing scheme. The model provides information on how non-Maxwellian features develop in the distribution function in the transition <span class="hlt">region</span> from collision dominated to collisionless flow. By taking moments of the distribution the evolution of higher order moments, such as the heat flow, can be studied.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014EGUGA..16.2997M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014EGUGA..16.2997M"><span>Anywhere the <span class="hlt">Wind</span> Blows does Really Matter</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Montaldo, Nicola; Oren, Ram</p> <p>2014-05-01</p> <p>The variation of net ecosystem carbon exchange (NEE) has been explained at coarse scales with variation of forcing variables among climate <span class="hlt">regions</span> and associated biomes, at the intermediate, mesoscale, with differences among dominating vegetation types and conditions, and at the misoscale with heterogeneity of the eddy covariance footprint properties. <span class="hlt">Wind</span> is rarely considered in analysis of surface fluxes for its effects on periodic budgets of water and carbon. In many <span class="hlt">regions</span> conditions change frequently between maritime and continental depending on <span class="hlt">wind</span> velocity (VW) and direction. In these <span class="hlt">regions</span>, water and carbon fluxes may respond to mesoscale weather patterns extending maritime influences far inland. Using eddy-covariance data from Sardinia, we show that daytime net carbon exchange (NEE) of a mixed pasture-woodland (grass-wild olive) ecosystem (Detto et al., 2006; Montaldo et al., 2008) increased with VW, especially during summer-dry conditions. As VW increased, the air, humidified over sea, remains relatively moist and cool to a greater distance inland, reaching only ~50 km during slow Saharan Sirocco <span class="hlt">wind</span> but >160 km during mostly Mistral <span class="hlt">wind</span> (4 m/s) from Continental Europe. A 30% lower vapor pressure deficit (D) associated with high VW (average 2 kPa at 4 m/s), allowed a 50% higher canopy stomatal conductance (gc) and, thus, photosynthesis. However, because gc and D have opposite effects on evapotranspiration (Ee), Ee was unaffected by VW. Thus, higher NEE during summertime Mistral reflects increased ecosystem water-use efficiency (We) and a departure from a costly carbon-water tradeoff. Yet many <span class="hlt">regions</span> often experience high velocity <span class="hlt">winds</span>, attention is typically focused on the capacity of strong <span class="hlt">winds</span> to fan <span class="hlt">regional</span> fires, threatening human habitation and natural habitats, and reducing Carbon storage (C), NEE and latent heat flux. However, depending on their origin, high velocity <span class="hlt">winds</span> can bring continental air to the coast (e.g., Santa Ana <span class="hlt">winds</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-05-03/pdf/2010-10273.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-05-03/pdf/2010-10273.pdf"><span>75 FR 23223 - Meetings of the Agricultural Policy Advisory Committee for <span class="hlt">Trade</span> and the Agricultural Technical...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-05-03</p> <p>... the <span class="hlt">trade</span> policy of the United States. Topics will include Doha Round negotiations in the World <span class="hlt">Trade</span> Organization (WTO), WTO accession negotiations, and negotiations in bilateral and <span class="hlt">regional</span> free <span class="hlt">trade</span>... <span class="hlt">trade</span> agreement negotiations and/or other matters concerning the administration of <span class="hlt">trade</span> policy, the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=20090006612&hterms=Solar+still&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DSolar%2Bstill','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=20090006612&hterms=Solar+still&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DSolar%2Bstill"><span>Topological Origins of the Slow Solar <span class="hlt">Wind</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Antiochos, Spiro</p> <p>2008-01-01</p> <p>Although the slow solar <span class="hlt">wind</span> has been studied for decades with both in situ and remote sensing observations, its origin is still a matter of intense debate. In the standard quasi-steady model, the slow <span class="hlt">wind</span> is postulated to originate near coronal hole boundaries that define topologically well-behaved separatrices between open and closed field <span class="hlt">regions</span>. In the interchange model, on the other hand, the slow <span class="hlt">wind</span> is postulated to originate on open flux that is dynamically diffusing throughout the seemingly closed-field corona. We argue in favor of the quasi-steady scenario and propose that the slow <span class="hlt">wind</span> is due to two effects: First, the open-closed boundary is highly complex due to the complexity of the photospheric flux distribution. Second, this boundary is continuously driven by the transport of magnetic helicity from the closed field <span class="hlt">region</span> into the open. The implications of this model for the structure and dynamics of the corona and slow <span class="hlt">wind</span> are discussed, and observational tests of the mode</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990116485&hterms=SSM&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DSSM','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990116485&hterms=SSM&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D40%26Ntt%3DSSM"><span>Surface-<span class="hlt">Wind</span> Anomalies in North-Atlantic and North Pacific from SSM/I Observations: Influence on Temperature of Adjoining Land <span class="hlt">Regions</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Otterman, Joseph; Atlas, R.; Ingraham, J.; Ardizzone, J.; Starr, D.; Terry, J.</p> <p>1998-01-01</p> <p>Surface <span class="hlt">winds</span> over the oceans are derived from Special Sensor Microwave Imager (SSM/I) measurements, assigning direction by Variational Analysis Method (VAM). Validations by comparison with other measurements indicate highly-satisfactory data quality. Providing global coverage from 1988, the dataset is a convenient source for surface-<span class="hlt">wind</span> climatology. In this study, the interannual variability of zonal <span class="hlt">winds</span> is analyzed concentrating on the westerlies in North Atlantic and North Pacific, above 30 N. Interannual differences in the westerlies exceeding 10 m sec (exp -1) are observed over large <span class="hlt">regions</span>, often accompanied by changes of the same magnitude in the easterlies below 30 N. We concentrate on February/March, since elevated temperatures, by advancing snow-melt, can produce early spring. The extremely strong westerlies in 1997 observed in these months over North Atlantic (and also North Pacific) apparently contributed to large surface-temperature anomalies in western Europe, on the order of +3 C above the climatic monthly average for England and France. At these latitudes strong positive anomalies extended in a ring around the globe. We formulated an Index of South westerlies for the North Atlantic, which can serve as an indicator for day-by-day advection effects into Europe. In comparing 1997 and 1998 with the previous years, we establish significant correlations with the temperature anomalies (one to five days later, depending on the <span class="hlt">region</span>, and on the season). This variability of the ocean-surface <span class="hlt">winds</span> and of the temperature anomalies on land may be related to the El Nino/La Nina oscillations. Such large temperature fluctuations over large areas, whatever the cause, can be regarded as noise in attempts to assess long-term trends in global temperature.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22474363','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22474363"><span>Evolution of the global virtual water <span class="hlt">trade</span> network.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Dalin, Carole; Konar, Megan; Hanasaki, Naota; Rinaldo, Andrea; Rodriguez-Iturbe, Ignacio</p> <p>2012-04-17</p> <p>Global freshwater resources are under increasing pressure from economic development, population growth, and climate change. The international <span class="hlt">trade</span> of water-intensive products (e.g., agricultural commodities) or virtual water <span class="hlt">trade</span> has been suggested as a way to save water globally. We focus on the virtual water <span class="hlt">trade</span> network associated with international food <span class="hlt">trade</span> built with annual <span class="hlt">trade</span> data and annual modeled virtual water content. The evolution of this network from 1986 to 2007 is analyzed and linked to <span class="hlt">trade</span> policies, socioeconomic circumstances, and agricultural efficiency. We find that the number of <span class="hlt">trade</span> connections and the volume of water associated with global food <span class="hlt">trade</span> more than doubled in 22 years. Despite this growth, constant organizational features were observed in the network. However, both <span class="hlt">regional</span> and national virtual water <span class="hlt">trade</span> patterns significantly changed. Indeed, Asia increased its virtual water imports by more than 170%, switching from North America to South America as its main partner, whereas North America oriented to a growing intraregional <span class="hlt">trade</span>. A dramatic rise in China's virtual water imports is associated with its increased soy imports after a domestic policy shift in 2000. Significantly, this shift has led the global soy market to save water on a global scale, but it also relies on expanding soy production in Brazil, which contributes to deforestation in the Amazon. We find that the international food <span class="hlt">trade</span> has led to enhanced savings in global water resources over time, indicating its growing efficiency in terms of global water use.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFMGC33A1216B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFMGC33A1216B"><span><span class="hlt">WIND</span> SPEED Monitoring in Northern Eurasia</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Bulygina, O.; Korshunova, N. N.; Razuvaev, V. N.; Groisman, P. Y.</p> <p>2016-12-01</p> <p>The <span class="hlt">wind</span> regime of Russia varies a great deal due to the large size of the country's territory and variety of climate and terrain conditions. Changes in the regime of surface <span class="hlt">wind</span> are of great practical importance. They can affect heat and water balance. Strong <span class="hlt">wind</span> is one of the most hazardous meteorological event for various sectors of economy and for infrastructure. The main objective of this research is to monitoring <span class="hlt">wind</span> speed change in Northern Eurasia At meteorological stations <span class="hlt">wind</span> speed and <span class="hlt">wind</span> direction are measured at the height of 10-12 meters over the land surface with the help of <span class="hlt">wind</span> meters or <span class="hlt">wind</span> wanes. Calculations were made on the basis of data for the period of 1980-2015. It allowed the massive scale disruption of homogeneity to be eliminated and sufficient period needed to obtain sustainable statistic characteristics to be retained. Data on average and maximum <span class="hlt">wind</span> speed measured at 1457 stations of Russia were used. The analysis of changes in <span class="hlt">wind</span> characteristics was made on the basis of point data and series of average characteristics obtained for 18 quasi-homogeneous climatic <span class="hlt">regions</span>. Statistical characteristics (average and maximum values of <span class="hlt">wind</span> speed, prevailing <span class="hlt">wind</span> direction, values of the boundary of the 90%, 95% and 99%-confidence interval in the distribution of maximum <span class="hlt">wind</span> speed) were obtained for all seasons and for the year as a whole. Values of boundaries of the 95% and 99%-confidence interval in the distribution of maximum <span class="hlt">wind</span> speed were considered as indicators of extremeness of the <span class="hlt">wind</span> regime. The trend of changes in average and maximum <span class="hlt">wind</span> speed was assessed with a linear trend coefficient. A special attention was paid to <span class="hlt">wind</span> changes in the Arctic where dramatic changes in surface air temperature and sea ice extent and density have been observed during the past decade. The analysis of the results allowed seasonal and <span class="hlt">regional</span> features of changes in the <span class="hlt">wind</span> regime on the territory of the northern part of Eurasia to be</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2008AGUFM.A21E0221R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2008AGUFM.A21E0221R"><span>Model for <span class="hlt">wind</span> resource analysis and for <span class="hlt">wind</span> farm planning</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rozsavolgyi, K.</p> <p>2008-12-01</p> <p>Due to the ever increasing anthropogenic environmental pollution and the worldwide energy demand, the research and exploitation of environment-friendly renewable energy sources like <span class="hlt">wind</span>, solar, geothermal, biomass become more and more important. During the last decade <span class="hlt">wind</span> energy utilization has developed dynamically with big steps. Over just the past seven years, annual worldwide growth in installed <span class="hlt">wind</span> capacity is near 30 %. Over 94 000 MW installed currently all over the world. Besides important economic incentives, the most extensive and most accurate scientific results are required in order to provide beneficial help for <span class="hlt">regional</span> planning of <span class="hlt">wind</span> farms to find appropriate sites for optimal exploitation of this renewable energy source. This research is on the spatial allocation of possible <span class="hlt">wind</span> energy usage for <span class="hlt">wind</span> farms. In order to carry this out a new model (CMPAM = Complex Multifactoral Polygenetic Adaptive Model) is being developed, which basically is a <span class="hlt">wind</span> climate-oriented system, but other kind of factors are also considered. With this model those areas and terrains can be located where construction of large <span class="hlt">wind</span> farms would be reasonable under the given conditions. This model consist of different sub- modules such as <span class="hlt">wind</span> field modeling sub module (CMPAM/W) that is in high focus in this model development procedure. The <span class="hlt">wind</span> field modeling core of CMPAM is mainly based on sGs (sequential Gaussian simulation) hence geostatistics, but atmospheric physics and GIS are used as well. For the application developed for the test area (Hungary) WAsP visualization results were used from 10 m height as input data. This data was geocorrected (GIS geometric correction) before it was used for further calculations. Using optimized variography and sequential Gaussian simulation, results were applied for the test area (Hungary) at different heights. Simulation results were produced and summarized for different heights. Furthermore an exponential regressive function</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2014cosp...40E3557V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2014cosp...40E3557V"><span>Sources of the solar <span class="hlt">wind</span> - the heliospheric point of view</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Von Steiger, Rudolf; Shearer, Paul; Zurbuchen, Thomas</p> <p></p> <p>The solar <span class="hlt">wind</span> as observed in the heliosphere has several properties that can be interpreted as signatures of conditions and processes at its source in the solar atmosphere. Traditionally it has been customary to distinguish between solar <span class="hlt">wind</span> types solely based on its speed, "fast" and "slow" <span class="hlt">wind</span>. Over the last couple of decades new instruments resolving not only the main constituents (protons and alpha particles) but also heavy ions from C to Fe have added new observables, in particular the charge state and elemental composition of these ions. The charge states are indicators of the coronal temperature at the source <span class="hlt">region</span>; they have confirmed that the "fast" <span class="hlt">wind</span> emanates from the relatively cool coronal hole <span class="hlt">regions</span>, while the "slow" <span class="hlt">wind</span> originates from hotter sources such as the streamer belt and active <span class="hlt">regions</span>. Thus they are more reliable indicators of solar <span class="hlt">wind</span> source than the speed alone could be because they readily discriminate between "fast" <span class="hlt">wind</span> from coronal holes and fast coronal mass ejections (CMEs). The elemental composition in the solar <span class="hlt">wind</span> compared to the abundances in the photosphere shows a typical fractionation that depends on the first ionization potential (FIP) of the elements. Since that fractionation occurs beneath the corona, in the chromosphere, its strength is indicative of the conditions in that layer. While the "fast" <span class="hlt">wind</span> is very similar to photospheric composition, the fractionation of the "slow" <span class="hlt">wind</span> and of CMEs is higher and strongly variable. We will review the observations of the SWICS composition instruments on both the ACE and the Ulysses missions, which have made composition observations between 1 and 5 AU and at all latitudes in the heliosphere over the last two decades. Specifically, analysis of the "slow" <span class="hlt">wind</span> observations at all time scales, from hours to complete solar cycles, will be used to better characterize its source <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29570407','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29570407"><span>The Geometry of Nutrient Space-Based Life-History <span class="hlt">Trade</span>-Offs: Sex-Specific Effects of Macronutrient Intake on the <span class="hlt">Trade</span>-Off between Encapsulation Ability and Reproductive Effort in Decorated Crickets.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rapkin, James; Jensen, Kim; Archer, C Ruth; House, Clarissa M; Sakaluk, Scott K; Castillo, Enrique Del; Hunt, John</p> <p>2018-04-01</p> <p>Life-history theory assumes that traits compete for limited resources, resulting in <span class="hlt">trade</span>-offs. The most commonly manipulated resource in empirical studies is the quantity or quality of diet. Recent studies using the geometric framework for nutrition, however, suggest that <span class="hlt">trade</span>-offs are often regulated by the intake of specific nutrients, but a formal approach to identify and quantify the strength of such <span class="hlt">trade</span>-offs is lacking. We posit that <span class="hlt">trade</span>-offs occur whenever life-history traits are maximized in different <span class="hlt">regions</span> of nutrient space, as evidenced by nonoverlapping 95% confidence <span class="hlt">regions</span> of the global maximum for each trait and large angles (θ) between linear nutritional vectors and Euclidean distances (d) between global maxima. We then examined the effects of protein and carbohydrate intake on the <span class="hlt">trade</span>-off between reproduction and aspects of immune function in male and female Gryllodes sigillatus. Female encapsulation ability and egg production increased with the intake of both nutrients, whereas male encapsulation ability increased with protein intake but calling effort increased with carbohydrate intake. The <span class="hlt">trade</span>-offs between traits was therefore larger in males than in females, as demonstrated by significant negative correlations between the traits in males, nonoverlapping 95% confidence <span class="hlt">regions</span>, and larger estimates of θ and d. Under dietary choice, the sexes had similar regulated intakes, but neither optimally regulated nutrient intake for maximal trait expression. We highlight the fact that greater consideration of specific nutrient intake is needed when examining nutrient space-based <span class="hlt">trade</span>-offs.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4844684','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4844684"><span>Energy efficiency <span class="hlt">trade</span>-offs drive nucleotide usage in transcribed <span class="hlt">regions</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>Chen, Wei-Hua; Lu, Guanting; Bork, Peer; Hu, Songnian; Lercher, Martin J.</p> <p>2016-01-01</p> <p>Efficient nutrient usage is a trait under universal selection. A substantial part of cellular resources is spent on making nucleotides. We thus expect preferential use of cheaper nucleotides especially in transcribed sequences, which are often amplified thousand-fold compared with genomic sequences. To test this hypothesis, we derive a mutation-selection-drift equilibrium model for nucleotide skews (strand-specific usage of ‘A' versus ‘T' and ‘G' versus ‘C'), which explains nucleotide skews across 1,550 prokaryotic genomes as a consequence of selection on efficient resource usage. Transcription-related selection generally favours the cheaper nucleotides ‘U' and ‘C' at synonymous sites. However, the information encoded in mRNA is further amplified through translation. Due to unexpected <span class="hlt">trade</span>-offs in the codon table, cheaper nucleotides encode on average energetically more expensive amino acids. These <span class="hlt">trade</span>-offs apply to both strand-specific nucleotide usage and GC content, causing a universal bias towards the more expensive nucleotides ‘A' and ‘G' at non-synonymous coding sites. PMID:27098217</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/11623721','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/11623721"><span>Globalization and the <span class="hlt">trade</span> in human body parts.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Harrison, T</p> <p>1999-02-01</p> <p>Since the early 1980s, the number and variety of organ transplantations has increased enormously worldwide. Accompanying this increase has been the emergence of a market for human body parts. This paper argues that, while the <span class="hlt">trade</span> in human body parts is conditioned by technological advances, it must be understood in the broader context of globalization, specifically the extension and intensification of a capitalist mode of exchange. In this regard, it is argued that the <span class="hlt">trade</span> in human body parts mirrors the "normal" system of unequal exchanges that mark other forms of <span class="hlt">trade</span> between the developed and undeveloped <span class="hlt">regions</span> of the world.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/26642202','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/26642202"><span>Inequalities in Global <span class="hlt">Trade</span>: A Cross-Country Comparison of <span class="hlt">Trade</span> Network Position, Economic Wealth, Pollution and Mortality.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Prell, Christina; Sun, Laixiang; Feng, Kuishuang; Myroniuk, Tyler W</p> <p>2015-01-01</p> <p>In this paper we investigate how structural patterns of international <span class="hlt">trade</span> give rise to emissions inequalities across countries, and how such inequality in turn impact countries' mortality rates. We employ Multi-<span class="hlt">regional</span> Input-Output analysis to distinguish between sulfur-dioxide (SO2) emissions produced within a country's boarders (production-based emissions) and emissions triggered by consumption in other countries (consumption-based emissions). We use social network analysis to capture countries' level of integration within the global <span class="hlt">trade</span> network. We then apply the Prais-Winsten panel estimation technique to a panel data set across 172 countries over 20 years (1990-2010) to estimate the relationships between countries' level of integration and SO2 emissions, and the impact of <span class="hlt">trade</span> integration and SO2 emission on mortality rates. Our findings suggest a positive, (log-) linear relationship between a country's level of integration and both kinds of emissions. In addition, although more integrated countries are mainly responsible for both forms of emissions, our findings indicate that they also tend to experience lower mortality rates. Our approach offers a unique combination of social network analysis with multiregional input-output analysis, which better operationalizes intuitive concepts about global <span class="hlt">trade</span> and <span class="hlt">trade</span> structure.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/20640525','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/20640525"><span>Evolutionary behaviour, <span class="hlt">trade</span>-offs and cyclic and chaotic population dynamics.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Hoyle, Andy; Bowers, Roger G; White, Andy</p> <p>2011-05-01</p> <p>Many studies of the evolution of life-history traits assume that the underlying population dynamical attractor is stable point equilibrium. However, evolutionary outcomes can change significantly in different circumstances. We present an analysis based on adaptive dynamics of a discrete-time demographic model involving a <span class="hlt">trade</span>-off whose shape is also an important determinant of evolutionary behaviour. We derive an explicit expression for the fitness in the cyclic <span class="hlt">region</span> and consequently present an adaptive dynamic analysis which is algebraic. We do this fully in the <span class="hlt">region</span> of 2-cycles and (using a symbolic package) almost fully for 4-cycles. Simulations illustrate and verify our results. With equilibrium population dynamics, <span class="hlt">trade</span>-offs with accelerating costs produce a continuously stable strategy (CSS) whereas <span class="hlt">trade</span>-offs with decelerating costs produce a non-ES repellor. The transition to 2-cycles produces a discontinuous change: the appearance of an intermediate <span class="hlt">region</span> in which branching points occur. The size of this <span class="hlt">region</span> decreases as we move through the <span class="hlt">region</span> of 2-cycles. There is a further discontinuous fall in the size of the branching <span class="hlt">region</span> during the transition to 4-cycles. We extend our results numerically and with simulations to higher-period cycles and chaos. Simulations show that chaotic population dynamics can evolve from equilibrium and vice-versa.</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/2017AGUFMGC13B0776V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMGC13B0776V"><span>Effects of the international soybean <span class="hlt">trade</span> on the dynamics of Gross Primary Productivity in soybean-producing <span class="hlt">regions</span> in China and Brazil</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Viña, A.; Silva, R. F. B. D.; Yang, H.; Liu, J.</p> <p>2017-12-01</p> <p>The international <span class="hlt">trade</span> of agricultural commodities, such as soybean, is driven by a series of pull and push factors linked to market demand. These in turn fluctuate based on changes in economic affluence, infrastructure development, and socioeconomic homogenization, among others, in both sending and receiving systems. While many studies have analyzed some of these push/pull factors and their environmental effects in either sending or receiving systems, few studies have assessed these effects simultaneously in both sending and receiving systems. This study evaluates the effects of the soybean <span class="hlt">trade</span> between Brazil and China on the spatio-temporal patterns of gross primary productivity (GPP) in both sending and receiving systems. The GPP is a measure of the amount of biomass produced through photosynthesis across space and through time. This metric is directly related with the amount of carbon that is sequestered from the atmosphere, and thus is related with the impacts of land use/cover dynamics on global climate change. The spatio-temporal patterns of both GPP and land use/cover were evaluated simultaneously in two soybean-producing <span class="hlt">regions</span> (state of Mato Grosso in Brazil, and Heilongjiang province in China) through the use of surface reflectance data acquired by the Moderate Resolution Imaging Spectroradiometer (MODIS) onboard NASA's Terra satellite, combined with a production efficiency model (PEM) entirely based on remotely sensed data. Results from this analysis provide new insights on the consequences of the international <span class="hlt">trade</span> at local/<span class="hlt">regional</span> scales, and allow assessing how changes in market demand for agricultural commodities may generate drastic environmental effects in both sending and receiving systems, with global implications on carbon sequestration and thus on climate change.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24681223','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24681223"><span>Description and analysis of the poultry <span class="hlt">trading</span> network in the Lake Alaotra <span class="hlt">region</span>, Madagascar: implications for the surveillance and control of Newcastle disease.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rasamoelina-Andriamanivo, H; Duboz, R; Lancelot, R; Maminiaina, O F; Jourdan, M; Rakotondramaro, T M C; Rakotonjanahary, S N; de Almeida, R Servan; Rakotondravao; Durand, B; Chevalier, V</p> <p>2014-07-01</p> <p>Madagascar's 36.5-million-head poultry industry holds a foremost place in its economy and the livelihood of its people. Unfortunately, regular Newcastle disease outbreaks associated with high mortality causes high losses for smallholders and threatens their livelihood. Therefore, Madagascar is seeking concrete, achievable and sustainable methods for the surveillance and the control of Newcastle disease. In this paper, we present and analyze the results of a field study conducted in Madagascar between December 2009 and December 2010. The study area was the Lac Alaotra <span class="hlt">region</span>, a landlocked area in the north-eastern part of the country's center. Poultry <span class="hlt">trading</span> is suspected of playing a major role in the spread of avian diseases, especially in developing countries characterized by many live-bird markets and middlemen. Therefore, the goals of our study were to: (i) describe and analyze smallholders' poultry <span class="hlt">trading</span> network in the Lake Alaotra <span class="hlt">region</span> using social network analysis; (ii) assess the role of the network in the spread of Newcastle disease; and (iii) propose the implementation of a targeted disease surveillance based on the characteristics of the poultry <span class="hlt">trading</span> network. We focused our field study on the harvesting of two data sets. The first is a complete description of the poultry <span class="hlt">trading</span> network in the landlocked area of Lac Alaotra, including a description of the poultry movements between groups of villages. The second set of data measures the occurrence of outbreaks in the same area by combining a participatory approach with an event-based surveillance method. These data were used to determine the attributes of the network, and to statistically assess the association between the position of nodes and the occurrence of outbreaks. By using social network analysis techniques combined with a classification method and a logistic model, we finally identified 3 nodes (set of villages), of the 387 in the initial network, to focus on for surveillance and control</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/29328652','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/29328652"><span><span class="hlt">Trade</span>-Induced Atmospheric Mercury Deposition over China and Implications for Demand-Side Controls.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Chen, Long; Meng, Jing; Liang, Sai; Zhang, Haoran; Zhang, Wei; Liu, Maodian; Tong, Yindong; Wang, Huanhuan; Wang, Wei; Wang, Xuejun; Shu, Jiong</p> <p>2018-02-20</p> <p>Mercury (Hg) is of global concern because of its adverse effects on humans and the environment. In addition to long-range atmospheric transport, Hg emissions can be geographically relocated through economic <span class="hlt">trade</span>. Here, we investigate the effect of China's interregional <span class="hlt">trade</span> on atmospheric Hg deposition over China, using an atmospheric transport model and multiregional input-output analysis. In general, total atmospheric Hg deposition over China is 408.8 Mg yr -1 , and 32% of this is embodied in China's interregional <span class="hlt">trade</span>, with the hotspots occurring over Gansu, Henan, Hebei, and Yunnan provinces. Interprovincial <span class="hlt">trade</span> considerably redistributes atmospheric Hg deposition over China, with a range in deposition flux from -104% to +28%. Developed <span class="hlt">regions</span>, such as the Yangtze River Delta (Shanghai, Jiangsu, and Zhejiang) and Guangdong, avoid Hg deposition over their geographical boundaries, instead causing additional Hg deposition over developing provinces. Bilateral interaction among provinces is strong over some <span class="hlt">regions</span>, suggesting a need for joint mitigation, such as the Jing-Jin-Ji <span class="hlt">region</span> (Beijing, Tianjin, and Hebei) and the Yangtze River Delta. Transferring advanced technology from developed <span class="hlt">regions</span> to their developing <span class="hlt">trade</span> partners would be an effective measure to mitigate China's Hg pollution. Our findings are relevant to interprovincial efforts to reduce trans-boundary Hg pollution in China.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/24102909','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/24102909"><span><span class="hlt">Trade</span> policy and obesity prevention: challenges and innovation in the Pacific Islands.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Snowdon, W; Thow, A M</p> <p>2013-11-01</p> <p>The Pacific Island countries experience some of the highest rates of obesity in the world in part due to substantial dietary changes that mirror changes in the food supply in the <span class="hlt">region</span>. Economic and political ties, donor aid, and <span class="hlt">trade</span> links are key drivers of the changing availability and accessibility of processed and imported foods. Pacific Island countries have been innovative in developing <span class="hlt">trade</span>-related policy approaches to create a less obesogenic food environment. Taxation-based approaches that affect pricing in the <span class="hlt">region</span> include increased import and excise tariffs on sugared beverages and other high-sugar products, monosodium glutamate, and palm oil and lowered tariffs on fruits and vegetables. Other approaches highlight some higher-fat products through labeling and controlling the supply of high-fat meats. The bans on high-fat turkey tails and mutton flaps highlight the politics, <span class="hlt">trade</span> agreements and donor influences that can be significant barriers to the pursuit of policy options. Countries that are not signatories to <span class="hlt">trade</span> agreements may have more policy space for innovative action. However, potential effectiveness and practicality require consideration. The health sector's active engagement in the negotiation of <span class="hlt">trade</span> agreements is a key way to support healthier <span class="hlt">trade</span> in the <span class="hlt">region</span>. © 2013 The Authors. Obesity Reviews published by John Wiley & Sons Ltd on behalf of the International Association for the Study of Obesity.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018ApJ...853..164N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018ApJ...853..164N"><span>A Changing <span class="hlt">Wind</span> Collision</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nazé, Yaël; Koenigsberger, Gloria; Pittard, Julian M.; Parkin, Elliot Ross; Rauw, Gregor; Corcoran, Michael F.; Hillier, D. John</p> <p>2018-02-01</p> <p>We report on the first detection of a global change in the X-ray emitting properties of a wind–<span class="hlt">wind</span> collision, thanks to XMM-Newton observations of the massive Small Magellenic Cloud (SMC) system HD 5980. While its light curve had remained unchanged between 2000 and 2005, the X-ray flux has now increased by a factor of ∼2.5, and slightly hardened. The new observations also extend the observational coverage over the entire orbit, pinpointing the light-curve shape. It has not varied much despite the large overall brightening, and a tight correlation of fluxes with orbital separation is found without any hysteresis effect. Moreover, the absence of eclipses and of absorption effects related to orientation suggests a large size for the X-ray emitting <span class="hlt">region</span>. Simple analytical models of the wind–<span class="hlt">wind</span> collision, considering the varying <span class="hlt">wind</span> properties of the eruptive component in HD 5980, are able to reproduce the recent hardening and the flux-separation relationship, at least qualitatively, but they predict a hardening at apastron and little change in mean flux, contrary to observations. The brightness change could then possibly be related to a recently theorized phenomenon linked to the varying strength of thin-shell instabilities in shocked <span class="hlt">wind</span> <span class="hlt">regions</span>. Based on XMM-Newton and Chandra data.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MNRAS.471.1488N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MNRAS.471.1488N"><span>Centrifugally driven <span class="hlt">winds</span> from protostellar accretion discs - I. Formulation and initial results</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Nolan, C. A.; Salmeron, R.; Federrath, C.; Bicknell, G. V.; Sutherland, R. S.</p> <p>2017-10-01</p> <p>Protostellar discs play an important role in star formation, acting as the primary mass reservoir for accretion on to young stars and regulating the extent to which angular momentum and gas is released back into stellar nurseries through the launching of powerful disc <span class="hlt">winds</span>. In this study, we explore how disc structure relates to the properties of the <span class="hlt">wind</span>-launching <span class="hlt">region</span>, mapping out the <span class="hlt">regions</span> of protostellar discs where <span class="hlt">wind</span> launching could be viable. We combine a series of 1.5D semi-analytic, steady-state, vertical disc-<span class="hlt">wind</span> solutions into a radially extended 1+1.5D model, incorporating all three diffusion mechanisms (Ohm, Hall and ambipolar). We observe that the majority of mass outflow via disc <span class="hlt">winds</span> occurs over a radial width of a fraction of an astronomical unit, with outflow rates attenuating rapidly on either side. We also find that the mass accretion rate, magnetic field strength and surface density profile each have significant effects on both the location of the <span class="hlt">wind</span>-launching <span class="hlt">region</span> and the ejection/accretion ratio \\dot{M}_out/\\dot{M}_in. Increasing either the accretion rate or the magnetic field strength corresponds to a shift of the <span class="hlt">wind</span>-launching <span class="hlt">region</span> to smaller radii and a decrease in \\dot{M}_out/\\dot{M}_in, while increasing the surface density corresponds to launching <span class="hlt">regions</span> at larger radii with increased \\dot{M}_out/\\dot{M}_in. Finally, we discover a class of disc <span class="hlt">winds</span> containing an ineffective launching configuration at intermediate radii, leading to two radially separated <span class="hlt">regions</span> of <span class="hlt">wind</span> launching and diminished \\dot{M}_out/\\dot{M}_in. We find that the <span class="hlt">wind</span> locations and ejection/accretion ratio are consistent with current observational and theoretical estimates.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2005SPIE.5997..184S','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2005SPIE.5997..184S"><span>A quadranomial real options model for evaluation of emissions <span class="hlt">trading</span> and technology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Sarkis, Joseph; Tamarkin, Maurry</p> <p>2005-11-01</p> <p>Green house gas (GHG) emissions have been tied to global climate change. One popular policy instrument that seems to have gained credibility with explicit mention of its application in the Kyoto Protocol is the use of permit <span class="hlt">trading</span> and cap-and-<span class="hlt">trade</span> mechanisms. Organizations functioning within this environment will need to manage their resources appropriately to remain competitive. Organizations will either have the opportunity to purchase emissions credits (offsets) from a market <span class="hlt">trading</span> scheme or seek to reduce their emissions through different measures. Some measures may include investment in new technologies that will reduce their reliance on GHG emitting practices. In many countries, large organizations and institutions generate their own power to operate their facilities. Much of this power is generated (or bought) from GHG producing technology. Specific renewable energy sources such as <span class="hlt">wind</span> and solar photovoltaic technology may become more feasible alternatives available to a large percentage of these organizations if they are able to take advantage and incorporate the market for GHG emissions <span class="hlt">trading</span> in their analyses. To help organizations evaluate investment in these renewable energy technologies we introduce a real options based model that will take into consideration uncertainties associated with the technology and those associated with the GHG <span class="hlt">trading</span> market. The real options analysis will consider both the stochastic (uncertainty) nature of the exercise price of the technology and the stochastic nature of the market <span class="hlt">trading</span> price of the GHG emissions.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1330585','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1330585"><span>Offshore <span class="hlt">Wind</span> Market and Economic 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>Hamilton, Bruce Duncan</p> <p>2014-08-27</p> <p>This report is the third annual assessment of the U.S. offshore <span class="hlt">wind</span> market. It includes the following major sections: Section 1: key data on developments in the offshore <span class="hlt">wind</span> technology sector and the global development of offshore <span class="hlt">wind</span> projects, with a particular focus on progress in the United States; Section 2: analysis of policy developments at the federal and state levels that have been effective in advancing offshore <span class="hlt">wind</span> deployment in the United States; Section 3: analysis of actual and projected economic impact, including <span class="hlt">regional</span> development and job creation; Section 4: analysis of developments in relevant sectors of the economymore » with the potential to affect offshore <span class="hlt">wind</span> deployment in the United States« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22243129','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22243129"><span>Ecological network analysis on global virtual water <span class="hlt">trade</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Yang, Zhifeng; Mao, Xufeng; Zhao, Xu; Chen, Bin</p> <p>2012-02-07</p> <p>Global water interdependencies are likely to increase with growing virtual water <span class="hlt">trade</span>. To address the issues of the indirect effects of water <span class="hlt">trade</span> through the global economic circulation, we use ecological network analysis (ENA) to shed insight into the complicated system interactions. A global model of virtual water flow among agriculture and livestock production <span class="hlt">trade</span> in 1995-1999 is also built as the basis for network analysis. Control analysis is used to identify the quantitative control or dependency relations. The utility analysis provides more indicators for describing the mutual relationship between two <span class="hlt">regions</span>/countries by imitating the interactions in the ecosystem and distinguishes the beneficiary and the contributor of virtual water <span class="hlt">trade</span> system. Results show control and utility relations can well depict the mutual relation in <span class="hlt">trade</span> system, and direct observable relations differ from integral ones with indirect interactions considered. This paper offers a new way to depict the interrelations between <span class="hlt">trade</span> components and can serve as a meaningful start as we continue to use ENA in providing more valuable implications for freshwater study on a global scale.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19820005750','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19820005750"><span>Compensation for use of monthly-averaged <span class="hlt">winds</span> in numerical modeling</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Parkinson, C. L.</p> <p>1981-01-01</p> <p>Ratios R of the monthly averaged <span class="hlt">wind</span> speeds to the magnitudes of the monthly averaged <span class="hlt">wind</span> vectors are presented over a 41 x 41 grid covering the southern Ocean and the Antarctic continent. The ratio is found to vary from 1 to over 1000, with an average value of 1.86. These ratios R are relevant for converting from sensible and latent heats calculated with mean monthly data to those calculated with 12 hourly data. The corresponding ratios alpha for <span class="hlt">wind</span> stress, along with the angle deviations involved, are also presented over the same 41 x 41 grid. The values of alpha generally exceed those for R and average 2.66. <span class="hlt">Regions</span> in zones of variable <span class="hlt">wind</span> directions have larger R and alpha ratios, over the ice-covered portions of the southern Ocean averaging 2.74 and 4.35 for R and alpha respectively. Thus adjustments to compensate for the use of mean monthly <span class="hlt">wind</span> velocities should be stronger for <span class="hlt">wind</span> stress than for turbulent heats and stronger over ice covered <span class="hlt">regions</span> than over <span class="hlt">regions</span> with more persistent <span class="hlt">wind</span> directions, e.g., those in the belt of mid-latitude westerlies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.nrel.gov/grid/wwsis.html','SCIGOVWS'); return false;" href="https://www.nrel.gov/grid/wwsis.html"><span>Western <span class="hlt">Wind</span> and Solar Integration Study | Grid Modernization | NREL</span></a></p> <p><a target="_blank" href="http://www.science.gov/aboutsearch.html">Science.gov Websites</a></p> <p></p> <p></p> <p>Western <em><span class="hlt">Wind</span></em> and Solar Integration Study Western <em><span class="hlt">Wind</span></em> and Solar Integration Study Can we integrate large amounts of <em><span class="hlt">wind</span></em> and solar energy into the electric power system of the West? That's the question explored by the Western <em><span class="hlt">Wind</span></em> and Solar Integration Study, one of the largest such <span class="hlt">regional</span> studies to date</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814547D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814547D"><span>Improvement of background solar <span class="hlt">wind</span> predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dálya, Zsuzsanna; Opitz, Andrea</p> <p>2016-04-01</p> <p>In order to estimate the solar <span class="hlt">wind</span> properties at any heliospheric positions propagation tools use solar measurements as input data. The ballistic method extrapolates in-situ solar <span class="hlt">wind</span> observations to the target position. This works well for undisturbed solar <span class="hlt">wind</span>, while solar <span class="hlt">wind</span> disturbances such as Corotating Interaction <span class="hlt">Regions</span> (CIRs) and Coronal Mass Ejections (CMEs) need more consideration. We are working on dedicated ICME lists to clean these signatures from the input data in order to improve our prediction accuracy. These ICME lists are created from several heliospheric spacecraft measurements: ACE, <span class="hlt">WIND</span>, STEREO, SOHO, MEX and VEX. As a result, we are able to filter out these events from the time series. Our corrected predictions contribute to the investigation of the quiet solar <span class="hlt">wind</span> and space weather studies.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19900061730&hterms=viking+lander&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dviking%2Blander','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19900061730&hterms=viking+lander&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D10%26Ntt%3Dviking%2Blander"><span>Observations of Martian surface <span class="hlt">winds</span> at the Viking Lander 1 site</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Murphy, James R.; Leovy, Conway B.; Tillman, James E.</p> <p>1990-01-01</p> <p>Martian surface <span class="hlt">winds</span> at the Viking Lander 1 have been reconstructed using signals from partially failed <span class="hlt">wind</span> instrumentation. <span class="hlt">Winds</span> during early summer were controlled by <span class="hlt">regional</span> topography, and then underwent a transition to a regime controlled by the Hadley circulation. Diurnal <span class="hlt">wind</span> oscillations were controlled primarily by <span class="hlt">regional</span> topography and boundary layer forcing, although a global mode may have been influencing them during two brief episodes. Semidiurnal <span class="hlt">wind</span> oscillations were controlled by the westward-propagating semidiurnal tide from sol 210 onward. Comparison of the synoptic variations at the two sites suggests that the same eastward propagating wave trains were present at both sites.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1261099','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1261099"><span>Advanced Offshore <span class="hlt">Wind</span> Energy - Atlantic Consortium</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>Kempton, Willett</p> <p></p> <p>This project developed relationships among the lead institution, U of Delaware, <span class="hlt">wind</span> industry participants from 11 companies, and two other universities in the <span class="hlt">region</span>. The participating <span class="hlt">regional</span> universities were University of Maryland and Old Dominion University. Research was carried out in six major areas: Analysis and documentation of extreme oceanic <span class="hlt">wind</span> events & their impact on design parameters, calibration of corrosivity estimates measured on a coastal turbine, measurment and modeling of tower structures, measurement and modeling of the tribology of major drive components, and gearbox conditioning monitoring using acoustic sensors. The project also had several educational goals, including establishing amore » course in <span class="hlt">wind</span> energy and training graduate students. Going beyond these goals, three new courses were developed, a graduate certificate program in <span class="hlt">wind</span> power was developed and approved, and an exchange program in <span class="hlt">wind</span> energy was established with Danish Technical University. Related to the installation of a Gamesa G90 turbine on campus and a Gamesa-UD research program established in part due to this award, several additional research projects have been carried out based on mutual industry-university interests, and funded by turbine revenues. This award and the Gamesa partnership have jointly led to seven graduate students receiving full safety and climb training, to become “research climbers” as part of their <span class="hlt">wind</span> power training, and contributing to on-turbine research. As a result of the educational program, already six graduate students have taken jobs in the US <span class="hlt">wind</span> industry.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..150a2020P','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..150a2020P"><span><span class="hlt">Wind</span> speed and power characteristics of Kalasin province, Thailand</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Polnumtiang, Supachai; Tangchaichit, Kiatfa</p> <p>2018-05-01</p> <p>This paper presents a <span class="hlt">wind</span> energy assessment of Kalasin province in the Upper North-Eastern <span class="hlt">region</span> of Thailand. Four year <span class="hlt">wind</span> data were recorded continuously from January 2012 to December 2015 at different heights of 60, 90 and 120 m above ground level (AGL). The mean <span class="hlt">wind</span> speeds were found to be 3.14, 3.63 and 3.94 m/s at 60, 90 and 120 m AGL, respectively. The majority of <span class="hlt">wind</span> directions for this <span class="hlt">region</span> are distributed from the East to South directions. The highest <span class="hlt">wind</span> power density was observed in the summer season, followed by winter and rainy seasons, in order. Four commercial <span class="hlt">wind</span> turbines were selected to estimate energy yield output using the WAsP 10.0 software application; the results show that VESTAS with rated power of 2.0 MW was estimated to give 2,747 MWh/year with the highest capacity factor of 15.68%.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016EGUGA..1814085C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..1814085C"><span>The weather roulette: assessing the economic value of seasonal <span class="hlt">wind</span> speed predictions</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Christel, Isadora; Cortesi, Nicola; Torralba-Fernandez, Veronica; Soret, Albert; Gonzalez-Reviriego, Nube; Doblas-Reyes, Francisco</p> <p>2016-04-01</p> <p>Climate prediction is an emerging and highly innovative research area. For the <span class="hlt">wind</span> energy sector, predicting the future variability of <span class="hlt">wind</span> resources over the coming weeks or seasons is especially relevant to quantify operation and maintenance logistic costs or to inform energy <span class="hlt">trading</span> decision with potential cost savings and/or economic benefits. Recent advances in climate predictions have already shown that probabilistic forecasting can improve the current prediction practices, which are based in the use of retrospective climatology and the assumption that what happened in the past is the best estimation of future conditions. Energy decision makers now have this new set of climate services but, are they willing to use them? Our aim is to properly explain the potential economic benefits of adopting probabilistic predictions, compared with the current practice, by using the weather roulette methodology (Hagedorn & Smith, 2009). This methodology is a diagnostic tool created to inform in a more intuitive and relevant way about the skill and usefulness of a forecast in the decision making process, by providing an economic and financial oriented assessment of the benefits of using a particular forecast system. We have selected a <span class="hlt">region</span> relevant to the energy stakeholders where the predictions of the EUPORIAS climate service prototype for the energy sector (RESILIENCE) are skillful. In this <span class="hlt">region</span>, we have applied the weather roulette to compare the overall prediction success of RESILIENCE's predictions and climatology illustrating it as an effective interest rate, an economic term that is easier to understand for energy stakeholders.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2010-12-21/pdf/2010-31969.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2010-12-21/pdf/2010-31969.pdf"><span>75 FR 80038 - Notice of Meetings of the Agricultural Policy Advisory Committee for <span class="hlt">Trade</span> and the Agricultural...</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2010-12-21</p> <p>... the <span class="hlt">trade</span> policy of the United States. Topics will include Doha Round negotiations in the World <span class="hlt">Trade</span> Organization (WTO), WTO accession negotiations, and negotiations in bilateral and <span class="hlt">regional</span> free <span class="hlt">trade</span>... <span class="hlt">trade</span> agreement negotiations and/or other matters concerning the administration of <span class="hlt">trade</span> policy, the...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2016AGUFM.A13A0215X','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016AGUFM.A13A0215X"><span>High resolution <span class="hlt">regional</span> climate simulation of the Hawaiian Islands - Validation of the historical run from 2003 to 2012</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Xue, L.; Newman, A. J.; Ikeda, K.; Rasmussen, R.; Clark, M. P.; Monaghan, A. J.</p> <p>2016-12-01</p> <p>A high-resolution (a 1.5 km grid spacing domain nested within a 4.5 km grid spacing domain) 10-year <span class="hlt">regional</span> climate simulation over the entire Hawaiian archipelago is being conducted at the National Center for Atmospheric Research (NCAR) using the Weather Research and Forecasting (WRF) model version 3.7.1. Numerical sensitivity simulations of the Hawaiian Rainband Project (HaRP, a filed experiment from July to August in 1990) showed that the simulated precipitation properties are sensitive to initial and lateral boundary conditions, sea surface temperature (SST), land surface models, vertical resolution and cloud droplet concentration. The validations of model simulated statistics of the <span class="hlt">trade</span> <span class="hlt">wind</span> inversion, temperature, <span class="hlt">wind</span> field, cloud cover, and precipitation over the islands against various observations from soundings, satellites, weather stations and rain gauges during the period from 2003 to 2012 will be presented at the meeting.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23581666','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23581666"><span>The high price of "free" <span class="hlt">trade</span>: U.S. <span class="hlt">trade</span> agreements and access to medicines.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Lopert, Ruth; Gleeson, Deborah</p> <p>2013-01-01</p> <p>The United States' pursuit of increasingly TRIPS-Plus levels of intellectual property protection for medicines in bilateral and <span class="hlt">regional</span> <span class="hlt">trade</span> agreements is well recognized. Less so, however, are U.S. efforts through these agreements to influence and constrain the pharmaceutical coverage programs of its <span class="hlt">trading</span> partners. Although arguably unsuccessful in the Australia- U.S. Free <span class="hlt">Trade</span> Agreement (AUSFTA), the U.S. nevertheless succeeded in its bilateral FTA with South Korea (KORUS) in establishing prescriptive provisions pertaining to the operation of coverage and reimbursement programs for medicines and medical devices, which have the potential to adversely impact future access in that country. More recently, draft texts leaked from the current Trans Pacific Partnership Agreement (TPPA) negotiations show that U.S. objectives include not only AUSFTA-Plus and KORUS-Plus IP provisions but also ambitious inroads into the domestic health programs of its TPPA partners. This highlights the apparent conflict between <span class="hlt">trade</span> goals - pursued through multilateral legal instruments to promote economic "health"- and public health objectives, such as the development of treatments for neglected diseases, the pursuit of efficiency and equity in priority setting, and the procurement of medicines at prices that reflect their therapeutic value and facilitate affordable access. © 2013 American Society of Law, Medicine & Ethics, Inc.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19800010289','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19800010289"><span>MOD-1 <span class="hlt">Wind</span> Turbine Generator Analysis and Design Report, Volume 2</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p></p> <p>1979-01-01</p> <p>The MOD-1 detail design is appended. The supporting analyses presented include a parametric system <span class="hlt">trade</span> study, a verification of the computer codes used for rotor loads analysis, a metal blade study, and a definition of the design loads at each principal <span class="hlt">wind</span> turbine generator interface for critical loading conditions. Shipping and assembly requirements, composite blade development, and electrical stability are also discussed.</p> </li> </ol> <div class="pull-right"> <ul class="pagination"> <li><a href="#" onclick='return showDiv("page_1");'>«</a></li> <li><a href="#" onclick='return showDiv("page_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/2016EGUGA..18.4935N','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2016EGUGA..18.4935N"><span>China's international <span class="hlt">trade</span> and air pollution: 2000 - 2009</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ni, Ruijing; Lin, Jintai; Pan, Da; Wang, Jingxu; Yan, Yingying; Zhang, Qiang</p> <p>2016-04-01</p> <p>As the world's top <span class="hlt">trading</span> country, China is now the most polluted country. However, a large portion of pollution produced in China is associated with its production of goods for foreign consumption via international <span class="hlt">trade</span>. Along with China's rapid economic growth in recent years, its economic-<span class="hlt">trade</span> structure and volume has been changing all the time, resulting in large changes in total emissions and the shares of <span class="hlt">trade</span>-related emissions. Here, we assess the influence of China's changing total and export-related emissions between 2000 and 2009 on its atmospheric pollution loadings and transport, by exploiting simulations of a global chemical transport model GEOS-Chem. We find that both air pollution related to Chinese exports (PRE) which including nitrogen oxides (NOx), sulfur dioxide (SO2), carbon monoxide (CO), black carbon (BC), and primary organic aerosol (POA), and its share in total Chinese pollution have experienced continuous rapid growth until 2007, exposing more and more people to severely polluted air. After 2007, PRE decreases due to strengthened emission controls accompanied by declined exports as a result of the global financial crisis. Although production for exports contribute less than 35% SO2 over China in any year, the increasing trend of <span class="hlt">trade</span>-related SO2 contributes 51% of integral trend. The changing PRE of China also affects its downwind <span class="hlt">regions</span> such as the western United States. The contribution of export-related Chinese pollution to surface sulfate concentrations over the western United States has increased from 3% in 2000 to 12% in 2007. Overall, we find that the interannual variation of <span class="hlt">trade</span> and associated production is a critical factor driving the trend of pollution over China and its downwind <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25213212','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25213212"><span><span class="hlt">Trade</span> and investment liberalization and Asia's noncommunicable disease epidemic: a synthesis of data and existing literature.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Baker, Phillip; Kay, Adrian; Walls, Helen</p> <p>2014-09-12</p> <p><span class="hlt">Trade</span> and investment liberalization (<span class="hlt">trade</span> liberalization) can promote or harm health. Undoubtedly it has contributed, although unevenly, to Asia's social and economic development over recent decades with resultant gains in life expectancy and living standards. In the absence of public health protections, however, it is also a significant upstream driver of non-communicable diseases (NCDs) including cardiovascular disease, cancer and diabetes through facilitating increased consumption of the 'risk commodities' tobacco, alcohol and ultra-processed foods, and by constraining access to NCD medicines. In this paper we describe the NCD burden in Asian countries, trends in risk commodity consumption and the processes by which <span class="hlt">trade</span> liberalization has occurred in the <span class="hlt">region</span> and contributed to these trends. We further establish pressing questions for future research on strengthening regulatory capacity to address <span class="hlt">trade</span> liberalization impacts on risk commodity consumption and health. A semi-structured search of scholarly databases, institutional websites and internet sources for academic and grey literature. Data for descriptive statistics were sourced from Euromonitor International, the World Bank, the World Health Organization, and the World <span class="hlt">Trade</span> Organization. Consumption of tobacco, alcohol and ultra-processed foods was prevalent in the <span class="hlt">region</span> and increasing in many countries. We find that <span class="hlt">trade</span> liberalization can facilitate increased <span class="hlt">trade</span> in goods, services and investments in ways that can promote risk commodity consumption, as well as constrain the available resources and capacities of governments to enact policies and programmes to mitigate such consumption. Intellectual property provisions of <span class="hlt">trade</span> agreements may also constrain access to NCD medicines. Successive layers of the evolving global and <span class="hlt">regional</span> <span class="hlt">trade</span> regimes including structural adjustment, multilateral <span class="hlt">trade</span> agreements, and preferential <span class="hlt">trade</span> agreements have enabled transnational corporations that</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19960003992','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19960003992"><span>Atmospheric response in aurora experiment: Observations of E and F <span class="hlt">region</span> neutral <span class="hlt">winds</span> in a <span class="hlt">region</span> of postmidnight diffuse aurora</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Larsen, M. F.; Marshall, T. R.; Mikkelsen, I. S.; Emery, B. A.; Christensen, A.; Kayser, D.; Hecht, J.; Lyons, L.; Walterscheid, R.</p> <p>1995-01-01</p> <p>The goal of the Atmospheric Response in Aurora (ARIA) experiment carried out at Poker Flat, Alaska, on March 3, 1992, was to determine the response of the neutral atmosphere to the long-lived, large-scale forcing that is characteristic of the diffuse aurora in the post midnight sector. A combination of chemical release rocket <span class="hlt">wind</span> measurements, instrumented rocket composition measurements, and ground-based optical measurements were used to characterize the response of the neutral atmosphere. The rocket measurements were made at the end of a 90-min period of strong Joule heating. We focus on the neutral <span class="hlt">wind</span> measurements made with the rocket. The forcing was determined by running the assimilated mapping of ionospheric electrodynamics (AMIE) analysis procedure developed at the National Center for Atmospheric Research. The <span class="hlt">winds</span> expected at the latitude and longitude of the experiment were calculated using the spectral thermospheric general circulation model developed at the Danish Meteorological Institute. Comparisons of the observations and the model suggest that the neutral <span class="hlt">winds</span> responded strongly in two height ranges. An eastward <span class="hlt">wind</span> perturbation of approximately 100 m/s developed between 140 and 200 km altitude with a peak near 160 km. A southwestward <span class="hlt">wind</span> with peak magnitude of approximately 150 m/s developed near 115 km altitude. The large amplitude <span class="hlt">winds</span> at the lower altitude are particularly surprising. They appear to be associated with the upward propagating semidiurnal tide. However, the amplitude is much larger than predicted by any of the tidal models, and the shear found just below the peak in the <span class="hlt">winds</span> was nominally unstable with a Richardson number of approximately 0.08.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013AGUFMSH52A..03V','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013AGUFMSH52A..03V"><span>The Slow and Fast Solar <span class="hlt">Wind</span> Boundary, Corotating Interaction <span class="hlt">Regions</span>, and Coronal Mass Ejection observations with Solar Probe Plus and Solar Orbiter (Invited)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Velli, M. M.</p> <p>2013-12-01</p> <p>The Solar Probe Plus and Solar Orbiter missions have as part of their goals to understand the source <span class="hlt">regions</span> of the solar <span class="hlt">wind</span> and of the heliospheric magnetic field. In the heliosphere, the solar <span class="hlt">wind</span> is made up of interacting fast and slow solar <span class="hlt">wind</span> streams as well as a clearly intermittent source of flow and field, arising from coronal mass ejections (CMEs). In this presentation a summary of the questions associated with the distibution of <span class="hlt">wind</span> speeds and magnetic fields in the inner heliosphere and their origin on the sun will be summarized. Where and how does the sharp gradient in speeds develop close to the Sun? Is the <span class="hlt">wind</span> source for fast and slow the same, and is there a steady component or is its origin always intermittent in nature? Where does the heliospheric current sheet form and how stable is it close to the Sun? What is the distribution of CME origins and is there a continuum from large CMEs to small blobs of plasma? We will describe our current knowledge and discuss how SPP and SO will contribute to a more comprehensive understanding of the sources of the solar <span class="hlt">wind</span> and magnetic fields in the heliosphere.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19980200853','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19980200853"><span><span class="hlt">Trade-Wind</span> Cloudiness and Climate</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Randall, David A.</p> <p>1997-01-01</p> <p>Closed Mesoscale Cellular Convection (MCC) consists of mesoscale cloud patches separated by narrow clear <span class="hlt">regions</span>. Strong radiative cooling occurs at the cloud top. A dry two-dimensional Bousinesq model is used to study the effects of cloud-top cooling on convection. Wide updrafts and narrow downdrafts are used to indicate the asymmetric circulations associated with the mesoscale cloud patches. Based on the numerical results, a conceptual model was constructed to suggest a mechanism for the formation of closed MCC over cool ocean surfaces. A new method to estimate the radioative and evaporative cooling in the entrainment layer of a stratocumulus-topped boundary layer has been developed. The method was applied to a set of Large-Eddy Simulation (LES) results and to a set of tethered-balloon data obtained during FIRE. We developed a statocumulus-capped marine mixed layer model which includes a parameterization of drizzle based on the use of a predicted Cloud Condensation Nuclei (CCN) number concentration. We have developed, implemented, and tested a very elaborate new stratiform cloudiness parameterization for use in GCMs. Finally, we have developed a new, mechanistic parameterization of the effects of cloud-top cooling on the entrainment rate.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://eric.ed.gov/?q=database+AND+economic&pg=6&id=EJ440231','ERIC'); return false;" href="https://eric.ed.gov/?q=database+AND+economic&pg=6&id=EJ440231"><span>Western Europe--A <span class="hlt">Trading</span> Game.</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>Cox, Ann Curtis</p> <p>1991-01-01</p> <p>Presents a geography program to show students why the European Community was formed. Involves student research of economic data, creation of a computer database on the European Community, and simulation of <span class="hlt">trading</span>. Emphasizes geographic themes of movement, <span class="hlt">region</span> formation, and change in response to economic forces. Includes game rules, sample…</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/22848505','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/22848505"><span><span class="hlt">Wind</span> and wildlife in the Northern Great Plains: identifying low-impact areas for <span class="hlt">wind</span> development.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Fargione, Joseph; Kiesecker, Joseph; Slaats, M Jan; Olimb, Sarah</p> <p>2012-01-01</p> <p><span class="hlt">Wind</span> energy offers the potential to reduce carbon emissions while increasing energy independence and bolstering economic development. However, <span class="hlt">wind</span> energy has a larger land footprint per Gigawatt (GW) than most other forms of energy production and has known and predicted adverse effects on wildlife. The Northern Great Plains (NGP) is home both to some of the world's best <span class="hlt">wind</span> resources and to remaining temperate grasslands, the most converted and least protected ecological system on the planet. Thus, appropriate siting and mitigation of <span class="hlt">wind</span> development is particularly important in this <span class="hlt">region</span>. Steering energy development to disturbed lands with low wildlife value rather than placing new developments within large and intact habitats would reduce impacts to wildlife. Goals for <span class="hlt">wind</span> energy development in the NGP are roughly 30 GW of nameplate capacity by 2030. Our analyses demonstrate that there are large areas where <span class="hlt">wind</span> development would likely have few additional impacts on wildlife. We estimate there are ∼1,056 GW of potential <span class="hlt">wind</span> energy available across the NGP on areas likely to have low-impact for biodiversity, over 35 times development goals. New policies and approaches will be required to guide <span class="hlt">wind</span> energy development to low-impact areas.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1981EOSTr..62Q..33R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1981EOSTr..62Q..33R"><span>RACOONs amass <span class="hlt">wind</span> data</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Richman, Barbara T.</p> <p></p> <p>Balloons, not furry little animals, are being developed to provide new, inexpensive methods for gathering weather data in the tropics.RACOON—short for radiation-controlled balloon—is a zero-pressure balloon which will be used to provide stratospheric <span class="hlt">wind</span> data for equatorial <span class="hlt">regions</span>, according to the National Center for Atmospheric Research. These data are unavailable from satellites. Currently, the global rocket network gathers tropical <span class="hlt">wind</span> measurements for weather forecasting; however, the network is being phased out.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/1982JGR....8710025L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/1982JGR....8710025L"><span><span class="hlt">Wind</span> streaks in Tharsis and Elysium - Implications for sediment transport by slope <span class="hlt">winds</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, S. W.; Thomas, P. C.; Veverka, J.</p> <p>1982-11-01</p> <p>Detailed maps of <span class="hlt">wind</span> streaks in Tharsis and Elysium have been compiled from Viking Orbiter observations spanning one complete Martian year. The streak pattern is controlled by slope <span class="hlt">winds</span> on the central volcanoes and on the flanks of the Tharsis bulge, while the global circulation dominates in Elysium. Dust erosion by downslope <span class="hlt">winds</span> occurs over much of Tharsis and in the vicinity of Elysium Mons; this process is effective even at the low atmospheric pressures found near the summits of the large volcanoes. Erosional streaks are largely absent in Elysium Planitia; net deposition of dust might have occurred during the period of the observations. Surface properties such as slope, thermal inertia, and roughness may influence the efficiency of slope <span class="hlt">wind</span> production sufficiently to account for the pronounced differences in streak types and patterns present in these two <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/25839733','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/25839733"><span>Evolution, the loss of diversity and the role of <span class="hlt">trade</span>-offs.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Best, Alex; Bowers, Roger; White, Andy</p> <p>2015-06-01</p> <p>We investigate how the loss of previously evolved diversity in host resistance to disease is dependent on the complexity of the underlying evolutionary <span class="hlt">trade</span>-off. Working within the adaptive dynamics framework, using graphical tools (pairwise invasion plots, PIPs; trait evolution plots, TEPs) and algebraic analysis we consider polynomial <span class="hlt">trade</span>-offs of increasing degree. Our focus is on the evolutionary trajectory of the dimorphic population after it has been attracted to an evolutionary branching point. We show that for sufficiently complex <span class="hlt">trade</span>-offs (here, polynomials of degree three or higher) the resulting invasion boundaries can form closed 'oval' areas of invadability and strategy coexistence. If no attracting singular strategies exist within this <span class="hlt">region</span>, then the population is destined to evolve outside of the <span class="hlt">region</span> of coexistence, resulting in the loss of one strain. In particular, the loss of diversity in this model always occurs in such a way that the remaining strain is not attracted back to the branching point but to an extreme of the <span class="hlt">trade</span>-off, meaning the diversity is lost forever. We also show similar results for a non-polynomial but complex <span class="hlt">trade</span>-off, and for a different eco-evolutionary model. Our work further highlights the importance of <span class="hlt">trade</span>-offs to evolutionary behaviour. Copyright © 2015 Elsevier Inc. All rights reserved.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.epa.gov/emissions-trading-resources/nox-budget-trading-program-collaborative-innovative-approach-solving','PESTICIDES'); return false;" href="https://www.epa.gov/emissions-trading-resources/nox-budget-trading-program-collaborative-innovative-approach-solving"><span>The NOx Budget <span class="hlt">Trading</span> Program: A Collaborative, Innovative Approach to Solving a <span class="hlt">Regional</span> Air Pollution Problem</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 article examines the development and implementation of the NOx Budget <span class="hlt">Trading</span> Program (NBP) and the lessons the Environmental Protection Agency has learned from this seasonal emissions cap-and-<span class="hlt">trade</span> program.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2015EGUGA..1712530K','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2015EGUGA..1712530K"><span><span class="hlt">Wind</span> Power Energy in Southern Brazil: evaluation using a mesoscale meteorological model</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Krusche, Nisia; Stoevesandt, Bernhard; Chang, Chi-Yao; Peralta, Carlos</p> <p>2015-04-01</p> <p>In recent years, several <span class="hlt">wind</span> farms were build in the coast of Rio Grande do Sul state. This <span class="hlt">region</span> of Brazil was identified, in <span class="hlt">wind</span> energy studies, as most favorable to the development of <span class="hlt">wind</span> power energy, along with the Northeast part of the country. Site assessments of <span class="hlt">wind</span> power, over long periods to estimate the power production and forecasts over short periods can be used for planning of power distribution and enhancements on Brazil's present capacity to use this resource. The computational power available today allows the simulation of the atmospheric flow in great detail. For instance, one of the authors participated in a research that demonstrated the interaction between the lake and maritime breeze in this <span class="hlt">region</span> through the use of a atmospheric model. Therefore, we aim to evaluate simulations of <span class="hlt">wind</span> conditions and its potential to generate energy in this <span class="hlt">region</span>. The model applied is the Weather Research and Forecasting , which is the mesoscale weather forecast software. The calculation domain is centered in 32oS and 52oW, in the southern <span class="hlt">region</span> of Rio Grande do Sul state. The initial conditions of the simulation are taken from the global weather forecast in the time period from October 1st to October 31st, 2006. The <span class="hlt">wind</span> power potential was calculated for a generic turbine, with a blade length of 52 m, using the expression: P=1/2*d*A*Cp*v^3, where P is the <span class="hlt">wind</span> power energy (in Watts), d is the density (equal to 1.23 kg/m^3), A is the area section, which is equal to 8500 m2 , and v is the intensity of the velocity. The evaluation was done for a turbine placed at 50 m and 150 m of height. A threshold was chosen for a turbine production of 1.5 MW to estimate the potential of the site. In contrast to northern Brazilian <span class="hlt">region</span>, which has a rather constant <span class="hlt">wind</span> condition, this <span class="hlt">region</span> shows a great variation of power output due to the weather variability. During the period of the study, at least three frontal systems went over the <span class="hlt">region</span>, and thre was a</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://ntrs.nasa.gov/search.jsp?R=19990056504&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsolar%2Bintensity%2Bmeasurement','NASA-TRS'); return false;" href="https://ntrs.nasa.gov/search.jsp?R=19990056504&hterms=solar+intensity+measurement&qs=Ntx%3Dmode%2Bmatchall%26Ntk%3DAll%26N%3D0%26No%3D50%26Ntt%3Dsolar%2Bintensity%2Bmeasurement"><span>Solar <span class="hlt">wind</span> acceleration in the solar corona</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Giordano, S.; Antonucci, E.; Benna, C.; Kohl, J. L.; Noci, G.; Michels, J.; Fineschi, S.</p> <p>1997-01-01</p> <p>The intensity ratio of the O VI doublet in the extended area is analyzed. The O VI intensity data were obtained with the ultraviolet coronagraph spectrometer (UVCS) during the SOHO campaign 'whole sun month'. The long term observations above the north pole of the sun were used for the polar coronal data. Using these measurements, the solar <span class="hlt">wind</span> outflow velocity in the extended corona was determined. The 100 km/s level is running along the streamer borders. The acceleration of the solar <span class="hlt">wind</span> is found to be high in <span class="hlt">regions</span> between streamers. In the central part of streamers, the outflow velocity of the coronal plasma remains below 100 km/s at least within 3.8 solar radii. The <span class="hlt">regions</span> at the north and south poles, characterized by a more rapid acceleration of the solar <span class="hlt">wind</span>, correspond to <span class="hlt">regions</span> where the UVCS observes enhanced O VI line broadenings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4671716','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4671716"><span>Inequalities in Global <span class="hlt">Trade</span>: A Cross-Country Comparison of <span class="hlt">Trade</span> Network Position, Economic Wealth, Pollution and Mortality</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Prell, Christina; Sun, Laixiang; Feng, Kuishuang; Myroniuk, Tyler W.</p> <p>2015-01-01</p> <p>In this paper we investigate how structural patterns of international <span class="hlt">trade</span> give rise to emissions inequalities across countries, and how such inequality in turn impact countries’ mortality rates. We employ Multi-<span class="hlt">regional</span> Input-Output analysis to distinguish between sulfur-dioxide (SO2) emissions produced within a country’s boarders (production-based emissions) and emissions triggered by consumption in other countries (consumption-based emissions). We use social network analysis to capture countries’ level of integration within the global <span class="hlt">trade</span> network. We then apply the Prais-Winsten panel estimation technique to a panel data set across 172 countries over 20 years (1990–2010) to estimate the relationships between countries’ level of integration and SO2 emissions, and the impact of <span class="hlt">trade</span> integration and SO2 emission on mortality rates. Our findings suggest a positive, (log-) linear relationship between a country’s level of integration and both kinds of emissions. In addition, although more integrated countries are mainly responsible for both forms of emissions, our findings indicate that they also tend to experience lower mortality rates. Our approach offers a unique combination of social network analysis with multiregional input-output analysis, which better operationalizes intuitive concepts about global <span class="hlt">trade</span> and <span class="hlt">trade</span> structure. PMID:26642202</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23139883','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23139883"><span>Fragmentation reduces <span class="hlt">regional</span>-scale spatial genetic structure in a <span class="hlt">wind</span>-pollinated tree because genetic barriers are removed.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Wang, Rong; Compton, Stephen G; Shi, Yi-Su; Chen, Xiao-Yong</p> <p>2012-09-01</p> <p>Gene flow strongly influences the <span class="hlt">regional</span> genetic structuring of plant populations. Seed and pollen dispersal patterns can respond differently to the increased isolation resulting from habitat fragmentation, with unpredictable consequences for gene flow and population structuring. In a recently fragmented landscape we compared the pre- and post-fragmentation genetic structure of populations of a tree species where pollen and seed dispersal respond differentially to forest fragmentation generated by flooding. Castanopsis sclerophylla is <span class="hlt">wind</span>-pollinated, with seeds that are dispersed by gravity and rodents. Using microsatellites, we found no significant difference in genetic diversity between pre- and post-fragmentation cohorts. Significant genetic structure was observed in pre-fragmentation cohorts, due to an unknown genetic barrier that had isolated one small population. Among post-fragmentation cohorts this genetic barrier had disappeared and genetic structure was significantly weakened. The strengths of genetic structuring were at a similar level in both cohorts, suggesting that overall gene flow of C. sclerophylla has been unchanged by fragmentation at the <span class="hlt">regional</span> scale. Fragmentation has blocked seed dispersal among habitats, but this appears to have been compensated for by enhanced pollen dispersal, as indicated by the disappearance of a genetic barrier, probably as a result of increased <span class="hlt">wind</span> speeds and easier pollen movement over water. Extensive pollen flow can counteract some negative effects of fragmentation and assist the long-term persistence of small remnant populations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009lkic.conf..816C','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009lkic.conf..816C"><span>Building a Collaborative Network for Education and Training in International <span class="hlt">Trade</span> Facilitation Clusters</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Clendenin, John A.; Petrova, Nadya N.; Gill, Joshua K.</p> <p></p> <p>The authors present the benefits of collaboration rather than competition in developing educational and training resources for international <span class="hlt">trade</span> within a geographic <span class="hlt">region</span> and explore the challenges for business partners, governments and educational institutions. The paper indicates that flexibility in the 21st Century is critical, particularly when striving for virtual implementations of the solution services. It is essential, say the authors, for educators, governments and business executives to focus on performance and the careful orchestration and integration of business, policy and information technology for “Networking” that successfully stimulates inter-governmental cooperation and innovative policies that foster <span class="hlt">Regional</span> <span class="hlt">trade</span> facilitation. An innovative way to enhance 21st Century <span class="hlt">Trade</span> Facilitation is offered with Supply Chain Centers of <span class="hlt">Regional</span> Excellence (SCcORE).</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4568694','PMC'); return false;" href="https://www.pubmedcentral.nih.gov/articlerender.fcgi?tool=pmcentrez&artid=4568694"><span>Two methods for estimating limits to large-scale <span class="hlt">wind</span> power generation</span></a></p> <p><a target="_blank" href="http://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pmc">PubMed Central</a></p> <p>Miller, Lee M.; Brunsell, Nathaniel A.; Mechem, David B.; Gans, Fabian; Monaghan, Andrew J.; Vautard, Robert; Keith, David W.; Kleidon, Axel</p> <p>2015-01-01</p> <p><span class="hlt">Wind</span> turbines remove kinetic energy from the atmospheric flow, which reduces <span class="hlt">wind</span> speeds and limits generation rates of large <span class="hlt">wind</span> farms. These interactions can be approximated using a vertical kinetic energy (VKE) flux method, which predicts that the maximum power generation potential is 26% of the instantaneous downward transport of kinetic energy using the preturbine climatology. We compare the energy flux method to the Weather Research and Forecasting (WRF) <span class="hlt">regional</span> atmospheric model equipped with a <span class="hlt">wind</span> turbine parameterization over a 105 km2 <span class="hlt">region</span> in the central United States. The WRF simulations yield a maximum generation of 1.1 We⋅m−2, whereas the VKE method predicts the time series while underestimating the maximum generation rate by about 50%. Because VKE derives the generation limit from the preturbine climatology, potential changes in the vertical kinetic energy flux from the free atmosphere are not considered. Such changes are important at night when WRF estimates are about twice the VKE value because <span class="hlt">wind</span> turbines interact with the decoupled nocturnal low-level jet in this <span class="hlt">region</span>. Daytime estimates agree better to 20% because the <span class="hlt">wind</span> turbines induce comparatively small changes to the downward kinetic energy flux. This combination of downward transport limits and <span class="hlt">wind</span> speed reductions explains why large-scale <span class="hlt">wind</span> power generation in windy <span class="hlt">regions</span> is limited to about 1 We⋅m−2, with VKE capturing this combination in a comparatively simple way. PMID:26305925</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-10-05/pdf/2011-25738.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-10-05/pdf/2011-25738.pdf"><span>76 FR 61667 - Proposed Foreign-<span class="hlt">Trade</span> Zone-West Tennessee Area Under Alternative Site Framework; Application Filed</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-10-05</p> <p>... DEPARTMENT OF COMMERCE Foreign-<span class="hlt">Trade</span> Zones Board [Docket 59-2011] Proposed Foreign-<span class="hlt">Trade</span> Zone... submitted to the Foreign-<span class="hlt">Trade</span> Zones Board (the Board) by the Northwest Tennessee <span class="hlt">Regional</span> Port Authority to establish a general-purpose foreign-<span class="hlt">trade</span> zone at sites in Dyer, Gibson, Haywood, Lake, Lauderdale, Madison...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.osti.gov/servlets/purl/1148347','SCIGOV-STC'); return false;" href="https://www.osti.gov/servlets/purl/1148347"><span>National Offshore <span class="hlt">Wind</span> Energy Grid Interconnection Study</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>Daniel, John P.; Liu, Shu; Ibanez, Eduardo</p> <p>2014-07-30</p> <p>The National Offshore <span class="hlt">Wind</span> Energy Grid Interconnection Study (NOWEGIS) considers the availability and potential impacts of interconnecting large amounts of offshore <span class="hlt">wind</span> energy into the transmission system of the lower 48 contiguous United States. A total of 54GW of offshore <span class="hlt">wind</span> was assumed to be the target for the analyses conducted. A variety of issues are considered including: the anticipated staging of offshore <span class="hlt">wind</span>; the offshore <span class="hlt">wind</span> resource availability; offshore <span class="hlt">wind</span> energy power production profiles; offshore <span class="hlt">wind</span> variability; present and potential technologies for collection and delivery of offshore <span class="hlt">wind</span> energy to the onshore grid; potential impacts to existing utility systemsmore » most likely to receive large amounts of offshore <span class="hlt">wind</span>; and regulatory influences on offshore <span class="hlt">wind</span> development. The technologies considered the reliability of various high-voltage ac (HVAC) and high-voltage dc (HVDC) technology options and configurations. The utility system impacts of GW-scale integration of offshore <span class="hlt">wind</span> are considered from an operational steady-state perspective and from a <span class="hlt">regional</span> and national production cost perspective.« less</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2011AGUFMGC41D0845L','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2011AGUFMGC41D0845L"><span>Analysis and characterization of the vertical <span class="hlt">wind</span> profile in UAE</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Lee, W.; Ghedira, H.; Ouarda, T.; Gherboudj, I.</p> <p>2011-12-01</p> <p>In this study, temporal and spatial analysis of the vertical <span class="hlt">wind</span> profiles in the UAE has been performed to estimate <span class="hlt">wind</span> resource potential. Due to the very limited number of <span class="hlt">wind</span> masts (only two <span class="hlt">wind</span> masts in the UAE, operational for less than three years), the <span class="hlt">wind</span> potential analysis will be mainly derived from numerical-based models. Additional <span class="hlt">wind</span> data will be derived from the UAE met stations network (at 10 m elevation) managed by the UAE National Center of Meteorology and Seismology. However, since <span class="hlt">wind</span> turbines are generally installed at elevations higher than 80 m, it is vital to extrapolate <span class="hlt">wind</span> speed correctly from low heights to <span class="hlt">wind</span> turbine hub heights to predict potential <span class="hlt">wind</span> energy properly. To do so, firstly two boundary layer based models, power law and logarithmic law, were tested to find the best fitting model. Power law is expressed as v/v0 =(H/H0)^α and logarithmic law is represented as v/v0 =[ln(H/Z0))/(ln(H0/Z0)], where V is the <span class="hlt">wind</span> speed [m/s] at height H [m] and V0 is the known <span class="hlt">wind</span> speed at a reference height H0. The exponent (α) coefficient is an empirically derived value depending on the atmospheric stability and z0 is the roughness coefficient length [m] that depends on topography, land roughness and spacing. After testing the two models, spatial and temporal analysis for <span class="hlt">wind</span> profile was performed. Many studies about <span class="hlt">wind</span> in different <span class="hlt">regions</span> have shown that <span class="hlt">wind</span> profile parameters have hourly, monthly and seasonal variations. Therefore, it can be examined whether UAE <span class="hlt">wind</span> characteristics follow general <span class="hlt">wind</span> characteristics observed in other <span class="hlt">regions</span> or have specific <span class="hlt">wind</span> features due to its <span class="hlt">regional</span> condition. About 3 years data from August 2008 to February 2011 with 10-minutes resolution were used to derive monthly variation. The preliminary results(Fig.1) show that during that period, <span class="hlt">wind</span> profile parameters like alpha from power law and roughness length from logarithmic law have monthly variation. Both alpha and roughness have</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/2013JGS....15..319D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013JGS....15..319D"><span>Social networks and <span class="hlt">trade</span> of services: modelling interregional flows with spatial and network autocorrelation effects</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>de la Mata, Tamara; Llano, Carlos</p> <p>2013-07-01</p> <p>Recent literature on border effect has fostered research on informal barriers to <span class="hlt">trade</span> and the role played by network dependencies. In relation to social networks, it has been shown that intensity of <span class="hlt">trade</span> in goods is positively correlated with migration flows between pairs of countries/<span class="hlt">regions</span>. In this article, we investigate whether such a relation also holds for interregional <span class="hlt">trade</span> of services. We also consider whether interregional <span class="hlt">trade</span> flows in services linked with tourism exhibit spatial and/or social network dependence. Conventional empirical gravity models assume the magnitude of bilateral flows between <span class="hlt">regions</span> is independent of flows to/from <span class="hlt">regions</span> located nearby in space, or flows to/from <span class="hlt">regions</span> related through social/cultural/ethic network connections. With this aim, we provide estimates from a set of gravity models showing evidence of statistically significant spatial and network (demographic) dependence in the bilateral flows of the <span class="hlt">trade</span> of services considered. The analysis has been applied to the Spanish intra- and interregional monetary flows of services from the accommodation, restaurants and travel agencies for the period 2000-2009, using alternative datasets for the migration stocks and definitions of network effects.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2003EAEJA.....5636D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2003EAEJA.....5636D"><span>Observation of <span class="hlt">wind</span> field over heterogeneous terrain by the French-German airborne Doppler lidar <span class="hlt">WIND</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Dabas, A.; Werner, C.; Delville, P.; Reitebuch, O.; Drobinski, P.; Cousin, F.</p> <p>2003-04-01</p> <p>In summer 2001, the French-German airborne Doppler lidar <span class="hlt">WIND</span> participated to field campaign ESCOMPTE. ESCOMPTE was carried out in the <span class="hlt">region</span> of Marseille along the Mediterranean coast of France. It was dedicated to the observation of heavy pollution events in this industrialized, densely populated <span class="hlt">region</span> of nearly 4 million inhabitants. The aim was to gather a data base as comprehensive as possible on several pollution events and use them to check the ability of several <span class="hlt">regional</span> forecast models to predict such events. The specific mission devoted to <span class="hlt">WIND</span> was the characterization at mesoscale of the <span class="hlt">wind</span> field and the topography of the planetary boundary layer. Both are complex around Marseille due the heterogeneity of the surface with a transition sea/land to the south, the fore-Alps to the North, the Rhône valley to the North-West etc... Seven, 3-hr flights were carried out and gave excellent results. In 2002, first comparisons were made with mesoscale models. They will be shown during the presentation. They are good examples of the usefulness of airborne Doppler lidar for validating and improving atmospheric model simulations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2013BoLMe.149..103R','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2013BoLMe.149..103R"><span>The Effect of <span class="hlt">Wind</span>-Turbine Wakes on Summertime US Midwest Atmospheric <span class="hlt">Wind</span> Profiles as Observed with Ground-Based Doppler Lidar</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Rhodes, Michael E.; Lundquist, Julie K.</p> <p>2013-07-01</p> <p>We examine the influence of a modern multi-megawatt <span class="hlt">wind</span> turbine on <span class="hlt">wind</span> and turbulence profiles three rotor diameters (D) downwind of the turbine. Light detection and ranging (lidar) <span class="hlt">wind</span>-profile observations were collected during summer 2011 in an operating <span class="hlt">wind</span> farm in central Iowa at 20-m vertical intervals from 40 to 220 m above the surface. After a calibration period during which two lidars were operated next to each other, one lidar was located approximately 2D directly south of a <span class="hlt">wind</span> turbine; the other lidar was moved approximately 3D north of the same <span class="hlt">wind</span> turbine. Data from the two lidars during southerly flow conditions enabled the simultaneous capture of inflow and wake conditions. The inflow <span class="hlt">wind</span> and turbulence profiles exhibit strong variability with atmospheric stability: daytime profiles are well-mixed with little shear and strong turbulence, while nighttime profiles exhibit minimal turbulence and considerable shear across the rotor disk <span class="hlt">region</span> and above. Consistent with the observations available from other studies and with <span class="hlt">wind</span>-tunnel and large-eddy simulation studies, measurable reductions in wake <span class="hlt">wind</span>-speeds occur at heights spanning the <span class="hlt">wind</span> turbine rotor (43-117 m), and turbulent quantities increase in the wake. In generalizing these results as a function of inflow <span class="hlt">wind</span> speed, we find the <span class="hlt">wind</span>-speed deficit in the wake is largest at hub height or just above, and the maximum deficit occurs when <span class="hlt">wind</span> speeds are below the rated speed for the turbine. Similarly, the maximum enhancement of turbulence kinetic energy and turbulence intensity occurs at hub height, although observations at the top of the rotor disk do not allow assessment of turbulence in that <span class="hlt">region</span>. The <span class="hlt">wind</span> shear below turbine hub height (quantified here with the power-law coefficient) is found to be a useful parameter to identify whether a downwind lidar observes turbine wake or free-flow conditions. These field observations provide data for validating turbine-wake models and <span class="hlt">wind</span></p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2002AGUFMSA21B0463A','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2002AGUFMSA21B0463A"><span>Did the April 14-24 storms impact the mesopause <span class="hlt">region</span> sodium density, temperature and <span class="hlt">wind</span> over Fort Collins, CO (41N, 105W)</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Arnold, K. S.; She, C.; Yuan, T.; Williams, B. P.; Krueger, D. A.</p> <p>2002-12-01</p> <p>The April 14-24 storms is under intense study to determine, among other things, its MLTI response. The change in sodium density, neutral temperature and <span class="hlt">winds</span> in the mesopause <span class="hlt">region</span> (80-110km) is a useful signature to look for. The Colorado State Sodium Lidar happened to have made nocturnal observations of sodium density, neutral temperature and zonal <span class="hlt">wind</span> in April, 8th, 12th, 13th, 18th, and 22nd through 25th. We hope to determine and report if statistically meaningful changes in these important quantities had indeed occurred.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970011906','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970011906"><span><span class="hlt">Wind</span> Variability of B Supergiants. No. 2; The Two-component Stellar <span class="hlt">Wind</span> of gamma Arae</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Prinja, R. K.; Massa, D.; Fullerton, A. W.; Howarth, I. D.; Pontefract, M.</p> <p>1996-01-01</p> <p>The stellar <span class="hlt">wind</span> of the rapidly rotating early-B supergiant, gamma Ara, is studied using time series, high-resolution IUE spectroscopy secured over approx. 6 days in 1993 March. Results are presented based on an analysis of several line species, including N(N), C(IV), Si(IV), Si(III), C(II), and Al(III). The <span class="hlt">wind</span> of this star is grossly structured, with evidence for latitude-dependent mass loss which reflects the role of rapid rotation. Independent, co-existing time variable features are identified at low-velocity (redward of approx. -750 km/s) and at higher-speeds extending to approx. -1500 km/s. The interface between these structures is 'defined' by the appearance of a discrete absorption component which is extremely sharp (in velocity space). The central velocity of this 'Super DAC' changes only gradually, over several days, between approx. -400 and -750 km/s in most of the ions. However, its location is shifted redward by almost 400 km/s in Al(III) and C(II), indicating that the physical structure giving rise to this feature has a substantial velocity and ionization jump. Constraints on the relative ionization properties of the <span class="hlt">wind</span> structures are discussed, together with results based on SEI line-profile-fitting methods. The overall <span class="hlt">wind</span> activity in gamma Ara exhibits a clear ion dependence, such that low-speed features are promoted in low-ionization species, including Al(III), C(II), and Si(III). We also highlight that - in contrast to most OB stars - there are substantial differences in the epoch-to-epoch time-averaged <span class="hlt">wind</span> profiles of gamma Ara. We interpret the results in terms of a two-component <span class="hlt">wind</span> model for gamma Ara, with an equatorially compressed low ionization <span class="hlt">region</span>, and a high speed, higher-ionization polar outflow. This picture is discussed in the context of the predicted bi-stability mechanism for line-driven <span class="hlt">winds</span> in rapidly rotating early-B type stars, and the formation of compressed <span class="hlt">wind</span> <span class="hlt">regions</span> in rapidly rotating hot stars. The apparent</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/23763387','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/23763387"><span>Quantifying the hurricane catastrophe risk to offshore <span class="hlt">wind</span> power.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Rose, Stephen; Jaramillo, Paulina; Small, Mitchell J; Apt, Jay</p> <p>2013-12-01</p> <p>The U.S. Department of Energy has estimated that over 50 GW of offshore <span class="hlt">wind</span> power will be required for the United States to generate 20% of its electricity from <span class="hlt">wind</span>. Developers are actively planning offshore <span class="hlt">wind</span> farms along the U.S. Atlantic and Gulf coasts and several leases have been signed for offshore sites. These planned projects are in areas that are sometimes struck by hurricanes. We present a method to estimate the catastrophe risk to offshore <span class="hlt">wind</span> power using simulated hurricanes. Using this method, we estimate the fraction of offshore <span class="hlt">wind</span> power simultaneously offline and the cumulative damage in a <span class="hlt">region</span>. In Texas, the most vulnerable <span class="hlt">region</span> we studied, 10% of offshore <span class="hlt">wind</span> power could be offline simultaneously because of hurricane damage with a 100-year return period and 6% could be destroyed in any 10-year period. We also estimate the risks to single <span class="hlt">wind</span> farms in four representative locations; we find the risks are significant but lower than those estimated in previously published results. Much of the hurricane risk to offshore <span class="hlt">wind</span> turbines can be mitigated by designing turbines for higher maximum <span class="hlt">wind</span> speeds, ensuring that turbine nacelles can turn quickly to track the <span class="hlt">wind</span> direction even when grid power is lost, and building in areas with lower risk. © 2013 Society for Risk Analysis.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2009QuRes..71..409M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2009QuRes..71..409M"><span>Late Pleistocene eolian features in southeastern Maryland and Chesapeake Bay <span class="hlt">region</span> indicate strong WNW-NW <span class="hlt">winds</span> accompanied growth of the Laurentide Ice Sheet</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Markewich, Helaine W.; Litwin, Ronald J.; Pavich, Milan J.; Brook, George A.</p> <p>2009-05-01</p> <p>Inactive parabolic dunes are present in southeastern Maryland, USA, along the east bank of the Potomac River. More elongate and finer-grained eolian deposits and paha-like ridges characterize the Potomac River-Patuxent River upland and the west side of Chesapeake Bay. These ridges are streamlined erosional features, veneered with eolian sediment and interspersed with dunes in the low-relief headwaters of Potomac- and Patuxent-river tributaries. Axis data for the dunes and ridges indicate formation by WNW-NW <span class="hlt">winds</span>. Optically stimulated luminescence and radiocarbon age data suggest dune formation from ˜ 33-15 ka, agreeing with the 30-13 ka ages Denny, C.S., Owens, J.P., Sirkin, L., Rubin, M., 1979. The Parsonburg Sand in the central Delmarva Peninsula, Maryland and Delaware. U.S. Geol. Surv. Prof. Pap. 1067-B, 16 pp. suggested for eolian deposits east of Chesapeake Bay. Age range and paleowind direction(s) for eolian features in the Bay <span class="hlt">region</span> approximate those for late Wisconsin loess in the North American midcontinent. Formation of midcontinent loess and Bay-<span class="hlt">region</span> eolian features was coeval with rapid growth of the Laurentide Ice Sheet and strong cooling episodes (δ 18O minima) evident in Greenland ice cores. Age and paleowind-direction coincidence, for eolian features in the midcontinent and Bay <span class="hlt">region</span>, indicates strong mid-latitude WNW-NW <span class="hlt">winds</span> for several hundred kilometers south of the Laurentide glacial terminus that were oblique to previously simulated anticyclonic <span class="hlt">winds</span> for the last glacial maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://pubs.er.usgs.gov/publication/70035033','USGSPUBS'); return false;" href="https://pubs.er.usgs.gov/publication/70035033"><span>Late Pleistocene eolian features in southeastern Maryland and Chesapeake Bay <span class="hlt">region</span> indicate strong WNW-NW <span class="hlt">winds</span> accompanied growth of the Laurentide Ice Sheet</span></a></p> <p><a target="_blank" href="http://pubs.er.usgs.gov/pubs/index.jsp?view=adv">USGS Publications Warehouse</a></p> <p>Markewich, H.W.; Litwin, R.J.; Pavich, M.J.; Brook, G.A.</p> <p>2009-01-01</p> <p>Inactive parabolic dunes are present in southeastern Maryland, USA, along the east bank of the Potomac River. More elongate and finer-grained eolian deposits and paha-like ridges characterize the Potomac River-Patuxent River upland and the west side of Chesapeake Bay. These ridges are streamlined erosional features, veneered with eolian sediment and interspersed with dunes in the low-relief headwaters of Potomac- and Patuxent-river tributaries. Axis data for the dunes and ridges indicate formation by WNW-NW <span class="hlt">winds</span>. Optically stimulated luminescence and radiocarbon age data suggest dune formation from ??? 33-15??ka, agreeing with the 30-13??ka ages Denny, C.S., Owens, J.P., Sirkin, L., Rubin, M., 1979. The Parsonburg Sand in the central Delmarva Peninsula, Maryland and Delaware. U.S. Geol. Surv. Prof. Pap. 1067-B, 16??pp. suggested for eolian deposits east of Chesapeake Bay. Age range and paleowind direction(s) for eolian features in the Bay <span class="hlt">region</span> approximate those for late Wisconsin loess in the North American midcontinent. Formation of midcontinent loess and Bay-<span class="hlt">region</span> eolian features was coeval with rapid growth of the Laurentide Ice Sheet and strong cooling episodes (??18O minima) evident in Greenland ice cores. Age and paleowind-direction coincidence, for eolian features in the midcontinent and Bay <span class="hlt">region</span>, indicates strong mid-latitude WNW-NW <span class="hlt">winds</span> for several hundred kilometers south of the Laurentide glacial terminus that were oblique to previously simulated anticyclonic <span class="hlt">winds</span> for the last glacial maximum.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2010EGUGA..12.2959B','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2010EGUGA..12.2959B"><span>Monitoring, modeling and mitigating impacts of <span class="hlt">wind</span> farms on local meteorology</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Baidya Roy, Somnath; Traiteur, Justin; Kelley, Neil</p> <p>2010-05-01</p> <p><span class="hlt">Wind</span> power is one of the fastest growing sources of energy. Most of the growth is in the industrial sector comprising of large utility-scale <span class="hlt">wind</span> farms. Recent modeling studies have suggested that such <span class="hlt">wind</span> farms can significantly affect local and <span class="hlt">regional</span> weather and climate. In this work, we present observational evidence of the impact of <span class="hlt">wind</span> farms on near-surface air temperatures. Data from perhaps the only meteorological field campaign in an operational <span class="hlt">wind</span> farm shows that downwind temperatures are lower during the daytime and higher at night compared to the upwind environment. Corresponding radiosonde profiles at the nearby Edwards Air Force Base WMO meteorological station show that the diurnal environment is unstable while the nocturnal environment is stable during the field campaign. This behavior is consistent with the hypothesis proposed by Baidya Roy et al. (JGR 2004) that states that turbulence generated in the wake of rotors enhance vertical mixing leading to a warming/cooling under positive/negative potential temperature lapse rates. We conducted a set of 306 simulations with the <span class="hlt">Regional</span> Atmospheric Modeling System (RAMS) to test if <span class="hlt">regional</span> climate models can capture the thermal effects of <span class="hlt">wind</span> farms. We represented <span class="hlt">wind</span> turbines with a subgrid parameterization that assumes rotors to be sinks of momentum and sources of turbulence. The simulated <span class="hlt">wind</span> farms consistently generated a localized warming/cooling under positive/negative lapse rates as hypothesized. We found that these impacts are inversely correlated with background atmospheric boundary layer turbulence. Thus, if the background turbulence is high due to natural processes, the effects of additional turbulence generated by <span class="hlt">wind</span> turbine rotors are likely to be small. We propose the following strategies to minimize impacts of <span class="hlt">wind</span> farms: • Engineering solution: design rotors that generate less turbulence in their wakes. Sensitivity simulations show that these turbines also increase the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2018E%26ES..121b2021W','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2018E%26ES..121b2021W"><span>Experimental study on influence of vegetation coverage on runoff in <span class="hlt">wind</span>-water erosion crisscross <span class="hlt">region</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, Jinhua; Zhang, Ronggang; Sun, Juan</p> <p>2018-02-01</p> <p>Using artificial rainfall simulation method, 23 simulation experiments were carried out in water-<span class="hlt">wind</span> erosion crisscross <span class="hlt">region</span> in order to analyze the influence of vegetation coverage on runoff and sediment yield. The experimental plots are standard plots with a length of 20m, width of 5m and slope of 15 degrees. The simulation experiments were conducted in different vegetation coverage experimental plots based on three different rainfall intensities. According to the experimental observation data, the influence of vegetation coverage on runoff and infiltration was analyzed. Vegetation coverage has a significant impact on runoff, and the higher the vegetation coverage is, the smaller the runoff is. Under the condition of 0.6mm/min rainfall intensity, the runoff volume from the experimental plot with 18% vegetation coverage was 1.2 times of the runoff from the experimental with 30% vegetation coverage. What’s more, the difference of runoff is more obvious in higher rainfall intensity. If the rainfall intensity reaches 1.32mm/min, the runoff from the experimental plot with 11% vegetation coverage is about 2 times as large as the runoff from the experimental plot with 53%vegetation coverage. Under the condition of small rainfall intensity, the starting time of runoff in the experimental plot with higher vegetation coverage is later than that in the experimental plot with low vegetation coverage. However, under the condition of heavy rainfall intensity, there is no obvious difference in the beginning time of runoff. In addition, the higher the vegetation coverage is, the deeper the rainfall infiltration depth is.The results can provide reference for ecological construction carried out in <span class="hlt">wind</span> erosion crisscross <span class="hlt">region</span> with serious soil erosion.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AdSR...14...95T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AdSR...14...95T"><span>Ensemble using different Planetary Boundary Layer schemes in WRF model for <span class="hlt">wind</span> speed and direction prediction over Apulia <span class="hlt">region</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tateo, Andrea; Marcello Miglietta, Mario; Fedele, Francesca; Menegotto, Micaela; Monaco, Alfonso; Bellotti, Roberto</p> <p>2017-04-01</p> <p>The Weather Research and Forecasting mesoscale model (WRF) was used to simulate hourly 10 m <span class="hlt">wind</span> speed and direction over the city of Taranto, Apulia <span class="hlt">region</span> (south-eastern Italy). This area is characterized by a large industrial complex including the largest European steel plant and is subject to a <span class="hlt">Regional</span> Air Quality Recovery Plan. This plan constrains industries in the area to reduce by 10 % the mean daily emissions by diffuse and point sources during specific meteorological conditions named <span class="hlt">wind</span> days. According to the Recovery Plan, the <span class="hlt">Regional</span> Environmental Agency ARPA-PUGLIA is responsible for forecasting these specific meteorological conditions with 72 h in advance and possibly issue the early warning. In particular, an accurate <span class="hlt">wind</span> simulation is required. Unfortunately, numerical weather prediction models suffer from errors, especially for what concerns near-surface fields. These errors depend primarily on uncertainties in the initial and boundary conditions provided by global models and secondly on the model formulation, in particular the physical parametrizations used to represent processes such as turbulence, radiation exchange, cumulus and microphysics. In our work, we tried to compensate for the latter limitation by using different Planetary Boundary Layer (PBL) parameterization schemes. Five combinations of PBL and Surface Layer (SL) schemes were considered. Simulations are implemented in a real-time configuration since our intention is to analyze the same configuration implemented by ARPA-PUGLIA for operational runs; the validation is focused over a time range extending from 49 to 72 h with hourly time resolution. The assessment of the performance was computed by comparing the WRF model output with ground data measured at a weather monitoring station in Taranto, near the steel plant. After the analysis of the simulations performed with different PBL schemes, both simple (e.g. average) and more complex post-processing methods (e.g. weighted average</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017IAUS..329..186D','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017IAUS..329..186D"><span>The <span class="hlt">wind-wind</span> collision hole in eta Car</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Damineli, A.; Teodoro, M.; Richardson, N. D.; Gull, T. R.; Corcoran, M. F.; Hamaguchi, K.; Groh, J. H.; Weigelt, G.; Hillier, D. J.; Russell, C.; Moffat, A.; Pollard, K. R.; Madura, T. I.</p> <p>2017-11-01</p> <p>Eta Carinae is one of the most massive observable binaries. Yet determination of its orbital and physical parameters is hampered by obscuring <span class="hlt">winds</span>. However the effects of the strong, colliding <span class="hlt">winds</span> changes with phase due to the high orbital eccentricity. We wanted to improve measures of the orbital parameters and to determine the mechanisms that produce the relatively brief, phase-locked minimum as detected throughout the electromagnetic spectrum. We conducted intense monitoring of the He ii λ4686 line in η Carinae for 10 months in the year 2014, gathering ~300 high S/N spectra with ground- and space-based telescopes. We also used published spectra at the FOS4 SE polar <span class="hlt">region</span> of the Homunculus, which views the minimum from a different direction. We used a model in which the He ii λ4686 emission is produced by two mechanisms: a) one linked to the intensity of the <span class="hlt">wind-wind</span> collision which occurs along the whole orbit and is proportional to the inverse square of the separation between the companion stars; and b) the other produced by the `bore hole' effect which occurs at phases across the periastron passage. The opacity (computed from 3D SPH simulations) as convolved with the emission reproduces the behavior of equivalent widths both for direct and reflected light. Our main results are: a) a demonstration that the He ii λ4686 light curve is exquisitely repeatable from cycle to cycle, contrary to previous claims for large changes; b) an accurate determination of the longitude of periastron, indicating that the secondary star is `behind' the primary at periastron, a dispute extended over the past decade; c) a determination of the time of periastron passage, at ~4 days after the onset of the deep light curve minimum; and d) show that the minimum is simultaneous for observers at different lines of sight, indicating that it is not caused by an eclipse of the secondary star, but rather by the immersion of the <span class="hlt">wind-wind</span> collision interior to the inner <span class="hlt">wind</span> of the</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFM.A22A..06T','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFM.A22A..06T"><span>Transboundary health impacts of transported global air pollution and international <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Tong, D.; Zhang, Q.; Jiang, X.</p> <p>2017-12-01</p> <p>Millions of people die every year from diseases caused by exposure to outdoor air pollution. Some studies have estimated premature mortality related to local sources of air pollution, but local air quality can also be affected by atmospheric transport of pollution from distant sources. International <span class="hlt">trade</span> is contributing to the globalization of emission and pollution as a result of the production of goods (and their associated emissions) in one <span class="hlt">region</span> for consumption in another <span class="hlt">region</span>. The effects of international <span class="hlt">trade</span> on air pollutant emissions, air quality and health have been investigated <span class="hlt">regionally</span>, but a combined, global assessment of the health impacts related to international <span class="hlt">trade</span> and the transport of atmospheric air pollution is lacking. Here we combine four global models to estimate premature mortality caused by fine particulate matter (PM2.5) pollution as a result of atmospheric transport and the production and consumption of goods and services in different world <span class="hlt">regions</span>. We find that, of the 3.45 million premature deaths related to PM2.5 pollution in 2007 worldwide, about 12 per cent (411,100 deaths) were related to air pollutants emitted in a <span class="hlt">region</span> of the world other than that in which the death occurred, and about 22 per cent (762,400 deaths) were associated with goods and services produced in one <span class="hlt">region</span> for consumption in another. For example, PM2.5 pollution produced in China in 2007 is linked to more than 64,800 premature deaths in <span class="hlt">regions</span> other than China, including more than 3,100 premature deaths in western Europe and the USA; on the other hand, consumption in western Europe and the USA is linked to more than 108,600 premature deaths in China. Our results reveal that the transboundary health impacts of PM2.5 pollution associated with international <span class="hlt">trade</span> are greater than those associated with long-distance atmospheric pollutant transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.ncbi.nlm.nih.gov/pubmed/28358094','PUBMED'); return false;" href="https://www.ncbi.nlm.nih.gov/pubmed/28358094"><span>Transboundary health impacts of transported global air pollution and international <span class="hlt">trade</span>.</span></a></p> <p><a target="_blank" href="https://www.ncbi.nlm.nih.gov/entrez/query.fcgi?DB=pubmed">PubMed</a></p> <p>Zhang, Qiang; Jiang, Xujia; Tong, Dan; Davis, Steven J; Zhao, Hongyan; Geng, Guannan; Feng, Tong; Zheng, Bo; Lu, Zifeng; Streets, David G; Ni, Ruijing; Brauer, Michael; van Donkelaar, Aaron; Martin, Randall V; Huo, Hong; Liu, Zhu; Pan, Da; Kan, Haidong; Yan, Yingying; Lin, Jintai; He, Kebin; Guan, Dabo</p> <p>2017-03-29</p> <p>Millions of people die every year from diseases caused by exposure to outdoor air pollution. Some studies have estimated premature mortality related to local sources of air pollution, but local air quality can also be affected by atmospheric transport of pollution from distant sources. International <span class="hlt">trade</span> is contributing to the globalization of emission and pollution as a result of the production of goods (and their associated emissions) in one <span class="hlt">region</span> for consumption in another <span class="hlt">region</span>. The effects of international <span class="hlt">trade</span> on air pollutant emissions, air quality and health have been investigated <span class="hlt">regionally</span>, but a combined, global assessment of the health impacts related to international <span class="hlt">trade</span> and the transport of atmospheric air pollution is lacking. Here we combine four global models to estimate premature mortality caused by fine particulate matter (PM 2.5 ) pollution as a result of atmospheric transport and the production and consumption of goods and services in different world <span class="hlt">regions</span>. We find that, of the 3.45 million premature deaths related to PM 2.5 pollution in 2007 worldwide, about 12 per cent (411,100 deaths) were related to air pollutants emitted in a <span class="hlt">region</span> of the world other than that in which the death occurred, and about 22 per cent (762,400 deaths) were associated with goods and services produced in one <span class="hlt">region</span> for consumption in another. For example, PM 2.5 pollution produced in China in 2007 is linked to more than 64,800 premature deaths in <span class="hlt">regions</span> other than China, including more than 3,100 premature deaths in western Europe and the USA; on the other hand, consumption in western Europe and the USA is linked to more than 108,600 premature deaths in China. Our results reveal that the transboundary health impacts of PM 2.5 pollution associated with international <span class="hlt">trade</span> are greater than those associated with long-distance atmospheric pollutant transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017Natur.543..705Z','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017Natur.543..705Z"><span>Transboundary health impacts of transported global air pollution and international <span class="hlt">trade</span></span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Zhang, Qiang; Jiang, Xujia; Tong, Dan; Davis, Steven J.; Zhao, Hongyan; Geng, Guannan; Feng, Tong; Zheng, Bo; Lu, Zifeng; Streets, David G.; Ni, Ruijing; Brauer, Michael; van Donkelaar, Aaron; Martin, Randall V.; Huo, Hong; Liu, Zhu; Pan, Da; Kan, Haidong; Yan, Yingying; Lin, Jintai; He, Kebin; Guan, Dabo</p> <p>2017-03-01</p> <p>Millions of people die every year from diseases caused by exposure to outdoor air pollution. Some studies have estimated premature mortality related to local sources of air pollution, but local air quality can also be affected by atmospheric transport of pollution from distant sources. International <span class="hlt">trade</span> is contributing to the globalization of emission and pollution as a result of the production of goods (and their associated emissions) in one <span class="hlt">region</span> for consumption in another <span class="hlt">region</span>. The effects of international <span class="hlt">trade</span> on air pollutant emissions, air quality and health have been investigated <span class="hlt">regionally</span>, but a combined, global assessment of the health impacts related to international <span class="hlt">trade</span> and the transport of atmospheric air pollution is lacking. Here we combine four global models to estimate premature mortality caused by fine particulate matter (PM2.5) pollution as a result of atmospheric transport and the production and consumption of goods and services in different world <span class="hlt">regions</span>. We find that, of the 3.45 million premature deaths related to PM2.5 pollution in 2007 worldwide, about 12 per cent (411,100 deaths) were related to air pollutants emitted in a <span class="hlt">region</span> of the world other than that in which the death occurred, and about 22 per cent (762,400 deaths) were associated with goods and services produced in one <span class="hlt">region</span> for consumption in another. For example, PM2.5 pollution produced in China in 2007 is linked to more than 64,800 premature deaths in <span class="hlt">regions</span> other than China, including more than 3,100 premature deaths in western Europe and the USA; on the other hand, consumption in western Europe and the USA is linked to more than 108,600 premature deaths in China. Our results reveal that the transboundary health impacts of PM2.5 pollution associated with international <span class="hlt">trade</span> are greater than those associated with long-distance atmospheric pollutant transport.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017MS%26E..243a2037M','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017MS%26E..243a2037M"><span>Investigation of <span class="hlt">wind</span> behaviour around high-rise buildings</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Mat Isa, Norasikin; Fitriah Nasir, Nurul; Sadikin, Azmahani; Ariff Hairul Bahara, Jamil</p> <p>2017-09-01</p> <p>A study on the investigation of <span class="hlt">wind</span> behaviour around the high-rise buildings is done through an experiment using a <span class="hlt">wind</span> tunnel and computational fluid dynamics. High-rise buildings refer to buildings or structures that have more than 12 floors. <span class="hlt">Wind</span> is invisible to the naked eye; thus, it is hard to see and analyse its flow around and over buildings without the use of proper methods, such as the use of <span class="hlt">wind</span> tunnel and computational fluid dynamics software.The study was conducted on buildings located in Presint 4, Putrajaya, Malaysia which is the Ministry of Rural and <span class="hlt">Regional</span> Development, Ministry of Information Communications and Culture, Ministry of Urban Wellbeing, Housing and Local Government and the Ministry of Women, Family, and Community by making scaled models of the buildings. The parameters in which this study is conducted on are, four different <span class="hlt">wind</span> velocities used based on the seasonal monsoons, and <span class="hlt">wind</span> direction. ANSYS Fluent workbench software is used to compute the simulations in order to achieve the objectives of this study. The data from the computational fluid dynamics are validated with the experiment done through the <span class="hlt">wind</span> tunnel. From the results obtained through the use of the computation fluid dynamics, this study can identify the characteristics of <span class="hlt">wind</span> around buildings, including boundary layer of the buildings, separation flow, wake <span class="hlt">region</span> and etc. Then analyses is conducted on the occurance resulting from the <span class="hlt">wind</span> that passes the buildings based on the velocity difference between before and after the <span class="hlt">wind</span> passes the buildings.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/20040074203','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/20040074203"><span>Properties of Minor Ions in the Solar <span class="hlt">Wind</span> and Implications for the Background Solar <span class="hlt">Wind</span> Plasma</span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Wagner, William (Technical Monitor); Esser, Ruth</p> <p>2004-01-01</p> <p>The scope of the investigation is to extract information on the properties of the bulk solar <span class="hlt">wind</span> from the minor ion observations that are provided by instruments on board NASA space craft and theoretical model studies. Ion charge states measured in situ in interplanetary space are formed in the inner coronal <span class="hlt">regions</span> below 5 solar radii, hence they carry information on the properties of the solar <span class="hlt">wind</span> plasma in that <span class="hlt">region</span>. The plasma parameters that are important in the ion forming processes are the electron density, the electron temperature and the flow speeds of the individual ion species. In addition, if the electron distribution function deviates from a Maxwellian already in the inner corona, then the enhanced tail of that distribution function, also called halo, greatly effects the ion composition. This study is carried out using solar <span class="hlt">wind</span> models, coronal observations, and ion calculations in conjunction with the in situ observations.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://adsabs.harvard.edu/abs/2017AGUFMSH53A2550G','NASAADS'); return false;" href="http://adsabs.harvard.edu/abs/2017AGUFMSH53A2550G"><span>Studying Solar <span class="hlt">Wind</span> Properties Around CIRs and Their Effects on GCR Modulation</span></a></p> <p><a target="_blank" href="http://adsabs.harvard.edu/abstract_service.html">NASA Astrophysics Data System (ADS)</a></p> <p>Ghanbari, K.; Florinski, V. A.</p> <p>2017-12-01</p> <p>Corotating interaction <span class="hlt">region</span> (CIR) events occur when a fast solar <span class="hlt">wind</span> stream overtakes slow solar <span class="hlt">wind</span>, forming a compression <span class="hlt">region</span> ahead and a rarefaction <span class="hlt">region</span> behind in the fast solar <span class="hlt">wind</span>. Usually this phenomena occurs along with a crossing of heliospheric current sheet which is the surface separating solar magnetic fields of opposing polarities. In this work, the solar plasma data provided by the ACE science center are utilized to do a superposed epoch analysis on solar parameters including proton density, proton temperature, solar <span class="hlt">wind</span> speed and solar magnetic field in order to study how the variations of these parameters affect the modulation of galactic cosmic rays. Magnetic fluctuation variances in different parts a of CIR are computed and analyzed using similar techniques in order to understand the cosmic-ray diffusive transport in these <span class="hlt">regions</span>.</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('https://www.gpo.gov/fdsys/pkg/FR-2011-09-07/pdf/2011-22804.pdf','FEDREG'); return false;" href="https://www.gpo.gov/fdsys/pkg/FR-2011-09-07/pdf/2011-22804.pdf"><span>76 FR 55456 - The <span class="hlt">Trade</span> and Investment Partnership for the Middle East and North Africa</span></a></p> <p><a target="_blank" href="http://www.gpo.gov/fdsys/browse/collection.action?collectionCode=FR">Federal Register 2010, 2011, 2012, 2013, 2014</a></p> <p></p> <p>2011-09-07</p> <p>... facilitate more robust <span class="hlt">trade</span> within the <span class="hlt">region</span> and promote greater MENA integration with U.S. and other... integration with U.S. and European markets, and (3) open the door for those countries that adopt high... government actions that can enhance economic integration within the MENA <span class="hlt">region</span> and increase <span class="hlt">trade</span> and...</p> </li> <li> <p><a target="_blank" onclick="trackOutboundLink('http://hdl.handle.net/2060/19970023397','NASA-TRS'); return false;" href="http://hdl.handle.net/2060/19970023397"><span>Quality and Control of Water Vapor <span class="hlt">Winds</span></span></a></p> <p><a target="_blank" href="http://ntrs.nasa.gov/search.jsp">NASA Technical Reports Server (NTRS)</a></p> <p>Jedlovec, Gary J.; Atkinson, Robert J.</p> <p>1996-01-01</p> <p>Water vapor imagery from the geostationary satellites such as GOES, Meteosat, and GMS provides synoptic views of dynamical events on a continual basis. Because the imagery represents a non-linear combination of mid- and upper-tropospheric thermodynamic parameters (three-dimensional variations in temperature and humidity), video loops of these image products provide enlightening views of <span class="hlt">regional</span> flow fields, the movement of tropical and extratropical storm systems, the transfer of moisture between hemispheres and from the tropics to the mid- latitudes, and the dominance of high pressure systems over particular <span class="hlt">regions</span> of the Earth. Despite the obvious larger scale features, the water vapor imagery contains significant image variability down to the single 8 km GOES pixel. These features can be quantitatively identified and tracked from one time to the next using various image processing techniques. Merrill et al. (1991), Hayden and Schmidt (1992), and Laurent (1993) have documented the operational procedures and capabilities of NOAA and ESOC to produce cloud and water vapor <span class="hlt">winds</span>. These techniques employ standard correlation and template matching approaches to <span class="hlt">wind</span> tracking and use qualitative and quantitative procedures to eliminate bad <span class="hlt">wind</span> vectors from the <span class="hlt">wind</span> data set. Techniques have also been developed to improve the quality of the operational <span class="hlt">winds</span> though robust editing procedures (Hayden and Veldon 1991). These quality and control approaches have limitations, are often subjective, and constrain <span class="hlt">wind</span> variability to be consistent with model derived <span class="hlt">wind</span> fields. This paper describes research focused on the refinement of objective quality and control parameters for water vapor <span class="hlt">wind</span> vector data sets. New quality and control measures are developed and employed to provide a more robust <span class="hlt">wind</span> data set for climate analysis, data assimilation studies, as well as operational weather forecasting. The parameters are applicable to cloud-tracked <span class="hlt">winds</span> as well with minor</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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